Mineralogy of West Tithonium-Noctis Labyrinthus, Mars: Putative Volcanism on Noctis Canyons Floors

Details Mineralogy of West Tithonium-Noctis Labyrinthus, Mars: Putative Volcanism on Noctis Canyons Floors Mineralogy of West Tithonium-Noctis Labyrinthus, Mars: Putative Volcanism on Noctis Canyons Floors

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1592m&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

1

Scientific paper

A large number of pyroxene-rich areas are detected west of Valles
Marineris with OMEGA spectral data. Most of them consist of sand dunes,
but some rocky outcrops in the floor of Noctis could represent fresh
lava flows formed inside the canyons.

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