History
| 1675 | Rømer and Huygens, moons of Jupiter | 220,000 |
| 1729 | James Bradley, aberration of light | 301,000 |
| 1849 | Hippolyte Fizeau, toothed wheel | 315,000 |
| 1862 | Léon Foucault, rotating mirror | 298,000±500 |
| 1907 | Rosa and Dorsey, EM constants | 299,710±30 |
| 1926 | Albert Michelson, rotating mirror | 299,796±4 |
| 1950 | Essen and Gordon-Smith, cavity resonator | 299,792.5±3.0 |
| 1958 | K.D. Froome, radio interferometry | 299,792.50±0.10 |
| 1972 | Evenson et al., laser interferometry | 299,792.4562±0.0011 |
| 1983 | 17th CGPM, definition of the metre | 299,792.458 (exact) |
Until the early modern period, it was not known whether light travelled instantaneously or at a very fast finite speed. The first extant recorded examination of this subject was in ancient Greece. The ancient Greeks, Muslim scholars and classical European scientists long debated this until Rømer provided the first calculation of the speed of light. Einstein's Theory of Special Relativity concluded that the speed of light is constant regardless of one's frame of reference. Since then, scientists have provided increasingly accurate measurements.
Read more about this topic: Speed Of Light
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“The one duty we owe to history is to rewrite it.”
—Oscar Wilde (1854–1900)
“A poet’s object is not to tell what actually happened but what could or would happen either probably or inevitably.... For this reason poetry is something more scientific and serious than history, because poetry tends to give general truths while history gives particular facts.”
—Aristotle (384–323 B.C.)
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