Mathematics · Book 2 · Grades 10–12

High School Mathematics

High School Mathematics · Grades 10–12

4Reference Functions

A handful of simple functions — affine, square, inverse, square root, cube — appear everywhere, alone or combined. Knowing their graphs and variations by heart turns many problems into a quick sketch. This chapter studies each of them in turn and proves their variations with the comparison technique of Chapter 3.

4.1 Affine functions

Definition 4.1 (Affine function)

An affine function is a function of the form

f(x)=mx+p,f(x) = mx + p,

where mm and pp are fixed real numbers. Its graph is a straight line: mm is the slope and pp the yy-intercept (the line crosses the vertical axis at (0,p)(0, p)). When p=0p = 0 the function is linear: f(x)=mxf(x) = mx expresses proportionality.

Proposition 4.2 (Slope and variations)

Let f(x)=mx+pf(x) = mx + p.

  1. For any two distinct inputs uvu \neq v: m=f(v)f(u)vum = \dfrac{f(v) - f(u)}{v - u} (the slope is the change of the output per unit change of the input).
  2. If m>0m > 0, ff is strictly increasing on R\R; if m<0m < 0, strictly decreasing; if m=0m = 0, constant.

Proof. 1. Compute f(v)f(u)=(mv+p)(mu+p)=m(vu)f(v) - f(u) = (mv + p) - (mu + p) = m(v - u), then divide by vu0v - u \neq 0.

2. If u<vu < v, then f(v)f(u)=m(vu)f(v) - f(u) = m(v-u) has the sign of mm, since vu>0v - u > 0: positive mm gives f(u)<f(v)f(u) < f(v) (increasing), negative mm gives f(u)>f(v)f(u) > f(v) (decreasing).

Two affine functions: increasing for m = 1/2 > 0, decreasing for m = -1 < 0. Moving one unit to the right changes y by m.
Two affine functions: increasing for m=12>0m = \frac12 > 0, decreasing for m=1<0m = -1 < 0. Moving one unit to the right changes yy by mm.

Example 4.3

Find the affine function whose graph passes through A(1,3)A(1, 3) and B(4,9)B(4, 9). The slope is

m=9341=63=2.m = \frac{9 - 3}{4 - 1} = \frac{6}{3} = 2 .

Then f(x)=2x+pf(x) = 2x + p, and f(1)=3f(1) = 3 gives 2+p=32 + p = 3, so p=1p = 1: f(x)=2x+1f(x) = 2x + 1. Check with BB: f(4)=9f(4) = 9.

4.2 The square function

Proposition 4.4 (Square function)

The function f(x)=x2f(x) = x^2, defined on R\R:

  1. is strictly decreasing on (,0]\intoc{-\infty}{0} and strictly increasing on [0,+)\intco{0}{+\infty}, with minimum 00 at x=0x = 0;
  2. satisfies f(x)=f(x)f(-x) = f(x) for all xx: its graph, a parabola, is symmetric about the vertical axis.

Proof. 1. Let 0u<v0 \leq u < v. Then

f(v)f(u)=v2u2=(vu)(v+u)>0,f(v) - f(u) = v^2 - u^2 = (v - u)(v + u) > 0,

since vu>0v - u > 0 and v+u>0v + u > 0: ff is strictly increasing on [0,+)\intco{0}{+\infty}. If u<v0u < v \leq 0, then vu>0v - u > 0 but v+u<0v + u < 0, so f(v)f(u)<0f(v) - f(u) < 0: strictly decreasing. Finally x20=f(0)x^2 \geq 0 = f(0) for all xx.

2. (x)2=x2(-x)^2 = x^2; so the points (x,x2)(x, x^2) and (x,x2)(-x, x^2), mirror images across the vertical axis, are both on the graph.

Remark 4.5 (Squares and order)

Because the square function decreases on the negative side, taking squares reverses the order of negative numbers: 3<2-3 < -2 but 9>49 > 4. Never square both sides of an inequality without checking signs.

