Kinetics of Spinel Formation Under Circumstellar Conditions

Details Kinetics of Spinel Formation Under Circumstellar Conditions Kinetics of Spinel Formation Under Circumstellar Conditions

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2840h&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2840

Physics

Scientific paper

Spinel formation by a reaction between corundum and Mg gas was
experimentally studied. The condensation coefficient was estimated to be
~0.03 at the supersaturation ratio of ~10, which is applicable to spinel
formation in circumstellar environments.

Affiliated with

Also associated with

No associations

Rating

Kinetics of Spinel Formation Under Circumstellar Conditions 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 Kinetics of Spinel Formation Under Circumstellar Conditions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Kinetics of Spinel Formation Under Circumstellar Conditions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1398364