A Probable Fluid Lava Flow in the Hebes Mensa (Mars) Studied by HRSC Images

Details A Probable Fluid Lava Flow in the Hebes Mensa (Mars) Studied by HRSC Images A Probable Fluid Lava Flow in the Hebes Mensa (Mars) Studied by HRSC Images

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1648o&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1648

Physics

Scientific paper

A dark rills and pond features on the northern slope of the Hebes Mensa
could be formed by fluid lava flows. Mud and debris flows can be taken
into account, but the stability of the feature (observed during Viking
time) support a volcanic origin.

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