Formation of Jupiter using opacities based on detailed grain physics

Icarus

Volumn 209, Issue 2, 2010, Pages 616-624

  Movshovitz, Naor ^a,b   Bodenheimer, Peter ^c   Podolak, Morris ^b   Lissauer, Jack J ^d  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b TEL AVIV UNIVERSITY   (Israel)

^c University of California at Santa Cruz   (United States)

^d NASA AMES RESEARCH CENTER   (United States)

Author keywords

Accretion; Jovian planets; Jupiter, Interior; Planetary formation

Indexed keywords

EID: 77956274225     PISSN: 00191035     EISSN: 10902643     Source Type: Journal    
DOI: 10.1016/j.icarus.2010.06.009     Document Type: Article

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