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Gravity Field, Shape, and Moment of Inertia of Titan
DOI: 10.1126/science.1182583 Bibcode: 2010Sci...327.1367I

Stevenson, David J.; Iess, Luciano; Jacobson, Robert A. +5 more

Precise radio tracking of the spacecraft Cassini has provided a determination of Titan’s mass and gravity harmonics to degree 3. The quadrupole field is consistent with a hydrostatically relaxed body shaped by tidal and rotational effects. The inferred moment of inertia factor is about 0.34, implying incomplete differentiation, either in the sense…

2010 Science
Cassini 171
Cassini Finds an Oxygen-Carbon Dioxide Atmosphere at Saturn’s Icy Moon Rhea
DOI: 10.1126/science.1198366 Bibcode: 2010Sci...330.1813T

Coates, A. J.; Tokar, R. L.; Jones, G. H. +10 more

The flyby measurements of the Cassini spacecraft at Saturn’s moon Rhea reveal a tenuous oxygen (O2)-carbon dioxide (CO2) atmosphere. The atmosphere appears to be sustained by chemical decomposition of the surface water ice under irradiation from Saturn’s magnetospheric plasma. This in situ detection of an oxidizing atmosphere…

2010 Science
Cassini 104
An Evolving View of Saturn’s Dynamic Rings
DOI: 10.1126/science.1179118 Bibcode: 2010Sci...327.1470C

Clark, R. N.; Nicholson, P. D.; Kempf, S. +20 more

We review our understanding of Saturn’s rings after nearly 6 years of observations by the Cassini spacecraft. Saturn’s rings are composed mostly of water ice but also contain an undetermined reddish contaminant. The rings exhibit a range of structure across many spatial scales; some of this involves the interplay of the fluid nature and the self-g…

2010 Science
Cassini 88
Iapetus: Unique Surface Properties and a Global Color Dichotomy from Cassini Imaging
DOI: 10.1126/science.1177088 Bibcode: 2010Sci...327..435D

West, Robert A.; Porco, Carolyn C.; Burns, Joseph A. +8 more

Since 2004, Saturn’s moon Iapetus has been observed repeatedly with the Imaging Science Subsystem of the Cassini spacecraft. The images show numerous impact craters down to the resolution limit of ~10 meters per pixel. Small, bright craters within the dark hemisphere indicate a dark blanket thickness on the order of meters or less. Dark, equator-f…

2010 Science
Cassini 35
Saturn: Atmosphere, Ionosphere, and Magnetosphere
DOI: 10.1126/science.1179119 Bibcode: 2010Sci...327.1476G

Ingersoll, Andrew P.; Gombosi, Tamas I.

The Cassini spacecraft has been in orbit around Saturn since 30 June 2004, yielding a wealth of data about the Saturn system. This review focuses on the atmosphere and magnetosphere and briefly outlines the state of our knowledge after the Cassini prime mission. The mission has addressed a host of fundamental questions: What processes control the …

2010 Science
Cassini 11