Constraints on the Origin of Magnesian Chondrules and on the Gaseous Reservoirs in the Early Solar System: An Oxygen Study

Details Constraints on the Origin of Magnesian Chondrules and on the Gaseous Reservoirs in the Early Solar System: An Oxygen Study Constraints on the Origin of Magnesian Chondrules and on the Gaseous Reservoirs in the Early Solar System: An Oxygen Study

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.2017l&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Computer Science

Scientific paper

A survey of the oxygen isotopic composition of the major silicate phases
in magnesian chondrules shows that most of the olivines are relict
grains and that gas-melt interaction played a major role in the
chondrule crystallization history.

Affiliated with

Also associated with

No associations

Rating

Constraints on the Origin of Magnesian Chondrules and on the Gaseous Reservoirs in the Early Solar System: An Oxygen Study 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 Constraints on the Origin of Magnesian Chondrules and on the Gaseous Reservoirs in the Early Solar System: An Oxygen Study, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Constraints on the Origin of Magnesian Chondrules and on the Gaseous Reservoirs in the Early Solar System: An Oxygen Study will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-772659