Steep-sided domes on Venus - Characteristics, geologic setting, and eruption conditions from Magellan data

Details Steep-sided domes on Venus - Characteristics, geologic setting, and eruption conditions from Magellan data Steep-sided domes on Venus - Characteristics, geologic setting, and eruption conditions from Magellan data

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992jgr....9713445p&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 97, no. E8, Aug. 25, 1992, p. 13,445-13,478.

Mathematics

Logic

59

Domes (Geology), Magellan Spacecraft (Nasa), Planetary Geology, Satellite Imagery, Venus Surface, Data Flow Analysis, Planetary Structure, Rhyolite

Scientific paper

A survey of more than 95 percent of the Venus surface reveals 145 steep-sided domes which can be subdivided into a variety of morphologic forms, the most common being shaped like inverted bowls or flat-topped domes. Results of a preliminary analysis of the distribution and geologic setting of the domes are presented. The relation of the domes to analogous terrestrial features is examined, and possible models for their mode of emplacement are outlined.

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