Evolution of orbits at the 2:3 resonance with Neptune

Details Evolution of orbits at the 2:3 resonance with Neptune Evolution of orbits at the 2:3 resonance with Neptune

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..621i&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 621.

Physics

Evolution (Development), Many Body Problem, Resonance, Neptune (Planet), Planetary Orbits, Eccentricity, Libration

Scientific paper

In the present investigation of the evolution of orbits at the 2:3 resonance with Neptune, the six-body problem posed by the sun, four giant planets and a test body is integrated using the symplectic 'swift integrator' of Levinson and Duncan (1994) for an integration span of 20 years. It is found that even variations in initial orientations and initial positions in orbit can cause large vriations in the dependencies of eccentricity, inclination, and semimajor axis on time.

Affiliated with

Also associated with

No associations

Rating

Evolution of orbits at the 2:3 resonance with Neptune 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 Evolution of orbits at the 2:3 resonance with Neptune, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evolution of orbits at the 2:3 resonance with Neptune will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-872179