Crater Ejecta Rays

Crater Ejecta Rays is a geological surface feature consisting of radially outward-spreading, bright or high-albedo deposits of material ejected during the formation of an impact crater, distinguished from other ejecta patterns by their linear, ray-like morphology and often extensive reach beyond the crater rim.

64

Publications

3.5K

Citations

211

Authors

108

Institutions

Publications per year

2017–2026

10

Variants

Ejecta Rays

Authors

211

  1. BA
    B. A. Campbell

    Smithsonian Institution, United States

    5 publications · 274 citations

    6

    h-index

  2. BR
    B. R. Hawke

    University of Hawaii System, United States

    4 publications · 209 citations

    5

    h-index

  3. JW
    J. W. Head

    Brown University, United States

    5 publications · 603 citations

    5

    h-index

  4. PG
    P. G. Lucey

    University of Hawaiʻi at Mānoa, United States

    4 publications · 321 citations

    4

    h-index

  5. DT
    D. T. Blewett

    Johns Hopkins University Applied Physics Laboratory, United States

    4 publications · 250 citations

    4

    h-index

1–5 of 211

Venues

  1. Icarus

    17 publications · 1.1K citations

    17

    h-index

  2. Journal of Geophysical Research Atmospheres

    JGR · 11 publications · 770 citations

    11

    h-index

  3. Earth and Planetary Science Letters

    5 publications · 630 citations

    5

    h-index

  4. Journal of Geophysical Research Planets

    5 publications · 197 citations

    5

    h-index

  5. International Journal of Impact Engineering

    3 publications · 62 citations

    3

    h-index

1–5