Differentiated Meteorites

Differentiated Meteorites is a class of meteorites that originates from planetary bodies that underwent magmatic differentiation, distinguished by their composition reflecting separation into core, mantle, and crustal components due to internal melting and reconfiguration.

109

Publications

8.5K

Citations

398

Authors

168

Institutions

Publications per year

2017–2026

17

Authors

398

  1. ER
    E. R. D. Scott

    University of Hawaiʻi at Mānoa, United States

    6 publications · 948 citations

    6

    h-index

  2. MB
    Martin Bizzarro

    University of Copenhagen, Denmark

    6 publications · 566 citations

    6

    h-index

  3. CA
    C. A. Raymond

    Jet Propulsion Laboratory, United States

    6 publications · 1.1K citations

    6

    h-index

  4. HY
    H. Y. McSween

    University of Tennessee at Knoxville, United States

    5 publications · 1.1K citations

    5

    h-index

  5. CT
    C. T. Russell

    University of California, Los Angeles, United States

    5 publications · 1K citations

    5

    h-index

1–5 of 398

Venues

  1. Geochimica et Cosmochimica Acta

    18 publications · 1.2K citations

    18

    h-index

  2. Meteoritics and Planetary Science

    15 publications · 1K citations

    13

    h-index

  3. Science

    8 publications · 1.4K citations

    8

    h-index

  4. Nature

    8 publications · 727 citations

    8

    h-index

  5. Meteoritics

    6 publications · 292 citations

    6

    h-index

1–5