Integrated Math IHonors · 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.

11 units, 29 sections, 226 topics. Press / to search.

Unit 1 25 topics

Equations & Inequalities

Solving for an unknown, modeling with it, and describing ranges of answers.

1.1 Linear Equations

  1. 1.1.1

    Solving Linear Equations With Unknown Coefficients

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

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

    ax+b=c\displaystyle ax + b = c
    ⇒  x=c−ba(a≠0)\displaystyle \Rightarrow\; x = \frac{c - b}{a} \quad (a \ne 0)
  2. 1.1.2

    Solving Linear Equations With Unknown Coefficients by Factoring

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

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

    ax+bx=c\displaystyle ax + bx = c
    ⇒  x(a+b)=c\displaystyle \Rightarrow\; x(a + b) = c
    ⇒  x=ca+b\displaystyle \Rightarrow\; x = \frac{c}{a + b}
  3. 1.1.3

    Solving Linear Inequalities With Unknown Parameters

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

    ax>b  ⇒  {x>baa>0x<baa<0\displaystyle ax > b \;\Rightarrow\; \begin{cases} x > \frac{b}{a} & a > 0 \\[2pt] x < \frac{b}{a} & a < 0 \end{cases}
  4. 1.1.4

    Solving Many-Variable Equations

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

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

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

1.2 Modeling With Linear Equations

  1. 1.2.1

    Interpreting Linear Expressions

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

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

    total=m⏟per unit x+b⏟fixed\displaystyle \text{total} = \underbrace{m}_{\text{per unit}}\,x + \underbrace{b}_{\text{fixed}}
  2. 1.2.2

    Modeling With Linear Equations

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

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

  3. 1.2.3

    Consecutive Integer Problems

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

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

    n+(n+1)+(n+2)=3n+3\displaystyle n + (n + 1) + (n + 2) = 3n + 3
  4. 1.2.4

    Speed, Distance, Time Problems

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

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

    d=s t\displaystyle d = s\,t
  5. 1.2.5

    Further Speed, Distance, Time Problems

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

    t=gaps1−s2  (catching up)\displaystyle t = \frac{\text{gap}}{s_1 - s_2} \;\text{(catching up)}
    t=gaps1+s2  (approaching)\displaystyle t = \frac{\text{gap}}{s_1 + s_2} \;\text{(approaching)}
  6. 1.2.6

    Modeling Work Problems

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

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

    1a+1b=1t\displaystyle \frac{1}{a} + \frac{1}{b} = \frac{1}{t}
  7. 1.2.7

    Modeling Mixture Problems

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

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

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

1.3 Linear Inequalities

−6−5−4−3−2−10123456[−2, 3)−2 ≤ x < 3−6−5−4−3−2−10123456[1, ∞)x ≥ 1−6−5−4−3−2−10123456(−∞, −3) ∪ [2, ∞)x < −3 or x ≥ 2
Closed dot and square bracket: the endpoint is included. Open dot and parenthesis: it is not. Infinity always takes a parenthesis.
  1. 1.3.1

    Solving Compound Inequalities

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

    −1<2x+3<9\displaystyle -1 < 2x + 3 < 9
    ⇒  −4<2x<6\displaystyle \Rightarrow\; -4 < 2x < 6
    ⇒  −2<x<3\displaystyle \Rightarrow\; -2 < x < 3
  2. 1.3.2

    Interval Notation

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

    [a,b]: a≤x≤b\displaystyle [a, b]:\ a \le x \le b
    (a,b): a<x<b\displaystyle (a, b):\ a < x < b
    [a,b): a≤x<b\displaystyle [a, b):\ a \le x < b
  3. 1.3.3

    Unbounded Intervals

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

    x≥2  →  [2,∞)\displaystyle x \ge 2 \;\to\; [2, \infty)
    x<5  →  (−∞,5)\displaystyle x < 5 \;\to\; (-\infty, 5)
    all reals  →  (−∞,∞)\displaystyle \text{all reals} \;\to\; (-\infty, \infty)
  4. 1.3.4

    Unions of Intervals

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

    (−∞,1)∪[4,∞)\displaystyle (-\infty, 1) \cup [4, \infty)
  5. 1.3.5

    Intersections of Intervals

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

    [0,5]∩(3,8]=(3,5]\displaystyle [0, 5] \cap (3, 8] = (3, 5]
  6. 1.3.6

    Compound OR Inequalities

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

    x<−2  or  x≥1\displaystyle x < -2 \;\text{or}\; x \ge 1
    →  (−∞,−2)∪[1,∞)\displaystyle \to\; (-\infty, -2) \cup [1, \infty)
  7. 1.3.7

    Compound AND Inequalities

    Solve each part. The answer is the overlap, and if nothing overlaps there is no solution.

    x>−1  and  x≤4  →  (−1,4]\displaystyle x > -1 \;\text{and}\; x \le 4 \;\to\; (-1, 4]
  8. 1.3.8

    Introduction to Modeling With Inequalities

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

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

  9. 1.3.9

    Modeling With One-Step Inequalities

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

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

  10. 1.3.10

    Modeling With Two-Step Inequalities

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

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

    b+rx≤L\displaystyle b + rx \le L
  11. 1.3.11

    Modeling With Compound Inequalities

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

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

1.4 Nonlinear Equations

  1. 1.4.1

    Solving Equations Using the Square Root Method

    Isolate the square, then take the square root of both sides. Keep the negative root.

    e.g. (x−3)2=16⇒x−3=±4⇒x=7(x - 3)^2 = 16 \Rightarrow x - 3 = \pm 4 \Rightarrow x = 7 or −1-1

    x2=k  ⇒  x=±k(k≥0)\displaystyle x^2 = k \;\Rightarrow\; x = \pm\sqrt{k} \quad (k \ge 0)
  2. 1.4.2

    Solving Equations With Odd Exponents Using the Nth Root Method

    An odd power has exactly one real root, and it can be negative.

    e.g. x3=−64⇒x=−4x^3 = -64 \Rightarrow x = -4

    xn=k, n odd  ⇒  x=kn\displaystyle x^n = k,\ n \text{ odd} \;\Rightarrow\; x = \sqrt[n]{k}
  3. 1.4.3

    Solving Equations With Even Exponents Using the Nth Root Method

    An even power has two real roots when k>0k > 0, one when k=0k = 0, and none when k<0k < 0.

    e.g. x4=81⇒x=±3x^4 = 81 \Rightarrow x = \pm 3

    xn=k, n even, k>0\displaystyle x^n = k,\ n \text{ even},\ k > 0
    ⇒  x=±kn\displaystyle \Rightarrow\; x = \pm\sqrt[n]{k}

Unit 2 32 topics

Two-Variable Equations & Inequalities

Lines, the situations they model, and where they cross.

2.5 Graphs of Linear Equations

xy−2−1123456−4−3−2−1123(0, −2)(4, 0)(2, −1)One line, three formsy = ½x − 2slope-intercept: slope and y-intercepty + 1 = ½(x − 2)point-slope: slope and any pointx − 2y = 4standard: both intercepts quickly
Pick the form by what you know: slope and intercept, slope and a point, or a quick way to both intercepts.
  1. 2.5.1

    Equations of Lines in Slope-Intercept Form

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

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

    y=mx+b\displaystyle y = mx + b
    m=y2−y1x2−x1\displaystyle m = \frac{y_2 - y_1}{x_2 - x_1}
  2. 2.5.2

    Properties of Lines Given in Slope-Intercept Form

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

    x-intercept=−bm\displaystyle x\text{-intercept} = -\frac{b}{m}
  3. 2.5.3

    Equations of Lines in Point-Slope Form

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

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

    y−y1=m(x−x1)\displaystyle y - y_1 = m(x - x_1)
  4. 2.5.4

    Equations of Lines in Standard Form

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

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

    Ax+By=C\displaystyle Ax + By = C
  5. 2.5.5

    Properties of Lines Given in Standard Form

    Read the slope and intercepts straight from the coefficients.

