M1 Numbers, units and estimation
handle huge and tiny numbers, units and quick estimates with confidence.
Before you begin: school arithmetic. Start here after the preface.
Watch first
Chapters
- 0:00 From a proton to the universe
- 1:11 Powers of ten
- 2:34 Scientific notation
- 4:27 A ladder of prefixes
- 6:22 A number needs a unit
- 7:42 Where the metre came from
- 9:09 The kilogram in a vault
- 10:47 Converting units safely
- 12:44 Dimensional analysis
- 14:21 A formula from units alone
- 15:57 Fermi's paper scraps
- 17:05 How to estimate anything
- 18:27 Estimates for everyday life
- 19:47 Accuracy and precision
- 21:14 Random and systematic errors
- 22:34 Significant figures
- 23:46 Common mistakes
- 25:00 Recap and what's next
Notes
In this chapter
- Write very large and very small numbers in scientific notation, and multiply and divide them by adding and subtracting powers.
- Use the metric prefixes, from nano to giga.
- Convert units safely with conversion factors, including squared and cubed units.
- Use dimensional analysis to check an equation, and even to find the form of a formula.
- Make Fermi estimates: break a "how many?" question into steps and land within a factor of ten.
- Tell accuracy from precision and random from systematic error, and report results with error bars and sensible significant figures.
Powers of ten
FIRST, MAKE A PREDICTION
TRY IT / FOLLOW THE REASONING
Move the power down one step at a time. Describe what happens to the value, then move through zero into positive powers.
Power of ten: 0
- Value
- 1
Model assumptions
A reference value of 1. Negative exponents still give positive numbers.
MAKE THE CONNECTION
Key idea
A power of ten counts zeros. A negative power is a small number, not a negative one.
\(10^n\) means ten multiplied by itself \(n\) times. For whole positive powers, \(n\) is the number of zeros after the 1: \(10^6 = 1\,000\,000\). Each step down divides by ten, so \(10^0 = 1\), \(10^{-1} = 0.1\) and \(10^{-3} = 0.001\).
Powers of ten
Checkpoint: Powers of ten (1 of 2)
Question 1 of 2 Commit to an answer first, then look.
Checkpoint: Powers of ten (2 of 2)
Question 2 of 2 Commit to an answer first, then look.
Scientific notation
FIRST, MAKE A PREDICTION
TRY IT / FOLLOW THE REASONING
Write 300 000 000 as 3, then record how many multiplications by ten restore the original. Try the same reasoning with 0.003 before opening the explanation.
MAKE THE CONNECTION
A number between 1 and 10, times a power of ten: \(300\,000\,000 = 3 \times 10^8\). To convert, move the decimal point until one digit is in front of it and count the places: left gives a positive power, right gives a negative one.
If the front number comes out at 10 or more, tidy it up: \(20\times10^5 = 2\times10^6\).
Checkpoint: Scientific notation (1 of 2)
Question 1 of 2 Commit to an answer first, then look.
Checkpoint: Scientific notation (2 of 2)
Question 2 of 2 Commit to an answer first, then look.
Multiplying and dividing
FIRST, MAKE A PREDICTION
TRY IT / FOLLOW THE REASONING
Expand 10³ × 10² into individual factors of ten. Count the factors, then compare multiplication with cancelling factors in a division.
MAKE THE CONNECTION
- \(a, b\): the front numbers, between 1 and 10
- \(m, n\): the powers of ten
Checkpoint: Multiplying and dividing (1 of 3)
Question 1 of 3 Commit to an answer first, then look.
Checkpoint: Multiplying and dividing (2 of 3)
Question 2 of 3 Commit to an answer first, then look.
Checkpoint: Multiplying and dividing (3 of 3)
Question 3 of 3 Commit to an answer first, then look.
Metric prefixes
FIRST, MAKE A PREDICTION
TRY IT / FOLLOW THE REASONING
Use the prefix table to write both lengths in metres. Circle the exponent before comparing the leading numbers. Find another pair where the bigger written number is the smaller length.
| Prefix | Symbol | Power | Example |
|---|---|---|---|
| giga | G | \(10^9\) | a gigabyte |
| mega | M | \(10^6\) | a megawatt |
| kilo | k | \(10^3\) | a kilometre |
| milli | m | \(10^{-3}\) | a millimetre |
| micro | µ | \(10^{-6}\) | a micrometre (a hair is about 70 µm wide) |
| nano | n | \(10^{-9}\) | a nanometre |
MAKE THE CONNECTION
2 mm is 2000 micrometres, so it is four times as long as 500 micrometres.
