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SAT Math Fundamentalsthe reference sheet

Every topic in the course, boiled down to its rule, its formula, and one worked example. For review and quick lookups, not for learning a topic the first time.

17 units, 68 sections, 651 topics. Press / to search.

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Unit 1 68 topics

Preliminaries

Addition and Subtraction of Rational Numbers, Multiplication and Division of Rational Numbers, Exponents, and more.

1.1 Addition and Subtraction of Rational Numbers

−6−5−4−3−2−101234562 + (−5) = −3−3 − (−4) = 1
Adding a negative moves left. Subtracting a negative moves right, the same as adding.
  1. 1.1.1

    Subtracting a Positive Number From a Smaller Positive Number

    The answer is negative. Find the gap, then make it negative.

    e.g. 3−8=−53 - 8 = -5

    a−b=−(b−a)when b>a\displaystyle a - b = -(b - a) \quad \text{when } b > a
  2. 1.1.2

    Subtracting a Positive Number From a Negative Number

    Move further left. Add the sizes, keep the negative sign.

    e.g. −4−6=−10-4 - 6 = -10

    −a−b=−(a+b)\displaystyle -a - b = -(a + b)
  3. 1.1.3

    Subtracting a Positive Fraction From a Smaller Fraction

    Get a common denominator, then subtract the same way.

    14−23=312−812=−512\displaystyle \frac{1}{4} - \frac{2}{3} = \frac{3}{12} - \frac{8}{12} = -\frac{5}{12}
  4. 1.1.4

    Subtracting a Positive Decimal From a Smaller Decimal

    Line up the decimal points, subtract larger minus smaller, attach the negative.

    1.2−3.75=−2.55\displaystyle 1.2 - 3.75 = -2.55
  5. 1.1.5

    Adding a Positive Number to a Negative Number

    Signs differ: subtract the sizes and keep the sign of the bigger size.

    −7+3=−4\displaystyle -7 + 3 = -4
    −2+9=7\displaystyle -2 + 9 = 7
  6. 1.1.6

    Adding a Negative Number

    Adding a negative is the same as subtracting.

    e.g. 5+(−8)=−35 + (-8) = -3

    a+(−b)=a−b\displaystyle a + (-b) = a - b
  7. 1.1.7

    Subtracting a Negative Number

    Subtracting a negative is the same as adding.

    e.g. −2−(−6)=4-2 - (-6) = 4

    a−(−b)=a+b\displaystyle a - (-b) = a + b
  8. 1.1.8

    Additive Inverses of Numbers

    A number and its opposite add to zero. They sit the same distance from 0 on opposite sides.

    a+(−a)=0\displaystyle a + (-a) = 0
  9. 1.1.9

    Interpreting Additive Opposites and Addition Using Absolute Value

    Absolute value is distance from zero, so it is never negative. a+ba + b lands ∣b∣\lvert b \rvert units from aa.

    ∣a∣=distance from 0\displaystyle \lvert a \rvert = \text{distance from } 0
    ∣−5∣=∣5∣=5\displaystyle \lvert -5 \rvert = \lvert 5 \rvert = 5
  10. 1.1.10

    Solving Problems Using Addition and Subtraction of Rational Numbers

    Model it on a number line: right or up is +, left or down is −. Temperatures, elevation, bank balances.

    e.g. 3°F falls 10° → 3−10=−73 - 10 = -7°F

1.2 Multiplication and Division of Rational Numbers

×+−+−+−−+Same signs → positiveDifferent signs → negativeWorks for × and ÷ alike.Count the negatives: even → +, odd → −
Sign rules for multiplying and dividing.
  1. 1.2.1

    Multiplying Positive Numbers With Negative Numbers

    Different signs give a negative.

    e.g. 4×(−3)=−124 \times (-3) = -12

    (+)(−)=(−)\displaystyle (+)(-) = (-)
  2. 1.2.2

    Multiplying Negative Numbers

    Same signs give a positive. An even count of negatives is positive; an odd count is negative.

    e.g. (−2)(−3)(−1)=−6(-2)(-3)(-1) = -6

    (−)(−)=(+)\displaystyle (-)(-) = (+)
  3. 1.2.3

    Dividing With Negative Numbers

    Same sign rules as multiplication.

    −124=−3\displaystyle \frac{-12}{4} = -3
    −12−4=3\displaystyle \frac{-12}{-4} = 3
  4. 1.2.4

    Equivalent Fractions With Negative Numbers

    One negative can sit in any of three places. Two negatives cancel.

    −ab=−ab=a−b\displaystyle -\frac{a}{b} = \frac{-a}{b} = \frac{a}{-b}
    −a−b=ab\displaystyle \frac{-a}{-b} = \frac{a}{b}
  5. 1.2.5

    Dividing With Negative Decimals and Fractions

    Settle the sign first, then divide the sizes. For fractions, multiply by the reciprocal.

    e.g. −34÷12=−34⋅2=−32-\tfrac34 \div \tfrac12 = -\tfrac34 \cdot 2 = -\tfrac32

  6. 1.2.6

    Reciprocals of Rational Numbers

    Flip the fraction. A number times its reciprocal is 1. The sign stays; zero has no reciprocal.

    e.g. reciprocal of −25-\tfrac25 is −52-\tfrac52

    ab⋅ba=1\displaystyle \frac{a}{b} \cdot \frac{b}{a} = 1
  7. 1.2.7

    Multiplying and Dividing With Zero

    Anything times zero is zero. Zero divided by a number is zero. Dividing by zero is undefined.

    a×0=0\displaystyle a \times 0 = 0
    0a=0\displaystyle \frac{0}{a} = 0
    a0 is undefined\displaystyle \frac{a}{0} \text{ is undefined}
  8. 1.2.8

    Fractions of Fractions

    “Of” means multiply. Multiply across.

    e.g. 23\tfrac23 of 34\tfrac34 =612=12= \tfrac{6}{12} = \tfrac12

    ab⋅cd=acbd\displaystyle \frac{a}{b} \cdot \frac{c}{d} = \frac{ac}{bd}
  9. 1.2.9

    Solving Problems Using Multiplication and Division of Rational Numbers

    Decide the operation, settle the sign, then compute.

    e.g. Drops 1.5 m per hour for 4 hours → −1.5×4=−6-1.5 \times 4 = -6 m

  10. 1.2.10

    Solving Problems Using the Four Operations on Rational Numbers

    Use order of operations and the sign rules together.

    e.g. −3+4×(−2)=−3−8=−11-3 + 4 \times (-2) = -3 - 8 = -11

1.3 Exponents

x³ · x²=xxxxx= x⁵Count the copies of x. Multiplying adds them: 3 + 2 = 5.Dividing cancels them: x⁵ ÷ x² leaves 3 copies, so x³.
Why the product rule works. Every exponent rule comes from counting copies.
  1. 1.3.1

    Squaring Rational Numbers

    Multiply the number by itself. A negative squared is positive.

    x2=x⋅x\displaystyle x^2 = x \cdot x
    (−23)2=49\displaystyle \left(-\tfrac{2}{3}\right)^2 = \tfrac{4}{9}
  2. 1.3.2

    Cubing Rational Numbers

    Three copies multiplied. A cube keeps the sign.

    x3=x⋅x⋅x\displaystyle x^3 = x \cdot x \cdot x
    (−2)3=−8\displaystyle (-2)^3 = -8
  3. 1.3.3

    Exponents With Rational Bases

    Raise the top and the bottom. Watch the parentheses: the exponent only touches what it is attached to.

    (ab)n=anbn\displaystyle \left(\frac{a}{b}\right)^n = \frac{a^n}{b^n}
    −32=−9(−3)2=9\displaystyle -3^2 = -9 \quad (-3)^2 = 9
  4. 1.3.4

    The Zeroth Power

    Any nonzero number to the zero power is 1.

    e.g. (−7)0=1(-7)^0 = 1

    a0=1(a≠0)\displaystyle a^0 = 1 \quad (a \ne 0)
  5. 1.3.5

    Powers of Negative One

    Even power gives 1, odd power gives −1.

    (−1)n={1n even−1n odd\displaystyle (-1)^n = \begin{cases} 1 & n \text{ even} \\ -1 & n \text{ odd} \end{cases}
  6. 1.3.6

    Negative Exponents

    A negative exponent means reciprocal. It does not make the number negative.

    e.g. 2−3=182^{-3} = \tfrac18

    a−n=1an\displaystyle a^{-n} = \frac{1}{a^n}
    (ab)−n=(ba)n\displaystyle \left(\frac{a}{b}\right)^{-n} = \left(\frac{b}{a}\right)^{n}
  7. 1.3.7

    The Product Rule for Exponents

    Same base, multiplying: add the exponents.

    e.g. x3⋅x4=x7x^3 \cdot x^4 = x^7

    am⋅an=am+n\displaystyle a^m \cdot a^n = a^{m+n}
  8. 1.3.8

    The Quotient Rule for Exponents

    Same base, dividing: subtract the exponents.

    e.g. x7x2=x5\tfrac{x^7}{x^2} = x^5

    aman=am−n\displaystyle \frac{a^m}{a^n} = a^{m-n}
  9. 1.3.9

    The Power Rule for Exponents

    Power of a power: multiply the exponents.

    e.g. (x2)5=x10(x^2)^5 = x^{10}

    (am)n=amn\displaystyle (a^m)^n = a^{mn}
  10. 1.3.10

    The Power of Product Rule for Exponents

    The exponent goes to every factor inside.

    e.g. (2x)3=8x3(2x)^3 = 8x^3

    (ab)n=anbn\displaystyle (ab)^n = a^n b^n
  11. 1.3.11

    The Power of Quotient Rule for Exponents

    The exponent goes to the top and the bottom.

    (ab)n=anbn\displaystyle \left(\frac{a}{b}\right)^n = \frac{a^n}{b^n}
  12. 1.3.12

    Combining the Rules of Exponents

    Work inside parentheses, apply outside powers, combine like bases, finish with positive exponents.

    e.g. (x2)3⋅xx4=x7x4=x3\dfrac{(x^2)^3 \cdot x}{x^4} = \dfrac{x^7}{x^4} = x^3

1.4 Radicals

na=a1/nindexradicand√(x²) = |x|a square root is nevernegative∛(x³) = xodd roots keep the sign
A root is a fractional power. Even roots need an absolute value when the sign of x is unknown; odd roots do not.
  1. 1.4.1

    The Square Root of a Perfect Square

     \sqrt{\ } asks “what nonnegative number squared gives this?” Know squares through 15² = 225.

    e.g. 49=7\sqrt{49} = 7, 916=34\sqrt{\tfrac{9}{16}} = \tfrac34

    a2=a(a≥0)\displaystyle \sqrt{a^2} = a \quad (a \ge 0)
  2. 1.4.2

    Squaring a Square Root

    Squaring undoes the square root.

    e.g. (7)2=7(\sqrt{7})^2 = 7

    (a)2=a(a≥0)\displaystyle \left(\sqrt{a}\right)^2 = a \quad (a \ge 0)
  3. 1.4.3

    The Cube Root of a Perfect Cube

    Asks “what cubed gives this?” Negatives are allowed and stay negative.

    a33=a\displaystyle \sqrt[3]{a^3} = a
    −273=−3\displaystyle \sqrt[3]{-27} = -3
  4. 1.4.4

    Surds

    A root that never comes out to a whole number or fraction, like 2\sqrt2. It is irrational, so leave it in exact form.

    e.g. 2,3,5\sqrt2, \sqrt3, \sqrt5 are surds; 9\sqrt9 is not

  5. 1.4.5

    Simplifying Expressions With Surds

    Pull out the largest perfect-square factor.

    72=36⋅2=62\displaystyle \sqrt{72} = \sqrt{36 \cdot 2} = 6\sqrt{2}
  6. 1.4.6

    Evaluating Numerical Expressions Containing Radicals

    A radical acts like parentheses: simplify everything under it first.

    e.g. 3+25−9=3+4=73 + \sqrt{25 - 9} = 3 + 4 = 7

  7. 1.4.7

    Adding and Subtracting Radicals

    Only like radicals (same number under the root) combine. Simplify each one first.

    32+52=82\displaystyle 3\sqrt{2} + 5\sqrt{2} = 8\sqrt{2}
    8+2=22+2=32\displaystyle \sqrt{8} + \sqrt{2} = 2\sqrt2 + \sqrt2 = 3\sqrt{2}
  8. 1.4.8

    Rationalizing Denominators

    Clear a root from the bottom by multiplying top and bottom by that root.

    e.g. 63=633=23\tfrac{6}{\sqrt3} = \tfrac{6\sqrt3}{3} = 2\sqrt3

    ab=abb\displaystyle \frac{a}{\sqrt{b}} = \frac{a\sqrt{b}}{b}
  9. 1.4.9

    Rationalizing Denominators With Two Terms

    Multiply by the conjugate: the same two terms with the middle sign flipped. The difference of squares clears the root.

    e.g. 13+2=3−27\tfrac{1}{3 + \sqrt2} = \tfrac{3 - \sqrt2}{7}

    1a+b⋅a−ba−b=a−ba2−b\displaystyle \frac{1}{a + \sqrt{b}} \cdot \frac{a - \sqrt{b}}{a - \sqrt{b}} = \frac{a - \sqrt{b}}{a^2 - b}
  10. 1.4.10

    Radicals as Fractional Exponents

    A root is a fractional power. The bottom of the fraction is the root.

    e.g. 82/3=(83)2=48^{2/3} = (\sqrt[3]{8})^2 = 4

    an=a1/n\displaystyle \sqrt[n]{a} = a^{1/n}
    amn=am/n\displaystyle \sqrt[n]{a^m} = a^{m/n}
  11. 1.4.11

    The Product Rule for Radicals

    The root of a product is the product of the roots.

    e.g. 312=36=6\sqrt{3}\sqrt{12} = \sqrt{36} = 6

    ab=a b(a,b≥0)\displaystyle \sqrt{ab} = \sqrt{a}\,\sqrt{b} \quad (a, b \ge 0)
  12. 1.4.12

    The Quotient Rule for Radicals

    The root of a quotient is the quotient of the roots.

    e.g. 254=52\sqrt{\tfrac{25}{4}} = \tfrac52

    ab=ab\displaystyle \sqrt{\frac{a}{b}} = \frac{\sqrt{a}}{\sqrt{b}}
  13. 1.4.13

    Applying the Distributive Law to Radical Expressions

    Distribute or FOIL as usual, multiply radicals together, then simplify. Conjugates eliminate the radical.

    e.g. 3(6+2)=18+23=32+23\sqrt3(\sqrt6 + 2) = \sqrt{18} + 2\sqrt3 = 3\sqrt2 + 2\sqrt3

    a (b+c)=ab+ac\displaystyle \sqrt a\,(\sqrt b + \sqrt c) = \sqrt{ab} + \sqrt{ac}
    (a+b)(a−b)=a−b2\displaystyle (\sqrt a + b)(\sqrt a - b) = a - b^2
  14. 1.4.14

    Comparing Radicals

    Move each coefficient inside the root by squaring it, then compare the numbers under the roots. A larger radicand means a larger root.

    e.g. 35=453\sqrt5 = \sqrt{45} and 52=505\sqrt2 = \sqrt{50}, so 525\sqrt2 is larger

    ab=a2b(a≥0)\displaystyle a\sqrt b = \sqrt{a^2 b} \quad (a \ge 0)

1.5 Order of Operations

PParenthesesinside firstEExponentsand rootsM DMultiply, divideleft to rightA SAdd, subtractleft to right
Order of operations. M and D share a step, as do A and S: whichever comes first, reading left to right, goes first.
  1. 1.5.1

    Natural Numbers, Integers, and Rational Numbers

    Each set sits inside the next. Rational means it can be written as a fraction of integers.

    N⊂Z⊂Q\displaystyle \mathbb{N} \subset \mathbb{Z} \subset \mathbb{Q}
    rational=ab, a,b integers, b≠0\displaystyle \text{rational} = \frac{a}{b},\ a, b \text{ integers},\ b \ne 0
  2. 1.5.2

    Rational Numbers as Finite or Repeating Decimals

    Every rational number either ends or repeats. It ends when the simplified denominator has only 2s and 5s as prime factors.

    38=0.375\displaystyle \frac{3}{8} = 0.375
    13=0.3‾\displaystyle \frac{1}{3} = 0.\overline{3}
    211=0.18‾\displaystyle \frac{2}{11} = 0.\overline{18}
  3. 1.5.3

    Evaluating Rational Number Expressions Without Exponents

    Parentheses first. Then multiply and divide left to right. Then add and subtract left to right.

    e.g. 8−6÷3×2=8−4=48 - 6 \div 3 \times 2 = 8 - 4 = 4

  4. 1.5.4

    Evaluating Expressions With Positive Integer Exponents

    PEMDAS: exponents come right after parentheses.

    e.g. 2+3⋅42=2+48=502 + 3 \cdot 4^2 = 2 + 48 = 50

    P→E→MD→AS\displaystyle \text{P} \to \text{E} \to \text{MD} \to \text{AS}
  5. 1.5.5

    Evaluating Expressions With Integer Exponents

    Handle negative exponents at the exponent step by turning them into reciprocals.

    e.g. 2+3⋅2−1=2+32=722 + 3 \cdot 2^{-1} = 2 + \tfrac32 = \tfrac72

1.6 Algebraic Expressions

−5x+8coefficientvariableconstanttermtermThe sign in frontbelongs to the term.
Parts of an expression.
  1. 1.6.1

    Introduction to Algebraic Expressions

    Numbers, variables, and operations with no equals sign. A variable stands for a number you don't know yet.

    3x+5\displaystyle 3x + 5
  2. 1.6.2

    Constructing Algebraic Expressions

    Translate the words. Sum +, difference −, product ×, quotient ÷. “Less than” and “more than” flip the order.

    e.g. “5 less than twice nn” → 2n−52n - 5

  3. 1.6.3

    Evaluating Linear Expressions

    Substitute the value in parentheses, then follow order of operations.

    3x−4, x=−2\displaystyle 3x - 4,\ x = -2
    3(−2)−4=−10\displaystyle 3(-2) - 4 = -10
  4. 1.6.4

    Evaluating Rational Expressions

    Work out the top and the bottom separately, then divide. The bottom can never be 0.

    e.g. x+4x−1\dfrac{x+4}{x-1} at x=3x=3 → 72\tfrac72

  5. 1.6.5

    Identifying Terms in Linear Expressions

    Terms are the pieces separated by + or −. The sign in front belongs to the term.

    e.g. 4x−7y+24x - 7y + 2 has terms 4x4x, −7y-7y, 22

  6. 1.6.6

    Identifying Coefficients and Constants

    The coefficient is the number multiplying a variable. The constant has no variable. A lone xx has coefficient 1.

    e.g. In −5x+8-5x + 8: coefficient −5-5, constant 88

  7. 1.6.7

    The Greatest Common Factor of Two Linear Expressions

    Factor each fully, then keep what they share.

    6x+9=3(2x+3)\displaystyle 6x + 9 = 3(2x + 3)
    12x+18=6(2x+3)\displaystyle 12x + 18 = 6(2x + 3)
    GCF=3(2x+3)\displaystyle \text{GCF} = 3(2x + 3)

1.7 Simplifying Linear Expressions

4x12x344(x + 3)= 4x + 12
Area model. The outside number multiplies every piece inside. Factoring reads the picture right to left.
  1. 1.7.1

    Identifying Like Terms in Linear Expressions

    Like terms have the same variable to the same power. Constants are like each other.

    e.g. 3x3x and −5x-5x: like. 3x3x and 3y3y: not.

  2. 1.7.2

    Collecting Like Terms in Linear Expressions

    Add the coefficients of like terms; the variable part stays.

    3x+5−x+2=2x+7\displaystyle 3x + 5 - x + 2 = 2x + 7
  3. 1.7.3

    Applying the Distributive Law With Linear Expressions

    Multiply the outside number by every term inside.

    e.g. 4(x+3)=4x+124(x + 3) = 4x + 12

    a(b+c)=ab+ac\displaystyle a(b + c) = ab + ac
  4. 1.7.4

    The Distributive Law With Three Terms

    Same rule, one more term.

    e.g. 2(x−y+5)=2x−2y+102(x - y + 5) = 2x - 2y + 10

    a(b+c+d)=ab+ac+ad\displaystyle a(b + c + d) = ab + ac + ad
  5. 1.7.5

    Distributing the Negative Sign in a Linear Expression

    A minus in front flips the sign of every term inside.

    −(a−b+c)=−a+b−c\displaystyle -(a - b + c) = -a + b - c
  6. 1.7.6

    Simplifying Linear Expressions Using the Distributive Law

    Distribute first, then collect like terms.

    2(x+3)+4x=6x+6\displaystyle 2(x + 3) + 4x = 6x + 6
  7. 1.7.7

    Simplifying Linear Expressions When a Group of Terms Is Subtracted

    Distribute the −1 (or −k) to every term in the group.

    5x−(2x−3)=5x−2x+3=3x+3\displaystyle 5x - (2x - 3) = 5x - 2x + 3 = 3x + 3
  8. 1.7.8

    Simplifying Linear Expressions Containing Fractions

    Distribute, then combine with a common denominator.

    12(4x−6)=2x−3\displaystyle \tfrac{1}{2}(4x - 6) = 2x - 3
    x2+x3=5x6\displaystyle \tfrac{x}{2} + \tfrac{x}{3} = \tfrac{5x}{6}
  9. 1.7.9

    Factoring Numerical Expressions

    Pull out the GCF. Factoring is distributing in reverse.

    12+18=6(2+3)\displaystyle 12 + 18 = 6(2 + 3)
  10. 1.7.10

    Factoring Linear Expressions

    Find the GCF of the terms and write it outside.

    ab+ac=a(b+c)\displaystyle ab + ac = a(b + c)
    8x−12=4(2x−3)\displaystyle 8x - 12 = 4(2x - 3)

Unit 2 26 topics

Algebra - Linear Equations in One Variable

Solving Linear Equations, and Modeling With Linear Equations.

2.8 Solving Linear Equations

xx + 37=Take 3 fromboth sides:x = 4
An equation is a balance. Whatever you do to one side, do to the other.
  1. 2.8.1

    Solving Linear Equations by Trial and Error

    Guess a value, substitute, check whether both sides match, adjust the guess.

    e.g. 3x+1=133x + 1 = 13: try 4 → 1313 ✓

  2. 2.8.2

    Solving One-Step Addition and Subtraction Equations

    Do the opposite operation to both sides.

    x+a=b⇒x=b−a\displaystyle x + a = b \Rightarrow x = b - a
    x−a=b⇒x=b+a\displaystyle x - a = b \Rightarrow x = b + a
  3. 2.8.3

    Solving One-Step Multiplication and Division Equations

    Divide to undo multiplying, multiply to undo dividing.

    ax=b⇒x=ba\displaystyle ax = b \Rightarrow x = \frac{b}{a}
    xa=b⇒x=ab\displaystyle \frac{x}{a} = b \Rightarrow x = ab
  4. 2.8.4

    Solving Two-Step Equations

    Undo adding or subtracting first, then undo multiplying or dividing.

    e.g. 3x+4=19⇒3x=15⇒x=53x + 4 = 19 \Rightarrow 3x = 15 \Rightarrow x = 5

    ax+b=c⇒x=c−ba\displaystyle ax + b = c \Rightarrow x = \frac{c - b}{a}
  5. 2.8.5

    Solving Linear Equations With Fractional Coefficients

    Multiply both sides by the reciprocal of the coefficient.

    23x=8⇒x=8⋅32=12\displaystyle \tfrac{2}{3}x = 8 \Rightarrow x = 8 \cdot \tfrac{3}{2} = 12
  6. 2.8.6

    Solving Linear Equations With Decimal Coefficients

    Multiply both sides by 10, 100, … to clear the decimals, then solve.

    0.3x+1.2=3→×103x+12=30\displaystyle 0.3x + 1.2 = 3 \xrightarrow{\times 10} 3x + 12 = 30
  7. 2.8.7

    Solving Linear Equations With Variables on Both Sides

    Gather the variable terms on one side and the numbers on the other.

    5x+2=3x+10\displaystyle 5x + 2 = 3x + 10
    2x=8⇒x=4\displaystyle 2x = 8 \Rightarrow x = 4
  8. 2.8.8

    Solving Linear Equations Containing Binomials

    Expand every product, including a negative sign in front of parentheses. If x2x^2 terms appear on both sides, they cancel and the equation becomes linear. Then collect xx terms and solve.

    e.g. (x+3)(x−2)=(x+1)(x+4)(x+3)(x-2) = (x+1)(x+4): x2+x−6=x2+5x+4x^2 + x - 6 = x^2 + 5x + 4, so −4x=10-4x = 10 and x=−52x = -\tfrac52

  9. 2.8.9

    Solving Linear Equations Containing Binomials by Factoring

    When the same binomial appears more than once, treat it as a single unit. Collect it on one side, solve for the binomial, then solve for xx.

    e.g. 5(x−3)=2(x−3)+12⇒3(x−3)=12⇒x−3=4⇒x=75(x-3) = 2(x-3) + 12 \Rightarrow 3(x-3) = 12 \Rightarrow x - 3 = 4 \Rightarrow x = 7

    a(x+h)=b(x+h)+c\displaystyle a(x+h) = b(x+h) + c
    ⇒  (a−b)(x+h)=c\displaystyle \Rightarrow\; (a-b)(x+h) = c
  10. 2.8.10

    Solving Linear Equations by Clearing a Rational Expression

    Multiply every term by the LCD of all the denominators.

    x3+x4=7→×124x+3x=84\displaystyle \frac{x}{3} + \frac{x}{4} = 7 \xrightarrow{\times 12} 4x + 3x = 84
  11. 2.8.11

    Solving Linear Equations Using Cross-Multiplication

    When one fraction equals another, multiply diagonally.

    e.g. x4=96⇒6x=36⇒x=6\tfrac{x}{4} = \tfrac{9}{6} \Rightarrow 6x = 36 \Rightarrow x = 6

    ab=cd⇒ad=bc\displaystyle \frac{a}{b} = \frac{c}{d} \Rightarrow ad = bc
  12. 2.8.12

    Manipulating Expressions and Equations

    Do the same operation to both sides to isolate a variable or to turn one side into the exact expression asked for. On the SAT, often you do not need each variable's value.

    e.g. If 2x+3=72x + 3 = 7, then 6x+9=3(2x+3)=216x + 9 = 3(2x + 3) = 21

  13. 2.8.13

    Solving Two-Variable Equations

    Solve for one variable in terms of the other, or plug in a given value.

    2x+y=10⇒y=10−2x\displaystyle 2x + y = 10 \Rightarrow y = 10 - 2x
  14. 2.8.14

    Linear Equations With Infinitely Many Solutions

    The variables cancel and leave something always true. Every number works.

    2(x+1)=2x+2  →  2=2\displaystyle 2(x + 1) = 2x + 2 \;\to\; 2 = 2
  15. 2.8.15

    Linear Equations With No Solutions

    The variables cancel and leave something false. No number works.

    3x+1=3x+5  →  1=5\displaystyle 3x + 1 = 3x + 5 \;\to\; 1 = 5
  16. 2.8.16

    Solving Linear Equations With Unknown Coefficients

    Treat the other letters as numbers and isolate the variable you want. Divide by its coefficient only when that coefficient can’t be zero.

    e.g. Solve ax−3=7ax - 3 = 7 for xx: x=10ax = \tfrac{10}{a}

    ax+b=c\displaystyle ax + b = c
    ⇒  x=c−ba(a≠0)\displaystyle \Rightarrow\; x = \frac{c - b}{a} \quad (a \ne 0)
  17. 2.8.17

    Solving Linear Equations With Unknown Coefficients by Factoring

    When the variable appears in more than one term, gather those terms, factor the variable out, then divide.

    e.g. kx+2x=9⇒x=9k+2kx + 2x = 9 \Rightarrow x = \tfrac{9}{k + 2}

    ax+bx=c\displaystyle ax + bx = c
    ⇒  x(a+b)=c\displaystyle \Rightarrow\; x(a + b) = c
    ⇒  x=ca+b\displaystyle \Rightarrow\; x = \frac{c}{a + b}
  18. 2.8.18

    Solving Linear Inequalities With Unknown Parameters

    Same steps as an equation. If you divide by a parameter, its sign decides whether the inequality flips.

    ax>b  ⇒  {x>baa>0x<baa<0\displaystyle ax > b \;\Rightarrow\; \begin{cases} x > \frac{b}{a} & a > 0 \\[2pt] x < \frac{b}{a} & a < 0 \end{cases}
  19. 2.8.19

    Solving Many-Variable Equations

    To solve a formula for one variable, undo the operations around it until it stands alone.

    e.g. P=2l+2w⇒w=P−2l2P = 2l + 2w \Rightarrow w = \tfrac{P - 2l}{2}

    A=12bh  ⇒  h=2Ab\displaystyle A = \tfrac{1}{2}bh \;\Rightarrow\; h = \frac{2A}{b}

2.9 Modeling With Linear Equations

  1. 2.9.1

    Interpreting Linear Expressions

    In mx+bmx + b, bb is the fixed starting amount and mm is the amount added for each unit of xx.

    e.g. 25+0.15m25 + 0.15m: a $25 fee plus 15¢ per mile

    total=m⏟per unit x+b⏟fixed\displaystyle \text{total} = \underbrace{m}_{\text{per unit}}\,x + \underbrace{b}_{\text{fixed}}
  2. 2.9.2

    Modeling With Linear Equations

    Name the unknown, write the equation the words describe, solve, and check that the answer makes sense.

    e.g. $30 to join plus $10 a month, $110 spent → 30+10m=11030 + 10m = 110, m=8m = 8 months

  3. 2.9.3

    Consecutive Integer Problems

    Call the first integer nn. Consecutive integers are n,n+1,n+2n, n+1, n+2. Consecutive even or odd integers are n,n+2,n+4n, n+2, n+4.

    e.g. Three consecutive integers sum to 48 → 3n+3=483n + 3 = 48, n=15n = 15

    n+(n+1)+(n+2)=3n+3\displaystyle n + (n + 1) + (n + 2) = 3n + 3
  4. 2.9.4

    Speed, Distance, Time Problems

    Write d=std = st for each traveler, then connect them: same distance, same time, or distances that add up.

    e.g. Cars leave together at 50 and 60 mph in opposite directions → 110t=330110t = 330 when 330 mi apart, t=3t = 3 h

    d=s t\displaystyle d = s\,t
  5. 2.9.5

    Further Speed, Distance, Time Problems

    A chaser closes a gap at the difference of the speeds. Travelers heading toward each other close it at the sum.

    t=gaps1−s2  (catching up)\displaystyle t = \frac{\text{gap}}{s_1 - s_2} \;\text{(catching up)}
    t=gaps1+s2  (approaching)\displaystyle t = \frac{\text{gap}}{s_1 + s_2} \;\text{(approaching)}
  6. 2.9.6

    Modeling Work Problems

    Each worker does a fraction of the job per hour. Working together, the rates add.

    e.g. Pipes fill a tank in 3 h and 6 h → 13+16=12\tfrac13 + \tfrac16 = \tfrac12 → together 2 h

    1a+1b=1t\displaystyle \frac{1}{a} + \frac{1}{b} = \frac{1}{t}
  7. 2.9.7

    Modeling Mixture Problems

    Track the pure ingredient: concentration times volume, added across the parts.

    e.g. 10 L at 20% plus xx L at 50% makes 30% → 2+0.5x=0.3(10+x)2 + 0.5x = 0.3(10 + x), x=5x = 5

    c1V1+c2V2=c (V1+V2)\displaystyle c_1V_1 + c_2V_2 = c\,(V_1 + V_2)

Unit 3 39 topics

Algebra - Linear Equations in Two Variables

Graphs of Linear Equations, Modeling With Two-Variable Linear Equations, and Systems of Equations.

3.10 Graphs of Linear Equations

xy−2−1123456−4−3−2−1123(0, −2)(4, 0)(2, −1)One line, three formsy = ½x − 2slope-intercept: slope and y-intercepty + 1 = ½(x − 2)point-slope: slope and any pointx − 2y = 4standard: both intercepts quickly
Pick the form by what you know: slope and intercept, slope and a point, or a quick way to both intercepts.
  1. 3.10.1

    The Cartesian Coordinate System

    A point is (x,y)(x, y): across first, then up. Four quadrants, numbered counterclockwise from upper right.

    e.g. Quadrant I: (+,+)(+,+), II: (−,+)(-,+), III: (−,−)(-,-), IV: (+,−)(+,-)

    (x,y)\displaystyle (x, y)
  2. 3.10.2

    Distances Between Points in the Coordinate Plane

    Points that share an xx or a yy: subtract the other coordinates and take the absolute value.

    e.g. (3,−2)(3, -2) to (3,5)(3, 5) → 77

    same x:∣y2−y1∣\displaystyle \text{same } x: \lvert y_2 - y_1 \rvert
    same y:∣x2−x1∣\displaystyle \text{same } y: \lvert x_2 - x_1 \rvert
  3. 3.10.3

    Two-Variable Linear Equations and Their Solutions

    A solution is an (x,y)(x, y) pair that makes the equation true. All solutions together form a line.

    e.g. (1,8)(1, 8) solves y=2x+6y = 2x + 6

  4. 3.10.4

    Graphing Linear Equations

    Pick two or three xx values, find each yy, plot the points, draw the line through them.

