Geologic overview of the terrestrial planets

Details Geologic overview of the terrestrial planets Geologic overview of the terrestrial planets

Sep 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981mmsai..52..333a&link_type=abstract

(NATO, Advanced Study Institute on Comparative Study of the Planets, Vulcano, Italy, Sept. 14-25, 1981.) Società Astronomica Ita

Mathematics

Logic

Galilean Satellites, Planetary Geology, Terrestrial Planets, Lunar Geology, Mars (Planet), Mars Atmosphere, Planetary Evolution, Pre-Imbrian Period, Stratigraphy, Topography, Venus (Planet)

Scientific paper

The geologies of the terrestrial planets and satellites, with the exception of the earth, are reviewed. The lunar stratigraphic column is discussed, and the four systems within the column, the Pre-Imbrian, Imbrian, Eratosthenian and Copernican systems, are characterized. The global geologic evolution of Mars is outlined based primarily on Viking Orbiter and Mariner 9 data, and geologic processes associated with the presence of water and a thin atmosphere on Mars are considered. The topographic features of Venus observed by earth-based and Pioneer-Venus radars are discussed, and implications of the topography distributions for the relative internal structures of Venus and the earth are pointed out. Finally, attention is given to the geological histories of the Galilean satellites Callisto, Ganymede, Io and Europa as derived from the Voyager 1 and 2 encounters.

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