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Algebra for Physics · Lesson 4 of 6

Ratio, Proportion and Scaling

14 min read3 ideas6 checksBy Asheshanand Acharya
What you will learn 0 / 3
Ratio proportion and scaling
Look around
The year of Mars, from the year of the Earth

Mars goes round the Sun at \(1.52\) times the Earth's distance. How long is its year? The chapter Gravitational Energy and Orbits gives the period as \(T^2 = (4\pi^2/GM)\,a^3\), where \(M\) is the Sun's mass. The question seems to need \(G\) and \(M\). It needs neither, because the same constant belongs to every planet of the Sun.

you will answer "if \(r\) doubles, what happens?" in one line for any power law. You will also find the year of Mars from the year of the Earth.

Proportional means a fixed ratio

Two quantities are proportional when their ratio stays the same. The blades of a ceiling fan all turn at one angular speed \(\omega\), so the speed of a point is \(v = r\omega\). A point twice as far from the axis moves twice as fast, because \(v/r = \omega\) is the same for every point. We write \(v \propto r\), and the fixed ratio \(\omega\) is the constant of proportionality.

RememberScaling by a power law
\[ y = kx^n \quad\Longrightarrow\quad \dfrac{y_2}{y_1} = \left(\dfrac{x_2}{x_1}\right)^n \]
Holds whenfor any real power \(n\), when the same constant \(k\) applies to both cases compared. Everything else in the law must stay fixed.
Symbols\(y_1, y_2\) the quantity in the two cases, \(x_1, x_2\) the variable it depends on, \(n\) the power, \(k\) the constant of proportionality
Unitsthe ratios have no unit, so \(x_1\) and \(x_2\) need only be in the same unit, and likewise \(y_1\) and \(y_2\)
definition 6.2
Proportional to a power

A quantity \(y\) is proportional to the \(n\)th power of \(x\), written \(y \propto x^n\), when \(y = kx^n\) with the same constant \(k\) in every case compared. The power \(n\) may be any real number: negative for an inverse law, a fraction for a root.

Deriving \(\dfrac{y_2}{y_1} = \left(\dfrac{x_2}{x_1}\right)^n\) step 1 of 3
1

\[ y_1 = kx_1^n, \qquad y_2 = kx_2^n \]

Why. the same law, with the same constant \(k\), holds in both cases.

The constant has cancelled, and so has every unit. So a ratio question never needs the constant: not \(G\), not \(M\), not the viscosity of air. The words "if \(x\) doubles" mean \(x_2/x_1 = 2\), and then \(y\) changes by the factor \(2^n\). If \(x\) is multiplied by any factor \(k\), \(y\) is multiplied by \(k^n\).

CheckpointUnanswered

The gravitational force between two bodies varies as \(1/r^2\). The distance between them is tripled. What happens to the force?

Direct inverse and inverse square

Direct, inverse and inverse square

A handful of powers covers most of physics. In a direct law, \(y \propto x\), both grow together in the same ratio. In an inverse law, \(y \propto 1/x\), one falls as the other grows. At a fixed temperature, a gas squeezed to a third of its volume has three times the pressure. In an inverse-square law, \(y \propto 1/x^2\), doubling the distance cuts the effect to a quarter. Gravity, the force between charges and the intensity of a lamp all fall off this way.

Property
If x doubles, y becomes
A law of this form
\(y \propto x\)
\(2y\)
the speed \(v = r\omega\) of a point on a fan blade
\(y \propto x^2\)
\(4y\)
the stopping distance \(u^2/2a\) of a car
\(y \propto x^{3/2}\)
\(2.83\,y\)
the period of a planet, Kepler's third law
\(y \propto 1/x\)
\(y/2\)
the pressure of a gas at a fixed temperature, Boyle's law
\(y \propto 1/x^2\)
\(y/4\)
the gravitational force, the Coulomb force, the intensity of a lamp
CheckpointUnanswered

The terminal velocity of a small raindrop varies as the square of its radius. A drop of twice the radius falls at how many times the speed?

Scaling laws of physics

Higher powers magnify a change

The higher the power of a power law, the more a change is magnified. In the figure below, a slider multiplies a radius \(r\) by a factor \(k\). At \(k = 2\) the fourth power grows sixteen times. At \(k = 0.8\), a cut of only 20 %, the fourth power falls to \(0.41\) of its old value. This is why a narrowed artery or a pinched drip tube changes the flow so much: the flow through a tube grows as \(r^4\).

Higher powers magnify a changeFour bars show by what factor r, r squared, r cubed and r to the fourth power change when r is multiplied by a factor k, set by a slider from 0.5 to 2. A dashed line marks a factor of 1, no change. At k = 2 the bars stand at 2, 4, 8 and 16. At k = 0.8, a 20 per cent cut in r, they stand at 0.80, 0.64, 0.51 and 0.41. At k = 0.5 the fourth power has fallen to 0.0625. The higher the power, the more a change in r is magnified, both upward and downward. 1 r 2.00 r² 4.00 r³ 8.00 r⁴ 16.00 r × 2.00: r² × 4.00, r³ × 8.00, r⁴ × 16.0
SimThe factors by which \(r\), \(r^2\), \(r^3\) and \(r^4\) change when \(r\) is multiplied by \(k\). Move the slider. The dashed line marks no change. Above it every power magnifies the growth; below it every power magnifies the fall.

