The distribution of small domes on Venus based on Venera-15 and -16 radar data

Details The distribution of small domes on Venus based on Venera-15 and -16 radar data The distribution of small domes on Venus based on Venera-15 and -16 radar data

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988avest..22..287s&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 22, Oct.-Dec. 1988, p. 287-297. In Russian.

Mathematics

Logic

3

Geological Surveys, Planetary Geology, Radar Maps, Satellite Observation, Venus Surface, Cupolas, Domes, Spatial Distribution, Tectonics, Venera Satellites

Scientific paper

Radar images have revealed the presence of small (1-20 km in diameter) domes on the surface of Venus. These domes, which are volcanic in nature, are unevenly distributed with most being organized into clusters. Some of these clusters are believed to be independent structural-tectonic formations since they are well defined in the relief and gravitational field of the planet.

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