Titan's obliquity as evidence of a subsurface ocean?

Astronomy and Astrophysics

Volumn 530, Issue , 2011, Pages

  Baland, R M ^a,b   Van Hoolst, T ^a   Yseboodt, M ^a   Karatekin, O ^a  

^a ROYAL OBSERVATORY OF BELGIUM   (Belgium)

^b UNIVERSITÉ CATHOLIQUE DE LOUVAIN   (Belgium)

Author keywords

celestial mechanics; planets and satellites: individual: Titan; planets and satellites: interiors

Indexed keywords

CASSINI; CASSINI SPACECRAFT; CELESTIAL MECHANICS; ICE SHELLS; LIQUID WATER; MOMENT OF INERTIA; NEW MODEL; PLANETS AND SATELLITES: INDIVIDUAL: TITAN; PLANETS AND SATELLITES: INTERIORS; RADAR OBSERVATIONS; ROTATION AXIS; ROTATION STATE; STATE MODELS; SUB-SURFACE OCEAN;

ASTROPHYSICS; MECHANICS; PLANETS; SATELLITES;

ROTATION;

EID: 79957615516     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201116578     Document Type: Article

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