Fully analytical kinetic model of resonance dynamics in the Solar system

Details Fully analytical kinetic model of resonance dynamics in the Solar system Fully analytical kinetic model of resonance dynamics in the Solar system

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006pobeo..80..173c&link_type=abstract

Publications of the Astronomical Observatory of Belgrade, Vol. 80, p. 173-177

Astronomy and Astrophysics

Astronomy

Scientific paper

We propose a fractional kinetic equation to model the transport in eccentricity of objects in the mean motion resonances in the Elliptic Planar Restricted Three-Body Problem. Making use of the renormalization group formalism, we show how the fractional exponents and the diffusion coefficient can be estimated analytically, making use of the degeneracy of the problem. We apply our model to selected Mean Motion Resonances in the Solar System and explain some basic properties of transport in these resonances.

Affiliated with

Also associated with

No associations

Rating

Fully analytical kinetic model of resonance dynamics in the Solar system 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 Fully analytical kinetic model of resonance dynamics in the Solar system, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Fully analytical kinetic model of resonance dynamics in the Solar system will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-931985