Several factors multiply

A law may depend on several quantities. Then each quantity brings its own factor, and the factors multiply. The period of a pendulum is \(T = 2\pi\sqrt{l/g}\), so \(T \propto l^{1/2}g^{-1/2}\). Take a pendulum four times as long to a place where \(g\) is half as large. Its period changes by \(4^{1/2} \times (1/2)^{-1/2} = 2 \times 1.41 = 2.83\).

Back to the planets

Kepler's third law says \(T^2 \propto a^3\) for every planet of the Sun, so \(T \propto a^{3/2}\). Measure distances in units of the Earth's orbit, astronomical units, and periods in Earth years. Then the Earth has \(a = 1\) and \(T = 1\), and every other planet has \(T = a^{3/2}\) exactly. The figure below shows what this means: a planet twice as far away takes \(2^{3/2} = 2.83\) years, so the Earth laps it almost three times.

A wider orbit, a much longer yearThe Sun at the centre, the Earth on its circular orbit of radius 1 astronomical unit, and a second planet, orange, on a circular orbit whose radius a is set by a slider from 1 to 4 astronomical units. Press play: one second of play is one year. By Kepler's third law the second planet's year is a to the power three halves Earth years, and the readout gives it. At a = 1.52, the orbit of Mars, the year is 1.87 Earth years. At a = 2 it is 2.83 years, so the Earth goes round almost three times while the planet goes round once. At a = 4 it is 8 years. blue: the Earth, 1 AU orbit 1.52 AU: year = 1.87 Earth years
SimThe Earth, blue, on its orbit of \(1\,\text{AU}\), and a second planet, orange, on an orbit whose radius is set by the slider. Press play; one second is one year. The readout gives the planet's year, \(a^{3/2}\) Earth years. Set \(a = 1.52\) for Mars and \(a = 4\) for an asteroid with an eight-year orbit.
ExampleThis is the law of periods of Gravitational Energy and Orbits, lesson 7, done with the tool

Mars orbits the Sun at \(a = 1.52\,\text{AU}\) and Jupiter at \(5.2\,\text{AU}\). Find the length of the year of each planet, in Earth years.

Reveal one step at a time and finish the rest yourself.
Checkpoint · numericUnanswered

Saturn orbits the Sun at \(9.5\,\text{AU}\). Use Kepler's third law to find its year, in Earth years.

years± 2 %
Checkpoint · numericUnanswered

The filament of a lamp radiates as a black body, \(P = \sigma AT^4\). Its absolute temperature rises from \(2000\,\text{K}\) to \(2400\,\text{K}\). By what factor does the radiated power grow?

± 2 %
Checkpoint · numericUnanswered

The flow through a narrow tube is \(Q \propto Pr^4\), where \(P\) is the pressure difference. An artery narrows to \(90\,\%\) of its radius. By what factor must the pressure difference rise to keep the same flow?

± 2 %
CheckpointUnanswered

A pendulum is made four times as long and taken to a planet where \(g\) is half the Earth's value. How does its period change? Use \(T = 2\pi\sqrt{l/g}\).

Common mistake

A proportion holds only while every other quantity stays fixed, and only inside the range of the law. \(v = u + at\) is not \(v \propto t\) unless \(u = 0\): a constant added to the law spoils the ratio. Stokes' law, and with it \(v_t \propto r^2\), holds only for small, slow spheres. Temperatures in Stefan's law must be in kelvin. The ratio \(327/27\) in degrees Celsius is meaningless, while \(600/300\) in kelvin is right.

In the world
Where this tool works in physics

Ratios answer the "what if" questions of every chapter. Kepler's law of periods compares planets. The fourth power of the radius in Poiseuille's law explains a narrowed artery, and merged raindrops fall faster by the square of their radius. Stefan's law compares hot bodies by the fourth power of their temperature. The laws of a vibrating string compare lengths, tensions and masses per length, and the speed of sound compares temperatures and gases. A wire that is stretched, cut or folded changes its resistance by a ratio. The same reasoning gives the extension of a wire and the stopping distance at a higher speed. It also explains the blue of the sky and the force of a hydraulic lift.

Exam traps
  1. Forgetting the power when a quantity changes.
    Write the law as \(y \propto x^n\) first. A factor \(k\) in \(x\) gives \(k^n\) in \(y\), not \(k\).
  2. Using a ratio when the law has an added constant.
    A ratio works only for \(y = kx^n\). For \(v = u + at\) or a stopping distance with a reaction time, work out both cases in full.
  3. Mixing units, or using degrees Celsius, in a ratio.
    Put both values in the same unit, and use kelvin wherever a temperature is raised to a power or divided.

Where this tool works in the book

The physics that leans on this lesson. Each card opens the topic where the tool is at work.