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- W1480923194 abstract "Approximately 950 impact craters have been identified on the surface of Venus, mainly in Magellan radar images. From a combination of Earth-based Arecibo, Venera 15/1, and Magellan radar images, we have interpreted 72 as unequivocal peak-ring craters and four as multiringed basins. The morphological and structural preservation of these craters is high owing to the low level of geologic activity on the venusian surface (which is in some ways similar to the terrestrial benthic environment). Thus these craters should prove crucial to understanding the mechanics of ringed crater formation. They are also the most direct analogs for craters formed on the Earth in Phanerozoic time, such as Chicxulub. We summarize our findings to date concerning these structures." @default.
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- W1480923194 date "1994-01-01" @default.
- W1480923194 modified "2023-09-27" @default.
- W1480923194 title "Some Implications of Large Impact Craters and Basins on Venus for Terrestrial Ringed Craters and Planetary Evolution" @default.
- W1480923194 hasPublicationYear "1994" @default.
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