Titan’s obliquity as evidence of a subsurface ocean?

DOI10.1051/0004-6361/201116578zbMath1260.85002arXiv1104.2741OpenAlexW3102255640WikidataQ68679281 ScholiaQ68679281MaRDI QIDQ4905730

Marie Yseboodt, Tim Van Hoolst, Ö. Karatekin, Rose-Marie Baland

Publication date: 20 February 2013

Published in: Astronomy & Astrophysics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1104.2741

zbMATH Keywords

celestial mechanicsplanets and satellites: interiorsplanets and satellites: Titan

Mathematics Subject Classification ID

Celestial mechanics (70F15) Galactic and stellar dynamics (85A05) General questions in astronomy and astrophysics (85A04)

Related Items (4)

A symplectic mapping for the synchronous spin-orbit problem ⋮ Rotation of a rigid satellite with a fluid component: a new light onto Titan's obliquity ⋮ Cassini states of a rigid body with a liquid core ⋮ Coupling between the spin precession and polar motion of a synchronously rotating satellite: application to Titan

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