Enceladus's internal ocean and ice shell constrained from Cassini gravity, shape, and libration data-Reference-Cited by-同舟云学术

Enceladus's internal ocean and ice shell constrained from Cassini gravity, shape, and libration data

Published:2016-06-11 Issue:11 Volume:43 Page:5653-5660
ISSN:0094-8276
Container-title:Geophysical Research Letters
language:en
Short-container-title:Geophys. Res. Lett.

Author:

Čadek Ondřej¹,Tobie Gabriel²,Van Hoolst Tim³⁴,Massé Marion²,Choblet Gaël²,Lefèvre Axel²,Mitri Giuseppe²,Baland Rose-Marie³,Běhounková Marie¹,Bourgeois Olivier²,Trinh Anthony³

Affiliation:

1. Department of Geophysics, Faculty of Mathematics and Physics; Charles University in Prague; Prague 8 Czech Republic

2. Laboratoire de Planétologie et Géodynamique, UMR-CNRS; University of Nantes; Nantes France

3. Royal Observatory of Belgium; Brussels Belgium

4. Instituut voor Sterrenkunde; KU Leuven; Leuven Belgium

Funder

European Community's Seventh Framework Programme

Publisher

American Geophysical Union (AGU)

Subject

General Earth and Planetary Sciences,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1002/2016GL068634/fullpdf

Reference36 articles.

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2. Timing of water plume eruptions on Enceladus explained by interior viscosity structure;Běhounková;Nat. Geosci.,2015

3. Convection-driven compaction as a possible origin of Enceladus's long wavelength topography;Besserer;J. Geophys. Res. Planets,2013

4. Constraining the heat flux between Enceladus' tiger stripes: Numerical modeling of funiscular plains formation;Bland;Icarus,2015

5. Čadek , O. G. Choblet M. Běhounková G. Tobie T. Kozubek 2015 Effect of ice-shell thickness variations on the tidal deformation of Enceladus

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