---
title: "Orders of Magnitude: Measuring the Universe"
book: "High School Physics"
subject: physics
language: en
chapter: 1
exercises: 15
source: https://one-course.com/books/physics/2/en/chapter/1-orders-of-magnitude-measuring-the-universe
---

# Chapter 1 — Orders of Magnitude: Measuring the Universe

Physics begins where opinion ends: with a measurement. But the things physics measures span an absurd range — an atomic nucleus is about $10^{-15}\,\mathrm{m}$ across, the observable universe about $10^{27}\,\mathrm{m}$: a factor of $10^{42}$, far beyond anything a mental picture can hold. This chapter installs the toolkit that tames the range — [units](#def-g10-orders-of-magnitude-unit), powers of ten, [significant figures](#def-g10-orders-of-magnitude-sigfig) — and two habits used on every page after this one: write the [unit](#def-g10-orders-of-magnitude-unit), and check the [order of magnitude](#def-g10-orders-of-magnitude-oom).

## 1.1 Units: the grammar of measurement

**Definition 1.1 (Physical quantities and SI units).**

A *physical quantity* is a property of the world that can be measured: a length, a duration, a mass. Measuring it means counting how many times a reference quantity — the *unit* — fits into it. The *International System of Units* (SI) fixes seven base units, of which three run this whole volume: the *metre* ($\mathrm{m}$) for length, the *kilogram* ($\mathrm{kg}$) for mass and the *second* ($\mathrm{s}$) for time. (The other four — ampere, kelvin, mole, candela — will join when electricity, heat and chemistry enter the story.)

**Remark 1.2 (A number without a unit is not a result).**

“The distance is $384$” means nothing: $384\,\mathrm{mm}$, $384\,\mathrm{km}$ and $384\,\mathrm{Mm}$ are three different worlds (the last happens to be the distance to the Moon). In 1999, NASA lost the $327-million *Mars Climate Orbiter* because one program computed thruster forces in pounds-force while another read them as newtons. House rule, from this line to the end of the book: every measured or computed number carries its [unit](#def-g10-orders-of-magnitude-unit), on every line of the calculation.

**Definition 1.3 (SI prefixes).**

A *prefix* glued to a [unit](#def-g10-orders-of-magnitude-unit) multiplies it by a fixed power of ten:

| femto | f | $10^{-15}$ | centi | c | $10^{-2}$ |
| --- | --- | --- | --- | --- | --- |
| pico | p | $10^{-12}$ | kilo | k | $10^{3}$ |
| nano | n | $10^{-9}$ | mega | M | $10^{6}$ |
| micro | $\mu$ | $10^{-6}$ | giga | G | $10^{9}$ |
| milli | m | $10^{-3}$ | tera | T | $10^{12}$ |

Thus $1\,\mathrm{nm} = 10^{-9}\,\mathrm{m}$ and $1\,\mathrm{km} = 10^{3}\,\mathrm{m}$.

**Example 1.4 (Reading prefixes).**

Green light has wavelength about $500\,\mathrm{nm} = 5.00 \times 10^{-7}\,\mathrm{m}$; a human hair is about $70\,\text{µ}\mathrm{m} = 7.0 \times 10^{-5}\,\mathrm{m}$ thick; the Moon orbits at $384\,\mathrm{Mm} = 3.84 \times 10^{8}\,\mathrm{m}$. One raindrop has mass about $30\,\mathrm{mg} = 3.0 \times 10^{-5}\,\mathrm{kg}$ — note that the SI base [unit](#def-g10-orders-of-magnitude-unit) of mass, alone among the seven, carries a [prefix](#def-g10-orders-of-magnitude-prefixes) already.

## 1.2 Scientific notation and significant figures

**Definition 1.5 (Scientific notation).**

A number is in *scientific notation* when written as

$$
a \times 10^{n}, \qquad 1 \leq a < 10, \quad n \text{ an integer.}
$$

The factor $a$ is the *mantissa*, the integer $n$ the *exponent*. Thus $149\,600\,000 = 1.496 \times 10^{8}$ and $0.000\,52 = 5.2 \times 10^{-4}$.

**Proposition 1.6 (Computing with powers of ten).**

For all integers $m$ and $n$:

$$
10^{m} \times 10^{n} = 10^{m+n}, \qquad
\frac{1}{10^{n}} = 10^{-n}, \qquad
\left(10^{m}\right)^{n} = 10^{mn}.
$$

**Partial proof.** For positive [exponents](#def-g10-orders-of-magnitude-scinot), count the factors: $10^{m} \times 10^{n}$ is a product of $m + n$ tens, and $(10^m)^n$ chains $n$ groups of $m$ tens. Writing $10^{-n}$ for $1/10^{n}$ is precisely the convention that keeps the first rule true for all integers: it forces $10^{n} \times 10^{-n} = 10^{0} = 1$. The companion mathematics volume studies the [exponent](#def-g10-orders-of-magnitude-scinot) rules in full. ∎

**Example 1.7 (Multiplying in scientific notation).**

How many Earths fit in the Sun, by mass? With $m_{\text{Sun}} = 1.99 \times 10^{30}\,\mathrm{kg}$ and $m_{\text{Earth}} = 5.97 \times 10^{24}\,\mathrm{kg}$:

$$
\frac{1.99 \times 10^{30}}{5.97 \times 10^{24}}
= \frac{1.99}{5.97} \times 10^{30-24}
= 0.333 \times 10^{6}
= 3.33 \times 10^{5}.
$$

[Mantissas](#def-g10-orders-of-magnitude-scinot) and [exponents](#def-g10-orders-of-magnitude-scinot) are handled separately; the final answer is re-normalized so that the [mantissa](#def-g10-orders-of-magnitude-scinot) lands back in $[1, 10)$.

