Mars Crustal Dichotomy: Large Lowland Impact Basins may have Formed in Pre-Thinned Crust

Details Mars Crustal Dichotomy: Large Lowland Impact Basins may have Formed in Pre-Thinned Crust Mars Crustal Dichotomy: Large Lowland Impact Basins may have Formed in Pre-Thinned Crust

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1342f&link_type=abstract

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

Computer Science

Scientific paper

Large impact basins in the martian lowlands have thinner crust than do
basins of comparable size in the highlands, perhaps because they formed
on crust already thinned by some earlier process.

Affiliated with

Also associated with

No associations

Rating

Mars Crustal Dichotomy: Large Lowland Impact Basins may have Formed in Pre-Thinned Crust 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 Mars Crustal Dichotomy: Large Lowland Impact Basins may have Formed in Pre-Thinned Crust, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Mars Crustal Dichotomy: Large Lowland Impact Basins may have Formed in Pre-Thinned Crust will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-769341