Nebular Condensation Under Incomplete Equilibrium: Implications for the Fine-grained Spinel-rich CAIs

Details Nebular Condensation Under Incomplete Equilibrium: Implications for the Fine-grained Spinel-rich CAIs Nebular Condensation Under Incomplete Equilibrium: Implications for the Fine-grained Spinel-rich CAIs

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1238p&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1238

Computer Science

1

Scientific paper

The fine-grained spinel-rich CAIs could have formed by incomplete
condensation of a gas of solar composition at low pressures, when the
cooling rate of a parcel of gas is higher than the growth rate of the
mineral condensing from this gas.

Affiliated with

Also associated with

No associations

Rating

Nebular Condensation Under Incomplete Equilibrium: Implications for the Fine-grained Spinel-rich CAIs 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 Nebular Condensation Under Incomplete Equilibrium: Implications for the Fine-grained Spinel-rich CAIs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Nebular Condensation Under Incomplete Equilibrium: Implications for the Fine-grained Spinel-rich CAIs will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1353661