A proof that tidal heating in a synchronous rotation is always larger than in an asymptotic nonsynchronous rotation state
- Author
- LEVRARD, B1 2
[1] Astronomie et Systèmes Dynamiques, IMCCE-CNRS UMR 8028, 77 Avenue Denfert-Rochereau, 75014 Paris, France
[2] Université de Lyon 1, Centre de Recherche Astrophysique de Lyon, Ecole Normale Supérieure de Lyon, CNRS, 46 allée d'Italie, 69364 Lyon, France - Source
Icarus (New York, NY). 2008, Vol 193, Num 2, pp 641-643, 3 p ; ref : 1/4 p
- CODEN
- ICRSA5
- ISSN
- 0019-1035
- Scientific domain
- Astronomy earth cosmic environment; Geology
- Publisher
- Elsevier, San Diego, CA
- Publication country
- United States
- Document type
- Article
- Language
- English
- Author keyword
- Extrasolar dynamics; Tides planets; Extrasolar planets; Satellites solid body
- Keyword (fr)
- Corps tournant Dynamique Excentricité Obliquité Orbite Planète extrasolaire Résonance Système solaire
- Keyword (en)
- Rotating bodies Dynamics Eccentricity Obliqueness Orbits Extrasolar planets Resonance Solar system
- Keyword (es)
- Oblicuidad
- Classification
- Pascal
- 001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03B Solar system
- Discipline
- Astronomy
- Origin
- Inist-CNRS
- Database
- PASCAL
- INIST identifier
- 20118853
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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DOI
10.1016/j.icarus.2007.10.003 
https://dx.doi.org/10.1016/j.icarus.2007.10.003
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