Asteroidal Regolith

Asteroidal Regolith is a type of planetary regolith composed of fragmented rock and dust material produced by impact and space weathering processes specifically on the surfaces of asteroids, distinguished from regolith on planets or moons by its formation in microgravity environments and its unique compositional and structural characteristics derived from primitive, unmelted precursor materials.

174

Publications

12.2K

Citations

937

Authors

363

Institutions

Publications per year

2017–2026

49

Authors

937

  1. CM
    C. M. Pieters

    Brown University, United States

    9 publications · 1.8K citations

    9

    h-index

  2. ME
    M. E. Zolensky

    Johnson Space Center, United States

    9 publications · 861 citations

    9

    h-index

  3. CR
    C. R. Chapman

    Southwest Research Institute, United States

    8 publications · 824 citations

    8

    h-index

  4. PC
    P. C. Thomas

    Cornell University, United States

    7 publications · 913 citations

    7

    h-index

  5. BR
    B. Rozitis

    The Open University, United Kingdom

    7 publications · 273 citations

    7

    h-index

1–5 of 937

Venues

  1. Icarus

    28 publications · 1.9K citations

    22

    h-index

  2. Meteoritics and Planetary Science

    20 publications · 2K citations

    17

    h-index

  3. Science

    11 publications · 2.3K citations

    11

    h-index

  4. Journal of Geophysical Research Atmospheres

    JGR · 6 publications · 426 citations

    6

    h-index

  5. NASA Technical Reports Server (NASA)

    Repository · 6 publications · 163 citations

    6

    h-index

1–5