  5. 3.10.5

    Horizontal and Vertical Lines

    y=by = b is horizontal with slope 0. x=ax = a is vertical with undefined slope.

    y=b\displaystyle y = b
    x=a\displaystyle x = a
  6. 3.10.6

    Calculating Slopes of Straight Lines

    Slope is rise over run between any two points.

    e.g. (1,2)(1, 2) to (4,8)(4, 8) → m=63=2m = \tfrac63 = 2

    m=y2−y1x2−x1=riserun\displaystyle m = \frac{y_2 - y_1}{x_2 - x_1} = \frac{\text{rise}}{\text{run}}
  7. 3.10.7

    Equations of Lines in Slope-Intercept Form

    mm is the slope and bb is the yy-intercept.

    e.g. y=−2x+5y = -2x + 5: slope −2-2, crosses the yy-axis at (0,5)(0, 5)

    y=mx+b\displaystyle y = mx + b
    m=y2−y1x2−x1\displaystyle m = \frac{y_2 - y_1}{x_2 - x_1}
  8. 3.10.8

    Properties of Lines Given in Slope-Intercept Form

    Positive mm rises, negative mm falls, zero is flat. Larger ∣m∣\lvert m \rvert means steeper. The xx-intercept is where y=0y = 0.

    x-intercept=−bm\displaystyle x\text{-intercept} = -\frac{b}{m}
  9. 3.10.9

    Working With Lines in Slope-Intercept Form

    mm is the slope and bb is the yy-intercept. To find the line through two points, compute mm, then plug in one point to get bb. Parallel lines share mm. Perpendicular slopes multiply to −1-1.

    e.g. Through (1,5)(1, 5) and (3,9)(3, 9): m=42=2m = \tfrac{4}{2} = 2, 5=2(1)+b5 = 2(1) + b, so y=2x+3y = 2x + 3

    y=mx+b\displaystyle y = mx + b
    m=y2−y1x2−x1\displaystyle m = \frac{y_2 - y_1}{x_2 - x_1}
  10. 3.10.10

    Equations of Lines in Point-Slope Form

    Use it when you know the slope and one point on the line.

    e.g. Slope 3 through (2,−1)(2, -1): y+1=3(x−2)y + 1 = 3(x - 2)

    y−y1=m(x−x1)\displaystyle y - y_1 = m(x - x_1)
  11. 3.10.11

    Equations of Lines in Standard Form

    Integer coefficients with xx and yy on the same side. The quickest form for finding both intercepts.

    e.g. 2x+3y=122x + 3y = 12: intercepts (6,0)(6, 0) and (0,4)(0, 4)

    Ax+By=C\displaystyle Ax + By = C
  12. 3.10.12

    Properties of Lines Given in Standard Form

    Read the slope and intercepts straight from the coefficients.

    m=−AB\displaystyle m = -\frac{A}{B}
    x-int=CAy-int=CB\displaystyle x\text{-int} = \frac{C}{A} \qquad y\text{-int} = \frac{C}{B}
  13. 3.10.13

    Parallel Lines in the Coordinate Plane

    Parallel lines have the same slope and different yy-intercepts. All vertical lines are parallel to each other.

    e.g. y=2x+1y = 2x + 1 and y=2x−4y = 2x - 4 are parallel

    m1=m2\displaystyle m_1 = m_2
  14. 3.10.14

    Finding Equations of Parallel Lines

    Keep the slope, then put the given point into point-slope form.

    e.g. Parallel to y=3x−2y = 3x - 2 through (1,5)(1, 5): y=3x+2y = 3x + 2

    y−y1=m(x−x1)\displaystyle y - y_1 = m(x - x_1)
  15. 3.10.15

    Perpendicular Lines in the Coordinate Plane

    Perpendicular slopes are negative reciprocals: they multiply to −1-1. Horizontal and vertical lines are perpendicular.

    e.g. Slope 23\tfrac23 → perpendicular slope −32-\tfrac32

    m1m2=−1\displaystyle m_1 m_2 = -1
    m2=−1m1\displaystyle m_2 = -\frac{1}{m_1}
  16. 3.10.16

    Finding Equations of Perpendicular Lines

    Flip the slope and change its sign, then use the given point.

    e.g. Perpendicular to y=2x+1y = 2x + 1 through (4,1)(4, 1): y=−12x+3y = -\tfrac12x + 3

    y−y1=−1m(x−x1)\displaystyle y - y_1 = -\frac{1}{m}(x - x_1)

3.11 Modeling With Two-Variable Linear Equations

timedistanceslope = speedflat: stoppedheading backDistance–timetimespeedspeeding upflat: steady speedarea = distanceSpeed–time
On a distance–time graph the slope is the speed. On a speed–time graph the slope is the acceleration, and the shaded area is the distance traveled.
  1. 3.11.1

    Modeling With Linear Equations in Two Variables

    Find the starting value (the intercept) and the rate (the slope), then write y=mx+by = mx + b.

    e.g. Plant 4 cm tall growing 1.5 cm a week: h=1.5w+4h = 1.5w + 4

  2. 3.11.2

    Modeling Totals Using Two-Variable Linear Equations

    Two kinds of item with a fixed total: price times count for each, added.

    e.g. Adult tickets $12, child $8, $200 total: 12a+8c=20012a + 8c = 200

    ax+by=T\displaystyle ax + by = T
  3. 3.11.3

    Interpreting Coefficients of Two-Variable Equations

    In y=mx+by = mx + b, mm is the change in yy per one unit of xx and bb is the value when x=0x = 0. In ax+by=cax + by = c, aa and bb are the per-unit amounts and cc is the total.

    e.g. C=25+0.5mC = 25 + 0.5m: a $25 flat fee plus $0.50 per mile

  4. 3.11.4

    Analyzing and Interpreting Graphs of Linear Equations

    The slope is the rate of change, in yy-units per xx-unit. The yy-intercept is the value when x=0x = 0. The xx-intercept is where the quantity hits zero.

  5. 3.11.5

    Further Modeling With Linear Equations in Two Variables

    From two data points, compute the slope, then use point-slope form.

    e.g. $50 for 2 h, $80 for 4 h → m=15m = 15, C=15h+20C = 15h + 20

    m=ΔyΔx\displaystyle m = \frac{\Delta y}{\Delta x}
  6. 3.11.6

    Distance-Time Graphs

    The slope is the speed. A flat stretch means stopped; a steeper line means faster; a falling line means heading back.

    speed=slope=ΔdΔt\displaystyle \text{speed} = \text{slope} = \frac{\Delta d}{\Delta t}
  7. 3.11.7

    Speed-Time Graphs

    The slope is the acceleration. A flat stretch means constant speed, not stopped.

    acceleration=ΔvΔt\displaystyle \text{acceleration} = \frac{\Delta v}{\Delta t}
  8. 3.11.8

    Calculating Distance From a Speed-Time Graph

    Distance traveled is the area under the graph. Split it into rectangles and triangles.

    e.g. 0 to 10 m/s over 4 s → 12⋅4⋅10=20\tfrac12 \cdot 4 \cdot 10 = 20 m

    d=area under the v–t graph\displaystyle d = \text{area under the } v\text{–}t \text{ graph}

3.12 Systems of Equations

One solutionlines crossNo solutionparallel: 0 = 5Infinitely manysame line: 0 = 0
A system’s solution is where the lines meet. When elimination cancels both variables, the leftover statement tells you which case you have.
  1. 3.12.1

    Introduction to Systems of Linear Equations

    Two equations sharing variables. The solution is where the lines cross: one point, none (parallel), or infinitely many (same line).

  2. 3.12.2

    Solving Systems of Equations by Substitution

    Solve one equation for a variable, substitute into the other, solve, then plug back in.

    y=2x,x+y=9\displaystyle y = 2x,\quad x + y = 9
    x+2x=9⇒x=3, y=6\displaystyle x + 2x = 9 \Rightarrow x = 3,\ y = 6
  3. 3.12.3

    Introduction to the Elimination Method

    Add or subtract the equations so that one variable cancels.

    e.g. So x=7x = 7 and y=3y = 3

    x+y=10x−y=42x=14\displaystyle \begin{array}{r} x + y = 10 \\ x - y = 4 \\ \hline 2x = 14 \end{array}
  4. 3.12.4

    Solving Systems of Linear Equations Using Elimination: One Transformation

    Multiply one equation so a variable’s coefficients become opposites, then add.

    e.g. 2x+y=72x + y = 7, x−3y=7x - 3y = 7: triple the first, add → 7x=287x = 28, x=4x = 4, y=−1y = -1

  5. 3.12.5

    Solving Systems of Linear Equations Using Elimination: Two Transformations

    Multiply each equation by the other’s coefficient so one variable matches.

    e.g. 3x+2y=163x + 2y = 16, 2x−5y=−22x - 5y = -2: ×2 and ×3 → 19y=3819y = 38, y=2y = 2, x=4x = 4

  6. 3.12.6

    Systems of Linear Equations With Fractional Coefficients

    Clear the fractions first: multiply each equation by its LCD.

    x2+y3=4  →×6  3x+2y=24\displaystyle \tfrac{x}{2} + \tfrac{y}{3} = 4 \;\xrightarrow{\times 6}\; 3x + 2y = 24
  7. 3.12.7

    Systems of Linear Equations With Decimal Coefficients

    Multiply by 10 or 100 to turn the decimals into integers.

    0.2x+0.5y=1.6  →×10  2x+5y=16\displaystyle 0.2x + 0.5y = 1.6 \;\xrightarrow{\times 10}\; 2x + 5y = 16
  8. 3.12.8

    Systems of Equations With No Solutions and Infinitely Many Solutions

    Both variables cancel. A false statement like 0=50 = 5 means no solution (parallel lines). A true one like 0=00 = 0 means infinitely many (the same line).

  9. 3.12.9

    Parametrizing Systems With Infinitely Many Solutions

    If both equations describe the same line, every point on it is a solution. Set one variable equal to a parameter tt and solve for the other in terms of tt.

    e.g. x+2y=4x + 2y = 4 and 2x+4y=82x + 4y = 8: let y=ty = t, then x=4−2tx = 4 - 2t, so the solutions are (4−2t, t)(4 - 2t,\ t)

  10. 3.12.10

    Determining Unknown Parameters in Systems of Linear Equations

    Compare the coefficients of a1x+b1y=c1a_1x + b_1y = c_1 and a2x+b2y=c2a_2x + b_2y = c_2. Equal slopes with different intercepts means no solution. The same line means infinitely many. Different slopes means exactly one.

    e.g. 3x+ky=53x + ky = 5 and 6x+4y=76x + 4y = 7: 36=k4\tfrac36 = \tfrac{k}{4} gives k=2k = 2, and 57≠12\tfrac57 \ne \tfrac12, so no solution when k=2k = 2

    a1a2=b1b2≠c1c2: none\displaystyle \frac{a_1}{a_2} = \frac{b_1}{b_2} \ne \frac{c_1}{c_2}:\ \text{none}
    a1a2=b1b2=c1c2: infinite\displaystyle \frac{a_1}{a_2} = \frac{b_1}{b_2} = \frac{c_1}{c_2}:\ \text{infinite}
    a1a2≠b1b2: one\displaystyle \frac{a_1}{a_2} \ne \frac{b_1}{b_2}:\ \text{one}
  11. 3.12.11

    Calculating the Intersection of Two Lines

    Set the two expressions for yy equal, solve for xx, then find yy.

    e.g. y=2x+1y = 2x + 1 and y=−x+7y = -x + 7 → 3x=63x = 6 → they meet at (2,5)(2, 5)

    m1x+b1=m2x+b2\displaystyle m_1x + b_1 = m_2x + b_2
  12. 3.12.12

    Solving Systems of Linear Equations by Identifying Structure

    When asked for a combination like x+yx + y, add or subtract the equations as given instead of solving for each variable.

    e.g. 3x+y=103x + y = 10 and x+3y=6x + 3y = 6: adding gives 4x+4y=164x + 4y = 16, so x+y=4x + y = 4

  13. 3.12.13

    Larger Systems of Equations

    With three equations in three unknowns, use pairs of equations to eliminate the same variable twice. Solve the resulting two-variable system, then back-substitute.

    e.g. x+y+z=6x+y+z=6, x−y+z=2x-y+z=2, x+y−z=0x+y-z=0: subtracting the 2nd from the 1st gives y=2y = 2, subtracting the 3rd gives z=3z = 3, so x=1x = 1

  14. 3.12.14

    Modeling Using Systems of Linear Equations

    Two unknowns need two equations. Usually one counts the items and one counts their value.

    e.g. 150 tickets, adults $10, children $6, $1,140 → a+c=150a + c = 150, 10a+6c=114010a + 6c = 1140 → a=60a = 60

  15. 3.12.15

    Modeling Coin Problems Using Systems of Linear Equations

    One equation for how many coins, one for what they’re worth. Work in cents.

    e.g. → d=14d = 14 dimes, n=16n = 16 nickels

    n+d=30\displaystyle n + d = 30
    5n+10d=220\displaystyle 5n + 10d = 220

Unit 4 25 topics

Algebra - Linear Inequalities

Linear Inequalities, Two-Variable Linear Inequalities, and Modeling With Inequalities.

4.13 Linear Inequalities

−6−5−4−3−2−10123456[−2, 3)−2 ≤ x < 3−6−5−4−3−2−10123456[1, ∞)x ≥ 1−6−5−4−3−2−10123456(−∞, −3) ∪ [2, ∞)x < −3 or x ≥ 2
Closed dot and square bracket: the endpoint is included. Open dot and parenthesis: it is not. Infinity always takes a parenthesis.
  1. 4.13.1

    Inequalities

    A statement that one side is bigger or smaller. Its solution is a range of numbers.

    <    >    ≤    ≥\displaystyle < \;\; > \;\; \le \;\; \ge
  2. 4.13.2

    Compound Inequalities

    “And” means both are true, so xx is between. “Or” means at least one is true.

    −2<x≤5\displaystyle -2 < x \le 5
    x<−1  or  x>4\displaystyle x < -1 \;\text{or}\; x > 4
  3. 4.13.3

    Verifying Solutions of Linear Inequalities

    Substitute the value and check whether the statement is true.

    e.g. Is 3 a solution of 2x−1>42x - 1 > 4? 5>45 > 4 ✓

  4. 4.13.4

    Solving One-Step Linear Inequalities

    Solve like an equation, with one rule: multiplying or dividing by a negative flips the sign.

    −3x<12⇒x>−4\displaystyle -3x < 12 \Rightarrow x > -4
  5. 4.13.5

    Solving Two-Step Inequalities

    Same order as a two-step equation. Watch for the flip.

    5−2x≥11⇒−2x≥6⇒x≤−3\displaystyle 5 - 2x \ge 11 \Rightarrow -2x \ge 6 \Rightarrow x \le -3
  6. 4.13.6

    Representing Solutions to Inequalities on Number Lines

    Open circle for < or >. Closed circle for ≤ or ≥. Shade toward the solutions.

  7. 4.13.7

    Further Solving Linear Inequalities

    Distribute, collect, move variables to one side; flip if you divide by a negative.

    3(x−2)>5x+4\displaystyle 3(x - 2) > 5x + 4
    −2x>10⇒x<−5\displaystyle -2x > 10 \Rightarrow x < -5
  8. 4.13.8

    Solving Compound Inequalities

    For a<bx+c<da < bx + c < d, do each operation to all three parts. Dividing by a negative flips both signs.

    −1<2x+3<9\displaystyle -1 < 2x + 3 < 9
    ⇒  −4<2x<6\displaystyle \Rightarrow\; -4 < 2x < 6
    ⇒  −2<x<3\displaystyle \Rightarrow\; -2 < x < 3
  9. 4.13.9

    Interval Notation

    A square bracket includes the endpoint; a parenthesis excludes it.

    [a,b]: a≤x≤b\displaystyle [a, b]:\ a \le x \le b
    (a,b): a<x<b\displaystyle (a, b):\ a < x < b
    [a,b): a≤x<b\displaystyle [a, b):\ a \le x < b
  10. 4.13.10

    Unbounded Intervals

    Infinity always takes a parenthesis, because it is not a number you can reach.

    x≥2  →  [2,∞)\displaystyle x \ge 2 \;\to\; [2, \infty)
    x<5  →  (−∞,5)\displaystyle x < 5 \;\to\; (-\infty, 5)
    all reals  →  (−∞,∞)\displaystyle \text{all reals} \;\to\; (-\infty, \infty)
  11. 4.13.11

    Unions of Intervals

    ∪\cup means “or”: everything in either interval.

    (−∞,1)∪[4,∞)\displaystyle (-\infty, 1) \cup [4, \infty)
  12. 4.13.12

    Intersections of Intervals

    ∩\cap means “and”: only the part both intervals share.

    [0,5]∩(3,8]=(3,5]\displaystyle [0, 5] \cap (3, 8] = (3, 5]
  13. 4.13.13

    Compound OR Inequalities

    Solve each part on its own. The answer is the union.

    x<−2  or  x≥1\displaystyle x < -2 \;\text{or}\; x \ge 1
    →  (−∞,−2)∪[1,∞)\displaystyle \to\; (-\infty, -2) \cup [1, \infty)
  14. 4.13.14

    Optimizing Sums, Differences, Products, and Quotients

    Given a range for each variable, pick the endpoints that push the result furthest. A difference is largest with the biggest first value and the smallest second value. For products and quotients with negatives, test all endpoint pairs.

    e.g. 2≤x≤52 \le x \le 5, 1≤y≤41 \le y \le 4: max of x−yx - y is 5−1=45 - 1 = 4, min of xy\tfrac{x}{y} is 24=12\tfrac24 = \tfrac12

    max⁡(x+y)=xmax⁡+ymax⁡\displaystyle \max(x + y) = x_{\max} + y_{\max}
    max⁡(x−y)=xmax⁡−ymin⁡\displaystyle \max(x - y) = x_{\max} - y_{\min}
    max⁡xy=xmax⁡ymin⁡  (x,y>0)\displaystyle \max\tfrac{x}{y} = \tfrac{x_{\max}}{y_{\min}}\ \ (x, y > 0)

4.14 Two-Variable Linear Inequalities

xy−5−4−3−2−1123456−4−3−2−112345test (0, 0)solutionsy > −½x + 2Test (0, 0): 0 > 2 is false,so shade the other side.Dashed for < and >Solid for ≤ and ≥
Draw the boundary line, decide dashed or solid, then use a test point to pick the side to shade.
  1. 4.14.1

    Graphing Strict Two-Variable Linear Inequalities

    For < or >, draw the boundary dashed, then shade the side that makes the inequality true. Test (0,0)(0, 0) if it isn’t on the line.

    y>mx+b\displaystyle y > mx + b
    →  dashed, shade above\displaystyle \to\; \text{dashed, shade above}
  2. 4.14.2

    Graphing Non-Strict Two-Variable Linear Inequalities

    For ≤ or ≥, draw the boundary solid, because points on the line count.

    y≤mx+b\displaystyle y \le mx + b
    →  solid, shade below\displaystyle \to\; \text{solid, shade below}
  3. 4.14.3

    Further Graphing of Two-Variable Linear Inequalities

    Rearrange into y=…y = \ldots first. Dividing by a negative flips the sign, which flips the shading.

    2x−3y>6  ⇒  y<23x−2\displaystyle 2x - 3y > 6 \;\Rightarrow\; y < \tfrac{2}{3}x - 2
  4. 4.14.4

    Systems of Linear Inequalities

    Graph each inequality. The solutions are where all the shadings overlap.

4.15 Modeling With Inequalities

  1. 4.15.1

    Introduction to Modeling With Inequalities

    Translate the words: at least ≥, at most ≤, no more than ≤, more than >, fewer than <.

    e.g. “At least 18 years old” → a≥18a \ge 18

  2. 4.15.2

    Modeling With One-Step Inequalities

    Write it, solve it, then round in the direction the situation demands.

    e.g. Bags hold 12 lb, 50 lb of sand → 12b≥5012b \ge 50, b≥4.17b \ge 4.17 → 5 bags

  3. 4.15.3

    Modeling With Two-Step Inequalities

    A fixed amount plus a rate, compared with a limit.

    e.g. $40 budget, $10 entry plus $6 per ride → 10+6r≤4010 + 6r \le 40, r≤5r \le 5

    b+rx≤L\displaystyle b + rx \le L
  4. 4.15.4

    Modeling With Compound Inequalities

    A quantity that must stay inside a range gives a three-part inequality.

    e.g. Keep milk between 35°F and 40°F → 35≤T≤4035 \le T \le 40

  5. 4.15.5

    Modeling With Two-Variable Linear Inequalities

    A budget or capacity limit becomes ax+by≤Cax + by \le C. Only sensible points count, often whole and nonnegative.

    e.g. $60 for $5 books and $12 games: 5b+12g≤605b + 12g \le 60

  6. 4.15.6

    Modeling With Systems of Linear Inequalities

    Each constraint is one inequality. The workable choices lie in the overlap.

  7. 4.15.7

    Modeling and Solving Systems of Linear Inequalities Using Technology

    Enter each inequality in a graphing tool, read the overlap, and check its corner points.

Unit 5 32 topics

Geometry - Points, Lines, & Angles

Introduction to Geometry, Angles, Advanced Angles, and Geometric Transformations.

5.16 Introduction to Geometry

ABLineno endsABRayone endABSegmenttwo ends
Line, ray, segment. The arrowheads say which way it keeps going.
  1. 5.16.1

    Units of Area and Volume

    Area is in square units, volume in cubic units. To convert, square or cube the length conversion.

    1 ft2=122=144 in2\displaystyle 1\text{ ft}^2 = 12^2 = 144\text{ in}^2
    1 yd3=33=27 ft3\displaystyle 1\text{ yd}^3 = 3^3 = 27\text{ ft}^3
  2. 5.16.2

    Points, Lines, Rays, and Segments

    A line runs forever both ways. A ray starts at a point and runs one way. A segment has two endpoints.

    AB↔AB→AB‾\displaystyle \overleftrightarrow{AB} \qquad \overrightarrow{AB} \qquad \overline{AB}
  3. 5.16.3

    Parallel and Perpendicular Lines

    Parallel lines never meet. Perpendicular lines meet at a right angle.

    ℓ∥mℓ⊥m\displaystyle \ell \parallel m \qquad \ell \perp m
  4. 5.16.4

    Measures of Segments

    ABAB with no bar means the length of AB‾\overline{AB}, a number.

    AB=length of AB‾\displaystyle AB = \text{length of } \overline{AB}
  5. 5.16.5

    Congruent Segments

    Same length. Marked with matching tick marks.

    AB‾≅CD‾  ⟺  AB=CD\displaystyle \overline{AB} \cong \overline{CD} \iff AB = CD
  6. 5.16.6

    Midpoints

    The point that splits a segment into two equal halves.

    AM=MB=12AB\displaystyle AM = MB = \tfrac{1}{2}AB
  7. 5.16.7

    Collinear Points

    Points that all lie on one line. Any two points are always collinear.

  8. 5.16.8

    The Segment Addition Postulate

    If BB is on the segment between AA and CC, the pieces add to the whole.

    e.g. AB=4AB = 4, BC=7BC = 7 → AC=11AC = 11

    AB+BC=AC\displaystyle AB + BC = AC

5.17 Angles

Acute< 90°Right= 90°Obtuse90°–180°Straight= 180°Reflex> 180°
Angle types by size. A full turn is 360°; a null angle is 0°.
  1. 5.17.1

    Angles and Measures of Angles

    Two rays from one point (the vertex). Measured in degrees. The vertex goes in the middle of the name.

    m∠ABC\displaystyle m\angle ABC
  2. 5.17.2

    Connecting Angles and Circles

    A full turn is 360°. A degree is 1360\tfrac{1}{360} of a full turn.

    e.g. Quarter turn =90∘= 90^\circ

    full turn=360∘\displaystyle \text{full turn} = 360^\circ
  3. 5.17.3

    Measuring Angles Using a Protractor

    Center on the vertex, line up 0 with one ray, read the scale that starts at 0 on that ray.

  4. 5.17.4

    Sums of Angles

    Angles side by side add up.

    m∠ABD=m∠ABC+m∠CBD\displaystyle m\angle ABD = m\angle ABC + m\angle CBD
  5. 5.17.5

    Right, Straight, Full, and Null Angles

    Right 90°, straight 180°, full 360°, null 0°.

    0∘90∘180∘360∘\displaystyle 0^\circ \quad 90^\circ \quad 180^\circ \quad 360^\circ
  6. 5.17.6

    Acute, Obtuse, and Reflex Angles

    Acute is less than 90°. Obtuse is between 90° and 180°. Reflex is between 180° and 360°.

  7. 5.17.7

    Congruent Angles

    Same measure. Marked with matching arcs.

    ∠A≅∠B  ⟺  m∠A=m∠B\displaystyle \angle A \cong \angle B \iff m\angle A = m\angle B
  8. 5.17.8

    Vertical Angles

    When two lines cross, the opposite angles are equal.

  9. 5.17.9

    Solving Problems With Angles

    Write an equation from a known relationship (sum, equal, straight line), then solve.

    e.g. 2x+40=180⇒x=702x + 40 = 180 \Rightarrow x = 70

5.18 Advanced Angles

ℓmt12345678When ℓ ∥ m:Corresponding angles: congruent1 & 5, 2 & 6, 3 & 7, 4 & 8Alternate interior: congruent3 & 6, 4 & 5Consecutive interior: sum to 180°3 & 5, 4 & 6Vertical angles: congruent1 & 4, 2 & 3, 5 & 8, 6 & 7
The angle numbers used in the proofs below. Highlighted: 4 and 5, a pair of alternate interior angles.
  1. 5.18.1

    Complementary Angles

    Two angles that add to 90°.

    α+β=90∘\displaystyle \alpha + \beta = 90^\circ
  2. 5.18.2

    Non-Adjacent Complementary Angles

    They still add to 90° even when they are not side by side.

  3. 5.18.3

    Supplementary Angles

    Two angles that add to 180°. Side by side on a line, they form a linear pair.

    α+β=180∘\displaystyle \alpha + \beta = 180^\circ
  4. 5.18.4

    Corresponding Angles

    Same position at each crossing of the transversal. Equal when the lines are parallel.

  5. 5.18.5

    Alternate Angles

    On opposite sides of the transversal, both inside (or both outside) the lines. Equal when the lines are parallel.

  6. 5.18.6

    Consecutive Angles

    Same side of the transversal, both inside the lines. Supplementary when the lines are parallel.

    α+β=180∘\displaystyle \alpha + \beta = 180^\circ
  7. 5.18.7

    Angle Criteria for Parallel Lines

    Run it backward: equal corresponding angles, equal alternate angles, or supplementary consecutive angles prove the lines are parallel.

  8. 5.18.8

    Angle Bisectors

    A ray that splits an angle into two equal angles.

    e.g. Bisect 70° → two 35° angles

  9. 5.18.9

    Segment Bisectors and the Perpendicular Bisector Theorem

    A segment bisector passes through the midpoint. Any point on the perpendicular bisector is the same distance from both endpoints.

    PA=PB\displaystyle PA = PB

5.19 Geometric Transformations

TranslateslideReflectflipRotateturnDilatescale
Dashed: the original. Solid: the image. Translations, reflections, and rotations keep size and shape. A dilation keeps the shape and changes the size. A reflection reverses orientation.
  1. 5.19.1

    Translations of Geometric Figures

    Slide every point the same distance in the same direction. Size, shape, and orientation stay the same.

    e.g. Translate (2,1)(2, 1) by (3,−4)(3, -4) → (5,−3)(5, -3)

    (x,y)→(x+a, y+b)\displaystyle (x, y) \to (x + a,\ y + b)
  2. 5.19.2

    Rotations of Geometric Figures

    Turn every point through the same angle about a center. Counterclockwise is the positive direction. Size and shape stay the same.

    e.g. A 90° rotation carries each point a quarter of the way around the center

  3. 5.19.3

    Reflections of Geometric Figures in the Cartesian Plane

    Flip across a line: each point lands the same distance away on the other side. Orientation reverses.

    x-axis: (x,y)→(x, −y)\displaystyle x\text{-axis}:\ (x, y) \to (x,\ -y)
    y-axis: (x,y)→(−x, y)\displaystyle y\text{-axis}:\ (x, y) \to (-x,\ y)
    y=x: (x,y)→(y, x)\displaystyle y = x:\ (x, y) \to (y,\ x)
  4. 5.19.4

    Reflections of Figures Across Arbitrary Lines

    The mirror line is the perpendicular bisector of each point and its image. For a vertical or horizontal line, measure across and go the same distance past.

    e.g. Reflect (1,4)(1, 4) in x=3x = 3 → (5,4)(5, 4)

    x=k: (x,y)→(2k−x, y)\displaystyle x = k:\ (x, y) \to (2k - x,\ y)
    y=k: (x,y)→(x, 2k−y)\displaystyle y = k:\ (x, y) \to (x,\ 2k - y)
  5. 5.19.5

    Reflective Symmetry

    A line of symmetry is a mirror line that maps the shape onto itself. A regular nn-gon has nn of them.

    e.g. A rectangle has 2 lines of symmetry; a square has 4

  6. 5.19.6

    Rotational Symmetry

    A shape has rotational symmetry when a turn of less than 360° maps it onto itself. Its order is how many times it fits in one full turn.

    e.g. A regular hexagon has order 6: it fits every 60°

    smallest angle=360∘order\displaystyle \text{smallest angle} = \frac{360^\circ}{\text{order}}

Unit 6 27 topics

Geometry - Polygons & Solids

Triangles, Right Triangles, Polygons, and Solid Geometry.

6.20 Triangles

abcda + b + c = 180°d = a + bexterior angle equals thetwo far inside angles
The two triangle angle facts.
  1. 6.20.1

    Interior Angles of Triangles

    The three inside angles always add to 180°.

    a+b+c=180∘\displaystyle a + b + c = 180^\circ
  2. 6.20.2

    Exterior Angles of Triangles

    An outside angle equals the two inside angles not touching it.

    d=a+b\displaystyle d = a + b
  3. 6.20.3

    Problem Solving With Angles of Triangles

    Combine the 180° sum, the exterior angle rule, and straight-line facts.

  4. 6.20.4

    Classifying Triangles

    By sides: equilateral (3 equal), isosceles (2 equal), scalene (none). By angles: acute, right, obtuse.

  5. 6.20.5

    The Triangle Inequality

    Any two sides together are longer than the third.

    e.g. 3, 4, 8 fails: 3+4<83 + 4 < 8

    a+b>c\displaystyle a + b > c
  6. 6.20.6

    The Isosceles Triangle Theorem

    Two equal sides means the two base angles are equal, and the reverse is true too.

  7. 6.20.7

    Heights of Triangles

    A height runs from a vertex perpendicular to the line holding the opposite side. In an obtuse triangle it can land outside.

