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

Authors

453

  1. FN
    F. Nimmo

    University of California, Santa Cruz, United States

    12 publications · 749 citations

    12

    h-index

  2. RH
    René Heller

    Helmholtz-Zentrum Dresden-Rossendorf, Germany

    11 publications · 537 citations

    11

    h-index

  3. RB
    Rory Barnes

    University of Washington, United States

    11 publications · 769 citations

    11

    h-index

  4. RG
    R. Greenberg

    University of Arizona, United States

    9 publications · 613 citations

    9

    h-index

  5. BJ
    Brian Jackson

    Boise State University, United States

    7 publications · 625 citations

    7

    h-index

1–5 of 453

Venues

  1. The Astrophysical Journal

    ApJ · 33 publications · 2.8K citations

    26

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    27 publications · 1.4K citations

    20

    h-index

  3. Icarus

    20 publications · 1.4K citations

    18

    h-index

  4. Astronomy and Astrophysics

    13 publications · 984 citations

    13

    h-index

  5. Physical review. D/Physical review. D.

    PRD · 10 publications · 420 citations

    11

    h-index

1–5