Comparison of Pyrrhotite from Interplanetary Dust and Meteorites: Evidence for Different Formation Environments

Details Comparison of Pyrrhotite from Interplanetary Dust and Meteorites: Evidence for Different Formation Environments Comparison of Pyrrhotite from Interplanetary Dust and Meteorites: Evidence for Different Formation Environments

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1411f&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1411

Physics

Scientific paper

Five pyrrhotite-dominated IDPs, examined by x-ray microprobe, have Se
contents averaging ~1.6 times the Se content of pyrrhotite from the CI
meteorite Orgueil, indicating IDP pyrrhotite formed in a different
environment than Orgueil pyrrhotite.

Affiliated with

Also associated with

No associations

Rating

Comparison of Pyrrhotite from Interplanetary Dust and Meteorites: Evidence for Different Formation Environments 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 Comparison of Pyrrhotite from Interplanetary Dust and Meteorites: Evidence for Different Formation Environments, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Comparison of Pyrrhotite from Interplanetary Dust and Meteorites: Evidence for Different Formation Environments will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1616485