**Definition 1.8 (Significant figures).**

The *significant figures* of a measured number are the digits actually vouched for by the measurement: all written digits except the leading zeros. Trailing zeros count — $5.20 \times 10^{-3}\,\mathrm{s}$ (three significant figures) promises more than $5.2 \times 10^{-3}\,\mathrm{s}$ (two). [Scientific notation](#def-g10-orders-of-magnitude-scinot) shows the count at a glance: the [mantissa](#def-g10-orders-of-magnitude-scinot) carries exactly the significant figures.

**Method 1.9 (How many digits to keep).**

A computed result cannot be more precise than its ingredients.

1. In a product or quotient, keep as many [significant figures](#def-g10-orders-of-magnitude-sigfig) as the *least* precise factor.
2. Round only the final answer, never the intermediate steps.
3. When in doubt, three [significant figures](#def-g10-orders-of-magnitude-sigfig) is the working precision of this book.

**Example 1.10 (Earth’s circumference).**

Earth’s diameter is $d = 1.27 \times 10^{7}\,\mathrm{m}$ (three [significant figures](#def-g10-orders-of-magnitude-sigfig)), so its circumference is $\pi d = 3.141\,59 \times 1.27 \times 10^{7}\,\mathrm{m} = 3.99 \times 10^{7}\,\mathrm{m}$ — three figures, not the eight the calculator displays. Writing $39\,898\,227\,\mathrm{m}$ would claim to know the planet to the [metre](#def-g10-orders-of-magnitude-unit).

![A ruler on which each equal step multiplies by ten. The small ticks are 200, 300, …, 900: a whole decade crowds into each segment. On this ruler 300 leans toward 102 and 7000 toward 104 — their orders of magnitude.](https://one-course.com/images/onecourse/chapters/physics-2/g10-orders-of-magnitude/fig-75f975736dc2.svg)

*A ruler on which each equal step *multiplies* by ten. The small ticks are $200, 300, \dots, 900$: a whole decade crowds into each segment. On this ruler $300$ leans toward $10^{2}$ and $7000$ toward $10^{4}$ — their orders of magnitude.*

## 1.3 The ladder of the universe

**Definition 1.11 (Order of magnitude).**

The *order of magnitude* of a quantity is the power of ten closest to it: write the quantity as $a \times 10^{n}$ with $1 \leq a < 10$ and take $10^{n}$ if $a < 5$, $10^{n+1}$ if $a \geq 5$. (The exact boundary convention never matters: an order-of-magnitude statement is only ever meant to within a factor of ten.)

**Example 1.12 (Orders of magnitude).**

A human life lasts about $80$ years, i.e. $80 \times 3.16 \times 10^{7}\,\mathrm{s} \approx 2.5 \times 10^{9}\,\mathrm{s}$: [order of magnitude](#def-g10-orders-of-magnitude-oom) $10^{9}\,\mathrm{s}$ — a few billion seconds, spend them well. A human is $1.7\,\mathrm{m}$ tall: order $10^{0}\,\mathrm{m}$. Mount Everest, $8848\,\mathrm{m}$: order $10^{4}\,\mathrm{m}$, since $8.848 \geq 5$.

Stacking such estimates by [exponent](#def-g10-orders-of-magnitude-scinot) produces the master picture of this chapter: a ladder whose every rung is a world ten times wider than the one below.

![The ladder of the universe, in metres: 42 powers of ten separate the atomic nucleus from the observable universe, and a human stands ten rungs from the atom but twenty-seven from the top.](https://one-course.com/images/onecourse/chapters/physics-2/g10-orders-of-magnitude/fig-28b14eb54206.svg)

*The ladder of the universe, in [metres](#def-g10-orders-of-magnitude-unit): $42$ powers of ten separate the atomic nucleus from the observable universe, and a human stands ten rungs from the atom but twenty-seven from the top.*

Above the Earth rung, [metres](#def-g10-orders-of-magnitude-unit) stop being convenient; astronomy keeps its own [units](#def-g10-orders-of-magnitude-unit), both defined from the ladder itself.

**Definition 1.13 (Astronomical unit and light-year).**

The *astronomical unit* ($1\,\mathrm{au} = 1.496 \times 10^{11}\,\mathrm{m}$) is the average Earth–Sun distance. The *light-year* ($\mathrm{ly}$) is the distance light travels in one year. Light moves in vacuum at

$$
c = 3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s},
$$

the fastest speed nature allows — so the light-year is a distance, not a time.

![Distances from Earth on the multiplicative ruler, with light’s travel time in red beneath each: the Moon is light-seconds away, the planets light-hours, the stars light-years.](https://one-course.com/images/onecourse/chapters/physics-2/g10-orders-of-magnitude/fig-16567f659041.svg)

*Distances from Earth on the multiplicative ruler, with light’s travel time in red beneath each: the Moon is light-seconds away, the planets light-hours, the stars [light-years](#def-g10-orders-of-magnitude-lightyear).*

**Example 1.14 (The light-year in metres).**

A year holds $365.25 \times 24 \times 3600 = 3.156 \times 10^{7}\,\mathrm{s}$ (pleasantly close to $\pi \times 10^{7}\,\mathrm{s}$). Hence

$$
1\,\mathrm{ly} = c \times 3.156 \times 10^{7}\,\mathrm{s}
= 3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s} \times 3.156 \times 10^{7}\,\mathrm{s}
= 9.47 \times 10^{15}\,\mathrm{m}.
$$

Proxima Centauri, the nearest star after the Sun, lies $4.2\,\mathrm{ly} \approx 4.0 \times 10^{16}\,\mathrm{m}$ away: light, which crosses an Earth–Sun distance in eight minutes, needs over four years to arrive from there.