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

2.6 Modeling With Two-Variable Linear Equations

timedistanceslope = speedflat: stoppedheading backDistance–timetimespeedspeeding upflat: steady speedarea = distanceSpeed–time
On a distance–time graph the slope is the speed. On a speed–time graph the slope is the acceleration, and the shaded area is the distance traveled.
  1. 2.6.1

    Modeling With Linear Equations in Two Variables

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

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

  2. 2.6.2

    Modeling Totals Using Two-Variable Linear Equations

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

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

    ax+by=T\displaystyle ax + by = T
  3. 2.6.3

    Analyzing and Interpreting Graphs of Linear Equations

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

  4. 2.6.4

    Further Modeling With Linear Equations in Two Variables

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

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

    m=ΔyΔx\displaystyle m = \frac{\Delta y}{\Delta x}
  5. 2.6.5

    Distance-Time Graphs

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

    speed=slope=ΔdΔt\displaystyle \text{speed} = \text{slope} = \frac{\Delta d}{\Delta t}
  6. 2.6.6

    Speed-Time Graphs

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

    acceleration=ΔvΔt\displaystyle \text{acceleration} = \frac{\Delta v}{\Delta t}
  7. 2.6.7

    Calculating Distance From a Speed-Time Graph

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

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

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

2.7 Systems of Equations

One solutionlines crossNo solutionparallel: 0 = 5Infinitely manysame line: 0 = 0
A system’s solution is where the lines meet. When elimination cancels both variables, the leftover statement tells you which case you have.
  1. 2.7.1

    Introduction to the Elimination Method

    Add or subtract the equations so that one variable cancels.

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

    x+y=10x−y=42x=14\displaystyle \begin{array}{r} x + y = 10 \\ x - y = 4 \\ \hline 2x = 14 \end{array}
  2. 2.7.2

    Solving Systems of Linear Equations Using Elimination: One Transformation

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

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

  3. 2.7.3

    Solving Systems of Linear Equations Using Elimination: Two Transformations

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

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

  4. 2.7.4

    Systems of Linear Equations With Fractional Coefficients

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

    x2+y3=4  →×6  3x+2y=24\displaystyle \tfrac{x}{2} + \tfrac{y}{3} = 4 \;\xrightarrow{\times 6}\; 3x + 2y = 24
  5. 2.7.5

    Systems of Linear Equations With Decimal Coefficients

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

    0.2x+0.5y=1.6  →×10  2x+5y=16\displaystyle 0.2x + 0.5y = 1.6 \;\xrightarrow{\times 10}\; 2x + 5y = 16
  6. 2.7.6

    Systems of Equations With No Solutions and Infinitely Many Solutions

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

  7. 2.7.7

    Consistency and Dependency in Linear Systems

    Consistent: at least one solution. Inconsistent: none. Dependent: infinitely many. Independent: exactly one.

    e.g. One solution is consistent and independent; the same line twice is consistent and dependent

  8. 2.7.8

    Calculating the Intersection of Two Lines

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

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

    m1x+b1=m2x+b2\displaystyle m_1x + b_1 = m_2x + b_2
  9. 2.7.9

    Modeling Using Systems of Linear Equations

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

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

  10. 2.7.10

    Modeling Coin Problems Using Systems of Linear Equations

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

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

    n+d=30\displaystyle n + d = 30
    5n+10d=220\displaystyle 5n + 10d = 220
  11. 2.7.11

    Solving Systems of Nonlinear Equations Using Graphs

    Graph both. Each crossing point is a solution. A line and a parabola cross 0, 1, or 2 times.

  12. 2.7.12

    Approximating Solutions to Systems of Linear Equations

    Read the crossing off a graph, then check it by substituting. A graph reading is an estimate.

  13. 2.7.13

    Approximating Solutions to Systems of Nonlinear Equations

    Use a graph or a table to find where the two sides are closest, then narrow in.

2.8 Two-Variable Linear Inequalities

xy−5−4−3−2−1123456−4−3−2−112345test (0, 0)solutionsy > −½x + 2Test (0, 0): 0 > 2 is false,so shade the other side.Dashed for < and >Solid for ≤ and ≥
Draw the boundary line, decide dashed or solid, then use a test point to pick the side to shade.
  1. 2.8.1

    Graphing Strict Two-Variable Linear Inequalities

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

    y>mx+b\displaystyle y > mx + b
    →  dashed, shade above\displaystyle \to\; \text{dashed, shade above}
  2. 2.8.2

    Graphing Non-Strict Two-Variable Linear Inequalities

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

    y≤mx+b\displaystyle y \le mx + b
    →  solid, shade below\displaystyle \to\; \text{solid, shade below}
  3. 2.8.3

    Further Graphing of Two-Variable Linear Inequalities

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

    2x−3y>6  ⇒  y<23x−2\displaystyle 2x - 3y > 6 \;\Rightarrow\; y < \tfrac{2}{3}x - 2
  4. 2.8.4

    Systems of Linear Inequalities

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

  5. 2.8.5

    Modeling With Two-Variable Linear Inequalities

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

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

  6. 2.8.6

    Modeling With Systems of Linear Inequalities

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

  7. 2.8.7

    Modeling and Solving Systems of Linear Inequalities Using Technology

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

Unit 3 13 topics

Units

Converting measurements, and quantities that vary together.

3.9 Working With Units

60 mi1 h×5,280 ft1 mi×1 h3,600 s=88 ft1 sArrange each fraction so the unit you want gone is on top once and on the bottom once.
A conversion factor equals 1, so multiplying by it changes the units without changing the amount. The struck-through units cancel.
  1. 3.9.1

    Unit Conversions Using Base Units of Mass

    Metric prefixes are powers of ten: kilo is 1,000, centi is 1100\tfrac{1}{100}, milli is 11000\tfrac{1}{1000}. US: 16 oz = 1 lb, 2,000 lb = 1 ton.

    e.g. 3.4 kg=3400 g3.4\text{ kg} = 3400\text{ g}

    1 kg=1000 g\displaystyle 1\text{ kg} = 1000\text{ g}
    1 g=1000 mg\displaystyle 1\text{ g} = 1000\text{ mg}
  2. 3.9.2

    Unit Conversions Using Base Units of Length

    1 km = 1,000 m and 1 m = 100 cm = 1,000 mm. US: 12 in = 1 ft, 3 ft = 1 yd, 5,280 ft = 1 mi.

    e.g. 2.5 km=2500 m2.5\text{ km} = 2500\text{ m}

  3. 3.9.3

    Unit Conversions Using Units of Time

    60 s = 1 min, 60 min = 1 h, 24 h = 1 day, 7 days = 1 week.

    1 h=3600 s\displaystyle 1\text{ h} = 3600\text{ s}
  4. 3.9.4

    Two-Step Unit Conversions

    Multiply by conversion fractions arranged so the unwanted units cancel.

    60 mi1 h⋅5280 ft1 mi⋅1 h3600 s=88 fts\displaystyle \frac{60\text{ mi}}{1\text{ h}} \cdot \frac{5280\text{ ft}}{1\text{ mi}} \cdot \frac{1\text{ h}}{3600\text{ s}} = 88\ \frac{\text{ft}}{\text{s}}
  5. 3.9.5

    Converting Units of Area to Smaller Units

    Square the length factor. Going to a smaller unit, multiply.

    1 m2=1002 cm2=10,000 cm2\displaystyle 1\text{ m}^2 = 100^2\text{ cm}^2 = 10{,}000\text{ cm}^2
  6. 3.9.6

    Converting Units of Area to Larger Units

    Square the length factor and divide.

    5000 cm2=500010,000 m2=0.5 m2\displaystyle 5000\text{ cm}^2 = \frac{5000}{10{,}000}\text{ m}^2 = 0.5\text{ m}^2
  7. 3.9.7

    Converting Between Mixed Units

    Convert everything to the smallest unit, compute, then convert back.

    e.g. 2 h 45 min =165= 165 min; 200 min == 3 h 20 min

  8. 3.9.8

    Determining Units in Formulas

    Units follow the same algebra as the numbers: they multiply and divide.

    m×m=m2\displaystyle \text{m} \times \text{m} = \text{m}^2
    ms÷s=ms2\displaystyle \frac{\text{m}}{\text{s}} \div \text{s} = \frac{\text{m}}{\text{s}^2}
  9. 3.9.9

    Selecting Units for Rates of Change

    A rate’s unit is the yy-unit per xx-unit. Choose a scale that gives sensible numbers.

    e.g. Fingernail growth in mm per week, not km per year

    rate unit=y-unitx-unit\displaystyle \text{rate unit} = \frac{y\text{-unit}}{x\text{-unit}}
  10. 3.9.10

    Degrees of Accuracy

    A measurement rounded to some unit can be off by up to half that unit either way.

