Stability and Origin of Lunar Polar Volatiles

Details Stability and Origin of Lunar Polar Volatiles Stability and Origin of Lunar Polar Volatiles

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1185b&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1185

Other

1

Scientific paper

All detected species except H2, CO, and CH4 are stable against
evaporation at the LCROSS impact site. Cometary NH3, C2H4, CH3OH, and
CH4 can survive during low-speed impacts while other detected species
can be formed during impacts of O-rich comets.

Affiliated with

Also associated with

No associations

Rating

Stability and Origin of Lunar Polar Volatiles 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 Stability and Origin of Lunar Polar Volatiles, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stability and Origin of Lunar Polar Volatiles will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-866688