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A POSSIBLE CARBON-RICH INTERIOR IN SUPER-EARTH 55 Cancri e

Author
MADHUSUDHAN, Nikku1 ; LEE, Kanani K. M2 ; MOUSIS, Olivier3 4
[1] Department of Physics and Department of Astronomy, Yale University, New Haven, CT 06511, United States
[2] Department of Geology and Geophysics, Yale University, New Haven, CT 06511, United States
[3] Universite de Franche-Comté, Institut UTINAM, CNRS/INSU, UMR 6213, Observatoire des Sciences de l'Univers THETA, CP 1615, 25010 Besançon, France
[4] Universite de Toulouse, UPS-OMP, CNRS-INSU, IRAP, 14 Avenue Edouard Belin, 31400 Toulouse, France
Source

The Astrophysical journal. 2012, Vol 759, Num 2 ; 759L40.1-759L40.5 ; 2 ; ref : 1/4 p

CODEN
ASJOAB
ISSN
0004-637X
Scientific domain
Astronomy earth cosmic environment
Publisher
IOP, Bristol
Publication country
United Kingdom
Document type
Article
Language
English
Author keyword
planetary systems planets and satellites: general planets and satellites: individual (55 Cancri e)
Keyword (fr)
Abondance stellaire Abondance élément Atmosphère planétaire Mesure masse Modèle Nébuleuse proto planétaire Planète extrasolaire Planète terrestre Structure interne planétaire Système planétaire Système solaire
Keyword (en)
Stellar abundance Element abundance Planetary atmospheres Mass measurement Models Proto planetary nebula Extrasolar planets Terrestrial planet Planetary interiors Planetary system Solar system
Keyword (es)
Abundancia estelar Modelo Nebulosa proto planetaria Planeta terrestre Sistema planetario
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
26584651

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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