**Method 1.15 (Sanity check by order of magnitude).**

Before trusting any computed result:

1. round every input to its [order of magnitude](#def-g10-orders-of-magnitude-oom) ;
2. redo the computation with powers of ten alone, using [Proposition 1.6](#prop-g10-orders-of-magnitude-powers) — this takes seconds;
3. compare: the precise answer must agree with the estimate to within a factor of ten or so, and its [unit](#def-g10-orders-of-magnitude-unit) must be the right one. If either check fails, hunt down the error before moving on.

**Remark 1.16 (Why bother).**

A calculator will happily report that an apple has mass $4 \times 10^{8}\,\mathrm{kg}$ — it cannot know better. No formula flags the absurd; the habit does. Physicists estimate first and compute second: the estimate catches misplaced decimal points, swapped [units](#def-g10-orders-of-magnitude-unit) and inverted fractions, the three errors behind most wrong answers at every level.

## 1.4 Measurement and uncertainty

No instrument reads the true value. A measurement is honest only when it also reports how far off it might be.

**Definition 1.17 (Absolute and relative uncertainty).**

A measurement of a quantity $x$ is stated as

$$
x = x_{\text{m}} \pm \Delta x ,
$$

where $x_{\text{m}}$ is the measured value and the *absolute uncertainty* $\Delta x > 0$, in the same [unit](#def-g10-orders-of-magnitude-unit), bounds the plausible error: the true value is claimed to lie between $x_{\text{m}} - \Delta x$ and $x_{\text{m}} + \Delta x$. The *relative uncertainty* is the ratio $\Delta x / x_{\text{m}}$, usually quoted in percent; it is what the word “precise” measures.

**Method 1.18 (Reading a graduated instrument).**

For a ruler, a measuring cylinder, a dial:

1. read the graduation nearest the mark, eye perpendicular to the scale (a slanted eye shifts the reading);
2. take at least half the smallest graduation as the [absolute uncertainty](#def-g10-orders-of-magnitude-uncertainty) — more if the object’s edge or the liquid’s surface is fuzzy;
3. write the result as $x_{\text{m}} \pm \Delta x$ with its [unit](#def-g10-orders-of-magnitude-unit) , and keep no digit beyond the uncertain one.

![Reading a millimetre ruler: the rod’s end falls nearest the 127\, mm graduation, and the shaded band of half a graduation on each side is the honest claim.](https://one-course.com/images/onecourse/chapters/physics-2/g10-orders-of-magnitude/fig-9ff0d7ee00e5.svg)

*Reading a millimetre ruler: the rod’s end falls nearest the $127\,\mathrm{mm}$ graduation, and the shaded band of half a graduation on each side is the honest claim.*

**Example 1.19 (Relative precision).**

The reading above has [relative uncertainty](#def-g10-orders-of-magnitude-uncertainty) $\frac{0.5}{127} \approx 0.4\%$. The same ruler measuring a $12\,\mathrm{mm}$ bolt gives $\frac{0.5}{12} \approx 4\%$: the identical instrument is ten times less precise on the small object. Precision is a property of the *measurement*, not of the tool.

**Remark 1.20 (Small absolute, huge relative — and conversely).**

Laser stations measure the Earth–Moon distance, $3.84 \times 10^{8}\,\mathrm{m}$, to about $\pm3\,\mathrm{cm}$: a [relative uncertainty](#def-g10-orders-of-magnitude-uncertainty) of $10^{-10}$, among the sharpest measurements ever made — with an absolute error no ruler would boast of. Always ask *relative to what*: the pair $(\Delta x,\ \Delta x / x_{\text{m}})$ tells the whole story, and either number alone can mislead.

## 1.5 Exercises

**Exercise 1.1 ★.**

Convert to [metres](#def-g10-orders-of-magnitude-unit), in [scientific notation](#def-g10-orders-of-magnitude-scinot):

1. $750\,\mathrm{nm}$ (wavelength of red light);
2. $2.5\,\mathrm{km}$ ;
3. $3.2\,\text{µ}\mathrm{m}$ (a soil bacterium);
4. $0.15\,\mathrm{Tm}$ (the Earth–Sun distance, in an unusual costume).

**Solution of Exercise 1.1.**

*1.* $750\,\mathrm{nm} = 750 \times 10^{-9}\,\mathrm{m} = 7.50 \times 10^{-7}\,\mathrm{m}$. *2.* $2.5\,\mathrm{km} = 2.5 \times 10^{3}\,\mathrm{m}$. *3.* $3.2\,\text{µ}\mathrm{m} = 3.2 \times 10^{-6}\,\mathrm{m}$. *4.* $0.15\,\mathrm{Tm} = 0.15 \times 10^{12}\,\mathrm{m} = 1.5 \times 10^{11}\,\mathrm{m}$ — one [astronomical unit](#def-g10-orders-of-magnitude-lightyear).

**Exercise 1.2 ★.**

Write in [scientific notation](#def-g10-orders-of-magnitude-scinot) and give the number of [significant figures](#def-g10-orders-of-magnitude-sigfig):

1. the Earth–Sun distance, $149\,600\,000\,\mathrm{km}$ , in [metres](#def-g10-orders-of-magnitude-unit) ;
2. the diameter of a hydrogen atom, $0.000\,000\,000\,106\,\mathrm{m}$ ;
3. the world population, about $8\,100\,000\,000$ ;
4. a duration of $0.005\,20\,\mathrm{s}$ .

**Solution of Exercise 1.2.**

*1.* $149\,600\,000\,\mathrm{km} = 1.496 \times 10^{11}\,\mathrm{m}$: $4$ [significant figures](#def-g10-orders-of-magnitude-sigfig). *2.* $1.06 \times 10^{-10}\,\mathrm{m}$: $3$ [significant figures](#def-g10-orders-of-magnitude-sigfig) (leading zeros never count). *3.* $8.1 \times 10^{9}$: $2$ [significant figures](#def-g10-orders-of-magnitude-sigfig). *4.* $5.20 \times 10^{-3}\,\mathrm{s}$: $3$ [significant figures](#def-g10-orders-of-magnitude-sigfig) (the trailing zero is a promise).

