出典:Wiktionary
Named after French astronomer Édouard Roche, who first calculated the limit in 1848.
Roche limit (複数形 Roche limits)
出典:Wikipedia
出典:『Wikipedia』 (2011/07/12 21:54 UTC 版)
The Roche limit (
/ˈroʊʃ/), sometimes referred to as the Roche radius, is the distance within which a celestial body, held together only by its own gravity, will disintegrate due to a second celestial body's tidal forces exceeding the first body's gravitational self-attraction. Inside the Roche limit, orbiting material will tend to disperse and form rings, while outside the limit, material will tend to coalesce. The term is named after Édouard Roche, the French astronomer who first calculated this theoretical limit in 1848.