4.3 The inverse function

Proposition 4.6 (Inverse function)

The function f(x)=1xf(x) = \dfrac1x, defined for x0x \neq 0:

  1. is strictly decreasing on (,0)\intoo{-\infty}{0} and strictly decreasing on (0,+)\intoo{0}{+\infty};
  2. satisfies f(x)=f(x)f(-x) = -f(x): its graph, a hyperbola, is symmetric about the origin.

Proof. 1. Let 0<u<v0 < u < v. Then

f(v)f(u)=1v1u=uvuv<0,f(v) - f(u) = \frac1v - \frac1u = \frac{u - v}{uv} < 0,

since uv<0u - v < 0 and uv>0uv > 0: strictly decreasing on (0,+)\intoo{0}{+\infty}. On (,0)\intoo{-\infty}{0} the same quotient has uv<0u - v < 0 and uv>0uv > 0 again (product of two negatives), so ff decreases there too.

2. 1x=1x\frac{1}{-x} = -\frac1x.

Remark 4.7

Careful: 1x\frac1x is not decreasing on its whole domain. From u=1u = -1 to v=1v = 1 the value jumps from 1-1 up to 11. The two branches must be studied separately.

The parabola y = x2 (symmetric about the vertical axis) and the hyperbola y = 1x (two branches, symmetric about the origin). The parabola y = x2 (symmetric about the vertical axis) and the hyperbola y = 1x (two branches, symmetric about the origin).
The parabola y=x2y = x^2 (symmetric about the vertical axis) and the hyperbola y=1xy = \frac1x (two branches, symmetric about the origin).

4.4 Square root and cube

Proposition 4.8 (Square root function)

The function f(x)=xf(x) = \sqrt{x}, defined on [0,+)\intco{0}{+\infty}, is strictly increasing.

Proof. Let 0u<v0 \leq u < v. Multiply and divide by the conjugate:

vu=(vu)(v+u)v+u=vuv+u>0,\sqrt v - \sqrt u = \frac{(\sqrt v - \sqrt u)(\sqrt v + \sqrt u)}{\sqrt v + \sqrt u} = \frac{v - u}{\sqrt v + \sqrt u} > 0,

since vu>0v - u > 0 and v+u>0\sqrt v + \sqrt u > 0 (note v>0v > 0, so v>0\sqrt v > 0).

Proposition 4.9 (Cube function)

The function f(x)=x3f(x) = x^3, defined on R\R, is strictly increasing, and its graph is symmetric about the origin.

Proof. Admitted at this level.

The square root (defined for x ≥ 0 only) and the cube, both increasing. The square root (defined for x ≥ 0 only) and the cube, both increasing.
The square root (defined for x0x \geq 0 only) and the cube, both increasing.

Proposition 4.10 (Comparing xx, x2x^2 and x\sqrt x)

For 0<x<10 < x < 1: x2<x<xx^2 < x < \sqrt x. For x>1x > 1: x<x<x2\sqrt x < x < x^2. At x=0x = 0 and x=1x = 1 the three values are equal.

Proof. Suppose 0<x<10 < x < 1. Multiplying x<1x < 1 by x>0x > 0 gives x2<xx^2 < x. Next, x<xx < \sqrt x: since both sides are positive and squaring is increasing on positive numbers, this inequality is equivalent to x2<xx^2 < x, which we just proved. For x>1x > 1, multiplying x>1x > 1 by xx gives x2>xx^2 > x, and x<x\sqrt x < x follows by the same squaring argument.

The three curves cross at (0,0) and (1,1) and swap order there: between 0 and 1, x2 is the smallest and √ x the largest; beyond 1 the order is reversed.
The three curves cross at (0,0)(0,0) and (1,1)(1,1) and swap order there: between 00 and 11, x2x^2 is the smallest and x\sqrt x the largest; beyond 11 the order is reversed.

Method 4.11 (Comparing images)

To compare f(a)f(a) and f(b)f(b) for a reference function ff:

  1. place aa and bb on an interval where the variations of ff are known;
  2. if ff increases there, images are in the same order as the inputs; if ff decreases, the order is reversed;
  3. if aa and bb are not in the same interval of monotonicity, deal with signs first (e.g. for the square: a negative and a positive input).