Checkpoint: Metric prefixes (1 of 2)
Question 1 of 2 Commit to an answer first, then look.
Checkpoint: Metric prefixes (2 of 2)
Question 2 of 2 Commit to an answer first, then look.
Forty-two powers of ten
FIRST, MAKE A PREDICTION
TRY IT / FOLLOW THE REASONING
Place the proton, a metre and the observable universe on an exponent line. Compare the ratio of the largest to the smallest without writing out either length.
MAKE THE CONNECTION
From a proton (about \(10^{-15}\) m) to the observable universe (about \(10^{27}\) m) is a factor of \(10^{42}\).
Forty-two powers of ten
Checkpoint: Forty-two powers of ten
Question Commit to an answer first, then look.
Units
FIRST, MAKE A PREDICTION
TRY IT / FOLLOW THE REASONING
Give three different physical meanings to the number 12 by changing its unit. Use the SI list to identify which measurements are lengths, times and masses.
MAKE THE CONNECTION
Key idea
A number without a unit is incomplete.
The international system (SI) has seven base units: the second, metre, kilogram, ampere, kelvin, mole and candela. Since 20 May 2019, all seven have been defined by fixing seven constants of nature, such as the speed of light and the Planck constant. Every other unit (the newton, the watt, the pascal…) is built from these seven.
Checkpoint: Units (1 of 2)
Question 1 of 2 Commit to an answer first, then look.
Checkpoint: Units (2 of 2)
Question 2 of 2 Commit to an answer first, then look.
Converting units
FIRST, MAKE A PREDICTION
TRY IT / FOLLOW THE REASONING
Write 1000 m / 1 km as a fraction equal to one. Choose its orientation so kilometres cancel in 2 km, then reverse the conversion as a check.
MAKE THE CONNECTION
Key idea
A conversion factor is a fraction equal to one, like \(\dfrac{1000\ \text{m}}{1\ \text{km}}\). Multiply by it, and cancel units like algebra.
Converting units
Checkpoint: Converting units
Question Commit to an answer first, then look.
Squared and cubed units
FIRST, MAKE A PREDICTION
TRY IT / FOLLOW THE REASONING
Change the length multiplier and compare the area and volume multipliers. Then use the same reasoning for a 100-fold change of length unit.
Length multiplier: 1 ×
- Area multiplier
- 1 ×
- Volume multiplier
- 1 ×
Model assumptions
Similar shapes: every length changes by the same factor. Bars use a common scale.
MAKE THE CONNECTION
For squared or cubed units, square or cube the factor: \(1\ \text{m}^2 = 10\,000\ \text{cm}^2\), and \(1\ \text{m}^3 = 10^6\ \text{cm}^3 = 1000\) litres.
Checkpoint: Squared and cubed units (1 of 2)
Question 1 of 2 Commit to an answer first, then look.
Checkpoint: Squared and cubed units (2 of 2)
Question 2 of 2 Commit to an answer first, then look.
Density: a derived unit
FIRST, MAKE A PREDICTION
TRY IT / FOLLOW THE REASONING
Imagine 1 litre of water, then join it to an identical litre. Calculate mass divided by volume before and after joining them, keeping the units visible.
MAKE THE CONNECTION
Many useful quantities are ratios of two others, and their units are built the same way. Density is mass per unit volume, \(\rho = m/V\), in kilograms per cubic metre (kg/m³).
- Water is about 1000 kg/m³ (one litre has a mass of one kilogram).
- Air is about 1.2 kg/m³.
- Steel is about 7850 kg/m³.
Density: a derived unit
A density-units story: the Gimli Glider
The Gimli Glider (see History) is a density-units story: the fuel was worked out with 1.77 pounds per litre where 0.803 kilograms per litre was needed, so the plane took off with about half the fuel it needed.
Density: a derived unit
Density is taught properly, with practice, in P6 · Matter in bulk.
