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HSC Physics · Module 7 · The Nature of Light · 15 min read

Special relativity

Special relativity is what happens when you take one fact seriously: every observer measures the same speed of light. From that, moving clocks run slow, moving objects are shorter, nothing with mass can reach the speed of light, and mass is a store of energy. HSC questions test all four, and they nearly always turn on one decision: which observer measures which quantity.

This guide covers the two postulates and the evidence for them, time dilation and length contraction (with proper time and proper length made clear), the muon evidence worked in both frames, relativistic momentum and E = mc². Then the mistakes that cost marks, a quick quiz and a full worked example.

What you need to know

The equations (from the 2019 HSC data sheet unless marked):

t = t0 / √(1 − v2/c2)Time dilation. t0 is the proper time; t, measured by an observer the clock moves past, is always longer.
l = l0 √(1 − v2/c2)Length contraction along the direction of motion. l0 is the proper length; l is always shorter.
pv = m0v / √(1 − v2/c2)Relativistic momentum. m0 is the rest mass. It grows without limit as v approaches c.
E = mc2Mass–energy equivalence. c = 3.00 × 108 m s−1 (data sheet). Mass in kg gives energy in J.
γ = 1 / √(1 − v2/c2) not on the data sheetThe Lorentz factor, a shorthand: t = γt0, l = l0/γ, pv = γm0v. It is 1 at low speed and grows quickly near c.

Dot points: PH-M7-15, PH-M7-16, PH-M7-17, PH-M7-18 (2017 Physics syllabus, HSC 2026 and 2027), in our own words.

Mini lesson

Einstein's two postulates and the evidence

An inertial frame of reference is one that is not accelerating: a smooth train at constant velocity, not one braking or going round a bend. Special relativity rests on two postulates:

Evidence: the Michelson–Morley experiment (1887) looked for a change in the speed of light as Earth moved through a supposed 'aether' and found none (a null result), which fits the second postulate and removes the need for a preferred frame. In 1964 at CERN, gamma rays given off by neutral pions travelling at more than 0.999c were measured moving at c, not nearly 2c. No experiment since has found a preferred frame or a light speed that depends on the source.

Postulate 2 clashes with everyday (Galilean) velocity addition: a torch on a fast train should give light at c + v. Einstein kept the postulates and gave up absolute time and space instead. Time dilation and length contraction follow.

Time dilation and proper time

Einstein's light clock is a pulse of light bouncing between two mirrors. On board, the light goes straight up and down. To someone the clock moves past, the light follows a longer zigzag path, but at the same speed c, so each tick takes longer. Moving clocks run slow: t = t0/√(1 − v2/c2).

Proper time t0 is the time between two events measured by a clock that is present at both of them, so the events happen at the same place in that clock's frame. It is always the shortest time any observer measures. Every other inertial observer, who sees the clock move, measures the longer, dilated time t. There is more on choosing it in our page on proper time in relativity.

The effect is tiny at everyday speeds: at 300 m s−1 (a fast jet) √(1 − v2/c2) differs from 1 by about 5 parts in 1013. Even at 0.14c it is only a 1% effect; it becomes large only close to c.

Two light clocks. Left: a clock at rest, with the light pulse going straight up between the mirrors. Right: a moving clock, with the light pulse following a longer diagonal path from the bottom mirror to the top mirror and down again as the clock moves to the right.at rest: t0vmoving: longer path, t > t0
Same light speed, longer path: the observer who sees the clock moving measures a longer time between ticks (t > t0).

Length contraction and proper length

Moving objects are shorter along their direction of motion: l = l0√(1 − v2/c2). Lengths at right angles to the motion do not change.

Proper length l0 is the length measured in the frame where the object is at rest. A spaceship's proper length is measured by its crew; a stretch of road's proper length is measured by people standing beside it. Anyone the object moves past measures it shorter.