**Exercise 1.3 ★.**

Compute without a calculator, giving each result in [scientific notation](#def-g10-orders-of-magnitude-scinot):

$$
(3\times10^{8})\times(2\times10^{-5}), \qquad
\frac{8\times10^{4}}{4\times10^{-3}}, \qquad
(5\times10^{6})^{2}, \qquad
\frac{(4\times10^{-3})\times(3\times10^{-9})}{6\times10^{-7}} .
$$

**Solution of Exercise 1.3.**

[Mantissas](#def-g10-orders-of-magnitude-scinot) and [exponents](#def-g10-orders-of-magnitude-scinot) separately ([Proposition 1.6](#prop-g10-orders-of-magnitude-powers)):

$$
3 \times 2 \times 10^{8-5} = 6 \times 10^{3}, \qquad
\tfrac{8}{4} \times 10^{4-(-3)} = 2 \times 10^{7},
$$

$$
5^{2} \times 10^{12} = 2.5 \times 10^{13}, \qquad
\tfrac{4 \times 3}{6} \times 10^{-3-9+7} = 2 \times 10^{-5} .
$$

**Exercise 1.4 ★.**

Give the [order of magnitude](#def-g10-orders-of-magnitude-oom), with its [unit](#def-g10-orders-of-magnitude-unit), of: a human height of $1.7\,\mathrm{m}$; Mount Everest, $8848\,\mathrm{m}$; an *E. coli* bacterium, $2 \times 10^{-6}\,\mathrm{m}$; the mass of the Earth, $5.97 \times 10^{24}\,\mathrm{kg}$.

**Solution of Exercise 1.4.**

Human: $1.7 < 5$, order $10^{0}\,\mathrm{m}$. Everest: $8848\,\mathrm{m} = 8.848 \times 10^{3}\,\mathrm{m}$ and $8.848 \geq 5$: order $10^{4}\,\mathrm{m}$. Bacterium: order $10^{-6}\,\mathrm{m}$. Earth: $5.97 \geq 5$, order $10^{25}\,\mathrm{kg}$.

**Exercise 1.5 ★.**

A ruler is graduated in millimetres. You measure a pencil at $127\,\mathrm{mm}$.

1. State the result with its [absolute uncertainty](#def-g10-orders-of-magnitude-uncertainty) .
2. Compute the [relative uncertainty](#def-g10-orders-of-magnitude-uncertainty) .
3. The same ruler measures a $12\,\mathrm{mm}$ eraser. Which of the two measurements is the more precise, and by what factor?

**Solution of Exercise 1.5.**

*1.* Half a graduation: $L = (127.0 \pm 0.5)\,\mathrm{mm}$. *2.* $\Delta L / L = 0.5/127 \approx 0.4\%$. *3.* Eraser: $0.5/12 \approx 4\%$. The pencil measurement is about ten times more precise — same ruler, same [absolute uncertainty](#def-g10-orders-of-magnitude-uncertainty), ten times longer object.

**Exercise 1.6 ★★.**

Using $c = 3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s}$ and $1\,\mathrm{ly} = 9.47 \times 10^{15}\,\mathrm{m}$:

1. Express in [metres](#def-g10-orders-of-magnitude-unit) the distances to Proxima Centauri ( $4.24\,\mathrm{ly}$ ) and to Sirius ( $8.6\,\mathrm{ly}$ ).
2. The probe *Voyager 1* is about $2.4 \times 10^{13}\,\mathrm{m}$ from Earth. How long does its radio signal, travelling at $c$ , take to reach us? Express the answer in hours.

**Solution of Exercise 1.6.**

*1.* Proxima: $4.24 \times 9.47 \times 10^{15}\,\mathrm{m} = 4.01 \times 10^{16}\,\mathrm{m}$. Sirius: $8.6 \times 9.47 \times 10^{15}\,\mathrm{m} = 8.1 \times 10^{16}\,\mathrm{m}$ (two [significant figures](#def-g10-orders-of-magnitude-sigfig), like the input). *2.* $t = d/c = 2.4 \times 10^{13}\,\mathrm{m} / 3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s}
= 8.0 \times 10^{4}\,\mathrm{s}$, i.e. $8.0 \times 10^{4}/3600 \approx 22\,\mathrm{h}$: almost a full day for every message from the probe.

**Exercise 1.7 ★★.**

How long does light take to reach Earth from the Moon ($3.84 \times 10^{8}\,\mathrm{m}$), from the Sun ($1.496 \times 10^{11}\,\mathrm{m}$) and from Neptune ($4.50 \times 10^{12}\,\mathrm{m}$)? Give each answer in a sensible [unit](#def-g10-orders-of-magnitude-unit), and complete the sentence: “When you look at Neptune, you see it as it was…”

**Solution of Exercise 1.7.**

$t = d/c$ each time. Moon: $3.84 \times 10^{8}\,\mathrm{m}/3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s} = 1.28\,\mathrm{s}$. Sun: $1.496 \times 10^{11}\,\mathrm{m}/3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s} = 499\,\mathrm{s} \approx
8.3\,\mathrm{min}$. Neptune: $4.50 \times 10^{12}\,\mathrm{m}/3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s} = 1.50 \times 10^{4}\,\mathrm{s} \approx
4.2\,\mathrm{h}$. When you look at Neptune, you see it as it was about four hours ago — every telescope is a mild time machine.

**Exercise 1.8 ★★.**

A ream of $500$ sheets of paper, measured with a millimetre ruler, is $52.0\,\mathrm{mm}$ thick, with uncertainty $\pm0.5\,\mathrm{mm}$.

