Planet formation: statistics of spin rates and obliquities of extrasolar planets

We develop a simple model of planetary formation, focusing our attention on those planets with masses less than 10 M⊕ and studying particularly the primordial spin parameters of planets resulting from the accretion of planetesimals and produced by the collisions between the embryos. As initial condi...

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Detalles Bibliográficos
Autores principales:	Miguel, Yamila, Brunini, Adrián
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2010
Materias:	Ciencias Astronómicas Planets satellites formation
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/82511
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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