Difficulties of Chondrule Formation by Nebular Shock Waves

Details Difficulties of Chondrule Formation by Nebular Shock Waves Difficulties of Chondrule Formation by Nebular Shock Waves

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..341..893u&link_type=abstract

Chondrites and the Protoplanetary Disk, ASP Conference Series, Vol. 341, Proceedings of a workshop held 8-11 November 2004 in Ka

Astronomy and Astrophysics

Astronomy

2

Scientific paper

In this paper we investigate two constraints on chondrule formation by solar nebula shocks: the transport of FeS inclusions by internal flows in the molten silicate, and the formation of compound chondrules. A recent study has shown that if chondrules formed due to nebular shock waves, a high-speed (˜5 cm s-1) rotational flow occurs in chondrules during melting, which will greatly affect the final placement of FeS inclusions in the chondrules. Collision between chondrules while they are molten or partially molten, can cause them to stick and form compound chondrules, but only in a a suitable range of relative velocities. These features of chondrules place important constraints on the chondrule formation process.

Affiliated with

Also associated with

No associations

Rating

Difficulties of Chondrule Formation by Nebular Shock Waves 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 Difficulties of Chondrule Formation by Nebular Shock Waves, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Difficulties of Chondrule Formation by Nebular Shock Waves will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1033038