    7 cm (to the nearest cm)\displaystyle 7\text{ cm (to the nearest cm)}
    ⇒  6.5≤x<7.5\displaystyle \Rightarrow\; 6.5 \le x < 7.5

3.10 Direct and Inverse Variation

(1, 1)(2, 2)(4, 4)y = kxdouble x, double y(1, 4)(2, 2)(4, 1)y = k/xdouble x, halve y
Direct variation is a line through the origin, with y ÷ x constant. Inverse variation is a curve, with x × y constant.
  1. 3.10.1

    Modeling with Direct Variation

    yy varies directly with xx when y=kxy = kx. Find kk from one pair of values, then use it.

    e.g. y=12y = 12 when x=3x = 3 → k=4k = 4 → at x=5x = 5, y=20y = 20

    y=kx,k=yx\displaystyle y = kx,\quad k = \frac{y}{x}
  2. 3.10.2

    Inverse Variation

    When one quantity doubles, the other halves. Their product stays constant.

    y=kx⇔xy=k\displaystyle y = \frac{k}{x} \quad\Leftrightarrow\quad xy = k
  3. 3.10.3

    Modeling With Inverse Variation

    Find k=xyk = xy from one pair, then y=kxy = \tfrac{k}{x}.

    e.g. 4 workers take 6 days → k=24k = 24 → 8 workers take 3 days

    k=xy\displaystyle k = xy

Unit 4 17 topics

Radicals and Rationals

Roots with variables, and fractions with variables.

4.11 Radical Expressions

na=a1/nindexradicand√(x²) = |x|a square root is nevernegative∛(x³) = xodd roots keep the sign
A root is a fractional power. Even roots need an absolute value when the sign of x is unknown; odd roots do not.
  1. 4.11.1

    Writing Radical Expressions Using Fractional Exponents

    The denominator is the root; the numerator is the power.

    e.g. x3/2=x3x^{3/2} = \sqrt{x^3}

    am/n=amn=(an)m\displaystyle a^{m/n} = \sqrt[n]{a^m} = \left(\sqrt[n]{a}\right)^m
  2. 4.11.2

    The Square Root of a Perfect Square With Algebraic Expressions

    Halve each exponent.

    a2n=an\displaystyle \sqrt{a^{2n}} = a^n
    x2y4=xy2(x≥0)\displaystyle \sqrt{x^2y^4} = xy^2 \quad (x \ge 0)
  3. 4.11.3

    The Square Root of a Perfect Square With Domain Restrictions

    With no sign given, x2\sqrt{x^2} is the distance ∣x∣\lvert x \rvert, because a square root is never negative.

    e.g. (−5)2=5\sqrt{(-5)^2} = 5, not −5-5

    x2=∣x∣\displaystyle \sqrt{x^2} = \lvert x \rvert
    x6=∣x3∣\displaystyle \sqrt{x^6} = \lvert x^3 \rvert
  4. 4.11.4

    The Cube Root of a Perfect Cube With Algebraic Expressions

    Divide each exponent by 3. No absolute value: a cube root keeps the sign.

    x33=x\displaystyle \sqrt[3]{x^3} = x
    −8a63=−2a2\displaystyle \sqrt[3]{-8a^6} = -2a^2
  5. 4.11.5

    Simplifying Square Root Expressions Using the Product Rule

    Split off the largest perfect square, including even powers of the variables.

    ab=a b\displaystyle \sqrt{ab} = \sqrt{a}\,\sqrt{b}
    50x3=25x2⋅2x=5x2x\displaystyle \sqrt{50x^3} = \sqrt{25x^2 \cdot 2x} = 5x\sqrt{2x}
  6. 4.11.6

    Combining Radical Expressions Using the Product Rule

    Multiply the outside numbers together and the insides together, then simplify.

    e.g. 23⋅56=1018=3022\sqrt3 \cdot 5\sqrt6 = 10\sqrt{18} = 30\sqrt2

    ab⋅cd=acbd\displaystyle a\sqrt{b} \cdot c\sqrt{d} = ac\sqrt{bd}
  7. 4.11.7

    Simplifying Square Root Expressions Using the Quotient Rule

    Split the root over top and bottom, or simplify the fraction inside first.

    e.g. 18x32x=9x2=3x\sqrt{\tfrac{18x^3}{2x}} = \sqrt{9x^2} = 3x for x>0x > 0

    ab=ab\displaystyle \sqrt{\frac{a}{b}} = \frac{\sqrt{a}}{\sqrt{b}}
  8. 4.11.8

    Evaluating Algebraic Radical Expressions

    Substitute, simplify everything under the root, then take the root.

    e.g. b2−4ac\sqrt{b^2 - 4ac} at a=1,b=5,c=6a = 1, b = 5, c = 6 → 1=1\sqrt{1} = 1

  9. 4.11.9

    Adding and Subtracting Radical Expressions

    Only like radicals combine: same index, same radicand. Simplify each one first.

    3x+5x=8x\displaystyle 3\sqrt{x} + 5\sqrt{x} = 8\sqrt{x}
    12+27=23+33=53\displaystyle \sqrt{12} + \sqrt{27} = 2\sqrt3 + 3\sqrt3 = 5\sqrt3

4.12 Rational Expressions

  1. 4.12.1

    Equivalent Expressions With Fractions

    Multiply or divide top and bottom by the same nonzero expression.

    ab=akbk(k≠0)\displaystyle \frac{a}{b} = \frac{ak}{bk} \quad (k \ne 0)
  2. 4.12.2

    Simplifying Rational Expressions

    Cancel common factors, never terms. Values that made the original denominator zero stay excluded.

    6x29x=2x3, x≠0\displaystyle \frac{6x^2}{9x} = \frac{2x}{3},\ x \ne 0
    x+2x≠2\displaystyle \frac{x + 2}{x} \ne 2
  3. 4.12.3

    Simplifying Rational Expressions by Factoring

    Factor top and bottom completely, then cancel the shared factors.

    x2−9x2+3x=(x−3)(x+3)x(x+3)=x−3x\displaystyle \frac{x^2 - 9}{x^2 + 3x} = \frac{(x - 3)(x + 3)}{x(x + 3)} = \frac{x - 3}{x}
  4. 4.12.4

    Splitting Rational Expressions Into Separate Terms

    A single denominator can be split under each term on top. The reverse fails: a sum in the denominator can’t be split.

    e.g. 6x2+3x3x=2x+1\tfrac{6x^2 + 3x}{3x} = 2x + 1 for x≠0x \ne 0

    a+bc=ac+bc\displaystyle \frac{a + b}{c} = \frac{a}{c} + \frac{b}{c}
    ca+b≠ca+cb\displaystyle \frac{c}{a + b} \ne \frac{c}{a} + \frac{c}{b}

4.13 Rational Equations

abcd=⟹ad = bcThen check that no denominator is zero.
Cross-multiplying is multiplying both sides by both denominators at once. It only works when each side is a single fraction.
  1. 4.13.1

    Solving Rational Equations Containing One Fractional Term

    Isolate the fraction, then multiply both sides by its denominator. Exclude values that make it zero.

    e.g. 6x+1=4⇒6x=3⇒x=2\tfrac6x + 1 = 4 \Rightarrow \tfrac6x = 3 \Rightarrow x = 2

  2. 4.13.2

    Solving Rational Equations Using Cross-Multiplication

    When one fraction equals another, multiply diagonally.

    ab=cd  ⇒  ad=bc\displaystyle \frac{a}{b} = \frac{c}{d} \;\Rightarrow\; ad = bc
  3. 4.13.3

    Solving Rational Equations Containing Binomials Using Cross-Multiplication

    Cross-multiply, distribute both sides, solve. Check that no denominator becomes zero.

    e.g. x=8x = 8

    x+13=x−22\displaystyle \frac{x + 1}{3} = \frac{x - 2}{2}
    ⇒  2x+2=3x−6\displaystyle \Rightarrow\; 2x + 2 = 3x - 6
  4. 4.13.4

    Solving Rational Equations Using the Flip Method

    If two fractions are equal, their reciprocals are too. Handy when the variable is in a denominator.

    e.g. 3x−1=14⇒x−13=4⇒x=13\tfrac{3}{x - 1} = \tfrac14 \Rightarrow \tfrac{x - 1}{3} = 4 \Rightarrow x = 13

    ab=cd  ⇒  ba=dc\displaystyle \frac{a}{b} = \frac{c}{d} \;\Rightarrow\; \frac{b}{a} = \frac{d}{c}

Unit 5 14 topics

Functions

Rules that turn each input into exactly one output.

