Trojan asteroids - Relations between dynamical parameters

Details Trojan asteroids - Relations between dynamical parameters Trojan asteroids - Relations between dynamical parameters

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...175..299s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 175, no. 1-2, March 1987, p. 299-302.

Computer Science

Numerical Analysis

17

Asteroids, Long Term Effects, Orbital Elements, Trojan Orbits, Inclination, Librational Motion, Magnitude, Numerical Analysis, Periodic Variations, Secular Variations, Asteroids, Trojan Asteroids, Dynamics, Paramters, Astronomy, Libration, Physical Properties, Period, Eccentricity, Inclination, Orbits, Data, Distribution, Absolute Magnitude, Brightness

Scientific paper

Previously obtained results for three proper elements of the numbered Trojan asteroids are used to study both the distribution of these qualities and their relationships to other dynamical parameters. Attention is given to the relation of B(1,0), which is the absolute blue magnitude, to the proper inclination. The results obtained indicate the usefulness of inclination distribution studies in the separation of the material into classes, with respect to a suitable parameter of brightness.

Affiliated with

Also associated with

No associations

Rating

Trojan asteroids - Relations between dynamical parameters 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 Trojan asteroids - Relations between dynamical parameters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Trojan asteroids - Relations between dynamical parameters will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1451660