Gravity Field, Shape, and Moment of Inertia of Titan

Author:

Iess Luciano1,Rappaport Nicole J.2,Jacobson Robert A.2,Racioppa Paolo1,Stevenson David J.3,Tortora Paolo4,Armstrong John W.2,Asmar Sami W.2

Affiliation:

1. Dipartimento di Ingegneria Aerospaziale ed Astronautica, Università La Sapienza, via Eudossiana 18, 00184 Rome, Italy.

2. Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, USA.

3. California Institute of Technology, 150-21 Pasadena, CA 91125, USA.

4. DIEM-II Facolta' di Ingegneria, Universita' di Bologna, I-47100 Forli, Italy.

Abstract

Titan Through to the Core Gravity measurements acquired from orbiting spacecraft can provide useful information about the interior of planets and their moons. Iess et al. (p. 1367 ; see the Perspective by Sohl ) used gravity data from four flybys of the Cassini spacecraft past Saturn's moon, Titan, to model the moon's gravity field and probe its deep interior structure. Their analysis implies that Titan is a partially differentiated body with a core consisting of a mix of ice and rock or hydrated silicates.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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