Checkpoint: Density: a derived unit (1 of 2)
Question 1 of 2 Commit to an answer first, then look.
Checkpoint: Density: a derived unit (2 of 2)
Question 2 of 2 Commit to an answer first, then look.
Dimensional analysis
FIRST, MAKE A PREDICTION
TRY IT / FOLLOW THE REASONING
Write the units beside each candidate expression. Cross out the impossible ones, then ask whether having the right units is enough to guarantee the right numerical factor.
MAKE THE CONNECTION
Key idea
Every quantity has a dimension: length \(L\), mass \(M\), time \(T\) and so on. You can only add or compare things with the same dimensions, so both sides of a correct equation have the same dimensions.
- \(d = \tfrac12 g t^2\): \([g t^2] = \dfrac{L}{T^2}\times T^2 = L\). ✓
- \(d = g t\): \([g t] = \dfrac{L}{T}\), a speed, not a length. ✗
Checkpoint: Dimensional analysis (1 of 2)
Question 1 of 2 Commit to an answer first, then look.
Checkpoint: Dimensional analysis (2 of 2)
Question 2 of 2 Commit to an answer first, then look.
A formula from units alone
FIRST, MAKE A PREDICTION
TRY IT / FOLLOW THE REASONING
Replace L and g by their dimensions. Find the combination that leaves only time, then compare with the full pendulum formula to identify what units alone could not supply.
MAKE THE CONNECTION
Worked number: the pendulum
The period \(T\) can depend only on \(L\), \(m\) and \(g\). Nothing else contains mass, so \(m\) can't appear; and \(\sqrt{L/g}\) has dimension \(T\). So \(T \propto \sqrt{L/g}\).
The full result is \(T = 2\pi\sqrt{L/g}\), about 2 s for a 1 m pendulum. Units can't supply the \(2\pi\).
A formula from units alone
A formula from units alone
Myth: a heavier pendulum swings more slowly
The mass drops out. For small swings, heavy and light pendulums of the same length keep time together, as long as air resistance is small.
Checkpoint: A formula from units alone (1 of 2)
Question 1 of 2 Commit to an answer first, then look.
Checkpoint: A formula from units alone (2 of 2)
Question 2 of 2 Commit to an answer first, then look.
Fermi estimates
FIRST, MAKE A PREDICTION
TRY IT / FOLLOW THE REASONING
Build your own factor chain for the tuners question. Attach a unit to each factor, cancel down to people, and test which assumption changes your result most.
MAKE THE CONNECTION
Key idea
Break a question you can't answer into factors you can guess, round each, keep the units, multiply with powers of ten, and check that the answer is reasonable. The errors partly cancel, so the answer usually lands within a factor of ten.
For example:
- Piano tuners in 1940s Chicago: about 100.
- The air in a 4 × 5 × 2.5 m room: about 60 kg.
- Breaths in a lifetime: about \(6\times10^8\).
- Heartbeats in a lifetime: about \(3\times10^9\), roughly five per breath.
Fermi estimates
Checkpoint: Fermi estimates (1 of 2)
Question 1 of 2 Commit to an answer first, then look.
Checkpoint: Fermi estimates (2 of 2)
Question 2 of 2 Commit to an answer first, then look.
Accuracy and precision
FIRST, MAKE A PREDICTION
TRY IT / FOLLOW THE REASONING
Sketch repeated measurements as dots around a target. Make one cluster tight but off-centre, and another spread around the centre. Match the sketches to accuracy and precision.
MAKE THE CONNECTION
Key idea
Accuracy: how close a result is to the true value. Precision: how close repeated results are to each other.
Accuracy and precision
Checkpoint: Accuracy and precision
Question Commit to an answer first, then look.
Random and systematic errors
FIRST, MAKE A PREDICTION
TRY IT / FOLLOW THE REASONING
Write three readings with positive and negative random deviations, then three with the same offset. Compare their means and decide which problem calls for calibration.
MAKE THE CONNECTION
- Random errors scatter results either way; averaging repeated measurements reduces them.
- Systematic errors push every result the same way; averaging doesn't help, but calibration does.
Checkpoint: Random and systematic errors (1 of 2)
Question 1 of 2 Commit to an answer first, then look.