Time dilation and length contraction are two views of the same thing. If a ship's crew time a trip with their own clock (proper time), the distance they cover, as they see it, is the contracted length of the route.

The evidence: muons, clocks, accelerators and supernovae

Cosmic-ray muons. Muons are made when cosmic rays hit the upper atmosphere, about 15 km up. Their mean lifetime at rest is about 2.2 μs, and even at 0.995c that is enough to travel only about 660 m. Yet large numbers reach the ground. Both frames explain this, and a full answer gives both:

Two panels. Earth frame: a muon falls 15 kilometres from the top of the atmosphere to the ground and its lifetime is dilated. Muon frame: the muon is at rest and the atmosphere, contracted to about 1.5 kilometres, moves up past it.Earth frameμ15 kmlifetimedilatedMuon frameμ at rest1.5 kmatmospherecontracted,moving up
Same result, two explanations: Earth sees a longer muon lifetime; the muon sees a thinner atmosphere (not to scale).

Hafele–Keating (1971). Caesium atomic clocks were flown around the world on airliners, eastward and westward, and compared with clocks left on the ground. The eastward clocks lost about 59 ns and the westward clocks gained about 273 ns, close to the predicted values (the predictions include a gravitational effect from general relativity as well as time dilation).

Particle accelerators. Fast unstable particles live longer by exactly the predicted factor. In a 1977 CERN experiment, muons circling a storage ring with a Lorentz factor of about 29 lived about 29 times longer than muons at rest.

Cosmological evidence. The brightening and fading of very distant supernovae is stretched out in time by the amount predicted for their recession, a time-dilation effect seen across the universe.

The twin paradox is a thought experiment, not evidence, and the travelling twin accelerates (a non-inertial frame), so don't use it as an example of experimental support.

Relativistic momentum and the speed limit

At low speeds momentum is mv. Near the speed of light it is pv = m0v/√(1 − v2/c2), where m0 is the rest mass. As v gets close to c the denominator heads to zero, so the momentum grows without limit.

That sets the speed limit. Pushing a particle with a force keeps increasing its momentum and its energy, but the speed only creeps closer to c. Reaching c would need infinite momentum and so infinite energy, so nothing with mass can reach or pass the speed of light. Particle accelerators show this: adding more energy to electrons that are already very close to c barely changes their speed.

Say 'its momentum (and energy) increase without limit', rather than 'its mass becomes infinite'. HSC questions use relativistic momentum, not a changing mass.

Graph of momentum against speed. The Newtonian line p equals m v rises steadily and crosses the speed of light. The relativistic curve starts on the same line at low speed, then curves up steeply and never reaches the vertical dashed line at the speed of light.pvcNewtonian, p = mvrelativistic p(grows without limit)
At low speed the two agree. Near c the relativistic momentum rises without limit, so v = c can't be reached.

E = mc²: mass is a store of energy

Einstein showed that mass and energy are equivalent: E = mc2. When a system gives out energy, its mass drops by Δm = E/c2. Because c2 is huge (9.0 × 1016 m2 s−2), a tiny mass is a vast amount of energy.

Common mistakes

Mini quiz

6 quick questions. Pick an answer to see if you're right and why.

  1. A spaceship moving at 0.60c towards Earth shines a laser beam forwards. What speed do observers on Earth measure for the laser light?
    Show answer

    B. By Einstein's second postulate, every inertial observer measures light in a vacuum at c, whatever the motion of the source. Adding the speeds (1.6c) is Galilean thinking, which fails for light.

  2. A clock on a spaceship ticks once every 1.0 s as measured by the crew. The ship passes Earth at 0.80c. What time between ticks do Earth observers measure?
    Show answer

    C. The crew's clock is at both ticks, so t0 = 1.0 s. t = 1.0 ÷ √(1 − 0.802) = 1.0 ÷ 0.60 = 1.7 s. 0.60 s multiplies instead of dividing, and 2.8 s forgets the square root.

