Computer Science
Scientific paper
Oct 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986icar...68...77l&link_type=abstract
Icarus (ISSN 0019-1035), vol. 68, Oct. 1986, p. 77-86.
Computer Science
24
Cratering, Deimos, Ejecta, Moon, Phobos, Planetary Craters, Size Distribution, Spatial Distribution, Planets, Satellites, Phobos, Deimos, Mars, Earth, Moon, Distribution, Size, Ejecta, Craters, Comparisons, Techniques, Photographs
Scientific paper
Ejecta block characteristics observed on Phobos, Deimos, and the moon are examined. The analyzed source craters on Deimos are 0.8-2.3 km in diameter, those on Phobos are 1.5-10 km, and the lunar craters are between 0.2-3.5 km in diameter. The size and radial distribution of the ejecta blocks for the three bodies are compared. It is observed that the size distribution of the ejecta blocks surrounding craters on the three objects are basically similar, and the radial distribution of the blocks for Phobos and the moon are the same (within 2 radii of the crater center); however, the ejecta on Deimos are more dispersed (greater than or equal to 2 radii from the crater center).
Lee Wai Shing
Thomas Patrick
Ververka J.
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