Impact Vapor Generation Inferred from Run-out Flows on Venus

Details Impact Vapor Generation Inferred from Run-out Flows on Venus Impact Vapor Generation Inferred from Run-out Flows on Venus

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996lpi....27.1287s&link_type=abstract

Lunar and Planetary Science, volume 27, page 1287

Physics

1

Craters, Impact Vapor, Impacts, Run-Out Flows, Venus

Scientific paper

Oblique impact craters on Venus are commonly associated with long run-out flows extending downrange. Parametric hydrocode calculations are used to assess the variables controlling the downrange off-set of the source region of such flows. We find that the impact-angle dependence of the downrange offset of the source region of the run-out flows measured from the point of impact can be readily explained by energy and momentum coupling efficiencies in the downrange impact vapor/melt.

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