Computer Science
Scientific paper
Sep 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990icar...87..156b&link_type=abstract
Icarus (ISSN 0019-1035), vol. 87, Sept. 1990, p. 156-179.
Computer Science
82
Impact Damage, Mars Craters, Mars Surface, Meteorite Craters, Statistical Correlation, Ejecta, Gravitational Effects, Hypervelocity Impact, Planetary Composition
Scientific paper
An effort is made to establish the ability of a correlation between crater morphology and latitude, diameter, and terrain, to discriminate among the effects of impact energy, atmosphere, and subsurface volatiles in 3819 larger-than-8 km diameter craters distributed over the Martian surface. It is noted that changes in ejecta and interior morphology correlate with increases in crater diameter, and that while many of the interior structures exhibit distributions interpretable as terrain-dependent, central peak and peak ring interior morphologies exhibit minimal relationships with planetary properties.
Barlow Nadine G.
Bradley Tracy L.
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