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A steady-state model of NEA binaries formed by tidal disruption of gravitational aggregates

Author
WALSH, Kevin J1 ; RICHARDSON, Derek C1
[1] Department of Astronomy, University of Maryland, College Park, MD 20742-2421, United States
Source

Icarus (New York, NY). 2008, Vol 193, Num 2, pp 553-566, 14 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
English
Author keyword
Asteroids dynamics; Satellites of asteroids
Keyword (fr)
Action marée Astéroïde Ceinture astéroïdale Distribution courant Durée vie Dynamique Modèle Mécanisme formation Méthode Monte Carlo Probabilité Propriété physique Système solaire
Keyword (en)
Tide effect Asteroids Asteroid belt Current distribution Lifetime Dynamics Models Formation mechanism Monte Carlo methods Probability Physical properties Solar system
Keyword (es)
Acción marea Cintura asteroidal Modelo Mecanismo formacion
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
20118845

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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