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
Parents
64
A crater and its ejecta: An interpretation of Deep Impact
K. A. Holsapple, K. R. Housen · Icarus · 2006 · 268 citations
How old are young lunar craters?
H. Hiesinger, C. H. van der Bogert, J. H. Pasckert et al. · Journal of Geophysical Research Atmospheres · 2011 · 203 citations · Full text
The origin of lunar crater rays
B. R. Hawke, D. T. Blewett, P. G. Lucey et al. · Icarus · 2004 · 154 citations
1–5 of 64
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Johns Hopkins University Applied Physics Laboratory, United States
4 publications · 250 citations
4
h-index
1–5 of 211
108
Planetary Science Institute
Tucson, United States
9 h-index
13 publications
616 citations
University of Arizona
Tucson, United States
6 h-index
9 publications
710 citations
Smithsonian Institution
Washington, United States
5 h-index
6 publications
308 citations
Goddard Space Flight Center
Greenbelt, United States
5 h-index
9 publications
391 citations

Lunar and Planetary Institute
Houston, United States
4 h-index
4 publications
207 citations
United States Geological Survey
Reston, United States
3 h-index
4 publications
201 citations
Brown University
Providence, United States
3 h-index
5 publications
500 citations

Cornell University
Ithaca, United States
3 h-index
4 publications
231 citations
1–8 of 108
17 publications · 1.1K citations
17
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JGR · 11 publications · 770 citations
11
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5 publications · 630 citations
5
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5 publications · 197 citations
5
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3 publications · 62 citations
3
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