Constraints on Tessera Composition from Modeling of Tellus Regio, Venus

Details Constraints on Tessera Composition from Modeling of Tellus Regio, Venus Constraints on Tessera Composition from Modeling of Tellus Regio, Venus

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2053g&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2053

Computer Science

Scientific paper

Fold wavelengths in a collision zone in Tellus Regio are used to
constrain tessera lithospheric parameters including composition. Dry
mafic and felsic rheologies are reasonable, as well as some wet mafic
and felsic rheologies under high strain rate.

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