Dynamical evolution of comets from high-eccentricity trans-Neptunian orbits to near-Earth space

Details Dynamical evolution of comets from high-eccentricity trans-Neptunian orbits to near-Earth space Dynamical evolution of comets from high-eccentricity trans-Neptunian orbits to near-Earth space

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005dpps.conf..323e&link_type=abstract

Dynamics of Populations of Planetary Systems, Proceedings of IAU Colloquium #197, held 31 August - 4 Spetember, 2004 in Belgrade

Physics

1

Celestial Mechanics, Comets: General, Kuiper Belt, Oort Cloud.

Scientific paper

The contribution of high-eccentricity trans-Neptunian objects to the observed populations of both short-period and long-period comets is estimated. About 10(10) objects with a radius R>0.7 km in orbits with perihelion distances 280.7 km.

Affiliated with

Also associated with

No associations

Rating

Dynamical evolution of comets from high-eccentricity trans-Neptunian orbits to near-Earth space 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 Dynamical evolution of comets from high-eccentricity trans-Neptunian orbits to near-Earth space, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamical evolution of comets from high-eccentricity trans-Neptunian orbits to near-Earth space will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1358171