Venus - The nature of the surface from Venera panoramas

Details Venus - The nature of the surface from Venera panoramas Venus - The nature of the surface from Venera panoramas

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984jgr....89.3381g&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 89, May 10, 1984, p. 3381-3399.

Mathematics

Logic

42

Planetary Geology, Satellite-Borne Photography, Venera Satellites, Venus Surface, Landing Sites, Lava, Panoramic Cameras, Petrology, Viking Lander Spacecraft, Venus, Surface, Venera Missions, Imagery, Venra 9, Venra 10, Venera 13, Venera 14, Landers, Anlysis, Geology, Beta Phoebe, Landing Sites, Data, Comparisons, Features, Eolian Processes, Hypotheses, Lava Flows, Crust, Formation, Cooling, Fractures, Morphology, Terrain, Image Processing, Topography, Basalts, Geochemistry, Erosion, Remote Sensing, Equipme

Scientific paper

The present investigation has the objective to analyze the information collected by the Soviet Venera 9, 10, 13, and 14 lander spacecraft imaging systems. The analysis is to make a systematic comparison with other planetary surfaces possible, and an improved understanding of the surface of the planet Venus is to be provided. Attention is given to the imaging systems and transformation methods, observations, the observed characteristics of Venera lander sites, and an interpretation of the geological processes responsible for the features observed in the Venera panoramas. It is concluded that the present Venus environment is considerably different in terms of temperature, pressure, and atmosphere composition from the present terrestrial subaerial environment.

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