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- Q232086 subject Q6133127.
- Q232086 subject Q6274556.
- Q232086 subject Q6429350.
- Q232086 subject Q8970766.
- Q232086 abstract "The Roche limit (pronounced /ʁoʃ/ in IPA, similar to the sound of rosh), 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 disperses and forms rings whereas outside the limit material tends to coalesce. The term is named after Édouard Roche, who is the French astronomer who first calculated this theoretical limit in 1848.".
- Q232086 thumbnail Roche_limit_(far_away_sphere).svg?width=300.
- Q232086 wikiPageExternalLink 1963ApJ...138.1182C.
- Q232086 wikiPageExternalLink books?id=8dPPAAAAMAAJ&pg=PA436.
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- Q232086 wikiPageExternalLink books?id=UmoVAAAAQAAJ&pg=PA333.
- Q232086 wikiPageExternalLink books?id=coE-AAAAYAAJ&pg=PA35.
- Q232086 wikiPageExternalLink books?id=x3gVAAAAQAAJ&pg=PA21.
- Q232086 wikiPageExternalLink episode-48-tidal-forces-across-the-universe.
- Q232086 wikiPageExternalLink Roche.
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- Q232086 comment "The Roche limit (pronounced /ʁoʃ/ in IPA, similar to the sound of rosh), 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 disperses and forms rings whereas outside the limit material tends to coalesce.".
- Q232086 label "Roche limit".
- Q232086 depiction Roche_limit_(far_away_sphere).svg.