Physics, drawn.

Physics is taught in equations and understood in pictures, and the pictures are usually the part left out. This is a collection of essays about the second kind — one idea at a time, illustrated to the point where the argument becomes visible.

The field of a dipole. Field lines traced from a positive charge toward a negative one. Every line does eventually close on the negative charge, but the outer ones loop far outside any frame, so this picture is a crop rather than the whole field.
Fig. 1 The field around a positive and a negative charge. Every line is traced by stepping along the local field direction, so the shape is a consequence of the inverse-square law rather than a drawing of what it ought to look like. The lines running off the edge do close on the negative charge — they simply do it outside the frame.

Nine fields

the divisions physics is conventionally cut into

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one from each field, of 515

The pendulum's phase portrait. Angle plotted against angular velocity. Closed loops are swinging back and forth; the open curves above and below are rotating all the way round; the dashed curve between them is the separatrix. Mechanics

The pendulum, and the small lie that makes it simple

A pendulum's period does not depend on how far it swings. This is one of the most useful false statements in physics, and it is worth knowing exactly how false.

5 figures
A travelling wave, caught at one instant. A sine wave plotted against position at a fixed moment. The wavelength is the distance between repeats. The ghosted curve is the same wave a moment later. Waves

A wave is a shape that travels, and nothing else does

In a wave on water, no water goes anywhere. What moves is the shape — and separating the two motions is the whole of wave physics.

4 figures
Refraction from n = 1 into n = 1.5. A ray crossing a boundary between media of refractive index 1 and 1.5, bending by the amount Snell's law requires. Optics

The bend at the boundary, and what it is really about

Light changes direction when it changes speed. Snell's law is the geometry of that statement, and it can be derived without knowing anything about light at all.

4 figures
The field of a dipole. Field lines traced from a positive charge toward a negative one. Every line does eventually close on the negative charge, but the outer ones loop far outside any frame, so this picture is a crop rather than the whole field. Electromagnetism

Field lines are a choice, not a discovery

Nothing in space is arranged in lines. The lines are a drawing convention — and an unusually good one, because three separate facts about the field survive the translation.

5 figures
Molecular speeds at 4 temperatures. The distribution of molecular speeds in a gas, with each curve enclosing the same area. Raising the temperature moves the peak right and lowers it: the same molecules, spread over a wider range of speeds. Thermodynamics

The speeds in a still room

The air in a quiet room is not still. Every molecule in it is moving at hundreds of metres per second, and temperature is a single number summarising an entire distribution.

4 figures
A spacetime diagram at β = 0.5. Position across, time up, in units where light travels at 45°. The shaded wedges are the future and past reachable by light; the tilted axes belong to an observer moving at 0.5 of the speed of light. Relativity

Two axes, one speed, and a diagram that does the arguing

Put position across and time up, insist that light travels at forty-five degrees for everyone, and nearly every result in special relativity becomes something to read off rather than derive.

4 figures
The blackbody spectrum, against what classical physics predicted. Spectral exitance against wavelength for a blackbody at 3000, 4000, 5000 kelvin, in kilowatts per square metre per nanometre. Each curve peaks at the wavelength Wien's displacement law gives — 966 nm at 3000 K, 724 nm at 4000 K, 580 nm at 5000 K — and falls to nothing at short wavelengths. Quantum

The curve that would not come down

Classical physics predicted that a warm object radiates infinite power at short wavelengths. Every step of the derivation was correct, the prediction was absurd, and closing the gap required assuming that energy comes in lumps.

4 figures
Three vessels, one pressure. Three vessels filled to the same depth of 3 m. The pressure on each base is 29.4 kPa — identical, because pressure is set by depth — while the weight of water each holds differs by a factor of 4.7. The base of the flaring vessel carries more force than the water standing over it weighs. Fluids

The pressure that only knows depth

A litre of water and a swimming pool press equally hard on a floor at the same depth. Pressure in a still fluid is a scalar with no direction of its own, it depends on how far down and on nothing else, and the shape of the container falls out of the arithmetic entirely.

5 figures
Light crossing an accelerating box. A pulse crosses a box 6 m wide while the box accelerates at 9.81 m/s². The crossing takes 2·10⁻⁸ s, in which the far wall gains 1.96·10⁻⁷ m/s, so the pulse lands 1.96·10⁻¹⁵ m below the height it left at — and the path is a parabola. An observer sealed inside cannot tell that from a beam of light bending in a gravitational field, and the equivalence principle says there is nothing to tell. The sag is drawn 5.6·10¹⁴ times its true size. Astrophysics

The floor that cannot be told from gravity

Seal a laboratory, take away the windows, and no experiment inside it can distinguish standing in a gravitational field from accelerating through empty space. That is not a philosophical remark — it forces light to bend, forces clocks to disagree, and has a size at which it stops being true.

4 figures

Recently added

40 essays, 16 September 2026

Everything that has arrived, group by group

All 515 essays · every field · every ladder · every object named · every figure · what is taught wrongly · search

Threads running through

themes, not chapters

What stays the same

Conservation laws, and the habit of solving a problem by refusing to look at the middle of it.

137 essays

The same equation again

A pendulum, a circuit, a molecule and a bridge, all obeying one differential equation and not knowing about each other.

117 essays

Approximations that lie

The small-angle assumption, the frictionless plane, the point mass — where each is fine, and precisely where it stops being.

84 essays

Fields, not forces

Replacing action at a distance with something that fills space, and what that buys.

59 essays

The arrow of time

Nearly every law works equally well backwards. Almost nothing else does, and the gap between those facts is thermodynamics.

56 essays

Where the model stops

Every picture in physics has a domain of validity, and the interesting physics usually lives at its edge.

120 essays

Made into an instrument

The point at which a principle stops explaining something and starts measuring it — a critical angle sold as a refractometer, a Doppler shift weighing a planet, a null result testing a law.

123 essays

Order out of the random

Enormous numbers of unpredictable particles producing quantities you can print on a dial.

70 essays

The shape decides

A number that looks as though it should depend on the forces involved and turns out to depend only on the arrangement — a falloff exponent, a capacitance, a moment of inertia, the angle a rainbow has to be.

98 essays

Who is measuring

Quantities that are not properties of the thing but of the thing and an observer: which events are simultaneous, how long something is, how fast it is going and whose second is being counted.

83 essays

What happens at the edge

Quantities that live on a surface rather than in a volume, and conditions imposed at an edge that decide what the whole interior may do — a skin that costs energy per unit area, charge that sits entirely on the outside of a conductor, a clamped end that permits some frequencies and forbids the rest, a wall that quantises a box, and the interface where light has to change direction.

78 essays

Only some values fit

Continuous objects producing discrete answers. A string that will sound some frequencies and not others, three permitted exponents, a speed no composition can exceed — the first sightings of quantisation, in a subject that has not reached it yet.

67 essays