1. Deduce the thickness of one sheet, with its [absolute uncertainty](#def-g10-orders-of-magnitude-uncertainty) .
2. What is the [relative uncertainty](#def-g10-orders-of-magnitude-uncertainty) of that thickness?
3. Why is measuring the ream enormously better than measuring one sheet directly with the same ruler? Quantify.

**Solution of Exercise 1.8.**

*1.* One sheet: $52.0\,\mathrm{mm}/500 = 0.104\,\mathrm{mm}
= 1.04 \times 10^{-4}\,\mathrm{m}$. The uncertainty divides too: $0.5\,\mathrm{mm}/500 = 0.001\,\mathrm{mm}$, so $t = (104 \pm 1)\,\text{µ}\mathrm{m}$. *2.* $1/104 \approx 1\%$. *3.* Measuring one sheet directly would give $(0.1 \pm 0.5)\,\mathrm{mm}$: a [relative uncertainty](#def-g10-orders-of-magnitude-uncertainty) of about $500\%$ — the ruler cannot even prove the sheet exists. Stacking $500$ sheets multiplies the measured length by $500$ while the ruler’s [absolute uncertainty](#def-g10-orders-of-magnitude-uncertainty) stays fixed: the [relative uncertainty](#def-g10-orders-of-magnitude-uncertainty) shrinks by that same factor $500$.

**Exercise 1.9 ★★.**

Take $2 \times 10^{-10}\,\mathrm{m}$ as the diameter of an atom. How many atoms, side by side, span: a bacterium of $2.0\,\text{µ}\mathrm{m}$; a hair of $70\,\text{µ}\mathrm{m}$; a human of $1.7\,\mathrm{m}$? Give the last answer as an [order of magnitude](#def-g10-orders-of-magnitude-oom) too.

**Solution of Exercise 1.9.**

Divide each length by $2 \times 10^{-10}\,\mathrm{m}$. Bacterium: $2.0 \times 10^{-6}\,\mathrm{m}/2 \times 10^{-10}\,\mathrm{m} = 1.0 \times 10^{4}$ atoms. Hair: $7.0 \times 10^{-5}\,\mathrm{m}/2 \times 10^{-10}\,\mathrm{m} = 3.5 \times 10^{5}$. Human: $1.7/2 \times 10^{-10} = 8.5 \times 10^{9}$, [order of magnitude](#def-g10-orders-of-magnitude-oom) $10^{10}$: ten billion atoms head to toe.

**Exercise 1.10 ★★.**

A scale model represents the Sun (diameter $1.39 \times 10^{9}\,\mathrm{m}$) by a football of diameter $22\,\mathrm{cm}$.

1. Compute the scale factor of the model.
2. Find the model diameter of the Earth ( $1.27 \times 10^{7}\,\mathrm{m}$ ) and its model distance from the football (real distance $1.496 \times 10^{11}\,\mathrm{m}$ ).
3. How far from the model Earth is the model Moon (real distance $3.84 \times 10^{8}\,\mathrm{m}$ )? And how far away is model Neptune (real distance $4.50 \times 10^{12}\,\mathrm{m}$ )?

**Solution of Exercise 1.10.**

*1.* $s = 0.22\,\mathrm{m}/1.39 \times 10^{9}\,\mathrm{m} = 1.58 \times 10^{-10}$. *2.* Earth: $1.27 \times 10^{7}\,\mathrm{m} \times 1.58 \times 10^{-10} = 2.0 \times 10^{-3}\,\mathrm{m} =
2.0\,\mathrm{mm}$ — a peppercorn — orbiting at $1.496 \times 10^{11}\,\mathrm{m} \times 1.58 \times 10^{-10} = 23.7\,\mathrm{m} \approx
24\,\mathrm{m}$ from the football. *3.* Moon: $3.84 \times 10^{8}\,\mathrm{m} \times 1.58 \times 10^{-10} = 6.1\,\mathrm{cm}$ from the peppercorn. Neptune: $4.50 \times 10^{12}\,\mathrm{m} \times 1.58 \times 10^{-10} \approx 710\,\mathrm{m}$: the model does not fit in the schoolyard.

**Exercise 1.11 ★★.**

[Significant figures](#def-g10-orders-of-magnitude-sigfig) at work.

1. An A4 sheet measures $21.0\,\mathrm{cm}$ by $29.7\,\mathrm{cm}$ . Give its area with the correct number of [significant figures](#def-g10-orders-of-magnitude-sigfig) .
2. A sprinter covers $100.0\,\mathrm{m}$ in $12.3\,\mathrm{s}$ . Give the average speed correctly rounded.
3. Explain in one sentence what would be dishonest about announcing the area as $623.70\,\mathrm{cm}^{2}$ .

**Solution of Exercise 1.11.**

*1.* $21.0 \times 29.7 = 623.7\,\mathrm{cm}^{2}$, rounded to the three [significant figures](#def-g10-orders-of-magnitude-sigfig) of the inputs: $624\,\mathrm{cm}^{2}$. *2.* $v = 100.0\,\mathrm{m}/12.3\,\mathrm{s} = 8.13\,\mathrm{m}/\mathrm{s}$ (three figures, set by the time). *3.* Five [significant figures](#def-g10-orders-of-magnitude-sigfig) would claim the area to $0.01\,\mathrm{cm}^{2}$, a precision the millimetre-level inputs never delivered — a forged decimal is still a forgery.

**Exercise 1.12 ★★★.**

A drop of oil of volume $1.0\,\mathrm{mm}^{3}$ is deposited on still water and spreads into a circular film of diameter $1.1\,\mathrm{m}$ — a film that later chapters will show to be one molecule thick.

1. Compute the area of the film, then its thickness.
2. Deduce an [order of magnitude](#def-g10-orders-of-magnitude-oom) for the size of a molecule, and check it against the atom rung of the ladder.

