The big ideaSpecial relativity connects measurements made in different inertial frames, while cosmology uses redshift, the cosmic microwave background, and primordial element abundances to test the history of an expanding universe.
Name the frame first
Relativity questions become manageable when you say where the clock or object is at rest.
Not sure about the basics underneath this lesson?
1
Proper time
One clock is present at both events.
2
Proper length
The object is at rest in the measuring frame.
3
Transform
Multiply proper time by γ; divide proper parallel length by γ.
4
Optional reference
NASA's universe overview summarizes cosmic history and expansion evidence. It supports the cosmology section, not the relativity calculations.
Quick check — answer out loud before you peek
Which frame measures a spaceship's proper length?
The spaceship's rest frame.
Got it now? Scroll back up and re-read the section — it should land differently.
Symbols and reference values
Symbol
Meaning
Unit or value
v
Relative speed
m/s
c
Vacuum speed of light
2.998 × 10⁸ m/s
γ
Lorentz factor
dimensionless
Δτ
Proper time
s
L₀
Proper length
m
CMB temperature
Present blackbody temperature
about 2.725 K
1 Mpc
One megaparsec
about 3.26 million light-years
Before you start Review square roots, ratios, scientific notation, and graph proportionality. Relativity calculations also require you to name the observer's inertial frame.
Two relativity postulates
First, the laws of physics have the same form in every inertial frame; there is no preferred frame of absolute rest. Second, every inertial observer measures the same vacuum speed c for light, independent of source or observer motion. These statements require space and time measurements to transform together.
The two inertial frames use the same laws and both measure c. Because the moving-frame light path is longer, their time and distance coordinates differ.
Proper quantities and frames
Proper time Δτ is measured by one clock present at both events. Proper length L₀ is measured in the object's rest frame. An observer who sees the clock moving measures a longer interval Δt = γΔτ. An observer who sees the object moving measures a shorter dimension parallel to its motion, L = L₀/γ. Perpendicular dimensions are unchanged. These are consistent frame-dependent measurements, not merely a visual illusion.
Relativity formulas
Lorentz factor
γ=1−v2/c21
γ is dimensionless and is at least 1.
Time dilation
Δt=γΔτ
Δτ is proper time on the clock moving with the events.
Length contraction
L=γL0
Only the dimension parallel to relative motion contracts.
Rest energy
E0=mc2
m is invariant mass; total energy and momentum depend on frame.
Hubble-Lemaître relation
v≈H0d
For nearby galaxies in the smooth expansion, recession rate is approximately proportional to distance.
Solve a relativity problem
Name the frames
State which object or clock is at rest in each frame.
Find the proper quantity
Proper time uses one co-located clock; proper length belongs to the object's rest frame.
Calculate γ
Use v/c as a dimensionless ratio.
Choose multiply or divide
Moving clocks have a longer coordinate interval: multiply proper time by γ. Moving parallel lengths are shorter: divide proper length by γ.
Check the direction
The result must approach the classical value as v becomes small compared with c.
Not sure about this bit?
Write one sentence naming the rest frame before using a formula.
1
Frame
Identify where the object or one clock is at rest.
2
Gamma
Calculate γ from v/c.
3
Direction
Time interval grows by γ; parallel length shrinks by γ.
Got it now? Scroll back up and re-read the section — it should land differently.
Worked relativity examples
Clock moving at 0.60c
Relative speed.v=0.60c
Proper time.Δτ=8.0s
Find the time interval in the frame where the clock moves.
Calculate the Lorentz factor.
γ=1−0.6021=1.25
Dilate the proper time.
Δt=(1.25)(8.0s)
Δt = 10.0 s.
One-meter rod moving at 0.70c
Proper length.L0=1.00m
Relative speed.v=0.70c
Find the measured length parallel to motion.
Find γ.
γ=1−0.7021=1.400
Contract only the parallel dimension.
L=1.4001.00m
L = 0.714 m. A perpendicular one-meter dimension would remain one meter.
From expansion to the hot Big Bang
The Big Bang model describes an early hot, dense state followed by expansion of space; it is not an explosion from one location into preexisting empty space. General relativity extrapolated too far reaches a limit where present theory is incomplete, so a physical singularity should not be presented as an experimentally established object. The universe's current age is about 13.8 billion years.
Cosmological redshift is evidence that space has expanded; it is not a chemical explosion into empty space.
Three evidence lines
Expansion: on large scales, more distant galaxies generally show greater cosmological redshift, consistent with expanding space.
Cosmic microwave background: nearly uniform thermal radiation at about 2.725 K is relic light from the early universe, with small anisotropies that seeded later structure.
Primordial nuclei: hot Big Bang nucleosynthesis predicts mostly hydrogen and helium, with deuterium and trace lithium, broadly matching observations.