Example 4.12

Compare 12.3\dfrac{1}{2.3} and 12.4\dfrac{1}{2.4}: both inputs are in (0,+)\intoo{0}{+\infty}, where the inverse function decreases, and 2.3<2.42.3 < 2.4, so 12.3>12.4\dfrac{1}{2.3} > \dfrac{1}{2.4}. Compare (1.2)2(-1.2)^2 and (1.5)2(-1.5)^2: on (,0]\intoc{-\infty}{0} the square decreases, and 1.5<1.2-1.5 < -1.2, so (1.5)2>(1.2)2(-1.5)^2 > (-1.2)^2 — indeed 2.25>1.442.25 > 1.44.

4.5 Exercises

Exercise 4.1

For each affine function, give its slope, its yy-intercept, and say whether it is increasing or decreasing:

f(x)=3x2,g(x)=12x+4,h(x)=7,k(x)=x.f(x) = 3x - 2, \qquad g(x) = -\tfrac12 x + 4, \qquad h(x) = 7, \qquad k(x) = -x .
Solution

Solution of Exercise 4.1.

ff: slope 33, intercept 2-2, increasing. gg: slope 12-\frac12, intercept 44, decreasing. hh: slope 00, intercept 77, constant. kk: slope 1-1, intercept 00, decreasing (and linear).

Exercise 4.2

Find the affine function whose graph passes through (2,1)(2, 1) and (5,10)(5, 10); then the one through (1,4)(-1, 4) and (3,4)(3, -4).

Solution

Solution of Exercise 4.2.

Through (2,1)(2,1) and (5,10)(5,10): slope m=10152=3m = \frac{10 - 1}{5 - 2} = 3; then 1=3×2+p1 = 3 \times 2 + p gives p=5p = -5: f(x)=3x5f(x) = 3x - 5.

Through (1,4)(-1,4) and (3,4)(3,-4): slope m=443(1)=84=2m = \frac{-4 - 4}{3 - (-1)} = \frac{-8}{4} = -2; then 4=2×(1)+p4 = -2 \times (-1) + p gives p=2p = 2: f(x)=2x+2f(x) = -2x + 2.

Exercise 4.3

Without a calculator, compare:

(3.1)2 and (3.2)2;(2.7)2 and (2.8)2;15.1 and 15.2;17 and 15.(3.1)^2 \text{ and } (3.2)^2; \qquad (-2.7)^2 \text{ and } (-2.8)^2; \qquad \frac{1}{5.1} \text{ and } \frac{1}{5.2}; \qquad \sqrt{17} \text{ and } \sqrt{15}.
Solution

Solution of Exercise 4.3.

(3.1)2<(3.2)2(3.1)^2 < (3.2)^2: the square increases on positives.

(2.7)2<(2.8)2(-2.7)^2 < (-2.8)^2: the square decreases on negatives and 2.8<2.7-2.8 < -2.7.

15.1>15.2\frac{1}{5.1} > \frac{1}{5.2}: the inverse decreases on positives.

17>15\sqrt{17} > \sqrt{15}: the square root increases.

Exercise 4.4

Using the graph of the square function, solve x2=16x^2 = 16, then x216x^2 \leq 16, then x2>9x^2 > 9.

Solution

Solution of Exercise 4.4.

x2=16x^2 = 16: two solutions, x=4x = 4 and x=4x = -4 (the horizontal line y=16y = 16 cuts the parabola twice).

x216x^2 \leq 16: the parabola is below the line between the two intersection points: x[4,4]x \in \intcc{-4}{4}.

x2>9x^2 > 9: the parabola is strictly above y=9y = 9 outside [3,3]\intcc{-3}{3}: x(,3)(3,+)x \in \intoo{-\infty}{-3} \cup \intoo{3}{+\infty}.

Exercise 4.5

Let x(0,1)x \in \intoo{0}{1}. Order the numbers xx, x2x^2, x3x^3 and x\sqrt x from smallest to largest, and check your answer with x=0.25x = 0.25.

Solution

Solution of Exercise 4.5.

For 0<x<10 < x < 1: multiplying x<1x < 1 repeatedly by xx gives x3<x2<xx^3 < x^2 < x, and Proposition 4.10 gives x<xx < \sqrt x, so

x3<x2<x<x.x^3 < x^2 < x < \sqrt x .