(This back-of-the-envelope experiment, first tried by Benjamin Franklin on a London pond, was one of humanity’s first honest measures of the molecular world.)

**Solution of Exercise 1.12.**

*1.* Radius $r = 0.55\,\mathrm{m}$, area $A = \pi r^{2} = \pi \times 0.55^{2} \approx 0.95\,\mathrm{m}^{2}$. Volume $V = 1.0\,\mathrm{mm}^{3} = 1.0 \times 10^{-9}\,\mathrm{m}^{3}$, and a film is (area) $\times$ (thickness), so

$$
e = \frac{V}{A} = \frac{1.0 \times 10^{-9}\,\mathrm{m}^{3}}{0.95\,\mathrm{m}^{2}}
= 1.1 \times 10^{-9}\,\mathrm{m} .
$$

*2.* A molecule is of order $10^{-9}\,\mathrm{m}$ — one rung above the atom’s $10^{-10}\,\mathrm{m}$, consistent with a molecule being a small cluster of atoms. Franklin’s teaspoon of oil calmed half an acre of pond and, without his knowing it, measured the nanometre.

**Exercise 1.13 ★★★.**

Estimate the number of heartbeats in a human lifetime. State your assumptions (resting heart rate, life span), keep the arithmetic to powers of ten and one digit of [mantissa](#def-g10-orders-of-magnitude-scinot), and give the final answer as an [order of magnitude](#def-g10-orders-of-magnitude-oom) only. Why would quoting it to four [significant figures](#def-g10-orders-of-magnitude-sigfig) be meaningless?

**Solution of Exercise 1.13.**

Assumptions: about $70$ beats per minute at rest, a life of $80$ years. Per day: $70 \times 60 \times 24 \approx 1 \times 10^{5}$ beats. Per year: $1 \times 10^{5} \times 365 \approx 4 \times 10^{7}$. Per life: $4 \times 10^{7} \times 80 \approx 3 \times 10^{9}$ — [order of magnitude](#def-g10-orders-of-magnitude-oom) $10^{9}$, a few billion heartbeats. Four [significant figures](#def-g10-orders-of-magnitude-sigfig) would pretend to know a heart rate, minute by minute, for eighty years: the inputs are order-of-magnitude guesses, and no output can outrank its inputs ([Method 1.9](#met-g10-orders-of-magnitude-sigfig)).

**Exercise 1.14 ★★★.**

A sheet of paper is $0.10\,\mathrm{mm}$ thick, and each fold doubles the thickness of the stack. Using $2^{10} \approx 10^{3}$:

1. After how many folds would the stack overtop Mount Everest ( $8848\,\mathrm{m}$ )?
2. After how many folds would it reach the Moon ( $3.84 \times 10^{8}\,\mathrm{m}$ )?
3. In practice a sheet cannot be folded more than about seven times. Does that invalidate the arithmetic, or only the experiment?

**Solution of Exercise 1.14.**

After $n$ folds the thickness is $2^{n} \times 1.0 \times 10^{-4}\,\mathrm{m}$. *1.* Need $2^{n} \geq 8848/1.0 \times 10^{-4} = 8.8 \times 10^{7}$. Since $2^{26} \approx 6.7 \times 10^{7}$ falls short and $2^{27} \approx 1.3 \times 10^{8}$ suffices: $27$ folds (stack $\approx 13\,\mathrm{km}$). *2.* Need $2^{n} \geq 3.84 \times 10^{12}$: $2^{41} \approx
2.2 \times 10^{12}$ is short, $2^{42} \approx 4.4 \times 10^{12}$ reaches — $42$ folds, stack $4.4 \times 10^{8}\,\mathrm{m}$, comfortably past the Moon. *3.* Only the experiment: each fold halves the area, and after seven folds the stack is thicker than it is wide. The arithmetic of doubling is untouched — exponential growth simply outruns what paper (and intuition) can follow.

**Exercise 1.15 ★★★.**

Laser ranging gives the Earth–Moon distance as $3.84 \times 10^{8}\,\mathrm{m} \pm 3\,\mathrm{cm}$; a good ruler gives a table as $1.000\,\mathrm{m} \pm 1\,\mathrm{mm}$.

1. Compute both relative uncertainties. Which measurement is the more precise, and by what factor?
2. With what [absolute uncertainty](#def-g10-orders-of-magnitude-uncertainty) would you need to measure the table to match the Moon measurement’s relative precision? Compare that length with the size of an atom, and conclude with due respect.

**Solution of Exercise 1.15.**

*1.* Moon: $0.03\,\mathrm{m}/3.84 \times 10^{8}\,\mathrm{m} = 7.8 \times 10^{-11}$. Table: $0.001\,\mathrm{m}/1.000\,\mathrm{m} = 1.0 \times 10^{-3}$. The Moon measurement is more precise by a factor $1.0 \times 10^{-3}/7.8 \times 10^{-11} \approx 1.3 \times 10^{7}$ — over ten million. *2.* Matching $7.8 \times 10^{-11}$ on a [one-metre](#def-g10-orders-of-magnitude-unit) table means $\Delta x = 7.8 \times 10^{-11}\,\mathrm{m}$, smaller than one atom ($\approx 10^{-10}\,\mathrm{m}$): the table’s edge is not even *defined* that sharply. Relatively speaking, the Earth–Moon laser distance is one of the finest measurements our species owns.

