Planetary migration in a planetesimal disk: Why did Neptune stop at 30 AU?

Icarus

Volumn 170, Issue 2, 2004, Pages 492-507

  Gomes, Rodney S ^a   Morbidelli, Alessandro ^b   Levison, Harold F ^c  

^a MCT   (Brazil)

^b UNIVERSITÉ CÔTE D'AZUR   (France)

^c SOUTHWEST RESEARCH INSTITUTE   (United States)

Author keywords

Kuiper belt; Resonance; Solar System formation

Indexed keywords

EID: 3342972114     PISSN: 00191035     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.icarus.2004.03.011     Document Type: Article

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