Geological-morphological structure of Bell Regio (Photomaps of the Venus surface, sheet B-23)

Details Geological-morphological structure of Bell Regio (Photomaps of the Venus surface, sheet B-23) Geological-morphological structure of Bell Regio (Photomaps of the Venus surface, sheet B-23)

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987avest..21...16m&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 21, Jan.-Mar. 1987, p. 16-25. In Russian.

Mathematics

Logic

Geological Surveys, Photomaps, Planetary Geology, Venus Surface, Morphology, Photointerpretation, Plains, Planetary Evolution, Planetary Mapping, Tectonics, Volcanoes

Scientific paper

Four geological-morphological units are distinguished on the map: (1) remnants of pre-plain complexes, (2) striped plains, (3) smooth plains, (4) volcano-tectonical complexes. The Bell dome comprises several individual large volcanic constructions. Faults of different orientations and impact craters are recognised. A brief description of local geologic history is given.

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