Models of Hecate Chasma, Venus and Implications for Active (?) Extension

Details Models of Hecate Chasma, Venus and Implications for Active (?) Extension Models of Hecate Chasma, Venus and Implications for Active (?) Extension

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1422s&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1422

Physics

Scientific paper

A simple uniform extension model applied to Hecate Chasma provides a
good fit to rift style and width for an extensional velocity of ~0.1
cm/yr. The transition between narrow and wide rifts occurs at a similar
width (~125 km) as for rifts on Earth.

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