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
- 1 December 2011
- journal article
- Published by Elsevier BV in Icarus
- Vol. 216 (2), 535-550
- https://doi.org/10.1016/j.icarus.2011.09.017
Abstract
No abstract availableKeywords
Funding Information
- Institut Universitaire de France (IUF)
- EMERGENCE UPMC (EME0911)
- US Government
- French Programme National de Planétologie (PNP)
This publication has 55 references indexed in Scilit:
- Dione’s spectral and geological propertiesIcarus, 2009
- Constraints on gas giant satellite formation from the interior states of partially differentiated satellitesIcarus, 2008
- A belt of moonlets in Saturn’s A ringNature, 2007
- Shapes of the saturnian icy satellites and their significanceIcarus, 2007
- 100-metre-diameter moonlets in Saturn's A ring from observations of 'propeller' structuresNature, 2006
- Radar imaging of Saturn's ringsIcarus, 2005
- Viscosity in a Dense Planetary Ring with Self-Gravitating ParticlesIcarus, 2001
- Accretion in the Roche Zone: Coexistence of Rings and RingmoonsIcarus, 1995
- Contribution of tidal dissipation to lunar thermal historyIcarus, 1978
- Love numbers of the giant planetsIcarus, 1977