Nebula Models of Non-Equilibrium Mineralogy: Wark-Lovering Rims

Details Nebula Models of Non-Equilibrium Mineralogy: Wark-Lovering Rims Nebula Models of Non-Equilibrium Mineralogy: Wark-Lovering Rims

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.2095c&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.2095

Physics

3

Scientific paper

Non-equilibrium minerals in CAIs and AOAs can survive if the alteration
time, plausibly the time for atoms to diffuse into the mineral at the
local temperature, exceeds their evolution time to cooler regions,
plausibly due to turbulent diffusion.

Affiliated with

Also associated with

No associations

Rating

Nebula Models of Non-Equilibrium Mineralogy: Wark-Lovering Rims 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 Nebula Models of Non-Equilibrium Mineralogy: Wark-Lovering Rims, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Nebula Models of Non-Equilibrium Mineralogy: Wark-Lovering Rims will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1358202