5.14 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. 5.14.1

    Introduction to Functions

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

    f(x)=2x+1  ⇒  f(3)=7\displaystyle f(x) = 2x + 1 \;\Rightarrow\; f(3) = 7
  2. 5.14.2

    Visual Representations of Functions

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

  3. 5.14.3

    Graphs of Functions

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

  4. 5.14.4

    The Domain of a Function

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

    f(x)=1x−2: x≠2\displaystyle f(x) = \frac{1}{x - 2}:\ x \ne 2
    g(x)=x+5: x≥−5\displaystyle g(x) = \sqrt{x + 5}:\ x \ge -5
  5. 5.14.5

    The Vertical Line Test

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

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

  6. 5.14.6

    Global Extrema of Functions

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

  7. 5.14.7

    End Behavior of Functions

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

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

  8. 5.14.8

    The Range of a Function

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

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

  9. 5.14.9

    The Range of a Function: Advanced Cases

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

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

  10. 5.14.10

    The Roots of a Function

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

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

    f(x)=0\displaystyle f(x) = 0
  11. 5.14.11

    Increasing and Decreasing Functions

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

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

  12. 5.14.12

    Piecewise Functions

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

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

    f(x)={x+2x<0x2x≥0\displaystyle f(x) = \begin{cases} x + 2 & x < 0 \\ x^2 & x \ge 0 \end{cases}
  13. 5.14.13

    Modeling With Linear Functions

    A constant rate of change means a linear model, f(x)=mx+bf(x) = mx + b.

  14. 5.14.14

    Constructing Linear Functions

    Find the slope from two points, then solve for bb.

    e.g. f(1)=5f(1) = 5, f(3)=11f(3) = 11 → m=3m = 3, f(x)=3x+2f(x) = 3x + 2

    m=f(x2)−f(x1)x2−x1\displaystyle m = \frac{f(x_2) - f(x_1)}{x_2 - x_1}

Unit 6 6 topics

Absolute Value

Distance from zero, in expressions, equations, and inequalities.

6.15 Absolute Value Expressions, Equations & Inequalities

−101234567822|x − 3| < 2between: 1 < x < 5−1012345678|x − 3| ≥ 2outside: x ≤ 1 or x ≥ 5
|x − 3| is the distance from x to 3. Less than means close to 3; greater than means far from it.
  1. 6.15.1

    Absolute Value Expressions

    Absolute value is distance from zero, so it is never negative. Evaluate inside first.

    e.g. ∣3−8∣=5\lvert 3 - 8 \rvert = 5

    ∣x∣={xx≥0−xx<0\displaystyle \lvert x \rvert = \begin{cases} x & x \ge 0 \\ -x & x < 0 \end{cases}
  2. 6.15.2

    Rules of Absolute Value

    It passes through multiplication and division, but not through addition.

    ∣ab∣=∣a∣ ∣b∣\displaystyle \lvert ab \rvert = \lvert a \rvert\,\lvert b \rvert
    ∣ab∣=∣a∣∣b∣\displaystyle \left\lvert \tfrac{a}{b} \right\rvert = \tfrac{\lvert a \rvert}{\lvert b \rvert}
    ∣a+b∣≤∣a∣+∣b∣\displaystyle \lvert a + b \rvert \le \lvert a \rvert + \lvert b \rvert
  3. 6.15.3

    Further Rules of Absolute Value

    A number and its opposite have the same absolute value.

    ∣−a∣=∣a∣\displaystyle \lvert -a \rvert = \lvert a \rvert
    ∣a∣2=a2\displaystyle \lvert a \rvert^2 = a^2
    a2=∣a∣\displaystyle \sqrt{a^2} = \lvert a \rvert
  4. 6.15.4

    Absolute Value Equations

    Isolate the absolute value, then split into two equations. A negative right side has no solution.

    e.g. ∣2x−1∣=7⇒x=4\lvert 2x - 1 \rvert = 7 \Rightarrow x = 4 or −3-3

    ∣A∣=k, k≥0\displaystyle \lvert A \rvert = k,\ k \ge 0
    ⇒  A=k or A=−k\displaystyle \Rightarrow\; A = k \text{ or } A = -k
  5. 6.15.5

    Further Absolute Value Equations

    When two absolute values are equal, the insides are equal or opposite.

    ∣A∣=∣B∣\displaystyle \lvert A \rvert = \lvert B \rvert
    ⇒  A=B or A=−B\displaystyle \Rightarrow\; A = B \text{ or } A = -B
  6. 6.15.6

    Absolute Value Inequalities

    Less than means between, an “and.” Greater than means outside, an “or.”

    ∣A∣<k  ⇒  −k<A<k\displaystyle \lvert A \rvert < k \;\Rightarrow\; -k < A < k
    ∣A∣>k  ⇒  A<−k or A>k\displaystyle \lvert A \rvert > k \;\Rightarrow\; A < -k \text{ or } A > k

Unit 7 21 topics

Exponents

Exponent rules, and quantities that grow or shrink by a fixed factor.

7.16 Rules of Exponents

  1. 7.16.1

    The Product Rule for Exponents With Algebraic Expressions

    Multiply the coefficients, add the exponents of matching bases.

    e.g. 3x2⋅4x5=12x73x^2 \cdot 4x^5 = 12x^7

    am⋅an=am+n\displaystyle a^m \cdot a^n = a^{m+n}
  2. 7.16.2

    The Quotient Rule for Exponents With Algebraic Expressions

    Divide the coefficients, subtract the exponents of matching bases.

    e.g. 10x6y2x2y=5x4\tfrac{10x^6y}{2x^2y} = 5x^4

    aman=am−n\displaystyle \frac{a^m}{a^n} = a^{m-n}
  3. 7.16.3

    The Power Rule for Exponents With Algebraic Expressions

    A power of a power multiplies the exponents.

    e.g. (x3)4=x12(x^3)^4 = x^{12}

    (am)n=amn\displaystyle (a^m)^n = a^{mn}
  4. 7.16.4

    The Power of Product Rule With Algebraic Expressions

    The outside power goes to every factor, including the coefficient and its sign.

    e.g. (−2x3y)2=4x6y2(-2x^3y)^2 = 4x^6y^2

    (ab)n=anbn\displaystyle (ab)^n = a^nb^n
  5. 7.16.5

    The Power of Quotient Rule With Algebraic Expressions

    The outside power goes to the top and the bottom.

    e.g. (x23)3=x627\left(\tfrac{x^2}{3}\right)^3 = \tfrac{x^6}{27}

    (ab)n=anbn\displaystyle \left(\frac{a}{b}\right)^n = \frac{a^n}{b^n}
  6. 7.16.6

    Combining the Rules of Exponents With Algebraic Expressions

    Apply outside powers, combine matching bases, and finish with positive exponents.

    e.g. (2x2)34x−1=8x64x−1=2x7\dfrac{(2x^2)^3}{4x^{-1}} = \dfrac{8x^6}{4x^{-1}} = 2x^7

7.17 Exponential Expressions and Equations

  1. 7.17.1

    Solving Exponential Equations

    Rewrite both sides with the same base, then set the exponents equal.

    e.g. 2x+1=32=25⇒x=42^{x+1} = 32 = 2^5 \Rightarrow x = 4

    bm=bn  ⇒  m=n\displaystyle b^m = b^n \;\Rightarrow\; m = n
  2. 7.17.2

    Solving Exponential Equations with Fractional Solutions

    Use a base that both sides are powers of.

    4x=8  ⇒  22x=23  ⇒  x=32\displaystyle 4^x = 8 \;\Rightarrow\; 2^{2x} = 2^3 \;\Rightarrow\; x = \tfrac{3}{2}
  3. 7.17.3

    Creating Exponential Growth Expressions

    Growth by rate rr multiplies by 1+r1 + r each period.

    e.g. $500 growing 4% a year: 500(1.04)t500(1.04)^t

    a(1+r)t\displaystyle a(1 + r)^t
  4. 7.17.4

    Creating Exponential Decay Expressions

    Decay by rate rr multiplies by 1−r1 - r each period.

    e.g. A $20,000 car losing 15% a year: 20,000(0.85)t20{,}000(0.85)^t

    a(1−r)t\displaystyle a(1 - r)^t

7.18 Exponential Functions

0163248640123456y = 8xy = 2ˣLinear adds:0, 8, 16, 24, 32, 40, 48Exponential multiplies:1, 2, 4, 8, 16, 32, 64Exponential starts behindand still wins.
Equal differences mean linear; equal ratios mean exponential. Any exponential growth eventually passes any linear growth.
  1. 7.18.1

    Exponential Functions

    Starting value aa, multiplied by base bb at each step. Growth if b>1b > 1, decay if 0<b<10 < b < 1.

    f(x)=a bx(a≠0, b>0, b≠1)\displaystyle f(x) = a\,b^x \quad (a \ne 0,\ b > 0,\ b \ne 1)
  2. 7.18.2

    Modeling Exponential Growth With Functions

    Find the starting amount and the growth factor per time unit. For doubling every dd units, use 2t/d2^{t/d}.

