Venusian Surface Composition

Venusian Surface Composition is a geoscientific construct that specifies the elemental, mineralogical, and chemical makeup of the planetary surface of Venus, distinguished from other terrestrial planetary surface compositions by its unique geochemical signatures, volcanic origins, and extreme surface conditions.

72

Publications

3.4K

Citations

212

Authors

98

Institutions

Publications per year

2017–2026

17

Authors

212

  1. BF
    Bruce Fegley

    Planetary Science Institute, United States

    6 publications · 222 citations

    6

    h-index

  2. AH
    A. H. Treiman

    Lunar and Planetary Institute, United States

    4 publications · 250 citations

    4

    h-index

  3. WB
    William Bains

    Massachusetts Institute of Technology, United States

    4 publications · 106 citations

    4

    h-index

  4. JJ
    Janusz J. Petkowski

    Massachusetts Institute of Technology, United States

    4 publications · 106 citations

    4

    h-index

  5. SS
    Sara Seager

    Massachusetts Institute of Technology, United States

    4 publications · 106 citations

    4

    h-index

1–5 of 212

Venues

  1. Icarus

    26 publications · 1.1K citations

    20

    h-index

  2. Journal of Geophysical Research Atmospheres

    JGR · 5 publications · 494 citations

    5

    h-index

  3. Astrobiology

    5 publications · 155 citations

    5

    h-index

  4. Planetary and Space Science

    5 publications · 201 citations

    5

    h-index

  5. Geological Society of America Bulletin

    3 publications · 181 citations

    3

    h-index

1–5