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Integrated Math IIHonors · the 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.

12 units, 45 sections, 335 topics. Press / to search.

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Unit 1 10 topics

Number Systems

The Number System, and Introduction to Complex Numbers.

1.1 The Number System

Real numbers ℝRational ℚIrrational√2πnever repeator end−3/40.666…fractionsIntegers ℤ−5Whole0Natural ℕ1, 2, 3, …7
Every natural number is whole, every whole number is an integer, and every integer is rational. Rational and irrational numbers sit side by side and together make up the reals.
  1. 1.1.1

    The Real Number System

    Natural numbers are 1,2,3,…1, 2, 3, \dots; whole numbers add 00; integers add the negatives. Rational numbers are fractions pq\tfrac{p}{q} of integers (q≠0q \ne 0), with decimals that end or repeat. Irrational numbers have decimals that never end or repeat, and rationals and irrationals together make up the real numbers.

    e.g. 0.75=340.75 = \tfrac34 and −5-5 are rational; 2\sqrt2 and π\pi are irrational

    N⊂Z⊂Q⊂R\displaystyle \mathbb{N} \subset \mathbb{Z} \subset \mathbb{Q} \subset \mathbb{R}
    R=Q∪irrationals\displaystyle \mathbb{R} = \mathbb{Q} \cup \text{irrationals}
  2. 1.1.2

    Writing Repeating Decimals as Fractions

    Set xx equal to the decimal. Multiply by 10n10^n, where nn is the number of repeating digits, and subtract xx so the repeating tail cancels. If the repeat starts later, first multiply to move the decimal point to where the repeat begins.

    e.g. x=0.16‾x = 0.1\overline{6}: 100x−10x=16.6‾−1.6‾=15100x - 10x = 16.\overline{6} - 1.\overline{6} = 15, so x=1590=16x = \tfrac{15}{90} = \tfrac16

    x=0.36‾\displaystyle x = 0.\overline{36}
    100x=36.36‾\displaystyle 100x = 36.\overline{36}
    100x−x=36\displaystyle 100x - x = 36
    ⇒  x=3699=411\displaystyle \Rightarrow\; x = \frac{36}{99} = \frac{4}{11}
  3. 1.1.3

    Sums and Products of Rational and Irrational Numbers

    Rational plus rational and rational times rational are always rational. Rational plus irrational is irrational, and a nonzero rational times an irrational is irrational. Two irrationals can give either kind.

    e.g. 3+23 + \sqrt2 is irrational; 2⋅2=2\sqrt2 \cdot \sqrt2 = 2 is rational; 2⋅3=6\sqrt2 \cdot \sqrt3 = \sqrt6 is irrational

1.2 Introduction to Complex Numbers

realimaginary−11234−ii2i3i3 + 2iPowers of i repeat every 4i¹ = ii² = −1i³ = −ii⁴ = 1× i
The number 3 + 2i sits 3 units along the real axis and 2 units up the imaginary axis. Each multiplication by i turns a quarter turn, so the powers of i cycle i, −1, −i, 1.
  1. 1.2.1

    Imaginary Numbers

    The imaginary unit ii is defined by i2=−1i^2 = -1. For b>0b > 0, −b=ib\sqrt{-b} = i\sqrt{b}. Rewrite with ii before multiplying square roots of negatives.

    e.g. −18=3i2\sqrt{-18} = 3i\sqrt2; −4⋅−9=(2i)(3i)=6i2=−6\sqrt{-4} \cdot \sqrt{-9} = (2i)(3i) = 6i^2 = -6

    i=−1\displaystyle i = \sqrt{-1}
    i2=−1\displaystyle i^2 = -1
    −b=ib(b>0)\displaystyle \sqrt{-b} = i\sqrt{b} \quad (b > 0)
  2. 1.2.2

    Quadratic Equations with Purely Imaginary Solutions

    Isolate x2x^2. If it equals a negative number, take ±\pm the square root to get two imaginary solutions.

    e.g. 2x2+18=0⇒x2=−9⇒x=±3i2x^2 + 18 = 0 \Rightarrow x^2 = -9 \Rightarrow x = \pm 3i

    x2=−k(k>0)\displaystyle x^2 = -k \quad (k > 0)
    ⇒  x=±ik\displaystyle \Rightarrow\; x = \pm i\sqrt{k}
  3. 1.2.3

    Complex Numbers

    A complex number has the form a+bia + bi with aa and bb real. aa is the real part and bb is the imaginary part. Every real number is complex (with b=0b = 0), and two complex numbers are equal only when both parts match.

    e.g. −3+4i-3 + 4i: real part −3-3, imaginary part 44

    z=a+bi\displaystyle z = a + bi
    Re⁡(z)=a,  Im⁡(z)=b\displaystyle \operatorname{Re}(z) = a,\; \operatorname{Im}(z) = b
  4. 1.2.4

    Adding and Subtracting Complex Numbers

    Combine real parts with real parts and imaginary parts with imaginary parts. When subtracting, distribute the minus sign to both parts.

    e.g. (5−2i)−(3−6i)=2+4i(5 - 2i) - (3 - 6i) = 2 + 4i

    (a+bi)+(c+di)\displaystyle (a + bi) + (c + di)
    =(a+c)+(b+d)i\displaystyle = (a + c) + (b + d)i
    (a+bi)−(c+di)\displaystyle (a + bi) - (c + di)
    =(a−c)+(b−d)i\displaystyle = (a - c) + (b - d)i
  5. 1.2.5

    Multiplying Complex Numbers

    Multiply like binomials, replace i2i^2 with −1-1, then combine like terms. A number times its conjugate is real.

    e.g. (2+3i)(1−4i)=2−8i+3i−12i2=14−5i(2 + 3i)(1 - 4i) = 2 - 8i + 3i - 12i^2 = 14 - 5i

    (a+bi)(c+di)\displaystyle (a + bi)(c + di)
    =(ac−bd)+(ad+bc)i\displaystyle = (ac - bd) + (ad + bc)i
    (a+bi)(a−bi)=a2+b2\displaystyle (a + bi)(a - bi) = a^2 + b^2
  6. 1.2.6

    Solving Quadratic Equations With Complex Roots

    When the discriminant b2−4acb^2 - 4ac is negative, the quadratic formula gives two complex roots. They are conjugates, p±qip \pm qi.

    e.g. x2−4x+13=0x^2 - 4x + 13 = 0: x=4±−362=2±3ix = \tfrac{4 \pm \sqrt{-36}}{2} = 2 \pm 3i

    x=−b±b2−4ac2a\displaystyle x = \frac{-b \pm \sqrt{b^2 - 4ac}}{2a}
    b2−4ac<0⇒complex roots\displaystyle b^2 - 4ac < 0 \Rightarrow \text{complex roots}
  7. 1.2.7

    The Cyclic Property of the Imaginary Unit

    Powers of ii repeat every 4 steps: i,−1,−i,1i, -1, -i, 1. To find ini^n, divide nn by 4 and use the remainder rr (a remainder of 0 gives 1).

    e.g. i43i^{43}: 43=4⋅10+343 = 4 \cdot 10 + 3, so i43=i3=−ii^{43} = i^3 = -i

    i1=i,  i2=−1\displaystyle i^1 = i,\; i^2 = -1
    i3=−i,  i4=1\displaystyle i^3 = -i,\; i^4 = 1
    in=ir,  r=remainder of n÷4\displaystyle i^n = i^r,\; r = \text{remainder of } n \div 4

Unit 2 31 topics

Polynomials

Polynomials, Quadratic Equations, Factoring Polynomials, and Polynomial Equations.

2.3 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. 2.3.1

    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)}
  2. 2.3.2

    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

  3. 2.3.3

    Describing Relationships Using Polynomial Identities

    A polynomial identity is an equation that is true for every value of its variables. Prove one by expanding or factoring one side until it matches the other. Identities explain number patterns.

    e.g. (n+1)2−n2=2n+1(n + 1)^2 - n^2 = 2n + 1, so consecutive squares always differ by an odd number: 52−42=95^2 - 4^2 = 9

    (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
    a2−b2=(a+b)(a−b)\displaystyle a^2 - b^2 = (a + b)(a - b)

2.4 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. 2.4.1

    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. 2.4.2

    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}
  3. 2.4.3

    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}
  4. 2.4.4

    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
  5. 2.4.5

    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
  6. 2.4.6

    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}
  7. 2.4.7

    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
  8. 2.4.8

    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
  9. 2.4.9

    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
  10. 2.4.10

    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
  11. 2.4.11

    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
  12. 2.4.12

    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

  13. 2.4.13

    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

  14. 2.4.14

    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}
  15. 2.4.15

    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}
  16. 2.4.16

    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
  17. 2.4.17

    Modeling With Quadratic Equations

    Write the area, motion, or number relationship as a quadratic, solve, and reject answers that make no sense, such as negative lengths.

    e.g. Length 3 more than width, area 40 → w(w+3)=40⇒w=5w(w + 3) = 40 \Rightarrow w = 5

  18. 2.4.18

    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
  19. 2.4.19

    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}

2.5 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. 2.5.1

    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. 2.5.2

    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. 2.5.3

    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. 2.5.4

    Factoring Sums and Differences of Cubes

    Write both terms as cubes and use the pattern. Signs follow SOAP: Same, Opposite, Always Positive. The trinomial factor does not factor further over the reals.

    e.g. 8x3−27=(2x−3)(4x2+6x+9)8x^3 - 27 = (2x - 3)(4x^2 + 6x + 9)

    a3+b3\displaystyle a^3 + b^3
    =(a+b)(a2−ab+b2)\displaystyle = (a + b)(a^2 - ab + b^2)
    a3−b3\displaystyle a^3 - b^3
    =(a−b)(a2+ab+b2)\displaystyle = (a - b)(a^2 + ab + b^2)
  5. 2.5.5

    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

2.6 Polynomial Equations

  1. 2.6.1

    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
  2. 2.6.2

    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

  3. 2.6.3

    Solving Cubic Equations by Grouping

    Set the cubic equal to 0, factor by grouping, then set each factor equal to 0.

    e.g. x3−2x2−9x+18=0⇒(x−2)(x−3)(x+3)=0⇒x=2,±3x^3 - 2x^2 - 9x + 18 = 0 \Rightarrow (x - 2)(x - 3)(x + 3) = 0 \Rightarrow x = 2, \pm 3

    x2(x+a)+b(x+a)=0\displaystyle x^2(x + a) + b(x + a) = 0
    ⇒  (x+a)(x2+b)=0\displaystyle \Rightarrow\; (x + a)(x^2 + b) = 0
  4. 2.6.4

    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}

Unit 3 18 topics

Quadratic Functions

Quadratic Functions, and Modeling With Quadratic Functions.

3.7 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. 3.7.1

    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. 3.7.2

    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. 3.7.3

    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. 3.7.4

    Roots of Quadratic Functions

    Where the parabola meets the xx-axis: solve ax2+bx+c=0ax^2 + bx + c = 0.

  5. 3.7.5

    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. 3.7.6

    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. 3.7.7

    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. 3.7.8

    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. 3.7.9

    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. 3.7.10

    Domain and Range of Quadratic Functions

    The domain is all real numbers. The range starts at the vertex: [k,∞)[k, \infty) if a>0a > 0, (−∞,k](-\infty, k] if a<0a < 0.

  11. 3.7.11

    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
  12. 3.7.12

    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

3.8 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. 3.8.1

    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. 3.8.2

    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. 3.8.3

    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. 3.8.4

    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. 3.8.5

    Constructing Revenue, Cost, and Profit Functions

    When price depends on quantity, revenue is quadratic.

    p=50−2q\displaystyle p = 50 - 2q
    ⇒  R=q(50−2q)=50q−2q2\displaystyle \Rightarrow\; R = q(50 - 2q) = 50q - 2q^2
  6. 3.8.6

    Maximizing Profit and Break-Even Points

    Maximum profit is at the vertex of PP. Break-even is where R=CR = C, which means P=0P = 0.

    e.g. P=−2q2+40q−150P = -2q^2 + 40q - 150: best at q=10q = 10, profit 50

    qmax⁡=−b2a\displaystyle q_{\max} = -\frac{b}{2a}

Unit 4 30 topics

Functions

Functions, and Graph Transformations of Functions.

4.9 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. 4.9.1

    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
  2. 4.9.2

    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))
  3. 4.9.3

    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)).

