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One of the most valuable — and least drilled — skills in physics is the ability to make a rough-but-reliable estimate of a physical quantity. A good physicist can tell you, to within a factor of ten, the kinetic energy of a running human, the number of atoms in a teaspoon of water, or the frequency of a typical human heartbeat, without looking anything up.
OCR examines this explicitly in Module 2 of the A-Level Physics A specification, under "Estimation of physical quantities". You should be able to: give an order-of-magnitude estimate; use approximate values for common constants; sanity-check a numerical answer; and perform simple dimensional analysis. This lesson trains all four skills.
The order of magnitude of a quantity is the power of ten closest to it. More formally, if a quantity is written as a × 10ⁿ, with 1 ≤ a < 10, then the order of magnitude is n. (Some textbooks round differently — OCR accepts either convention as long as it is consistent.)
For example:
| Quantity | Value | Order of Magnitude |
|---|---|---|
| Diameter of a hydrogen atom | 1 × 10⁻¹⁰ m | −10 |
| Thickness of a sheet of paper | 1 × 10⁻⁴ m | −4 |
| Height of a human | 1.7 m | 0 |
| Height of Mount Everest | 8.8 × 10³ m | 4 |
| Distance to the Moon | 3.8 × 10⁸ m | 8 |
| Distance to the nearest star | 4 × 10¹⁶ m | 16 |
When two quantities differ by more than an order of magnitude, one is clearly much bigger than the other. When they differ by less than an order, they are in the same "ballpark".
Exam Tip: If OCR asks you to "estimate the order of magnitude" of a quantity, you only need to give the power of ten. A more exact figure is not required and can lose marks for over-precision on an estimation question.
You should know the approximate values of the following, to within an order of magnitude, without a data sheet.
| Quantity | Typical Value |
|---|---|
| Mass of an electron | 10⁻³⁰ kg |
| Mass of a proton | 10⁻²⁷ kg |
| Mass of a human | 70 kg |
| Mass of a car | 10³ kg |
| Mass of the Earth | 6 × 10²⁴ kg |
| Radius of an atom | 10⁻¹⁰ m |
| Radius of a nucleus | 10⁻¹⁵ m |
| Radius of the Earth | 6 × 10⁶ m |
| Radius of the Sun | 7 × 10⁸ m |
| Speed of sound in air | 340 m s⁻¹ |
| Speed of light in vacuum | 3 × 10⁸ m s⁻¹ |
| Acceleration of free fall (UK) | 9.81 m s⁻² |
| Atmospheric pressure | 10⁵ Pa |
| Density of water | 10³ kg m⁻³ |
| Age of the universe | 4 × 10¹⁷ s (≈ 14 × 10⁹ years) |
| Avogadro constant | 6 × 10²³ mol⁻¹ |
| Boltzmann constant | 1.4 × 10⁻²³ J K⁻¹ |
| Planck constant | 6.6 × 10⁻³⁴ J s |
| Elementary charge | 1.6 × 10⁻¹⁹ C |
You are not expected to recite the exact value of Planck's constant — the data sheet provides it — but you should be able to say "about 10⁻³⁴ J s" and use that in an estimation question.
The Italian-American physicist Enrico Fermi was legendary for his ability to make good estimates with minimal information. A famous example: on the morning of the Trinity nuclear test in 1945, Fermi stood at the observation point, dropped small pieces of paper, and by watching how far the blast wind blew them, estimated the explosive yield of the world's first atomic bomb to within a factor of two of the true value — before any instruments had reported in.
The trick Fermi used is called Fermi estimation: break a hard question into smaller, easier sub-questions, each of which you can estimate to within a factor of 10, and combine the results. Errors tend to cancel, so your final answer is usually surprisingly accurate.
Estimate the number of breaths a typical human takes in a lifetime.
Solution:
Multiply:
15 × 60 × 24 × 400 × 80 ≈ 15 × 60 × 24 × 3.2 × 10⁴ ≈ 900 × 24 × 3.2 × 10⁴ ≈ 2.2 × 10⁴ × 3.2 × 10⁴ ≈ 7 × 10⁸ breaths
About a billion — the order of magnitude is 10⁸ to 10⁹. An exam question would accept anything in that range.
An apple falls from a tree of height 3 m. Estimate the kinetic energy with which it hits the ground.
Solution:
Gravitational PE lost = kinetic energy gained:
E_k ≈ mgh = 0.2 × 10 × 3 = 6 J
Order of magnitude: 10⁰ to 10¹ J.
Estimate the number of atoms in a 70 kg human.
Solution:
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