Regular ArticleOn the Inclination Distribution of the Jovian Irregular Satellites
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Analysis of motion in RTBP with variable mass based on Loglogistic distribution
2024, Results in PhysicsEarly impact chronology of the icy regular satellites of the outer solar system
2021, IcarusCitation Excerpt :Apart from Enceladus, all satellites have surface ages that are older than 4 Gyr using the chronology that we obtained from the Scattered Disc migration simulations. It is very likely that the irregular satellites of the planets were captured during mutual encounters (Nesvorný et al. 2007) and that they subsequently evolved collisionally (Bottke et al. 2010) and though the Kozai mechanism, which enables encounters with the regular satellites (Carruba et al. 2002; Nesvorný et al. 2003). However, such planetary encounters will also eject any pre-existing satellites, so that the last encounter will be the one that establishes the irregular satellite populations.
Evolution of MU69 from a binary planetesimal into contact by Kozai-Lidov oscillations and nebular drag
2021, IcarusCitation Excerpt :For highly inclined orbits, the Kozai-Lidov resonance can drive very high eccentricity. This mechanism has been invoked to explain why no irregular satellites have inclinations in the range 50°–140° (Nesvorný et al., 2003): such satellites would be driven by Kozai cycles either to pericenters that impact the planets (or massive inner moons), or to apocenters that lie outside the Hill sphere (Carruba et al., 2002). Thomas and Morbidelli (1996), applying it to a triple system of Sun-Jupiter-comet, showed that Kozai-Lidov oscillations can make cometary orbits become Sun-grazing.
Empirical stability boundary for hierarchical triples
2022, Publications of the Astronomical Society of AustraliaThe Lidov-Kozai resonance at different scales
2021, Proceedings of the International Astronomical Union