    P(t)=P0(1+r)t\displaystyle P(t) = P_0(1 + r)^t
    P(t)=P0⋅2t/d\displaystyle P(t) = P_0 \cdot 2^{t/d}
  3. 7.18.3

    Interpreting Exponential Growth

    In a(1.06)ta(1.06)^t, aa is the starting value and 1.061.06 means 6% growth each period.

    e.g. b=1.25b = 1.25 → 25% growth per period

    r=b−1\displaystyle r = b - 1
  4. 7.18.4

    Solving Exponential Growth Problems

    Substitute tt to find a future value. To find tt, match bases or try values.

    e.g. 3,000 bacteria doubling hourly → after 4 h, 3000⋅24=48,0003000 \cdot 2^4 = 48{,}000

  5. 7.18.5

    Modeling Exponential Decay With Functions

    Use the decay factor per period, or a half-life hh.

    P(t)=P0(1−r)t\displaystyle P(t) = P_0(1 - r)^t
    P(t)=P0(12)t/h\displaystyle P(t) = P_0\left(\tfrac{1}{2}\right)^{t/h}
  6. 7.18.6

    Interpreting Exponential Decay

    b=0.9b = 0.9 means 90% is kept each period, so 10% is lost.

    r=1−b\displaystyle r = 1 - b
  7. 7.18.7

    Solving Exponential Decay Problems

    Count the periods, then apply the factor that many times.

    e.g. 80 mg with a 6 h half-life → after 18 h, 80(12)3=1080\left(\tfrac12\right)^3 = 10 mg

  8. 7.18.8

    Linear vs. Exponential Growth and Decay

    Linear adds the same amount each step. Exponential multiplies by the same factor.

    linear: yn+1−yn=m\displaystyle \text{linear: } y_{n+1} - y_n = m
    exponential: yn+1yn=b\displaystyle \text{exponential: } \frac{y_{n+1}}{y_n} = b
  9. 7.18.9

    Linear vs. Exponential Growth and Decay Models

    In a table, constant differences mean linear and constant ratios mean exponential. Exponential growth eventually passes any linear growth.

    e.g. 3, 6, 12, 24: ratio 2 → exponential

  10. 7.18.10

    Graphing Exponential Growth Functions

    Passes through (0,a)(0, a), rises ever faster to the right, and flattens toward y=0y = 0 on the left without touching it.

    y=a bx, b>1\displaystyle y = a\,b^x,\ b > 1
  11. 7.18.11

    Graphing Exponential Decay Functions

    Passes through (0,a)(0, a) and falls toward y=0y = 0 on the right without reaching it.

    y=a bx, 0<b<1\displaystyle y = a\,b^x,\ 0 < b < 1

Unit 8 20 topics

Polynomials

Building, multiplying, and taking apart expressions in powers of x.

8.19 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. 8.19.1

    Introduction to Polynomials

    A sum of terms axnax^n with whole-number exponents. No variables in a denominator or under a root.

    e.g. 1x\tfrac1x and x\sqrt{x} are not polynomial terms

    3x4−x2+7x−5\displaystyle 3x^4 - x^2 + 7x - 5
  2. 8.19.2

    The Degree of a Polynomial

    The highest exponent. For a term with several variables, add their exponents. Standard form lists terms from highest degree down.

    deg⁡(5x3−2x+1)=3\displaystyle \deg(5x^3 - 2x + 1) = 3
    deg⁡(4x2y3)=5\displaystyle \deg(4x^2y^3) = 5
  3. 8.19.3

    Simplifying Polynomials

    Combine like terms: same variables raised to the same powers.

    3x2+5x−x2+2x=2x2+7x\displaystyle 3x^2 + 5x - x^2 + 2x = 2x^2 + 7x
  4. 8.19.4

    The Distributive Law for Polynomials

    Multiply the outside term by every term inside.

    2x(x2−3x+4)=2x3−6x2+8x\displaystyle 2x(x^2 - 3x + 4) = 2x^3 - 6x^2 + 8x
  5. 8.19.5

    Adding and Subtracting Polynomials

    Combine like terms. When subtracting, flip the sign of every term in the second polynomial.

    (4x2+3x)−(x2−5x)=3x2+8x\displaystyle (4x^2 + 3x) - (x^2 - 5x) = 3x^2 + 8x
  6. 8.19.6

    Monomials, Binomials and Trinomials

    One term, two terms, three terms.

    7x3x+4x2−5x+6\displaystyle 7x^3 \qquad x + 4 \qquad x^2 - 5x + 6
  7. 8.19.7

    Multiplying Binomials

    Every term times every term: First, Outer, Inner, Last.

    (a+b)(c+d)=ac+ad+bc+bd\displaystyle (a + b)(c + d) = ac + ad + bc + bd
    (x+3)(x−5)=x2−2x−15\displaystyle (x + 3)(x - 5) = x^2 - 2x - 15
  8. 8.19.8

    Multiplying Polynomials

    Multiply each term of the first by each term of the second, then combine like terms.

    (x+2)(x2−x+3)\displaystyle (x + 2)(x^2 - x + 3)
    =x3+x2+x+6\displaystyle = x^3 + x^2 + x + 6
  9. 8.19.9

    Squaring Binomials

    Square, twice the product, square. The middle term is the one people forget.

    e.g. (x+4)2=x2+8x+16(x + 4)^2 = x^2 + 8x + 16, not x2+16x^2 + 16

    (a+b)2=a2+2ab+b2\displaystyle (a + b)^2 = a^2 + 2ab + b^2
    (a−b)2=a2−2ab+b2\displaystyle (a - b)^2 = a^2 - 2ab + b^2
  10. 8.19.10

    Expanding Binomials Using Pascal's Triangle

    Row nn gives the coefficients of (a+b)n(a + b)^n; each entry is the sum of the two above it. Powers of aa fall as powers of bb rise.

    e.g. Rows: 1 · 1 1 · 1 2 1 · 1 3 3 1 · 1 4 6 4 1

    (a+b)3=a3+3a2b+3ab2+b3\displaystyle (a + b)^3 = a^3 + 3a^2b + 3ab^2 + b^3
  11. 8.19.11

    The Difference of Squares Formula

    The middle terms cancel.

    e.g. (x+7)(x−7)=x2−49(x + 7)(x - 7) = x^2 - 49

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

8.20 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. 8.20.1

    The Greatest Common Factor of Two Monomials

    GCF of the coefficients, times each shared variable at its lowest power.

    GCF(12x3y, 18x2y4)=6x2y\displaystyle \text{GCF}(12x^3y,\ 18x^2y^4) = 6x^2y
  2. 8.20.2

    Factoring Polynomials Using GCFs

    Always look for a common factor first.

    6x3−9x2=3x2(2x−3)\displaystyle 6x^3 - 9x^2 = 3x^2(2x - 3)
  3. 8.20.3

    Factoring Perfect Square Trinomials

    First and last terms are squares and the middle is twice their product.

    a2+2ab+b2=(a+b)2\displaystyle a^2 + 2ab + b^2 = (a + b)^2
    x2−10x+25=(x−5)2\displaystyle x^2 - 10x + 25 = (x - 5)^2
  4. 8.20.4

    Factoring Perfect Square Trinomials With Leading Coefficients

    The same test, with a coefficient on the first term.

    4x2+12x+9=(2x+3)2\displaystyle 4x^2 + 12x + 9 = (2x + 3)^2
  5. 8.20.5

    Factoring Differences of Squares

    Two squares with a minus between them.

    e.g. A sum of squares a2+b2a^2 + b^2 doesn’t factor

    a2−b2=(a+b)(a−b)\displaystyle a^2 - b^2 = (a + b)(a - b)
    9x2−16=(3x+4)(3x−4)\displaystyle 9x^2 - 16 = (3x + 4)(3x - 4)
  6. 8.20.6

    Factoring Trinomials

    For x2+bx+cx^2 + bx + c, find two numbers that multiply to cc and add to bb.

    e.g. x2+7x+12=(x+3)(x+4)x^2 + 7x + 12 = (x + 3)(x + 4)

    x2+bx+c=(x+p)(x+q)\displaystyle x^2 + bx + c = (x + p)(x + q)
    pq=c,p+q=b\displaystyle pq = c,\quad p + q = b
  7. 8.20.7

    Factoring Trinomials Using Common Factors

    Pull out the GCF first, then factor what is left.