  4. 4.9.4

    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

  5. 4.9.5

    One-To-One Functions

    A function is one-to-one if different inputs always give different outputs. Horizontal line test: no horizontal line crosses the graph more than once.

    e.g. f(x)=2x+1f(x) = 2x + 1 is one-to-one; g(x)=x2g(x) = x^2 is not, since g(−2)=g(2)=4g(-2) = g(2) = 4

    f(a)=f(b)⇒a=b\displaystyle f(a) = f(b) \Rightarrow a = b
  6. 4.9.6

    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}
  7. 4.9.7

    Calculating the Inverse of a Function

    The inverse f−1f^{-1} undoes ff. Replace f(x)f(x) with yy, swap xx and yy, then solve for yy. Note f−1(x)f^{-1}(x) does not mean 1f(x)\tfrac{1}{f(x)}.

    e.g. f(x)=3x−6f(x) = 3x - 6: x=3y−6⇒f−1(x)=x3+2x = 3y - 6 \Rightarrow f^{-1}(x) = \tfrac{x}{3} + 2

    f(a)=b  ⟺  f−1(b)=a\displaystyle f(a) = b \iff f^{-1}(b) = a
    f(f−1(x))=f−1(f(x))=x\displaystyle f(f^{-1}(x)) = f^{-1}(f(x)) = x
  8. 4.9.8

    Inverses of Quadratic Functions

    A quadratic is not one-to-one, so first restrict its domain to one side of the vertex. Then swap xx and yy, solve with square roots, and keep the sign that matches the restricted domain.

    e.g. f(x)=(x−2)2+1f(x) = (x - 2)^2 + 1, x≥2x \ge 2: f−1(x)=2+x−1f^{-1}(x) = 2 + \sqrt{x - 1}, x≥1x \ge 1

    f(x)=a(x−h)2+k,  x≥h\displaystyle f(x) = a(x - h)^2 + k,\; x \ge h
    f−1(x)=h+x−ka\displaystyle f^{-1}(x) = h + \sqrt{\frac{x - k}{a}}
  9. 4.9.9

    Graphs of Inverse Functions

    The graph of f−1f^{-1} is the graph of ff reflected across the line y=xy = x. Each point (a,b)(a, b) on ff becomes (b,a)(b, a) on f−1f^{-1}.

    e.g. f(x)=x3f(x) = x^3 passes through (2,8)(2, 8), so f−1(x)=x3f^{-1}(x) = \sqrt[3]{x} passes through (8,2)(8, 2)

    (a,b)→(b,a)\displaystyle (a, b) \to (b, a)
  10. 4.9.10

    Domain and Range of Inverse Functions

    Inputs and outputs trade places. The domain of f−1f^{-1} is the range of ff, and the range of f−1f^{-1} is the domain of ff.

    e.g. f(x)=x−3f(x) = \sqrt{x - 3}: domain x≥3x \ge 3, range y≥0y \ge 0. f−1(x)=x2+3f^{-1}(x) = x^2 + 3: domain x≥0x \ge 0, range y≥3y \ge 3

    domain of f−1=range of f\displaystyle \text{domain of } f^{-1} = \text{range of } f
    range of f−1=domain of f\displaystyle \text{range of } f^{-1} = \text{domain of } f
  11. 4.9.11

    Invertible Functions

    A function has an inverse function exactly when it is one-to-one, so it passes the horizontal line test. A function that is not one-to-one can be made invertible by restricting its domain.

    e.g. f(x)=x3f(x) = x^3 is invertible; g(x)=∣x∣g(x) = \lvert x \rvert is not, but it is on x≥0x \ge 0

  12. 4.9.12

    Plotting X as a Function of Y

    In x=g(y)x = g(y), yy is the input. Pick yy-values, compute xx, and plot the points (x,y)(x, y). The graph is the graph of y=g(x)y = g(x) reflected across y=xy = x.

    e.g. x=y2x = y^2: y=−2,0,2y = -2, 0, 2 give (4,−2),(0,0),(4,2)(4, -2), (0, 0), (4, 2), a parabola opening right

    x=g(y)\displaystyle x = g(y)
  13. 4.9.13

    Periodic Functions

    A periodic function repeats its values at regular intervals. The period pp is the smallest positive shift that maps the graph onto itself.

    e.g. Period 4 and f(1)=7f(1) = 7: then f(9)=7f(9) = 7 and f(−3)=7f(-3) = 7

    f(x+p)=f(x)  for all x\displaystyle f(x + p) = f(x) \;\text{for all } x
  14. 4.9.14

    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}
  15. 4.9.15

    Products of Even and Odd Functions

    These multiply like signs, with even as ++ and odd as −-. Even times even and odd times odd are even; even times odd is odd. Quotients follow the same rules.

    e.g. x⋅x3=x4x \cdot x^3 = x^4 (odd times odd, even); x2⋅x3=x5x^2 \cdot x^3 = x^5 (even times odd, odd)

    even⋅even=even\displaystyle \text{even} \cdot \text{even} = \text{even}
    odd⋅odd=even\displaystyle \text{odd} \cdot \text{odd} = \text{even}
    even⋅odd=odd\displaystyle \text{even} \cdot \text{odd} = \text{odd}
  16. 4.9.16

    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
  17. 4.9.17

    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}

4.10 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. 4.10.1

    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. 4.10.2

    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. 4.10.3

    Vertical Stretches of Functions

    For a>0a > 0, af(x)a f(x) multiplies every yy-coordinate by aa. It is a stretch if a>1a > 1 and a compression if 0<a<10 < a < 1. Points on the xx-axis stay fixed.

    e.g. y=3x2y = 3x^2: the point (2,4)(2, 4) on y=x2y = x^2 moves to (2,12)(2, 12)

    y=af(x)\displaystyle y = a f(x)
    (x,y)→(x,ay)\displaystyle (x, y) \to (x, ay)
  4. 4.10.4

    Horizontal Stretches of Functions

    For b>0b > 0, f(bx)f(bx) divides every xx-coordinate by bb. It is a compression if b>1b > 1 and a stretch if 0<b<10 < b < 1. Points on the yy-axis stay fixed.

    e.g. y=f(2x)y = f(2x): the point (6,1)(6, 1) on ff moves to (3,1)(3, 1)

    y=f(bx)\displaystyle y = f(bx)
    (x,y)→(xb,y)\displaystyle (x, y) \to \left(\frac{x}{b}, y\right)
  5. 4.10.5

    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)
  6. 4.10.6

    Horizontal Reflections of Functions

    f(−x)f(-x) reflects the graph across the yy-axis. Every xx-coordinate changes sign.

    e.g. y=−xy = \sqrt{-x} passes through (−4,2)(-4, 2) instead of (4,2)(4, 2); domain x≤0x \le 0

    y=f(−x)\displaystyle y = f(-x)
    (x,y)→(−x,y)\displaystyle (x, y) \to (-x, y)
  7. 4.10.7

    Combining Graph Transformations: Two Operations

    Handle outputs and inputs separately. For outputs, follow order of operations: stretch or reflect first, then shift. A horizontal change and a vertical change can be done in either order.

    e.g. y=2f(x)+3y = 2f(x) + 3: the point (1,4)(1, 4) on ff moves to (1,11)(1, 11)

    y=af(x)+k\displaystyle y = a f(x) + k
    (x,y)→(x,ay+k)\displaystyle (x, y) \to (x, ay + k)
  8. 4.10.8

    Combining Graph Transformations: Three or More Operations

    Write the function as af(b(x−h))+ka f(b(x - h)) + k, factoring bb out of the inside first. Horizontally, stretch by 1b\tfrac{1}{b}, then shift by hh. Vertically, stretch or reflect by aa, then shift by kk.

    e.g. y=−2f(3x−6)+1=−2f(3(x−2))+1y = -2f(3x - 6) + 1 = -2f(3(x - 2)) + 1: (6,5)→(4,−9)(6, 5) \to (4, -9)

    y=af(b(x−h))+k\displaystyle y = a f(b(x - h)) + k
    (x,y)→(xb+h,  ay+k)\displaystyle (x, y) \to \left(\frac{x}{b} + h,\; ay + k\right)
  9. 4.10.9

    Constructing Functions Using Transformations

    Start with the parent function and apply each step in the order given. Horizontal changes go inside on xx (shifts with the opposite sign); vertical changes go outside. Each later step acts on everything built so far.

    e.g. Shift y=x2y = x^2 right 3, stretch vertically by 2, then shift up 1: y=2(x−3)2+1y = 2(x - 3)^2 + 1

  10. 4.10.10

    Combining Reflections With Other Graph Transformations

    A reflection is a stretch by −1-1. For outputs, reflect before shifting. For inputs, factor out the negative: f(−x+h)=f(−(x−h))f(-x + h) = f(-(x - h)) means reflect across the yy-axis, then shift right hh.

    e.g. y=−x+3=−(x−3)y = \sqrt{-x + 3} = \sqrt{-(x - 3)}: reflect x\sqrt{x} across the yy-axis, shift right 3; starts at (3,0)(3, 0), domain x≤3x \le 3

    y=−f(x)+k\displaystyle y = -f(x) + k
    y=f(−(x−h))\displaystyle y = f(-(x - h))
  11. 4.10.11

    Finding Points on Transformed Curves

    Map a known point (x,y)(x, y) on ff. Set the inside expression equal to the old xx and solve for the new xx. Run the old yy through the outside operations to get the new yy.

    e.g. (2,3)(2, 3) on ff, g(x)=4f(x+1)−5g(x) = 4f(x + 1) - 5: x+1=2⇒x=1x + 1 = 2 \Rightarrow x = 1, 4(3)−5=74(3) - 5 = 7, so (1,7)(1, 7)

    y=af(b(x−h))+k\displaystyle y = a f(b(x - h)) + k
    (x,y)→(xb+h,  ay+k)\displaystyle (x, y) \to \left(\frac{x}{b} + h,\; ay + k\right)
  12. 4.10.12

    The Domain and Range of Transformed Functions

    Horizontal changes affect only the domain: divide by bb, then add hh. Vertical changes affect only the range: multiply by aa, then add kk. A negative multiplier flips the interval, so reorder its endpoints.

    e.g. ff: domain [0,4][0, 4], range [−1,2][-1, 2]. g(x)=−3f(x−1)+2g(x) = -3f(x - 1) + 2: domain [1,5][1, 5], range [−4,5][-4, 5]

    y=af(b(x−h))+k\displaystyle y = a f(b(x - h)) + k
  13. 4.10.13

    Absolute Value Graph Transformations

    y=a∣x−h∣+ky = a\lvert x - h \rvert + k is a V shape with vertex (h,k)(h, k). It opens up if a>0a > 0 and down if a<0a < 0. The right arm has slope aa and the left arm has slope −a-a.

    e.g. y=−2∣x+1∣+3y = -2\lvert x + 1 \rvert + 3: vertex (−1,3)(-1, 3), opens down, slopes −2-2 (right) and 22 (left)

    y=a∣x−h∣+k\displaystyle y = a\lvert x - h \rvert + k
    vertex (h,k)\displaystyle \text{vertex } (h, k)

Unit 5 8 topics

Absolute Value Functions

Absolute Value Functions.

5.11 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. 5.11.1

    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. 5.11.2

    Vertical Reflections of Absolute Value Graphs

    A negative sign in front flips the V upside down.

    y=−∣x∣\displaystyle y = -\lvert x \rvert
  3. 5.11.3

    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. 5.11.4

    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. 5.11.5

    Domain and Range of Absolute Value Functions

    The domain is all real numbers. The range starts at kk: [k,∞)[k, \infty) if it opens up, (−∞,k](-\infty, k] if down.

  6. 5.11.6

    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

  7. 5.11.7

    Equations Connecting Absolute Value and Linear Functions

    When the other side contains xx, split into two cases and keep only answers where that side is ≥0\ge 0.

  8. 5.11.8

    Absolute Value Equations With Extraneous Solutions

    Check every answer in the original equation. Some solutions of the split equations fail.

    e.g. ∣x+1∣=2x\lvert x + 1 \rvert = 2x → x=1x = 1 works; x=−13x = -\tfrac13 fails

Unit 6 35 topics

Exponentials & Logarithms

Introduction to Logarithms, The Laws of Logarithms, Graphs of Exponential Functions, and more.

6.12 Introduction to Logarithms

log28=3⇔23=8resultexponentbaseA logarithmis an exponent.logb y = xmeans bx = yAsk: 2 to whatpower gives 8?
log₂ 8 = 3 and 2³ = 8 say the same thing. The base stays the base, the log’s value becomes the exponent, and the number inside the log is the result.
  1. 6.12.1

    Converting From Exponential to Logarithmic Form

    A logarithm is an exponent. log⁡bx\log_b x is the power you raise bb to in order to get xx. The base must satisfy b>0b > 0, b≠1b \ne 1, and the input must satisfy x>0x > 0.

    e.g. 25=32⇒log⁡232=52^5 = 32 \Rightarrow \log_2 32 = 5

    by=x  ⟺  log⁡bx=y\displaystyle b^y = x \iff \log_b x = y
  2. 6.12.2

    Converting From Logarithmic to Exponential Form

    The base of the log becomes the base of the power, and the value of the log becomes the exponent.

    e.g. log⁡381=4⇒34=81\log_3 81 = 4 \Rightarrow 3^4 = 81

    log⁡bx=y  ⟺  by=x\displaystyle \log_b x = y \iff b^y = x
  3. 6.12.3

    Evaluating Logarithms

    Rewrite the input as a power of the base, then read off the exponent.

    e.g. log⁡218=log⁡22−3=−3\log_2 \tfrac18 = \log_2 2^{-3} = -3

    log⁡bbk=k\displaystyle \log_b b^k = k
    log⁡b1=0,  log⁡bb=1\displaystyle \log_b 1 = 0,\; \log_b b = 1
  4. 6.12.4

    The Natural Logarithm

    ln⁡x\ln x is the logarithm with base e≈2.718e \approx 2.718. It follows every rule of other logs.

    e.g. ln⁡e7=7\ln e^7 = 7

    ln⁡x=log⁡ex\displaystyle \ln x = \log_e x
    ln⁡e=1,  ln⁡1=0\displaystyle \ln e = 1,\; \ln 1 = 0
    ln⁡ex=x,  eln⁡x=x\displaystyle \ln e^x = x,\; e^{\ln x} = x
  5. 6.12.5

    The Common Logarithm

    log⁡x\log x with no base written means base 10.

    e.g. log⁡0.001=log⁡10−3=−3\log 0.001 = \log 10^{-3} = -3

    log⁡x=log⁡10x\displaystyle \log x = \log_{10} x
    log⁡10k=k\displaystyle \log 10^k = k
  6. 6.12.6

    Simplifying Logarithmic Expressions

    A log and a power with the same base undo each other.

    e.g. 5log⁡59=95^{\log_5 9} = 9 and log⁡332x=2x\log_3 3^{2x} = 2x

    log⁡bbx=x\displaystyle \log_b b^x = x
    blog⁡bx=x(x>0)\displaystyle b^{\log_b x} = x \quad (x > 0)

6.13 The Laws of Logarithms

  1. 6.13.1

    The Product Rule for Logarithms

    The log of a product is the sum of the logs. Both inputs must be positive.

    e.g. log⁡28+log⁡24=log⁡232=5\log_2 8 + \log_2 4 = \log_2 32 = 5

    log⁡b(MN)=log⁡bM+log⁡bN\displaystyle \log_b (MN) = \log_b M + \log_b N
  2. 6.13.2

    The Quotient Rule for Logarithms

    The log of a quotient is the log of the top minus the log of the bottom.

    e.g. log⁡354−log⁡32=log⁡327=3\log_3 54 - \log_3 2 = \log_3 27 = 3

    log⁡bMN=log⁡bM−log⁡bN\displaystyle \log_b \frac{M}{N} = \log_b M - \log_b N
  3. 6.13.3

