Luminiferous aether

In the 19th century, luminiferous aether (or ether), meaning light-bearing aether, was the term used to describe a medium for the propagation of light (electromagnetic radiation). However, a series of increasingly complex experiments had been carried out in the late 1800s like the Michelson-Morley experiment in an attempt to detect the motion of earth through the aether, and had failed to do so. A range of proposed aether-dragging theories could explain the null result but these were more complex, and tended to use arbitrary-looking coefficients and physical assumptions. Hendrik Lorentz and George Francis FitzGerald offered within the framework of Lorentz ether theory a more elegant solution to how the motion of an absolute aether could be undetectable (length contraction), but if their equations were correct, Albert Einstein's 1905 special theory of relativity could generate the same mathematics without referring to an aether at all. This led most physicists to conclude that the classical notion of aether was not a useful concept.

See also: History of special relativity

Gravitational aether

Main article: Mechanical explanations of gravitation

From the 16th until the late 19th century, gravitational phenomena had also been modeled utilizing an aetherial concept. The most well-known concept is Le Sage's theory of gravitation. Other concepts were made by Isaac Newton, Bernhard Riemann, Lord Kelvin etc.