    2x2−8x−24=2(x2−4x−12)\displaystyle 2x^2 - 8x - 24 = 2(x^2 - 4x - 12)
    =2(x−6)(x+2)\displaystyle = 2(x - 6)(x + 2)
  8. 8.20.8

    Factoring Trinomials With Leading Coefficients

    For ax2+bx+cax^2 + bx + c, find two numbers that multiply to acac and add to bb. Split the middle term and factor by grouping.

    e.g. 2x2+7x+32x^2 + 7x + 3: ac=6ac = 6 → 6 and 1 → 2x2+6x+x+3=(2x+1)(x+3)2x^2 + 6x + x + 3 = (2x + 1)(x + 3)

  9. 8.20.9

    Further Factoring Trinomials With Leading Coefficients

    With a negative leading coefficient, factor out −1-1 first. Check by multiplying back.

    e.g. −3x2+x+2=−(3x2−x−2)=−(3x+2)(x−1)-3x^2 + x + 2 = -(3x^2 - x - 2) = -(3x + 2)(x - 1)

Unit 9 12 topics

Sequences

Ordered lists built by a rule, especially adding the same amount each time.

9.21 Introduction to Sequences

  1. 9.21.1

    Introduction to Sequences

    An ordered list of terms. ana_n is the nnth term. An explicit formula gives any term straight from nn.

    an=n2  ⇒  1,4,9,16,…\displaystyle a_n = n^2 \;\Rightarrow\; 1, 4, 9, 16, \ldots
  2. 9.21.2

    Recursive Sequences

    Each term is built from the one before, starting from a given first term.

    e.g. 3, 7, 15, 31, …

    a1=3,an=2an−1+1\displaystyle a_1 = 3,\quad a_n = 2a_{n-1} + 1
  3. 9.21.3

    Fibonacci Sequences

    Each term is the sum of the two before it.

    e.g. 1, 1, 2, 3, 5, 8, 13, …

    Fn=Fn−1+Fn−2,F1=F2=1\displaystyle F_n = F_{n-1} + F_{n-2},\quad F_1 = F_2 = 1

9.22 Arithmetic Sequences

  1. 9.22.1

    Arithmetic Sequences

    Add the same common difference dd each time.

    e.g. 5, 8, 11, 14: d=3d = 3

    d=an+1−an\displaystyle d = a_{n+1} - a_n
  2. 9.22.2

    Recursive Formulas for Arithmetic Sequences

    Give the first term and the rule for the next.

    a1=first term,an=an−1+d\displaystyle a_1 = \text{first term},\quad a_n = a_{n-1} + d
  3. 9.22.3

    The Nth Term of an Arithmetic Sequence

    Start at a1a_1 and take n−1n - 1 steps of dd.

    e.g. 5, 8, 11, … → a20=5+19⋅3=62a_{20} = 5 + 19 \cdot 3 = 62

    an=a1+(n−1)d\displaystyle a_n = a_1 + (n - 1)d
  4. 9.22.4

    Translating Between Explicit and Recursive Formulas for Arithmetic Sequences

    Both use the same a1a_1 and dd.

    an=an−1+d\displaystyle a_n = a_{n-1} + d
    ↔  an=a1+(n−1)d\displaystyle \leftrightarrow\; a_n = a_1 + (n - 1)d
  5. 9.22.5

    Finding the Common Difference of an Arithmetic Sequence

    Subtract any term from the next. From two terms further apart, divide the gap by the number of steps.

    d=am−akm−k\displaystyle d = \frac{a_m - a_k}{m - k}
  6. 9.22.6

    Finding the Nth Term of an Arithmetic Sequence Given Two Terms

    Find dd, step back to a1a_1, then write the formula.

    e.g. a3=10a_3 = 10, a7=22a_7 = 22 → d=3d = 3, a1=4a_1 = 4, an=3n+1a_n = 3n + 1

  7. 9.22.7

    Determining Indexes of Terms in Arithmetic Sequences

    Set the formula equal to the value and solve for nn. If nn isn’t a positive whole number, the value isn’t in the sequence.

    e.g. Is 100 in an=3n+1a_n = 3n + 1? n=33n = 33, yes

  8. 9.22.8

    Solving for Variables in Arithmetic Sequences

    Three terms in a row are arithmetic when the middle one is the average of the other two.

    e.g. x, 2x+1, 5x−3x,\ 2x + 1,\ 5x - 3 → 2(2x+1)=6x−32(2x + 1) = 6x - 3 → x=52x = \tfrac52

    b=a+c2\displaystyle b = \frac{a + c}{2}
  9. 9.22.9

    Modeling With Arithmetic Sequences

    A fixed amount added per step is arithmetic. Check whether counting starts at n=0n = 0 or n=1n = 1.

    e.g. 20 seats in row 1, 2 more per row → row 15 has 20+14⋅2=4820 + 14 \cdot 2 = 48

Unit 10 60 topics

Geometry

Angle proofs, congruent triangles, transformations, right triangles, circles, and coordinates.

10.23 Geometric Proofs

ℓmt12345678When ℓ ∥ m:Corresponding angles: congruent1 & 5, 2 & 6, 3 & 7, 4 & 8Alternate interior: congruent3 & 6, 4 & 5Consecutive interior: sum to 180°3 & 5, 4 & 6Vertical angles: congruent1 & 4, 2 & 3, 5 & 8, 6 & 7
The angle numbers used in the proofs below. Highlighted: 4 and 5, a pair of alternate interior angles.
  1. 10.23.1

    Identifying Angle Postulates

    A postulate is accepted without proof and used as a starting point. The ones used most: angle addition, linear pairs, and corresponding angles.

    e.g. A proof is a list of statements, each with a reason: given, a definition, a postulate, or a theorem already proved

    m∠ABD=m∠ABC+m∠CBD\displaystyle m\angle ABD = m\angle ABC + m\angle CBD
    linear pair: m∠1+m∠2=180∘\displaystyle \text{linear pair: } m\angle 1 + m\angle 2 = 180^\circ
    ℓ∥m  ⇒  corresponding angles≅\displaystyle \ell \parallel m \;\Rightarrow\; \text{corresponding angles} \cong
  2. 10.23.2

    Identifying Angle Theorems

    A theorem is proved from postulates and earlier theorems. Vertical angles are congruent. With parallel lines, alternate angles are congruent and consecutive interior angles are supplementary. Complements or supplements of congruent angles are congruent.

    e.g. In the diagram: ∠1≅∠4\angle 1 \cong \angle 4 (vertical), ∠4≅∠5\angle 4 \cong \angle 5 (alternate interior)

  3. 10.23.3

    Proving Alternate Angle Theorems

    To prove alternate interior angles congruent when the lines are parallel, go through a corresponding pair and a vertical pair, then chain them.

    ∠4≅∠8corresponding angles\displaystyle \angle 4 \cong \angle 8 \quad \text{corresponding angles}
    ∠8≅∠5vertical angles\displaystyle \angle 8 \cong \angle 5 \quad \text{vertical angles}
    ∴ ∠4≅∠5transitive property\displaystyle \therefore\ \angle 4 \cong \angle 5 \quad \text{transitive property}
  4. 10.23.4

    Further Proving Alternate Angle Theorems

    The converse: if alternate angles are congruent, the lines are parallel. Turn the alternate pair into a corresponding pair using vertical angles, then use the converse of the corresponding angles postulate.

    ∠4≅∠5  ⇒  ℓ∥m\displaystyle \angle 4 \cong \angle 5 \;\Rightarrow\; \ell \parallel m
  5. 10.23.5

    Proving Consecutive Angle Theorems

    To prove consecutive interior angles supplementary when the lines are parallel, combine a corresponding pair with a linear pair and substitute.