    The Power Rule for Logarithms

    An exponent on the input moves to the front as a multiplier.

    e.g. log⁡285=5log⁡28=15\log_2 8^5 = 5 \log_2 8 = 15

    log⁡bMp=plog⁡bM\displaystyle \log_b M^p = p \log_b M
  4. 6.13.4

    Combining the Laws of Logarithms

    Use the product, quotient, and power rules together to expand or condense. When condensing, move coefficients up as exponents first.

    e.g. 2log⁡5+log⁡4=log⁡(25⋅4)=log⁡100=22\log 5 + \log 4 = \log(25 \cdot 4) = \log 100 = 2

    log⁡bx2yz\displaystyle \log_b \frac{x^2 y}{z}
    =2log⁡bx+log⁡by−log⁡bz\displaystyle = 2\log_b x + \log_b y - \log_b z
  5. 6.13.5

    The Change of Base Formula for Logarithms

    Rewrites a log in any base you like, such as base 10 or ee for a calculator.

    e.g. log⁡48=log⁡28log⁡24=32\log_4 8 = \tfrac{\log_2 8}{\log_2 4} = \tfrac32

    log⁡bx=log⁡xlog⁡b=ln⁡xln⁡b\displaystyle \log_b x = \frac{\log x}{\log b} = \frac{\ln x}{\ln b}

6.14 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. 6.14.1

    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
  2. 6.14.2

    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
  3. 6.14.3

    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
  4. 6.14.4

    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
  5. 6.14.5

    Combining Graph Transformations of Exponential Functions

    Shift right hh and up kk. A negative aa reflects across the xx-axis, and ∣a∣\lvert a \rvert stretches or shrinks vertically. Apply the stretch and reflection before the vertical shift.

    e.g. y=−3⋅2x−1+5y = -3 \cdot 2^{x-1} + 5: reflect, stretch by 3, right 1, up 5; asymptote y=5y = 5, passes (1,2)(1, 2)

    y=a⋅bx−h+k\displaystyle y = a \cdot b^{x - h} + k
  6. 6.14.6

    Properties of Transformed Exponential Functions

    For y=a⋅bx−h+ky = a \cdot b^{x-h} + k, the domain is all real numbers and the horizontal asymptote is y=ky = k. The sign of aa decides which side of the asymptote the graph is on.

    e.g. y=−2⋅3x+1y = -2 \cdot 3^x + 1: range y<1y < 1, yy-intercept −1-1

    Domain: (−∞,∞)\displaystyle \text{Domain: } (-\infty, \infty)
    Asymptote: y=k\displaystyle \text{Asymptote: } y = k
    Range: y>k    (a>0)\displaystyle \text{Range: } y > k \;\; (a > 0)
    Range: y<k    (a<0)\displaystyle \text{Range: } y < k \;\; (a < 0)

6.15 Graphs of Logarithmic Functions

xy(0, 1)(1, 0)y = xy = 2ˣy = log2 xhorizontalasymptote y = 0vertical asymptotex = 0Inverse functionsy = 2ˣy = log2 x(0, 1)(1, 0)(1, 2)(2, 1)(2, 4)(4, 2)Swap each point to gofrom one graph to the other.
y = 2ˣ and y = log₂ x are inverses, so each is the other reflected across y = x. The exponential never touches y = 0 and the log never touches x = 0.
  1. 6.15.1

    Graphing Logarithmic Functions

    y=log⁡bxy = \log_b x is the reflection of y=bxy = b^x across the line y=xy = x. It has domain x>0x > 0, vertical asymptote x=0x = 0, and passes through (1,0)(1, 0) and (b,1)(b, 1).

    e.g. y=log⁡2xy = \log_2 x passes (12,−1)(\tfrac12, -1), (1,0)(1, 0), (2,1)(2, 1), (4,2)(4, 2)

    (1b,−1),  (1,0),  (b,1)\displaystyle (\tfrac1b, -1),\; (1, 0),\; (b, 1)
  2. 6.15.2

    Combining Graph Transformations of Logarithmic Functions

    Shift right hh and up kk. A negative aa reflects across the xx-axis, and ∣a∣\lvert a \rvert stretches or shrinks vertically. The vertical asymptote moves to x=hx = h.

    e.g. y=log⁡2(x+3)−1y = \log_2(x + 3) - 1: left 3, down 1; asymptote x=−3x = -3, passes (−2,−1)(-2, -1)

    y=alog⁡b(x−h)+k\displaystyle y = a \log_b (x - h) + k
  3. 6.15.3

    Properties of Transformed Logarithmic Functions

    For y=alog⁡b(x−h)+ky = a \log_b(x - h) + k, the input must be positive, so the domain is x>hx > h. The range is all real numbers. Find the xx-intercept by setting y=0y = 0.

    e.g. y=ln⁡(x−2)+1y = \ln(x - 2) + 1: domain x>2x > 2, asymptote x=2x = 2, xx-intercept 2+e−12 + e^{-1}

    Domain: x>h\displaystyle \text{Domain: } x > h
    Range: (−∞,∞)\displaystyle \text{Range: } (-\infty, \infty)
    Asymptote: x=h\displaystyle \text{Asymptote: } x = h
  4. 6.15.4

    Inverses of Exponential and Logarithmic Functions

    bxb^x and log⁡bx\log_b x undo each other. To find an inverse, swap xx and yy, then solve for yy.

    e.g. f(x)=3x+2f(x) = 3^x + 2: x=3y+2⇒f−1(x)=log⁡3(x−2)x = 3^y + 2 \Rightarrow f^{-1}(x) = \log_3(x - 2)

    f(x)=bx  ⟺  f−1(x)=log⁡bx\displaystyle f(x) = b^x \iff f^{-1}(x) = \log_b x

6.16 Exponential Equations

  1. 6.16.1

    Solving Exponential Equations Using Logarithms

    Isolate the power, then take the log of both sides or rewrite in log form.

    e.g. 3x=20⇒x=ln⁡20ln⁡3≈2.733^x = 20 \Rightarrow x = \tfrac{\ln 20}{\ln 3} \approx 2.73

    bx=c\displaystyle b^x = c
    ⇒  x=log⁡bc=ln⁡cln⁡b\displaystyle \Rightarrow\; x = \log_b c = \frac{\ln c}{\ln b}
  2. 6.16.2

    Solving Equations Containing the Exponential Function

    Isolate e(…)e^{(\ldots)}, then take ln⁡\ln of both sides. There is no solution if e(…)e^{(\ldots)} equals zero or a negative number.

    e.g. 4e2x=36⇒e2x=9⇒x=ln⁡92=ln⁡34e^{2x} = 36 \Rightarrow e^{2x} = 9 \Rightarrow x = \tfrac{\ln 9}{2} = \ln 3

    ex=c  ⇒  x=ln⁡c    (c>0)\displaystyle e^x = c \;\Rightarrow\; x = \ln c \;\; (c > 0)
  3. 6.16.3

    Solving Exponential Equations With Different Bases

    Write both sides as powers of a common base, then set the exponents equal.

    e.g. 4x=8x−1⇒22x=23x−3⇒x=34^x = 8^{x-1} \Rightarrow 2^{2x} = 2^{3x-3} \Rightarrow x = 3

    bM=bN  ⇒  M=N\displaystyle b^M = b^N \;\Rightarrow\; M = N
  4. 6.16.4

    Solving Exponential Equations With Different Bases Using Logarithms

    When no common base exists, take ln⁡\ln of both sides, bring exponents down with the power rule, and collect the xx terms.

    e.g. 2x=3x−1⇒xln⁡2=(x−1)ln⁡3⇒x=ln⁡3ln⁡3−ln⁡2≈2.712^x = 3^{x-1} \Rightarrow x\ln 2 = (x-1)\ln 3 \Rightarrow x = \tfrac{\ln 3}{\ln 3 - \ln 2} \approx 2.71

    af(x)=bg(x)\displaystyle a^{f(x)} = b^{g(x)}
    ⇒  f(x)ln⁡a=g(x)ln⁡b\displaystyle \Rightarrow\; f(x)\ln a = g(x)\ln b
  5. 6.16.5

    Solving Exponential Equations Using the Zero-Product Property

    Factor, then set each factor to zero. For forms like b2x+…b^{2x} + \ldots, substitute u=bxu = b^x. Since bx>0b^x > 0 always, a factor like exe^x is never zero and bx=−2b^x = -2 has no solution.

    e.g. 4x−6⋅2x+8=04^x - 6 \cdot 2^x + 8 = 0: u=2xu = 2^x, (u−2)(u−4)=0(u - 2)(u - 4) = 0, so x=1x = 1 or x=2x = 2

    ex(x−a)=0  ⇒  x=a\displaystyle e^x(x - a) = 0 \;\Rightarrow\; x = a

6.17 Logarithmic Equations

  1. 6.17.1

    Solving Logarithmic Equations

    Isolate the log, rewrite in exponential form, and solve. Check that every log input is positive.

    e.g. log⁡3(2x−1)=2⇒2x−1=9⇒x=5\log_3(2x - 1) = 2 \Rightarrow 2x - 1 = 9 \Rightarrow x = 5

    log⁡bx=c  ⇒  x=bc\displaystyle \log_b x = c \;\Rightarrow\; x = b^c
  2. 6.17.2

    Solving Logarithmic Equations Containing the Natural Logarithm

    Isolate ln⁡\ln, then rewrite with base ee.

    e.g. 2ln⁡(x+1)=6⇒ln⁡(x+1)=3⇒x=e3−1≈19.092\ln(x + 1) = 6 \Rightarrow \ln(x + 1) = 3 \Rightarrow x = e^3 - 1 \approx 19.09

    ln⁡x=c  ⇒  x=ec\displaystyle \ln x = c \;\Rightarrow\; x = e^c
  3. 6.17.3

    Solving Logarithmic Equations Using the Laws of Logarithms

    Combine the logs into a single log, convert to exponential form, and solve. Reject any answer that makes an original log input zero or negative.

    e.g. log⁡2x+log⁡2(x−2)=3⇒x(x−2)=8⇒x=4\log_2 x + \log_2(x - 2) = 3 \Rightarrow x(x - 2) = 8 \Rightarrow x = 4 (x=−2x = -2 rejected)

    log⁡bM+log⁡bN=c\displaystyle \log_b M + \log_b N = c
    ⇒  MN=bc\displaystyle \Rightarrow\; MN = b^c
  4. 6.17.4

    Solving Logarithmic Equations by Combining the Laws of Logarithms

    Use the power rule to move coefficients up first, then the product and quotient rules to reach one log. Check answers in the original equation.

    e.g. 2log⁡x−log⁡4=2⇒log⁡x24=2⇒x2=400⇒x=202\log x - \log 4 = 2 \Rightarrow \log \tfrac{x^2}{4} = 2 \Rightarrow x^2 = 400 \Rightarrow x = 20 (x=−20x = -20 rejected)

    alog⁡bM−log⁡bN=log⁡bMaN\displaystyle a\log_b M - \log_b N = \log_b \frac{M^a}{N}
  5. 6.17.5

    Solving Logarithmic Equations With Logarithms on Both Sides

    With a single log of the same base on each side, set the inputs equal. Check that both original inputs are positive.

    e.g. ln⁡(3x−4)=ln⁡(x+6)⇒3x−4=x+6⇒x=5\ln(3x - 4) = \ln(x + 6) \Rightarrow 3x - 4 = x + 6 \Rightarrow x = 5

    log⁡bM=log⁡bN  ⇒  M=N\displaystyle \log_b M = \log_b N \;\Rightarrow\; M = N
  6. 6.17.6

    Solving Logarithmic Equations Using the Zero-Product Property

    Move everything to one side and factor, often by treating log⁡bx\log_b x as a single variable. Set each factor to zero and solve each. The log itself may be zero or negative; only its input must be positive.

    e.g. (log⁡x)2−3log⁡x=0⇒log⁡x(log⁡x−3)=0⇒x=1(\log x)^2 - 3\log x = 0 \Rightarrow \log x(\log x - 3) = 0 \Rightarrow x = 1 or x=1000x = 1000

6.18 Modeling with Exponential Functions

  1. 6.18.1

    Modeling With Compound Interest

    PP is the principal, rr the annual rate as a decimal, nn the number of compounding periods per year, and tt the time in years.

    e.g. $500 at 4 percent compounded quarterly for 3 years: 500(1.01)12≈563.41500(1.01)^{12} \approx 563.41

    A=P(1+rn)nt\displaystyle A = P\left(1 + \frac{r}{n}\right)^{nt}
  2. 6.18.2

    Continuously Compounded Interest

    Interest compounded continuously uses base ee. The rate rr is a decimal and tt is in years.

    e.g. $2,000 at 5 percent for 10 years: 2000e0.5≈3297.442000e^{0.5} \approx 3297.44

    A=Pert\displaystyle A = Pe^{rt}
  3. 6.18.3

    Converting Between Exponents

    Rewrite an exponential with a different base or time unit using exponent rules. Use b=eln⁡bb = e^{\ln b} to switch to base ee, and ek=be^k = b to switch from base ee. To change the time unit, split the exponent.

    e.g. 500(1.08)t=500e0.077t500(1.08)^t = 500e^{0.077t}, since ln⁡1.08≈0.077\ln 1.08 \approx 0.077

    bt=etln⁡b\displaystyle b^t = e^{t \ln b}
    bt=(b1/m)mt\displaystyle b^t = \left(b^{1/m}\right)^{mt}

Unit 7 17 topics

Sequences & Series

Geometric Sequences, Arithmetic Series, and The Binomial Theorem.