Checkpoint: Random and systematic errors (2 of 2)
Question 2 of 2 Commit to an answer first, then look.
Error bars
FIRST, MAKE A PREDICTION
TRY IT / FOLLOW THE REASONING
Draw the interval on a number line and place the accepted value on it. Compare this result with a tighter interval centred at the same value; state what the quoted uncertainty means before treating it as a probability.
MAKE THE CONNECTION
Error bars: \(g = 9.7 \pm 0.2\ \text{m/s}^2\) means the true value probably lies between 9.5 and 9.9. The accepted 9.81 is inside, so the measurement agrees.
Error bars
Checkpoint: Error bars (1 of 2)
Question 1 of 2 Commit to an answer first, then look.
Checkpoint: Error bars (2 of 2)
Question 2 of 2 Commit to an answer first, then look.
Significant figures
FIRST, MAKE A PREDICTION
TRY IT / FOLLOW THE REASONING
Compare 0.0042 with 0.00420 in scientific notation. Decide which digits locate the scale and which tell a reader how precisely the value was recorded.
MAKE THE CONNECTION
Significant figures are the digits that carry real information. Leading zeros don't count. Give answers to about as many significant figures as your least precise measurement.
Significant figures
Myth: more digits means a more accurate answer
Digits beyond what you measured are false precision: they claim knowledge you don't have.
Checkpoint: Significant figures
Question Commit to an answer first, then look.
Key terms
Key terms
- Exponent (power)
- The small raised number: how many times ten is multiplied (or, if negative, divided).
- Scientific notation
- A number from 1 to 10 times a power of ten.
- Conversion factor
- A fraction equal to one, used to change units without changing the quantity.
- Dimension
- The kind of quantity (length, mass, time…), whatever the units.
Key terms
- Fermi problem
- An estimate built from simple, rough steps.
- Accuracy / precision
- Closeness to the true value / closeness of repeated results to each other.
- Random / systematic error
- Scatter either way / a shift in the same direction every time.
- Significant figures
- The digits that carry real information.
Key terms
- False precision
- More digits than a measurement supports.
History and sources
Charles and Ray Eames (Chicago, 1977)
Charles and Ray Eames (Chicago, 1977). The film Powers of Ten zooms out from a picnic by a factor of ten every ten seconds, then back in to an atom. It was adapted from Kees Boeke's book Cosmic View (1957). Source: Eames Foundation.
The Mars Climate Orbiter (1999)
The Mars Climate Orbiter (1999). Ground software reported thruster impulse in pound-force seconds; the navigation software expected newton-seconds (1 lbf·s ≈ 4.45 N·s). The probe approached Mars far too low, and was lost. Source: Mars Climate Orbiter Mishap Investigation Board, Phase I Report, 10 November 1999.
The metre: Jean-Baptiste Delambre and Pierre Méchain (France, 1792–1798)
The metre: Jean-Baptiste Delambre and Pierre Méchain (France, 1792–1798). The metre was defined as one ten-millionth of the distance from the North Pole to the equator. The two astronomers measured the meridian arc from Dunkirk to Barcelona by triangulation. The metre was redefined in 1960 (krypton light) and again in 1983 (the distance light travels in 1/299 792 458 s). Source: BIPM, 17th CGPM Resolution 1 (1983).
The kilogram: Le Grand K and the 2019 redefinition
The kilogram: Le Grand K and the 2019 redefinition. A platinum–iridium cylinder defined the kilogram from 1889. On 16 November 2018 the 26th General Conference on Weights and Measures voted to define it by fixing the Planck constant; the change took effect on 20 May 2019. The kilogram is realised with the Kibble balance, invented by Bryan Kibble at the UK's National Physical Laboratory in 1975. Sources: BIPM, 26th CGPM Resolution 1 (2018) · NIST: SI redefinition · BIPM: the SI.
The Gimli Glider (Air Canada Flight 143, 1983)
The Gimli Glider (Air Canada Flight 143, 1983). The fuel for an all-metric Boeing 767 was worked out with a density in pounds per litre (1.77) instead of kilograms per litre (about 0.8). The plane had less than half the fuel it needed, ran out at 41,000 feet, and was glided to a safe landing at Gimli, Manitoba. Source: Canadian Aviation Safety Board report, 1985.