  8. 6.20.8

    Medians and Centroids of Triangles

    A median joins a vertex to the midpoint of the opposite side. The three medians meet at the centroid, 23\tfrac23 of the way along each median from its vertex. Its coordinates average the vertices’.

    e.g. Vertices (0,0),(6,0),(0,9)(0, 0), (6, 0), (0, 9) → centroid (2,3)(2, 3)

    G=(x1+x2+x33, y1+y2+y33)\displaystyle G = \left(\frac{x_1 + x_2 + x_3}{3},\ \frac{y_1 + y_2 + y_3}{3}\right)

6.21 Right Triangles

11√245°45°45°–45°–90°1√3230°60°30°–60°–90°a² + b² = c²for every right triangleScale the sides byany factor: theratios stay the same.
Memorize these two shapes. Any 45°–45°–90° triangle has sides in the ratio 1 : 1 : √2; any 30°–60°–90° triangle, 1 : √3 : 2. The hypotenuse is always the longest side.
  1. 6.21.1

    The Pythagorean Theorem

    In a right triangle, the square of the hypotenuse (the side opposite the right angle) equals the sum of the squares of the legs. It works in reverse too: if the sides fit, the angle is right.

    e.g. Legs 5 and 12 → c=169=13c = \sqrt{169} = 13

    a2+b2=c2\displaystyle a^2 + b^2 = c^2
  2. 6.21.2

    Isosceles Right Triangles

    The 45°–45°–90° triangle. The legs are equal and the hypotenuse is a leg times 2\sqrt2.

    e.g. Leg 4 → hypotenuse 424\sqrt2; hypotenuse 10 → legs 525\sqrt2

    s:s:s2\displaystyle s : s : s\sqrt{2}
  3. 6.21.3

    30-60-90 Triangles

    Half of an equilateral triangle. The short leg faces 30°; the hypotenuse is twice it; the long leg is 3\sqrt3 times it.

    e.g. Short leg 5 → long leg 535\sqrt3, hypotenuse 10

    s:s3:2s\displaystyle s : s\sqrt{3} : 2s
  4. 6.21.4

    The Area of an Isosceles Right Triangle

    The two legs are the base and the height.

    e.g. Leg 6 → A=18A = 18

    A=12s2\displaystyle A = \tfrac{1}{2}s^2
    A=14h2   from the hypotenuse h\displaystyle A = \tfrac{1}{4}h^2 \;\text{ from the hypotenuse } h
  5. 6.21.5

    The Area of a 30-60-90 Triangle

    The two legs are the base and the height.

    e.g. Short leg 2 → A=23A = 2\sqrt3

    A=12⋅s⋅s3=32s2\displaystyle A = \tfrac{1}{2} \cdot s \cdot s\sqrt{3} = \frac{\sqrt{3}}{2}s^2
  6. 6.21.6

    The Area of an Equilateral Triangle

    Its height splits it into two 30-60-90 triangles, so the height is 32\tfrac{\sqrt3}{2} of a side.

    e.g. Side 6 → A=93A = 9\sqrt3

    h=32s\displaystyle h = \frac{\sqrt{3}}{2}s
    A=34s2\displaystyle A = \frac{\sqrt{3}}{4}s^2
  7. 6.21.7

    Diagonals of Squares

    A diagonal cuts a square into two isosceles right triangles.

    e.g. Side 7 → diagonal 727\sqrt2

    d=s2\displaystyle d = s\sqrt{2}
    A=12d2\displaystyle A = \tfrac{1}{2}d^2
  8. 6.21.8

    Recognizing 30-60-90 Triangles

    The sides are in the ratio 1:3:21 : \sqrt3 : 2. The short leg is opposite 30∘30^\circ, the hypotenuse is twice the short leg, and the long leg is 3\sqrt3 times the short leg. A right triangle with a hypotenuse twice one leg is a 30-60-90.

    e.g. Hypotenuse 10: short leg 5, long leg 535\sqrt3

    x:x3:2x\displaystyle x : x\sqrt3 : 2x
  9. 6.21.9

    Solving Geometry Problems by Manipulating Radicals

    Simplify by pulling out perfect squares and rationalizing denominators so answers match the choices.

    e.g. A square with diagonal 6 has side 62=32\tfrac{6}{\sqrt2} = 3\sqrt2 and area (32)2=18(3\sqrt2)^2 = 18

    ab=a b\displaystyle \sqrt{ab} = \sqrt a\,\sqrt b
    ab=abb\displaystyle \frac{a}{\sqrt b} = \frac{a\sqrt b}{b}

6.22 Polygons

MABCDOpposite sides parallelOpposite sides equalOpposite angles equalDiagonals bisect each otherNeighboring angles add to 180°
Arrowheads mark parallel sides, tick marks mark equal lengths, and matching arcs mark equal angles. The diagonals cut each other in half at M.
  1. 6.22.1

    Polygons

    A closed shape made of straight sides. Named by side count: 3 triangle, 4 quadrilateral, 5 pentagon, 6 hexagon, 8 octagon, 10 decagon.

  2. 6.22.2

    Interior Angles of Polygons

    Split into n−2n - 2 triangles from one vertex.

    e.g. Hexagon: 4×180=720∘4 \times 180 = 720^\circ

    sum=(n−2)×180∘\displaystyle \text{sum} = (n - 2) \times 180^\circ
  3. 6.22.3

    Exterior Angles of Polygons

    One at each vertex, and they always add to 360°, whatever the number of sides.

    sum=360∘\displaystyle \text{sum} = 360^\circ
  4. 6.22.4

    Congruent Polygons

    Same shape and size: every matching side and angle is equal. List vertices in matching order.

  5. 6.22.5

    Regular Polygons

    All sides equal and all angles equal.

    e.g. Regular octagon: 135∘135^\circ inside

    each interior=(n−2)×180∘n\displaystyle \text{each interior} = \frac{(n - 2) \times 180^\circ}{n}
    each exterior=360∘n\displaystyle \text{each exterior} = \frac{360^\circ}{n}
  6. 6.22.6

    Properties of Rectangles and Squares

    Opposite sides equal and parallel, four right angles, equal diagonals that cut each other in half. A square’s diagonals also meet at right angles.

6.23 Solid Geometry

rhrhℓrCylinderV = πr²hSA = 2πr² + 2πrhConeV = ⅓πr²hSA = πr² + πrℓSphereV = ⁴⁄₃πr³SA = 4πr²
A cone holds exactly one third of the cylinder with the same base and height. The cone’s slant height ℓ, not its height h, goes in the surface area.
  1. 6.23.1

    Identifying Three-Dimensional Shapes

    A prism has two congruent, parallel bases joined by rectangles or parallelograms. A pyramid has one polygon base and triangular faces that meet at a point (the apex). Cylinders, cones, and spheres have curved surfaces, so they are not polyhedrons.

    e.g. Two triangular bases and three rectangular faces: a triangular prism

  2. 6.23.2

    Faces, Vertices, and Edges of Polyhedrons

    A polyhedron is a solid whose faces are all flat polygons. Edges are where two faces meet, and vertices are the corners where edges meet. For a base with nn sides:

    e.g. Hexagonal prism (n=6n = 6): F=8F = 8, V=12V = 12, E=18E = 18

    Prism: F=n+2,  V=2n,  E=3n\displaystyle \text{Prism: } F = n + 2,\; V = 2n,\; E = 3n
    Pyramid: F=n+1,  V=n+1,  E=2n\displaystyle \text{Pyramid: } F = n + 1,\; V = n + 1,\; E = 2n
  3. 6.23.3

    Nets of Polyhedrons

    A net is a flat pattern that folds up into a solid. Every face appears exactly once, and faces that share an edge in the solid must connect correctly when folded.

    e.g. A square pyramid's net is a square with a triangle attached to each of its four sides.

  4. 6.23.4

    Finding Surface Areas Using Nets

    Surface area is the total area of all the faces. Unfold the solid into a net, find the area of each face, and add them.

    e.g. 2×3×42 \times 3 \times 4 box: faces 6,6,8,8,12,126, 6, 8, 8, 12, 12, so SA=52SA = 52

Unit 7 24 topics

Geometry - Congruence & Similarity

Congruence, and Similarity.

7.24 Congruence

SSSthree sidesSASangle between sidesASAside between anglesAASside not betweenHLright triangles only
Thick sides and shaded angles are the parts that must match. Any one of these five is enough to prove two triangles congruent. SSA and AAA are not.
  1. 7.24.1

    The ASA Congruence Criterion

    Two angles and the side between them match, so the triangles are congruent.

    ∠A≅∠D,AB‾≅DE‾,∠B≅∠E\displaystyle \angle A \cong \angle D,\quad \overline{AB} \cong \overline{DE},\quad \angle B \cong \angle E
    ⇒  △ABC≅△DEF\displaystyle \Rightarrow\; \triangle ABC \cong \triangle DEF
  2. 7.24.2

    The AAS Congruence Criterion

    Two angles and a side that is not between them. It works because the third angles must also match (the angles sum to 180°), which turns it into ASA.

  3. 7.24.3

    The SAS Congruence Criterion

    Two sides and the angle between them. The angle must be the one the two sides form.

    AB‾≅DE‾,∠A≅∠D,AC‾≅DF‾\displaystyle \overline{AB} \cong \overline{DE},\quad \angle A \cong \angle D,\quad \overline{AC} \cong \overline{DF}
  4. 7.24.4

    The SSS Congruence Criterion

    All three pairs of sides match. Three side lengths fix a triangle’s shape completely.

  5. 7.24.5

    The HL Congruence Criterion

    Right triangles only: the hypotenuse and one leg match. The Pythagorean theorem forces the other legs to match too.

  6. 7.24.6

    Combining Congruence Criteria for Triangles

    List what is given, add what you can deduce (a shared side, vertical angles, a third angle), then pick the criterion that fits. SSA and AAA do not prove congruence.

    e.g. A side shared by two triangles is congruent to itself (reflexive property)

  7. 7.24.7

    Solving Problems Describing Congruent Triangles

    In a congruence statement, the letter order tells which parts match. Corresponding sides and angles are equal, so set them equal and solve.

    e.g. △ABC≅△DEF\triangle ABC \cong \triangle DEF, AB=2x+1AB = 2x + 1, DE=9DE = 9: 2x+1=92x + 1 = 9, so x=4x = 4

    △ABC≅△DEF\displaystyle \triangle ABC \cong \triangle DEF
    ⇒  AB=DE, ∠C≅∠F\displaystyle \Rightarrow\; AB = DE,\ \angle C \cong \angle F
  8. 7.24.8

    Reasoning About Congruent Triangles

    Triangles are congruent by SSS, SAS, ASA, AAS, or HL (right triangles only). SSA and AAA do not prove congruence. Once congruent, matching parts are congruent (CPCTC).

    AB≅CB, AD≅CDgiven\displaystyle AB \cong CB,\ AD \cong CD \quad \text{given}
    BD≅BDreflexive\displaystyle BD \cong BD \quad \text{reflexive}
    △ABD≅△CBDSSS\displaystyle \triangle ABD \cong \triangle CBD \quad \text{SSS}
    ∠A≅∠CCPCTC\displaystyle \angle A \cong \angle C \quad \text{CPCTC}

7.25 Similarity

4358610k = 2sides × k3, 4, 5 → 6, 8, 10angles stay the samematching arcs = equal anglesarea × k²6 → 24, which is × 4volume × k³ (solids)k = 2 gives × 8
Multiplying every side by k = 2 keeps the angles the same. Area grows by k², so the bigger triangle has 4 times the area.
  1. 7.25.1

    Similarity and Similar Polygons

    Two polygons are similar (∼\sim) when all corresponding angles are congruent and all corresponding sides are in the same ratio. That ratio is the scale factor kk.

    e.g. A 2×32 \times 3 rectangle and a 4×64 \times 6 rectangle are similar with k=2k = 2.

    ABCD∼EFGH\displaystyle ABCD \sim EFGH
    EFAB=FGBC=⋯=k\displaystyle \frac{EF}{AB} = \frac{FG}{BC} = \cdots = k
  2. 7.25.2

    Side Lengths and Angle Measures of Similar Polygons

    Corresponding angles have equal measures. To find a missing side, set up a proportion using sides in the same order as the similarity statement.

    e.g. △ABC∼△DEF\triangle ABC \sim \triangle DEF, AB=4AB = 4, DE=6DE = 6, BC=5BC = 5: 46=5EF⇒EF=7.5\tfrac46 = \tfrac{5}{EF} \Rightarrow EF = 7.5

    ABDE=BCEF=ACDF\displaystyle \frac{AB}{DE} = \frac{BC}{EF} = \frac{AC}{DF}
  3. 7.25.3

    Areas of Similar Polygons

    If the scale factor between similar polygons is kk, the ratio of their areas is k2k^2.

    e.g. Scale factor 3 and smaller area 5 cm²: larger area =5⋅9=45= 5 \cdot 9 = 45 cm²

    A2A1=(s2s1)2=k2\displaystyle \frac{A_2}{A_1} = \left(\frac{s_2}{s_1}\right)^2 = k^2
  4. 7.25.4

    Working With Areas of Similar Polygons

    To go from an area ratio back to a side ratio, take the square root.

    e.g. Areas 16 and 25 give side ratio 4:54 : 5. A side of 8 on the smaller figure matches 1010 on the larger.

    k=A2A1\displaystyle k = \sqrt{\frac{A_2}{A_1}}
  5. 7.25.5

    Working With Descriptions of Similar Shapes

    Similar shapes have equal corresponding angles and proportional corresponding sides. The letter order in a statement like ABCD∼EFGHABCD \sim EFGH tells you which parts match.

    e.g. ABCD∼EFGHABCD \sim EFGH, AB=4AB = 4, EF=6EF = 6, BC=10BC = 10: scale factor 64=1.5\tfrac64 = 1.5, so FG=15FG = 15

    ABEF=BCFG=CDGH\displaystyle \frac{AB}{EF} = \frac{BC}{FG} = \frac{CD}{GH}
  6. 7.25.6

    The AA Similarity Criterion

    If two angles of one triangle are congruent to two angles of another, the triangles are similar.

    e.g. Two triangles each have angles 40∘40^\circ and 60∘60^\circ, so they are similar (both have a third angle of 80∘80^\circ).

    ∠A≅∠D,  ∠B≅∠E\displaystyle \angle A \cong \angle D,\; \angle B \cong \angle E
    ⇒  △ABC∼△DEF\displaystyle \Rightarrow\; \triangle ABC \sim \triangle DEF
  7. 7.25.7

    The SSS Similarity Criterion

    If all three pairs of corresponding sides are in the same ratio, the triangles are similar.

    e.g. Sides 3, 4, 5 and 6, 8, 10: every ratio is 2, so the triangles are similar.

    DEAB=EFBC=DFAC\displaystyle \frac{DE}{AB} = \frac{EF}{BC} = \frac{DF}{AC}
  8. 7.25.8

    The SAS Similarity Criterion

    If two pairs of sides are in the same ratio and the angles between them (the included angles) are congruent, the triangles are similar.

    e.g. AB=4AB = 4, AC=6AC = 6, DE=6DE = 6, DF=9DF = 9, ∠A=∠D=50∘\angle A = \angle D = 50^\circ: both ratios are 1.5, so similar.

    DEAB=DFAC,  ∠A≅∠D\displaystyle \frac{DE}{AB} = \frac{DF}{AC},\; \angle A \cong \angle D
  9. 7.25.9

    Combining Similarity Criteria for Triangles

    Pick the criterion that fits the given facts: AA for angles, SSS for three sides, SAS for two sides and the included angle. Look for hidden facts such as a shared angle, vertical angles, or parallel lines.

    e.g. DD on AB‾\overline{AB}, EE on AC‾\overline{AC}, AD=2AD = 2, AB=6AB = 6, AE=3AE = 3, AC=9AC = 9: ratios both 13\tfrac13 with shared ∠A\angle A, so △ADE∼△ABC\triangle ADE \sim \triangle ABC by SAS.

  10. 7.25.10

    Solving Angle Problems From Descriptions of Similar Triangles

    Corresponding angles of similar triangles are equal. Match angles by letter position, then use the triangle angle sum of 180∘180^\circ.

    e.g. △ABC∼△DEF\triangle ABC \sim \triangle DEF, ∠A=50∘\angle A = 50^\circ, ∠E=70∘\angle E = 70^\circ: ∠F=∠C=180∘−50∘−70∘=60∘\angle F = \angle C = 180^\circ - 50^\circ - 70^\circ = 60^\circ

    △ABC∼△DEF\displaystyle \triangle ABC \sim \triangle DEF
    ⇒  ∠A=∠D, ∠B=∠E\displaystyle \Rightarrow\; \angle A = \angle D,\ \angle B = \angle E
    ∠C=∠F\displaystyle \angle C = \angle F
  11. 7.25.11

    Reasoning About Similar Triangles

    Triangles are similar by AA (two pairs of equal angles), SSS (all sides in the same ratio), or SAS (two sides in the same ratio with equal included angles). Similar triangles have equal side ratios within each triangle, so their trig ratios match.

    e.g. A 3-4-5 right triangle is similar to one with short leg 9: scale factor 3, so the sides are 9, 12, 15

    AA, SSS, SAS similarity\displaystyle \text{AA},\ \text{SSS},\ \text{SAS similarity}
    ABBC=DEEF\displaystyle \frac{AB}{BC} = \frac{DE}{EF}
  12. 7.25.12

    Solving Parallel Line Problems From Descriptions

    A line parallel to one side of a triangle cuts off a smaller triangle similar to the original. It also divides the other two sides proportionally.

    e.g. AD=3AD = 3, AB=9AB = 9, BC=12BC = 12: DE=12⋅39=4DE = 12 \cdot \tfrac39 = 4

    DE∥BC⇒△ADE∼△ABC\displaystyle DE \parallel BC \Rightarrow \triangle ADE \sim \triangle ABC
    ADAB=AEAC=DEBC\displaystyle \frac{AD}{AB} = \frac{AE}{AC} = \frac{DE}{BC}
    ADDB=AEEC\displaystyle \frac{AD}{DB} = \frac{AE}{EC}
  13. 7.25.13

    The Midpoint Theorem

    The segment joining the midpoints of two sides of a triangle is parallel to the third side and half as long.

    e.g. DD, EE are midpoints of AB‾\overline{AB}, AC‾\overline{AC} and BC=14BC = 14, so DE=7DE = 7.

    DE∥BC\displaystyle DE \parallel BC
    DE=12BC\displaystyle DE = \tfrac12 BC
  14. 7.25.14

    The Triangle Proportionality Theorem

    A line parallel to one side of a triangle divides the other two sides proportionally. The converse is also true.

    e.g. AD=4AD = 4, DB=6DB = 6, AE=6AE = 6: 46=6EC⇒EC=9\tfrac46 = \tfrac{6}{EC} \Rightarrow EC = 9

    DE∥BC\displaystyle DE \parallel BC
    ⇒  ADDB=AEEC\displaystyle \Rightarrow\; \frac{AD}{DB} = \frac{AE}{EC}
  15. 7.25.15

    Surface Areas and Volumes of Similar Solids

    If two similar solids have scale factor kk (ratio of corresponding lengths), their surface areas are in ratio k2k^2 and their volumes in ratio k3k^3.

    e.g. Lengths 2:32 : 3, so volumes 8:278 : 27. Small volume 16 → large volume 16⋅278=5416 \cdot \tfrac{27}{8} = 54

    A1A2=k2\displaystyle \frac{A_1}{A_2} = k^2
    V1V2=k3\displaystyle \frac{V_1}{V_2} = k^3
  16. 7.25.16

    Working With Descriptions of Similar Solids

    If two solids are similar with scale factor kk, every length scales by kk, every area by k2k^2, and the volume by k3k^3.

    e.g. Similar cylinders with radii 2 and 6: k=3k = 3. Small volume 10π10\pi → large volume 10π⋅27=270π10\pi \cdot 27 = 270\pi

    length×k\displaystyle \text{length} \times k
    surface area×k2\displaystyle \text{surface area} \times k^2
    volume×k3\displaystyle \text{volume} \times k^3

Unit 8 35 topics

Geometry - Length, Area & Volume

Perimeter & Area of Plane Figures, Coordinate Geometry, Inscribed Shapes in Two Dimensions, and Surface Area and Volume.

8.26 Perimeter & Area of Plane Figures

lwA = lwbhA = bhbhA = ½bhb1b2hA = ½(b1 + b2)h
Height is always measured straight up from the base, at a right angle. Never use the slanted side.
  1. 8.26.1

    The Perimeter of a Polygon

    Add up the sides. For a regular polygon, multiply.

    P=n⋅s(regular)\displaystyle P = n \cdot s \quad \text{(regular)}
  2. 8.26.2

    Areas of Rectangles and Squares

    Length times width.

    A=lw\displaystyle A = lw
    A=s2\displaystyle A = s^2
  3. 8.26.3

    Areas of Parallelograms

    Base times the perpendicular height, not the slanted side.

    A=bh\displaystyle A = bh
  4. 8.26.4

    Areas of Triangles

    Half of a parallelogram.

    A=12bh\displaystyle A = \tfrac{1}{2}bh
  5. 8.26.5

    Areas of Trapezoids

    Average the two bases, times the height.

    A=12(b1+b2)h\displaystyle A = \tfrac{1}{2}(b_1 + b_2)h
  6. 8.26.6

    Areas and Perimeters of Composite Shapes

    Split into simple shapes and add the areas. For perimeter, count only the outside edges.

  7. 8.26.7

    The Area Between Two Shapes

    Big area minus small area.

    A=Aouter−Ainner\displaystyle A = A_{\text{outer}} - A_{\text{inner}}
  8. 8.26.8

    Border Problems

    The area of a border is the outer area minus the inner area. A border of uniform width xx adds 2x2x to each dimension.

    e.g. An 8 in by 6 in photo with a 1 in frame: 10⋅8−8⋅6=80−48=3210 \cdot 8 - 8 \cdot 6 = 80 - 48 = 32 in²

    Aborder=Aouter−Ainner\displaystyle A_{\text{border}} = A_{\text{outer}} - A_{\text{inner}}
    outer=(l+2x)(w+2x)\displaystyle \text{outer} = (l + 2x)(w + 2x)
  9. 8.26.9

    Constructing Functions Representing Properties of 2D Shapes

    Write every dimension in terms of one variable, then substitute into the perimeter or area formula.

    e.g. Area of a square in terms of its perimeter pp: side p4\tfrac{p}{4}, so A(p)=p216A(p) = \tfrac{p^2}{16}

    A(w)=w(w+3)\displaystyle A(w) = w(w + 3)
    P(w)=2w+2(w+3)=4w+6\displaystyle P(w) = 2w + 2(w + 3) = 4w + 6

8.27 Coordinate Geometry

2468246810A(1, 1)B(7, 9)M(4, 5)Δx = 6Δy = 8d = √(Δx² + Δy²)= √(36 + 64) = 10M = average of the coordinates= ((1 + 7)/2, (1 + 9)/2) = (4, 5)slope = Δy/Δx = 8/6 = 4/3perpendicular slope = −3/4
The changes in x and y form a right triangle, so distance comes from the Pythagorean theorem. The midpoint averages the endpoints.
  1. 8.27.1

    Midpoints in the Coordinate Plane

    Average the xx-coordinates and average the yy-coordinates.

    e.g. (2,7)(2, 7) and (8,−1)(8, -1) → (5,3)(5, 3)

    M=(x1+x22, y1+y22)\displaystyle M = \left(\frac{x_1 + x_2}{2},\ \frac{y_1 + y_2}{2}\right)
  2. 8.27.2

    The Distance Formula

    The Pythagorean theorem applied to the horizontal and vertical changes.

    e.g. (1,2)(1, 2) to (4,6)(4, 6) → 9+16=5\sqrt{9 + 16} = 5

    d=(x2−x1)2+(y2−y1)2\displaystyle d = \sqrt{(x_2 - x_1)^2 + (y_2 - y_1)^2}
  3. 8.27.3

    Calculating Perimeters in the Plane

    Find each side with the distance formula and add. Horizontal and vertical sides are simple differences.

    e.g. Triangle (0,0),(4,0),(4,3)(0, 0), (4, 0), (4, 3): 4+3+5=124 + 3 + 5 = 12

    P=sum of the side lengths\displaystyle P = \text{sum of the side lengths}
  4. 8.27.4

    Calculating Areas of Rectangles in the Plane

    Find two adjacent sides with the distance formula and multiply. Check the corner is square: the slopes multiply to −1-1.

    e.g. (0,0),(4,2),(3,4),(−1,2)(0, 0), (4, 2), (3, 4), (-1, 2): sides 20\sqrt{20} and 5\sqrt5 → A=10A = 10

    A=l×w\displaystyle A = l \times w
  5. 8.27.5

    Calculating Areas of Triangles and Quadrilaterals in the Plane

    Use a horizontal or vertical side as the base when you can. Otherwise box the shape in a rectangle and subtract the corner triangles, or use the formula below.

    e.g. (0,0),(6,0),(2,5)(0, 0), (6, 0), (2, 5): base 6, height 5 → A=15A = 15

    A=12∣x1(y2−y3)+x2(y3−y1)\displaystyle A = \tfrac{1}{2}\big\lvert x_1(y_2 - y_3) + x_2(y_3 - y_1)
    +x3(y1−y2)∣\displaystyle \qquad + x_3(y_1 - y_2)\big\rvert
  6. 8.27.6

    Equations of Tangent Lines to Circles

    The tangent at point PP is perpendicular to the radius to PP. Its slope is the negative reciprocal of the radius slope. A horizontal radius gives a vertical tangent, and vice versa.

    e.g. x2+y2=25x^2 + y^2 = 25 at (3,4)(3, 4): radius slope 43\tfrac43, tangent y−4=−34(x−3)y - 4 = -\tfrac34(x - 3)

    mtan=−1mradius\displaystyle m_{\text{tan}} = -\frac{1}{m_{\text{radius}}}
    y−y1=m(x−x1)\displaystyle y - y_1 = m(x - x_1)

8.28 Inscribed Shapes in Two Dimensions

  1. 8.28.1

    Circles Inscribed in Squares

    The circle touches all four sides, so its diameter equals the side of the square.

    e.g. Side 10 → r=5r = 5, area 25π25\pi

    d=s,r=s2\displaystyle d = s,\quad r = \tfrac{s}{2}
    Acircle=π4s2\displaystyle A_{\text{circle}} = \frac{\pi}{4}s^2
  2. 8.28.2

    Squares Inscribed in Circles

    The square’s corners touch the circle, so its diagonal is a diameter.

    e.g. r=5r = 5 → side 525\sqrt2, area 50

    s2=2r  ⇒  s=r2\displaystyle s\sqrt{2} = 2r \;\Rightarrow\; s = r\sqrt{2}
    Asquare=2r2\displaystyle A_{\text{square}} = 2r^2
  3. 8.28.3

    Equilateral Triangles Inscribed in Circles

    The circle's center is the triangle's center. The radius RR is 23\tfrac23 of the triangle's height hh, and the side is R3R\sqrt3.

    e.g. R=4R = 4: s=43s = 4\sqrt3, area =34(43)2=34⋅48=123= \tfrac{\sqrt3}{4}(4\sqrt3)^2 = \tfrac{\sqrt3}{4} \cdot 48 = 12\sqrt3

    s=R3\displaystyle s = R\sqrt3
    R=s33=23h\displaystyle R = \frac{s\sqrt3}{3} = \frac23 h
  4. 8.28.4

    Circles Inscribed in Equilateral Triangles

    The inscribed circle's center is the triangle's center. Its radius rr is 13\tfrac13 of the height, which is half the circumscribed radius.

    e.g. s=6s = 6: h=33h = 3\sqrt3, r=3r = \sqrt3, circle area =3π= 3\pi

    r=s36=13h\displaystyle r = \frac{s\sqrt3}{6} = \frac13 h
    h=s32\displaystyle h = \frac{s\sqrt3}{2}
  5. 8.28.5

    Areas of Inscribed Triangles

    A triangle inscribed in a circle with a diameter as one side is a right triangle, so its legs are the base and height. A triangle with one side along a rectangle's side and its third vertex on the opposite side has half the rectangle's area.

    e.g. Circle of radius 5, a diameter as one side, one leg 6: other leg 100−36=8\sqrt{100 - 36} = 8, area =12⋅6⋅8=24= \tfrac12 \cdot 6 \cdot 8 = 24

    A=12bh\displaystyle A = \tfrac12 bh
    side is a diameter⇒90∘\displaystyle \text{side is a diameter} \Rightarrow 90^\circ

8.29 Surface Area and Volume

lhwdface diagonal√(l² + w²)space diagonald = √(l² + w² + h²)V = lwhSA = 2(lw + lh + wh)
The face diagonal across the bottom and the height form a right triangle whose hypotenuse is the space diagonal. Using the Pythagorean theorem twice gives d = √(l² + w² + h²).
  1. 8.29.1

    Volumes of Cubes

    Cube the edge length. To find the edge from the volume, take the cube root.

    e.g. s=4s = 4: V=64V = 64. V=125V = 125: s=1253=5s = \sqrt[3]{125} = 5

    V=s3\displaystyle V = s^3
  2. 8.29.2

    Surface Areas of Cubes

    A cube has 6 congruent square faces.

    e.g. s=3s = 3: SA=6⋅9=54SA = 6 \cdot 9 = 54

    SA=6s2\displaystyle SA = 6s^2
  3. 8.29.3

    Face Diagonals of Cubes

    A face diagonal crosses one square face from corner to corner. It is the hypotenuse of a 45-45-90 triangle with legs ss.

    e.g. s=5s = 5: d=52≈7.07d = 5\sqrt2 \approx 7.07

    d=s2\displaystyle d = s\sqrt{2}
  4. 8.29.4

    Surface Areas of Rectangular Solids

    Three pairs of congruent rectangular faces.

    e.g. 3×4×53 \times 4 \times 5: 2(12+15+20)=942(12 + 15 + 20) = 94

    SA=2(lw+lh+wh)\displaystyle SA = 2(lw + lh + wh)
  5. 8.29.5

    Volumes of Rectangular Solids

    Multiply length, width, and height.

    e.g. 3×4×53 \times 4 \times 5: V=60V = 60

    V=lwh\displaystyle V = lwh
  6. 8.29.6

    Volumes of Cylinders

    Base area times height, like a prism with a circular base.

    e.g. r=3r = 3, h=5h = 5: V=45π≈141.4V = 45\pi \approx 141.4

    V=πr2h\displaystyle V = \pi r^2 h
  7. 8.29.7

    Surface Areas of Cylinders

    Two circular bases plus the lateral surface, which unrolls into a rectangle 2πr2\pi r wide and hh tall.

    e.g. r=3r = 3, h=5h = 5: 18π+30π=48π≈150.818\pi + 30\pi = 48\pi \approx 150.8

    SA=2πr2+2πrh\displaystyle SA = 2\pi r^2 + 2\pi r h
  8. 8.29.8

    Volumes of Spheres

    A hemisphere has half the volume of the sphere.

    e.g. r=3r = 3: V=43⋅27π=36π≈113.1V = \tfrac43 \cdot 27\pi = 36\pi \approx 113.1

    V=43πr3\displaystyle V = \frac{4}{3}\pi r^3
  9. 8.29.9

    Slant Heights of Right Cones

    The radius, height, and slant height form a right triangle with the slant height ℓ\ell as the hypotenuse.

    e.g. r=5r = 5, h=12h = 12: ℓ=169=13\ell = \sqrt{169} = 13

    ℓ=r2+h2\displaystyle \ell = \sqrt{r^2 + h^2}
  10. 8.29.10

    Volumes of Right Cones

    One third of a cylinder with the same base and height. Use the perpendicular height, not the slant height.

    e.g. r=3r = 3, h=4h = 4: V=13⋅9⋅4π=12π≈37.7V = \tfrac13 \cdot 9 \cdot 4\pi = 12\pi \approx 37.7

    V=13πr2h\displaystyle V = \frac{1}{3}\pi r^2 h
  11. 8.29.11

    Volumes of Pyramids

    One third of base area times height. The height hh is perpendicular from the apex to the base, not the slant height.

    e.g. Square base side 6, h=5h = 5: V=13⋅36⋅5=60V = \tfrac13 \cdot 36 \cdot 5 = 60

    V=13Bh\displaystyle V = \frac{1}{3}Bh
  12. 8.29.12

    Constructing Functions Representing Properties of Rectangular Solids

    Write the length, width, and height in terms of one variable, then substitute into the volume or surface area formula.

    e.g. Square base of side xx, height 5: V(x)=5x2V(x) = 5x^2, S(x)=2(x2+5x+5x)=2x2+20xS(x) = 2(x^2 + 5x + 5x) = 2x^2 + 20x

    V=lwh\displaystyle V = lwh
    S=2(lw+lh+wh)\displaystyle S = 2(lw + lh + wh)
  13. 8.29.13

    Constructing Functions Representing Volumes of Cylinders, Cones, and Pyramids

    Write every dimension in terms of one variable, then substitute. A cone or pyramid has one third the volume of the cylinder or prism with the same base and height.

    e.g. Cone with height twice its radius: V(r)=13πr2(2r)=23πr3V(r) = \tfrac13 \pi r^2 (2r) = \tfrac23 \pi r^3

    Vcylinder=πr2h\displaystyle V_{\text{cylinder}} = \pi r^2 h
    Vcone=13πr2h\displaystyle V_{\text{cone}} = \frac13 \pi r^2 h
    Vpyramid=13Bh\displaystyle V_{\text{pyramid}} = \frac13 Bh
  14. 8.29.14

    Composite Solids

    Split the solid into simple pieces. Add volumes of the pieces and subtract any holes. For surface area, count only the faces on the outside.

    e.g. Cylinder (r=3r = 3, h=4h = 4) topped by a hemisphere: 36π+23π(27)=36π+18π=54π36\pi + \tfrac23 \pi (27) = 36\pi + 18\pi = 54\pi

    V=V1+V2−Vhole\displaystyle V = V_1 + V_2 - V_{\text{hole}}
  15. 8.29.15

    Surface Areas of Combined Prisms

    Add the two surface areas, then subtract twice the area where they touch, since that area is hidden on both solids.

    e.g. Two unit cubes glued face to face: 6+6−2(1)=106 + 6 - 2(1) = 10

    S=S1+S2−2Aoverlap\displaystyle S = S_1 + S_2 - 2A_{\text{overlap}}

Unit 9 24 topics

Geometry - Circles

Circles, Circles in the Coordinate Plane, and Radians.

