Possibility of Karst Morphology on the Martian Surface at the Meridiani Landing Site from Comparison with Terrestrial Analogs

Details Possibility of Karst Morphology on the Martian Surface at the Meridiani Landing Site from Comparison with Terrestrial Analogs Possibility of Karst Morphology on the Martian Surface at the Meridiani Landing Site from Comparison with Terrestrial Analogs

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1051b&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1051

Physics

Scientific paper

On Opportunity images of the 70-74 sols chains of pits forming a trench
pattern can be interpreted as dolines, the whole trench pattern as a
solution groove, both belonging to counterpart terrestrial karst
morphology.

Affiliated with

Also associated with

No associations

Rating

Possibility of Karst Morphology on the Martian Surface at the Meridiani Landing Site from Comparison with Terrestrial Analogs 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 Possibility of Karst Morphology on the Martian Surface at the Meridiani Landing Site from Comparison with Terrestrial Analogs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Possibility of Karst Morphology on the Martian Surface at the Meridiani Landing Site from Comparison with Terrestrial Analogs will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1352893