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Saturn’s Icy Moon Rhea: A Prediction for its Bulk Chemical Composition and Physical Structure at the Time of the Cassini Spacecraft First Flyby

Andrew J. R. Prentice A
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A School of Mathematical Sciences, Monash University, Melbourne VIC 3800, Australia. Email: andrew.prentice@sci.monash.edu.au

Publications of the Astronomical Society of Australia 23(1) 1-11 https://doi.org/10.1071/AS05041
Submitted: 30 November 2005  Accepted: 31 January 2006   Published: 29 March 2006



7 articles found in Crossref database.

Origin and chemical composition of the inner solar system
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Geochimica et Cosmochimica Acta. 2006 70(18). p.A504
Spectroscopic classification of icy satellites of Saturn II: Identification of terrain units on Rhea
Scipioni F., Tosi F., Stephan K., Filacchione G., Ciarniello M., Capaccioni F., Cerroni P.
Icarus. 2014 234 p.1
Thermal history and large scale differentiation of the Saturn’s satellite Rhea
Czechowski Leszek
Acta Geophysica. 2012 60(4). p.1192
Treatise on Geophysics (2007)
Hussmann H., Sotin C., Lunine J.I.
Treatise on Geophysics (2015)
Hussmann H., Sotin C., Lunine J.I.
Early Thermal History of Rhea: The Role of Serpentinization and Liquid State Convection
Czechowski Leszek, Łosiak Anna
Acta Geophysica. 2016 64(6). p.2677
Cassini at Saturn (2007)
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