9.30 Circles

θrsectorarcchordsegmentC = 2πrcircumferenceA = πr²areaL = (θ/360°) · 2πrarc lengthA = (θ/360°) · πr²sector areaA sector is the fraction θ/360° of the whole circle.
An arc is part of the edge, a sector is a slice, and a segment is cut off by a chord. Arc length and sector area are the same fraction, θ/360°, of the whole.
  1. 9.30.1

    Circles

    Every point at a fixed distance, the radius, from the center. The diameter is twice the radius. A chord joins two points on the circle; a diameter is the longest chord.

    d=2r\displaystyle d = 2r
  2. 9.30.2

    Arcs, Segments, and Sectors of Circles

    An arc is part of the edge. A sector is a slice bounded by two radii and an arc. A segment is the region between a chord and its arc. Minor arcs are under 180°, major arcs over.

  3. 9.30.3

    The Circumference of a Circle

    The distance around. π≈3.14159\pi \approx 3.14159 is circumference divided by diameter for every circle.

    e.g. r=5r = 5 → C=10π≈31.4C = 10\pi \approx 31.4

    C=2πr=πd\displaystyle C = 2\pi r = \pi d
  4. 9.30.4

    Areas of Circles

    Square the radius, not the diameter.

    e.g. d=10d = 10 → r=5r = 5, A=25πA = 25\pi

    A=πr2\displaystyle A = \pi r^2
  5. 9.30.5

    Central Angles and Arcs

    A central angle has its vertex at the center. The arc it cuts off has the same degree measure.

    arc measure=central angle\displaystyle \text{arc measure} = \text{central angle}
    whole circle=360∘\displaystyle \text{whole circle} = 360^\circ
  6. 9.30.6

    Calculating Arc Lengths of Circular Sectors

    The arc is the angle’s share of the whole circumference.

    e.g. r=6r = 6, θ=60∘\theta = 60^\circ → L=16⋅12π=2πL = \tfrac16 \cdot 12\pi = 2\pi

    L=θ360∘⋅2πr\displaystyle L = \frac{\theta}{360^\circ} \cdot 2\pi r
  7. 9.30.7

    Calculating Areas of Circular Sectors

    The sector is the angle’s share of the whole area.

    e.g. r=6r = 6, θ=60∘\theta = 60^\circ → A=16⋅36π=6πA = \tfrac16 \cdot 36\pi = 6\pi

    A=θ360∘⋅πr2\displaystyle A = \frac{\theta}{360^\circ} \cdot \pi r^2
  8. 9.30.8

    Further Calculating Areas of Sectors

    Work backward from an area or arc length to the angle or radius. Arc length and sector area are linked.

    e.g. Area 12π12\pi, r=6r = 6 → 12π36π=13\tfrac{12\pi}{36\pi} = \tfrac13 of the circle → θ=120∘\theta = 120^\circ

    A=12rL\displaystyle A = \tfrac{1}{2}rL
  9. 9.30.9

    Problem Solving With Circles

    Break the region into circles, sectors, and polygons, then add or subtract. A segment is a sector minus its triangle.

    e.g. Quarter circle of radius 4: segment =4π−8= 4\pi - 8

    Asegment=Asector−Atriangle\displaystyle A_{\text{segment}} = A_{\text{sector}} - A_{\text{triangle}}
  10. 9.30.10

    Tangent Lines to Circles

    A tangent line touches the circle at exactly one point and is perpendicular to the radius at that point. This makes a right triangle with the center and any outside point on the tangent.

    e.g. Radius 5, center to outside point 13: tangent length =169−25=12= \sqrt{169 - 25} = 12

    OP‾⊥tangent at P\displaystyle \overline{OP} \perp \text{tangent at } P
    r2+t2=d2\displaystyle r^2 + t^2 = d^2
  11. 9.30.11

    Tangent-Tangent Lines to Circles

    Two tangent segments from the same outside point are congruent. The angle between them is half the difference of the far and near arcs, which equals 180∘180^\circ minus the central angle.

    e.g. Near arc 120∘120^\circ, far arc 240∘240^\circ: m∠P=12(240−120)=60∘m\angle P = \tfrac12(240 - 120) = 60^\circ

    PA=PB\displaystyle PA = PB
    m∠P=12(far−near)\displaystyle m\angle P = \tfrac12(\text{far} - \text{near})
    =180∘−m∠AOB\displaystyle = 180^\circ - m\angle AOB
  12. 9.30.12

    Isosceles Triangles in Circles

    Two radii and a chord form an isosceles triangle, so its base angles are equal. The perpendicular from the center to the chord bisects the chord.

    e.g. Central angle 100∘100^\circ: base angles 40∘40^\circ. Radius 5, chord 3 from center: half chord 4, chord 8

    base angle=180∘−θ2\displaystyle \text{base angle} = \frac{180^\circ - \theta}{2}
    (c2)2+d2=r2\displaystyle \left(\tfrac{c}{2}\right)^2 + d^2 = r^2
  13. 9.30.13

    Perpendicular Bisectors of Chords

    The perpendicular bisector of any chord passes through the center. A radius perpendicular to a chord bisects it, which forms a right triangle with the radius.

    e.g. Radius 5, chord 8: distance from center =25−16=3= \sqrt{25 - 16} = 3

    (c2)2+d2=r2\displaystyle \left(\tfrac{c}{2}\right)^2 + d^2 = r^2

9.31 Circles in the Coordinate Plane

xy−2−10123456−3−2−1012345(h, k)r = 3(x, y)(x − h)² + (y − k)² = r²center (h, k), radius revery point is r from the centerHere: center (2, 1), r = 3(x − 2)² + (y − 1)² = 9Square the radius: 3² = 9
A circle is every point a fixed distance r from its center. The distance formula squared gives the equation, so the center is (2, 1) and the radius is 3.
  1. 9.31.1

    Circles in the Coordinate Plane

    A circle is every point at distance rr from the center. Use the distance formula to find a radius or test whether a point is on the circle.

    e.g. Center (1,2)(1, 2) through (4,6)(4, 6): r=9+16=5r = \sqrt{9 + 16} = 5

    d=(x2−x1)2+(y2−y1)2\displaystyle d = \sqrt{(x_2 - x_1)^2 + (y_2 - y_1)^2}
  2. 9.31.2

    Equations of Circles Centered at the Origin

    A circle with center (0,0)(0, 0) and radius rr.

    e.g. Through (3,4)(3, 4): r2=9+16=25r^2 = 9 + 16 = 25, so x2+y2=25x^2 + y^2 = 25

    x2+y2=r2\displaystyle x^2 + y^2 = r^2
  3. 9.31.3

    Equations of Circles

    Standard form for center (h,k)(h, k) and radius rr. Watch the signs: (x+3)(x + 3) means h=−3h = -3.

    e.g. Center (2,−3)(2, -3), r=4r = 4: (x−2)2+(y+3)2=16(x - 2)^2 + (y + 3)^2 = 16

    (x−h)2+(y−k)2=r2\displaystyle (x - h)^2 + (y - k)^2 = r^2
  4. 9.31.4

    Determining Circle Properties by Completing the Square

    Group the xx terms and the yy terms, move the constant, and complete the square on each. Add the same amounts to both sides.

    e.g. x2+y2−6x+4y−3=0⇒(x−3)2+(y+2)2=16x^2 + y^2 - 6x + 4y - 3 = 0 \Rightarrow (x - 3)^2 + (y + 2)^2 = 16: center (3,−2)(3, -2), r=4r = 4

    x2+Dx=(x+D2)2−D24\displaystyle x^2 + Dx = \left(x + \tfrac{D}{2}\right)^2 - \tfrac{D^2}{4}
  5. 9.31.5

    Calculating Circle Intercepts

    For xx-intercepts set y=0y = 0. For yy-intercepts set x=0x = 0. A circle can have 0, 1, or 2 of each.

    e.g. (x−3)2+y2=25(x - 3)^2 + y^2 = 25: x=8,−2x = 8, -2 and y=±4y = \pm 4

    x-intercepts: y=0\displaystyle x\text{-intercepts: } y = 0
    y-intercepts: x=0\displaystyle y\text{-intercepts: } x = 0
  6. 9.31.6

    Intersections of Circles with Lines

    Substitute the line into the circle and solve the quadratic. Two solutions means the line crosses twice, one means it is tangent, none means it misses.

    e.g. x2+y2=25x^2 + y^2 = 25, y=x+1y = x + 1: x2+x−12=0x^2 + x - 12 = 0, so (3,4)(3, 4) and (−4,−3)(-4, -3)

  7. 9.31.7

    Transforming Circles

    A circle (x−h)2+(y−k)2=r2(x - h)^2 + (y - k)^2 = r^2 has center (h,k)(h, k). A translation moves the center and keeps rr. A dilation by a factor cc about the origin multiplies the center coordinates and the radius by cc.

    e.g. (x−1)2+(y+2)2=9(x - 1)^2 + (y + 2)^2 = 9 moved left 3 and up 5: (x+2)2+(y−3)2=9(x + 2)^2 + (y - 3)^2 = 9

    (x−h)2+(y−k)2=r2\displaystyle (x - h)^2 + (y - k)^2 = r^2

9.32 Radians

1 radianrrarc = r2π radians = 360°π radians = 180°1 radian ≈ 57.3°arc s = rθsector A = ½r²θ(θ in radians)
One radian is the angle whose arc is exactly as long as the radius. About 6.28 radii fit around the circle, so 2π radians make a full turn.
  1. 9.32.1

    Introduction to Radians

    One radian is the central angle whose arc equals the radius. A full turn is 2π2\pi radians, so 180∘=π180^\circ = \pi radians.

    e.g. 135∘=135π180=3π4135^\circ = \tfrac{135\pi}{180} = \tfrac{3\pi}{4}; π6=30∘\tfrac{\pi}{6} = 30^\circ

    180∘=π rad\displaystyle 180^\circ = \pi \text{ rad}
    rad=deg⋅π180\displaystyle \text{rad} = \text{deg} \cdot \frac{\pi}{180}
    deg=rad⋅180π\displaystyle \text{deg} = \text{rad} \cdot \frac{180}{\pi}
  2. 9.32.2

    Calculating Arc Length Using Radians

    Arc length is radius times the central angle, with θ\theta in radians. Convert degrees first.

    e.g. r=6r = 6, θ=2π3\theta = \tfrac{2\pi}{3}: s=4π≈12.57s = 4\pi \approx 12.57

    s=rθ\displaystyle s = r\theta
  3. 9.32.3

    Calculating Areas of Sectors Using Radians

    A sector is the slice of a circle between two radii. Use θ\theta in radians.

    e.g. r=6r = 6, θ=π3\theta = \tfrac{\pi}{3}: A=12⋅36⋅π3=6π≈18.85A = \tfrac12 \cdot 36 \cdot \tfrac{\pi}{3} = 6\pi \approx 18.85

    A=12r2θ\displaystyle A = \frac{1}{2}r^2\theta
  4. 9.32.4

    Trigonometric Ratios With Radians

    The ratios are the same; only the angle units change. Convert to degrees or memorize the special angles, and set the calculator to radian mode.

    e.g. sin⁡π6=12\sin\tfrac{\pi}{6} = \tfrac12, cos⁡π4=22\cos\tfrac{\pi}{4} = \tfrac{\sqrt2}{2}, tan⁡π3=3\tan\tfrac{\pi}{3} = \sqrt3

    π6=30∘,  π4=45∘,  π3=60∘\displaystyle \frac{\pi}{6} = 30^\circ,\; \frac{\pi}{4} = 45^\circ,\; \frac{\pi}{3} = 60^\circ

Unit 10 31 topics

Trigonometry

Trigonometry, The Unit Circle, and Special Trigonometric Ratios.

10.33 Trigonometry

θadjacentoppositehypotenuseSOH CAH TOAsin θ = opp / hypcos θ = adj / hyptan θ = opp / adjOpposite and adjacent arenamed from the angle θ.
Each trig ratio compares two sides of a right triangle, named from the angle θ. The hypotenuse is always the longest side, across from the right angle.
  1. 10.33.1

    Angles and Sides in Right Triangles

    The hypotenuse is opposite the right angle and is the longest side. For an acute angle θ\theta, the opposite leg is across from θ\theta, and the adjacent leg is the leg that forms θ\theta. The two acute angles add to 90∘90^\circ.

    e.g. ∠C=90∘\angle C = 90^\circ, ∠A=35∘\angle A = 35^\circ: ∠B=55∘\angle B = 55^\circ. Side aa is opposite AA; side bb is adjacent to AA

    ∠A+∠B=90∘\displaystyle \angle A + \angle B = 90^\circ
    a2+b2=c2\displaystyle a^2 + b^2 = c^2
  2. 10.33.2

    The Trigonometric Ratios

    SOH-CAH-TOA. Each ratio compares two sides of a right triangle relative to an acute angle θ\theta.

    e.g. Legs 3 and 4, hypotenuse 5, θ\theta opposite 3: sin⁡θ=35\sin\theta = \tfrac35, cos⁡θ=45\cos\theta = \tfrac45, tan⁡θ=34\tan\theta = \tfrac34

    sin⁡θ=opphyp\displaystyle \sin\theta = \frac{\text{opp}}{\text{hyp}}
    cos⁡θ=adjhyp\displaystyle \cos\theta = \frac{\text{adj}}{\text{hyp}}
    tan⁡θ=oppadj\displaystyle \tan\theta = \frac{\text{opp}}{\text{adj}}
  3. 10.33.3

    Calculating Trigonometric Ratios Using the Pythagorean Theorem

    Given one ratio, label two sides of a right triangle, find the third side with the Pythagorean theorem, then read off any other ratio.

    e.g. sin⁡θ=513\sin\theta = \tfrac{5}{13}: adj =169−25=12= \sqrt{169 - 25} = 12, so cos⁡θ=1213\cos\theta = \tfrac{12}{13}, tan⁡θ=512\tan\theta = \tfrac{5}{12}

    opp2+adj2=hyp2\displaystyle \text{opp}^2 + \text{adj}^2 = \text{hyp}^2
  4. 10.33.4

    Calculating Side Lengths of Right Triangles Using Trigonometry

    Pick the ratio that uses the known angle, the known side, and the unknown side. Solve for the unknown. Set the calculator to degree mode.

    e.g. θ=40∘\theta = 40^\circ, adj =8= 8: opp =8tan⁡40∘≈6.71= 8\tan 40^\circ \approx 6.71

    opp=hyp⋅sin⁡θ\displaystyle \text{opp} = \text{hyp} \cdot \sin\theta
    adj=hyp⋅cos⁡θ\displaystyle \text{adj} = \text{hyp} \cdot \cos\theta
    opp=adj⋅tan⁡θ\displaystyle \text{opp} = \text{adj} \cdot \tan\theta
  5. 10.33.5

    Calculating Angles in Right Triangles Using Trigonometry

    Find a ratio from two known sides, then use the inverse function. sin⁡−1\sin^{-1} means inverse sine, not 1sin⁡\tfrac{1}{\sin}.

    e.g. opp =5= 5, adj =12= 12: θ=tan⁡−1 ⁣(512)≈22.6∘\theta = \tan^{-1}\!\left(\tfrac{5}{12}\right) \approx 22.6^\circ

    θ=sin⁡−1 ⁣(opphyp)\displaystyle \theta = \sin^{-1}\!\left(\frac{\text{opp}}{\text{hyp}}\right)
    θ=cos⁡−1 ⁣(adjhyp)\displaystyle \theta = \cos^{-1}\!\left(\frac{\text{adj}}{\text{hyp}}\right)
    θ=tan⁡−1 ⁣(oppadj)\displaystyle \theta = \tan^{-1}\!\left(\frac{\text{opp}}{\text{adj}}\right)
  6. 10.33.6

    Modeling With Trigonometry

    Sketch the right triangle and label what you know. The angle of elevation is measured up from the horizontal, and the angle of depression is measured down from the horizontal. The two are equal when they describe the same line of sight.

    e.g. Standing 20 ft from a tree, angle of elevation 50∘50^\circ: height =20tan⁡50∘≈23.8= 20\tan 50^\circ \approx 23.8 ft

  7. 10.33.7

    The Reciprocal Trigonometric Ratios

    Cosecant, secant, and cotangent are the reciprocals of sine, cosine, and tangent. Flip the fraction.

    e.g. Legs 3 and 4, hypotenuse 5, θ\theta opposite 3: csc⁡θ=53\csc\theta = \tfrac53, sec⁡θ=54\sec\theta = \tfrac54, cot⁡θ=43\cot\theta = \tfrac43

    csc⁡θ=1sin⁡θ=hypopp\displaystyle \csc\theta = \frac{1}{\sin\theta} = \frac{\text{hyp}}{\text{opp}}
    sec⁡θ=1cos⁡θ=hypadj\displaystyle \sec\theta = \frac{1}{\cos\theta} = \frac{\text{hyp}}{\text{adj}}
    cot⁡θ=1tan⁡θ=adjopp\displaystyle \cot\theta = \frac{1}{\tan\theta} = \frac{\text{adj}}{\text{opp}}
  8. 10.33.8

    Trigonometric Ratios in Similar Right Triangles

    Right triangles with the same acute angle are similar, so their sides are proportional. A trig ratio depends only on the angle, not on the size of the triangle.

    e.g. 3-4-5 and 6-8-10 triangles: sin⁡θ=35=610\sin\theta = \tfrac35 = \tfrac{6}{10}

  9. 10.33.9

    Trigonometric Functions of Complementary Angles

    The two acute angles of a right triangle are complementary, and the side opposite one is adjacent to the other. So each function equals its cofunction of the complement.

    e.g. sin⁡25∘=cos⁡65∘\sin 25^\circ = \cos 65^\circ. If sin⁡x=cos⁡2x\sin x = \cos 2x: x+2x=90∘x + 2x = 90^\circ, so x=30∘x = 30^\circ

    sin⁡θ=cos⁡(90∘−θ)\displaystyle \sin\theta = \cos(90^\circ - \theta)
    tan⁡θ=cot⁡(90∘−θ)\displaystyle \tan\theta = \cot(90^\circ - \theta)
    sec⁡θ=csc⁡(90∘−θ)\displaystyle \sec\theta = \csc(90^\circ - \theta)
  10. 10.33.10

    Calculating Trigonometric Ratios From Descriptions

    Sketch the right triangle, label the given sides, and find the missing side with the Pythagorean theorem. Then apply SOH CAH TOA. The sine of one acute angle equals the cosine of the other.

    e.g. sin⁡A=35\sin A = \tfrac35: sides 3, 4, 5, so cos⁡A=45\cos A = \tfrac45 and tan⁡A=34\tan A = \tfrac34

    sin⁡θ=opphyp\displaystyle \sin\theta = \frac{\text{opp}}{\text{hyp}}
    cos⁡θ=adjhyp\displaystyle \cos\theta = \frac{\text{adj}}{\text{hyp}}
    tan⁡θ=oppadj\displaystyle \tan\theta = \frac{\text{opp}}{\text{adj}}
    sin⁡θ=cos⁡(90∘−θ)\displaystyle \sin\theta = \cos(90^\circ - \theta)
  11. 10.33.11

    Special Trigonometric Ratios

    Exact values come from the 30-60-90 triangle (sides 1:3:21 : \sqrt3 : 2) and the 45-45-90 triangle (sides 1:1:21 : 1 : \sqrt2).

    e.g. 30-60-90 with hypotenuse 10: short leg 5, long leg 535\sqrt3

    sin⁡30∘=cos⁡60∘=12\displaystyle \sin 30^\circ = \cos 60^\circ = \frac{1}{2}
    sin⁡45∘=cos⁡45∘=22\displaystyle \sin 45^\circ = \cos 45^\circ = \frac{\sqrt2}{2}
    sin⁡60∘=cos⁡30∘=32\displaystyle \sin 60^\circ = \cos 30^\circ = \frac{\sqrt3}{2}
    tan⁡30∘=33,  tan⁡45∘=1\displaystyle \tan 30^\circ = \frac{\sqrt3}{3},\; \tan 45^\circ = 1
    tan⁡60∘=3\displaystyle \tan 60^\circ = \sqrt3
  12. 10.33.12

    Calculating Areas of Right Triangles Using Trigonometry

    The area is half the product of the legs. If a leg is missing, find it with trig first.

    e.g. Hypotenuse 10, angle 30∘30^\circ: legs 5 and 535\sqrt3, so A=2532≈21.65A = \tfrac{25\sqrt3}{2} \approx 21.65

    A=12⋅leg1⋅leg2\displaystyle A = \frac{1}{2} \cdot \text{leg}_1 \cdot \text{leg}_2
  13. 10.33.13

    Solving Multiple Right Triangles Using Trigonometry

    Start with the triangle that has enough information. Use the side the triangles share to carry the result into the next triangle.

    e.g. AD‾⊥BC‾\overline{AD} \perp \overline{BC}, AD=6AD = 6, ∠B=45∘\angle B = 45^\circ, ∠C=30∘\angle C = 30^\circ: BD=6BD = 6, DC=6tan⁡30∘=63DC = \tfrac{6}{\tan 30^\circ} = 6\sqrt3, so BC=6+63BC = 6 + 6\sqrt3

10.34 The Unit Circle

xyθP (cos θ, sin θ)1cos θsin θI allII sinIII tanIV cosx-coordinate = cos θy-coordinate = sin θcos²θ + sin²θ = 1tan θ = sin θ ÷ cos θPositive in each quadrant:All, Sin, Tan, Cos
On the unit circle, the point at angle θ is (cos θ, sin θ), so the legs of the triangle are cos θ and sin θ. The quadrant labels show which ratios are positive there.
  1. 10.34.1

    Angles in the Coordinate Plane

    An angle in standard position has its vertex at the origin and its initial side on the positive xx-axis. A positive angle rotates counterclockwise to its terminal side. The quadrant of the terminal side names the angle's quadrant.

    e.g. 200∘200^\circ ends in Quadrant III

    QI: 0∘<θ<90∘\displaystyle \text{QI: } 0^\circ < \theta < 90^\circ
    QII: 90∘<θ<180∘\displaystyle \text{QII: } 90^\circ < \theta < 180^\circ
    QIII: 180∘<θ<270∘\displaystyle \text{QIII: } 180^\circ < \theta < 270^\circ
    QIV: 270∘<θ<360∘\displaystyle \text{QIV: } 270^\circ < \theta < 360^\circ
  2. 10.34.2

    Negative Angles in the Coordinate Plane

    A negative angle rotates clockwise from the positive xx-axis. Go clockwise through IV, III, II, I.

    e.g. −120∘-120^\circ goes 30∘30^\circ past the negative yy-axis, so it ends in Quadrant III

    −90∘<θ<0∘  →  QIV\displaystyle -90^\circ < \theta < 0^\circ \;\to\; \text{QIV}
    −180∘<θ<−90∘  →  QIII\displaystyle -180^\circ < \theta < -90^\circ \;\to\; \text{QIII}
  3. 10.34.3

    Coterminal Angles

    Coterminal angles share the same terminal side. Add or subtract full turns to find them.

    e.g. 60∘60^\circ is coterminal with 420∘420^\circ and −300∘-300^\circ

    θ+360∘k(k an integer)\displaystyle \theta + 360^\circ k \quad (k \text{ an integer})
    θ+2πkin radians\displaystyle \theta + 2\pi k \quad \text{in radians}
  4. 10.34.4

    Calculating Reference Angles

    The reference angle is the acute angle between the terminal side and the xx-axis. First find a coterminal angle from 0∘0^\circ to 360∘360^\circ, then use its quadrant.

    e.g. 210∘210^\circ is in QIII, so its reference angle is 210∘−180∘=30∘210^\circ - 180^\circ = 30^\circ

    QI: θ\displaystyle \text{QI: } \theta
    QII: 180∘−θ\displaystyle \text{QII: } 180^\circ - \theta
    QIII: θ−180∘\displaystyle \text{QIII: } \theta - 180^\circ
    QIV: 360∘−θ\displaystyle \text{QIV: } 360^\circ - \theta
  5. 10.34.5

    Properties of the Unit Circle in the First Quadrant

    The unit circle has radius 1 and center at the origin. The terminal side of angle θ\theta meets it at the point (cos⁡θ,sin⁡θ)(\cos\theta, \sin\theta).

    e.g. At 30∘30^\circ the point is (32,12)\left(\tfrac{\sqrt3}{2}, \tfrac12\right), and 34+14=1\tfrac34 + \tfrac14 = 1

    x2+y2=1\displaystyle x^2 + y^2 = 1
    (x,y)=(cos⁡θ,sin⁡θ)\displaystyle (x, y) = (\cos\theta, \sin\theta)
  6. 10.34.6

    Extending the Trigonometric Ratios Using the Unit Circle

    For any angle, use a point (x,y)(x, y) on the terminal side at distance rr from the origin. On the unit circle r=1r = 1. Signs by quadrant: all positive in I, only sin in II, only tan in III, only cos in IV.

    e.g. Through (−3,4)(-3, 4): r=5r = 5, sin⁡θ=45\sin\theta = \tfrac45, cos⁡θ=−35\cos\theta = -\tfrac35, tan⁡θ=−43\tan\theta = -\tfrac43

    sin⁡θ=yr,  cos⁡θ=xr\displaystyle \sin\theta = \frac{y}{r},\; \cos\theta = \frac{x}{r}
    tan⁡θ=yx,  r=x2+y2\displaystyle \tan\theta = \frac{y}{x},\; r = \sqrt{x^2 + y^2}
  7. 10.34.7

    Extending the Trigonometric Ratios Using Angles in Radians

    A full turn is 2π2\pi radians, so π\pi radians is 180∘180^\circ. Find the reference angle in radians, take the ratio of that angle, then attach the quadrant's sign.

    e.g. cos⁡4π3\cos\tfrac{4\pi}{3}: reference angle π3\tfrac{\pi}{3} in QIII, so cos⁡4π3=−12\cos\tfrac{4\pi}{3} = -\tfrac12

    rad=deg⋅π180\displaystyle \text{rad} = \text{deg} \cdot \frac{\pi}{180}
    QII: π−θ,  QIII: θ−π\displaystyle \text{QII: } \pi - \theta,\; \text{QIII: } \theta - \pi
    QIV: 2π−θ\displaystyle \text{QIV: } 2\pi - \theta
  8. 10.34.8

    Extending the Trigonometric Ratios to Negative Angles

    Use a positive coterminal angle, or use the symmetry rules. Cosine is even. Sine and tangent are odd.

    e.g. sin⁡(−150∘)=−sin⁡150∘=−12\sin(-150^\circ) = -\sin 150^\circ = -\tfrac12

    sin⁡(−θ)=−sin⁡θ\displaystyle \sin(-\theta) = -\sin\theta
    cos⁡(−θ)=cos⁡θ\displaystyle \cos(-\theta) = \cos\theta
    tan⁡(−θ)=−tan⁡θ\displaystyle \tan(-\theta) = -\tan\theta
  9. 10.34.9

    Extending the Trigonometric Ratios to Large Angles

    Subtract 360∘360^\circ (or 2π2\pi) until the angle is between 0∘0^\circ and 360∘360^\circ. Coterminal angles have the same trig ratios.

    e.g. sin⁡750∘=sin⁡(750∘−720∘)=sin⁡30∘=12\sin 750^\circ = \sin(750^\circ - 720^\circ) = \sin 30^\circ = \tfrac12

    sin⁡(θ+360∘k)=sin⁡θ\displaystyle \sin(\theta + 360^\circ k) = \sin\theta
    cos⁡(θ+360∘k)=cos⁡θ\displaystyle \cos(\theta + 360^\circ k) = \cos\theta
  10. 10.34.10

    Using the Pythagorean Identity in the First Quadrant

    Since (cos⁡θ,sin⁡θ)(\cos\theta, \sin\theta) is on the unit circle, the squares add to 1. Given one ratio, solve for the other. In Quadrant I every ratio is positive.

    e.g. sin⁡θ=35\sin\theta = \tfrac35 in QI: cos⁡θ=1−925=45\cos\theta = \sqrt{1 - \tfrac{9}{25}} = \tfrac45, tan⁡θ=34\tan\theta = \tfrac34

    sin⁡2θ+cos⁡2θ=1\displaystyle \sin^2\theta + \cos^2\theta = 1
    cos⁡θ=1−sin⁡2θ\displaystyle \cos\theta = \sqrt{1 - \sin^2\theta}
  11. 10.34.11

    Extending the Pythagorean Identity to All Quadrants

    The identity holds for every angle. Solving gives ±\pm, so choose the sign from the quadrant.

    e.g. sin⁡θ=−513\sin\theta = -\tfrac{5}{13} in QIII: cos⁡θ=−1−25169=−1213\cos\theta = -\sqrt{1 - \tfrac{25}{169}} = -\tfrac{12}{13}

    sin⁡2θ+cos⁡2θ=1\displaystyle \sin^2\theta + \cos^2\theta = 1
    cos⁡θ=±1−sin⁡2θ\displaystyle \cos\theta = \pm\sqrt{1 - \sin^2\theta}
    sin⁡θ=±1−cos⁡2θ\displaystyle \sin\theta = \pm\sqrt{1 - \cos^2\theta}

10.35 Special Trigonometric Ratios

θradians0°030°π/645°π/460°π/390°π/2sin θ01/2√2/2√3/21cos θ1√3/2√2/21/20tan θ0√3/31√3undefinedPattern: sin runs √0/2, √1/2, √2/2, √3/2, √4/2. Cos runs the same list backward.
These exact values come from the 30-60-90 and 45-45-90 triangles. At 45° sine and cosine are equal, so tangent is 1.
  1. 10.35.1

    Finding Trigonometric Ratios of Quadrantal Angles

    Quadrantal angles land on an axis. Read cos⁡θ\cos\theta and sin⁡θ\sin\theta from the point. A ratio is undefined when its denominator is 0: tan and sec at 90∘90^\circ and 270∘270^\circ, cot and csc at 0∘0^\circ and 180∘180^\circ.

    e.g. cos⁡180∘=−1\cos 180^\circ = -1, sin⁡270∘=−1\sin 270^\circ = -1, tan⁡90∘\tan 90^\circ is undefined

    0∘→(1,0),  90∘→(0,1)\displaystyle 0^\circ \to (1, 0),\; 90^\circ \to (0, 1)
    180∘→(−1,0)\displaystyle 180^\circ \to (-1, 0)
    270∘→(0,−1)\displaystyle 270^\circ \to (0, -1)
  2. 10.35.2

    Trigonometric Ratios of Quadrantal Angles Outside the Standard Range

    Add or subtract full turns to reach 0∘0^\circ, 90∘90^\circ, 180∘180^\circ, or 270∘270^\circ, then read the point.

    e.g. sin⁡(−450∘)=sin⁡270∘=−1\sin(-450^\circ) = \sin 270^\circ = -1; cos⁡5π=cos⁡π=−1\cos 5\pi = \cos\pi = -1

  3. 10.35.3

    Finding Trigonometric Ratios of Special Angles Using the Unit Circle

    Memorize the first-quadrant points. For other angles, use the reference angle's values and the quadrant's signs.

    e.g. cos⁡135∘=−22\cos 135^\circ = -\tfrac{\sqrt2}{2} (reference 45∘45^\circ, QII); sin⁡300∘=−32\sin 300^\circ = -\tfrac{\sqrt3}{2}

    30∘  (π6):  (32,12)\displaystyle 30^\circ\;(\tfrac{\pi}{6}):\; \left(\tfrac{\sqrt3}{2}, \tfrac12\right)
    45∘  (π4):  (22,22)\displaystyle 45^\circ\;(\tfrac{\pi}{4}):\; \left(\tfrac{\sqrt2}{2}, \tfrac{\sqrt2}{2}\right)
    60∘  (π3):  (12,32)\displaystyle 60^\circ\;(\tfrac{\pi}{3}):\; \left(\tfrac12, \tfrac{\sqrt3}{2}\right)
  4. 10.35.4

    Evaluating Trigonometric Expressions

    Replace each ratio with its exact value, then simplify. sin⁡2θ\sin^2\theta means (sin⁡θ)2(\sin\theta)^2.

    e.g. 2sin⁡30∘+cos⁡245∘=2(12)+12=322\sin 30^\circ + \cos^2 45^\circ = 2\left(\tfrac12\right) + \tfrac12 = \tfrac32

  5. 10.35.5

    Further Extensions of the Special Trigonometric Ratios

    Reduce negative or large angles to a coterminal angle from 0∘0^\circ to 360∘360^\circ, then use the reference angle. The reciprocal ratios flip sin, cos, and tan.

    e.g. sec⁡(−405∘)=sec⁡315∘=12/2=2\sec(-405^\circ) = \sec 315^\circ = \dfrac{1}{\sqrt2/2} = \sqrt2

    csc⁡θ=1sin⁡θ,  sec⁡θ=1cos⁡θ\displaystyle \csc\theta = \frac{1}{\sin\theta},\; \sec\theta = \frac{1}{\cos\theta}
    cot⁡θ=cos⁡θsin⁡θ\displaystyle \cot\theta = \frac{\cos\theta}{\sin\theta}
  6. 10.35.6

    Trigonometric Ratios of Large Angles in Degrees

    Subtract 360∘360^\circ until the angle is between 0∘0^\circ and 360∘360^\circ. Then use the reference angle and the quadrant's sign.

    e.g. sin⁡495∘=sin⁡135∘=22\sin 495^\circ = \sin 135^\circ = \tfrac{\sqrt2}{2}

    sin⁡(θ+360∘)=sin⁡θ\displaystyle \sin(\theta + 360^\circ) = \sin\theta
    cos⁡(θ+360∘)=cos⁡θ\displaystyle \cos(\theta + 360^\circ) = \cos\theta
  7. 10.35.7

    Trigonometric Ratios of Large Angles in Radians

    Subtract 2π2\pi until the angle is between 00 and 2π2\pi. Then use the reference angle and the quadrant's sign.

    e.g. cos⁡13π6=cos⁡π6=32\cos \tfrac{13\pi}{6} = \cos \tfrac{\pi}{6} = \tfrac{\sqrt3}{2}

    sin⁡(θ+2π)=sin⁡θ\displaystyle \sin(\theta + 2\pi) = \sin\theta
    cos⁡(θ+2π)=cos⁡θ\displaystyle \cos(\theta + 2\pi) = \cos\theta

Unit 11 32 topics

Advanced Algebra - Functions

Functions, Linear Functions, and Graph Transformations of Functions.

