Subduction on the margins of coronae on Venus: Evidence from radiothermal emissivity measurements

Details Subduction on the margins of coronae on Venus: Evidence from radiothermal emissivity measurements Subduction on the margins of coronae on Venus: Evidence from radiothermal emissivity measurements

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993lpi....24.1205r&link_type=abstract

In Lunar and Planetary Inst., Twenty-Fourth Lunar and Planetary Science Conference. Part 3: N-Z p 1205-1206 (SEE N94-20636 05-91

Mathematics

Logic

Emissivity, Subduction (Geology), Venus (Planet), Coronas, Mineralogy, Planetary Crusts, Planetary Geology

Scientific paper

Retrograde subduction has been suggested to occur at three coronae on Venus: Latona, Artemis, and Eithinoha. Using the mineralogical arguments of Klose to explain surface emissivity, a study of radio thermal emissivity of Venus coronae showed that emissivity changes associated with Latona, Artemis, and Ceres imply the same crustal movements predicted by the subduction model of Sandwell and Schubert.

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