The unity of small bodies of the solar system

Details The unity of small bodies of the solar system The unity of small bodies of the solar system

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987prir........36t&link_type=abstract

Priroda (ISSN 0032-874X), Sept. 1987, p. 36-39. In Russian.

Computer Science

Chemical Composition, Meteoroids, Solar System, Chondrites, Orbital Elements

Scientific paper

It is noted that a mirror symmetry of the Tisserand-constant distribution characterizes the two main populations of small bodies in the solar system: short-period comets and asteroids. This phenomenon, together with sufficiently close values of the Tisserand constant for the majority of short-period comets and asteroids, indicates that these populations may have a common origin and nature.

Affiliated with

Also associated with

No associations

Rating

The unity 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 The unity 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 The unity of small bodies of the solar system will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1677674