Evidence for Possible Exposed Water Ice Deposits in Martian Low Latitude Chasms and Chaos

Details Evidence for Possible Exposed Water Ice Deposits in Martian Low Latitude Chasms and Chaos Evidence for Possible Exposed Water Ice Deposits in Martian Low Latitude Chasms and Chaos

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.2016l&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.2016

Physics

1

Scientific paper

Morphology, modeling of sublimational erosion, thermal inertia similar
to the north polar layered terrain, and relatively high albedo lead us
to propose that interior layer deposits in Juventae Chasma may consist
of residual water ice perhaps mixed with varying amounts of dust or
sand.

Affiliated with

Also associated with

No associations

Rating

Evidence for Possible Exposed Water Ice Deposits in Martian Low Latitude Chasms and Chaos does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Evidence for Possible Exposed Water Ice Deposits in Martian Low Latitude Chasms and Chaos, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evidence for Possible Exposed Water Ice Deposits in Martian Low Latitude Chasms and Chaos will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1642827