Mass Distribution Models

Mass Distribution Models is a theoretical framework in planetary science that specifies the spatial arrangement of mass within celestial bodies by mathematically representing density variations as a function of radial distance, thereby enabling the calculation of gravitational and rotational properties such as the moment of inertia.

259

Publications

19.8K

Citations

828

Authors

372

Institutions

Publications per year

2017–2026

45

Authors

828

  1. CC
    C. Carignan

    Université de Montréal, Canada

    6 publications · 568 citations

    6

    h-index

  2. JK
    Jean‐Paul Kneib

    Centre National de la Recherche Scientifique, France

    6 publications · 1.1K citations

    6

    h-index

  3. PT
    P. T. de Zeeuw

    Leiden University, Netherlands

    6 publications · 238 citations

    6

    h-index

  4. HD
    H. Dejonghe

    Ghent University, Belgium

    5 publications · 375 citations

    5

    h-index

  5. JB
    James Binney

    University of Oxford, United Kingdom

    5 publications · 1.2K citations

    5

    h-index

1–5 of 828

Venues

  1. 33

    h-index

  2. The Astrophysical Journal

    ApJ · 60 publications · 4.6K citations

    32

    h-index

  3. Astronomy and Astrophysics

    15 publications · 1.3K citations

    14

    h-index

  4. The Astronomical Journal

    AJ · 14 publications · 2K citations

    12

    h-index

  5. Icarus

    5 publications · 369 citations

    5

    h-index

1–5