Planetary Isostasy

Planetary Isostasy is a geophysical theory in planetary geophysics that describes the large-scale gravitational and buoyant equilibrium of a planet’s or moon’s outer shell, in which surface loads and topography are compensated by variations in crustal/lithospheric thickness or density above a deeper, nearly hydrostatic interior.

149

Publications

10.1K

Citations

420

Authors

178

Institutions

Publications per year

2017–2026

12

Authors

420

  1. MT
    M. T. Zuber

    Massachusetts Institute of Technology, United States

    5 publications · 336 citations

    5

    h-index

  2. NM
    Nils‐Axel Mörner

    Stockholm University, Sweden

    5 publications · 1K citations

    4

    h-index

  3. BG
    B. G. Bills

    Jet Propulsion Laboratory, United States

    4 publications · 163 citations

    4

    h-index

  4. RJ
    R. J. Phillips

    Southwest Research Institute, United States

    3 publications · 375 citations

    3

    h-index

  5. SC
    Sean C. Solomon

    Carnegie Institution for Science, United States

    3 publications · 114 citations

    3

    h-index

1–5 of 420

Venues

  1. Icarus

    35 publications · 1.9K citations

    23

    h-index

  2. Journal of Geophysical Research Atmospheres

    JGR · 10 publications · 700 citations

    10

    h-index

  3. Earth Moon and Planets

    9 publications · 320 citations

    9

    h-index

  4. Physics of The Earth and Planetary Interiors

    7 publications · 217 citations

    7

    h-index

  5. Celestial Mechanics and Dynamical Astronomy

    7 publications · 191 citations

    7

    h-index

1–5