7.19 Geometric Sequences

Arithmetic: add d = 325+38+311+314+3Geometric: multiply by r = 212×24×28×216×2aₙ = a₁ + (n − 1)daₙ = a₁ · rⁿ⁻¹
Arithmetic sequences grow by equal steps, like linear functions. Geometric sequences grow by equal factors, like exponential functions.
  1. 7.19.1

    Introduction to Geometric Sequences

    Multiply by the same common ratio rr each time.

    e.g. 3, 6, 12, 24: r=2r = 2

    r=an+1an\displaystyle r = \frac{a_{n+1}}{a_n}
  2. 7.19.2

    The Recursive Formula for a Geometric Sequence

    Give the first term and multiply by rr for the next.

    a1=first term,an=r an−1\displaystyle a_1 = \text{first term},\quad a_n = r\,a_{n-1}
  3. 7.19.3

    The Nth Term of a Geometric Sequence

    Start at a1a_1 and multiply by rr a total of n−1n - 1 times.

    e.g. 2, 6, 18, … → a6=2⋅35=486a_6 = 2 \cdot 3^5 = 486

    an=a1rn−1\displaystyle a_n = a_1r^{n-1}
  4. 7.19.4

    Translating Between Explicit and Recursive Formulas for Geometric Sequences

    Both use the same a1a_1 and rr.

    an=r an−1\displaystyle a_n = r\,a_{n-1}
    ↔  an=a1rn−1\displaystyle \leftrightarrow\; a_n = a_1r^{n-1}
  5. 7.19.5

    Finding the Common Ratio of a Geometric Sequence Given Two Terms

    Divide the later term by the earlier one, then take the root for the number of steps between them.

    e.g. a2=6a_2 = 6, a5=162a_5 = 162 → r3=27r^3 = 27, r=3r = 3

    rm−k=amak\displaystyle r^{m-k} = \frac{a_m}{a_k}
  6. 7.19.6

    Determining Indexes of Terms in Geometric Sequences

    Set a1rn−1a_1r^{n-1} equal to the value and match the powers of rr.

    e.g. 5, 10, 20, …: 640=5⋅27640 = 5 \cdot 2^7 → n=8n = 8

7.20 Arithmetic Series

11011291138114711561165117411831192111011110 columns1 + 2 + 3 + … + 1010 + 9 + 8 + … + 1Every column totals 11.10 columns × 11 = 110,so the sum is 55S = n(a1 + an) / 2= 10(1 + 10) / 2 = 55
Write the series forward and backward and add: every pair has the same total. Half of n pairs gives the sum.
  1. 7.20.1

    Sigma Notation

    ∑\sum means add. Plug each integer from the lower limit to the upper limit into the expression and add the results. There are (upper minus lower plus 1) terms.

    e.g. ∑k=14(2k+1)=3+5+7+9=24\sum_{k=1}^{4} (2k + 1) = 3 + 5 + 7 + 9 = 24

    ∑i=1nai=a1+a2+⋯+an\displaystyle \sum_{i=1}^{n} a_i = a_1 + a_2 + \cdots + a_n
  2. 7.20.2

    Properties of Finite Series

    A sum can be split across addition, and a constant factor can be pulled out. Summing a constant nn times gives nn times the constant.

    e.g. ∑i=110(3i+2)=3⋅55+2⋅10=185\sum_{i=1}^{10} (3i + 2) = 3 \cdot 55 + 2 \cdot 10 = 185

    ∑(ai+bi)=∑ai+∑bi\displaystyle \sum (a_i + b_i) = \sum a_i + \sum b_i
    ∑c ai=c∑ai\displaystyle \sum c\,a_i = c \sum a_i
    ∑i=1nc=cn\displaystyle \sum_{i=1}^{n} c = cn
    ∑i=1ni=n(n+1)2\displaystyle \sum_{i=1}^{n} i = \frac{n(n+1)}{2}
  3. 7.20.3

    Expressing an Arithmetic Series in Sigma Notation

    Write the general term a1+(k−1)da_1 + (k - 1)d, simplify it, and sum from k=1k = 1 to the number of terms.

    e.g. 4+7+10+⋯+31=∑k=110(3k+1)4 + 7 + 10 + \cdots + 31 = \sum_{k=1}^{10} (3k + 1)

    ∑k=1n(a1+(k−1)d)\displaystyle \sum_{k=1}^{n} \big(a_1 + (k - 1)d\big)
  4. 7.20.4

    Finding the Sum of an Arithmetic Series

    Average the first and last terms, then multiply by the number of terms. Use the second form when the last term is unknown.

    e.g. 2+5+8+⋯+292 + 5 + 8 + \cdots + 29: n=10n = 10, S=10(2+29)2=155S = \tfrac{10(2 + 29)}{2} = 155

    Sn=n(a1+an)2\displaystyle S_n = \frac{n(a_1 + a_n)}{2}
    Sn=n2(2a1+(n−1)d)\displaystyle S_n = \frac{n}{2}\big(2a_1 + (n - 1)d\big)
  5. 7.20.5

    Finding the First Term of an Arithmetic Series

    Substitute the known values into a sum formula and solve for a1a_1.

    e.g. S8=100S_8 = 100, d=3d = 3: 100=82(2a1+21)⇒25=2a1+21⇒a1=2100 = \tfrac82(2a_1 + 21) \Rightarrow 25 = 2a_1 + 21 \Rightarrow a_1 = 2

    a1=2Snn−an\displaystyle a_1 = \frac{2S_n}{n} - a_n
  6. 7.20.6

    Calculating the Number of Terms in an Arithmetic Series

    If the last term is known, use the formula below. If only the sum is known, set up SnS_n, solve the quadratic in nn, and keep the positive whole-number answer.

    e.g. 5+9+13+⋯+815 + 9 + 13 + \cdots + 81: n=81−54+1=20n = \tfrac{81 - 5}{4} + 1 = 20

    n=an−a1d+1\displaystyle n = \frac{a_n - a_1}{d} + 1
  7. 7.20.7

    Modeling With Arithmetic Series

    Use when a quantity changes by the same amount each step and you need the total. Identify a1a_1, dd, and nn, then apply the sum formula.

    e.g. 15 rows, 20 seats in row 1, 2 more per row: last row 20+14⋅2=4820 + 14 \cdot 2 = 48, total 15(20+48)2=510\tfrac{15(20 + 48)}{2} = 510

7.21 The Binomial Theorem

11112113311464115101051row 0row 1row 2row 3row 4row 5(a + b)4 =a4 + 4a3b + 6a2b2 + 4ab3 + b4Row n holds the coefficientsof (a + b)n.Each entry is the sum of thetwo above it: 3 + 3 = 6.
Each number in Pascal’s triangle is the sum of the two above it. Row 4 gives the coefficients 1, 4, 6, 4, 1 of (a + b)⁴.
  1. 7.21.1

    Pascal's Triangle and the Binomial Coefficients

    Each entry is the sum of the two entries above it. Row nn (counting the top as row 0) lists (n0)\binom{n}{0} through (nn)\binom{n}{n}.

    e.g. Row 4 is 1,4,6,4,11, 4, 6, 4, 1, so (42)=6\binom42 = 6

    (nr)=n!r! (n−r)!\displaystyle \binom{n}{r} = \frac{n!}{r!\,(n - r)!}
    (nr)=(n−1r−1)+(n−1r)\displaystyle \binom{n}{r} = \binom{n-1}{r-1} + \binom{n-1}{r}
  2. 7.21.2

    Expanding a Binomial Using Binomial Coefficients

    Powers of aa fall from nn to 0 while powers of bb rise from 0 to nn. Coefficients come from row nn of Pascal's triangle. Keep any negative sign with bb.

    e.g. (x−2)3=x3−6x2+12x−8(x - 2)^3 = x^3 - 6x^2 + 12x - 8

    (a+b)n=∑k=0n(nk)an−kbk\displaystyle (a + b)^n = \sum_{k=0}^{n} \binom{n}{k} a^{n-k} b^k
  3. 7.21.3

    The Special Case of the Binomial Theorem

    With a=1a = 1, the expansion of (1+x)n(1 + x)^n uses the binomial coefficients directly. Setting x=1x = 1 shows that row nn of Pascal's triangle sums to 2n2^n.

    e.g. (1+x)4=1+4x+6x2+4x3+x4(1 + x)^4 = 1 + 4x + 6x^2 + 4x^3 + x^4

    (1+x)n=∑k=0n(nk)xk\displaystyle (1 + x)^n = \sum_{k=0}^{n} \binom{n}{k} x^k
    =1+nx+(n2)x2+⋯\displaystyle = 1 + nx + \binom{n}{2}x^2 + \cdots
  4. 7.21.4

    Approximating Values Using the Binomial Theorem

    Write the number as (1+x)n(1 + x)^n with xx small and keep the first few terms. Later terms are tiny.

    e.g. 1.025≈1+5(0.02)+10(0.0004)=1.1041.02^5 \approx 1 + 5(0.02) + 10(0.0004) = 1.104

    (1+x)n≈1+nx+(n2)x2\displaystyle (1 + x)^n \approx 1 + nx + \binom{n}{2}x^2

Unit 8 7 topics

Rationals & Radicals

Rational Expressions, and Radical Equations.

8.22 Rational Expressions

  1. 8.22.1

    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)
  2. 8.22.2

    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}
  3. 8.22.3

    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}
  4. 8.22.4

    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}
  5. 8.22.5

    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}

8.23 Radical Equations

  1. 8.23.1

    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
  2. 8.23.2

    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

Unit 9 53 topics

Geometry

Similarity, Circles, Polygons, and more.

9.24 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. 9.24.1

    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. 9.24.2

    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. 9.24.3

    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. 9.24.4

    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. 9.24.5

    Similarity Transformations

    A similarity transformation is a dilation combined with any rigid motions (translations, rotations, reflections). Two figures are similar exactly when one maps onto the other by such a transformation.

    e.g. Dilate (1,3)(1, 3) by 2, then shift right 1: (1,3)→(2,6)→(3,6)(1, 3) \to (2, 6) \to (3, 6)

    dilation about origin:\displaystyle \text{dilation about origin:}
    (x,y)→(kx,ky)\displaystyle (x, y) \to (kx, ky)
  6. 9.24.6

    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. 9.24.7

    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. 9.24.8

    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. 9.24.9

    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. 9.24.10

    Proving Similarity Statements

    Back every condition of a criterion with a reason: given, reflexive property, vertical angles, or angles from parallel lines. After proving similarity, corresponding sides are proportional.

    e.g. AB‾∥DE‾\overline{AB} \parallel \overline{DE} with AE‾\overline{AE} and BD‾\overline{BD} crossing at CC: vertical angles at CC and alternate interior angles ∠A≅∠E\angle A \cong \angle E give △ABC∼△EDC\triangle ABC \sim \triangle EDC by AA.

    ∠A≅∠Areflexive\displaystyle \angle A \cong \angle A \quad \text{reflexive}
    ∠ADE≅∠Bcorr. angles\displaystyle \angle ADE \cong \angle B \quad \text{corr. angles}
    △ADE∼△ABCAA\displaystyle \triangle ADE \sim \triangle ABC \quad \text{AA}
  11. 9.24.11

    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
  12. 9.24.12

    Proving the Midpoint Theorem

    Show the small triangle is similar to the big one by SAS. Then the side ratio gives the length, and congruent corresponding angles give the parallel lines.

    e.g. ∠ADE≅∠B\angle ADE \cong \angle B are corresponding angles, so DE∥BCDE \parallel BC by the converse of the corresponding angles theorem.

    ADAB=AEAC=12midpoints\displaystyle \tfrac{AD}{AB} = \tfrac{AE}{AC} = \tfrac12 \quad \text{midpoints}
    ∠A≅∠Areflexive\displaystyle \angle A \cong \angle A \quad \text{reflexive}
    △ADE∼△ABCSAS\displaystyle \triangle ADE \sim \triangle ABC \quad \text{SAS}
    ⇒  DE=12BC,  DE∥BC\displaystyle \Rightarrow\; DE = \tfrac12 BC,\; DE \parallel BC
  13. 9.24.13

    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}

9.25 Circles

2θθsame arcdiameterThalesInscribed angle= ½ central angleon the same arcAngle on a diameter= 90°half of the 180° arc
An inscribed angle is half the central angle that stands on the same arc. A diameter cuts off a 180° arc, so any angle standing on it is 90°.
  1. 9.25.1

    Inscribed Angles

    An inscribed angle has its vertex on the circle and chords as sides. It measures half its intercepted arc. A central angle equals its arc.

    e.g. Intercepted arc 110∘110^\circ: inscribed angle 55∘55^\circ

    m∠ACB=12 mAB⌢\displaystyle m\angle ACB = \tfrac12\, m\overset{\frown}{AB}
  2. 9.25.2

    Problem-Solving With Inscribed Angles

    Inscribed angles that intercept the same arc are congruent. An inscribed angle is half the central angle on the same arc. Arcs around a circle total 360∘360^\circ.

    e.g. ∠ACB\angle ACB and ∠ADB\angle ADB intercept the same arc: 3x+5=5x−15⇒x=103x + 5 = 5x - 15 \Rightarrow x = 10, so each angle is 35∘35^\circ.

    m∠inscribed=12 m∠central\displaystyle m\angle \text{inscribed} = \tfrac12\, m\angle \text{central}
  3. 9.25.3

    Thales' Theorem

    An angle inscribed in a semicircle is a right angle. Conversely, the hypotenuse of a right triangle inscribed in a circle is a diameter.

    e.g. Inscribed right triangle with legs 6 and 8: hypotenuse =10= 10 is a diameter, so the radius is 5.

