Mercury Thermal Evolution

Mercury Thermal Evolution is a planetary science theory that elucidates the temporal development and dissipation of internal heat within Mercury, distinguishing itself by integrating the planet's unique thermochemical properties, rapid cooling history, and prolonged tectonic deformation to explain observed surface features and global contraction.

129

Publications

5.5K

Citations

385

Authors

203

Institutions

Publications per year

2017–2026

18

Authors

385

  1. SC
    Sean C. Solomon

    Carnegie Institution for Science, United States

    6 publications · 496 citations

    6

    h-index

  2. MM
    Matteo Massironi

    University of Padua, Italy

    4 publications · 87 citations

    4

    h-index

  3. SE
    Stephen E. Grasby

    Geological Survey of Canada, Canada

    3 publications · 94 citations

    3

    h-index

  4. KC
    Kamel Charrada

    Institut Préparatoire aux Études d'Ingénieurs de Monastir, Tunisia

    3 publications · 67 citations

    3

    h-index

  5. CR
    C. R. Chapman

    Southwest Research Institute, United States

    3 publications · 202 citations

    3

    h-index

1–5 of 385

Venues

  1. Icarus

    15 publications · 1.3K citations

    13

    h-index

  2. Earth and Planetary Science Letters

    10 publications · 482 citations

    10

    h-index

  3. 7

    h-index

  4. Journal of Non-Crystalline Solids

    5 publications · 91 citations

    5

    h-index

  5. Planetary and Space Science

    5 publications · 175 citations

    5

    h-index

1–5