Introduction to the Special Theory of Relativity
Senior 5 · Physics
Introduction to the Special Theory of Relativity
Lesson 2 of 4
25 min
In 1905 Albert Einstein was 26 and worked as a technical expert at the Swiss patent office in Bern, examining applications for electrical inventions, many of them about synchronising clocks by electrical signals. In June of that year he sent a paper, "On the Electrodynamics of Moving Bodies", to the journal Annalen der Physik. Instead of trying to rescue the ether, he took the experimental facts at face value and raised them to two principles. Everything in this unit follows from them, including the most surprising consequence of all: two events that are simultaneous for one observer are not simultaneous for another.

The first postulate extends Galileo's principle from mechanics to all of physics. The second is what the Michelson–Morley experiment found. Together they make the ether unnecessary: there is no special frame "at rest".
Each postulate on its own seems harmless. Together they are revolutionary, because they contradict the Galilean velocity rule . If a lamp on a moving train sends a pulse forward, the passenger and the person on the platform must both measure its speed as . Speed is distance divided by time, so if they agree on the speed of light, they must disagree about distances and times. Space and time are not absolute.
Definition
Special relativity is Einstein's 1905 theory of how measurements of space and time in different inertial frames are related; it rests on two postulates: (1) the laws of physics are the same in all inertial frames; (2) the speed of light in a vacuum is the same, , in all inertial frames. Example: a scientist on a spacecraft moving at and a scientist on Earth both measure the same light pulse travelling at exactly .
Einstein's own thought experiment: a long train moves at speed past a platform. At the instant the middle of the train, where observer O′ sits, passes observer O on the platform, lightning strikes both ends of the train, leaving scorch marks at A and B on the platform, equal distances from O.
For O on the platform: the two flashes travel equal distances at the same speed and reach O together. O concludes, correctly, that the strikes were simultaneous.
For O′ on the train: she is moving towards B and away from A, so (as seen from the platform) she meets the flash from B first. In her own frame she is at rest, exactly halfway between the two ends of the train, and by the second postulate both flashes travel towards her at . Since the flash from B arrived first, she concludes, also correctly, that the strike at B happened before the strike at A.
Neither observer is mistaken. Events that are simultaneous in one frame are not simultaneous in another frame moving relative to it, if the events are separated along the direction of motion. Whether two separate events happen "at the same time" depends on the frame. Only for events at the same place do all observers agree.
The effect is tiny at everyday speeds. In the Lorentz transformation, which replaces the Galilean one, , where (Lesson 3). Two events simultaneous in S and a distance apart along are separated in S′ by
Worked example 1: how big is the disagreement?
Two lamps 300 m apart on a platform flash at the same instant in the platform frame. Find the time between the flashes for an observer moving along the line of the lamps at (a) 30 m s⁻¹, (b) ().
Solution
(a) : s: far too small to notice.
(b) s : easily measured with modern clocks.
Because times and distances change between frames, the Galilean rule must also change. If an object moves with velocity in frame S′, which itself moves at relative to S (both along ), its velocity in S is
At everyday speeds is negligible and the Galilean rule is recovered. But however the speeds are combined, the result never exceeds , and if , then : light has the same speed in both frames, exactly as the second postulate requires.
Worked example 2: a probe from a spaceship
A spaceship moving at relative to Earth launches a probe forward at relative to the ship. Find the probe's speed relative to Earth (a) by the Galilean rule, (b) by special relativity.
Solution
(a) , faster than light, which is impossible.
(b) .
Worked example 3: checking the second postulate
The spaceship in Worked example 2 switches on a headlight. Use the velocity-addition formula to find the speed of the light relative to Earth.
Solution
Exactly , as both postulates demand.
Warning
Relativity is not "everything is relative". Observers disagree about times, lengths and simultaneity, but they all agree on the laws of physics, on the speed of light and on the order of events that could be cause and effect. A strike cannot precede the thunder it causes in any frame.
Tip
Two postulates, one consequence: if everyone measures the same , then everyone cannot measure the same distances and times. Keep returning to that sentence when a result seems strange.
Relativity of Simultaneity, minutephysics. Watch how two observers moving relative to each other disagree about which of two events happened first, and why both are right.
Practice
Key points
Sources and credits
Written by Ganzaa. The train diagram (drawn for ), the worked examples and the practice exercises are by Ganzaa.