Check with x=0.25x = 0.25: x3=0.015625x^3 = 0.015625, x2=0.0625x^2 = 0.0625, x=0.25x = 0.25, x=0.5\sqrt x = 0.5.

Exercise 4.6 ★★

Solve graphically, then algebraically: 1x=2\dfrac1x = 2, and 1x<2\dfrac1x < 2 for x>0x > 0. What changes if we also allow x<0x < 0?

Solution

Solution of Exercise 4.6.

1x=2\frac1x = 2 has the unique solution x=12x = \frac12 (the hyperbola meets the horizontal line y=2y = 2 once, on the positive branch).

For x>0x > 0: 1x<2\frac1x < 2. Multiplying by x>0x > 0: 1<2x1 < 2x, so x>12x > \frac12: solution set (12,+)\intoo{\frac12}{+\infty}.

If x<0x < 0 is allowed: every negative xx satisfies 1x<0<2\frac1x < 0 < 2, so the full solution set is (,0)(12,+)\intoo{-\infty}{0} \cup \intoo{\frac12}{+\infty}.

Exercise 4.7 ★★

Knowing that the square function decreases on (,0]\intoc{-\infty}{0} and increases on [0,+)\intco{0}{+\infty}, frame x2x^2 when:

(a) x[2,5];(b) x[3,1];(c) x[2,3].\text{(a) } x \in \intcc{2}{5}; \qquad \text{(b) } x \in \intcc{-3}{-1}; \qquad \text{(c) } x \in \intcc{-2}{3}.

(In case (c), be careful: the minimum of x2x^2 is not at an endpoint.)

Solution

Solution of Exercise 4.7.

(a) On [2,5]\intcc{2}{5}, all inputs are positive and squaring increases: 4x2254 \leq x^2 \leq 25.

(b) On [3,1]\intcc{-3}{-1}, squaring decreases: the largest square comes from 3-3: 1x291 \leq x^2 \leq 9.

(c) On [2,3]\intcc{-2}{3}, the interval contains 00, where the square reaches its minimum 00; the maximum is the larger of (2)2=4(-2)^2 = 4 and 32=93^2 = 9. So 0x290 \leq x^2 \leq 9.

Exercise 4.8 ★★

A taxi company charges a fixed fee of 44 plus 1.51.5 per kilometer; another charges no fee and 22 per kilometer. Model each price by an affine function of the distance xx, plot both lines, and find from which distance the first company is cheaper.

Solution

Solution of Exercise 4.8.

First company: f(x)=1.5x+4f(x) = 1.5x + 4; second: g(x)=2xg(x) = 2x. The first is cheaper when

1.5x+4<2x  4<0.5x  x>8.1.5x + 4 < 2x \ \Longleftrightarrow\ 4 < 0.5x \ \Longleftrightarrow\ x > 8 .

Beyond 88 km, the first company is cheaper; at exactly 88 km both charge 1616.

Exercise 4.9 ★★

Show that for all a,b0a, b \geq 0: a+ba+b\sqrt{a + b} \leq \sqrt a + \sqrt b. (Hint: both sides are nonnegative, so compare their squares.) When is there equality?

Solution

Solution of Exercise 4.9.

Both sides are nonnegative, so the inequality is equivalent to the one between their squares:

(a+b)2=a+band(a+b)2=a+2ab+b.\left(\sqrt{a+b}\right)^2 = a + b \qquad\text{and}\qquad \left(\sqrt a + \sqrt b\right)^2 = a + 2\sqrt a \sqrt b + b .

Since 2ab02\sqrt a\sqrt b \geq 0, the second square is at least the first, which proves a+ba+b\sqrt{a+b} \leq \sqrt a + \sqrt b. Equality holds exactly when ab=0\sqrt a \sqrt b = 0, i.e. when a=0a = 0 or b=0b = 0.

Exercise 4.10 ★★★

Let f(x)=2x+1x1f(x) = \dfrac{2x + 1}{x - 1}, defined for x1x \neq 1.