  3. A spaceship flies past a space station at 0.5c. Who measures the proper length of the spaceship?
    Show answer

    B. Proper length is measured in the object's rest frame, and the ship is at rest relative to its crew. Station observers see it contracted.

  4. A rod has a proper length of 100 m. It moves along its length at 0.60c past an observer. What length does the observer measure?
    Show answer

    B. l = 100 × √(1 − 0.602) = 100 × 0.80 = 80 m. 64 m forgets the square root and 125 m divides instead of multiplying: a moving rod is always shorter than its proper length.

  5. Why can't a proton in an accelerator be pushed to the speed of light?
    Show answer

    B. pv = m0v/√(1 − v2/c2) increases without limit as v → c. Each push adds momentum and energy, but the speed only edges closer to c.

  6. An electron and a positron annihilate, and all of their mass becomes gamma-ray energy. How much energy is released? (me = 9.109 × 10−31 kg)
    Show answer

    B. E = mc2 with the mass of both particles: 2 × 9.109 × 10−31 × (3.00 × 108)2 = 1.64 × 10−13 J. 8.2 × 10−14 J counts only one particle; 5.5 × 10−22 J forgets to square c.

Worked example

In a particle accelerator, a beam of charged pions travels along a straight beam pipe at a constant 0.980c. In the pions' own rest frame their mean lifetime is 2.60 × 10−8 s.

(a) Calculate the mean lifetime of the pions as measured in the laboratory. (2 marks)

(b) Calculate the mean distance a pion travels along the pipe, as measured in the laboratory, before it decays. (2 marks)

(c) In its own frame a pion lives only 2.60 × 10−8 s. Use length contraction to show that an observer moving with the pion agrees it reaches the point where the laboratory sees it decay. (2 marks)

(6 marks)

I'll think out loud, the way you should in the exam, using KNOW-UD: Knowns, Not known, Organise, Work it out, Units, Direction.

Prediction first. At 0.980c, 1 − v2/c2 ≈ 1 − 0.96 = 0.04, and √0.04 = 0.2, so the Lorentz factor is about 5. I predict a lab lifetime about 5 × 26 ns ≈ 130 ns. The pion covers about 0.3 m every nanosecond, so in 130 ns it goes about 38 m. Without relativity it would manage only about 7.6 m.

K · Knowns

I sketch the beam pipe, which is at rest in the lab, and the pion moving along it. Then the key decision: which time is proper? The pion's lifetime in its own rest frame is measured by a 'clock' that travels with it, present at both its creation and its decay. So 2.60 × 10−8 s is t0.

  • v = 0.980c, c = 3.00 × 108 m s−1
  • t0 = 2.60 × 10−8 s (pion's rest frame: proper time)
  • the pipe's length is a proper length in the lab frame
A pion moving at 0.980 c along a straight beam pipe that is at rest in the lab, decaying a distance d further along. Notes give the proper lifetime 2.60 times ten to the minus eight seconds in the pion's frame, and ask for the lab-frame time and distance.pion's frame: t0 = 2.60 × 10⁻⁸ slab frame: t = ?v = 0.980cdecaysd = ? (lab frame)beam pipe at rest in the lab
Knowns on the sketch: v = 0.980c, t0 = 2.60 × 10−8 s in the pion's frame. Unknowns: the lab lifetime t and the lab distance d.

N · Not known

Part (a) wants a time in the lab frame, part (b) a distance in the lab frame, part (c) a length in the pion's frame to compare.

  • (a) t = ? s
  • (b) d = ? m
  • (c) l (lab distance as seen by the pion) = ? m

O · Organise

I write each step in symbols. In (b) I use the lab's own time and speed together, so I stay in one frame. In (c) the lab distance d is a proper length (it's measured in the frame where the pipe is at rest), so the pion sees it contracted.

