A comparison between families obtained from different proper elements

Details A comparison between families obtained from different proper elements A comparison between families obtained from different proper elements

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992acm..proc..675z&link_type=abstract

In Lunar and Planetary Inst., Asteroids, Comets, Meteors 1991 p 675-678 (SEE N93-19113 06-90)

Statistics

Computation

4

Asteroid Belts, Asteroids, Classifications, Physical Properties, Collisions, Impact, Perturbation Theory

Scientific paper

Using the hierarchical method of family identification developed by Zappala et al., the results coming from the data set of proper elements computed by Williams (about 2100 numbered + about 1200 PLS 2 asteroids) and by Milani and Knezevic (5.7 version, about 4200 asteroids) are compared. Apart from some expected discrepancies due to the different data sets and/or low accuracy of proper elements computed in peculiar dynamical zones, a good agreement was found in several cases. It follows that these high reliability families represent a sample which can be considered independent on the methods used for their proper elements computation. Therefore, they should be considered as the best candidates for detailed physical studies.

Affiliated with

Also associated with

No associations

Rating

A comparison between families obtained from different proper elements 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 A comparison between families obtained from different proper elements, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A comparison between families obtained from different proper elements will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1112900