Enrico Fermi at Trinity (New Mexico, 1945)
Enrico Fermi at Trinity (New Mexico, 1945). Fermi dropped scraps of paper as the blast wave passed; they moved about 2½ metres, from which he estimated about 10,000 tons of TNT. Later measurements put the yield at roughly twice that. Sources: Fermi, "My Observations During the Explosion at Trinity on July 16, 1945" · J. Katz, "Fermi at Trinity" (2021).
The Hubble Space Telescope (1990)
The Hubble Space Telescope (1990). The main mirror was polished very precisely to the wrong shape, about 2.2 micrometres too flat at the edge, because a test instrument had a lens out of place. Corrective optics were fitted in 1993. Sources: NASA: Hubble's mirror flaw · the Allen report, Hubble Space Telescope Optical Systems Failure Report, 1990.
Worked example: weighing the atmosphere
Watch the worked example
The problem
Problem. Air pressure at sea level is about 100,000 Pa and the Earth's radius is about 6400 km. Estimate the mass of the Earth's atmosphere.
Solution
- Pressure is force per area. 100,000 Pa means 100,000 N pressing on each square metre: the weight of the air above it.
- Mass from weight: \(m = \dfrac{W}{g} = \dfrac{10^5\ \text{N}}{10\ \text{N/kg}} = 10^4\ \text{kg}\) above each square metre. Units: \(\dfrac{\text{N/m}^2}{\text{N/kg}} = \text{kg/m}^2\). ✓
- Area of the Earth: \(R = 6400\ \text{km} = 6.4\times10^6\ \text{m}\), so \(4\pi R^2 \approx 12.6 \times 4.1\times10^{13} \approx 5\times10^{14}\ \text{m}^2\).
Solution
- Multiply: \(10^4\ \text{kg/m}^2 \times 5\times10^{14}\ \text{m}^2 = 5\times10^{18}\ \text{kg}\).
- Check: careful studies give about \(5.15\times10^{18}\) kg (Trenberth & Smith, Journal of Climate, 2005). Using \(g = 10\) instead of 9.8 makes our answer slightly small, and ignoring high ground (with less air above it) makes it slightly big; the two roughly cancel. The air is less than a millionth of the Earth's mass (about \(6\times10^{24}\) kg).
Practice
★ Warm-up
-
Write in scientific notation: (a) 93,000,000 (b) 0.000 052 (c) 602,000,000,000,000,000,000,000.
Problem 2 (★ Warm-up)
-
Work out (a) \((3\times10^4)\times(2\times10^{-6})\) and (b) \((8\times10^9)\div(4\times10^3)\).
Problem 3 (★ Warm-up)
-
Convert 72 km/h to metres per second.
Problem 4 (★ Warm-up)
-
How many cubic metres are 2.5 litres?
Problem 5 (★ Warm-up)
-
How many significant figures: (a) 0.00420 (b) \(3.00\times10^8\) (c) 50.06?
Problem 6 (★ Warm-up)
-
A room is 4 m × 5 m × 2.5 m, and air has a density of about 1.2 kg/m³. What is the mass of the air in the room?
Problem 7 (★ Warm-up)
-
A 2.0 litre bottle is full of olive oil, of mass 1.84 kg. What is the oil's density in kg/m³? Will it float on water?
★★ Standard
-
Check the dimensions of (a) \(v^2 = 2ad\) and (b) \(d = v t^2\), where \(v\) is a speed, \(a\) an acceleration, \(d\) a distance and \(t\) a time.
Hint
Write each side in L, M and T. Replace every symbol by its dimension, cancel, and compare what is left.
Problem 9 (★★ Standard)
-
The speed \(v\) of a wave on a string depends on the tension \(F\) (a force, dimensions \(M L T^{-2}\)) and the mass per unit length \(\mu\) (dimensions \(M L^{-1}\)). Use dimensional analysis to find how \(v\) depends on them.
Hint
Mass appears in both \(F\) and \(\mu\), and \(v\) has none. Combine \(F\) and \(\mu\) so M cancels, then see what dimensions are left.
Problem 10 (★★ Standard)
-
A floor is 3 m by 4 m. What is its area in square centimetres?