11.36 Functions

3f2x + 17f(3) = 7: one input, one outputfunction ✓not a function ✗
A function sends each input to exactly one output. On a graph, a vertical line that hits twice means some input has two outputs.
  1. 11.36.1

    Introduction to Functions

    A function gives each input exactly one output. f(x)f(x), read “f of x,” is the output at input xx.

    f(x)=2x+1  ⇒  f(3)=7\displaystyle f(x) = 2x + 1 \;\Rightarrow\; f(3) = 7
  2. 11.36.2

    Visual Representations of Functions

    Mapping diagrams, tables, and graphs. It is a function if no input has two arrows, two rows, or two points.

  3. 11.36.3

    Graphs of Functions

    The graph is every point (x,f(x))(x, f(x)). The value f(a)f(a) is the height of the graph above x=ax = a.

  4. 11.36.4

    The Domain of a Function

    The allowed inputs. Exclude anything that divides by zero or takes an even root of a negative.

    f(x)=1x−2: x≠2\displaystyle f(x) = \frac{1}{x - 2}:\ x \ne 2
    g(x)=x+5: x≥−5\displaystyle g(x) = \sqrt{x + 5}:\ x \ge -5
  5. 11.36.5

    The Vertical Line Test

    A graph is a function if no vertical line crosses it more than once.

    e.g. A circle fails; the parabola y=x2y = x^2 passes

  6. 11.36.6

    Global Extrema of Functions

    The highest output anywhere is the global maximum; the lowest is the global minimum. Some functions have neither.

  7. 11.36.7

    Local Extrema of Functions

    A local maximum is a point higher than all nearby points, and a local minimum is lower than all nearby points. They sit at the tops of hills and bottoms of valleys, where the graph switches between increasing and decreasing. The extreme value is the yy-coordinate.

    e.g. f(x)=x3−3xf(x) = x^3 - 3x: local max 22 at x=−1x = -1, local min −2-2 at x=1x = 1

  8. 11.36.8

    End Behavior of Functions

    What f(x)f(x) does as x→∞x \to \infty and as x→−∞x \to -\infty: rises, falls, or levels off.

    e.g. f(x)=−x2f(x) = -x^2 falls at both ends

  9. 11.36.9

    The Range of a Function

    The outputs the function actually produces. Read them off the graph’s lowest and highest points.

    e.g. Range of x2+1x^2 + 1: [1,∞)[1, \infty)

  10. 11.36.10

    The Range of a Function: Advanced Cases

    Watch for values the graph approaches but never reaches, and for gaps.

    e.g. f(x)=1xf(x) = \tfrac1x: range (−∞,0)∪(0,∞)(-\infty, 0) \cup (0, \infty)

  11. 11.36.11

    The Roots of a Function

    Inputs where f(x)=0f(x) = 0: where the graph crosses or touches the xx-axis.

    e.g. Roots of x2−4x^2 - 4: ±2\pm 2

    f(x)=0\displaystyle f(x) = 0
  12. 11.36.12

    Increasing and Decreasing Functions

    Increasing where the graph rises left to right, decreasing where it falls. State the xx-interval.

    e.g. x2x^2 decreases on (−∞,0)(-\infty, 0) and increases on (0,∞)(0, \infty)

  13. 11.36.13

    Unbounded Behavior of Functions Near a Point

    A function is unbounded near x=ax = a if its values grow without limit (toward ∞\infty or −∞-\infty) as xx gets close to aa. The graph has a vertical asymptote at x=ax = a, often where a denominator is 0.

    e.g. f(x)=1x−2f(x) = \tfrac{1}{x - 2}: as xx approaches 2 from the right, f(x)→∞f(x) \to \infty; from the left, f(x)→−∞f(x) \to -\infty

    x→a  ⇒  f(x)→±∞\displaystyle x \to a \;\Rightarrow\; f(x) \to \pm\infty
  14. 11.36.14

    Piecewise Functions

    Different rules on different parts of the domain. Find which piece the input belongs to, then use that rule.

    e.g. f(−3)=−1f(-3) = -1, f(3)=9f(3) = 9

    f(x)={x+2x<0x2x≥0\displaystyle f(x) = \begin{cases} x + 2 & x < 0 \\ x^2 & x \ge 0 \end{cases}
  15. 11.36.15

    The Arithmetic of Functions

    Add, subtract, multiply, or divide the outputs at the same input.

    (f+g)(x)=f(x)+g(x)\displaystyle (f + g)(x) = f(x) + g(x)
    (fg)(x)=f(x) g(x)\displaystyle (fg)(x) = f(x)\,g(x)
    (fg)(x)=f(x)g(x), g(x)≠0\displaystyle \left(\tfrac{f}{g}\right)(x) = \tfrac{f(x)}{g(x)},\ g(x) \ne 0
  16. 11.36.16

    Function Composition

    Feed one function’s output into another. Work from the inside out.

    e.g. f(x)=x2f(x) = x^2, g(x)=x+1g(x) = x + 1: f(g(2))=9f(g(2)) = 9, g(f(2))=5g(f(2)) = 5

    (f∘g)(x)=f(g(x))\displaystyle (f \circ g)(x) = f(g(x))
  17. 11.36.17

    Describing Function Composition

    Read f(g(x))f(g(x)) as “do gg, then ff.” Order matters: usually f(g(x))≠g(f(x))f(g(x)) \ne g(f(x)).

  18. 11.36.18

    Introduction to Inverse Functions

    f−1f^{-1} undoes ff. To find it, swap xx and yy and solve for yy. Its graph is the reflection of ff in y=xy = x.

    f(f−1(x))=x\displaystyle f(f^{-1}(x)) = x
    f(x)=2x+3  ⇒  f−1(x)=x−32\displaystyle f(x) = 2x + 3 \;\Rightarrow\; f^{-1}(x) = \frac{x - 3}{2}
  19. 11.36.19

    Even and Odd Functions

    Even: f(−x)=f(x)f(-x) = f(x), symmetric about the yy-axis. Odd: f(−x)=−f(x)f(-x) = -f(x), symmetric about the origin. Most functions are neither.

    e.g. f(x)=x3−xf(x) = x^3 - x: f(−x)=−x3+x=−f(x)f(-x) = -x^3 + x = -f(x), so odd. x2+1x^2 + 1 is even.

    f(−x)=f(x)even\displaystyle f(-x) = f(x) \quad \text{even}
    f(−x)=−f(x)odd\displaystyle f(-x) = -f(x) \quad \text{odd}
  20. 11.36.20

    The Average Rate of Change of a Function

    The change in output divided by the change in input between two points. It is the slope of the line through those two points on the graph.

    e.g. f(x)=x2f(x) = x^2 from x=1x = 1 to x=4x = 4: 16−14−1=5\tfrac{16 - 1}{4 - 1} = 5

    f(b)−f(a)b−a\displaystyle \frac{f(b) - f(a)}{b - a}
  21. 11.36.21

    Introduction to Sequences

    An ordered list of terms. ana_n is the nnth term. An explicit formula gives any term straight from nn.

    an=n2  ⇒  1,4,9,16,…\displaystyle a_n = n^2 \;\Rightarrow\; 1, 4, 9, 16, \ldots

11.37 Linear Functions

  1. 11.37.1

    Modeling With Linear Functions

    A constant rate of change means a linear model, f(x)=mx+bf(x) = mx + b.

  2. 11.37.2

    Constructing Linear Functions

    Find the slope from two points, then solve for bb.

    e.g. f(1)=5f(1) = 5, f(3)=11f(3) = 11 → m=3m = 3, f(x)=3x+2f(x) = 3x + 2

    m=f(x2)−f(x1)x2−x1\displaystyle m = \frac{f(x_2) - f(x_1)}{x_2 - x_1}
  3. 11.37.3

    Linear Functions in Tabular Form

    A table is linear when yy changes by the same amount for each equal step in xx. The slope is the change in yy over the change in xx. The yy-intercept is the output at x=0x = 0.

    e.g. xx: 0, 1, 2 and yy: 5, 8, 11 → y=3x+5y = 3x + 5

    m=y2−y1x2−x1\displaystyle m = \frac{y_2 - y_1}{x_2 - x_1}
  4. 11.37.4

    Analyzing Linear Functions in Tabular Form

    Find the slope from any two rows, then find bb by plugging in one row. Use the equation to fill in or predict values.

    e.g. Rows (2,7)(2, 7) and (5,16)(5, 16): m=93=3m = \tfrac93 = 3, b=7−6=1b = 7 - 6 = 1, so f(10)=31f(10) = 31

    m=y2−y1x2−x1\displaystyle m = \frac{y_2 - y_1}{x_2 - x_1}
    b=y1−mx1\displaystyle b = y_1 - m x_1
  5. 11.37.5

    Transformations of Linear Functions in Tabular Form

    For g(x)=af(x)+kg(x) = a f(x) + k, apply the change to each output in the table: multiply by aa, then add kk. For g(x)=f(x−h)g(x) = f(x - h), each output moves hh units to the right in xx.

    e.g. f(1)=4f(1) = 4, f(2)=7f(2) = 7, g(x)=2f(x)−1g(x) = 2f(x) - 1: g(1)=7g(1) = 7, g(2)=13g(2) = 13

    g(x)=a f(x)+k\displaystyle g(x) = a\,f(x) + k
    g(x+h)=f(x) if g(x)=f(x−h)\displaystyle g(x + h) = f(x) \text{ if } g(x) = f(x - h)
  6. 11.37.6

    Linear Functions in Tabular Form Containing Unknown Parameters

    A linear table has the same slope between every pair of rows. Set two slopes equal and solve for the unknown.

    e.g. Rows (1,2)(1, 2), (3,8)(3, 8), (4,k)(4, k): slope 62=3\tfrac62 = 3, so k=8+3=11k = 8 + 3 = 11

    y2−y1x2−x1=y3−y2x3−x2\displaystyle \frac{y_2 - y_1}{x_2 - x_1} = \frac{y_3 - y_2}{x_3 - x_2}

11.38 Graph Transformations of Functions

xy−3−2−112345−112345y = x²y = (x − 2)² + 1right 2, up 1y = a·f(b(x − h)) + khshift right(inside, opposite sign)kshift upavertical stretch;a < 0 flips over x-axisbhorizontal squeeze by 1/b;b < 0 flips over y-axis
Replacing x with x − 2 and adding 1 moves every point of y = x² right 2 and up 1. Changes inside the function act on x and run opposite to how they look.
  1. 11.38.1

    Vertical Translations of Functions

    f(x)+kf(x) + k shifts the graph up kk units if k>0k > 0 and down if k<0k < 0. Only the yy-coordinates change.

    e.g. y=x2−3y = x^2 - 3 is y=x2y = x^2 shifted down 3; vertex (0,−3)(0, -3)

    y=f(x)+k\displaystyle y = f(x) + k
    (x,y)→(x,y+k)\displaystyle (x, y) \to (x, y + k)
  2. 11.38.2

    Horizontal Translations of Functions

    f(x−h)f(x - h) shifts the graph right hh units if h>0h > 0 and left if h<0h < 0. The shift is opposite the sign inside, so f(x+2)f(x + 2) moves left 2.

    e.g. y=x+2y = \sqrt{x + 2} is y=xy = \sqrt{x} shifted left 2; it starts at (−2,0)(-2, 0)

    y=f(x−h)\displaystyle y = f(x - h)
    (x,y)→(x+h,y)\displaystyle (x, y) \to (x + h, y)
  3. 11.38.3

    Vertical Reflections of Functions

    −f(x)-f(x) reflects the graph across the xx-axis. Every yy-coordinate changes sign.

    e.g. y=−xy = -\sqrt{x} passes through (4,−2)(4, -2) instead of (4,2)(4, 2)

    y=−f(x)\displaystyle y = -f(x)
    (x,y)→(x,−y)\displaystyle (x, y) \to (x, -y)
  4. 11.38.4

    Finding Equations of Translated Functions

    To shift right hh, replace xx with x−hx - h. To shift up kk, add kk. Left and down use the opposite signs.

    e.g. y=x2y = x^2 shifted left 2 and down 3: y=(x+2)2−3y = (x + 2)^2 - 3

    y=f(x−h)+k\displaystyle y = f(x - h) + k
  5. 11.38.5

    Transforming Polynomial Functions

    Apply the transformation to the whole rule, then simplify. Shifts work as for any function. A negative outside reflects over the xx-axis, and a negative on xx reflects over the yy-axis.

    e.g. f(x)=x2+3xf(x) = x^2 + 3x, g(x)=f(x−1)=(x−1)2+3(x−1)=x2+x−2g(x) = f(x - 1) = (x - 1)^2 + 3(x - 1) = x^2 + x - 2

    y=f(x−h)+k\displaystyle y = f(x - h) + k
    −f(x): reflect over x-axis\displaystyle -f(x)\text{: reflect over } x\text{-axis}
    f(−x): reflect over y-axis\displaystyle f(-x)\text{: reflect over } y\text{-axis}
    af(x): vertical stretch by a\displaystyle a f(x)\text{: vertical stretch by } a

Unit 12 11 topics

Advanced Algebra - Absolute Value

Absolute Value Expressions and Equations, and Absolute Value Functions.

12.39 Absolute Value Expressions and Equations

−101234567822|x − 3| < 2between: 1 < x < 5−1012345678|x − 3| ≥ 2outside: x ≤ 1 or x ≥ 5
|x − 3| is the distance from x to 3. Less than means close to 3; greater than means far from it.
  1. 12.39.1

    Absolute Value Expressions

    Absolute value is distance from zero, so it is never negative. Evaluate inside first.

    e.g. ∣3−8∣=5\lvert 3 - 8 \rvert = 5

    ∣x∣={xx≥0−xx<0\displaystyle \lvert x \rvert = \begin{cases} x & x \ge 0 \\ -x & x < 0 \end{cases}
  2. 12.39.2

    Rules of Absolute Value

    It passes through multiplication and division, but not through addition.

    ∣ab∣=∣a∣ ∣b∣\displaystyle \lvert ab \rvert = \lvert a \rvert\,\lvert b \rvert
    ∣ab∣=∣a∣∣b∣\displaystyle \left\lvert \tfrac{a}{b} \right\rvert = \tfrac{\lvert a \rvert}{\lvert b \rvert}
    ∣a+b∣≤∣a∣+∣b∣\displaystyle \lvert a + b \rvert \le \lvert a \rvert + \lvert b \rvert
  3. 12.39.3

    Further Rules of Absolute Value

    A number and its opposite have the same absolute value.

    ∣−a∣=∣a∣\displaystyle \lvert -a \rvert = \lvert a \rvert
    ∣a∣2=a2\displaystyle \lvert a \rvert^2 = a^2
    a2=∣a∣\displaystyle \sqrt{a^2} = \lvert a \rvert
  4. 12.39.4

    Absolute Value Equations

    Isolate the absolute value, then split into two equations. A negative right side has no solution.

    e.g. ∣2x−1∣=7⇒x=4\lvert 2x - 1 \rvert = 7 \Rightarrow x = 4 or −3-3

    ∣A∣=k, k≥0\displaystyle \lvert A \rvert = k,\ k \ge 0
    ⇒  A=k or A=−k\displaystyle \Rightarrow\; A = k \text{ or } A = -k
  5. 12.39.5

    Further Absolute Value Equations

    When two absolute values are equal, the insides are equal or opposite.

    ∣A∣=∣B∣\displaystyle \lvert A \rvert = \lvert B \rvert
    ⇒  A=B or A=−B\displaystyle \Rightarrow\; A = B \text{ or } A = -B
  6. 12.39.6

    Absolute Value Inequalities

    Less than means between, an “and.” Greater than means outside, an “or.”

    ∣A∣<k  ⇒  −k<A<k\displaystyle \lvert A \rvert < k \;\Rightarrow\; -k < A < k
    ∣A∣>k  ⇒  A<−k or A>k\displaystyle \lvert A \rvert > k \;\Rightarrow\; A < -k \text{ or } A > k

12.40 Absolute Value Functions

xy−4−3−2−112345−3−2−11234vertex (1, −2)y = |x|y = a|x − h| + kvertex at (h, k)arms have slopes a and −aa < 0 flips it upside down|a| > 1 makes it narrowerHere: y = |x − 1| − 2
Every absolute value graph is the V of y = |x| moved, flipped, or stretched. Find the vertex first.
  1. 12.40.1

    Absolute Value Graphs

    y=∣x∣y = \lvert x \rvert is a V with its corner at the origin. Shifted, the corner (vertex) is at (h,k)(h, k).

    y=a∣x−h∣+k\displaystyle y = a\lvert x - h \rvert + k
  2. 12.40.2

    Vertical Reflections of Absolute Value Graphs

    A negative sign in front flips the V upside down.

    y=−∣x∣\displaystyle y = -\lvert x \rvert
  3. 12.40.3

    Stretches of Absolute Value Graphs

    ∣a∣>1\lvert a \rvert > 1 narrows the V; 0<∣a∣<10 < \lvert a \rvert < 1 widens it. The arms have slopes aa and −a-a.

  4. 12.40.4

    Combining Transformations of Absolute Value Graphs

    Plot the vertex (h,k)(h, k), then step out with slopes ±a\pm a. Note that ∣x+3∣\lvert x + 3 \rvert shifts left 3.

    e.g. y=−2∣x+3∣+4y = -2\lvert x + 3 \rvert + 4: vertex (−3,4)(-3, 4), opens down

  5. 12.40.5

    Roots of Absolute Value Functions

    Set y=0y = 0 and solve the absolute value equation. There can be zero, one, or two roots.

    e.g. ∣x−2∣−3=0⇒x=5\lvert x - 2 \rvert - 3 = 0 \Rightarrow x = 5 or −1-1

Unit 13 93 topics

Advanced Algebra - Polynomials

Polynomials, Factoring Polynomials, Quadratic Equations, and more.

13.41 Polynomials

a²ababb²abab(a + b)² = a² + 2ab + b²Two ab rectangles make themiddle term people forget.(x + 4)² = x² + 8x + 16
A square with side a + b splits into four pieces. Its area is not a² + b²; the two rectangles make up the difference.
  1. 13.41.1

    Introduction to Polynomials

    A sum of terms axnax^n with whole-number exponents. No variables in a denominator or under a root.

    e.g. 1x\tfrac1x and x\sqrt{x} are not polynomial terms

    3x4−x2+7x−5\displaystyle 3x^4 - x^2 + 7x - 5
  2. 13.41.2

    The Degree of a Polynomial

    The highest exponent. For a term with several variables, add their exponents. Standard form lists terms from highest degree down.

    deg⁡(5x3−2x+1)=3\displaystyle \deg(5x^3 - 2x + 1) = 3
    deg⁡(4x2y3)=5\displaystyle \deg(4x^2y^3) = 5
  3. 13.41.3

    Simplifying Polynomials

    Combine like terms: same variables raised to the same powers.

    3x2+5x−x2+2x=2x2+7x\displaystyle 3x^2 + 5x - x^2 + 2x = 2x^2 + 7x
  4. 13.41.4

    The Distributive Law for Polynomials

    Multiply the outside term by every term inside.

    2x(x2−3x+4)=2x3−6x2+8x\displaystyle 2x(x^2 - 3x + 4) = 2x^3 - 6x^2 + 8x
  5. 13.41.5

    Adding and Subtracting Polynomials

    Combine like terms. When subtracting, flip the sign of every term in the second polynomial.

    (4x2+3x)−(x2−5x)=3x2+8x\displaystyle (4x^2 + 3x) - (x^2 - 5x) = 3x^2 + 8x
  6. 13.41.6

    Monomials, Binomials and Trinomials

    One term, two terms, three terms.

    7x3x+4x2−5x+6\displaystyle 7x^3 \qquad x + 4 \qquad x^2 - 5x + 6
  7. 13.41.7

    Multiplying Binomials

    Every term times every term: First, Outer, Inner, Last.

    (a+b)(c+d)=ac+ad+bc+bd\displaystyle (a + b)(c + d) = ac + ad + bc + bd
    (x+3)(x−5)=x2−2x−15\displaystyle (x + 3)(x - 5) = x^2 - 2x - 15
  8. 13.41.8

    Multiplying Polynomials

    Multiply each term of the first by each term of the second, then combine like terms.

    (x+2)(x2−x+3)\displaystyle (x + 2)(x^2 - x + 3)
    =x3+x2+x+6\displaystyle = x^3 + x^2 + x + 6
  9. 13.41.9

    Squaring Binomials

    Square, twice the product, square. The middle term is the one people forget.

    e.g. (x+4)2=x2+8x+16(x + 4)^2 = x^2 + 8x + 16, not x2+16x^2 + 16

    (a+b)2=a2+2ab+b2\displaystyle (a + b)^2 = a^2 + 2ab + b^2
    (a−b)2=a2−2ab+b2\displaystyle (a - b)^2 = a^2 - 2ab + b^2
  10. 13.41.10

    The Difference of Squares Formula

    The middle terms cancel.

    e.g. (x+7)(x−7)=x2−49(x + 7)(x - 7) = x^2 - 49

    (a+b)(a−b)=a2−b2\displaystyle (a + b)(a - b) = a^2 - b^2

13.42 Factoring Polynomials

x²3x4x12x+3x+4x² + 7x + 12Two numbers thatmultiply to 12 and add to 7:3 and 4= (x + 3)(x + 4)
Factoring runs the box backward: the corners hold x² and the constant, the two middle cells add to the middle term, and the edges are the factors.
  1. 13.42.1

    The Greatest Common Factor of Two Monomials

    GCF of the coefficients, times each shared variable at its lowest power.

    GCF(12x3y, 18x2y4)=6x2y\displaystyle \text{GCF}(12x^3y,\ 18x^2y^4) = 6x^2y
  2. 13.42.2

    The Least Common Multiple of Two Monomials

    Take the LCM of the coefficients. Then take each variable to the highest power it has in either monomial.

    e.g. LCM of 6x2y6x^2y and 8xy38xy^3 is 24x2y324x^2y^3

    LCM(xm,xn)=xmax⁡(m,n)\displaystyle \text{LCM}(x^m, x^n) = x^{\max(m, n)}
  3. 13.42.3

    The Least Common Multiple of Two Polynomials

    Factor each polynomial completely. The LCM uses every factor that appears, each raised to the highest power it has in either polynomial.

    e.g. x2−9=(x−3)(x+3)x^2 - 9 = (x - 3)(x + 3) and x2+6x+9=(x+3)2x^2 + 6x + 9 = (x + 3)^2: LCM =(x−3)(x+3)2= (x - 3)(x + 3)^2

  4. 13.42.4

    Factoring Polynomials Using GCFs

    Always look for a common factor first.

    6x3−9x2=3x2(2x−3)\displaystyle 6x^3 - 9x^2 = 3x^2(2x - 3)
  5. 13.42.5

    Factoring Perfect Square Trinomials

    First and last terms are squares and the middle is twice their product.

    a2+2ab+b2=(a+b)2\displaystyle a^2 + 2ab + b^2 = (a + b)^2
    x2−10x+25=(x−5)2\displaystyle x^2 - 10x + 25 = (x - 5)^2
  6. 13.42.6

    Factoring Perfect Square Trinomials With Leading Coefficients

    The same test, with a coefficient on the first term.

    4x2+12x+9=(2x+3)2\displaystyle 4x^2 + 12x + 9 = (2x + 3)^2
  7. 13.42.7

    Factoring Differences of Squares

    Two squares with a minus between them.

    e.g. A sum of squares a2+b2a^2 + b^2 doesn’t factor

    a2−b2=(a+b)(a−b)\displaystyle a^2 - b^2 = (a + b)(a - b)
    9x2−16=(3x+4)(3x−4)\displaystyle 9x^2 - 16 = (3x + 4)(3x - 4)
  8. 13.42.8

    Factoring Differences of Squares Using Surds

    Any positive number is a square of its square root, so x2−bx^2 - b factors for any b>0b > 0.

    e.g. x2−12=(x−23)(x+23)x^2 - 12 = (x - 2\sqrt3)(x + 2\sqrt3)

    x2−b=(x−b)(x+b)\displaystyle x^2 - b = (x - \sqrt b)(x + \sqrt b)
  9. 13.42.9

    Factoring Trinomials

    For x2+bx+cx^2 + bx + c, find two numbers that multiply to cc and add to bb.

    e.g. x2+7x+12=(x+3)(x+4)x^2 + 7x + 12 = (x + 3)(x + 4)

    x2+bx+c=(x+p)(x+q)\displaystyle x^2 + bx + c = (x + p)(x + q)
    pq=c,p+q=b\displaystyle pq = c,\quad p + q = b
  10. 13.42.10

    Factoring Trinomials Using Common Factors

    Pull out the GCF first, then factor what is left.

    2x2−8x−24=2(x2−4x−12)\displaystyle 2x^2 - 8x - 24 = 2(x^2 - 4x - 12)
    =2(x−6)(x+2)\displaystyle = 2(x - 6)(x + 2)
  11. 13.42.11

    Factoring Trinomials With Leading Coefficients

    For ax2+bx+cax^2 + bx + c, find two numbers that multiply to acac and add to bb. Split the middle term and factor by grouping.

    e.g. 2x2+7x+32x^2 + 7x + 3: ac=6ac = 6 → 6 and 1 → 2x2+6x+x+3=(2x+1)(x+3)2x^2 + 6x + x + 3 = (2x + 1)(x + 3)

  12. 13.42.12

    Further Factoring Trinomials With Leading Coefficients

    With a negative leading coefficient, factor out −1-1 first. Check by multiplying back.

    e.g. −3x2+x+2=−(3x2−x−2)=−(3x+2)(x−1)-3x^2 + x + 2 = -(3x^2 - x - 2) = -(3x + 2)(x - 1)

  13. 13.42.13

    Factoring Biquadratic Expressions

    A biquadratic has the form ax4+bx2+cax^4 + bx^2 + c. Substitute u=x2u = x^2, factor the quadratic in uu, then put x2x^2 back and factor further if possible.

    e.g. x4−5x2+4=(x2−1)(x2−4)=(x−1)(x+1)(x−2)(x+2)x^4 - 5x^2 + 4 = (x^2 - 1)(x^2 - 4) = (x - 1)(x + 1)(x - 2)(x + 2)

    ax4+bx2+c\displaystyle ax^4 + bx^2 + c
    u=x2:  au2+bu+c\displaystyle u = x^2:\; au^2 + bu + c
  14. 13.42.14

    Factoring Expressions Containing Binomials

    Treat a repeated binomial as a single factor and pull it out. If two binomials are opposites, use b−a=−(a−b)b - a = -(a - b) to make them match.

    e.g. x(x+3)−2(x+3)=(x+3)(x−2)x(x + 3) - 2(x + 3) = (x + 3)(x - 2)

    aB+cB=(a+c)B\displaystyle aB + cB = (a + c)B
    b−a=−(a−b)\displaystyle b - a = -(a - b)
  15. 13.42.15

    Factoring Expressions Containing Hidden Factors

    Pull out the greatest common factor first, then factor what is left. Keep going until no factor can be factored further. Watch for a quadratic in disguise, such as one in x2x^2.

    e.g. 3x3−12x=3x(x2−4)=3x(x−2)(x+2)3x^3 - 12x = 3x(x^2 - 4) = 3x(x - 2)(x + 2)

    x4−5x2+4\displaystyle x^4 - 5x^2 + 4
    =(x2−1)(x2−4)\displaystyle = (x^2 - 1)(x^2 - 4)
    =(x−1)(x+1)(x−2)(x+2)\displaystyle = (x-1)(x+1)(x-2)(x+2)
  16. 13.42.16

    Equating Polynomial Coefficients

    Two polynomials equal for every xx have equal coefficients term by term.

    e.g. (x+k)2=x2+8x+m⇒k=4, m=16(x + k)^2 = x^2 + 8x + m \Rightarrow k = 4,\ m = 16

    ax2+bx+c≡px2+qx+r\displaystyle ax^2 + bx + c \equiv px^2 + qx + r
    ⇒  a=p, b=q, c=r\displaystyle \Rightarrow\; a = p,\ b = q,\ c = r

13.43 Quadratic Equations

D > 0two solutionsD = 0one solutionD < 0no real solution
D = b² − 4ac. The solutions are where the parabola meets the x-axis, so D says whether it crosses twice, touches once, or misses.
  1. 13.43.1

    Introduction to Quadratic Equations

    Degree 2. Written in standard form, it has at most two real solutions.

    ax2+bx+c=0(a≠0)\displaystyle ax^2 + bx + c = 0 \quad (a \ne 0)
  2. 13.43.2

    Solving Equations Using the Square Root Method

    Isolate the square, then take the square root of both sides. Keep the negative root.

    e.g. (x−3)2=16⇒x−3=±4⇒x=7(x - 3)^2 = 16 \Rightarrow x - 3 = \pm 4 \Rightarrow x = 7 or −1-1

    x2=k  ⇒  x=±k(k≥0)\displaystyle x^2 = k \;\Rightarrow\; x = \pm\sqrt{k} \quad (k \ge 0)
  3. 13.43.3

    Solving Equations With Odd Exponents Using the Nth Root Method

    An odd power has exactly one real root, and it can be negative.

    e.g. x3=−64⇒x=−4x^3 = -64 \Rightarrow x = -4

    xn=k, n odd  ⇒  x=kn\displaystyle x^n = k,\ n \text{ odd} \;\Rightarrow\; x = \sqrt[n]{k}
  4. 13.43.4

    Solving Equations With Even Exponents Using the Nth Root Method

    An even power has two real roots when k>0k > 0, one when k=0k = 0, and none when k<0k < 0.

    e.g. x4=81⇒x=±3x^4 = 81 \Rightarrow x = \pm 3

    xn=k, n even, k>0\displaystyle x^n = k,\ n \text{ even},\ k > 0
    ⇒  x=±kn\displaystyle \Rightarrow\; x = \pm\sqrt[n]{k}
  5. 13.43.5

    Solving Perfect Square Quadratic Equations

    Write it as a square equal to a number, then take ±\pm square roots.

    e.g. (x−2)2=9⇒x=5(x - 2)^2 = 9 \Rightarrow x = 5 or −1-1

    (x+p)2=k  ⇒  x=−p±k\displaystyle (x + p)^2 = k \;\Rightarrow\; x = -p \pm \sqrt{k}
  6. 13.43.6

    Perfect Square Quadratic Equations with One or No Solutions

    k=0k = 0 gives one solution. k<0k < 0 gives none, since no real number squares to a negative.

