Physics
Scientific paper
Feb 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990georl..17..175b&link_type=abstract
Geophysical Research Letters (ISSN 0094-8276), vol. 17, Feb. 1990, p. 175-178.
Physics
9
Geomorphology, Planetary Craters, Planetary Geology, Venus Surface, Volcanoes, Calderas, Geochronology, Hypervelocity Impact, Tectonics, Venus, Cleopatra, Craters, Venera 15 Mission, Venera 16 Mission, Depth, Venera Missions, Origin, Formation, Impacts, Volcanism, Morphology, Morphometry, Photographs, Size
Scientific paper
The morphology and morphometry of the 100-km diameter, 2.4-km deep Cleopatra crater on Venus are examined using Venera 15/16 images. The Cleopatra crater is compared to circular structures on Venus, Mercury, Mars, the earth and the moon. Consideration is given to the possible causes for the genesis of the Cleopatra crater. It is concluded that Cleopatra has a clear impact basin morphology with an anomalous crater depth.
Basilevsky Alexander T.
Ivanov Boris A.
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