  1. Show that f(x)=2+3x1f(x) = 2 + \dfrac{3}{x - 1} for all x1x \neq 1.
  2. Deduce the variations of ff on (1,+)\intoo{1}{+\infty} from those of the inverse function.
Solution

Solution of Exercise 4.10.

1. Put the right-hand side over a common denominator:

2+3x1=2(x1)+3x1=2x+1x1=f(x).2 + \frac{3}{x-1} = \frac{2(x-1) + 3}{x - 1} = \frac{2x + 1}{x - 1} = f(x).

2. On (1,+)\intoo{1}{+\infty}, as xx increases, x1x - 1 increases and stays positive, so 3x1\frac{3}{x-1} decreases (inverse function, times the positive constant 33), so f(x)=2+3x1f(x) = 2 + \frac{3}{x-1} decreases: ff is strictly decreasing on (1,+)\intoo{1}{+\infty}.

4.6 Problem: The laws of nature speak in reference functions

Problem 4.1

Weekend problem — braking distances grow as v2v^2, levers obey 1/d1/d, planets follow a3/2a^{3/2}: reading physics with the reference functions

Open a physics book and the same few graphs appear on every page: the parabola, the hyperbola, the root curve. Nature writes its laws with this chapter’s reference functions — and knowing their shapes (Proposition 4.4, Proposition 4.6, Proposition 4.8, Proposition 4.9) is enough to brake a car, balance a lever, and time the planets. The grand finale is Kepler’s third law, read straight off the solar system’s data.

Part I — The square law of braking. A rule of thumb for a car’s braking distance on dry road: d=(v10)2d = \left(\frac{v}{10}\right)^{2} meters, at speed vv km/h.

  1. Compute the braking distances at 3030, 5050, 9090 and 130130 km/h.
  2. Doubling the speed multiplies the braking distance by how much? Explain from the square function’s scaling, and check on 5010050 \to 100 km/h.
  3. Forensics: skid marks measure 5050 m. What speed does the formula convict the driver of (to the km/h)? Which reference function answered — and on which domain is the reading unambiguous (Proposition 4.8)?
  4. Compare the extra distance caused by one km/h more, at low and at high speed: compute d(31)d(30)d(31) - d(30) and d(91)d(90)d(91) - d(90). Which property of the parabola (Proposition 4.4) do the two answers illustrate?
  5. Real stopping adds reaction time — about one second, during which the car covers 0.28v0.28v meters: D(v)=0.28v+(v10)2D(v) = 0.28v + \left(\frac{v}{10}\right)^2. Compute D(50)D(50) and D(130)D(130). Which of the two terms — affine or square — dominates at city speed, and which on the highway?

Part II — The hyperbolas of daily life.

  1. A lever balances when force ×\times distance is the same on both sides. A 6060 kg child sits 22 m from the pivot; the balancing force at distance dd on the other side is F(d)=120dF(d) = \frac{120}{d} (in kg-equivalents). Compute F(0.5)F(0.5), F(1)F(1), F(3)F(3).
  2. What do the variations of the inverse function (Proposition 4.6) say about levers — and why does Archimedes’ boast (“give me a place to stand and I shall move the Earth”) hide in the hyperbola’s tail? What forbids d=0d = 0?
  3. Sound and light fade with the square of the distance: at 11 m from a lamp the intensity is 100100 units; give it at 22, 33 and 1010 m. Explain the exponent 22 with a sphere: over what area has the light spread at distance dd (Archimedes’ tombstone problem, in the Middle School volume)?
  4. A bus for the school trip costs 600600 euros, split equally among nn participants. Tabulate the cost per head for n=10,20,30n = 10, 20, 30, find how many participants bring it to 2525 euros or less, and state what the hyperbola’s shape promises — and refuses — as nn grows.
  5. Producing xx posters costs 2x+32x + 3 euros (33 euros of setup). Show that the average cost per poster is a(x)=2+3xa(x) = 2 + \frac3x, describe its variations, and interpret its horizontal asymptote economically. (Compare the algebra of Exercise 4.10.)

