Other
Scientific paper
May 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009rmxac..35q.286l&link_type=abstract
XII Latin American IAU Regional Meeting (Eds. G. Magris, G. Bruzual, & L. Carigi) Revista Mexicana de Astronomía y Astrofísica (
Other
Scientific paper
We have analyzed the dynamical behavior of objects located in a position 22 < a < 26 AU which corresponds to the mean motion resonances 3:2 and 2:3 with Neptune and Uranus respectively. Mostly of the studied objects migrate toward the external part of the Solar System, called Kuiper belt, a scattered disk in the a > 30 AU region. Some are ejected from the Solar System with e=∞. Of the test particles studied, less than 10% migrate toward the inner part, in some cases becoming Earth and Mars crossing. This fact may be a source of near-Earth objects (NEOs), as asteroids in the Main Belt lying near the 3:1 resonance with Jupiter. Many objects make numerous close approaches to Jupiter and Saturn. Other clones, a few, can reach the region a ˜ 500, e ˜ 0.78, i ˜ 15° (Sedna: a = 509 AU, e = 0.851, i = 11.9). This behavior of some clones occur when Neptune has a = 28 AU.
No associations
LandOfFree
Dynamical Evolution of Objects between 3:2 Resonance with Neptune and 2:3 Resonance with Uranus 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 Dynamical Evolution of Objects between 3:2 Resonance with Neptune and 2:3 Resonance with Uranus, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dynamical Evolution of Objects between 3:2 Resonance with Neptune and 2:3 Resonance with Uranus will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1111541