    AB diameter⇒m∠ACB=90∘\displaystyle AB \text{ diameter} \Rightarrow m\angle ACB = 90^\circ
  4. 9.25.4

    Angles in Inscribed Right Triangles

    If one side of an inscribed triangle is a diameter, the angle opposite it is 90∘90^\circ and the other two angles add to 90∘90^\circ.

    e.g. AB‾\overline{AB} is a diameter and m∠CAB=35∘m\angle CAB = 35^\circ: m∠ABC=55∘m\angle ABC = 55^\circ

    m∠A+m∠B=90∘\displaystyle m\angle A + m\angle B = 90^\circ
  5. 9.25.5

    Further Angles in Inscribed Right Triangles

    Draw the radius OC‾\overline{OC} to the right-angle vertex. It splits the triangle into two isosceles triangles, since all radii are equal. A central angle is twice the inscribed angle on the same arc.

    e.g. m∠CAB=25∘m\angle CAB = 25^\circ: m∠OCA=25∘m\angle OCA = 25^\circ, m∠AOC=130∘m\angle AOC = 130^\circ, m∠BOC=50∘m\angle BOC = 50^\circ, m∠ABC=65∘m\angle ABC = 65^\circ

    OA=OB=OC=r\displaystyle OA = OB = OC = r
    m∠BOC=2 m∠BAC\displaystyle m\angle BOC = 2\, m\angle BAC
  6. 9.25.6

    Inscribed Quadrilaterals

    A quadrilateral inscribed in a circle has opposite angles that are supplementary. The converse is also true.

    e.g. m∠A=70∘⇒m∠C=110∘m\angle A = 70^\circ \Rightarrow m\angle C = 110^\circ

    m∠A+m∠C=180∘\displaystyle m\angle A + m\angle C = 180^\circ
    m∠B+m∠D=180∘\displaystyle m\angle B + m\angle D = 180^\circ
  7. 9.25.7

    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
  8. 9.25.8

    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
  9. 9.25.9

    Secant-Secant Angles to Circles

    Two secants meeting outside the circle form an angle equal to half the difference of the intercepted arcs. Two chords crossing inside form an angle equal to half the sum of the intercepted arcs.

    e.g. Outside, arcs 100∘100^\circ and 30∘30^\circ: 35∘35^\circ. Inside, arcs 80∘80^\circ and 40∘40^\circ: 60∘60^\circ.

    outside: 12(far−near)\displaystyle \text{outside: } \tfrac12(\text{far} - \text{near})
    inside: 12(arc1+arc2)\displaystyle \text{inside: } \tfrac12(\text{arc}_1 + \text{arc}_2)
  10. 9.25.10

    Secant-Tangent Angles to Circles

    A secant and a tangent meeting outside the circle form an angle equal to half the difference of the intercepted arcs.

    e.g. Arcs 150∘150^\circ and 50∘50^\circ: m∠P=12(100)=50∘m\angle P = \tfrac12(100) = 50^\circ

    m∠P=12(far−near)\displaystyle m\angle P = \tfrac12(\text{far} - \text{near})
  11. 9.25.11

    The Tangent-Chord Theorem

    The angle between a tangent and a chord at the point of tangency is half the intercepted arc. It equals any inscribed angle on that same arc.

    e.g. Tangent and chord intercept a 140∘140^\circ arc: the angle is 70∘70^\circ.

    m∠=12 mAB⌢\displaystyle m\angle = \tfrac12\, m\overset{\frown}{AB}
  12. 9.25.12

    Circle Similarity

    All circles are similar. The scale factor is the ratio of the radii, so circumferences scale by kk and areas by k2k^2.

    e.g. Radii 3 and 6: k=2k = 2, circumference ratio 2, area ratio 4

    k=r2r1\displaystyle k = \frac{r_2}{r_1}
    C2C1=k,A2A1=k2\displaystyle \frac{C_2}{C_1} = k,\quad \frac{A_2}{A_1} = k^2
  13. 9.25.13

    Proving Circle Similarity

    Translate one circle so its center lands on the other's center. Then dilate about that center by the ratio of the radii. A similarity transformation maps one onto the other.

    e.g. Center (1,2)(1, 2), r=2r = 2 and center (4,0)(4, 0), r=6r = 6: translate by ⟨3,−2⟩\langle 3, -2 \rangle, then dilate by 3 about (4,0)(4, 0).

    translate O1 to O2\displaystyle \text{translate } O_1 \text{ to } O_2
    dilate by k=r2r1 about O2\displaystyle \text{dilate by } k = \tfrac{r_2}{r_1} \text{ about } O_2
    ⇒  the circles are similar\displaystyle \Rightarrow\; \text{the circles are similar}

9.26 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. 9.26.1

    Proving Triangle Theorems

    The angles of a triangle add to 180∘180^\circ. An exterior angle equals the sum of the two remote interior angles. Proof of the sum: draw a line through one vertex parallel to the opposite side.

    e.g. Remote interior angles 50∘50^\circ and 70∘70^\circ: exterior angle 120∘120^\circ

    draw ℓ∥BC through A\displaystyle \text{draw } \ell \parallel BC \text{ through } A
    ∠1≅∠B, ∠3≅∠Calt. int.\displaystyle \angle 1 \cong \angle B,\ \angle 3 \cong \angle C \quad \text{alt. int.}
    ∠1+∠A+∠3=180∘line\displaystyle \angle 1 + \angle A + \angle 3 = 180^\circ \quad \text{line}
  2. 9.26.2

    Proofs Involving Isosceles Triangles

    Base angles theorem: if two sides are congruent, the angles opposite them are congruent, and conversely. Proof: bisect the vertex angle with AD‾\overline{AD}, which is shared by both halves (reflexive).

    e.g. Vertex angle 40∘40^\circ: each base angle is 12(180−40)=70∘\tfrac12(180 - 40) = 70^\circ

    AB≅ACgiven\displaystyle AB \cong AC \quad \text{given}
    ∠BAD≅∠CADbisector\displaystyle \angle BAD \cong \angle CAD \quad \text{bisector}
    △ABD≅△ACDSAS\displaystyle \triangle ABD \cong \triangle ACD \quad \text{SAS}
    ∠B≅∠CCPCTC\displaystyle \angle B \cong \angle C \quad \text{CPCTC}
  3. 9.26.3

    Proofs Involving Medians and Centroids

    A median joins a vertex to the midpoint of the opposite side. The three medians meet at the centroid GG, which divides each median 2:12 : 1 from the vertex. Proof below: medians BE‾\overline{BE} and CF‾\overline{CF} meet at GG.

    e.g. A median of length 18: vertex to centroid 12, centroid to midpoint 6

    FE∥BC, FE=12BCmidpt.\displaystyle FE \parallel BC,\ FE = \tfrac12 BC \quad \text{midpt.}
    △GFE∼△GCBAA\displaystyle \triangle GFE \sim \triangle GCB \quad \text{AA}
    ⇒  BG=2 GE,  CG=2 GF\displaystyle \Rightarrow\; BG = 2\,GE,\; CG = 2\,GF
  4. 9.26.4

    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
  5. 9.26.5

    Properties of Parallelograms

    Opposite sides are parallel and congruent. Opposite angles are congruent and consecutive angles are supplementary. The diagonals bisect each other.

    e.g. Diagonals meet at EE with AE=2x+1AE = 2x + 1, EC=3x−4EC = 3x - 4: x=5x = 5, so AC=22AC = 22

    AB=CD,  BC=DA\displaystyle AB = CD,\; BC = DA
    m∠A=m∠C\displaystyle m\angle A = m\angle C
    m∠A+m∠B=180∘\displaystyle m\angle A + m\angle B = 180^\circ
  6. 9.26.6

    Proving Properties of Parallelograms

    Draw diagonal AC‾\overline{AC}, which is shared by both triangles (reflexive). Each pair of parallel sides gives alternate interior angles, so the triangles are congruent by ASA.

    e.g. CPCTC also gives ∠B≅∠D\angle B \cong \angle D, so opposite angles are congruent.

    ∠BAC≅∠DCAalt. int.\displaystyle \angle BAC \cong \angle DCA \quad \text{alt. int.}
    ∠BCA≅∠DACalt. int.\displaystyle \angle BCA \cong \angle DAC \quad \text{alt. int.}
    △ABC≅△CDAASA\displaystyle \triangle ABC \cong \triangle CDA \quad \text{ASA}
    ⇒  AB≅CD, BC≅DA\displaystyle \Rightarrow\; AB \cong CD,\ BC \cong DA
  7. 9.26.7

    Proving Criteria for Parallelograms and Rectangles

    A quadrilateral is a parallelogram if both pairs of opposite sides are congruent, one pair is both congruent and parallel, both pairs of opposite angles are congruent, or the diagonals bisect each other. A parallelogram with congruent diagonals or one right angle is a rectangle.

    e.g. The diagonals of ABCDABCD bisect each other and are both 10 long, so ABCDABCD is a rectangle.

    AE≅EC, BE≅EDgiven\displaystyle AE \cong EC,\ BE \cong ED \quad \text{given}
    △AEB≅△CEDSAS\displaystyle \triangle AEB \cong \triangle CED \quad \text{SAS}
    ∠BAE≅∠DCECPCTC\displaystyle \angle BAE \cong \angle DCE \quad \text{CPCTC}
    ⇒  AB∥CDalt. int.\displaystyle \Rightarrow\; AB \parallel CD \quad \text{alt. int.}

9.27 Circles

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. 9.27.1

    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. 9.27.2

    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. 9.27.3

    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. 9.27.4

    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. 9.27.5

    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. 9.27.6

    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. 9.27.7

    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. 9.27.8

    Perpendicular Bisectors of Diameters in the Coordinate Plane

    The midpoint of a diameter is the center. The perpendicular bisector of a diameter passes through the center with the negative reciprocal slope, and it contains the perpendicular diameter.

    e.g. Diameter from (1,2)(1, 2) to (5,6)(5, 6): center (3,4)(3, 4), slope 1, bisector y=−x+7y = -x + 7

    M=(x1+x22,y1+y22)\displaystyle M = \left(\tfrac{x_1 + x_2}{2}, \tfrac{y_1 + y_2}{2}\right)
    m⊥=−1m\displaystyle m_\perp = -\tfrac{1}{m}
  9. 9.27.9

    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
  10. 9.27.10

    Perpendicular Bisectors of Chords in the Coordinate Plane

    Find the perpendicular bisectors of two chords. They meet at the center. Then the radius is the distance from the center to any point on the circle.

    e.g. Points (0,0)(0, 0), (6,0)(6, 0), (0,4)(0, 4): bisectors x=3x = 3 and y=2y = 2, center (3,2)(3, 2), r=13r = \sqrt{13}

  11. 9.27.11

    Thales' Theorem in the Coordinate Plane

    If AB‾\overline{AB} is a diameter and CC is another point on the circle, then CA‾⊥CB‾\overline{CA} \perp \overline{CB}, so their slopes multiply to −1-1. Conversely, the hypotenuse of an inscribed right triangle is a diameter, and its midpoint is the center.

    e.g. x2+y2=25x^2 + y^2 = 25, A(−5,0)A(-5, 0), B(5,0)B(5, 0), C(3,4)C(3, 4): slopes 12\tfrac12 and −2-2, product −1-1

    mCA⋅mCB=−1\displaystyle m_{CA} \cdot m_{CB} = -1

9.28 Parabolas

xy−4−3−2−1124−2234F(0, 1)Pequalequaldirectrix y = −1y = x²/4(x − h)² = 4p(y − k)vertex (h, k)focus: p above the vertexdirectrix: p below itHere: x² = 4y, so p = 1Every point is as far fromthe focus as from the directrix.
Every point on a parabola is the same distance from the focus as from the directrix. For x² = 4y, p = 1, so the focus is 1 above the vertex and the directrix is 1 below.
  1. 9.28.1

    Upward and Downward Opening Parabolas

    A parabola with a vertical axis has vertex (h,k)(h, k). It opens up if p>0p > 0 and down if p<0p < 0.

    e.g. x2=−12yx^2 = -12y: 4p=−124p = -12, p=−3p = -3, opens down

    (x−h)2=4p(y−k)\displaystyle (x - h)^2 = 4p(y - k)
    p>0 up,p<0 down\displaystyle p > 0 \text{ up},\quad p < 0 \text{ down}
  2. 9.28.2

    Left and Right Opening Parabolas

    When yy is the squared variable, the axis is horizontal. It opens right if p>0p > 0 and left if p<0p < 0.

    e.g. y2=−8xy^2 = -8x: 4p=−84p = -8, p=−2p = -2, opens left

    (y−k)2=4p(x−h)\displaystyle (y - k)^2 = 4p(x - h)
    p>0 right,p<0 left\displaystyle p > 0 \text{ right},\quad p < 0 \text{ left}
  3. 9.28.3

    The Vertex of a Parabola

    The vertex is the turning point, (h,k)(h, k) in either form. It lies on the axis of symmetry, halfway between the focus and the directrix.

    e.g. (y+1)2=12(x−4)(y + 1)^2 = 12(x - 4): vertex (4,−1)(4, -1), opens right

    (x−h)2=4p(y−k)→(h,k)\displaystyle (x - h)^2 = 4p(y - k) \to (h, k)
    (y−k)2=4p(x−h)→(h,k)\displaystyle (y - k)^2 = 4p(x - h) \to (h, k)
  4. 9.28.4

    Calculating the Vertex of a Parabola by Completing the Square

    Put the squared variable's terms on one side, complete the square, and factor the other side into the form 4p(…)4p(\ldots). If the squared term has a coefficient, divide by it first.

    e.g. y=x2−6x+5⇒(x−3)2=y+4y = x^2 - 6x + 5 \Rightarrow (x - 3)^2 = y + 4: vertex (3,−4)(3, -4)

    x2+bx=(x+b2)2−b24\displaystyle x^2 + bx = \left(x + \tfrac{b}{2}\right)^2 - \tfrac{b^2}{4}
  5. 9.28.5

    The Focus-Directrix Property of a Parabola

    Every point on a parabola is the same distance from the focus (a point) and the directrix (a line). The vertex is midway between them, ∣p∣\lvert p \rvert from each.

    e.g. Focus (0,2)(0, 2), directrix y=−2y = -2: x2=8yx^2 = 8y. Point (4,2)(4, 2) is 4 from both.