Part III — Kepler’s harmony. For each planet, let aa be its mean distance to the Sun (in astronomical units, Earth =1= 1) and TT its period (in years). Data: Mars a=1.52a = 1.52, T=1.88T = 1.88; Jupiter a=5.20a = 5.20, T=11.86T = 11.86; Saturn a=9.54a = 9.54, T=29.4T = 29.4.

  1. Compute a3a^3 and T2T^2 for the Earth, Mars and Jupiter. What did Kepler notice in 1618?
  2. State the law as a function: T=a3=aaT = \sqrt{a^3} = a\sqrt a. Test it on Saturn.
  3. Two predictions: an asteroid orbits at a=4a = 4 AU — find its period (the numbers come out whole); a comet returns every 2727 years — find its mean distance (look for a perfect cube).
  4. Which three reference functions does the law braid together? And its scaling rule: when aa is multiplied by 44, what happens to TT? (Check with the asteroid against the Earth.)
  5. Kepler read this law in Tycho Brahe’s data seventy years before Newton’s gravitation explained it. In one sentence: what does this episode say about the power of recognizing a reference function in a table of numbers?

Part IV — The tortoise and the hare.

  1. Order x\sqrt x, xx and x2x^2 on (0,1)\intoo{0}{1} and on (1,+)\intoo{1}{+\infty} (Proposition 4.10), and verify the two orderings at x=0.25x = 0.25 and x=4x = 4.
  2. Solve x>x\sqrt x > x completely (for x0x \geq 0, square soundly and finish with a sign table).
  3. Bring in the cube: order xx, x2x^2, x3x^3 at x=0.5x = 0.5 and at x=2x = 2, and find all points where the square and the cube functions cross.
  4. Two savings schemes pay, after tt years, 100t100\sqrt t euros (scheme A) or 10t210 t^2 euros (scheme B). Show that B overtakes A when t3=100t^3 = 100, and give the crossover time to the month. Moral about roots against powers in the long run?
  5. Finale: for each law of this problem — braking (v2v^2), the lever (1/d1/d), the lamp (1/d21/d^2), Kepler (a3/2a^{3/2}), scheme A (t\sqrt t) — say in one clause which feature of its reference graph carries the physical meaning (steepening rise, vertical asymptote, spreading sphere, scaling exponent, flattening growth). Conclusion: the reference functions are the alphabet; nature writes with them.
Solution

Solution of Problem 4.1.

1. d(30)=32=9d(30) = 3^2 = 9 m; d(50)=25d(50) = 25 m; d(90)=81d(90) = 81 m; d(130)=169d(130) = 169 m.

2. Doubling vv doubles v10\frac v{10} and multiplies its square by 44: d(100)=100d(100) = 100 m =4×d(50)= 4 \times d(50). Twice the speed, four times the distance — the square function’s scaling.

3. (v10)2=50\left(\frac{v}{10}\right)^2 = 50 gives v10=50\frac{v}{10} = \sqrt{50}, so v=105071v = 10\sqrt{50} \approx 71 km/h. The square root answered; the reading is unambiguous because speeds are positive, and on [0,+)\intco{0}{+\infty} the square function climbs strictly (Proposition 4.8: one positive preimage).

4. d(31)d(30)=9.619=0.61d(31) - d(30) = 9.61 - 9 = 0.61 m, while d(91)d(90)=82.8181=1.81d(91) - d(90) = 82.81 - 81 = 1.81 m: the same +1+1 km/h costs three times more distance at high speed. The parabola not only rises, it steepens — its rate of climb grows with xx.

5. D(50)=14+25=39D(50) = 14 + 25 = 39 m; D(130)=36.4+169=205.4D(130) = 36.4 + 169 = 205.4 m. In town the affine (reaction) term is the bigger share; on the highway the square term crushes it — affine grows steadily, squares run away.

6. F(0.5)=240F(0.5) = 240, F(1)=120F(1) = 120, F(3)=40F(3) = 40.

7. The inverse function decreases: the further from the pivot, the smaller the needed force — with a long enough lever arm (dd huge), any force, however small, balances any load: Archimedes’ boast lives in the hyperbola’s tail, which approaches 00 without reaching it. And d=0d = 0 is the forbidden value: no arm, no lever — the vertical asymptote.

