A study of the high-inclination population in the Kuiper belt - II. The Twotinos
arXiv:1402.5924 · doi:10.1093/mnras/stu1239
Abstract
As the second part of our study, in this paper we proceed to explore the dynamics of the high-inclination Twotinos in the 1:2 Neptune mean motion resonance (NMMR). Depending on the inclination , we show the existence of two critical eccentricities and , which are lower limits of the eccentricity for the resonant angle to exhibit libration and asymmetric libration, respectively. Accordingly, we have determined the libration centres for inclined orbits, which are strongly dependent on . With initial on a fine grid of , the stability of orbits in the 1:2 NMMR is probed by 4-Gyr integrations. It is shown that symmetric librators are totally unstable for ; while stable asymmetric librators exist for up to . We further investigate the 1:2 NMMR capture and retention of planetesimals with initial inclinations in the planet migration model using a time-scale of yr. We find that: (1) the capture efficiency of the 1:2 NMMR decreases drastically with the increase of , and it goes to 0 when ; (2) the probability of discovering Twotinos with , beyond observed values, is roughly estimated to be per cent; (3) more particles are captured into the leading rather than the trailing asymmetric resonance for , but this number difference appears to be the opposite at and is continuously varying for even larger ; (4) captured Twotinos residing in the trailing resonance or having are practically outside the Kozai mechanism, like currently observed samples.
13 pages, 10 figures, Accepted by MNRAS. Comments welcome!
References in corpus (3)
Cited by in corpus (11)
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