Physics
Scientific paper
Jun 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975jgr....80.2444g&link_type=abstract
Journal of Geophysical Research, vol. 80, June 10, 1975, p. 2444-2460. Research supported by the Natural Environment Research C
Physics
52
Cratering, Gravitational Effects, Lunar Craters, Mercury (Planet), Meteorite Craters, Planetary Surfaces, Morphology, Mosaics, Planetary Structure, Spaceborne Photography
Scientific paper
Although the general morphologies of fresh mercurian and lunar craters are remarkably similar, comparisons of ejecta deposits, interior structures, and changes in morphology with size reveal important differences between the two populations of craters. The differences are attributable to the different gravity fields in which the craters were formed and have significant implications for the interpretation of cratering processes and their effects on all planetary bodies.
Dzurisin Dan
Gault Donald E.
Guest John E.
Malin Michael C.
Murray John B.
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