Problem 11 (★★ Standard)
-
Light travels at \(3\times10^8\) m/s, and a year is about \(3.15\times10^7\) s. (a) How far is a light-year in metres? (b) How long does sunlight take to reach us from \(1.5\times10^{11}\) m away?
Hint
Distance is speed times time. For (b), time is distance divided by speed. Multiply or divide the front numbers, and add the powers of ten when multiplying but subtract them when dividing.
Problem 12 (★★ Standard)
-
Two students measure \(g\): Ana gets \(9.6\pm0.3\ \text{m/s}^2\); Ben gets \(10.4\pm0.1\ \text{m/s}^2\). The accepted value is 9.81. Which result agrees with it? Which is more precise? What might have gone wrong for the other?
Hint
Write each result as a range, value minus error to value plus error. Does 9.81 fall inside it? A smaller error bar means more precise.
★★★ Stretch
-
The "try it" from the video. How many litres of water do you drink in your lifetime? Give a range, not just one number.
Hint
Litres per day × days per year × years. What's a sensible low and high value for each?
Problem 14 (★★★ Stretch)
-
Estimate the number of hairs on a human head.
Hint
Estimate the area of scalp with hair, and how far apart the hairs are (or how many grow per square centimetre).
Problem 15 (★★★ Stretch)
-
A mass \(m\) on a spring of stiffness \(k\) (unit N/m, dimensions \(M T^{-2}\)) bounces up and down. Use dimensional analysis to find how its period depends on \(m\) and \(k\). Does a heavier mass bounce faster or slower?
Hint
Find the combination of \(m\) and \(k\) with dimension T squared. Then think about what happens to it when \(m\) grows.
Problem 16 (★★★ Stretch)
-
If you counted one number every second without stopping, how long would it take to reach a billion? Is your answer an overestimate or an underestimate?
Hint
Divide a billion seconds by the number of seconds in a year. Then ask whether anything in real counting makes it slower than one number per second.
Check yourself
Answer these out loud, from memory. Then try again in a few days.
Check yourself
- How can order-of-magnitude estimates reveal whether an answer is physically reasonable?
Check yourself
- What is a physical quantity, and how do a numerical value and a unit describe it?
Check yourself
- What are the SI base units, how are they defined through fixed constants of nature, and how are derived units constructed?
Check yourself
- How do scientific notation and metric prefixes describe very large or small quantities?
Check yourself
- How can units be converted without changing the physical quantity being measured?
Check yourself
- What is dimensional analysis, and how can it detect mistakes or suggest relationships?
Check yourself
- How do accuracy and precision differ?
Check yourself
- What are random and systematic measurement errors?
Check yourself
- How should uncertainty, significant figures, and rounding be reported?
Check yourself
- How do calibration, repeated measurements, and error bars help assess an experimental result?
The roadmap's other §01–§02 questions (models and theories, controlled experiments, conservation laws, resolution and sensitivity, combining uncertainties) are picked up later: P0, P3, P40 and M14.
Check yourself
Summary
Summary
KEEP THE THREAD GOING
Next: Algebra and graphs for physicsContinue when you’re ready, or return to any question above.
Your results for each stage appear here when scripting is on. Nothing is graded and nothing is sent anywhere.
Further learning
Khan Academy: videos and refreshers on notation, exponents, units and significant figures.
- Scientific notation example: 0.0000000003457 (video)
- Negative exponent intuition (video)
- Multiplying multiples of powers of 10 (video)
- Multiplying & dividing in scientific notation (video)
- Exponent properties review (article)
- Worked example: Dimensional analysis (video)
- Significant figures rules (video)
- Multiplying and dividing with significant figures (video)
Free textbook: OpenStax, University Physics Volume 1, chapter 1: 1.2 Units and Standards · 1.3 Unit Conversion · 1.4 Dimensional Analysis · 1.5 Estimates and Fermi Calculations · 1.6 Significant Figures
Simulation: PhET: Estimation: practise estimating lengths, areas and volumes.
Books: Sanjoy Mahajan, Street-Fighting Mathematics (estimation and dimensional analysis); John R. Taylor, An Introduction to Error Analysis (uncertainty).
