The relevant observations fall into two categories: observations of certain astronomical facts from which the existence of a finite velocity of light and its magnitude as an absolute property of it has been inferred; and terrestrial experiments which permitted direct observation of a process of propagation connected with the establishment of light in space resulting in the measurement of its speed. To the latter category belong the experiments of Fizeau (1849) and Foucault (1850) as well as the Michelson-Morley experiment with its implications for Einstein’s Theory of Relativity. The former category is represented by Roemer’s observations of certain apparent irregularities in the times of revolution of one of Jupiter’s moons (1676), and by Bradley’s investigation into the reason for the apparent rhythmic changes of the positions of the fixed stars (1728).