Implications from the motion of outer belt asteroids

Details Implications from the motion of outer belt asteroids Implications from the motion of outer belt asteroids

Dec 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979icar...40..329f&link_type=abstract

Icarus, vol. 40, Dec. 1979, p. 329-334.

Other

3

Asteroids, Orbit Perturbation, Particle Motion, Eccentricity, Gravitational Effects, Orbital Mechanics, Spatial Distribution, Asteroids, Asteroid Belt, Motion, Distribution, Perturbations, Planets, Density, Dynamics, Orbits, Eccentricity, Observations, Librations, Conjunction, Resonance, Distance, Parameters, Absolute Magnitudes

Scientific paper

A principal feature of the asteroidal distribution is the rapid truncation of its population outward from approximately 3.4 AU. This paper presents further evidence, based on the motion and distribution of certain minor planets with large semimajor axes, that this truncation cannot be strictly the result of gravitational perturbations of the major planets even acting over times of approximately one-billion years. The motion of other outer asteroids sets a probable upper limit of 0.081 on Jupiter's eccentricity.

Affiliated with

Also associated with

No associations

Rating

Implications from the motion of outer belt 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 Implications from the motion of outer belt asteroids, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Implications from the motion of outer belt asteroids will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1447333