Roche Limits
Roche Limits is a theoretical threshold in orbital dynamics defining the minimum distance at which a celestial body, held together primarily by self-gravitation, can approach a more massive body without being torn apart by tidal forces induced by the latter's gravitational gradient.
96
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6.2K
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412
Authors
214
Institutions
Publications per year
2017–2026
29
Variants
Roche Limit
96
Black-hole-neutron-star collisions
James M. Lattimer, David N. Schramm · The Astrophysical Journal · 1974 · 886 citations · Full text
TIDAL EVOLUTION OF CLOSE-IN PLANETS
Soko Matsumura, S. J. Peale, Frederic A. Rasio · The Astrophysical Journal · 2010 · 235 citations · Full text
Natural Sciences, Astronomy, Physics +17
On the Relation between Hot Jupiters and the Roche Limit
Eric B. Ford, Frederic A. Rasio · The Astrophysical Journal · 2006 · 161 citations · Full text
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214

Centre National de la Recherche Scientifique
Paris, France
8 h-index
25 publications
1.3K citations
Northwestern University
Evanston, United States
6 h-index
12 publications
1.2K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
5 h-index
11 publications
527 citations

Ames Research Center
Mountain View, United States
5 h-index
9 publications
372 citations
University of Cambridge
Cambridge, United Kingdom
5 h-index
10 publications
562 citations
University of Maryland, College Park
College Park, United States
5 h-index
7 publications
509 citations

Cornell University
Ithaca, United States
5 h-index
10 publications
639 citations
Massachusetts Institute of Technology
Cambridge, United States
4 h-index
11 publications
705 citations
1–8 of 214
ApJ · 34 publications · 2.6K citations
23
h-index
10 publications · 606 citations
10
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9 publications · 594 citations
8
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6 publications · 264 citations
6
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4 publications · 240 citations
4
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