Origin of the Refractory Component in Ferromagnesian Chondrules and Constraints on their Thermal Histories: Clues from Glass Inclusions in Olivine from Carbonaceous Chondrites

Details Origin of the Refractory Component in Ferromagnesian Chondrules and Constraints on their Thermal Histories: Clues from Glass Inclusions in Olivine from Carbonaceous Chondrites Origin of the Refractory Component in Ferromagnesian Chondrules and Constraints on their Thermal Histories: Clues from Glass Inclusions in Olivine from Carbonaceous Chondrites

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2071b&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2071

Computer Science

Scientific paper

Compositions of glass inclusions in olivine from CM, CR, and CV
chondrites can be described as mixtures of Type C CAIs and SiO2 that are
far from olivine saturation. This places severe constraints on possible
thermal histories.

Affiliated with

Also associated with

No associations

Rating

Origin of the Refractory Component in Ferromagnesian Chondrules and Constraints on their Thermal Histories: Clues from Glass Inclusions in Olivine from Carbonaceous Chondrites 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 Origin of the Refractory Component in Ferromagnesian Chondrules and Constraints on their Thermal Histories: Clues from Glass Inclusions in Olivine from Carbonaceous Chondrites, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Origin of the Refractory Component in Ferromagnesian Chondrules and Constraints on their Thermal Histories: Clues from Glass Inclusions in Olivine from Carbonaceous Chondrites will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1391606