    (x+p)2=0  ⇒  x=−p\displaystyle (x + p)^2 = 0 \;\Rightarrow\; x = -p
    (x+p)2=−4  ⇒  no real solution\displaystyle (x + p)^2 = -4 \;\Rightarrow\; \text{no real solution}
  7. 13.43.7

    The Zero Product Rule for Solving Quadratic Equations

    If a product is zero, one of the factors is zero. One side must be 0 first.

    e.g. (x−3)(x+5)=0⇒x=3(x - 3)(x + 5) = 0 \Rightarrow x = 3 or −5-5

    ab=0  ⇒  a=0 or b=0\displaystyle ab = 0 \;\Rightarrow\; a = 0 \text{ or } b = 0
  8. 13.43.8

    The Zero Product Rule for Solving Polynomial Equations

    If a product is zero, at least one factor is zero. Move everything to one side, factor completely, and set each factor equal to zero. Never divide both sides by the variable, since that loses the root x=0x = 0.

    e.g. x3=4x⇒x(x−2)(x+2)=0⇒x=0,±2x^3 = 4x \Rightarrow x(x - 2)(x + 2) = 0 \Rightarrow x = 0, \pm 2

    ab=0⇒a=0 or b=0\displaystyle ab = 0 \Rightarrow a = 0 \text{ or } b = 0
  9. 13.43.9

    Solving Quadratic Equations Using a Difference of Squares

    Factor the difference of squares and use the zero product rule.

    e.g. 4x2−25=0⇒x=±524x^2 - 25 = 0 \Rightarrow x = \pm\tfrac52

    x2−k2=0\displaystyle x^2 - k^2 = 0
    ⇒  (x−k)(x+k)=0\displaystyle \Rightarrow\; (x - k)(x + k) = 0
    ⇒  x=±k\displaystyle \Rightarrow\; x = \pm k
  10. 13.43.10

    Solving Quadratic Equations with No Constant Term

    Factor out xx. Zero is always a solution; dividing by xx would lose it.

    ax2+bx=0\displaystyle ax^2 + bx = 0
    ⇒  x(ax+b)=0\displaystyle \Rightarrow\; x(ax + b) = 0
    ⇒  x=0 or x=−ba\displaystyle \Rightarrow\; x = 0 \text{ or } x = -\tfrac{b}{a}
  11. 13.43.11

    Solving Quadratic Equations by Factoring

    Get 0 on one side, factor, then set each factor to zero.

    e.g. x=3x = 3 or −2-2

    x2−x−6=0\displaystyle x^2 - x - 6 = 0
    ⇒  (x−3)(x+2)=0\displaystyle \Rightarrow\; (x - 3)(x + 2) = 0
  12. 13.43.12

    Solving Quadratic Equations with Leading Coefficients by Factoring

    Factor ax2+bx+cax^2 + bx + c with the acac method, then set each factor to zero.

    e.g. x=−13x = -\tfrac13 or 22

    3x2−5x−2=0\displaystyle 3x^2 - 5x - 2 = 0
    ⇒  (3x+1)(x−2)=0\displaystyle \Rightarrow\; (3x + 1)(x - 2) = 0
  13. 13.43.13

    Completing the Square

    Add the square of half the xx-coefficient.

    e.g. x2+6x+9=(x+3)2x^2 + 6x + 9 = (x + 3)^2

    x2+bx+(b2)2=(x+b2)2\displaystyle x^2 + bx + \left(\tfrac{b}{2}\right)^2 = \left(x + \tfrac{b}{2}\right)^2
  14. 13.43.14

    Completing the Square With Odd Linear Terms

    The same rule; half of an odd number is a fraction.

    x2+5x+254=(x+52)2\displaystyle x^2 + 5x + \tfrac{25}{4} = \left(x + \tfrac{5}{2}\right)^2
  15. 13.43.15

    Completing the Square With Leading Coefficients

    Factor aa out of the xx-terms, complete the square inside, and adjust the constant.

    2x2+12x+5=2(x+3)2−13\displaystyle 2x^2 + 12x + 5 = 2(x + 3)^2 - 13
  16. 13.43.16

    Solving Quadratic Equations by Completing the Square

    Move cc across, complete the square on both sides, take ±\pm roots.

    e.g. x2+6x=7⇒(x+3)2=16⇒x=1x^2 + 6x = 7 \Rightarrow (x + 3)^2 = 16 \Rightarrow x = 1 or −7-7

  17. 13.43.17

    Solving Quadratic Equations With Leading Coefficients by Completing the Square

    Divide every term by aa first, then complete the square.

    e.g. 2x2−8x−10=0⇒x2−4x=5⇒(x−2)2=9⇒x=52x^2 - 8x - 10 = 0 \Rightarrow x^2 - 4x = 5 \Rightarrow (x - 2)^2 = 9 \Rightarrow x = 5 or −1-1

  18. 13.43.18

    The Quadratic Formula

    Works for every quadratic in standard form.

    e.g. x2−4x+1=0⇒x=2±3x^2 - 4x + 1 = 0 \Rightarrow x = 2 \pm \sqrt3

    x=−b±b2−4ac2a\displaystyle x = \frac{-b \pm \sqrt{b^2 - 4ac}}{2a}
  19. 13.43.19

    The Discriminant of a Quadratic Equation

    b2−4acb^2 - 4ac tells how many real solutions there are without solving.

    D=b2−4ac\displaystyle D = b^2 - 4ac
    D>0: two solutions\displaystyle D > 0:\ \text{two solutions}
    D=0: one solution\displaystyle D = 0:\ \text{one solution}
    D<0: no real solution\displaystyle D < 0:\ \text{no real solution}
  20. 13.43.20

    Vieta's Formulas

    The sum and product of the roots come straight from the coefficients.

    e.g. x2−7x+10x^2 - 7x + 10: roots sum to 7 and multiply to 10 (they are 2 and 5)

    r1+r2=−ba\displaystyle r_1 + r_2 = -\frac{b}{a}
    r1r2=ca\displaystyle r_1r_2 = \frac{c}{a}
  21. 13.43.21

    Solving Biquadratic Equations

    Let u=x2u = x^2 and solve the quadratic in uu. Then solve x2=ux^2 = u for each value of uu. A negative uu gives imaginary solutions, so there can be up to 4 solutions.

    e.g. x4−5x2−36=0⇒(x2−9)(x2+4)=0⇒x=±3,±2ix^4 - 5x^2 - 36 = 0 \Rightarrow (x^2 - 9)(x^2 + 4) = 0 \Rightarrow x = \pm 3, \pm 2i

    ax4+bx2+c=0\displaystyle ax^4 + bx^2 + c = 0
    u=x2:  au2+bu+c=0\displaystyle u = x^2:\; au^2 + bu + c = 0
    x=±u\displaystyle x = \pm\sqrt{u}
  22. 13.43.22

    Solving Quadratic Equations Containing Unknown Parameters

    Treat the parameter as a known number. If you know one solution, substitute it to find the parameter. Otherwise factor or use the quadratic formula to get xx in terms of the parameter.

    e.g. x2−kx+12=0x^2 - kx + 12 = 0 has root 3: 9−3k+12=0⇒k=79 - 3k + 12 = 0 \Rightarrow k = 7, and the other root is 4

    x=−b±b2−4ac2a\displaystyle x = \frac{-b \pm \sqrt{b^2 - 4ac}}{2a}
  23. 13.43.23

    Determining Unknown Parameters in Quadratic Equations With One Real Solution

    Set the discriminant equal to zero and solve for the parameter.

    e.g. x2+kx+9=0x^2 + kx + 9 = 0 has one solution when k2=36k^2 = 36, k=±6k = \pm 6

    b2−4ac=0\displaystyle b^2 - 4ac = 0
  24. 13.43.24

    Solving Elementary Quadratic Inequalities

    For c>0c > 0: x2<cx^2 < c gives the values between the roots, and x2>cx^2 > c gives the values outside them. If c<0c < 0, x2<cx^2 < c has no solution and x2>cx^2 > c holds for all xx.

    e.g. x2≤9⇒−3≤x≤3x^2 \le 9 \Rightarrow -3 \le x \le 3

    x2<c  ⇒  −c<x<c\displaystyle x^2 < c \;\Rightarrow\; -\sqrt{c} < x < \sqrt{c}
    x2>c  ⇒  x<−c\displaystyle x^2 > c \;\Rightarrow\; x < -\sqrt{c}
    or  x>c\displaystyle \text{or}\; x > \sqrt{c}
  25. 13.43.25

    Determining Unknown Parameters in Quadratic Equations With Real Solutions

    ax2+bx+c=0ax^2 + bx + c = 0 has real solutions when the discriminant is at least 0, and two distinct real solutions when it is positive. Solve that inequality for the parameter.

    e.g. x2+kx+9=0x^2 + kx + 9 = 0: k2−36≥0⇒k≤−6k^2 - 36 \ge 0 \Rightarrow k \le -6 or k≥6k \ge 6

    b2−4ac≥0\displaystyle b^2 - 4ac \ge 0
  26. 13.43.26

    Determining Unknown Parameters in Quadratic Equations With No Real Solutions

    A quadratic has no real solutions when its discriminant is negative. Solve that inequality for the parameter.

    e.g. x2+4x+k=0x^2 + 4x + k = 0: 16−4k<0⇒k>416 - 4k < 0 \Rightarrow k > 4

    b2−4ac<0\displaystyle b^2 - 4ac < 0
  27. 13.43.27

    Reasoning About Coefficients of Quadratics Using Standard and Factored Forms

    Expanding factored form links the zeros to the coefficients. The zeros add to −ba-\tfrac{b}{a} and multiply to ca\tfrac{c}{a}.

    e.g. Zeros 2 and −5-5, a=3a = 3: 3(x−2)(x+5)=3x2+9x−303(x - 2)(x + 5) = 3x^2 + 9x - 30

    a(x−r)(x−s)\displaystyle a(x - r)(x - s)
    =ax2−a(r+s)x+ars\displaystyle = ax^2 - a(r + s)x + ars
    r+s=−ba,rs=ca\displaystyle r + s = -\frac{b}{a},\quad rs = \frac{c}{a}

13.44 Quadratic Functions

xy−3−2−112345−5−4−3−2−11234vertex (1, −4)rootroot(0, −3)axis x = 1y = x² − 2x − 3= (x − 1)² − 4= (x + 1)(x − 3)axis: x = −b ÷ 2a = 1roots: −1 and 3y-intercept: c = −3Standard, vertex, and factoredforms of one parabola.
The axis of symmetry runs through the vertex, halfway between the roots. Each form of the equation shows one of these features at a glance.
  1. 13.44.1

    Graphing Elementary Quadratic Functions

    y=x2y = x^2 is a U-shaped parabola with its vertex at the origin. In y=ax2y = ax^2, a larger ∣a∣\lvert a \rvert makes it narrower.

    y=ax2\displaystyle y = ax^2
  2. 13.44.2

    Vertical Reflections of Quadratic Functions

    A negative aa opens the parabola downward, so the vertex becomes a maximum.

    y=−x2\displaystyle y = -x^2
  3. 13.44.3

    Graphs of General Quadratic Functions

    aa sets direction and width; cc is the yy-intercept.

    y=ax2+bx+c\displaystyle y = ax^2 + bx + c
  4. 13.44.4

    Roots of Quadratic Functions

    Where the parabola meets the xx-axis: solve ax2+bx+c=0ax^2 + bx + c = 0.

  5. 13.44.5

    The Discriminant of a Quadratic Function

    Counts the xx-intercepts: two, one (vertex on the axis), or none.

    D=b2−4ac\displaystyle D = b^2 - 4ac
  6. 13.44.6

    The Axis of Symmetry of a Parabola

    A vertical line through the vertex. The parabola mirrors across it.

    e.g. y=x2−6x+5y = x^2 - 6x + 5: axis x=3x = 3

    x=−b2a\displaystyle x = -\frac{b}{2a}
  7. 13.44.7

    The Average of the Roots Formula

    The axis sits exactly halfway between the roots.

    e.g. Roots 1 and 5 → vertex at x=3x = 3

    xvertex=r1+r22\displaystyle x_{\text{vertex}} = \frac{r_1 + r_2}{2}
  8. 13.44.8

    The Vertex Form of a Parabola

    The vertex is at (h,k)(h, k). Watch the sign inside: (x−h)(x - h).

    e.g. y=2(x+1)2−3y = 2(x + 1)^2 - 3: vertex (−1,−3)(-1, -3)

    y=a(x−h)2+k\displaystyle y = a(x - h)^2 + k
  9. 13.44.9

    Writing the Equation of a Parabola in Vertex Form

    Complete the square, or find h=−b2ah = -\tfrac{b}{2a} and then k=f(h)k = f(h).

    e.g. y=x2−6x+5=(x−3)2−4y = x^2 - 6x + 5 = (x - 3)^2 - 4

  10. 13.44.10

    Fitting Quadratic Functions to Data Using Vertex Form

    Find the vertex (h,k)(h, k) from the data, often the turning point or the middle of matching yy-values. Then plug in one other point to solve for aa.

    e.g. Vertex (2,5)(2, 5), point (4,13)(4, 13): 13=4a+5⇒a=213 = 4a + 5 \Rightarrow a = 2, so y=2(x−2)2+5y = 2(x - 2)^2 + 5

    y=a(x−h)2+k\displaystyle y = a(x - h)^2 + k
  11. 13.44.11

    Reasoning About Coefficients of Quadratics Using Symmetry

    Two points on a parabola with the same yy-value are mirror images across the axis of symmetry. The axis lies halfway between them.

    e.g. f(1)=f(7)f(1) = f(7): axis x=4x = 4. If a=1a = 1, then −b2=4-\tfrac{b}{2} = 4, so b=−8b = -8

    x=x1+x22=−b2a\displaystyle x = \frac{x_1 + x_2}{2} = -\frac{b}{2a}

13.45 Systems of Equations

  1. 13.45.1

    Solving Systems of Nonlinear Equations Using Graphs

    Graph both. Each crossing point is a solution. A line and a parabola cross 0, 1, or 2 times.

  2. 13.45.2

    Solving Systems of Nonlinear Equations by Identifying Structure

    Look for an expression that appears in both equations, such as x2x^2, and treat it as a single unknown. Then add, subtract, or substitute the whole expression.

    e.g. x2+y=11x^2 + y = 11 and x2−y=7x^2 - y = 7: add to get 2x2=182x^2 = 18, so x=±3x = \pm 3 and y=2y = 2

  3. 13.45.3

    Solving Systems of Nonlinear Equations

    Substitute one equation into the other, set it to zero, and solve the quadratic.

    e.g. Solutions (2,4)(2, 4) and (−1,1)(-1, 1)

    y=x2, y=x+2\displaystyle y = x^2,\ y = x + 2
    ⇒  x2−x−2=0\displaystyle \Rightarrow\; x^2 - x - 2 = 0
  4. 13.45.4

    Finding Intersections of Lines and Quadratic Functions

    Set the two equal. The discriminant of the result gives 2 crossings, 1 (the line just touches), or 0.

    ax2+bx+c=mx+d\displaystyle ax^2 + bx + c = mx + d
  5. 13.45.5

    Determining Unknown Parameters in Quadratic Systems With One Intersection Point

    Set the equations equal and rearrange to ax2+bx+c=0ax^2 + bx + c = 0. Exactly one intersection means the discriminant is zero.

    e.g. y=x2+4y = x^2 + 4, y=kxy = kx: x2−kx+4=0x^2 - kx + 4 = 0, k2−16=0k^2 - 16 = 0, so k=±4k = \pm 4

    b2−4ac=0\displaystyle b^2 - 4ac = 0
  6. 13.45.6

    Determining Unknown Parameters in Quadratic Systems With Zero or Two Intersection

    Set the equations equal and rearrange to ax2+bx+c=0ax^2 + bx + c = 0. A positive discriminant gives two intersections, and a negative one gives none.

    e.g. y=x2y = x^2, y=x+cy = x + c: x2−x−c=0x^2 - x - c = 0, discriminant 1+4c1 + 4c. Two points if c>−14c > -\tfrac14, none if c<−14c < -\tfrac14

    b2−4ac>0  →  two points\displaystyle b^2 - 4ac > 0 \;\to\; \text{two points}
    b2−4ac<0  →  no points\displaystyle b^2 - 4ac < 0 \;\to\; \text{no points}

13.46 Modeling With Quadratic Functions

01632486401234time (s)height (ft)peak (2, 64)lands t = 4h(t) = −16t² + 64tpeak at t = −b ÷ 2a = 2h(2) = 64 ftlands when h(t) = 0:−16t(t − 4) = 0 → t = 4
A thrown object’s height is a downward parabola in time. The vertex gives the peak; the positive root gives the landing.
  1. 13.46.1

    Modeling Downwards Vertical Motion

    A dropped object falls 16t216t^2 feet in tt seconds.

    e.g. Dropped from 144 ft → lands when 16t2=14416t^2 = 144, t=3t = 3 s

    h(t)=−16t2+h0\displaystyle h(t) = -16t^2 + h_0
    h(t)=−4.9t2+h0  (meters)\displaystyle h(t) = -4.9t^2 + h_0 \;\text{(meters)}
  2. 13.46.2

    Modeling Upwards Vertical Motion

    Launched upward at speed v0v_0 from height h0h_0.

    h(t)=−16t2+v0t+h0\displaystyle h(t) = -16t^2 + v_0t + h_0
  3. 13.46.3

    Vertical Motion

    Maximum height is at the vertex. It lands when h(t)=0h(t) = 0; keep the positive root.

    e.g. h=−16t2+64th = -16t^2 + 64t peaks at t=2t = 2 s, 64 ft

    tpeak=−b2a=v032\displaystyle t_{\text{peak}} = -\frac{b}{2a} = \frac{v_0}{32}
  4. 13.46.4

    Revenue, Cost, and Profit Functions

    Revenue is price times quantity. Profit is revenue minus cost.

    R=p q\displaystyle R = p\,q
    P=R−C\displaystyle P = R - C
  5. 13.46.5

    Modeling Using Systems of Non-Linear Equations

    Write one equation for each condition, then solve by substitution. On the SAT, graphing both equations in Desmos and reading the intersection is often fastest. Keep only solutions that make sense in context.

    e.g. Rectangle with area 24 and perimeter 20: l+w=10l + w = 10, lw=24⇒w2−10w+24=0⇒lw = 24 \Rightarrow w^2 - 10w + 24 = 0 \Rightarrow 6 by 4

13.47 Polynomial Expressions & Equations

  1. 13.47.1

    Further Factoring of Polynomials Using GCFs

    Factor out the GCF first, including common variable powers (and −1-1 if the leading term is negative). The GCF can be a binomial. Then factor what remains.

    e.g. 3x3−12x2−36x=3x(x2−4x−12)=3x(x−6)(x+2)3x^3 - 12x^2 - 36x = 3x(x^2 - 4x - 12) = 3x(x - 6)(x + 2)

  2. 13.47.2

    Factoring Higher-Order Polynomials as a Difference of Squares

    Write both terms as squares and use a2−b2=(a+b)(a−b)a^2 - b^2 = (a + b)(a - b). Check whether a factor is again a difference of squares. A sum of squares a2+b2a^2 + b^2 does not factor over the reals.

    e.g. x4−16=(x2+4)(x2−4)=(x2+4)(x+2)(x−2)x^4 - 16 = (x^2 + 4)(x^2 - 4) = (x^2 + 4)(x + 2)(x - 2)

    a2−b2=(a+b)(a−b)\displaystyle a^2 - b^2 = (a + b)(a - b)
    x4−y4\displaystyle x^4 - y^4
    =(x2+y2)(x+y)(x−y)\displaystyle = (x^2 + y^2)(x + y)(x - y)
  3. 13.47.3

    Factoring Cubic Expressions by Grouping

    Split the four terms into two pairs. Factor the GCF out of each pair, then factor out the common binomial.

    e.g. x3+3x2−4x−12=x2(x+3)−4(x+3)=(x+3)(x+2)(x−2)x^3 + 3x^2 - 4x - 12 = x^2(x + 3) - 4(x + 3) = (x + 3)(x + 2)(x - 2)

    x3+ax2+bx+ab\displaystyle x^3 + ax^2 + bx + ab
    =x2(x+a)+b(x+a)\displaystyle = x^2(x + a) + b(x + a)
    =(x+a)(x2+b)\displaystyle = (x + a)(x^2 + b)
  4. 13.47.4

    Determining the Roots of Polynomials

    The roots are the xx-values that make the polynomial equal 0. Factor completely and set each factor equal to 0. A factor (x−r)k(x - r)^k gives the root rr with multiplicity kk.

    e.g. p(x)=(x−2)2(x+5)p(x) = (x - 2)^2(x + 5): roots 22 (multiplicity 2) and −5-5

    (x−r)(x−s)=0\displaystyle (x - r)(x - s) = 0
    ⇒  x=r  or  x=s\displaystyle \Rightarrow\; x = r \;\text{or}\; x = s
  5. 13.47.5

    Solving Polynomial Equations Using the GCF

    Move every term to one side so the equation equals 0. Factor out the GCF, then set each factor equal to 0. Never divide both sides by xx, since that loses the root x=0x = 0.

    e.g. 2x3=18x⇒2x(x−3)(x+3)=0⇒x=0,±32x^3 = 18x \Rightarrow 2x(x - 3)(x + 3) = 0 \Rightarrow x = 0, \pm 3

13.48 Polynomial Theorems

  1. 13.48.1

    The Factor Theorem

    (x−c)(x - c) is a factor of p(x)p(x) exactly when p(c)=0p(c) = 0.

    e.g. p(x)=x3−8p(x) = x^3 - 8: p(2)=0p(2) = 0, so x−2x - 2 is a factor

    p(c)=0  ⟺  (x−c) is a factor\displaystyle p(c) = 0 \iff (x - c) \text{ is a factor}
  2. 13.48.2

    Reasoning About Coefficients in Quadratic Equations Using the Factor Theorem

    (x−r)(x - r) is a factor of p(x)p(x) exactly when p(r)=0p(r) = 0. Substitute rr and solve for the unknown coefficient. A factor (x+3)(x + 3) means p(−3)=0p(-3) = 0.

    e.g. x−2x - 2 is a factor of x2+bx−10x^2 + bx - 10: 4+2b−10=04 + 2b - 10 = 0, so b=3b = 3

    (x−r) is a factor  ⟺  p(r)=0\displaystyle (x - r) \text{ is a factor} \iff p(r) = 0
  3. 13.48.3

    Factoring Cubic Polynomials Using the Factor Theorem

    Test small divisors of the constant term until p(c)=0p(c) = 0. Divide by (x−c)(x - c), then factor the remaining quadratic.

    e.g. x3−6x2+11x−6x^3 - 6x^2 + 11x - 6: p(1)=0p(1) = 0, so (x−1)(x2−5x+6)=(x−1)(x−2)(x−3)(x - 1)(x^2 - 5x + 6) = (x - 1)(x - 2)(x - 3)

    p(x)=(x−c) q(x)\displaystyle p(x) = (x - c)\,q(x)
  4. 13.48.4

    Multiplicities of the Roots of Polynomials

    A root's multiplicity is the number of times its factor appears. At a root of odd multiplicity the graph crosses the xx-axis. At even multiplicity it touches and turns back.

    e.g. (x−1)2(x+3)(x - 1)^2(x + 3): x=1x = 1 has multiplicity 2 (touches), x=−3x = -3 has multiplicity 1 (crosses)

    p(x)=(x−c)m q(x)\displaystyle p(x) = (x - c)^m\,q(x)
    q(c)≠0\displaystyle q(c) \ne 0
  5. 13.48.5

    Dividing Polynomials Using Synthetic Division

    To divide by x−cx - c, write cc and the coefficients (0 for any missing power). Bring down the first, multiply by cc, add to the next column, and repeat. The last number is the remainder; the rest are the quotient's coefficients, one degree lower.

    e.g. (x3−2x2−5x+6)÷(x−3)(x^3 - 2x^2 - 5x + 6) \div (x - 3): 1,−2,−5,61, -2, -5, 6 becomes 1,1,−2,01, 1, -2, 0, so x2+x−2x^2 + x - 2, remainder 0

    p(x)=(x−c) q(x)+R\displaystyle p(x) = (x - c)\,q(x) + R
  6. 13.48.6

    The Remainder Theorem

    When p(x)p(x) is divided by (x−c)(x - c), the remainder is p(c)p(c).

    e.g. (x3−2x+5)÷(x−2)(x^3 - 2x + 5) \div (x - 2): remainder p(2)=8−4+5=9p(2) = 8 - 4 + 5 = 9

    p(x)=(x−c) q(x)+p(c)\displaystyle p(x) = (x - c)\,q(x) + p(c)

13.49 Graphs of Polynomials

xycrossescrosses(odd multiplicity)touches(even multiplicity)−23y = ¼(x + 2)(x − 1)2(x − 3)single roots −2 and 3, double root 1End behaviora > 0a < 0evendegreeodddegreea = leading coefficient
A root of odd multiplicity crosses the x-axis and a root of even multiplicity only touches it. The degree and the sign of the leading coefficient fix which way the two ends point.
  1. 13.49.1

    Graphing Elementary Cubic Functions

    y=x3y = x^3 passes through the origin, rises from left to right, and is symmetric about the origin. In the transformed form the center point moves to (h,k)(h, k) and a negative aa flips the graph.

    e.g. y=(x−1)3+2y = (x - 1)^3 + 2: center (1,2)(1, 2), also through (2,3)(2, 3) and (0,1)(0, 1)

    y=a(x−h)3+k\displaystyle y = a(x - h)^3 + k
  2. 13.49.2

    Graphing Cubic Curves Containing Three Distinct Real Roots

    The graph crosses the xx-axis at each root. If a>0a > 0 it falls on the left and rises on the right; if a<0a < 0 the reverse. Plug in x=0x = 0 for the yy-intercept.

    e.g. y=(x+1)(x−1)(x−2)y = (x + 1)(x - 1)(x - 2): crosses at −1,1,2-1, 1, 2; yy-intercept 2

    y=a(x−r1)(x−r2)(x−r3)\displaystyle y = a(x - r_1)(x - r_2)(x - r_3)
  3. 13.49.3

    Graphing Cubic Curves Containing a Double Root

    The squared factor gives a root where the graph touches the xx-axis and turns back. The graph crosses at the single root.

    e.g. y=(x−1)2(x+2)y = (x - 1)^2(x + 2): touches at x=1x = 1, crosses at x=−2x = -2, yy-intercept 2

    y=a(x−r)2(x−s)\displaystyle y = a(x - r)^2(x - s)
  4. 13.49.4

    Graphing Cubic Curves Containing One Distinct Real Root

    The cubic factors as a linear factor times a quadratic with no real roots, so the graph crosses the xx-axis only once.

    e.g. y=(x−2)(x2+1)y = (x - 2)(x^2 + 1): crosses only at x=2x = 2, yy-intercept −2-2

    y=a(x−r)(x2+bx+c)\displaystyle y = a(x - r)(x^2 + bx + c)
    b2−4c<0\displaystyle b^2 - 4c < 0
  5. 13.49.5

    End Behavior of Polynomials

    For large ∣x∣\lvert x \rvert the leading term anxna_n x^n controls the graph. Even degree: both ends point the same way, up if an>0a_n > 0. Odd degree: the ends point opposite ways, rising on the right if an>0a_n > 0.

    e.g. f(x)=−2x3+xf(x) = -2x^3 + x: as x→∞x \to \infty, f(x)→−∞f(x) \to -\infty; as x→−∞x \to -\infty, f(x)→∞f(x) \to \infty

  6. 13.49.6

    Graphing General Polynomials

    Factor to find the roots and their multiplicities, find the yy-intercept, and use the end behavior. Cross at odd multiplicity, touch at even, and connect smoothly. A degree nn polynomial has at most n−1n - 1 turning points.

    e.g. y=x(x−2)2(x+1)y = x(x - 2)^2(x + 1): degree 4 with a>0a > 0, so both ends up; crosses at −1-1 and 0, touches at 2

  7. 13.49.7

    Identifying Valid Outputs of Factored Polynomials

    The zeros split the number line into intervals, and p(x)p(x) keeps one sign on each interval. Test one input per interval to find the sign. The sign does not change at a factor raised to an even power.

    e.g. p(x)=(x+1)(x−3)p(x) = (x + 1)(x - 3): p(0)=−3p(0) = -3, so p(x)<0p(x) < 0 for all −1<x<3-1 < x < 3. p(1)p(1) could not be 5

Unit 14 33 topics

Advanced Algebra - Exponential Equations & Functions

Exponential Expressions & Equations, Exponential Functions, and Graphs of Exponential Functions.

14.50 Exponential Expressions & Equations

  1. 14.50.1

    Writing Radical Expressions Using Fractional Exponents

    The denominator is the root; the numerator is the power.

    e.g. x3/2=x3x^{3/2} = \sqrt{x^3}

    am/n=amn=(an)m\displaystyle a^{m/n} = \sqrt[n]{a^m} = \left(\sqrt[n]{a}\right)^m
  2. 14.50.2

    The Product Rule for Exponents With Algebraic Expressions

    Multiply the coefficients, add the exponents of matching bases.

    e.g. 3x2⋅4x5=12x73x^2 \cdot 4x^5 = 12x^7

    am⋅an=am+n\displaystyle a^m \cdot a^n = a^{m+n}
  3. 14.50.3

    The Quotient Rule for Exponents With Algebraic Expressions

    Divide the coefficients, subtract the exponents of matching bases.

    e.g. 10x6y2x2y=5x4\tfrac{10x^6y}{2x^2y} = 5x^4

    aman=am−n\displaystyle \frac{a^m}{a^n} = a^{m-n}
  4. 14.50.4

    The Power Rule for Exponents With Algebraic Expressions

    A power of a power multiplies the exponents.

    e.g. (x3)4=x12(x^3)^4 = x^{12}

    (am)n=amn\displaystyle (a^m)^n = a^{mn}
  5. 14.50.5

    The Power of Product Rule With Algebraic Expressions

    The outside power goes to every factor, including the coefficient and its sign.

    e.g. (−2x3y)2=4x6y2(-2x^3y)^2 = 4x^6y^2

    (ab)n=anbn\displaystyle (ab)^n = a^nb^n
  6. 14.50.6

    The Power of Quotient Rule With Algebraic Expressions

    The outside power goes to the top and the bottom.

    e.g. (x23)3=x627\left(\tfrac{x^2}{3}\right)^3 = \tfrac{x^6}{27}

    (ab)n=anbn\displaystyle \left(\frac{a}{b}\right)^n = \frac{a^n}{b^n}
  7. 14.50.7

    Combining the Rules of Exponents With Algebraic Expressions

    Apply outside powers, combine matching bases, and finish with positive exponents.

    e.g. (2x2)34x−1=8x64x−1=2x7\dfrac{(2x^2)^3}{4x^{-1}} = \dfrac{8x^6}{4x^{-1}} = 2x^7

  8. 14.50.8

    Rewriting Radical Expressions Using the Laws of Exponents

    Rewrite each root as a fractional exponent, combine with the exponent laws, then convert back if needed.

    e.g. x⋅x3=x12+13=x5/6\sqrt{x} \cdot \sqrt[3]{x} = x^{\frac12 + \frac13} = x^{5/6}

    xmn=xm/n\displaystyle \sqrt[n]{x^m} = x^{m/n}
    1xn=x−1/n\displaystyle \frac{1}{\sqrt[n]{x}} = x^{-1/n}
  9. 14.50.9

    Applying the Distributive Law to Exponential Expressions

    Distribute by adding exponents on the same base. In reverse, factor out the smallest power.

    e.g. 3x+2−3x=3x(9−1)=8⋅3x3^{x+2} - 3^x = 3^x(9 - 1) = 8 \cdot 3^x

    am(an+ap)=am+n+am+p\displaystyle a^m(a^n + a^p) = a^{m+n} + a^{m+p}
    ax+n+ax=ax(an+1)\displaystyle a^{x+n} + a^x = a^x(a^n + 1)
  10. 14.50.10

    Combining Exponential Expressions

    Rewrite the terms with a common base, then apply the exponent laws.

    e.g. 8x⋅2x=23x⋅2x=24x8^x \cdot 2^x = 2^{3x} \cdot 2^x = 2^{4x}

    aman=am+n\displaystyle a^m a^n = a^{m+n}
    aman=am−n\displaystyle \frac{a^m}{a^n} = a^{m-n}
    (am)n=amn\displaystyle (a^m)^n = a^{mn}
  11. 14.50.11

    Solving Exponential Equations

    Rewrite both sides with the same base, then set the exponents equal.

    e.g. 2x+1=32=25⇒x=42^{x+1} = 32 = 2^5 \Rightarrow x = 4

    bm=bn  ⇒  m=n\displaystyle b^m = b^n \;\Rightarrow\; m = n
  12. 14.50.12

    Solving Exponential Equations with Fractional Solutions

    Use a base that both sides are powers of.

    4x=8  ⇒  22x=23  ⇒  x=32\displaystyle 4^x = 8 \;\Rightarrow\; 2^{2x} = 2^3 \;\Rightarrow\; x = \tfrac{3}{2}
  13. 14.50.13

    Creating Exponential Growth Expressions

    Growth by rate rr multiplies by 1+r1 + r each period.

    e.g. $500 growing 4% a year: 500(1.04)t500(1.04)^t

    a(1+r)t\displaystyle a(1 + r)^t
  14. 14.50.14

    Creating Exponential Decay Expressions

    Decay by rate rr multiplies by 1−r1 - r each period.

    e.g. A $20,000 car losing 15% a year: 20,000(0.85)t20{,}000(0.85)^t

    a(1−r)t\displaystyle a(1 - r)^t

14.51 Exponential Functions

0163248640123456y = 8xy = 2ˣLinear adds:0, 8, 16, 24, 32, 40, 48Exponential multiplies:1, 2, 4, 8, 16, 32, 64Exponential starts behindand still wins.
Equal differences mean linear; equal ratios mean exponential. Any exponential growth eventually passes any linear growth.
  1. 14.51.1

    Exponential Functions

    Starting value aa, multiplied by base bb at each step. Growth if b>1b > 1, decay if 0<b<10 < b < 1.

    f(x)=a bx(a≠0, b>0, b≠1)\displaystyle f(x) = a\,b^x \quad (a \ne 0,\ b > 0,\ b \ne 1)
  2. 14.51.2

    Modeling Exponential Growth With Functions

    Find the starting amount and the growth factor per time unit. For doubling every dd units, use 2t/d2^{t/d}.

