Microscale Distribution and Behavior of Th and K in Late-Stage Melts and Shock Melts in Olivine-Phyric Shergottites: Implications for the Interpretation of Remote Sensing and In Situ Measurements of the Martian Surface

Details Microscale Distribution and Behavior of Th and K in Late-Stage Melts and Shock Melts in Olivine-Phyric Shergottites: Implications for the Interpretation of Remote Sensing and In Situ Measurements of the Martian Surface Microscale Distribution and Behavior of Th and K in Late-Stage Melts and Shock Melts in Olivine-Phyric Shergottites: Implications for the Interpretation of Remote Sensing and In Situ Measurements of the Martian Surface

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.2317b&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.2317

Physics

Scientific paper

Th and K in many of the Mars surface lithologies are not reflected in
the martian meteorite collection. In this study, we examine the
variation in Sm, Th, K, and major elements in both late stage-melt and
shock-melt assemblages in martian meteorites.

Affiliated with

Also associated with

No associations

Rating

Microscale Distribution and Behavior of Th and K in Late-Stage Melts and Shock Melts in Olivine-Phyric Shergottites: Implications for the Interpretation of Remote Sensing and In Situ Measurements of the Martian Surface 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 Microscale Distribution and Behavior of Th and K in Late-Stage Melts and Shock Melts in Olivine-Phyric Shergottites: Implications for the Interpretation of Remote Sensing and In Situ Measurements of the Martian Surface, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Microscale Distribution and Behavior of Th and K in Late-Stage Melts and Shock Melts in Olivine-Phyric Shergottites: Implications for the Interpretation of Remote Sensing and In Situ Measurements of the Martian Surface will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1507173