Geological-morphological description of the Lukelong-Okipeta Dorsa area (Venus surface photomap, sheet B-2)

Details Geological-morphological description of the Lukelong-Okipeta Dorsa area (Venus surface photomap, sheet B-2) Geological-morphological description of the Lukelong-Okipeta Dorsa area (Venus surface photomap, sheet B-2)

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988avest..22....3s&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 22, Jan.-Mar. 1988, p. 3-12. In Russian.

Mathematics

Logic

1

Geological Surveys, Photointerpretation, Planetary Geology, Venus Surface, Geological Faults, Plains, Venera Satellites

Scientific paper

An examination of sheet B-2 obtained from Veerna 15 and 16 radar data indicates that submeridional ridge belts at 175-245 deg E were produced by the extension of the lithosphere and the instrusion of linear magmatic bodies, forming ridges and banks on the surface. Latitudinal (normal to the belts) fault systems are visible on plain strips between the belts. The belt system as a whole is symmetric with respect to the axis along 200-210 deg E, where several hot spots are located.

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