An impact hypothesis for Venus argon anomalies

Details An impact hypothesis for Venus argon anomalies An impact hypothesis for Venus argon anomalies

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..701k&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 701.

Computer Science

Venus Surface, Anomalies, Argon, Abundance, Planetary Composition

Scientific paper

The Ar-36+38 argon-excess anomally of Venus has been hypothesized to have its origin in the impact of an outer solar system body of about 100-km diameter. A critical evaluation is made of this hypothesis and its competitors; it is judged that its status must for the time being remain one of 'Sherlock Holmes' type, in that something so improbable must be accepted when all alternatives are eliminated.

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