The orbital dispersion of the macroscopic Taurid objects

Details The orbital dispersion of the macroscopic Taurid objects The orbital dispersion of the macroscopic Taurid objects

Jun 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996mnras.280..806s&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 280, Issue 3, pp. 806-822.

Astronomy and Astrophysics

Astronomy

10

Methods: Numerical, Celestial Mechanics, Stellar Dynamics, Comets: General, Minor Planets, Asteroids

Scientific paper

If the Taurid Complex asteroids (plus 2P/Encke) are derived from the fragmentation of a giant comet over the past 20-30 kyr, as we have suggested elsewhere, then we need to identify some mechanism which could cause the observed dispersion in semimajor axes (1.8<a<2.6 au), eccentricities (0.64<e<0.85), and longitudes of perihelion (100 deg

Affiliated with

Also associated with

No associations

Rating

The orbital dispersion of the macroscopic Taurid objects 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 orbital dispersion of the macroscopic Taurid objects, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The orbital dispersion of the macroscopic Taurid objects will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1301502