    ∠4≅∠8corresponding angles\displaystyle \angle 4 \cong \angle 8 \quad \text{corresponding angles}
    m∠6+m∠8=180∘linear pair\displaystyle m\angle 6 + m\angle 8 = 180^\circ \quad \text{linear pair}
    ∴ m∠6+m∠4=180∘substitution\displaystyle \therefore\ m\angle 6 + m\angle 4 = 180^\circ \quad \text{substitution}
  6. 10.23.6

    Further Proving Consecutive Angle Theorems

    The converse: if consecutive interior angles are supplementary, the lines are parallel. Use a linear pair to show a corresponding pair is congruent.

    m∠4+m∠6=180∘  ⇒  ℓ∥m\displaystyle m\angle 4 + m\angle 6 = 180^\circ \;\Rightarrow\; \ell \parallel m
  7. 10.23.7

    Proving Perpendicular Line Theorems

    If two lines form a linear pair of congruent angles, each angle is 90°, so the lines are perpendicular. If two lines meet at one right angle, all four angles are right angles.

    x+x=180∘  ⇒  x=90∘\displaystyle x + x = 180^\circ \;\Rightarrow\; x = 90^\circ
  8. 10.23.8

    Further Proving Perpendicular Line Theorems

    A line perpendicular to one of two parallel lines is perpendicular to the other. Two lines perpendicular to the same line are parallel. Both follow from corresponding angles.

    t⊥ℓ, ℓ∥m  ⇒  t⊥m\displaystyle t \perp \ell,\ \ell \parallel m \;\Rightarrow\; t \perp m
    ℓ⊥t, m⊥t  ⇒  ℓ∥m\displaystyle \ell \perp t,\ m \perp t \;\Rightarrow\; \ell \parallel m

10.24 Geometric Transformations

TranslateslideReflectflipRotateturnDilatescale
Dashed: the original. Solid: the image. Translations, reflections, and rotations keep size and shape. A dilation keeps the shape and changes the size. A reflection reverses orientation.
  1. 10.24.1

    Translations of Geometric Figures

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

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

    (x,y)→(x+a, y+b)\displaystyle (x, y) \to (x + a,\ y + b)
  2. 10.24.2

    Rotations of Geometric Figures

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

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

  3. 10.24.3

    Rotating Objects in the Coordinate Plane Using Functions

    Counterclockwise rotations about the origin.

    e.g. (3,1)(3, 1) rotated 90° → (−1,3)(-1, 3)

    90∘: (x,y)→(−y, x)\displaystyle 90^\circ:\ (x, y) \to (-y,\ x)
    180∘: (x,y)→(−x, −y)\displaystyle 180^\circ:\ (x, y) \to (-x,\ -y)
    270∘: (x,y)→(y, −x)\displaystyle 270^\circ:\ (x, y) \to (y,\ -x)
  4. 10.24.4

    Reflections of Geometric Figures in the Cartesian Plane

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

    x-axis: (x,y)→(x, −y)\displaystyle x\text{-axis}:\ (x, y) \to (x,\ -y)
    y-axis: (x,y)→(−x, y)\displaystyle y\text{-axis}:\ (x, y) \to (-x,\ y)
    y=x: (x,y)→(y, x)\displaystyle y = x:\ (x, y) \to (y,\ x)
  5. 10.24.5

    Reflections of Figures Across Arbitrary Lines

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

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

    x=k: (x,y)→(2k−x, y)\displaystyle x = k:\ (x, y) \to (2k - x,\ y)
    y=k: (x,y)→(x, 2k−y)\displaystyle y = k:\ (x, y) \to (x,\ 2k - y)
  6. 10.24.6

    Dilations of Geometric Figures

    Scale every distance from a center by a factor kk. k>1k > 1 enlarges, 0<k<10 < k < 1 shrinks. Angles stay the same; lengths multiply by kk and areas by k2k^2.

    new length=k×old\displaystyle \text{new length} = k \times \text{old}
    new area=k2×old\displaystyle \text{new area} = k^2 \times \text{old}
  7. 10.24.7

    Dilations of Figures in the Coordinate Plane

    Centered at the origin, multiply both coordinates by kk. From another center, scale each point’s offset from that center.

    e.g. Dilate (2,−3)(2, -3) by 3 about the origin → (6,−9)(6, -9)

    (x,y)→(kx, ky)\displaystyle (x, y) \to (kx,\ ky)
    about (a,b): x′=a+k(x−a)\displaystyle \text{about } (a, b):\ x' = a + k(x - a)
    about (a,b): y′=b+k(y−b)\displaystyle \phantom{\text{about } (a, b):\ } y' = b + k(y - b)
  8. 10.24.8

    Stretches of Geometric Figures

    Scale in one direction only, so the shape changes: a square becomes a rectangle, a circle an oval.

    horizontal by k: (x,y)→(kx, y)\displaystyle \text{horizontal by } k:\ (x, y) \to (kx,\ y)
    vertical by k: (x,y)→(x, ky)\displaystyle \text{vertical by } k:\ (x, y) \to (x,\ ky)
  9. 10.24.9

    Combining Stretches of Geometric Figures

    Stretching by aa horizontally and bb vertically multiplies areas by abab. Equal stretches make a dilation.

    (x,y)→(ax, by)\displaystyle (x, y) \to (ax,\ by)
    area×ab\displaystyle \text{area} \times ab
  10. 10.24.10

    Combining Geometric Transformations

    Apply them in order; the order usually matters. Translations, rotations, and reflections keep size and shape (congruence). Add a dilation and only the shape is kept (similarity).

    e.g. Translate right 2, then reflect in the yy-axis: (1,1)→(3,1)→(−3,1)(1, 1) \to (3, 1) \to (-3, 1). In the other order it ends at (1,1)(1, 1)

  11. 10.24.11

    Reflective Symmetry

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

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

  12. 10.24.12

    Rotational Symmetry

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

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

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

10.25 Congruence

SSSthree sidesSASangle between sidesASAside between anglesAASside not betweenHLright triangles only
Thick sides and shaded angles are the parts that must match. Any one of these five is enough to prove two triangles congruent. SSA and AAA are not.
  1. 10.25.1

    The ASA Congruence Criterion

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

    ∠A≅∠D,AB‾≅DE‾,∠B≅∠E\displaystyle \angle A \cong \angle D,\quad \overline{AB} \cong \overline{DE},\quad \angle B \cong \angle E
    ⇒  △ABC≅△DEF\displaystyle \Rightarrow\; \triangle ABC \cong \triangle DEF
  2. 10.25.2

    The AAS Congruence Criterion

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

  3. 10.25.3

    The SAS Congruence Criterion

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

    AB‾≅DE‾,∠A≅∠D,AC‾≅DF‾\displaystyle \overline{AB} \cong \overline{DE},\quad \angle A \cong \angle D,\quad \overline{AC} \cong \overline{DF}
  4. 10.25.4

    The SSS Congruence Criterion

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

  5. 10.25.5

    The HL Congruence Criterion

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

  6. 10.25.6

    Combining Congruence Criteria for Triangles

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

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

  7. 10.25.7

    Rigid Motions and Congruence

    Two figures are congruent exactly when some sequence of translations, rotations, and reflections maps one onto the other. Then every matching part is congruent (CPCTC: corresponding parts of congruent triangles are congruent).

  8. 10.25.8

    Properties of Congruence

    Congruence is reflexive, symmetric, and transitive.

    reflexive: F≅F\displaystyle \text{reflexive: } F \cong F
    symmetric: F≅G  ⇒  G≅F\displaystyle \text{symmetric: } F \cong G \;\Rightarrow\; G \cong F
    transitive: F≅G, G≅H  ⇒  F≅H\displaystyle \text{transitive: } F \cong G,\ G \cong H \;\Rightarrow\; F \cong H
  9. 10.25.9

    Proving Congruence Statements

    Give each step a reason: the givens, the deduced facts, then the criterion. Vertex order matters: △ABC≅△DEF\triangle ABC \cong \triangle DEF pairs AA with DD, BB with EE, and CC with FF. Once the triangles are congruent, CPCTC gives any matching part.

10.26 Triangles

11√245°45°45°–45°–90°1√3230°60°30°–60°–90°a² + b² = c²for every right triangleScale the sides byany factor: theratios stay the same.
Memorize these two shapes. Any 45°–45°–90° triangle has sides in the ratio 1 : 1 : √2; any 30°–60°–90° triangle, 1 : √3 : 2. The hypotenuse is always the longest side.
  1. 10.26.1

    The Pythagorean Theorem

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

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

    a2+b2=c2\displaystyle a^2 + b^2 = c^2
  2. 10.26.2

    Isosceles Right Triangles

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

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

    s:s:s2\displaystyle s : s : s\sqrt{2}
  3. 10.26.3

    30-60-90 Triangles

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

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

    s:s3:2s\displaystyle s : s\sqrt{3} : 2s
  4. 10.26.4

    The Area of an Isosceles Right Triangle

    The two legs are the base and the height.

    e.g. Leg 6 → A=18A = 18

    A=12s2\displaystyle A = \tfrac{1}{2}s^2
    A=14h2   from the hypotenuse h\displaystyle A = \tfrac{1}{4}h^2 \;\text{ from the hypotenuse } h
  5. 10.26.5

    The Area of a 30-60-90 Triangle

    The two legs are the base and the height.