    PF=PD\displaystyle PF = PD
    x2+(y−p)2=∣y+p∣\displaystyle \sqrt{x^2 + (y - p)^2} = \lvert y + p \rvert
    ⇒  x2=4py\displaystyle \Rightarrow\; x^2 = 4py
  6. 9.28.6

    Calculating the Focus of a Parabola

    Find the vertex and pp, then move pp units from the vertex along the axis, toward the inside of the curve.

    e.g. (x−1)2=8(y+2)(x - 1)^2 = 8(y + 2): p=2p = 2, vertex (1,−2)(1, -2), focus (1,0)(1, 0)

    (x−h)2=4p(y−k)→(h,k+p)\displaystyle (x - h)^2 = 4p(y - k) \to (h, k + p)
    (y−k)2=4p(x−h)→(h+p,k)\displaystyle (y - k)^2 = 4p(x - h) \to (h + p, k)
  7. 9.28.7

    Calculating the Directrix of a Parabola

    The directrix is the line pp units from the vertex on the opposite side from the focus.

    e.g. (y−3)2=−12(x−1)(y - 3)^2 = -12(x - 1): p=−3p = -3, vertex (1,3)(1, 3), directrix x=4x = 4

    (x−h)2=4p(y−k)→y=k−p\displaystyle (x - h)^2 = 4p(y - k) \to y = k - p
    (y−k)2=4p(x−h)→x=h−p\displaystyle (y - k)^2 = 4p(x - h) \to x = h - p
  8. 9.28.8

    Calculating Intercepts of Parabolas

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

    e.g. (x−2)2=4(y+1)(x - 2)^2 = 4(y + 1): y=0y = 0 gives x=0,4x = 0, 4. x=0x = 0 gives y=0y = 0.

    x-intercepts: y=0\displaystyle x\text{-intercepts: } y = 0
    y-intercepts: x=0\displaystyle y\text{-intercepts: } x = 0
  9. 9.28.9

    Intersections of Parabolas With Lines

    Substitute the line into the parabola and solve the quadratic. Two solutions means two crossing points, one means the line touches once, none means no intersection.

    e.g. x2=4yx^2 = 4y, y=x+3y = x + 3: x2−4x−12=0x^2 - 4x - 12 = 0, so (6,9)(6, 9) and (−2,1)(-2, 1)

Unit 10 26 topics

Solid Geometry

Introduction to Solid Geometry, Rectangular Solids and Pyramids, and Non-Polyhedrons.

10.29 Introduction to Solid Geometry

netfoldcube6 faces8 vertices12 edgesV − E + F = 28 − 12 + 6 = 2Euler’s formula
Six squares in a cross fold up into a cube. Counting vertices, edges, and faces on any polyhedron like this one gives V − E + F = 2.
  1. 10.29.1

    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. 10.29.2

    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. 10.29.3

    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. 10.29.4

    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

  5. 10.29.5

    The Distance Formula in Three Dimensions

    Like the 2D distance formula, with a third squared difference for zz.

    e.g. (1,2,3)(1, 2, 3) to (3,5,9)(3, 5, 9): 4+9+36=49=7\sqrt{4 + 9 + 36} = \sqrt{49} = 7

    d=(x2−x1)2+(y2−y1)2+(z2−z1)2\displaystyle d = \sqrt{(x_2 - x_1)^2 + (y_2 - y_1)^2 + (z_2 - z_1)^2}
  6. 10.29.6

    Euler's Formula for Polyhedra

    For any convex polyhedron, vertices minus edges plus faces equals 2. Use it to find a missing count.

    e.g. V=12V = 12, E=30E = 30: F=2−12+30=20F = 2 - 12 + 30 = 20

    V−E+F=2\displaystyle V - E + F = 2
  7. 10.29.7

    The Five Platonic Solids

    A Platonic solid is a convex polyhedron whose faces are congruent regular polygons, with the same number of faces meeting at every vertex. There are exactly five: tetrahedron (4 triangles), cube (6 squares), octahedron (8 triangles), dodecahedron (12 pentagons), and icosahedron (20 triangles).

    e.g. Octahedron: E=8×32=12E = \tfrac{8 \times 3}{2} = 12, V=2−8+12=6V = 2 - 8 + 12 = 6

    E=F×(sides per face)2\displaystyle E = \frac{F \times (\text{sides per face})}{2}
  8. 10.29.8

    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

10.30 Rectangular Solids and Pyramids

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. 10.30.1

    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. 10.30.2

    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. 10.30.3

    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. 10.30.4

    Diagonals of Cubes

    The space diagonal runs through the inside of the cube between opposite vertices. It is the hypotenuse of a right triangle with legs ss and s2s\sqrt2.

    e.g. s=4s = 4: D=43≈6.93D = 4\sqrt3 \approx 6.93

    D=s3\displaystyle D = s\sqrt{3}
  5. 10.30.5

    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. 10.30.6

    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)
  7. 10.30.7

    Diagonals of Rectangular Solids

    The space diagonal connects opposite corners through the interior. It extends the Pythagorean theorem to three dimensions.

    e.g. 3×4×123 \times 4 \times 12: 9+16+144=169=13\sqrt{9 + 16 + 144} = \sqrt{169} = 13

    d=l2+w2+h2\displaystyle d = \sqrt{l^2 + w^2 + h^2}
  8. 10.30.8

    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
  9. 10.30.9

    Surface Areas of Pyramids

    Add the base area to the areas of the triangular faces. For a regular pyramid, the lateral area is half the base perimeter times the slant height ℓ\ell.

    e.g. Square base side 6, ℓ=5\ell = 5: 36+12⋅24⋅5=36+60=9636 + \tfrac12 \cdot 24 \cdot 5 = 36 + 60 = 96

    SA=B+L\displaystyle SA = B + L
    L=12Pℓ(regular)\displaystyle L = \frac{1}{2}P\ell \quad \text{(regular)}

10.31 Non-Polyhedrons

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. 10.31.1

    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
  2. 10.31.2

    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
  3. 10.31.3

    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
  4. 10.31.4

    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}
  5. 10.31.5

    Surface Areas of Right Cones

    Circular base plus the lateral area πrℓ\pi r \ell, where ℓ\ell is the slant height.

    e.g. r=3r = 3, ℓ=5\ell = 5: 9π+15π=24π≈75.49\pi + 15\pi = 24\pi \approx 75.4

    SA=πr2+πrℓ\displaystyle SA = \pi r^2 + \pi r \ell
  6. 10.31.6

    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
  7. 10.31.7

    Surface Areas of Spheres

    Four times the area of a great circle. A hemisphere's curved surface is 2πr22\pi r^2; add πr2\pi r^2 for its flat base.

    e.g. r=5r = 5: SA=100π≈314.2SA = 100\pi \approx 314.2

    SA=4πr2\displaystyle SA = 4\pi r^2
  8. 10.31.8

    Conical Frustums

    A frustum is the part of a cone left after cutting off the top with a plane parallel to the base. It has radii RR (bottom) and rr (top) and height hh. You can also find its volume as the big cone minus the small cone.

    e.g. R=4R = 4, r=2r = 2, h=3h = 3: V=π(16+8+4)=28πV = \pi(16 + 8 + 4) = 28\pi

    V=13πh (R2+Rr+r2)\displaystyle V = \frac{1}{3}\pi h\,(R^2 + Rr + r^2)
    ℓ=h2+(R−r)2\displaystyle \ell = \sqrt{h^2 + (R - r)^2}
    L=π(R+r)ℓ\displaystyle L = \pi (R + r)\ell
  9. 10.31.9

    Volumes of Revolution

    Spinning a flat region around an axis sweeps out a solid. A rectangle spun around a side makes a cylinder, a right triangle spun around a leg makes a cone, and a semicircle spun around its diameter makes a sphere. Identify rr and hh, then use the solid's volume formula.

    e.g. Right triangle with legs 3 and 6, spun around the leg of 6: cone with r=3r = 3, h=6h = 6, V=13⋅9⋅6π=18πV = \tfrac13 \cdot 9 \cdot 6\pi = 18\pi

Unit 11 57 topics

Trigonometry

Introduction to Trigonometry, Radians, The Unit Circle, and more.

11.32 Introduction to 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. 11.32.1

    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. 11.32.2

    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. 11.32.3

    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. 11.32.4

    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. 11.32.5

    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. 11.32.6

    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. 11.32.7

    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. 11.32.8

    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. 11.32.9

    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. 11.32.10

    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
  11. 11.32.11

    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
  12. 11.32.12

    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

11.33 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. 11.33.1

    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. 11.33.2

    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. 11.33.3

    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. 11.33.4

    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

11.34 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. 11.34.1

    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. 11.34.2

    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. 11.34.3

    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. 11.34.4

    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. 11.34.5

    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. 11.34.6

    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. 11.34.7

    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. 11.34.8

    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. 11.34.9

    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. 11.34.10

    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. 11.34.11

    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}

11.35 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. 11.35.1

    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. 11.35.2

    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. 11.35.3

    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. 11.35.4

    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. 11.35.5

    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}

11.36 Graphing Trigonometric Functions

π/2π3π/22π1−1xyy = sin xy = cos xperiod 2πBoth waves repeatevery 2π.−1 ≤ sin x ≤ 1−1 ≤ cos x ≤ 1Cosine is sine shiftedleft by π/2.
Sine starts at 0 and cosine starts at 1, but they are the same wave shifted by π/2. Both repeat every 2π and stay between −1 and 1.
  1. 11.36.1

    Graphing Sine and Cosine

    Both waves have period 2π2\pi and range [−1,1][-1, 1]. Plot the five key points over one period and repeat. Sine starts at the midline going up. Cosine starts at its maximum.

    e.g. sin⁡5π2=sin⁡π2=1\sin\tfrac{5\pi}{2} = \sin\tfrac{\pi}{2} = 1 because the graph repeats every 2π2\pi

    x:  0,  π2,  π,  3π2,  2π\displaystyle x:\; 0,\; \tfrac{\pi}{2},\; \pi,\; \tfrac{3\pi}{2},\; 2\pi
    sin⁡x:  0,  1,  0,  −1,  0\displaystyle \sin x:\; 0,\; 1,\; 0,\; -1,\; 0
    cos⁡x:  1,  0,  −1,  0,  1\displaystyle \cos x:\; 1,\; 0,\; -1,\; 0,\; 1
  2. 11.36.2

    Graphing Tangent and Cotangent

    Both have period π\pi and a vertical asymptote wherever the denominator is 0. Tangent rises left to right between asymptotes. Cotangent falls.

    e.g. tan⁡\tan passes through (−π4,−1)(-\tfrac{\pi}{4}, -1), (0,0)(0, 0), (π4,1)(\tfrac{\pi}{4}, 1)

    tan⁡x=sin⁡xcos⁡x,  cot⁡x=cos⁡xsin⁡x\displaystyle \tan x = \frac{\sin x}{\cos x},\; \cot x = \frac{\cos x}{\sin x}
    tan⁡:  asymptotes x=π2+kπ\displaystyle \tan:\; \text{asymptotes } x = \tfrac{\pi}{2} + k\pi
    cot⁡:  asymptotes x=kπ\displaystyle \cot:\; \text{asymptotes } x = k\pi
  3. 11.36.3

    Graphing Secant and Cosecant

    Sketch cos (for sec) or sin (for csc) first. Draw asymptotes where that curve is 0. Draw U-shaped branches from each maximum and minimum, opening away from the xx-axis. Period 2π2\pi.

    e.g. csc⁡π2=1\csc\tfrac{\pi}{2} = 1: a branch opens up from (π2,1)(\tfrac{\pi}{2}, 1) between asymptotes x=0x = 0 and x=πx = \pi

    sec⁡x=1cos⁡x,  csc⁡x=1sin⁡x\displaystyle \sec x = \frac{1}{\cos x},\; \csc x = \frac{1}{\sin x}

11.37 Properties of Trigonometric Functions

xy1−1x = −π/2x = π/2−ππ0y = tan xtan x = sin x ÷ cos xasymptotes wherecos x = 0zeros where sin x = 0period πEach branch repeatsevery π.
Tangent is sine divided by cosine, so it blows up wherever cosine is 0. Its branches repeat every π, half the period of sine.
  1. 11.37.1

    Describing Properties of the Sine Function

    Sine is odd, so its graph is symmetric about the origin. It increases on (−π2,π2)(-\tfrac{\pi}{2}, \tfrac{\pi}{2}). Here kk is any integer.

    e.g. Zeros of sin⁡x\sin x on [0,2π][0, 2\pi]: x=0,π,2πx = 0, \pi, 2\pi

    Domain R,  range [−1,1]\displaystyle \text{Domain } \mathbb{R},\; \text{range } [-1, 1]
    Period 2π,  zeros x=kπ\displaystyle \text{Period } 2\pi,\; \text{zeros } x = k\pi
    Max 1 at x=π2+2kπ\displaystyle \text{Max } 1 \text{ at } x = \tfrac{\pi}{2} + 2k\pi
    Min −1 at x=3π2+2kπ\displaystyle \text{Min } -1 \text{ at } x = \tfrac{3\pi}{2} + 2k\pi
  2. 11.37.2

    Describing Properties of the Cosine Function

    Cosine is even, so its graph is symmetric about the yy-axis. It decreases on (0,π)(0, \pi). Here kk is any integer.

    e.g. Zeros of cos⁡x\cos x on [0,2π][0, 2\pi]: x=π2,3π2x = \tfrac{\pi}{2}, \tfrac{3\pi}{2}

    Domain R,  range [−1,1]\displaystyle \text{Domain } \mathbb{R},\; \text{range } [-1, 1]
    Period 2π,  zeros x=π2+kπ\displaystyle \text{Period } 2\pi,\; \text{zeros } x = \tfrac{\pi}{2} + k\pi
    Max 1 at x=2kπ\displaystyle \text{Max } 1 \text{ at } x = 2k\pi
    Min −1 at x=π+2kπ\displaystyle \text{Min } -1 \text{ at } x = \pi + 2k\pi
  3. 11.37.3

    Describing Properties of the Tangent Function

    Tangent is odd and increases between each pair of asymptotes. It has no maximum or minimum. Here kk is any integer.

    e.g. On (−π2,π2)(-\tfrac{\pi}{2}, \tfrac{\pi}{2}) the only zero is x=0x = 0

    Domain x≠π2+kπ\displaystyle \text{Domain } x \ne \tfrac{\pi}{2} + k\pi
    Range R,  period π\displaystyle \text{Range } \mathbb{R},\; \text{period } \pi
    Zeros x=kπ\displaystyle \text{Zeros } x = k\pi
  4. 11.37.4

    Describing Properties of the Secant Function

    Secant is even and has no zeros. Its asymptotes are at the zeros of cosine. Here kk is any integer.

