Re-Os isotopic constraints on the crystallization history of IIAB iron meteorites

Details Re-Os isotopic constraints on the crystallization history of IIAB iron meteorites Re-Os isotopic constraints on the crystallization history of IIAB iron meteorites

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28.1341s&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 341.

Computer Science

1

Iron Meteorites, Rhenium Isotopes, Osmium Isotopes, Crystallization, Group 2B Compounds, Meteoritic Composition, Iridium, Nickel, Minerals

Scientific paper

The formation time of IIAB iron meteorites is resolved. IIA samples were chosen to cover the whole range of Ir concentrations in order to obtain the maximum range in the Re/Os ratio. For the IIB subgroup, samples were confined to Ir contents greater than 0.05 ppm to avoid higher uncertainty introduced by the R blank. Re-Os expermental results for the IIB meteorites along with previously published IIA isochron are shown.

Affiliated with

Also associated with

No associations

Rating

Re-Os isotopic constraints on the crystallization history of IIAB iron meteorites 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 Re-Os isotopic constraints on the crystallization history of IIAB iron meteorites, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Re-Os isotopic constraints on the crystallization history of IIAB iron meteorites will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-874166