A discussion of the solution for the motion of Pluto

Details A discussion of the solution for the motion of Pluto A discussion of the solution for the motion of Pluto

May 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978cemec..17..405n&link_type=abstract

Celestial Mechanics, vol. 17, May 1978, p. 405-421.

Computer Science

6

Orbit Calculation, Phase-Space Integral, Pluto (Planet), Uranus (Planet), Eccentricity, Librational Motion, Orbit Perturbation, Resonance, Motion, Pluto, Resonance, Planets, Uranus, Neptune, Eccentricity, Inclination, Perihelion, Perturbations

Scientific paper

The semianalytical solution for Pluto given by Nacozy and Diehl (1978) is compared with the numerical solution obtained by Williams and Benson (1971). The effect of the Pluto-Uranus near resonance is discussed along with how it can be incorporated into the solution. Details are given on the calculation of certain quantities in the long-term solution. A calculation of librational periods of the perihelion, eccentricity, and inclination is performed. The calculation is based on the method of Giacaglia and Hori (1968).

Affiliated with

Also associated with

No associations

Rating

A discussion of the solution for the motion of Pluto 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 A discussion of the solution for the motion of Pluto, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A discussion of the solution for the motion of Pluto will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1296245