Future destabilisation of Titan as a result of Saturn’s tilting
| Autor: | Melaine Saillenfest, Giacomo Lari |
|---|---|
| Přispěvatelé: | Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Lille-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Dipartimento di Matematica [Pisa], University of Pisa - Università di Pisa |
| Jazyk: | angličtina |
| Rok vydání: | 2021 |
| Předmět: |
010504 meteorology & atmospheric sciences
planets and satellites: dynamical evolution and stability FOS: Physical sciences Context (language use) 01 natural sciences symbols.namesake Planet Saturn 0103 physical sciences planets and satellites: formation 010303 astronomy & astrophysics 0105 earth and related environmental sciences Earth and Planetary Astrophysics (astro-ph.EP) Physics Uranus Astronomy Astronomy and Astrophysics Radius celestial mechanics Exoplanet 13. Climate action Space and Planetary Science Physics::Space Physics Precession symbols Astrophysics::Earth and Planetary Astrophysics Titan (rocket family) [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] Astrophysics - Earth and Planetary Astrophysics |
| Zdroj: | Astronomy and Astrophysics-A&A Astronomy and Astrophysics-A&A, EDP Sciences, 2021, 654, pp.A83. ⟨10.1051/0004-6361/202141467⟩ Astronomy and Astrophysics-A&A, 2021, 654, pp.A83. ⟨10.1051/0004-6361/202141467⟩ |
| ISSN: | 0004-6361 |
| DOI: | 10.1051/0004-6361/202141467⟩ |
| Popis: | Context: As a result of Titan's migration and Saturn's probable capture in secular spin-orbit resonance, recent works show that Saturn's obliquity could be steadily increasing today and may reach large values in the next billions of years. Satellites around high-obliquity planets are known to be unstable near their Laplace radius, but the approximations used so far are invalidated in this regime. Aims: We aim to investigate the behaviour of a planet and its satellite when the satellite crosses its Laplace radius while the planet is locked in secular spin-orbit resonance. Methods: We expand on previous works and revisit the concept of Laplace surface. We use it to build an averaged analytical model that couples the planetary spin-axis and satellite dynamics. Results: We show that the dynamics is organised around a critical point, S1, at which the phase-space structure is singular, located at 90{\deg} obliquity and near the Laplace radius. If the spin-axis precession rate of the planet is maintained fixed by a resonance while the satellite migrates outwards or inwards, then S1 acts as an attractor towards which the system is forced to evolve. When it reaches the vicinity of S1, the entire system breaks down, either because the planet is expelled from the resonance or because the satellite is ejected or collides into the planet. Conclusions: Provided that Titan's migration is not halted in the future, Titan and Saturn may reach instability between a few gigayears and several tens of gigayears from now, depending on Titan's migration rate. The evolution would destabilise Titan and drive Saturn towards an obliquity of 90{\deg}. Our findings may have important consequences for Uranus. They also provide a straightforward mechanism for producing transiting exoplanets with a face-on massive ring, a configuration that is often put forward to explain some super-puff exoplanets. Comment: Accepted for publication in Astronomy and Astrophysics |
| Databáze: | OpenAIRE |
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