Self-Consistent Models of the Dusty Subdisk in the Solar Nebula: Implications for Meteorites

Details Self-Consistent Models of the Dusty Subdisk in the Solar Nebula: Implications for Meteorites Self-Consistent Models of the Dusty Subdisk in the Solar Nebula: Implications for Meteorites

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002lpi....33.1230w&link_type=abstract

33rd Annual Lunar and Planetary Science Conference, March 11-15, 2002, Houston, Texas, abstract no.1230

Physics

Scientific paper

The space density and relative velocities in a particle layer in the
nebular midplane are constrained by shear-induced turbulence. Chondrule
formation appears to require transient deviations from steady-state
conditions.

Affiliated with

Also associated with

No associations

Rating

Self-Consistent Models of the Dusty Subdisk in the Solar Nebula: Implications for Meteorites 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 Self-Consistent Models of the Dusty Subdisk in the Solar Nebula: Implications for Meteorites, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Self-Consistent Models of the Dusty Subdisk in the Solar Nebula: Implications for Meteorites will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-785834