8. 1004=25\frac{100}{4} = 25 at 22 m, 100911\frac{100}{9} \approx 11 at 33 m, 11 at 1010 m. At distance dd the light has spread over a sphere of area 4πd24\pi d^2 (Archimedes’ tombstone problem, in the Middle School volume): the same energy divided by an area growing like d2d^2 — hence the inverse square.

9. 6060, 3030, 2020 euros per head for n=10,20,30n = 10, 20, 30. For 600n25\frac{600}{n} \leq 25: n24n \geq 24 participants. The hyperbola promises ever-cheaper shares as nn grows — and refuses ever to reach 00: the bus is never free.

10. a(x)=2x+3x=2+3xa(x) = \frac{2x + 3}{x} = 2 + \frac3x: decreasing on (0,+)\intoo{0}{+\infty} (inverse function shifted), approaching the asymptote y=2y = 2. Economically: spreading the fixed 33 euros over more posters pushes the unit cost down towards the incompressible 22 euros of materials — economies of scale, with a hard floor.

11. Earth: a3=1a^3 = 1, T2=1T^2 = 1. Mars: 1.5233.511.52^3 \approx 3.51 and 1.8823.531.88^2 \approx 3.53. Jupiter: 5.203140.65.20^3 \approx 140.6 and 11.862140.711.86^2 \approx 140.7. Kepler’s notice: T2=a3T^2 = a^3 for every planet — one law for the whole sky.

12. T=a3T = \sqrt{a^3}: for Saturn 9.543=86829.5\sqrt{9.54^3} = \sqrt{868} \approx 29.5 years, against the observed 29.429.4: the law holds to a tenth.

13. Asteroid: T=43=64=8T = \sqrt{4^3} = \sqrt{64} = 8 years. Comet: a3=272=729=93a^3 = 27^2 = 729 = 9^3, so a=9a = 9 AU.

14. Square (T2T^2), cube (a3a^3) and square root (to extract TT). Scaling: multiplying aa by 44 multiplies TT by 44=84\sqrt4 = 8 — as the asteroid confirms (aa four times Earth’s, TT eight times).

15. A table of numbers, matched against the shapes of a few reference functions, yielded a law of the universe seventy years before anyone knew why it held — recognizing the function is half of science.

16. On (0,1)\intoo{0}{1}: x2<x<xx^2 < x < \sqrt x; on (1,+)\intoo{1}{+\infty}: x<x<x2\sqrt x < x < x^2. Checks: at x=0.25x = 0.25: 0.0625<0.25<0.50.0625 < 0.25 < 0.5; at x=4x = 4: 2<4<162 < 4 < 16.

17. For x0x \geq 0, both sides are 0\geq 0, so x>x    x>x2    x(1x)>0    x(0,1)\sqrt x > x \iff x > x^2 \iff x(1 - x) > 0 \iff x \in \intoo{0}{1}.

18. At x=0.5x = 0.5: x3=0.125<x2=0.25<x=0.5x^3 = 0.125 < x^2 = 0.25 < x = 0.5. At x=2x = 2: 2<4<82 < 4 < 8: the order reverses. Crossings of x2x^2 and x3x^3: x3x2=x2(x1)=0x^3 - x^2 = x^2(x - 1) = 0: at x=0x = 0 and x=1x = 1.

19. 10t2=100t10t^2 = 100\sqrt t gives t2=10tt^2 = 10\sqrt t; squaring, t4=100tt^4 = 100t, so t3=100t^3 = 100 and t=10034.64t = \sqrt[3]{100} \approx 4.64 years — about 44 years and 88 months. (Both schemes then pay about 215215 euros.) Moral: roots sprint early, powers win every marathon.

20. Braking: the parabola’s steepening is the danger of speed. Lever: the vertical asymptote at 00 and the long tail are the mechanic’s advantage. Lamp: the d2d^2 of the spreading sphere sets the fading. Kepler: the exponent 32\frac32 is the solar system’s tempo. Savings A: the root’s flattening is the slow saver’s fate. Five graphs, five laws: nature’s alphabet indeed.