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Numerical experiments with rubble piles: equilibrium shapes and spins

Author
RICHARDSON, Derek C1 ; ELANKUMARAN, Pradeep1 ; SANDERSON, Robyn E1
[1] Department of Astronomy, Computer and Space Sciences Building, Stadium Drive, University of Maryland, College Park, MD 20740-2421, United States
Source

Icarus (New York, NY). 2005, Vol 173, Num 2, pp 349-361, 13 p ; ref : 43 ref

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 Planetesimals Rotational dynamics Satellites of Jupiter Solid body tides
Keyword (fr)
Amalthea Astéroïde Continuum Dynamique Etude cas Fluide parfait Forme sphérique Forme équilibre Matériau granulaire Modèle Particule sphérique Planète Saturne Planétésimales Propriété dynamique Satellite Jupiter Simulation numérique Structure interne Système autogravitant Système solaire
Keyword (en)
Amalthea Asteroids Continuum Dynamics Case study Perfect fluid Spherical shape Equilibrium shape Granular materials Models Spherical particle Saturn planet Planetesimals Dynamic properties Jupiter satellite Digital simulation Internal structure Self-gravitating systems Solar system
Keyword (es)
Continuo Estudio caso Fluido perfecto Forma esférica Forma equilibrio Modelo Partícula esférica Propiedad dinámica Satélite Jupiter Estructura interna
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
16598547

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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