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

    A=12⋅s⋅s3=32s2\displaystyle A = \tfrac{1}{2} \cdot s \cdot s\sqrt{3} = \frac{\sqrt{3}}{2}s^2
  6. 10.26.6

    The Area of an Equilateral Triangle

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

    e.g. Side 6 → A=93A = 9\sqrt3

    h=32s\displaystyle h = \frac{\sqrt{3}}{2}s
    A=34s2\displaystyle A = \frac{\sqrt{3}}{4}s^2
  7. 10.26.7

    Diagonals of Squares

    A diagonal cuts a square into two isosceles right triangles.

    e.g. Side 7 → diagonal 727\sqrt2

    d=s2\displaystyle d = s\sqrt{2}
    A=12d2\displaystyle A = \tfrac{1}{2}d^2
  8. 10.26.8

    Medians and Centroids of Triangles

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

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

    G=(x1+x2+x33, y1+y2+y33)\displaystyle G = \left(\frac{x_1 + x_2 + x_3}{3},\ \frac{y_1 + y_2 + y_3}{3}\right)
  9. 10.26.9

    The Exterior Angle Theorem

    An exterior angle of a triangle equals the sum of the two interior angles not next to it.

    e.g. Interior angles 50° and 65° → the exterior angle at the third vertex is 115°

    d=a+b\displaystyle d = a + b

10.27 Circles

θrsectorarcchordsegmentC = 2πrcircumferenceA = πr²areaL = (θ/360°) · 2πrarc lengthA = (θ/360°) · πr²sector areaA sector is the fraction θ/360° of the whole circle.
An arc is part of the edge, a sector is a slice, and a segment is cut off by a chord. Arc length and sector area are the same fraction, θ/360°, of the whole.
  1. 10.27.1

    Circles

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

    d=2r\displaystyle d = 2r
  2. 10.27.2

    Arcs, Segments, and Sectors of Circles

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

  3. 10.27.3

    The Circumference of a Circle

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

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

    C=2πr=πd\displaystyle C = 2\pi r = \pi d
  4. 10.27.4

    Areas of Circles

    Square the radius, not the diameter.

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

    A=πr2\displaystyle A = \pi r^2
  5. 10.27.5

    Central Angles and Arcs

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

    arc measure=central angle\displaystyle \text{arc measure} = \text{central angle}
    whole circle=360∘\displaystyle \text{whole circle} = 360^\circ
  6. 10.27.6

    Calculating Arc Lengths of Circular Sectors

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

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

    L=θ360∘⋅2πr\displaystyle L = \frac{\theta}{360^\circ} \cdot 2\pi r
  7. 10.27.7

    Calculating Areas of Circular Sectors

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

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

    A=θ360∘⋅πr2\displaystyle A = \frac{\theta}{360^\circ} \cdot \pi r^2
  8. 10.27.8

    Further Calculating Areas of Sectors

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

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

    A=12rL\displaystyle A = \tfrac{1}{2}rL
  9. 10.27.9

    Problem Solving With Circles

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

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

    Asegment=Asector−Atriangle\displaystyle A_{\text{segment}} = A_{\text{sector}} - A_{\text{triangle}}
  10. 10.27.10

    Circles Inscribed in Squares

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

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

    d=s,r=s2\displaystyle d = s,\quad r = \tfrac{s}{2}
    Acircle=π4s2\displaystyle A_{\text{circle}} = \frac{\pi}{4}s^2
  11. 10.27.11

    Squares Inscribed in Circles

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

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

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

10.28 Coordinate Geometry

2468246810A(1, 1)B(7, 9)M(4, 5)Δx = 6Δy = 8d = √(Δx² + Δy²)= √(36 + 64) = 10M = average of the coordinates= ((1 + 7)/2, (1 + 9)/2) = (4, 5)slope = Δy/Δx = 8/6 = 4/3perpendicular slope = −3/4
The changes in x and y form a right triangle, so distance comes from the Pythagorean theorem. The midpoint averages the endpoints.
  1. 10.28.1

    Parallel Lines in the Coordinate Plane

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

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

    m1=m2\displaystyle m_1 = m_2
  2. 10.28.2

    Finding Equations of Parallel Lines

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

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

    y−y1=m(x−x1)\displaystyle y - y_1 = m(x - x_1)
  3. 10.28.3

    Perpendicular Lines in the Coordinate Plane

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

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

    m1m2=−1\displaystyle m_1 m_2 = -1
    m2=−1m1\displaystyle m_2 = -\frac{1}{m_1}
  4. 10.28.4

    Finding Equations of Perpendicular Lines

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

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

    y−y1=−1m(x−x1)\displaystyle y - y_1 = -\frac{1}{m}(x - x_1)
  5. 10.28.5

    Midpoints in the Coordinate Plane

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

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

    M=(x1+x22, y1+y22)\displaystyle M = \left(\frac{x_1 + x_2}{2},\ \frac{y_1 + y_2}{2}\right)
  6. 10.28.6

    Partitioning Line Segments

    The point a fraction tt of the way from AA to BB adds that fraction of each change. A ratio m:nm : n means t=mm+nt = \tfrac{m}{m + n}.

    e.g. A(1,2)A(1, 2) to B(7,11)B(7, 11) in ratio 1:21 : 2 → t=13t = \tfrac13 → (3,5)(3, 5)

    P=(x1+t(x2−x1), y1+t(y2−y1))\displaystyle P = \big(x_1 + t(x_2 - x_1),\ y_1 + t(y_2 - y_1)\big)
  7. 10.28.7

    The Distance Formula

    The Pythagorean theorem applied to the horizontal and vertical changes.

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

    d=(x2−x1)2+(y2−y1)2\displaystyle d = \sqrt{(x_2 - x_1)^2 + (y_2 - y_1)^2}
  8. 10.28.8

    The Shortest Distance Between a Point and a Line

    Measure along the perpendicular: find the perpendicular through the point, intersect it with the line, then use the distance formula. For a line Ax+By+C=0Ax + By + C = 0 there is a shortcut.

    e.g. (0,0)(0, 0) to 3x+4y−10=03x + 4y - 10 = 0 → 105=2\tfrac{10}{5} = 2

    d=∣Ax0+By0+C∣A2+B2\displaystyle d = \frac{\lvert Ax_0 + By_0 + C \rvert}{\sqrt{A^2 + B^2}}
  9. 10.28.9

    Calculating Perimeters in the Plane

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

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

    P=sum of the side lengths\displaystyle P = \text{sum of the side lengths}
  10. 10.28.10

    Calculating Areas of Rectangles in the Plane

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

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

    A=l×w\displaystyle A = l \times w
  11. 10.28.11

    Calculating Areas of Triangles and Quadrilaterals in the Plane

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

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

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

Unit 11 6 topics

Statistics

Two variables at once: plotting pairs, fitting a line, and what correlation can’t show.

11.29 Correlation

r ≈ 0.9strong positiver ≈ 0no linear patternr ≈ −0.8negative
r runs from −1 to 1. The sign gives the direction; the closer to ±1, the tighter the points hug the trend line.
  1. 11.29.1

    Scatter Plots

    Plot paired data (x,y)(x, y) as points to look for a relationship. The explanatory variable goes on the xx-axis.

  2. 11.29.2

    Trend Lines

    A straight line through the middle of the cloud, with about as many points above it as below.

    y^=mx+b\displaystyle \hat{y} = mx + b
  3. 11.29.3

    Making Predictions Using Trend Lines

    Substitute xx into the trend line. Predicting inside the data’s range (interpolation) is safer than beyond it (extrapolation).

  4. 11.29.4

    Interpreting Trend Line Coefficients

    The slope is the predicted change in yy for each one-unit increase in xx. The intercept is the predicted yy at x=0x = 0, which may be meaningless.

    e.g. y^=2.5x+60\hat{y} = 2.5x + 60, hours studied vs. score: each hour adds about 2.5 points

  5. 11.29.5

    Linear Correlation

    rr measures how tightly points hug a line, from −1-1 to 11. The sign gives direction; near 0 means no linear pattern. Correlation does not show cause.

    −1≤r≤1\displaystyle -1 \le r \le 1
  6. 11.29.6

    Correlation vs. Causation

    A strong correlation shows two variables move together, not that one causes the other. A third variable may drive both, the cause may run the other way, or it may be chance. A controlled experiment is what isolates a cause.

    e.g. Ice cream sales and drownings rise together because hot weather drives both

No topic matches that search. Try a single word, like “circle” or “slope.”

Topic numbers match the course outline, so a topic here lines up with the same number in the lesson list.