Possible Felsic Summit of Tuulikki Mons, Venus: Evidence from 1-Micron Surface Emissivity and Magellan-Viewed Morphology

Details Possible Felsic Summit of Tuulikki Mons, Venus: Evidence from 1-Micron Surface Emissivity and Magellan-Viewed Morphology Possible Felsic Summit of Tuulikki Mons, Venus: Evidence from 1-Micron Surface Emissivity and Magellan-Viewed Morphology

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1092b&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1092

Physics

Scientific paper

Based on the data taken by the Venus Monitoring Camera it was found that
the summit of Tuulikki Mons volcano shows the 1-µm emissivity
lower than that of the main body of the volcano. This suggests that the
volcano summit material may be close to felsic.

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