Stardust findings favor not only the planetary origin of comets but the underlying close-binary cosmogony of the Solar System as well
- Author
- DROBYSHEVSKI, Edward M1
[1] loffe Physical-Technical Institute, Russian Academy of Sciences, 194021 St. Petersburg, Russian Federation - Source
Icarus (New York, NY). 2008, Vol 197, Num 1, pp 203-210, 8 p ; ref : 3/4 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
- Russian
- Author keyword
- Comet Tempel-1 Comet Wild-2 Comets Origin Solar System Trans-neptunian planets origin
- Keyword (fr)
- Binaire serrée Comète courte période Comète longue période Condensation Cosmogonie Dynamique gaz Evolution dynamique Glace Haute température Jet Planète Jupiter Planète Neptune Rayonnement solaire Satellite Jupiter Satellite galiléen Soleil Sublimation Système multiple Système solaire Système stellaire Planète naine
- Keyword (en)
- Close binary stars Short period comet Long period comet Vapor condensation Cosmogony Gas dynamics Dynamical evolution Ice High temperature Jets Jupiter planet Neptune planet Solar radiation Jupiter satellite Galilean satellite Sun Sublimation Multiple system Solar system Stellar systems Dwarf planet
- Keyword (es)
- Cometa corto período Cometa largo período Cosmogonía Evolución dinámica Alta temperatura Satélite Jupiter Satélite galileano Sistema múltiple Planeta enana
- 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
- 20679965
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.2008.03.025 
https://dx.doi.org/10.1016/j.icarus.2008.03.025
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