    e.g. sec⁡0=1\sec 0 = 1 and sec⁡π=−1\sec\pi = -1

    Domain x≠π2+kπ\displaystyle \text{Domain } x \ne \tfrac{\pi}{2} + k\pi
    Range (−∞,−1]∪[1,∞)\displaystyle \text{Range } (-\infty, -1] \cup [1, \infty)
    Period 2π\displaystyle \text{Period } 2\pi
    Local min 1 at x=2kπ\displaystyle \text{Local min } 1 \text{ at } x = 2k\pi
    Local max −1 at x=π+2kπ\displaystyle \text{Local max } -1 \text{ at } x = \pi + 2k\pi
  5. 11.37.5

    Describing Properties of the Cosecant Function

    Cosecant is odd and has no zeros. Its asymptotes are at the zeros of sine. Here kk is any integer.

    e.g. csc⁡π2=1\csc\tfrac{\pi}{2} = 1 and csc⁡3π2=−1\csc\tfrac{3\pi}{2} = -1

    Domain x≠kπ\displaystyle \text{Domain } x \ne k\pi
    Range (−∞,−1]∪[1,∞)\displaystyle \text{Range } (-\infty, -1] \cup [1, \infty)
    Period 2π\displaystyle \text{Period } 2\pi
    Local min 1 at x=π2+2kπ\displaystyle \text{Local min } 1 \text{ at } x = \tfrac{\pi}{2} + 2k\pi
    Local max −1 at x=3π2+2kπ\displaystyle \text{Local max } -1 \text{ at } x = \tfrac{3\pi}{2} + 2k\pi
  6. 11.37.6

    Describing Properties of the Cotangent Function

    Cotangent is odd and decreases between each pair of asymptotes. It has no maximum or minimum. Here kk is any integer.

    e.g. On (0,π)(0, \pi) the only zero is x=π2x = \tfrac{\pi}{2}

    Domain x≠kπ\displaystyle \text{Domain } x \ne k\pi
    Range R,  period π\displaystyle \text{Range } \mathbb{R},\; \text{period } \pi
    Zeros x=π2+kπ\displaystyle \text{Zeros } x = \tfrac{\pi}{2} + k\pi

11.38 Graph Transformations of Trigonometric Functions

π/2π3π/22π5π/2−1123xmidline y = 1amplitude|A| = 2period 2π/B = 2πy = A sin(B(x − C)) + DAamplitude |A|Bperiod 2π/BCphase shift CDmidline y = DHere A = 2, B = 1,C = 0, D = 1.
A sinusoid is the sine wave stretched, shifted, and lifted. Read the midline first; the amplitude is how far the wave rises above it, and the period is the length of one full cycle.
  1. 11.38.1

    Vertical Translations of Trigonometric Functions

    Adding DD shifts the whole graph up DD units, or down if D<0D < 0. For sine and cosine the midline moves to y=Dy = D.

    e.g. y=cos⁡x−2y = \cos x - 2: midline y=−2y = -2, range [−3,−1][-3, -1]

    y=f(x)+D\displaystyle y = f(x) + D
  2. 11.38.2

    Vertical Stretches of Trigonometric Functions

    Multiplying by AA multiplies every yy-value by AA. For sine and cosine the amplitude is ∣A∣\lvert A \rvert. Tangent, cotangent, secant, and cosecant have no amplitude, but their points still scale.

    e.g. y=3sin⁡xy = 3\sin x: amplitude 3, range [−3,3][-3, 3]; y=2tan⁡xy = 2\tan x passes through (π4,2)(\tfrac{\pi}{4}, 2)

    y=Af(x)\displaystyle y = A f(x)
    amplitude=∣A∣\displaystyle \text{amplitude} = \lvert A \rvert
  3. 11.38.3

    Horizontal Translations of Trigonometric Functions

    Replacing xx with x−Cx - C shifts the graph right CC units, or left if C<0C < 0. This shift is the phase shift.

    e.g. y=cos⁡(x+π3)y = \cos(x + \tfrac{\pi}{3}): shift left π3\tfrac{\pi}{3}, so a maximum is at x=−π3x = -\tfrac{\pi}{3}

    y=f(x−C)\displaystyle y = f(x - C)
  4. 11.38.4

    Horizontal Stretches of Trigonometric Functions

    Replacing xx with BxBx (B>0B > 0) changes the period. B>1B > 1 squeezes the graph and 0<B<10 < B < 1 stretches it.

    e.g. y=sin⁡2xy = \sin 2x has period π\pi; y=cos⁡x2y = \cos\tfrac{x}{2} has period 4π4\pi

    sin⁡,cos⁡,sec⁡,csc⁡:  P=2πB\displaystyle \sin, \cos, \sec, \csc:\; P = \frac{2\pi}{B}
    tan⁡,cot⁡:  P=πB\displaystyle \tan, \cot:\; P = \frac{\pi}{B}
  5. 11.38.5

    Combining Graph Transformations of Sine and Cosine

    Write the function in this form with B>0B > 0, factoring BB out of the parentheses first. Then read off all four features.

    e.g. y=2sin⁡(3x−π)+1=2sin⁡(3(x−π3))+1y = 2\sin(3x - \pi) + 1 = 2\sin(3(x - \tfrac{\pi}{3})) + 1: amplitude 2, period 2π3\tfrac{2\pi}{3}, right π3\tfrac{\pi}{3}, midline y=1y = 1

    y=Asin⁡(B(x−C))+D\displaystyle y = A\sin(B(x - C)) + D
    amplitude ∣A∣,  period 2πB\displaystyle \text{amplitude } \lvert A \rvert,\; \text{period } \frac{2\pi}{B}
    phase shift C,  midline y=D\displaystyle \text{phase shift } C,\; \text{midline } y = D
  6. 11.38.6

    Graph Transformations of Tangent and Cotangent

    The same transformations apply, but the period is πB\tfrac{\pi}{B}. AA is a vertical stretch, not an amplitude. Shifts move the asymptotes too.

    e.g. y=tan⁡2xy = \tan 2x: period π2\tfrac{\pi}{2}, asymptotes x=π4+kπ2x = \tfrac{\pi}{4} + \tfrac{k\pi}{2}

    y=Atan⁡(B(x−C))+D\displaystyle y = A\tan(B(x - C)) + D
    period=πB\displaystyle \text{period} = \frac{\pi}{B}
  7. 11.38.7

    Combining Graph Transformations of Tangent and Cotangent

    Find the asymptotes by setting the inside equal to where the parent is undefined. Tangent's center point moves to (C,D)(C, D), halfway between two asymptotes.

    e.g. y=2tan⁡(x−π4)+1y = 2\tan(x - \tfrac{\pi}{4}) + 1: period π\pi, center (π4,1)(\tfrac{\pi}{4}, 1), asymptotes x=3π4+kπx = \tfrac{3\pi}{4} + k\pi

    tan⁡:  B(x−C)=π2+kπ\displaystyle \tan:\; B(x - C) = \tfrac{\pi}{2} + k\pi
    cot⁡:  B(x−C)=kπ\displaystyle \cot:\; B(x - C) = k\pi
  8. 11.38.8

    Combining Graph Transformations of Secant and Cosecant

    Graph the matching cosine or sine with the same AA, BB, CC, DD. Asymptotes go where that guide curve crosses its midline. Branches start at its maximums and minimums.

    e.g. y=2sec⁡2x+1y = 2\sec 2x + 1: period π\pi, asymptotes x=π4+kπ2x = \tfrac{\pi}{4} + \tfrac{k\pi}{2}, range (−∞,−1]∪[3,∞)(-\infty, -1] \cup [3, \infty)

    y=Asec⁡(B(x−C))+D\displaystyle y = A\sec(B(x - C)) + D
    period=2πB\displaystyle \text{period} = \frac{2\pi}{B}
  9. 11.38.9

    Graphing Reflections of Trigonometric Functions

    A negative AA flips the graph over the xx-axis (over the midline if there is a vertical shift). A negative sign on xx flips it over the yy-axis, and the even and odd rules simplify that.

    e.g. y=−2cos⁡xy = -2\cos x starts at a minimum (0,−2)(0, -2) instead of a maximum

    y=−f(x):  flip over x-axis\displaystyle y = -f(x):\; \text{flip over } x\text{-axis}
    y=f(−x):  flip over y-axis\displaystyle y = f(-x):\; \text{flip over } y\text{-axis}
    sin⁡(−x)=−sin⁡x,  cos⁡(−x)=cos⁡x\displaystyle \sin(-x) = -\sin x,\; \cos(-x) = \cos x
  10. 11.38.10

    Graphing Reflections of Trigonometric Functions: Three or More Transformations

    Rewrite in the form y=Af(B(x−C))+Dy = A f(B(x - C)) + D. Move each key point of the parent graph with the rule below. A negative AA reflects.

    e.g. y=−3sin⁡(2x−π2)+2=−3sin⁡(2(x−π4))+2y = -3\sin(2x - \tfrac{\pi}{2}) + 2 = -3\sin(2(x - \tfrac{\pi}{4})) + 2: reflected, amplitude 3, period π\pi, right π4\tfrac{\pi}{4}, range [−1,5][-1, 5]

    (x,y)→(xB+C,  Ay+D)\displaystyle (x, y) \to \left(\frac{x}{B} + C,\; Ay + D\right)

11.39 Properties of Transformed Trigonometric Functions

  1. 11.39.1

    Properties of Transformed Sine and Cosine Functions

    For y=Asin⁡(B(x−C))+Dy = A\sin(B(x - C)) + D or the cosine version, the domain is all real numbers. The graph swings ∣A∣\lvert A \rvert above and below the midline y=Dy = D.

    e.g. y=4cos⁡(π2x)−1y = 4\cos(\tfrac{\pi}{2}x) - 1: period 2ππ/2=4\tfrac{2\pi}{\pi/2} = 4, range [−5,3][-5, 3]

    max⁡=D+∣A∣,  min⁡=D−∣A∣\displaystyle \max = D + \lvert A \rvert,\; \min = D - \lvert A \rvert
    range [D−∣A∣,  D+∣A∣]\displaystyle \text{range } [D - \lvert A \rvert,\; D + \lvert A \rvert]
    period=2πB\displaystyle \text{period} = \frac{2\pi}{B}
  2. 11.39.2

    Finding Zeros and Extrema of Transformed Sine and Cosine Functions

    Let u=B(x−C)u = B(x - C). For zeros, set y=0y = 0 and solve for uu, then for xx. Extrema occur where the parent hits 1 or −1-1. If A<0A < 0, the maximums and minimums swap.

    e.g. y=2sin⁡2xy = 2\sin 2x: zeros x=kπ2x = \tfrac{k\pi}{2}; max 2 at x=π4+kπx = \tfrac{\pi}{4} + k\pi; min −2-2 at x=3π4+kπx = \tfrac{3\pi}{4} + k\pi

    sin⁡u=1 at u=π2+2kπ\displaystyle \sin u = 1 \text{ at } u = \tfrac{\pi}{2} + 2k\pi
    sin⁡u=−1 at u=3π2+2kπ\displaystyle \sin u = -1 \text{ at } u = \tfrac{3\pi}{2} + 2k\pi
    cos⁡u=1 at u=2kπ\displaystyle \cos u = 1 \text{ at } u = 2k\pi
    cos⁡u=−1 at u=π+2kπ\displaystyle \cos u = -1 \text{ at } u = \pi + 2k\pi
  3. 11.39.3

    Properties of Transformed Tangent and Cotangent Functions

    The range is all real numbers and there are no extrema. The domain leaves out the asymptotes. With D=0D = 0, tangent's zeros are at B(x−C)=kπB(x - C) = k\pi and cotangent's at B(x−C)=π2+kπB(x - C) = \tfrac{\pi}{2} + k\pi.

    e.g. y=3cot⁡x2y = 3\cot\tfrac{x}{2}: period 2π2\pi, asymptotes x=2kπx = 2k\pi, zeros x=π+2kπx = \pi + 2k\pi

    period=πB\displaystyle \text{period} = \frac{\pi}{B}
    tan⁡ asymptotes: B(x−C)=π2+kπ\displaystyle \tan \text{ asymptotes: } B(x - C) = \tfrac{\pi}{2} + k\pi
    cot⁡ asymptotes: B(x−C)=kπ\displaystyle \cot \text{ asymptotes: } B(x - C) = k\pi
  4. 11.39.4

    Properties of Transformed Secant and Cosecant Functions

    The range is shown below. There are zeros only if the vertical shift moves a branch across the xx-axis. Asymptotes sit where the guide cosine or sine is 0: secant at B(x−C)=π2+kπB(x - C) = \tfrac{\pi}{2} + k\pi, cosecant at B(x−C)=kπB(x - C) = k\pi.

    e.g. y=3csc⁡2x+1y = 3\csc 2x + 1: period π\pi, asymptotes x=kπ2x = \tfrac{k\pi}{2}, range (−∞,−2]∪[4,∞)(-\infty, -2] \cup [4, \infty)

    period=2πB\displaystyle \text{period} = \frac{2\pi}{B}
    (−∞,D−∣A∣]∪[D+∣A∣,∞)\displaystyle (-\infty, D - \lvert A \rvert] \cup [D + \lvert A \rvert, \infty)
  5. 11.39.5

    Interpreting Trigonometric Models

    In a real-world model, DD is the average level, ∣A∣\lvert A \rvert is how far it swings above and below that average, the period is the time for one full cycle, and CC tells when a cycle starts.

    e.g. T(t)=15cos⁡(π6(t−7))+60T(t) = 15\cos\left(\tfrac{\pi}{6}(t - 7)\right) + 60 (tt in months): average 60∘60^\circF, swing 15 degrees, period 12 months, high of 75∘75^\circF at t=7t = 7

  6. 11.39.6

    Modeling With Trigonometric Functions

    Get AA and DD from the max and min, and BB from the period. Use cosine if the data starts at a maximum, −cos⁡-\cos if it starts at a minimum, and sine if it starts at the midline going up.

    e.g. Ferris wheel from 5 ft to 45 ft, one turn per 8 min, rider starts at the bottom: h(t)=−20cos⁡(π4t)+25h(t) = -20\cos\left(\tfrac{\pi}{4}t\right) + 25

    A=max⁡−min⁡2\displaystyle A = \frac{\max - \min}{2}
    D=max⁡+min⁡2\displaystyle D = \frac{\max + \min}{2}
    B=2πperiod\displaystyle B = \frac{2\pi}{\text{period}}

Unit 12 43 topics

Probability & Statistics

Introduction to Probability, Compound Events in Probability, Conditional Probability, and more.

