Explore Einstein's theories of special and general relativity
Length contraction is the phenomenon where the length of an object moving at relativistic speeds appears shorter to a stationary observer. This effect is only noticeable at speeds approaching the speed of light.
| Object | Mass | Rest Energy | Equivalent |
|---|---|---|---|
| Electron | 9.1e-31 kg | 8.2e-14 J | 0.511 MeV |
| Proton | 1.67e-27 kg | 1.5e-10 J | 938 MeV |
| Uranium atom | 3.95e-25 kg | 3.55e-8 J | 221 GeV |
| 1 gram | 0.001 kg | 9e+13 J | 21 kilotons TNT |
| Human (70kg) | 70 kg | 6.3e+18 J | 1.5 gigatons TNT |
Einstein's theory of relativity revolutionized physics with two fundamental principles:
Albert Einstein's theory of relativity revolutionized our understanding of space, time, and gravity. It consists of two parts: special relativity (1905) and general relativity (1915).
| Concept | Special Relativity | General Relativity |
|---|---|---|
| Scope | Uniform motion in inertial frames | Accelerated motion and gravity |
| Key Principle | Speed of light is constant | Gravity as curvature of spacetime |
| Key Effects | Time dilation, length contraction | Gravitational time dilation, light bending |
| Mathematical Framework | Minkowski spacetime | Riemannian geometry |
| Applications | Particle physics, GPS corrections | Cosmology, black holes, gravitational waves |
Note: Relativistic effects become significant at speeds above 10% of light speed (30,000 km/s). At everyday speeds, Newtonian physics provides excellent approximations.