Light Clock & Time Dilation

This interactive simulator explores Light Clock & Time Dilation in Astronomy & The Sky. Two side-by-side light clocks — one at rest, one moving at v = βc — show why a moving clock ticks slower. The photon zig-zag traces a longer Pythagorean hypotenuse cT/2 vs the rest hypotenuse cT₀/2, giving T = γT₀ with γ = 1/√(1 − β²) live. The Pythagorean diagram and the running tick ratio make the special-relativistic time-dilation derivation visual rather than algebraic. Use the controls to change the scenario; watch the visualization and any graphs or readouts to connect the model with lectures, labs, and homework.

Who it's for: Best once you already know the basic definitions and want to build intuition. Typical context: Astronomy & The Sky.

Key terms

  • light
  • clock
  • time
  • dilation
  • light clock time dilation
  • astronomy

How it works

Side-by-side light clocks at rest and moving at v = βc demonstrate special-relativistic time dilation T = γT₀. Watch the photon zig-zag a longer Pythagorean path in the moving clock and the tick ratio approach 1/γ in real time.

Other simulators in this category — or see all 45.

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NewIntermediate

Length Contraction (Lorentz)

A ruler of proper length L₀ in S′ flies past the lab S at v = βc and is measured to be L = L₀/γ — only in the direction of motion. Animated fly-by with on-board ruler ticks and a dotted L₀ baseline makes the contraction L = L₀ √(1 − β²) immediately readable; same factor explains why GeV cosmic-ray muons reach the ground despite their ≈ 2 μs lifetime.

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NewAdvanced

Minkowski Spacetime Diagram (Lorentz Boost)

Interactive (x, ct) spacetime diagram: a Lorentz boost at v = βc rotates the (x′, ct′) axes inward by atan(β) toward the 45° light cone — relativity of simultaneity, time dilation and length contraction become pure geometry. Click events with Shift / Alt to read the invariant interval Δs² = (cΔt)² − (Δx)² and its time-/light-/space-like classification.

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NewAdvanced

Relativistic Doppler Effect

Source emits at rest frequency f₀ and moves at v = βc; observer at angle θ measures f_obs = f₀ √(1 − β²) / (1 − β cos θ). Animated lab-frame wavefronts, observer at any angle, and a 380–700 nm spectrum strip showing the apparent colour shift of a 555 nm reference line — including the purely relativistic transverse Doppler (θ = 90°) red-shift f₀/γ.

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NewIntermediate

Relativistic Energy–Momentum Hyperbola

Energy–momentum relation E² = (pc)² + (mc²)². The green hyperbola E = √(p² + 1) is bracketed by the Newtonian parabola E ≈ 1 + p²/2 (low-momentum limit) and the photon-like asymptote E = pc (ultra-relativistic). Pick β, p or T as the independent slider and watch all four quantities (β, γ, p, T) lock together — the operational core of accelerator and cosmic-ray physics.

Launch Simulator
NewAdvanced

Pair Production Threshold & σ(E_γ)

Pair creation channels γ + nucleus → e⁺e⁻ (Bethe–Heitler, σ ∝ Z²), the higher-threshold triplet γ + e⁻ → e⁻e⁺e⁻, and Breit–Wheeler γγ → e⁺e⁻ that limits TeV photons against the cosmic background. Live threshold marker, log-σ curve, and material presets (H, C, Al, Cu, Pb) make the 1.022 MeV / 4 m_e c² thresholds intuitive.

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NewAdvanced

CMB Power Spectrum (Acoustic Peaks)

Cosmic Microwave Background temperature D_ℓ vs ℓ with Sakharov peaks: tune Ω_b h², Ω_c h², n_s, A_s, τ, h and watch the parity flip between odd / even peaks, the Silk damping tail, and the Sachs–Wolfe plateau move. Pedagogical parametric ΛCDM model.

Launch Simulator