New studies of Martian volcanoes

Details New studies of Martian volcanoes New studies of Martian volcanoes

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pggp.rept..174m&link_type=abstract

In NASA, Washington, Reports of Planetary Geology and Geophysics Program, 1990 p 174-176 (SEE N92-10728 01-91)

Physics

Geophysics

1

Evolution (Development), Mars (Planet), Mars Surface, Mars Volcanoes, Morphology, Planetary Geology, Topography, Calderas, Color, Depth, Mars Photographs, Radar Measurement, Slopes, Surface Properties, Viking Orbiter Spacecraft

Scientific paper

To investigate the morphology, topography, and evolution of volcanic constructs on Mars, researchers have been studying the volcanoes Olympus Mons, Tyrrhena Patera, and Apollinaris Patera. These studies relied upon the analysis of digital Viking orbiter images to measure the depth and slopes of the summit area of Olympus Mons, upon new Earth-based radar measurements for the analysis of the slopes of Tyrrhena Patera, and upon the color characteristics of the flanks of Apollinaris Patera for information regarding surface properties.

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