12.40 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. 12.40.1

    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. 12.40.2

    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. 12.40.3

    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. 12.40.4

    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. 12.40.5

    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. 12.40.6

    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. 12.40.7

    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. 12.40.8

    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. 12.40.9

    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. 12.40.10

    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}}

12.41 Compound Events in Probability

  1. 12.41.1

    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. 12.41.2

    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. 12.41.3

    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. 12.41.4

    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. 12.41.5

    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. 12.41.6

    Computing Probabilities for Three Events Using Venn Diagrams

    Three circles make 8 regions. Fill from the center out: the triple overlap first, then each pair overlap minus the center, then each "only" region.

    e.g. 40 students: 20 Spanish, 15 French, 10 art; 5 Spanish and French, 4 Spanish and art, 3 French and art, 2 all three. P(at least one)=45−12+240=78P(\text{at least one}) = \tfrac{45 - 12 + 2}{40} = \tfrac78

    P(A∪B∪C)=P(A)+P(B)+P(C)\displaystyle P(A \cup B \cup C) = P(A) + P(B) + P(C)
    −P(A∩B)−P(A∩C)−P(B∩C)\displaystyle - P(A \cap B) - P(A \cap C) - P(B \cap C)
    +P(A∩B∩C)\displaystyle + P(A \cap B \cap C)

12.42 Conditional Probability

3/52/52/42/43/41/4RBRRR 3/5 × 2/4 = 6/20BRB 3/5 × 2/4 = 6/20RBR 2/5 × 3/4 = 6/20BBB 2/5 × 1/4 = 2/20Bag: 3 red,2 blue.Draw 2, noreplacing.Total:20/20 = 1Multiply along a branch, add across branches.P(one of each color) = P(RB) + P(BR) = 6/20 + 6/20 = 12/20 = 3/5
The second-draw branches change because the first marble is not put back. Multiply along a path to get one outcome; add outcomes to combine them.
  1. 12.42.1

    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)}
  2. 12.42.2

    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)}
  3. 12.42.3

    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)
  4. 12.42.4

    The Law of Total Probability

    Split into cases that do not overlap and cover everything, such as BB and B′B'. Find P(A)P(A) in each case and add.

    e.g. 60 percent of days are sunny. You bike on 90 percent of sunny days and 30 percent of others: P(bike)=0.9(0.6)+0.3(0.4)=0.66P(\text{bike}) = 0.9(0.6) + 0.3(0.4) = 0.66

    P(A)=P(A∣B)P(B)\displaystyle P(A) = P(A \mid B)P(B)
    +P(A∣B′)P(B′)\displaystyle \quad + P(A \mid B')P(B')
  5. 12.42.5

    Tree Diagrams for Dependent Events

    Each branch is a conditional probability given the path so far, so later branches change. Multiply along a path for that outcome, and add paths for an event. Branches from one point sum to 1.

    e.g. 4 red and 2 blue, draw 2 without replacement: P(one of each)=46⋅25+26⋅45=1630=815P(\text{one of each}) = \tfrac46 \cdot \tfrac25 + \tfrac26 \cdot \tfrac45 = \tfrac{16}{30} = \tfrac{8}{15}

  6. 12.42.6

    Tree Diagrams for Dependent Events: Applications

    Use a tree for multi-step situations such as medical tests. To reverse a condition, divide the path you want by the sum of all paths that give the observed result.

    e.g. 2 percent have a condition; the test is positive for 90 percent of them and 5 percent of others. P(has it∣+)=0.0180.018+0.049≈0.27P(\text{has it} \mid +) = \tfrac{0.018}{0.018 + 0.049} \approx 0.27

    P(B∣A)=P(B) P(A∣B)P(A)\displaystyle P(B \mid A) = \frac{P(B)\,P(A \mid B)}{P(A)}
  7. 12.42.7

    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)
  8. 12.42.8

    Tree Diagrams for Independent Events

    The branch probabilities repeat at every stage because earlier results do not affect later ones (for example, drawing with replacement). Multiply along each path.

    e.g. Makes 70 percent of free throws, shoots 2: P(exactly one)=0.7(0.3)+0.3(0.7)=0.42P(\text{exactly one}) = 0.7(0.3) + 0.3(0.7) = 0.42

  9. 12.42.9

    The Addition Law of Probability

    For "A or B," add the two probabilities and subtract the overlap so it is not counted twice.

    e.g. One card: P(heart or king)=1352+452−152=413P(\text{heart or king}) = \tfrac{13}{52} + \tfrac{4}{52} - \tfrac{1}{52} = \tfrac{4}{13}

    P(A∪B)=P(A)+P(B)\displaystyle P(A \cup B) = P(A) + P(B)
    −P(A∩B)\displaystyle \quad - P(A \cap B)
  10. 12.42.10

    Applying the Addition Law With Event Complements

    The addition law works with complements too. Use P(A′)=1−P(A)P(A') = 1 - P(A), and "at least one" is 1 minus "neither."

    e.g. P(A)=0.6P(A) = 0.6, P(B)=0.5P(B) = 0.5, P(A∩B)=0.3P(A \cap B) = 0.3: P(A′∩B)=0.2P(A' \cap B) = 0.2, so P(A′∪B)=0.4+0.5−0.2=0.7P(A' \cup B) = 0.4 + 0.5 - 0.2 = 0.7

    P(A′∪B)=P(A′)+P(B)\displaystyle P(A' \cup B) = P(A') + P(B)
    −P(A′∩B)\displaystyle \quad - P(A' \cap B)
    P(A∪B)=1−P(A′∩B′)\displaystyle P(A \cup B) = 1 - P(A' \cap B')
  11. 12.42.11

    Mutually Exclusive Events

    Events that cannot happen together: A∩B=∅A \cap B = \varnothing. The addition law then has no overlap term. Mutually exclusive events with nonzero probabilities are never independent.

    e.g. One die: P(1 or 6)=16+16=13P(1 \text{ or } 6) = \tfrac16 + \tfrac16 = \tfrac13

    P(A∩B)=0\displaystyle P(A \cap B) = 0
    P(A∪B)=P(A)+P(B)\displaystyle P(A \cup B) = P(A) + P(B)

12.43 Combinatorics

  1. 12.43.1

    The Rules of Sum and Product

    Product rule: a task done in steps with mm ways then nn ways can be done mnmn ways. Sum rule: choosing one option from mm choices or nn other choices (no overlap) gives m+nm + n ways.

    e.g. 4 shirts and 3 pants: 4×3=124 \times 3 = 12 outfits. One of 5 movies or 3 games: 5+3=85 + 3 = 8 choices

    steps (and): m×n\displaystyle \text{steps (and): } m \times n
    no overlap (or): m+n\displaystyle \text{no overlap (or): } m + n
  2. 12.43.2

    Factorials

    n!n! is the product of the whole numbers from nn down to 1. By definition 0!=10! = 1.

    e.g. 5!=5⋅4⋅3⋅2⋅1=1205! = 5 \cdot 4 \cdot 3 \cdot 2 \cdot 1 = 120, and 8!6!=8⋅7=56\tfrac{8!}{6!} = 8 \cdot 7 = 56

    n!=n(n−1)(n−2)⋯1\displaystyle n! = n(n-1)(n-2)\cdots 1
    0!=1\displaystyle 0! = 1
  3. 12.43.3

    Factorials in Variable Expressions

    Expand the larger factorial down to the smaller one so they cancel.

    e.g. (n+2)!n!=(n+2)(n+1)=n2+3n+2\tfrac{(n+2)!}{n!} = (n+2)(n+1) = n^2 + 3n + 2

    n!=n(n−1)!\displaystyle n! = n(n-1)!
    (n+1)!(n−1)!=(n+1)n\displaystyle \frac{(n+1)!}{(n-1)!} = (n+1)n
  4. 12.43.4

    Ordering Objects

    nn different objects can be arranged in a row in n!n! ways. If some objects are identical, divide by the factorial of each repeat count.

    e.g. 4 books on a shelf: 4!=244! = 24 orders. Letters of BOOK: 4!2!=12\tfrac{4!}{2!} = 12

    n!\displaystyle n!
    n!a! b!⋯  (repeats)\displaystyle \frac{n!}{a!\,b!\cdots} \;\text{(repeats)}
  5. 12.43.5

    Permutations

    Arrange rr of nn different objects when order matters.

    e.g. President, VP, and treasurer from 10 people: 10P3=10⋅9⋅8=720{}_{10}P_3 = 10 \cdot 9 \cdot 8 = 720

    nPr=n!(n−r)!\displaystyle {}_nP_r = \frac{n!}{(n-r)!}
  6. 12.43.6

    Combinations

    Choose rr of nn different objects when order does not matter. It is the permutation count divided by r!r!.

    e.g. A 3-person committee from 10: (103)=10⋅9⋅83⋅2⋅1=120\binom{10}{3} = \tfrac{10 \cdot 9 \cdot 8}{3 \cdot 2 \cdot 1} = 120

    (nr)=nCr=n!r! (n−r)!\displaystyle \binom{n}{r} = {}_nC_r = \frac{n!}{r!\,(n-r)!}
  7. 12.43.7

    Computing Probabilities Using Combinatorics

    Count the favorable outcomes and the total outcomes with combinations or permutations, then divide.

    e.g. 5 boys and 4 girls, pick 3 at random: P(all girls)=(43)(93)=484=121P(\text{all girls}) = \tfrac{\binom43}{\binom93} = \tfrac{4}{84} = \tfrac{1}{21}

    P=favorable counttotal count\displaystyle P = \frac{\text{favorable count}}{\text{total count}}

12.44 Analyzing 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. 12.44.1

    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. 12.44.2

    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. 12.44.3

    Variance and Standard Deviation

    Variance is the mean of the squared distances from the mean. Standard deviation is its square root, in the data's units. For a sample, divide by n−1n - 1 instead of nn.

    e.g. 2,4,6,82, 4, 6, 8: μ=5\mu = 5, squares 9,1,1,99, 1, 1, 9, σ2=204=5\sigma^2 = \tfrac{20}{4} = 5, σ=5≈2.24\sigma = \sqrt5 \approx 2.24 (sample: s2=203s^2 = \tfrac{20}{3})

    σ2=∑(xi−μ)2n\displaystyle \sigma^2 = \frac{\sum (x_i - \mu)^2}{n}
    σ=σ2\displaystyle \sigma = \sqrt{\sigma^2}
    s2=∑(xi−xˉ)2n−1\displaystyle s^2 = \frac{\sum (x_i - \bar x)^2}{n - 1}
  4. 12.44.4

    Estimating Means and Variances For Grouped Data

    Treat every value in a class as the class midpoint mm, weighted by its frequency ff. The results are estimates.

    e.g. Classes 0 to 10, 10 to 20, 20 to 30 with f=2,3,5f = 2, 3, 5: midpoints 5,15,255, 15, 25, xˉ≈10+45+12510=18\bar x \approx \tfrac{10 + 45 + 125}{10} = 18, σ2≈338+27+24510=61\sigma^2 \approx \tfrac{338 + 27 + 245}{10} = 61

    xˉ≈∑fm∑f\displaystyle \bar x \approx \frac{\sum f m}{\sum f}
    σ2≈∑f(m−xˉ)2∑f\displaystyle \sigma^2 \approx \frac{\sum f (m - \bar x)^2}{\sum f}
  5. 12.44.5

    Covariance

    Measures how two variables move together. Positive means they tend to rise together, negative means one rises as the other falls, and near 0 means no linear pattern. For a sample, divide by n−1n - 1.

    e.g. (1,1),(2,3),(3,5)(1,1), (2,3), (3,5): xˉ=2\bar x = 2, yˉ=3\bar y = 3, products 2,0,22, 0, 2, σxy=43\sigma_{xy} = \tfrac43 (sample: 22)

    σxy=∑(xi−xˉ)(yi−yˉ)n\displaystyle \sigma_{xy} = \frac{\sum (x_i - \bar x)(y_i - \bar y)}{n}
  6. 12.44.6

    Sums of Squares

    SxxS_{xx} and SyyS_{yy} add the squared deviations from the mean; SxyS_{xy} adds the products of paired deviations. The shortcut forms skip computing each deviation. Variance is Sxx/nS_{xx}/n and covariance is Sxy/nS_{xy}/n.

    e.g. x=1,2,3x = 1, 2, 3: Sxx=14−363=2S_{xx} = 14 - \tfrac{36}{3} = 2

    Sxx=∑(x−xˉ)2\displaystyle S_{xx} = \sum (x - \bar x)^2
    =∑x2−(∑x)2n\displaystyle = \sum x^2 - \frac{(\sum x)^2}{n}
    Sxy=∑xy−∑x∑yn\displaystyle S_{xy} = \sum xy - \frac{\sum x \sum y}{n}

12.45 Correlation and Regression

2468123456789xyresidual =actual − predictedŷ = 1.49 + 0.71xleast-squares lineresidual = y − ŷPoints above the line havepositive residuals.The line makes the sum ofsquared residuals smallest.
A residual is the vertical gap between a data point and the fitted line. The least-squares line is the one that makes the squared gaps add up to as little as possible.
  1. 12.45.1

    The Linear Correlation Coefficient

    rr measures the strength and direction of a linear relationship. Near 11 or −1-1 is strong, near 0 is weak or none. Correlation does not prove causation.

    e.g. (1,1),(2,3),(3,2)(1,1), (2,3), (3,2): Sxx=2S_{xx} = 2, Syy=2S_{yy} = 2, Sxy=1S_{xy} = 1, so r=14=0.5r = \tfrac{1}{\sqrt4} = 0.5

    r=SxySxx Syy\displaystyle r = \frac{S_{xy}}{\sqrt{S_{xx}\,S_{yy}}}
    −1≤r≤1\displaystyle -1 \le r \le 1
  2. 12.45.2

    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
  3. 12.45.3

    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.

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