Mercury Interior Structure

Mercury Interior Structure is a planetary interior model that specifies the compositional and physical stratification of Mercury’s internal layers, distinguished by its inference of a large, partially molten iron-rich core, thin mantle, and rigid lithosphere derived from geophysical and geochemical data.

56

Publications

2.7K

Citations

232

Authors

115

Institutions

Publications per year

2017–2026

14

Authors

232

  1. SC
    Sean C. Solomon

    Carnegie Institution for Science, United States

    9 publications · 1K citations

    9

    h-index

  2. TV
    Tim Van Hoolst

    Royal Observatory of Belgium, Belgium

    6 publications · 371 citations

    6

    h-index

  3. SA
    S. A. Hauck

    Case Western Reserve University, United States

    5 publications · 660 citations

    5

    h-index

  4. AR
    Attilio Rivoldini

    Royal Observatory of Belgium, Belgium

    4 publications · 260 citations

    4

    h-index

  5. MT
    M. T. Zuber

    Massachusetts Institute of Technology, United States

    4 publications · 522 citations

    4

    h-index

1–5 of 232

Venues

  1. Journal of Geophysical Research Planets

    9 publications · 422 citations

    9

    h-index

  2. Icarus

    9 publications · 485 citations

    9

    h-index

  3. Geophysical Research Letters

    8 publications · 222 citations

    8

    h-index

  4. Journal of Geophysical Research Atmospheres

    JGR · 5 publications · 168 citations

    5

    h-index

  5. Space Science Reviews

    4 publications · 223 citations

    4

    h-index

1–5