The Planetesimal Bow Shock Model for Chondrule Formation: Sizes of Highly Eccentric Planetesimals and Initial Simulations for a Radially Migrating Jupiter

Details The Planetesimal Bow Shock Model for Chondrule Formation: Sizes of Highly Eccentric Planetesimals and Initial Simulations for a Radially Migrating Jupiter The Planetesimal Bow Shock Model for Chondrule Formation: Sizes of Highly Eccentric Planetesimals and Initial Simulations for a Radially Migrating Jupiter

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2110h&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2110

Physics

1

Scientific paper

Improved simulations of planetesimal orbital evolution in the presence
of jovian resonances are reported to better evaluate the conditions
under which chondrules may have formed in bow shocks of highly eccentric
planetesimals.

Affiliated with

Also associated with

No associations

Rating

The Planetesimal Bow Shock Model for Chondrule Formation: Sizes of Highly Eccentric Planetesimals and Initial Simulations for a Radially Migrating Jupiter 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 The Planetesimal Bow Shock Model for Chondrule Formation: Sizes of Highly Eccentric Planetesimals and Initial Simulations for a Radially Migrating Jupiter, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Planetesimal Bow Shock Model for Chondrule Formation: Sizes of Highly Eccentric Planetesimals and Initial Simulations for a Radially Migrating Jupiter will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1041134