Synchronous Rotation
Synchronous Rotation is a state of orbital mechanics in which a celestial body's rotational period about its axis is equal to its orbital period around a primary body, resulting in the same hemisphere always facing the primary.
162
Publications
11.2K
Citations
534
Authors
250
Institutions
Publications per year
2017–2026
27
Variants
Tidal Locking
Parents
162
1–5 of 162
534
6
h-index
4
h-index
Institut de Mécanique Céleste et de Calcul des Éphémérides, France
4 publications · 156 citations
4
h-index
Institut de Mécanique Céleste et de Calcul des Éphémérides, France
4 publications · 156 citations
4
h-index
3
h-index
1–5 of 534
250

Centre National de la Recherche Scientifique
Paris, France
10 h-index
17 publications
1.5K citations
Massachusetts Institute of Technology
Cambridge, United States
8 h-index
11 publications
658 citations
Planetary Science Institute
Tucson, United States
8 h-index
16 publications
1K citations
University of Arizona
Tucson, United States
7 h-index
9 publications
1.4K citations

Kyoto University
Kyoto, Japan
7 h-index
25 publications
977 citations
Institut de Mécanique Céleste et de Calcul des Éphémérides
Paris, France
6 h-index
9 publications
333 citations
University of Washington
Seattle, United States
6 h-index
13 publications
922 citations

Cornell University
Ithaca, United States
6 h-index
15 publications
1.2K citations
1–8 of 250
ApJ · 31 publications · 4.4K citations
26
h-index
18 publications · 613 citations
14
h-index
AJ · 10 publications · 554 citations
10
h-index
8 publications · 319 citations
8
h-index
JGR · 6 publications · 225 citations
6
h-index
1–5