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Tides on Titan

Sohl, F. and Solomonidou, A. and Wagner, F.W. and Coustenis, A. and Hussmann, H. and Schulze-Makuch, D. (2013) Tides on Titan. 10th Annual Meeting Asia Oceania Geosciences Society (AOGS), 2013-06-24 - 2013-06-28, Brisbane, Australia.

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Abstract

In spite of its ice-rich bulk composition, Titan, Saturn's largest satellite, has many similarities to the early Earth, particularly in terms of atmospheric composition and organic chemistry. Titan is subject to time-variable radial and librational tides exerted by Saturn on the time-scale of its orbital period. The satellite's tidal response depends on its interior structure, thermal state, tidally effective rheology, and the frequency of tidal forcing. The tidally induced internal redistribution of mass results in variations of surface gravity, tilt, stress and strain, which could play a major role in triggering processes that are visible in Titan's geological surface record. We subdivide Titan's interior into four chemically homogeneous reservoirs and construct structural models that are required to satisfy the mean density, polar moment-of-inertia factor, and tidal potential Love number k2 as derived from Cassini gravity field data. It appears that outer ice shell thickness and the radial extent of the subsurface water-ammonia ocean are closely related to each other. Using corresponding linear combinations of the body tide Love-Shida numbers, we then calculate the expected amplitude patterns of tensile and maximum shear stresses at Titan's surface in response to the tidal forcing. We find peak-to-peak amplitudes of tide-induced surface displacement, tilt variation, and tidal stresses on the order of up to a few tens of meters, several arc seconds, and a few tens of kPa, respectively. Owing to the greater shell flexibility in the presence of an ocean, radial surface displacement is maximal over a tidal cycle, whereas tilt variation relative to the direction of gravity is minimal. The global pattern of maximum tidal distortion is broadly consistent with the zonal distribution of cryovolcanic candidate areas and lakes at high latitudes that may provide possible pathways for the release of methane in the satellite's atmosphere and are of great importance for basic conditions of habitability.

Item URL in elib:https://elib.dlr.de/83228/
Document Type:Conference or Workshop Item (Speech)
Title:Tides on Titan
Authors:
AuthorsInstitution or Email of AuthorsAuthor's ORCID iDORCID Put Code
Sohl, F.frank.sohl (at) dlr.dehttps://orcid.org/0000-0003-0355-1556UNSPECIFIED
Solomonidou, A.National and Kapodistrian University of Athens, Department of Geology and Geoenvironment, Athens, GreeceUNSPECIFIEDUNSPECIFIED
Wagner, F.W.frank.wagner (at) dlr.deUNSPECIFIEDUNSPECIFIED
Coustenis, A.Laboratoire d’Etudes Spatiales et d’Instrumentation en Astrophysique (LESIA), Observatoire de Paris-Meudon, 92195 Meudon Cedex, FranceUNSPECIFIEDUNSPECIFIED
Hussmann, H.hauke.hussmann (at) dlr.deUNSPECIFIEDUNSPECIFIED
Schulze-Makuch, D.School of Earth and Environmental Sciences, Washington State University, Pullman, USAUNSPECIFIEDUNSPECIFIED
Date:June 2013
Refereed publication:No
Open Access:No
Gold Open Access:No
In SCOPUS:No
In ISI Web of Science:No
Status:Published
Keywords:Titan, interior structure, solid body tides, tidal potential, tidal deformation, cryovolcanism, habitability.
Event Title:10th Annual Meeting Asia Oceania Geosciences Society (AOGS)
Event Location:Brisbane, Australia
Event Type:international Conference
Event Start Date:24 June 2013
Event End Date:28 June 2013
Organizer:AOGS
HGF - Research field:Aeronautics, Space and Transport
HGF - Program:Space
HGF - Program Themes:Space Exploration
DLR - Research area:Raumfahrt
DLR - Program:R EW - Space Exploration
DLR - Research theme (Project):R - Exploration of the Solar System
Location: Berlin-Adlershof
Institutes and Institutions:Institute of Planetary Research > Planetary Physics
Deposited By: Sohl, Dr. Frank
Deposited On:19 Sep 2013 11:59
Last Modified:24 Apr 2024 19:49

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