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
259
HIGH-RESOLUTION ROTATION CURVES AND GALAXY MASS MODELS FROM THINGS
The Astronomical Journal · 2008 · 924 citations · Full text
Natural Sciences, Astronomy, Physics +14
P. J. McMillan · Monthly Notices of the Royal Astronomical Society · 2011 · 789 citations · Full text
Natural Sciences, Astronomy, Physics +17
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372

Centre National de la Recherche Scientifique
Paris, France
20 h-index
58 publications
3.9K citations
University of Arizona
Tucson, United States
13 h-index
27 publications
3.1K citations
University of Copenhagen
Copenhagen, Denmark
12 h-index
15 publications
1K citations
California Institute of Technology
Pasadena, United States
11 h-index
14 publications
2.9K citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
11 h-index
21 publications
1.2K citations

University of Groningen
Groningen, The Netherlands
10 h-index
16 publications
1K citations

Space Telescope Science Institute
Baltimore, United States
10 h-index
31 publications
4.6K citations
Jet Propulsion Laboratory
Pasadena, United States
10 h-index
24 publications
2.8K citations
1–8 of 372
62 publications · 6K citations
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ApJ · 60 publications · 4.6K citations
32
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15 publications · 1.3K citations
14
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AJ · 14 publications · 2K citations
12
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5 publications · 369 citations
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