Tidal Heating Models
Tidal Heating Models is a theoretical framework within planetary science that quantifies the dissipation of tidal energy into internal heat within celestial bodies, distinguishing itself from other geophysical models by specifically accounting for periodic gravitational deformations induced by orbital interactions.
197
Publications
12.5K
Citations
453
Authors
270
Institutions
Publications per year
2017–2026
66
Parents
197
Disruption of dark matter substructure: fact or fiction?
Frank C. van den Bosch, Go Ogiya, Oliver Hahn et al. · Monthly Notices of the Royal Astronomical Society · 2017 · 310 citations · Full text
Natural Sciences, Astronomy, Physics +15
Peter Anninos, David Hobill, Edward Seidel et al. · Physical Review Letters · 1993 · 255 citations · Full text
How tidal heating in Io drives the galilean orbital resonance locks
C. F. Yoder · Nature · 1979 · 239 citations
Natural Sciences, Astronomy, Physics +14
1–5 of 197
453
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11
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11
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9
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7
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1–5 of 453
270
Planetary Science Institute
Tucson, United States
20 h-index
32 publications
2.5K citations
University of Arizona
Tucson, United States
18 h-index
39 publications
2.6K citations
University of California, Santa Cruz
Santa Cruz, United States
17 h-index
32 publications
2.8K citations
California Institute of Technology
Pasadena, United States
12 h-index
14 publications
1.5K citations

Centre National de la Recherche Scientifique
Paris, France
12 h-index
41 publications
3.5K citations
University of Washington
Seattle, United States
12 h-index
15 publications
1.1K citations
Princeton University
Princeton, United States
11 h-index
18 publications
1.8K citations
Jet Propulsion Laboratory
Pasadena, United States
10 h-index
14 publications
745 citations
1–8 of 270
ApJ · 33 publications · 2.8K citations
26
h-index
27 publications · 1.4K citations
20
h-index
20 publications · 1.4K citations
18
h-index
13 publications · 984 citations
13
h-index
PRD · 10 publications · 420 citations
11
h-index
1–5