    P(t)=P0(1+r)t\displaystyle P(t) = P_0(1 + r)^t
    P(t)=P0⋅2t/d\displaystyle P(t) = P_0 \cdot 2^{t/d}
  3. 14.51.3

    Interpreting Exponential Growth

    In a(1.06)ta(1.06)^t, aa is the starting value and 1.061.06 means 6% growth each period.

    e.g. b=1.25b = 1.25 → 25% growth per period

    r=b−1\displaystyle r = b - 1
  4. 14.51.4

    Solving Exponential Growth Problems

    Substitute tt to find a future value. To find tt, match bases or try values.

    e.g. 3,000 bacteria doubling hourly → after 4 h, 3000⋅24=48,0003000 \cdot 2^4 = 48{,}000

  5. 14.51.5

    Modeling Exponential Decay With Functions

    Use the decay factor per period, or a half-life hh.

    P(t)=P0(1−r)t\displaystyle P(t) = P_0(1 - r)^t
    P(t)=P0(12)t/h\displaystyle P(t) = P_0\left(\tfrac{1}{2}\right)^{t/h}
  6. 14.51.6

    Interpreting Exponential Decay

    b=0.9b = 0.9 means 90% is kept each period, so 10% is lost.

    r=1−b\displaystyle r = 1 - b
  7. 14.51.7

    Solving Exponential Decay Problems

    Count the periods, then apply the factor that many times.

    e.g. 80 mg with a 6 h half-life → after 18 h, 80(12)3=1080\left(\tfrac12\right)^3 = 10 mg

  8. 14.51.8

    Linear vs. Exponential Growth and Decay

    Linear adds the same amount each step. Exponential multiplies by the same factor.

    linear: yn+1−yn=m\displaystyle \text{linear: } y_{n+1} - y_n = m
    exponential: yn+1yn=b\displaystyle \text{exponential: } \frac{y_{n+1}}{y_n} = b
  9. 14.51.9

    Linear vs. Exponential Growth and Decay Models

    In a table, constant differences mean linear and constant ratios mean exponential. Exponential growth eventually passes any linear growth.

    e.g. 3, 6, 12, 24: ratio 2 → exponential

  10. 14.51.10

    Time-Shifting Exponential Models

    To restart the clock hh units later, replace tt with t+ht + h. The new starting value is the old model's value at t=ht = h.

    e.g. P(t)=100(2)tP(t) = 100(2)^t, tt = years since 2020. Measured from 2023: 100(2)t+3=800(2)t100(2)^{t+3} = 800(2)^t

    f(t)=abt\displaystyle f(t) = ab^t
    g(t)=f(t+h)=(abh) bt\displaystyle g(t) = f(t + h) = (ab^h)\,b^t
  11. 14.51.11

    Working With Equivalent Forms of Exponential Functions

    Use exponent rules to rewrite a model so its base matches the time period you need. Each form describes the same function.

    e.g. 1000(1.21)t=1000(1.1)2t1000(1.21)^t = 1000(1.1)^{2t}, so 21% growth per year is 10% growth per half-year

    abkt=a (bk)t\displaystyle ab^{kt} = a\,(b^k)^t
    abt/k=a (b1/k)t\displaystyle ab^{t/k} = a\,(b^{1/k})^t
    abt+c=(abc) bt\displaystyle ab^{t + c} = (ab^c)\,b^t

14.52 Graphs of Exponential Functions

xy−4−3−2−11234268up 3(0, 1)(0, 4)y = 3y = 2ˣ + 3y = 2ˣy = 2ˣ + 3Every point moves up 3.Asymptote:y = 0 → y = 3y-intercept:(0, 1) → (0, 4)The curve hugs y = 3 on theleft and never crosses it.
Adding 3 outside the exponential lifts the whole graph, including its asymptote. The y-intercept moves from (0, 1) to (0, 4).
  1. 14.52.1

    Graphing Exponential Growth Functions

    Passes through (0,a)(0, a), rises ever faster to the right, and flattens toward y=0y = 0 on the left without touching it.

    y=a bx, b>1\displaystyle y = a\,b^x,\ b > 1
  2. 14.52.2

    Graphing Exponential Decay Functions

    Passes through (0,a)(0, a) and falls toward y=0y = 0 on the right without reaching it.

    y=a bx, 0<b<1\displaystyle y = a\,b^x,\ 0 < b < 1
  3. 14.52.3

    Vertical Translations of Exponential Growth Functions

    For b>1b > 1, adding kk shifts the graph up kk units (down if k<0k < 0). The horizontal asymptote moves from y=0y = 0 to y=ky = k, and the range becomes y>ky > k.

    e.g. y=2x−3y = 2^x - 3: asymptote y=−3y = -3, yy-intercept 1−3=−21 - 3 = -2

    y=bx+k\displaystyle y = b^x + k
    asymptote: y=k\displaystyle \text{asymptote: } y = k
  4. 14.52.4

    Vertical Translations of Exponential Decay Functions

    For 0<b<10 < b < 1, adding kk shifts the graph up kk units (down if k<0k < 0). The graph falls toward the asymptote y=ky = k as xx increases.

    e.g. y=(12)x+4y = \left(\tfrac12\right)^x + 4: asymptote y=4y = 4, yy-intercept 55

    y=bx+k\displaystyle y = b^x + k
    asymptote: y=k\displaystyle \text{asymptote: } y = k
  5. 14.52.5

    Vertical Reflections of Exponential Functions

    A negative sign in front reflects the graph across the xx-axis. The asymptote stays y=0y = 0, but the graph lies below it, so the range is y<0y < 0. Note −2x-2^x means −(2x)-(2^x).

    e.g. y=−2xy = -2^x passes through (0,−1)(0, -1) and (1,−2)(1, -2)

    y=−bx\displaystyle y = -b^x
  6. 14.52.6

    Extrema of Exponential Functions

    f(x)=abx+kf(x) = ab^x + k always increases or always decreases. On a closed interval the max and min are at the endpoints. On all real numbers there is no max or min, since ff approaches y=ky = k but never reaches it.

    e.g. f(x)=3(2)xf(x) = 3(2)^x on [−1,2][-1, 2]: min f(−1)=1.5f(-1) = 1.5, max f(2)=12f(2) = 12

  7. 14.52.7

    Interpreting Graphs of Exponential Functions

    The yy-intercept is the starting value aa. The ratio of outputs one xx-unit apart is the factor bb: growth if b>1b > 1, decay if 0<b<10 < b < 1. The asymptote is the level the quantity approaches.

    e.g. Graph through (0,3)(0, 3) and (1,6)(1, 6): a=3a = 3, b=2b = 2, so y=3⋅2xy = 3 \cdot 2^x

    y=a⋅bx\displaystyle y = a \cdot b^x
  8. 14.52.8

    Determining Unknown Parameters in Exponential Functions

    For y=abxy = ab^x, the yy-intercept gives aa. Divide two outputs to find bb. If the graph is shifted to y=abx+ky = ab^x + k, read kk from the horizontal asymptote first.

    e.g. Through (0,5)(0, 5) and (2,45)(2, 45): a=5a = 5, b2=9b^2 = 9, so b=3b = 3

    a=f(0)\displaystyle a = f(0)
    bx2−x1=y2y1\displaystyle b^{x_2 - x_1} = \frac{y_2}{y_1}

Unit 15 31 topics

Advanced Algebra - Rational and Radical Equations

Rational Expressions, Rational Equations, and Radical Expressions.

15.53 Rational Expressions

  1. 15.53.1

    Equivalent Expressions With Fractions

    Multiply or divide top and bottom by the same nonzero expression.

    ab=akbk(k≠0)\displaystyle \frac{a}{b} = \frac{ak}{bk} \quad (k \ne 0)
  2. 15.53.2

    Simplifying Rational Expressions

    Cancel common factors, never terms. Values that made the original denominator zero stay excluded.

    6x29x=2x3, x≠0\displaystyle \frac{6x^2}{9x} = \frac{2x}{3},\ x \ne 0
    x+2x≠2\displaystyle \frac{x + 2}{x} \ne 2
  3. 15.53.3

    Simplifying Rational Expressions by Factoring

    Factor top and bottom completely, then cancel the shared factors.

    x2−9x2+3x=(x−3)(x+3)x(x+3)=x−3x\displaystyle \frac{x^2 - 9}{x^2 + 3x} = \frac{(x - 3)(x + 3)}{x(x + 3)} = \frac{x - 3}{x}
  4. 15.53.4

    Simplifying Rational Expressions Using Polynomial Factorization

    Factor the numerator and denominator fully, then cancel common factors, never single terms. Values that make the original denominator zero stay excluded.

    e.g. x2−9x2+x−6=(x−3)(x+3)(x+3)(x−2)=x−3x−2\tfrac{x^2 - 9}{x^2 + x - 6} = \tfrac{(x - 3)(x + 3)}{(x + 3)(x - 2)} = \tfrac{x - 3}{x - 2}, x≠−3,2x \ne -3, 2

    acbc=ab(b,c≠0)\displaystyle \frac{ac}{bc} = \frac{a}{b} \quad (b, c \ne 0)
  5. 15.53.5

    Splitting Rational Expressions Into Separate Terms

    A single denominator can be split under each term on top. The reverse fails: a sum in the denominator can’t be split.

    e.g. 6x2+3x3x=2x+1\tfrac{6x^2 + 3x}{3x} = 2x + 1 for x≠0x \ne 0

    a+bc=ac+bc\displaystyle \frac{a + b}{c} = \frac{a}{c} + \frac{b}{c}
    ca+b≠ca+cb\displaystyle \frac{c}{a + b} \ne \frac{c}{a} + \frac{c}{b}
  6. 15.53.6

    Adding and Subtracting Rational Expressions

    Factor the denominators, find the least common denominator, rewrite each fraction over it, and combine numerators. When subtracting, distribute the minus sign to the whole numerator.

    e.g. xx2−1−1x−1=x−(x+1)(x−1)(x+1)=−1x2−1\tfrac{x}{x^2 - 1} - \tfrac{1}{x - 1} = \tfrac{x - (x + 1)}{(x - 1)(x + 1)} = \tfrac{-1}{x^2 - 1}

    ac±bc=a±bc\displaystyle \frac{a}{c} \pm \frac{b}{c} = \frac{a \pm b}{c}
  7. 15.53.7

    Adding Rational Expressions With No Common Factors in the Denominator

    When the denominators share no factor, the common denominator is their product.

    e.g. 2x+3x+1=2(x+1)+3xx(x+1)=5x+2x(x+1)\tfrac{2}{x} + \tfrac{3}{x + 1} = \tfrac{2(x + 1) + 3x}{x(x + 1)} = \tfrac{5x + 2}{x(x + 1)}

    ab+cd=ad+bcbd\displaystyle \frac{a}{b} + \frac{c}{d} = \frac{ad + bc}{bd}
  8. 15.53.8

    Adding Rational Expressions Using Polynomial Factorization

    Factor every denominator. The LCD uses each factor the greatest number of times it appears. Rewrite each fraction over the LCD, add the numerators, then simplify.

    e.g. 1(x−1)(x+1)+x−1(x−1)(x+1)=xx2−1\tfrac{1}{(x-1)(x+1)} + \tfrac{x-1}{(x-1)(x+1)} = \tfrac{x}{x^2 - 1}

    pqr+sq=p+srqr\displaystyle \frac{p}{qr} + \frac{s}{q} = \frac{p + sr}{qr}
  9. 15.53.9

    Multiplying Rational Expressions

    Factor everything, cancel common factors between any numerator and any denominator, then multiply what remains.

    e.g. x2−43x⋅6x+2=2(x−2)x\tfrac{x^2 - 4}{3x} \cdot \tfrac{6}{x + 2} = \tfrac{2(x - 2)}{x}

    ab⋅cd=acbd\displaystyle \frac{a}{b} \cdot \frac{c}{d} = \frac{ac}{bd}
  10. 15.53.10

    Dividing Rational Expressions

    Multiply by the reciprocal of the divisor, then simplify. Also exclude values that make the divisor's numerator zero.

    e.g. x+3x÷x2−9x2=x+3x⋅x2(x−3)(x+3)=xx−3\tfrac{x + 3}{x} \div \tfrac{x^2 - 9}{x^2} = \tfrac{x + 3}{x} \cdot \tfrac{x^2}{(x - 3)(x + 3)} = \tfrac{x}{x - 3}

    ab÷cd=ab⋅dc\displaystyle \frac{a}{b} \div \frac{c}{d} = \frac{a}{b} \cdot \frac{d}{c}
  11. 15.53.11

    Fractions of Fractions With Algebraic Expressions

    Divide by multiplying by the reciprocal of the bottom. Or multiply the top and bottom by the LCD of all the small fractions. Keep the restrictions that make any denominator zero.

    e.g. 1+1x1−1x⋅xx=x+1x−1\dfrac{1 + \tfrac1x}{1 - \tfrac1x} \cdot \dfrac{x}{x} = \dfrac{x + 1}{x - 1}, x≠0,1x \ne 0, 1

    a/bc/d=ab⋅dc=adbc\displaystyle \frac{a/b}{c/d} = \frac{a}{b}\cdot\frac{d}{c} = \frac{ad}{bc}

15.54 Rational Equations

abcd=⟹ad = bcThen check that no denominator is zero.
Cross-multiplying is multiplying both sides by both denominators at once. It only works when each side is a single fraction.
  1. 15.54.1

    Solving Rational Equations Containing One Fractional Term

    Isolate the fraction, then multiply both sides by its denominator. Exclude values that make it zero.

    e.g. 6x+1=4⇒6x=3⇒x=2\tfrac6x + 1 = 4 \Rightarrow \tfrac6x = 3 \Rightarrow x = 2

  2. 15.54.2

    Solving Rational Equations Using Cross-Multiplication

    When one fraction equals another, multiply diagonally.

    ab=cd  ⇒  ad=bc\displaystyle \frac{a}{b} = \frac{c}{d} \;\Rightarrow\; ad = bc
  3. 15.54.3

    Solving Rational Equations Containing Binomials Using Cross-Multiplication

    Cross-multiply, distribute both sides, solve. Check that no denominator becomes zero.

    e.g. x=8x = 8

    x+13=x−22\displaystyle \frac{x + 1}{3} = \frac{x - 2}{2}
    ⇒  2x+2=3x−6\displaystyle \Rightarrow\; 2x + 2 = 3x - 6
  4. 15.54.4

    Solving Rational Equations Using the Flip Method

    If two fractions are equal, their reciprocals are too. Handy when the variable is in a denominator.

    e.g. 3x−1=14⇒x−13=4⇒x=13\tfrac{3}{x - 1} = \tfrac14 \Rightarrow \tfrac{x - 1}{3} = 4 \Rightarrow x = 13

    ab=cd  ⇒  ba=dc\displaystyle \frac{a}{b} = \frac{c}{d} \;\Rightarrow\; \frac{b}{a} = \frac{d}{c}
  5. 15.54.5

    Rational Equations With Three Terms

    Multiply every term by the LCD to clear the fractions, then solve. Reject any answer that makes a denominator zero.

    e.g. 3x−12=1x\frac{3}{x} - \frac{1}{2} = \frac{1}{x}: multiply by 2x2x: 6−x=26 - x = 2, so x=4x = 4

  6. 15.54.6

    Advanced Rational Equations

    Factor every denominator first to find the LCD and the excluded values. Multiply through, solve the resulting equation (often a quadratic), and discard extraneous roots.

    e.g. xx−2−1x+2=8x2−4\frac{x}{x - 2} - \frac{1}{x + 2} = \frac{8}{x^2 - 4} gives x2+x−6=0x^2 + x - 6 = 0, so x=−3x = -3 (x=2x = 2 is extraneous)

  7. 15.54.7

    Solving Many-Variable Rational Equations

    Treat the other letters as numbers. Multiply both sides by the LCD, move every term with the target variable to one side, factor it out, then divide.

    e.g. Solve y=xx+ky = \tfrac{x}{x + k} for xx: yx+yk=x⇒yk=x(1−y)⇒x=yk1−yyx + yk = x \Rightarrow yk = x(1 - y) \Rightarrow x = \tfrac{yk}{1 - y}

    1a+1b=1c\displaystyle \frac1a + \frac1b = \frac1c
    ⇒  c=aba+b\displaystyle \Rightarrow\; c = \frac{ab}{a + b}
  8. 15.54.8

    Graphing Reciprocal Functions

    y=kxy = \frac{k}{x} is a hyperbola with asymptotes x=0x = 0 and y=0y = 0. If k>0k > 0 the branches are in quadrants I and III; if k<0k < 0 they are in II and IV.

    e.g. y=4xy = \frac{4}{x} passes through (1,4)(1, 4), (2,2)(2, 2), and (−2,−2)(-2, -2)

    y=kx\displaystyle y = \frac{k}{x}
  9. 15.54.9

    Graph Transformations of Reciprocal Functions

    hh shifts the graph right, kk shifts it up, ∣a∣\lvert a \rvert stretches it, and a negative aa reflects it. The asymptotes move with the shifts.

    e.g. y=1x+3y = \frac{1}{x + 3} is 1x\frac{1}{x} shifted 3 left, with vertical asymptote x=−3x = -3

    y=ax−h+k\displaystyle y = \frac{a}{x - h} + k
    asymptotes: x=h,  y=k\displaystyle \text{asymptotes: } x = h,\; y = k

15.55 Radical Expressions

  1. 15.55.1

    The Square Root of a Perfect Square With Algebraic Expressions

    Halve each exponent.

    a2n=an\displaystyle \sqrt{a^{2n}} = a^n
    x2y4=xy2(x≥0)\displaystyle \sqrt{x^2y^4} = xy^2 \quad (x \ge 0)
  2. 15.55.2

    The Square Root of a Perfect Square With Domain Restrictions

    With no sign given, x2\sqrt{x^2} is the distance ∣x∣\lvert x \rvert, because a square root is never negative.

    e.g. (−5)2=5\sqrt{(-5)^2} = 5, not −5-5

    x2=∣x∣\displaystyle \sqrt{x^2} = \lvert x \rvert
    x6=∣x3∣\displaystyle \sqrt{x^6} = \lvert x^3 \rvert
  3. 15.55.3

    The Cube Root of a Perfect Cube With Algebraic Expressions

    Divide each exponent by 3. No absolute value: a cube root keeps the sign.

    x33=x\displaystyle \sqrt[3]{x^3} = x
    −8a63=−2a2\displaystyle \sqrt[3]{-8a^6} = -2a^2
  4. 15.55.4

    Simplifying Square Root Expressions Using the Product Rule

    Split off the largest perfect square, including even powers of the variables.

    ab=a b\displaystyle \sqrt{ab} = \sqrt{a}\,\sqrt{b}
    50x3=25x2⋅2x=5x2x\displaystyle \sqrt{50x^3} = \sqrt{25x^2 \cdot 2x} = 5x\sqrt{2x}
  5. 15.55.5

    Combining Radical Expressions Using the Product Rule

    Multiply the outside numbers together and the insides together, then simplify.

    e.g. 23⋅56=1018=3022\sqrt3 \cdot 5\sqrt6 = 10\sqrt{18} = 30\sqrt2

    ab⋅cd=acbd\displaystyle a\sqrt{b} \cdot c\sqrt{d} = ac\sqrt{bd}
  6. 15.55.6

    Simplifying Square Root Expressions Using the Quotient Rule

    Split the root over top and bottom, or simplify the fraction inside first.

    e.g. 18x32x=9x2=3x\sqrt{\tfrac{18x^3}{2x}} = \sqrt{9x^2} = 3x for x>0x > 0

    ab=ab\displaystyle \sqrt{\frac{a}{b}} = \frac{\sqrt{a}}{\sqrt{b}}
  7. 15.55.7

    Evaluating Algebraic Radical Expressions

    Substitute, simplify everything under the root, then take the root.

    e.g. b2−4ac\sqrt{b^2 - 4ac} at a=1,b=5,c=6a = 1, b = 5, c = 6 → 1=1\sqrt{1} = 1

  8. 15.55.8

    Adding and Subtracting Radical Expressions

    Only like radicals combine: same index, same radicand. Simplify each one first.

    3x+5x=8x\displaystyle 3\sqrt{x} + 5\sqrt{x} = 8\sqrt{x}
    12+27=23+33=53\displaystyle \sqrt{12} + \sqrt{27} = 2\sqrt3 + 3\sqrt3 = 5\sqrt3
  9. 15.55.9

    Solving Radical Equations

    Isolate the radical, raise both sides to its power, solve, then check every answer. Squaring can create false solutions.

    e.g. Gives x=1x = 1 or 66; only 66 checks

    x+3=x−3\displaystyle \sqrt{x + 3} = x - 3
    ⇒  x+3=x2−6x+9\displaystyle \Rightarrow\; x + 3 = x^2 - 6x + 9
  10. 15.55.10

    Solving Advanced Radical Equations

    Isolate one radical and square both sides. If a radical remains, isolate it and square again. Check every answer in the original equation, since squaring can create extraneous solutions.

    e.g. x+5=1+x⇒x+5=1+2x+x⇒x=2⇒x=4\sqrt{x + 5} = 1 + \sqrt{x} \Rightarrow x + 5 = 1 + 2\sqrt{x} + x \Rightarrow \sqrt{x} = 2 \Rightarrow x = 4

    A=B  ⇒  A=B2\displaystyle \sqrt{A} = B \;\Rightarrow\; A = B^2
    valid only if B≥0\displaystyle \text{valid only if } B \ge 0
  11. 15.55.11

    Solving Many-Variable Nonlinear Equations

    Undo operations in reverse order to isolate the target variable. Square both sides to remove a square root. Take a square root to undo a square, using ±\pm unless the quantity must be positive.

    e.g. T=2πL/gT = 2\pi\sqrt{L/g}: T2π=L/g⇒L=gT24π2\tfrac{T}{2\pi} = \sqrt{L/g} \Rightarrow L = \tfrac{gT^2}{4\pi^2}

    A=B⇒A=B2\displaystyle \sqrt{A} = B \Rightarrow A = B^2
    A2=B⇒A=±B\displaystyle A^2 = B \Rightarrow A = \pm\sqrt{B}

Unit 16 49 topics

Problem Solving - Ratios & Percentages

Ratios, Unit Rates, Proportional Relationships, and more.

16.56 Ratios

Cats444Dogs443 shares = 122 shares = 83 : 2 with a total of 20 → 5 shares → 1 share = 4
Tape diagram. A ratio is a count of equal shares; find one share and everything follows.
  1. 16.56.1

    Introduction to Ratios

    A ratio compares two quantities in a set order, read “a to b.” Order matters: 3 : 2 is not 2 : 3.

    e.g. 3 cats and 2 dogs → cats to dogs is 3:23:2

    a:b\displaystyle a : b
  2. 16.56.2

    Equivalent Ratios

    Multiply or divide both parts by the same nonzero number and the comparison stays the same.

    e.g. 2:3=4:6=10:152:3 = 4:6 = 10:15

    a:b=ka:kb\displaystyle a : b = ka : kb
  3. 16.56.3

    Writing Ratios Using Fractions

    The ratio a:ba:b can be written ab\tfrac{a}{b}. If a:ba:b is part to part, the whole has a+ba+b parts.

    e.g. boys : girls =3:2= 3:2 → boys are 35\tfrac{3}{5} of the class

    aa+b=fraction of the whole that is a\displaystyle \frac{a}{a+b} = \text{fraction of the whole that is } a
  4. 16.56.4

    Reasoning With Equivalent Ratios

    Find the scale factor between the parts you know, then apply it to the missing part.

    e.g. 2:5=6: ?2:5 = 6:\,? → scale ×3 → 1515

    ab=cd\displaystyle \frac{a}{b} = \frac{c}{d}
  5. 16.56.5

    Further Reasoning With Equivalent Ratios

    Given a total, split it into a+ba+b equal shares and hand out aa shares and bb shares.

    e.g. Split 40 in the ratio 3:53:5 → share =5=5 → 1515 and 2525

    one share=totala+b\displaystyle \text{one share} = \frac{\text{total}}{a+b}
  6. 16.56.6

    Ratio Tables

    Each column is an equivalent ratio. Move between columns by multiplying, or add two columns together.

    e.g. 2 : 3 → 4 : 6 → 6 : 9 → 8 : 12

  7. 16.56.7

    Graphing Ratios

    Plot equivalent ratios as points; they fall on a straight line through the origin.

    e.g. (2,3),(4,6),(6,9)(2,3),(4,6),(6,9) all lie on y=1.5xy=1.5x

    y=ba x\displaystyle y = \tfrac{b}{a}\,x

16.57 Unit Rates

  1. 16.57.1

    Unit Rates

    A rate compares different units. A unit rate is the amount “per 1.” Divide by the second quantity.

    e.g. $6 for 3 lb → $2 per lb

    unit rate=amountnumber of units\displaystyle \text{unit rate} = \frac{\text{amount}}{\text{number of units}}
  2. 16.57.2

    Solving Problems Using Unit Rates

    Find the unit rate, then multiply. For best buy, the lower price per unit wins.

    e.g. $2/lb × 7 lb = $14

    total=unit rate×units\displaystyle \text{total} = \text{unit rate} \times \text{units}
  3. 16.57.3

    Speed as a Unit Rate

    Speed is distance per unit of time. Cover the one you want to find.

    e.g. 150 miles in 3 hours → 50 mph

    s=dt\displaystyle s = \frac{d}{t}
    d=s t\displaystyle d = s\,t
    t=ds\displaystyle t = \frac{d}{s}
  4. 16.57.4

    Unit Rates Associated With Ratios of Fractions

    Divide the fractions: multiply by the reciprocal of the bottom one.

    e.g. 12\tfrac12 mile in 14\tfrac14 hour → 12⋅41=2\tfrac12 \cdot \tfrac41 = 2 mph

    a/bc/d=ab⋅dc\displaystyle \frac{a/b}{c/d} = \frac{a}{b} \cdot \frac{d}{c}
  5. 16.57.5

    Solving Unit Rate Problems Using Ratios of Fractions

    Same move: get the rate “per 1 whole unit,” then scale up or down.

    e.g. 23\tfrac23 cup per 12\tfrac12 batch → 43\tfrac43 cups per batch

  6. 16.57.6

    Manipulating Ratios in Various Contexts

    Multiply or divide both terms of a ratio by the same number to scale it. In a:ba:b, part aa is aa+b\frac{a}{a+b} of the total. To chain two ratios, rescale them so the shared term matches.

    e.g. a:b=2:3a:b = 2:3 and b:c=4:5⇒a:b:c=8:12:15b:c = 4:5 \Rightarrow a:b:c = 8:12:15

    part a=aa+b×total\displaystyle \text{part } a = \frac{a}{a + b}\times\text{total}

16.58 Proportional Relationships

y = 0.5x + 2(0, 0)y = 0.6x
Solid: proportional, a straight line through the origin. Dashed: a starting amount lifts the line off the origin, so it is not proportional.
  1. 16.58.1

    Understanding Proportional Relationships Using Tables

    Proportional when yx\tfrac{y}{x} is the same constant kk in every row.

    e.g. xx: 2, 4, 5 / yy: 6, 12, 15 → k=3k = 3 every time

    k=yx\displaystyle k = \frac{y}{x}
  2. 16.58.2

    Understanding Proportional Relationships Using Graphs

    A straight line through the origin (0,0)(0,0). The point (1,k)(1, k) shows the constant.

    y=kx\displaystyle y = kx
  3. 16.58.3

    Understanding Proportional Relationships From Descriptions

    Look for a constant rate (“per,” “each”) with no starting amount. A fixed fee breaks proportionality.

    e.g. $4 per ticket: yes. $4 per ticket + $5 fee: no.

    y=kx  (proportional)\displaystyle y = kx \;\text{(proportional)}
    y=kx+b, b≠0  (not proportional)\displaystyle y = kx + b,\ b \neq 0 \;\text{(not proportional)}
  4. 16.58.4

    Modeling with Direct Variation

    yy varies directly with xx when y=kxy = kx. Find kk from one pair of values, then use it.

    e.g. y=12y = 12 when x=3x = 3 → k=4k = 4 → at x=5x = 5, y=20y = 20

    y=kx,k=yx\displaystyle y = kx,\quad k = \frac{y}{x}

16.59 Percentages

0%025%2050%4075%60100%80percentamount
Percent bar. The whole is always 100%. Line the percents up with the amounts: 25% of 80 is 20.
  1. 16.59.1

    Understanding Percentages Using Models

    Percent means “per hundred.” A 10 × 10 grid or a bar split into 100 shows it.

    p%=p100\displaystyle p\% = \frac{p}{100}
  2. 16.59.2

    Converting Between Percentages and Fractions

    Percent to fraction: put it over 100 and simplify. Fraction to percent: multiply by 100%.

    35%=35100=720\displaystyle 35\% = \frac{35}{100} = \frac{7}{20}
    38×100%=37.5%\displaystyle \frac{3}{8} \times 100\% = 37.5\%
  3. 16.59.3

    Converting Between Percentages and Decimals

    Move the decimal point two places: left to go from percent to decimal, right to go back.

    45%=0.45\displaystyle 45\% = 0.45
    0.075=7.5%\displaystyle 0.075 = 7.5\%
  4. 16.59.4

    Comparing Fractions, Percents, and Decimals

    Convert everything to one form (decimals are easiest), then compare.

    e.g. 25=0.4\tfrac{2}{5} = 0.4, 38%=0.3838\% = 0.38 → 25\tfrac25 is larger

  5. 16.59.5

    Finding Part of a Number Given a Whole and a Percentage

    “Of” means multiply.

    e.g. 20% of 60 =0.2×60=12= 0.2 \times 60 = 12

    part=p100×whole\displaystyle \text{part} = \frac{p}{100} \times \text{whole}
  6. 16.59.6

    Finding Part of a Number Given a Whole and a Percentage: Word Problems

    Change the percent to a decimal and multiply by the whole.

    e.g. 35% of 240 students walk: 0.35×240=840.35 \times 240 = 84 students

    part=percent100×whole\displaystyle \text{part} = \frac{\text{percent}}{100}\times\text{whole}
  7. 16.59.7

    Finding a Percentage Given Two Numbers

    Divide the part by the whole, then convert to a percent.

    e.g. 12 out of 48 → 0.250.25 → 25%

    percent=partwhole×100%\displaystyle \text{percent} = \frac{\text{part}}{\text{whole}} \times 100\%
  8. 16.59.8

    Finding a Percentage Given Two Numbers: Word Problems

    The whole is the total, the original, or what follows “out of.”

    e.g. 18 correct out of 24 → 75%

  9. 16.59.9

    Finding a Total Given a Part and a Percentage

    Divide the part by the percent as a decimal.

    e.g. 30 is 40% of ? → 30÷0.4=7530 \div 0.4 = 75

    whole=partp/100\displaystyle \text{whole} = \frac{\text{part}}{p/100}
  10. 16.59.10

    Applying Percentage Increases

    Multiply by one plus the percent.

    e.g. $80 up 25% → 80×1.25=10080 \times 1.25 = 100

    new=old×(1+p100)\displaystyle \text{new} = \text{old} \times \left(1 + \frac{p}{100}\right)
  11. 16.59.11

    Applying Percentage Decreases

    Multiply by one minus the percent.

    e.g. $80 down 25% → 80×0.75=6080 \times 0.75 = 60

    new=old×(1−p100)\displaystyle \text{new} = \text{old} \times \left(1 - \frac{p}{100}\right)
  12. 16.59.12

    Calculating Percentage Change

    Change divided by the original. Always divide by the old value.

    e.g. 50 → 65: 1550=30%\tfrac{15}{50} = 30\% increase

    % change=new−oldold×100%\displaystyle \%\text{ change} = \frac{\text{new} - \text{old}}{\text{old}} \times 100\%
  13. 16.59.13

    Finding Original Values From Percentage Increases

    Divide the new value by the multiplier.

    e.g. 60 after a 20% rise → 60÷1.2=5060 \div 1.2 = 50

    old=new1+p/100\displaystyle \text{old} = \frac{\text{new}}{1 + p/100}
  14. 16.59.14

    Finding Original Values From Percentage Decreases

    Divide the new value by the multiplier.

    e.g. 45 after a 25% drop → 45÷0.75=6045 \div 0.75 = 60

    old=new1−p/100\displaystyle \text{old} = \frac{\text{new}}{1 - p/100}
  15. 16.59.15

    Applying Percentages in Succession

    Multiply the multipliers one after another. Never just add the percents.

    e.g. +10% then −10% → 1.1×0.9=0.991.1 \times 0.9 = 0.99 → 1% less than you started

    new=original×m1×m2\displaystyle \text{new} = \text{original} \times m_1 \times m_2
  16. 16.59.16

    Percentages in Commerce and Finance

    Write the percent as a decimal rr. An increase (markup, tax, tip) multiplies by 1+r1 + r. A decrease (discount) multiplies by 1−r1 - r. Simple interest is rr of the principal each year.

    e.g. $80 jacket, 25% off, then 6% tax: 80(0.75)(1.06)=$63.6080(0.75)(1.06) = \$63.60

    increase: P(1+r)\displaystyle \text{increase: } P(1 + r)
    decrease: P(1−r)\displaystyle \text{decrease: } P(1 - r)
    I=Prt\displaystyle I = Prt
  17. 16.59.17

    Further Percentages in Commerce and Finance

    To find the original amount, divide the final amount by the multiplier. Percent profit or loss is measured against the cost, not the selling price.

    e.g. After a 20% discount the price is $48: original =48÷0.8=$60= 48 \div 0.8 = \$60

    original=final1±r\displaystyle \text{original} = \frac{\text{final}}{1 \pm r}
    profit rate=sell−costcost\displaystyle \text{profit rate} = \frac{\text{sell} - \text{cost}}{\text{cost}}
  18. 16.59.18

    Solving Multipart Commerce and Finance Percentage Problems

    Apply each change as its own multiplier, in order. Successive percent changes multiply. They do not add.

    e.g. Up 20% then down 20%: 1.2×0.8=0.961.2 \times 0.8 = 0.96, a 4% net decrease

    P(1+r1)(1+r2)⋯\displaystyle P(1 + r_1)(1 + r_2)\cdots

16.60 Units

60 mi1 h×5,280 ft1 mi×1 h3,600 s=88 ft1 sArrange each fraction so the unit you want gone is on top once and on the bottom once.
A conversion factor equals 1, so multiplying by it changes the units without changing the amount. The struck-through units cancel.
  1. 16.60.1

    Unit Conversions Using Base Units of Mass

    Metric prefixes are powers of ten: kilo is 1,000, centi is 1100\tfrac{1}{100}, milli is 11000\tfrac{1}{1000}. US: 16 oz = 1 lb, 2,000 lb = 1 ton.

    e.g. 3.4 kg=3400 g3.4\text{ kg} = 3400\text{ g}

    1 kg=1000 g\displaystyle 1\text{ kg} = 1000\text{ g}
    1 g=1000 mg\displaystyle 1\text{ g} = 1000\text{ mg}
  2. 16.60.2

    Two-Step Unit Conversions

    Multiply by conversion fractions arranged so the unwanted units cancel.

