Planetary Tidal Locking is a geophysical state in which an astronomical body maintains a fixed rotational period relative to its orbital period around a host star, resulting in one hemisphere perpetually facing the star while the opposite hemisphere remains in permanent darkness.
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Publications
2.3K
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65
Authors
58
Institutions
Publications per year
2017–2026
15
Variants
Tidal Locking
Parents
Publications
29
Tidal locking of habitable exoplanets
Celestial Mechanics and Dynamical Astronomy · 2017 · 214 citations · Full text
1–5 of 29
Authors
65
- FS
3
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- ML
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- JY
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- IR
2
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- MH
2
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1–5 of 65
Institutions
58
University of Chicago
Chicago, United States
3 h-index
7 publications
371 citations
Peking University
Beijing, China
3 h-index
7 publications
179 citations
Planetary Science Institute
Tucson, United States
2 h-index
4 publications
274 citations
Laboratory for Atmospheric and Space Physics
Boulder, United States
2 h-index
2 publications
285 citations
NASA Astrobiology Institute
Mountain View, United States
2 h-index
4 publications
334 citations
California Institute of Technology
Pasadena, United States
2 h-index
1 publications
90 citations
Space Research Institute
Graz, Austria
2 h-index
5 publications
788 citations
Austrian Academy of Sciences
Vienna, Austria
2 h-index
5 publications
788 citations
1–8 of 58
Venues
- The Astrophysical Journal
ApJ · 6 publications · 481 citations
7
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- Astrobiology
3 publications · 81 citations
3
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- The Astrophysical Journal Letters
2 publications · 74 citations
2
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- Nature Astronomy
2 publications · 49 citations
2
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- Astronomy and Astrophysics
2 publications · 352 citations
2
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1–5