Magma Ocean Solidification

Magma Ocean Solidification is a planetary-scale thermal evolution process denoting the gradual crystallization and differentiation of a global, molten silicate layer enveloping a nascent terrestrial planet, driven by conductive and convective heat loss, gravitational settling of dense minerals, and buoyant rise of light components, ultimately establishing the primordial mantle stratification and initiating crustal formation.

114

Publications

9.3K

Citations

340

Authors

190

Institutions

Publications per year

2017–2026

60

Authors

340

  1. LT
    L. T. Elkins‐Tanton

    Massachusetts Institute of Technology, United States

    12 publications · 2.4K citations

    12

    h-index

  2. EM
    E. M. Parmentier

    Brown University, United States

    7 publications · 641 citations

    7

    h-index

  3. CB
    Charles‐Édouard Boukaré

    Centre National de la Recherche Scientifique, France

    5 publications · 329 citations

    5

    h-index

  4. WV
    W. van Westrenen

    Vrije Universiteit Amsterdam, Netherlands

    5 publications · 428 citations

    5

    h-index

  5. MB
    Martin Bizzarro

    University of Copenhagen, Denmark

    4 publications · 292 citations

    4

    h-index

1–5 of 340

Venues

  1. Earth and Planetary Science Letters

    13 publications · 1.8K citations

    13

    h-index

  2. Geophysical Research Letters

    10 publications · 444 citations

    10

    h-index

  3. Geochimica et Cosmochimica Acta

    8 publications · 514 citations

    8

    h-index

  4. Journal of Geophysical Research Planets

    6 publications · 310 citations

    6

    h-index

  5. Journal of Geophysical Research Solid Earth

    5 publications · 240 citations

    5

    h-index

1–5