## 1.6 Problem: From the atom to Andromeda

**Problem 1.1.**

Weekend problem — a single grain of sand sizes the atom, the Solar System, the galaxy and the observable universe, and locates you on the ladder between them

A grain of sand is the humblest object in physics, and this weekend it works overtime: first we count its atoms, then we shrink the Sun to its size and pace out the cosmos, then we let light do the surveying, and finally we count the atoms in *you*. Data, used throughout: grain diameter $0.5\,\mathrm{mm}$; atom diameter $2.5 \times 10^{-10}\,\mathrm{m}$; density of sand $2500\,\mathrm{kg}/\mathrm{m}^{3}$; diameters: Sun $1.39 \times 10^{9}\,\mathrm{m}$, Earth $1.27 \times 10^{7}\,\mathrm{m}$, Milky Way $9.5 \times 10^{20}\,\mathrm{m}$, observable universe $8.8 \times 10^{26}\,\mathrm{m}$; distances from us: Moon $3.84 \times 10^{8}\,\mathrm{m}$, Sun $1.496 \times 10^{11}\,\mathrm{m}$, Neptune $4.5 \times 10^{12}\,\mathrm{m}$, Proxima Centauri $4.0 \times 10^{16}\,\mathrm{m}$, Andromeda galaxy $2.4 \times 10^{22}\,\mathrm{m}$; $c = 3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s}$; a water molecule has mass $3.0 \times 10^{-26}\,\mathrm{kg}$ and contains three atoms.

**Part I — Anatomy of the grain.**

1. Write the grain diameter and the atom diameter in [metres](#def-g10-orders-of-magnitude-unit) , in [scientific notation](#def-g10-orders-of-magnitude-scinot) , and name the SI [prefix](#def-g10-orders-of-magnitude-prefixes) each is closest to.
2. How many atoms sit side by side across one grain diameter?
3. Model the grain as a cube of side $0.5\,\mathrm{mm}$ packed with atoms. Estimate the number of atoms in the grain, as an [order of magnitude](#def-g10-orders-of-magnitude-oom) .
4. Compute the volume of that cube, then the mass of the grain. Express the mass in milligrams.
5. Sanity-check the model: divide the grain’s mass by its number of atoms and compare with the known [order of magnitude](#def-g10-orders-of-magnitude-oom) of atomic masses (a few $10^{-26}\,\mathrm{kg}$ ). Verdict?

**Part II — The Sun as a grain of sand.** We build a scale model of the cosmos in which the Sun is the grain: every model size equals the real size times a factor $s$.

6. Compute the scale factor $s$ .
7. In the model, find the Earth’s diameter and its distance from the grain-Sun. What object of Part I’s world has roughly the model Earth’s size?
8. How far from the grain does model Neptune orbit? What piece of furniture would hold the entire planetary system?
9. How far away is the model Proxima Centauri?
10. Two grains of sand, $14\,\mathrm{km}$ apart, and almost nothing in between: state in one or two sentences what the model reveals about how empty the galaxy is.

**Part III — Light does the surveying.**

11. How long does light take to cross the real grain of sand?
12. How long does light take to reach us from the Moon, and from the Sun?
13. Recompute the [light-year](#def-g10-orders-of-magnitude-lightyear) in [metres](#def-g10-orders-of-magnitude-unit) from $c$ and the length of the year, and verify that the Proxima distance in the data corresponds to about $4.2\,\mathrm{ly}$ .
14. Convert the Andromeda distance to [light-years](#def-g10-orders-of-magnitude-lightyear) . Roughly when did the light now entering your eye leave Andromeda, and what was walking the Earth at the time?
15. How far does light travel in one nanosecond? A processor clocked at $3\,\mathrm{GHz}$ starts an operation every third of a nanosecond: explain in one sentence why a fast computer must be a small computer.

**Part IV — You, between atom and Andromeda.**

16. A human is roughly $70\,\mathrm{kg}$ of water. Using the data, estimate the average mass of one atom in water, then the number of atoms in a human.
17. Compare that count with the atoms in the grain (question 3) and with the roughly $2\times10^{23}$ stars of the observable universe. Give both factors.
18. On the ladder, are you nearer the atom or the observable universe? Compare the ratios $\text{(you)}/\text{(atom)}$ and $\text{(universe)}/\text{(you)}$ , taking $1.7\,\mathrm{m}$ for you.
19. Find the size $x$ sitting exactly halfway up the ladder between the nucleus ( $10^{-15}\,\mathrm{m}$ ) and the observable universe: $x$ must satisfy $x / 10^{-15} = 10^{26.9} / x$ (using $8.8 \times 10^{26}\,\mathrm{m} \approx 10^{26.9}\,\mathrm{m}$ ). What Solar-System object happens to have just that size?
20. The punchline. Shrink the observable universe by the Part II factor $s$ , so that the Sun is a grain of sand. Give the model universe’s diameter in [metres](#def-g10-orders-of-magnitude-unit) , then in [astronomical units](#def-g10-orders-of-magnitude-lightyear) , and conclude in one sentence: even with every star turned to a sand grain, the universe overflows every human scale — only powers of ten hold it.

**Solution of Problem 1.1.**

**1.** Grain: $0.5\,\mathrm{mm} = 5 \times 10^{-4}\,\mathrm{m}$, on the milli scale; atom: $2.5 \times 10^{-10}\,\mathrm{m} = 0.25\,\mathrm{nm}$, on the nano scale.

**2.** $5 \times 10^{-4}\,\mathrm{m}/2.5 \times 10^{-10}\,\mathrm{m} = 2.0 \times 10^{6}$: two million atoms across.

**3.** A cube of $2 \times 10^{6}$ atoms per edge holds $(2\times10^{6})^{3} = 8 \times 10^{18}$ atoms: [order of magnitude](#def-g10-orders-of-magnitude-oom) $10^{19}$.

**4.** $V = (5 \times 10^{-4}\,\mathrm{m})^{3} = 1.25 \times 10^{-10}\,\mathrm{m}^{3}$, so $m = \rho V = 2500\,\mathrm{kg}/\mathrm{m}^{3} \times 1.25 \times 10^{-10}\,\mathrm{m}^{3}
= 3.1 \times 10^{-7}\,\mathrm{kg} = 0.31\,\mathrm{mg}$.

