The morphometry of impact craters on Venus

Details The morphometry of impact craters on Venus The morphometry of impact craters on Venus

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989avest..23...39i&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 23, Jan.-Mar. 1989, p. 39-49. In Russian.

Astronomy and Astrophysics

Astronomy

2

Meteoritic Damage, Morphology, Planetary Craters, Venus (Planet), Radar Imagery, Radio Altimeters, Venera Satellites

Scientific paper

The paper presents the results of a morphometric analysis of impact craters on Venus identified on Venera 15/16 SAR images. Estimates are made of the depth of the craters, the heights of the central peaks over the crater floor, and the angle of the inner slope of the craters. The estimates obtained are compared with analogous data for terrestrial and lunar meteoritic craters. It is concluded that, in relation to the depth/diameter ratio, the craters of Venus are close to terrestrial impact craters.

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