Accretion of Saturn’s mid-sized moons during the viscous spreading of young massive rings: Solving the paradox of silicate-poor rings versus silicate-rich moons-Reference-Cited by-同舟云学术

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Accretion of Saturn’s mid-sized moons during the viscous spreading of young massive rings: Solving the paradox of silicate-poor rings versus silicate-rich moons

Published:2011-12 Issue:2 Volume:216 Page:535-550
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Charnoz Sébastien,Crida Aurélien,Castillo-Rogez Julie C.,Lainey Valery,Dones Luke,Karatekin Özgür,Tobie Gabriel,Mathis Stephane,Le Poncin-Lafitte Christophe,Salmon Julien

Funder

Institut Universitaire de France (IUF)

EMERGENCE UPMC

US Government

French Programme National de Planétologie (PNP)

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference70 articles.

1. Constraints on gas giant satellite formation from the interior states of partially differentiated satellites;Barr;Icarus,2008

2. Simulation of a late lunar-forming impact;Canup;Icarus,2004

3. Origin of Saturn’s rings and inner moons by mass removal from a lost Titan-sized satellites;Canup;Nature,2010

4. Accretion in the Roche zone: Coexistence of rings and ring moons;Canup;Icarus,1995

5. A common mass scaling for satellite systems of gaseous planets;Canup;Nature,2006

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