**5.** Mass per atom: $3.1 \times 10^{-7}\,\mathrm{kg}/(8\times10^{18}) = 3.9 \times 10^{-26}\,\mathrm{kg}$ — squarely in the “few $10^{-26}\,\mathrm{kg}$” range. The naive cube of atoms reproduces real atomic masses: the model passes the sanity check ([Method 1.15](#met-g10-orders-of-magnitude-sanity)) with honors.

**6.** $s = 5 \times 10^{-4}\,\mathrm{m}/1.39 \times 10^{9}\,\mathrm{m} = 3.6 \times 10^{-13}$.

**7.** Model Earth: diameter $1.27 \times 10^{7}\,\mathrm{m} \times 3.6 \times 10^{-13} = 4.6 \times 10^{-6}\,\mathrm{m}$ — the size of a bacterium — at distance $1.496 \times 10^{11}\,\mathrm{m} \times 3.6 \times 10^{-13} = 5.4\,\mathrm{cm}$ from the grain: the Earth is a microbe five centimetres from a grain of sand.

**8.** $4.5 \times 10^{12}\,\mathrm{m} \times 3.6 \times 10^{-13} = 1.6\,\mathrm{m}$: the entire planetary system orbits within a dining table.

**9.** $4.0 \times 10^{16}\,\mathrm{m} \times 3.6 \times 10^{-13} = 1.4 \times 10^{4}\,\mathrm{m}
= 14\,\mathrm{km}$.

**10.** The nearest star to our table-top Solar System is another grain of sand fourteen kilometres away, with essentially nothing in between: the galaxy is overwhelmingly empty space, which is why collisions between stars are almost unheard of.

**11.** $t = 5 \times 10^{-4}\,\mathrm{m}/3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s} = 1.7 \times 10^{-12}\,\mathrm{s}$ — under two picoseconds.

**12.** Moon: $3.84 \times 10^{8}\,\mathrm{m}/3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s} =
1.28\,\mathrm{s}$. Sun: $1.496 \times 10^{11}\,\mathrm{m}/3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s} =
499\,\mathrm{s} \approx 8.3\,\mathrm{min}$: sunlight is always eight minutes old.

**13.** One year is $365.25 \times 86400 = 3.156 \times 10^{7}\,\mathrm{s}$, so $1\,\mathrm{ly} = 3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s} \times 3.156 \times 10^{7}\,\mathrm{s}
= 9.47 \times 10^{15}\,\mathrm{m}$; then $4.0 \times 10^{16}\,\mathrm{m}/9.47 \times 10^{15}\,\mathrm{m} = 4.2$: the data distance is indeed about $4.2\,\mathrm{ly}$.

**14.** $2.4 \times 10^{22}\,\mathrm{m}/9.47 \times 10^{15}\,\mathrm{m} = 2.5 \times 10^{6}$: two and a half million [light-years](#def-g10-orders-of-magnitude-lightyear). That light left Andromeda about $2.5$ million years ago, when the first members of the genus *Homo* were learning to knap stones — and no *Homo sapiens* yet existed anywhere.

**15.** $3.00 \times 10^{8}\,\mathrm{m}/\mathrm{s} \times 1 \times 10^{-9}\,\mathrm{s} = 0.30\,\mathrm{m}$. In a third of a nanosecond a signal covers at most about $10\,\mathrm{cm}$, so any two parts of the machine that must talk within one clock tick have to sit within ten centimetres of each other: speed caps size.

**16.** Average atom in water: $3.0 \times 10^{-26}\,\mathrm{kg}/3 = 1.0 \times 10^{-26}\,\mathrm{kg}$. Number of atoms: $70\,\mathrm{kg}/1.0 \times 10^{-26}\,\mathrm{kg} = 7 \times 10^{27}$.

**17.** Against the grain: $7 \times 10^{27}/8 \times 10^{18} \approx 10^{9}$ — you contain a billion grains’ worth of atoms. Against the stars: $7 \times 10^{27}/2 \times 10^{23} = 3.5 \times 10^{4}$ — your atoms outnumber all the stars of the observable universe thirty-five thousand to one.

**18.** $\text{(you)}/\text{(atom)} =
1.7\,\mathrm{m}/2.5 \times 10^{-10}\,\mathrm{m} \approx 7 \times 10^{9} \approx 10^{10}$, while $\text{(universe)}/\text{(you)} =
8.8 \times 10^{26}\,\mathrm{m}/1.7\,\mathrm{m} \approx 5 \times 10^{26}$. On the ladder you stand about ten rungs above the atom and nearly twenty-seven below the universe: multiplicatively, humans live very close to their atoms.

**19.** The condition gives $x^{2} = 10^{-15} \times 10^{26.9} = 10^{11.9}$, so $x = 10^{5.95} \approx 9 \times 10^{5}\,\mathrm{m} \approx 900\,\mathrm{km}$ — almost exactly the diameter of Ceres, the largest asteroid ($\approx 940\,\mathrm{km}$). Halfway up the ladder between a nucleus and the cosmos sits a modest dwarf planet.

**20.** $8.8 \times 10^{26}\,\mathrm{m} \times 3.6 \times 10^{-13} = 3.2 \times 10^{14}\,\mathrm{m}$, i.e. $3.2 \times 10^{14}\,\mathrm{m}/1.496 \times 10^{11}\,\mathrm{m} \approx 2.1 \times 10^{3}$ [astronomical units](#def-g10-orders-of-magnitude-lightyear). Punchline: shrink the cosmos until the Sun is a grain of sand, and the observable universe still spans two thousand times the real Earth–Sun distance — no scale model brings the universe down to human size; only powers of ten can carry it.