Bulk Chemical and Isotopic Compositions of Spinel-, Hibonite-rich Spherules: Clues to Their Origin

Details Bulk Chemical and Isotopic Compositions of Spinel-, Hibonite-rich Spherules: Clues to Their Origin Bulk Chemical and Isotopic Compositions of Spinel-, Hibonite-rich Spherules: Clues to Their Origin

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.2211s&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.2211

Physics

Scientific paper

Calculations predict condensation of melilite after hibonite and before
spinel, yet in CMs hib-sp inclusions are much more common than hib-mel
inclusions. Did hib-sp inclusions originally contain mel and lose Si and
Ca by evaporation?

Affiliated with

Also associated with

No associations

Rating

Bulk Chemical and Isotopic Compositions of Spinel-, Hibonite-rich Spherules: Clues to Their Origin 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 Bulk Chemical and Isotopic Compositions of Spinel-, Hibonite-rich Spherules: Clues to Their Origin, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Bulk Chemical and Isotopic Compositions of Spinel-, Hibonite-rich Spherules: Clues to Their Origin will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1358785