Tidal constraints on the interior of Venus-Reference-Cited by-同舟云学术

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Tidal constraints on the interior of Venus

Published:2017-06 Issue:6 Volume:122 Page:1338-1352
ISSN:2169-9097
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:J. Geophys. Res. Planets

Author:

Dumoulin C.¹^ORCID,Tobie G.¹^ORCID,Verhoeven O.¹^ORCID,Rosenblatt P.²,Rambaux N.³^ORCID

Affiliation:

1. Laboratoire de Planétologie et Géodynamique, UMR-CNRS 6112; Université de Nantes; Nantes France

2. Royal Observatory of Brussels; Uccle Belgium

3. Institut de Mécanique Céleste et Calcul des Ephémérides; Université Pierre et Marie Curie; Paris France

Funder

Centre National d’Etudes Spatiales

Belgian PRODEX program managed by the European Space Agency

Région Pays de la Loire, project GeoPlaNet

Publisher

American Geophysical Union (AGU)

Subject

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

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1002/2016JE005249/fullpdf

Reference65 articles.

1. Venus' internal structure, temperature and core composition;Aitta;Icarus,2012

2. Thermal evolution of venus;Arkani-Hamed;Phys. Earth Planet. Int.,1984

3. Simulating the thermochemical magmatic and tectonic evolution of Venus's mantle and lithosphere: Two-dimensional models;Armann;J. Geophys. Res.,2012

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3. Development of a new more precise algorithm for computing tidal Love numbers;Доклады Российской академии наук. Физика, технические науки;2024-08-10

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