Structural and tidal models of Titan and inferences on cryovolcanism

Author:

Sohl F.1,Solomonidou A.234,Wagner F. W.15,Coustenis A.2,Hussmann H.1,Schulze-Makuch D.67

Affiliation:

1. DLR; Institute of Planetary Research; Berlin Germany

2. LESIA, Observatoire de Paris, CNRS; UPMC University Paris 06, University Paris-Diderot-Meudon; Paris France

3. Department of Geology and Geoenvironment; National and Kapodistrian University of Athens; Athens Greece

4. Now at Jet Propulsion Laboratory; California Institute of Technology; Pasadena California USA

5. Westphalian Wilhelms-University; Institute for Planetology; Münster Germany

6. School of Earth and Environmental Sciences; Washington State University; Pullman Washington USA

7. Center for Astronomy and Astrophysics; Technical University of Berlin; Berlin Germany

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Reference115 articles.

1. Thermal and chemical evolution of the terrestrial magma ocean;Abe;Phys. Earth Planet. Inter.,1997

2. Titan's methane cycle;Atreya;Planet. Space Sci.,2006

3. Titan's obliquity as evidence of a subsurface ocean?;Baland;Astron. Astrophys.,2011

4. Cassini observations of flow-like features in western Tui Regio, Titan;Barnes;Geophys. Res. Lett.,2006

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