  • t = t0 / √(1 − v2/c2)
  • d = vt (all lab-frame quantities)
  • l = d √(1 − v2/c2), compare with v × t0 (all pion-frame quantities)

W · Work it out

The denominator first, kept to full calculator precision, then each part.

  • √(1 − 0.9802) = √(1 − 0.9604) = √0.0396 = 0.19900
  • (a) t = 2.60 × 10−8 ÷ 0.19900 = 1.3065 × 10−7 s
  • (b) d = 0.980 × 3.00 × 108 × 1.3065 × 10−7 = 38.41 m
  • (c) l = 38.41 × 0.19900 = 7.644 m
  • distance the lab moves past the pion in its lifetime: v × t0 = 0.980 × 3.00 × 108 × 2.60 × 10−8 = 7.644 m
  • The two agree: in the pion's frame the 38.4 m stretch of pipe is contracted to 7.64 m, and that is exactly how far the pipe moves past the pion in its 26.0 ns life. Both frames agree on where it decays.

U · Units

Seconds for the time, metres for the distances. The data are to three significant figures, so I give three.

  • (a) t = 1.31 × 10−7 s
  • (b) d = 38.4 m
  • (c) l = 7.64 m = v × t0

D · Direction

These are a time and lengths, so instead of a direction I do the relativity sense checks: the dilated time must be longer than t0 (1.31 × 10−7 s > 2.60 × 10−8 s, yes), and the contracted length must be shorter than the proper length (7.64 m < 38.4 m, yes). The speed used was below c throughout.

  • t > t0 and l < l0, as they must be.

(a) The lab measures a mean lifetime of 1.31 × 10−7 s. (b) A pion travels a mean distance of 38.4 m along the pipe. (c) In the pion's frame that 38.4 m is contracted to 7.64 m, exactly the distance the pipe moves past the pion in 2.60 × 10−8 s, so both frames agree.

Check against the prediction. I predicted about 130 ns and about 38 m, with a Lorentz factor near 5. The answers are 131 ns and 38.4 m (the factor is 5.03), so they match. The 7.6 m 'no relativity' distance turns up again in (c) as the contracted length, which is the point of the question.

HSC advice

What markers keep saying

Summaries in our own words. Read NESA's own feedback with the exam packs: 2019 · 2022 · 2023 · 2024 · 2025.

How often it is examined

Special relativity questions were worth 49 marks across the seven HSC Physics exams from 2019 to 2025 (about 7.0 marks a paper), and appeared in 7 of 7 papers.

620196202072021720224202310202492025
Marks per paper (Module 7, Light and Special Relativity). Source: CortexHSC's own tagging of the NESA HSC Physics exams 2019–2025, each question counted under its main topic, so treat the numbers as close, not exact.

FAQ

What is the difference between proper time and dilated time?
Proper time t0 is measured by a clock present at both events, so the events happen at the same place in that clock's frame. Any observer who sees that clock moving measures a longer, dilated time t = t0/√(1 − v2/c2).
Which relativity equations are on the HSC data sheet?
The 2019 data sheet gives time dilation t = t0/√(1 − v2/c2), length contraction l = l0√(1 − v2/c2), relativistic momentum pv = m0v/√(1 − v2/c2) and E = mc2, plus c = 3.00 × 108 m s−1. The Lorentz factor γ is not printed.
Is the twin paradox evidence for special relativity?
No. It is a thought experiment, and the travelling twin accelerates, so that twin is not in an inertial frame. For evidence, use real experiments: muons reaching the ground, the Hafele–Keating clocks and particle lifetimes in accelerators.
Does mass increase at high speed?
The HSC course uses relativistic momentum with a fixed rest mass m0: the momentum grows without limit as v approaches c. Say that, rather than 'the mass increases'.
Why can't anything travel faster than light?
For anything with mass, the momentum and energy needed grow without limit as the speed approaches c, so reaching c would take infinite energy. Light itself has no rest mass and always travels at c.

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