From chondrules to planetesimals: solids and turbulence in the Solar Nebula.

Details From chondrules to planetesimals: solids and turbulence in the Solar Nebula. From chondrules to planetesimals: solids and turbulence in the Solar Nebula.

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996nascp3339..175d&link_type=abstract

Scientific conference: From stardust to planetesimals, p. 175 - 178

Physics

Solar Nebula: Chondrules, Solar Nebula: Planetesimals

Scientific paper

The usual theory of planetesimal formation is untenable because
turbulence inhibits gravitational instability. However, turbulence can
actually concentrate chrondule-sized particles by factors up to a
million near stagnation points. The implications for accretion may be
profound.

Affiliated with

Also associated with

No associations

Rating

From chondrules to planetesimals: solids and turbulence in the Solar Nebula. 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 From chondrules to planetesimals: solids and turbulence in the Solar Nebula., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and From chondrules to planetesimals: solids and turbulence in the Solar Nebula. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1138463