Complexes of small bodies of the Solar system.

Details Complexes of small bodies of the Solar system. Complexes of small bodies of the Solar system.

Dec 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994avest..28...70s&link_type=abstract

Astronomicheskii Vestnik, Tom 28, No. 6, p. 70 - 82

Other

Solar System: Families, Solar System: Comets, Solar System: Meteor Streams, Comets: Meteor Streams

Scientific paper

A new criterion for identification of the Solar system small bodies related genetically is introduced. For that purpose two first integrals of the limited circular three-body problem and the Tisserand invariant were used. Unlike osculating orbital elements the quasistationary parameters μ, ν and the Tisserand invariant Ti change slightly during long time intervals, and, in consequence, they may serve as a kind of memory about the origin of small bodies and their complexes. In other words, similarity of this parameters may serve as a criterion for ascertaining the genetic relations of small bodies in the Solar system. By means of this criterion seven cometary-meteor complexes were identified, each of them consists of some meteor swarms and of their possible parent bodies.

Affiliated with

Also associated with

No associations

Rating

Complexes of small bodies of the Solar system. 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 Complexes of small bodies of the Solar system., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Complexes of small bodies of the Solar system. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1327235