    60 mi1 h⋅5280 ft1 mi⋅1 h3600 s=88 fts\displaystyle \frac{60\text{ mi}}{1\text{ h}} \cdot \frac{5280\text{ ft}}{1\text{ mi}} \cdot \frac{1\text{ h}}{3600\text{ s}} = 88\ \frac{\text{ft}}{\text{s}}
  3. 16.60.3

    Unit Conversions Using Base Units of Length

    1 km = 1,000 m and 1 m = 100 cm = 1,000 mm. US: 12 in = 1 ft, 3 ft = 1 yd, 5,280 ft = 1 mi.

    e.g. 2.5 km=2500 m2.5\text{ km} = 2500\text{ m}

  4. 16.60.4

    Unit Conversions Using Units of Time

    60 s = 1 min, 60 min = 1 h, 24 h = 1 day, 7 days = 1 week.

    1 h=3600 s\displaystyle 1\text{ h} = 3600\text{ s}
  5. 16.60.5

    Converting Units of Area to Smaller Units

    Square the length factor. Going to a smaller unit, multiply.

    1 m2=1002 cm2=10,000 cm2\displaystyle 1\text{ m}^2 = 100^2\text{ cm}^2 = 10{,}000\text{ cm}^2
  6. 16.60.6

    Converting Units of Area to Larger Units

    Square the length factor and divide.

    5000 cm2=500010,000 m2=0.5 m2\displaystyle 5000\text{ cm}^2 = \frac{5000}{10{,}000}\text{ m}^2 = 0.5\text{ m}^2
  7. 16.60.7

    Determining Units in Formulas

    Units follow the same algebra as the numbers: they multiply and divide.

    m×m=m2\displaystyle \text{m} \times \text{m} = \text{m}^2
    ms÷s=ms2\displaystyle \frac{\text{m}}{\text{s}} \div \text{s} = \frac{\text{m}}{\text{s}^2}
  8. 16.60.8

    Selecting Units for Rates of Change

    A rate’s unit is the yy-unit per xx-unit. Choose a scale that gives sensible numbers.

    e.g. Fingernail growth in mm per week, not km per year

    rate unit=y-unitx-unit\displaystyle \text{rate unit} = \frac{y\text{-unit}}{x\text{-unit}}
  9. 16.60.9

    Converting Between Mixed Units

    Convert everything to the smallest unit, compute, then convert back.

    e.g. 2 h 45 min =165= 165 min; 200 min == 3 h 20 min

  10. 16.60.10

    Converting Between Mixed Units Containing Squares

    A squared unit needs the conversion factor squared. Convert each unit in a compound rate separately.

    e.g. 5 m/s2=5×602=18,000 m/min25\text{ m/s}^2 = 5 \times 60^2 = 18{,}000\text{ m/min}^2

    1 ft=12 in\displaystyle 1\text{ ft} = 12\text{ in}
    ⇒  1 ft2=144 in2\displaystyle \Rightarrow\; 1\text{ ft}^2 = 144\text{ in}^2
  11. 16.60.11

    Degrees of Accuracy

    A measurement rounded to some unit can be off by up to half that unit either way.

    7 cm (to the nearest cm)\displaystyle 7\text{ cm (to the nearest cm)}
    ⇒  6.5≤x<7.5\displaystyle \Rightarrow\; 6.5 \le x < 7.5
  12. 16.60.12

    Density

    Density is mass per unit volume. Population density is people per unit area. Rearrange to find mass or volume.

    e.g. A 200 g block with volume 25 cm³: ρ=20025=8\rho = \tfrac{200}{25} = 8 g/cm³

    ρ=mV\displaystyle \rho = \frac{m}{V}
    m=ρV\displaystyle m = \rho V
  13. 16.60.13

    Interpreting Descriptions of Physical Phenomena

    Turn the words into a model. Find the starting value and the rate, and check that the units match. A loss or decrease is a negative rate.

    e.g. A 500 gal pool drains 20 gal/min: V=500−20tV = 500 - 20t, empty at t=25t = 25 min

    amount=start+rate⋅t\displaystyle \text{amount} = \text{start} + \text{rate}\cdot t
  14. 16.60.14

    Interpreting Rates of Change of Physical Phenomena

    A rate of change is the slope, in output units per input unit. A positive rate means the quantity grows. A negative rate means it shrinks.

    e.g. d=300−60td = 300 - 60t (miles, hours): starts 300 miles away and gets 60 miles closer each hour

    rate=ΔyΔx\displaystyle \text{rate} = \frac{\Delta y}{\Delta x}

Unit 17 71 topics

Data Analysis - Statistics & Probability

Sampling, Summarizing Data, Frequency Tables, and more.

17.61 Sampling

  1. 17.61.1

    Sampling

    A sample is part of a population used to learn about the whole. A random sample (simple random, systematic, stratified, or cluster) avoids bias; convenience and voluntary samples often do not represent the population.

    e.g. Survey a random 100 of 1,200 students; 35 ride the bus, so estimate 0.35×1200=4200.35 \times 1200 = 420 riders

  2. 17.61.2

    Estimation From Samples

    If a sample is random, its proportion estimates the population proportion. Multiply that proportion by the population size.

    e.g. 12 of 80 sampled bulbs are bad. Of 5000 bulbs: 1280(5000)=750\tfrac{12}{80}(5000) = 750

    estimate=countsample size×N\displaystyle \text{estimate} = \frac{\text{count}}{\text{sample size}}\times N
  3. 17.61.3

    Biased and Unbiased Samples

    A sample is unbiased when every member of the population has an equal chance of being chosen, as in a random sample. It is biased when some groups are favored, as in convenience samples, volunteer responses, or sampling only one subgroup.

    e.g. Asking gym members how often town residents exercise is biased

  4. 17.61.4

    Interpreting Survey Results

    Results apply only to the population that was randomly sampled. A survey shows association, not cause. Cause needs an experiment with random assignment.

    e.g. A random sample of students at one school supports conclusions about that school only

  5. 17.61.5

    Sampling and Margin of Error

    The true population value is likely within estimate ±\pm margin of error. A larger random sample gives a smaller margin. The margin does not fix bias.

    e.g. 54%±3%54\% \pm 3\%: the true value is likely from 51% to 57%

    estimate±margin\displaystyle \text{estimate} \pm \text{margin}

17.62 Summarizing Data

2468102597410102030405060minutescountmedian ≈ 27.8mean ≈ 28.2 (balance point)skewed right:mean > medianThe long tail on the rightpulls the mean toward it.Median: splits the area in halfMean: where the bars balance
In a right-skewed histogram the few large values in the tail drag the mean to the right of the median. Here the mean is estimated from bin midpoints; the median is less affected by the tail.
  1. 17.62.1

    Introduction to Statistics

    Statistics is collecting, summarizing, and interpreting data. A statistical question expects answers that vary.

    e.g. “How tall are 8th graders?” is statistical; “How tall is Sam?” is not

  2. 17.62.2

    The Mean of a Data Set

    Add all the values and divide by how many there are. Write μ\mu for a population mean and xˉ\bar x for a sample mean.

    e.g. 3,5,7,93, 5, 7, 9: xˉ=244=6\bar x = \tfrac{24}{4} = 6

    xˉ=∑xin\displaystyle \bar x = \frac{\sum x_i}{n}
  3. 17.62.3

    The Median of a Data Set

    Sort, then take the middle value. With an even count, average the middle two.

    e.g. {1,3,4,8}\{1, 3, 4, 8\} → 3+42=3.5\tfrac{3+4}{2} = 3.5

  4. 17.62.4

    The Mode of a Data Set

    The value that shows up most. There can be several, or none.

    e.g. {2,3,3,7}\{2, 3, 3, 7\} → mode 3

  5. 17.62.5

    Range, Quartiles, and IQR

    Range is max − min. Q1 is the median of the lower half, Q3 of the upper half. IQR is the middle 50%.

    Range=max⁡−min⁡\displaystyle \text{Range} = \max - \min
    IQR=Q3−Q1\displaystyle \text{IQR} = Q_3 - Q_1
  6. 17.62.6

    Mean Absolute Deviation

    The average distance of each value from the mean.

    e.g. {2,4,9}\{2, 4, 9\}, mean 5 → 3+1+43=83\tfrac{3+1+4}{3} = \tfrac83

    MAD=∑∣x−xˉ∣n\displaystyle \text{MAD} = \frac{\sum \lvert x - \bar{x} \rvert}{n}
  7. 17.62.7

    Outliers

    A value far from the rest. The usual test is the 1.5 × IQR fence.

    below Q1−1.5⋅IQR\displaystyle \text{below } Q_1 - 1.5 \cdot \text{IQR}
    above Q3+1.5⋅IQR\displaystyle \text{above } Q_3 + 1.5 \cdot \text{IQR}
  8. 17.62.8

    Removing Outliers

    Dropping an outlier moves the mean, range, and SD a lot; the median and IQR barely move.

  9. 17.62.9

    Combining Means

    Turn each mean back into a total, add the totals, and divide by the total count. Do not just average the two means unless the groups are the same size.

    e.g. 10 students average 80, 15 average 90: 800+135025=86\tfrac{800 + 1350}{25} = 86

    xˉ=n1xˉ1+n2xˉ2n1+n2\displaystyle \bar{x} = \frac{n_1\bar{x}_1 + n_2\bar{x}_2}{n_1 + n_2}
  10. 17.62.10

    Determining Unknown Observations Given Statistical Metrics

    The sum of the data is the mean times the count. Subtract the known values to find the missing one.

    e.g. Scores 82, 90, 75, 88, and xx have mean 85: x=425−335=90x = 425 - 335 = 90

    sum=nxˉ\displaystyle \text{sum} = n\bar{x}
    x=nxˉ−(sum of others)\displaystyle x = n\bar{x} - \text{(sum of others)}

17.63 Frequency Tables

  1. 17.63.1

    Frequency Tables

    Each value (or interval) with a count of how often it occurs. The counts add up to nn.

  2. 17.63.2

    Joint Frequency Tables

    A two-way table counts items by two categories at once. Each cell is a joint frequency. Row and column totals are marginal frequencies.

    e.g. 12 of 50 students are 9th graders who play a sport: 1250=0.24\tfrac{12}{50} = 0.24

    joint rel. freq.=cellgrand total\displaystyle \text{joint rel. freq.} = \frac{\text{cell}}{\text{grand total}}
  3. 17.63.3

    Cumulative Frequency

    A running total of the frequencies up to and including each value or class. The last cumulative frequency equals the total count.

    e.g. Frequencies 3, 5, 4, 8 give cumulative frequencies 3, 8, 12, 20

  4. 17.63.4

    Calculating Means From Frequency Tables

    Multiply each value by its frequency, add the products, and divide by the total frequency.

    e.g. Values 1, 2, 3 with frequencies 2, 5, 3: 2+10+910=2.1\tfrac{2 + 10 + 9}{10} = 2.1

    xˉ=∑fx∑f\displaystyle \bar{x} = \frac{\sum f x}{\sum f}
  5. 17.63.5

    Calculating Medians From Frequency Tables

    Find the middle position, then use cumulative frequencies to see which value holds it. With an even count, average the two middle values.

    e.g. Values 1, 2, 3 with frequencies 2, 5, 3: 5th and 6th values are both 2, so median =2= 2

    position=n+12\displaystyle \text{position} = \frac{n + 1}{2}
  6. 17.63.6

    Calculating Modes From Frequency Tables

    The mode is the value with the highest frequency, not the frequency itself. A tie gives more than one mode.

    e.g. Values 1, 2, 3 with frequencies 2, 5, 3: mode =2= 2

17.64 Representing Data

02468101214161820minQ₁medianQ₃maxIQR = Q₃ − Q₁ = 7 (middle 50%)range = max − min = 16
Box plot. Each of the four pieces (whisker, half-box, half-box, whisker) holds about a quarter of the data.
  1. 17.64.1

    Dot Plots

    One dot per data point, stacked above a number line.

  2. 17.64.2

    Box Plots

    Draw the five-number summary. The box spans Q1 to Q3 with a line at the median; whiskers reach min and max.

    min⁡, Q1, median, Q3, max⁡\displaystyle \min,\ Q_1,\ \text{median},\ Q_3,\ \max
  3. 17.64.3

    Histograms

    Bars over equal-width intervals (bins). Height is the count. Bars touch because the intervals are continuous.

  4. 17.64.4

    Measuring Centrality From Dot Plots

    Count the dots to get nn. The tallest stack is the mode; count in from either end to find the median.

  5. 17.64.5

    Measuring Range and MAD From Dot Plots

    Range is the distance between the outermost dots. For MAD, find each dot’s distance from the mean.

  6. 17.64.6

    Measuring Quartiles and IQR From Dot Plots

    Find the median dot, then the middle of each half.

  7. 17.64.7

    Calculating Modes and Medians From Histograms

    The modal class is the tallest bar. Add bar heights from the left to find the bar that holds the middle position. That bar is the median class.

    e.g. Heights 4, 7, 5, 2 for 0 to 10, 10 to 20, 20 to 30, 30 to 40: n=18n = 18, median class and modal class are 10 to 20

    position=n+12\displaystyle \text{position} = \frac{n + 1}{2}
  8. 17.64.8

    Calculating Means From Histograms

    Multiply each bar's value (or midpoint, for a range) by its height, add, and divide by the total height. With ranges the result is an estimate.

    e.g. Heights 2, 5, 3 for 0 to 10, 10 to 20, 20 to 30: 2(5)+5(15)+3(25)10=16\tfrac{2(5) + 5(15) + 3(25)}{10} = 16

    xˉ≈∑f⋅midpoint∑f\displaystyle \bar{x} \approx \frac{\sum f \cdot \text{midpoint}}{\sum f}
  9. 17.64.9

    Symmetry, Skew, and Outliers

    Symmetric: mean ≈ median. Skewed right (long tail right): mean > median. Skewed left: mean < median.

17.65 Comparing Data

Class Amedian 70IQR = 82 − 60 = 22Class Bmedian 79IQR = 84 − 74 = 10405060708090100scoreCompare medians for center, IQRs for spread.Class B scored higher (median 79 vs 70) and more consistently (IQR 10 vs 22).
Two box plots on one scale make comparison quick: the median line shows the center, and the width of the box (the IQR) shows how spread out the middle half is.
  1. 17.65.1

    Comparing Means

    Find each mean and compare. Outliers pull the mean toward them. With equal counts, comparing the totals is enough.

    e.g. {2,4,6}\{2, 4, 6\} mean 4, {3,5,10}\{3, 5, 10\} mean 6: the second is greater by 2

  2. 17.65.2

    Comparing Medians

    Sort each set and find its middle value. The median barely moves when an outlier is present.

    e.g. {1,3,8}\{1, 3, 8\} median 3, {2,4,5,100}\{2, 4, 5, 100\} median 4.5

  3. 17.65.3

    Comparing Modes

    Find the most frequent value in each set and compare. A set can have several modes or none.

    e.g. {2,2,3,5}\{2, 2, 3, 5\} mode 2, {1,4,4,4}\{1, 4, 4, 4\} mode 4

  4. 17.65.4

    Comparing Data Sets Using Range and Quartiles

    A larger range or IQR means the data is more spread out. IQR ignores extremes; range doesn't.

  5. 17.65.5

    Comparing Data Set Visualizations Using Standard Deviation and MAD

    The plot whose values sit farther from the center has the larger SD and MAD.

  6. 17.65.6

    Comparing Data Sets Using Standard Deviation and MAD

    Both measure typical distance from the mean; bigger means more spread. SD squares the distances, so it reacts more to far-off values.

    σ=∑(x−xˉ)2n\displaystyle \sigma = \sqrt{\frac{\sum (x - \bar{x})^2}{n}}
  7. 17.65.7

    Comparing Measures of Center

    Symmetric with no outliers: use the mean. Skewed or with outliers: use the median.

  8. 17.65.8

    Comparing Measures of Spread

    Symmetric: use SD or MAD (they pair with the mean). Skewed: use IQR (it pairs with the median).

  9. 17.65.9

    Bounding Statistics for Grouped Data

    When data are grouped in intervals, the exact values are unknown. The smallest possible mean puts every value at its interval's low end, and the largest puts every value at the high end. The median lies in the median class.

    e.g. 3 values in 10 to 19 and 2 in 20 to 29: mean from 30+405=14\tfrac{30 + 40}{5} = 14 to 57+585=23\tfrac{57 + 58}{5} = 23

    ∑f⋅lown≤xˉ≤∑f⋅highn\displaystyle \frac{\sum f \cdot \text{low}}{n} \le \bar{x} \le \frac{\sum f \cdot \text{high}}{n}
  10. 17.65.10

    Effects of Data Change on the Mean

    A new value above the mean raises it, below lowers it, and equal leaves it unchanged. Changing one value by dd changes the mean by dn\frac{d}{n}.

    e.g. Mean of 4 values is 10. Add 20: 40+205=12\tfrac{40 + 20}{5} = 12

    new mean=sum+xnewn+1\displaystyle \text{new mean} = \frac{\text{sum} + x_{\text{new}}}{n + 1}
  11. 17.65.11

    Comparing Effects of Data Change on Measures of Centrality

    An outlier pulls the mean strongly. The median changes little or not at all, and the mode usually does not change. Raising the largest value never moves the median.

    e.g. {2,3,4,5,6}\{2, 3, 4, 5, 6\}: change 6 to 60. Mean goes 4 to 14.8, median stays 4

  12. 17.65.12

    Statistical Effects of Data Transformations

    Adding cc to every value adds cc to the mean, median, and mode but leaves the range and standard deviation unchanged. Multiplying every value by kk multiplies the mean, median, and mode by kk and the range and standard deviation by ∣k∣\lvert k \rvert.

    e.g. Mean 70, SD 8. Add 5: mean 75, SD 8. Double: mean 140, SD 16

    x+c:  xˉ+c, spread same\displaystyle x + c:\; \bar{x} + c,\ \text{spread same}
    kx:  kxˉ, SD×∣k∣\displaystyle kx:\; k\bar{x},\ \text{SD} \times \lvert k \rvert

17.66 Correlation

r ≈ 0.9strong positiver ≈ 0no linear patternr ≈ −0.8negative
r runs from −1 to 1. The sign gives the direction; the closer to ±1, the tighter the points hug the trend line.
  1. 17.66.1

    Scatter Plots

    Plot paired data (x,y)(x, y) as points to look for a relationship. The explanatory variable goes on the xx-axis.

  2. 17.66.2

    Trend Lines

    A straight line through the middle of the cloud, with about as many points above it as below.

    y^=mx+b\displaystyle \hat{y} = mx + b
  3. 17.66.3

    Making Predictions Using Trend Lines

    Substitute xx into the trend line. Predicting inside the data’s range (interpolation) is safer than beyond it (extrapolation).

  4. 17.66.4

    Comparing Data Points to Lines of Best Fit

    The residual is actual minus predicted. A point above the line has a positive residual, so the model underestimates it. A point below has a negative residual.

    e.g. Line y^=2x+1\hat{y} = 2x + 1, point (3,9)(3, 9): predicted 7, residual 2, point above the line

    residual=y−y^\displaystyle \text{residual} = y - \hat{y}
  5. 17.66.5

    Interpreting Trend Line Coefficients

    The slope is the predicted change in yy for each one-unit increase in xx. The intercept is the predicted yy at x=0x = 0, which may be meaningless.

    e.g. y^=2.5x+60\hat{y} = 2.5x + 60, hours studied vs. score: each hour adds about 2.5 points

  6. 17.66.6

    Linear Correlation

    rr measures how tightly points hug a line, from −1-1 to 11. The sign gives direction; near 0 means no linear pattern. Correlation does not show cause.

    −1≤r≤1\displaystyle -1 \le r \le 1
  7. 17.66.7

    Residuals and Residual Plots

    A residual is actual minus predicted. Positive means the point is above the line. A residual plot with random scatter around 0 means a linear model fits; a curve or other pattern means it does not.

    e.g. Line y^=2x+1\hat y = 2x + 1, point (3,8)(3, 8): y^=7\hat y = 7, residual =8−7=1= 8 - 7 = 1

    e=y−y^\displaystyle e = y - \hat y
  8. 17.66.8

    Quadratic Regression

    Fits a parabola to data that rise then fall, or fall then rise. Use a calculator or Desmos (type y1∼ax12+bx1+cy_1 \sim ax_1^2 + bx_1 + c). An R2R^2 close to 1 means a good fit.

    e.g. Points (0,1)(0, 1), (1,2)(1, 2), (2,5)(2, 5): c=1c = 1, a+b=1a + b = 1, 4a+2b=44a + 2b = 4, so a=1a = 1, b=0b = 0 and y=x2+1y = x^2 + 1

    y^=ax2+bx+c\displaystyle \hat y = ax^2 + bx + c
  9. 17.66.9

    Selecting a Regression Model

    Match the shape: linear for steady change, exponential for steady percent change, quadratic for a curve that turns. Leftover patterns in the residuals mean a poor fit.

17.67 Introduction to Probability

ABA onlyB onlyA ∩ Bneithersample spaceAddition lawP(A ∪ B) =P(A) + P(B) − P(A ∩ B)Subtract the overlap, orit gets counted twice.If A and B cannot bothhappen, P(A ∩ B) = 0.
A ∪ B is everything in either circle, and A ∩ B is the shaded overlap. Adding P(A) and P(B) counts the overlap twice, so subtract it once.
  1. 17.67.1

    Sets

    A set is a collection of distinct objects called elements. x∈Ax \in A means xx is an element of AA. The empty set ∅\varnothing has no elements, and A⊆BA \subseteq B means every element of AA is also in BB.

    e.g. Even numbers from 1 to 10: {2,4,6,8,10}\{2, 4, 6, 8, 10\}, a set with 5 elements

    A={1,2,3}\displaystyle A = \{1, 2, 3\}
    2∈A,  5∉A\displaystyle 2 \in A,\; 5 \notin A
  2. 17.67.2

    Experimental Probability

    The fraction of trials in which the event actually happened. More trials usually bring it closer to the theoretical probability.

    e.g. 27 heads in 50 flips: P(heads)≈2750=0.54P(\text{heads}) \approx \tfrac{27}{50} = 0.54

    P(A)≈successestrials\displaystyle P(A) \approx \frac{\text{successes}}{\text{trials}}
  3. 17.67.3

    Using Experimental Probability to Make Predictions

    Multiply the experimental probability by the number of future trials to predict how often the event will happen.

    e.g. Made 18 of 30 free throws. In 50 more shots, expect 1830×50=30\tfrac{18}{30} \times 50 = 30 makes

    expected count=P(A)×n\displaystyle \text{expected count} = P(A) \times n
  4. 17.67.4

    Sample Spaces and Events in Probability

    The sample space SS is the set of all possible outcomes. An event is any subset of SS.

    e.g. Flip two coins: S={HH,HT,TH,TT}S = \{HH, HT, TH, TT\}, and "at least one head" ={HH,HT,TH}= \{HH, HT, TH\}

    S={1,2,3,4,5,6}\displaystyle S = \{1, 2, 3, 4, 5, 6\}
    even={2,4,6}\displaystyle \text{even} = \{2, 4, 6\}
  5. 17.67.5

    The Likelihood of an Event

    Probability runs from 0 (impossible) to 1 (certain). Near 0 is unlikely, 12\tfrac12 is as likely as not, and near 1 is likely.

    e.g. One die: P(7)=0P(7) = 0 is impossible, and P(less than 7)=1P(\text{less than } 7) = 1 is certain

    0≤P(A)≤1\displaystyle 0 \le P(A) \le 1
  6. 17.67.6

    Single Events in Probability

    When all outcomes are equally likely, divide the number of favorable outcomes by the total number of outcomes.

    e.g. One die: P(prime)=36=12P(\text{prime}) = \tfrac{3}{6} = \tfrac12 (2, 3, 5)

    P(A)=n(A)n(S)\displaystyle P(A) = \frac{n(A)}{n(S)}
  7. 17.67.7

    Using Probability to Make Predictions

    Expected number of occurrences = probability × number of trials. It is a long-run average, not a guarantee.

    e.g. Roll a die 120 times: expect 120⋅16=20120 \cdot \tfrac16 = 20 sixes

    expected count=n⋅P(A)\displaystyle \text{expected count} = n \cdot P(A)
  8. 17.67.8

    The Complement of an Event

    The complement A′A' (also written AcA^c) is every outcome in SS that is not in AA. Its probability is 1 minus P(A)P(A).

    e.g. P(rain)=0.3⇒P(no rain)=0.7P(\text{rain}) = 0.3 \Rightarrow P(\text{no rain}) = 0.7

    P(A′)=1−P(A)\displaystyle P(A') = 1 - P(A)
  9. 17.67.9

    Venn Diagrams in Probability

    The rectangle is the sample space and each circle is an event. Fill each region with a count or probability; all regions together total n(S)n(S) or 1.

    e.g. 30 students: 12 soccer only, 8 both, 6 basketball only, 4 neither. P(soccer)=12+830=23P(\text{soccer}) = \tfrac{12 + 8}{30} = \tfrac23

  10. 17.67.10

    Geometric Probability

    When a point is chosen at random in a region, the probability is the favorable length, area, or volume divided by the total.

    e.g. A 4 by 4 square target on a 10 by 10 board: P=16100=0.16P = \tfrac{16}{100} = 0.16

    P=favorable areatotal area\displaystyle P = \frac{\text{favorable area}}{\text{total area}}

17.68 Compound Events in Probability

  1. 17.68.1

    The Union of Sets

    A∪BA \cup B ("A or B") is everything in AA, in BB, or in both. Each element is listed once.

    e.g. {1,2,3}∪{3,4}={1,2,3,4}\{1, 2, 3\} \cup \{3, 4\} = \{1, 2, 3, 4\}

    A∪B={x:x∈A or x∈B}\displaystyle A \cup B = \{x : x \in A \text{ or } x \in B\}
  2. 17.68.2

    The Intersection of Sets

    A∩BA \cap B ("A and B") is the elements in both AA and BB. If they share nothing, A∩B=∅A \cap B = \varnothing and the sets are disjoint.

    e.g. {1,2,3}∩{2,3,4}={2,3}\{1, 2, 3\} \cap \{2, 3, 4\} = \{2, 3\}

    A∩B={x:x∈A and x∈B}\displaystyle A \cap B = \{x : x \in A \text{ and } x \in B\}
  3. 17.68.3

    Compound Events in Probability From Experimental Data

    For "A and B," count the trials where both happened. For "A or B," count the trials where either happened, counting the overlap once. Divide by the total number of trials.

    e.g. 50 people: 20 own a dog, 15 a cat, 5 both. P(dog or cat)=20+15−550=0.6P(\text{dog or cat}) = \tfrac{20 + 15 - 5}{50} = 0.6

    P(A∩B)≈n(A∩B)total\displaystyle P(A \cap B) \approx \frac{n(A \cap B)}{\text{total}}
  4. 17.68.4

    Computing Probabilities for Compound Events Using Venn Diagrams

    Add the regions that make up the event. A∪BA \cup B is every region inside either circle; A∩BA \cap B is only the overlap.

    e.g. A only 0.3, both 0.1, B only 0.2, neither 0.4: P(A∪B)=0.3+0.1+0.2=0.6P(A \cup B) = 0.3 + 0.1 + 0.2 = 0.6, P(A∩B)=0.1P(A \cap B) = 0.1

  5. 17.68.5

    Computing Probabilities of Events Containing Complements Using Venn Diagrams

    A′A' is every region outside circle AA, including the region outside both circles. Work region by region.

    e.g. A only 0.3, both 0.1, B only 0.2, neither 0.4: P(A∩B′)=0.3P(A \cap B') = 0.3, P(A′)=0.2+0.4=0.6P(A') = 0.2 + 0.4 = 0.6

    A∩B′=A only\displaystyle A \cap B' = A \text{ only}
    (A∪B)′=neither\displaystyle (A \cup B)' = \text{neither}
  6. 17.68.6

    Conditional Probabilities From Venn Diagrams

    P(A∣B)P(A \mid B) is the probability of AA given that BB happened. Look only inside circle BB: divide the overlap by all of BB.

    e.g. A only 0.3, both 0.1, B only 0.2: P(A∣B)=0.10.1+0.2=13P(A \mid B) = \tfrac{0.1}{0.1 + 0.2} = \tfrac13

    P(A∣B)=P(A∩B)P(B)\displaystyle P(A \mid B) = \frac{P(A \cap B)}{P(B)}
  7. 17.68.7

    Conditional Probabilities From Tables

    Use only the row or column of the given condition. Divide the cell by that row or column total, not the grand total.

    e.g. 25 students play a sport, and 10 of them are in band: P(band∣sport)=1025=0.4P(\text{band} \mid \text{sport}) = \tfrac{10}{25} = 0.4

    P(A∣B)=n(A∩B)n(B)\displaystyle P(A \mid B) = \frac{n(A \cap B)}{n(B)}
  8. 17.68.8

    The Multiplication Law for Conditional Probability

    The probability that both happen is the probability of the first times the probability of the second given the first.

    e.g. 5 red and 3 blue marbles, draw 2 without replacement: P(both red)=58⋅47=514P(\text{both red}) = \tfrac58 \cdot \tfrac47 = \tfrac{5}{14}

    P(A∩B)=P(A)⋅P(B∣A)\displaystyle P(A \cap B) = P(A) \cdot P(B \mid A)
  9. 17.68.9

    Finding Conditional Probabilities From Frequency Tables

    For P(A∣B)P(A \mid B), use only the row or column for the given condition BB. Divide the count in both AA and BB by the total for BB.

    e.g. 10 of 40 juniors take chemistry: P(chem∣junior)=1040=0.25P(\text{chem} \mid \text{junior}) = \tfrac{10}{40} = 0.25

    P(A∣B)=n(A and B)n(B)\displaystyle P(A \mid B) = \frac{n(A \text{ and } B)}{n(B)}
  10. 17.68.10

    Independent Events

    AA and BB are independent if one happening does not change the probability of the other. Check with either equation.

    e.g. P(A)=0.5P(A) = 0.5, P(B)=0.4P(B) = 0.4, P(A∩B)=0.2=0.5⋅0.4P(A \cap B) = 0.2 = 0.5 \cdot 0.4, so independent

    P(A∣B)=P(A)\displaystyle P(A \mid B) = P(A)
    P(A∩B)=P(A)⋅P(B)\displaystyle P(A \cap B) = P(A) \cdot P(B)

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