Light Lithophile Element Trends in Nakhlite NWA 817 Pyroxenes: Implications for Water on Mars

Details Light Lithophile Element Trends in Nakhlite NWA 817 Pyroxenes: Implications for Water on Mars Light Lithophile Element Trends in Nakhlite NWA 817 Pyroxenes: Implications for Water on Mars

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1230m&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1230

Other

Scientific paper

Abundances of LLE are strongly zoned in augites of the NWA 817 nakhlite.
Be and B increase to grain rims, consistent with their geochemical
behavior as incompatible elements. Oddly, Li increases outward in some
rims, but decreases in others.

Affiliated with

Also associated with

No associations

Rating

Light Lithophile Element Trends in Nakhlite NWA 817 Pyroxenes: Implications for Water on Mars 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 Light Lithophile Element Trends in Nakhlite NWA 817 Pyroxenes: Implications for Water on Mars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Light Lithophile Element Trends in Nakhlite NWA 817 Pyroxenes: Implications for Water on Mars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1353630