An interesting difference in the distributions of the average motions of S- and C-asteroids

Details An interesting difference in the distributions of the average motions of S- and C-asteroids An interesting difference in the distributions of the average motions of S- and C-asteroids

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982avest..16...93s&link_type=abstract

(Astronomicheskii Vestnik, vol. 16, Apr.-June 1982, p. 93-99.) Solar System Research, vol. 16, no. 2, Oct. 1982, p. 69-74. Tran

Astronomy and Astrophysics

Astronomy

Asteroids, Protoplanets, Solar Orbits, Solar System, Planetary Evolution, Statistical Distributions, Stellar Magnitude

Scientific paper

The problem of the origin of asteroids with diameters greater than 84 km (group S) and greater than 150 km (group C) is discussed. C-asteroids are located in regions where the accumulation of material from the protoplanetary nebula was most effective, and are bodies which formed within the asteroid belt itself. It is proposed that it is possible that some S-type asteroids were formed in various regions of the Solar System with a subsequent transformation of their orbits into orbits characteristic of minor planets.

Affiliated with

Also associated with

No associations

Rating

An interesting difference in the distributions of the average motions of S- and C-asteroids 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 An interesting difference in the distributions of the average motions of S- and C-asteroids, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and An interesting difference in the distributions of the average motions of S- and C-asteroids will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1029474