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Cassini Imaging Science: Initial Results on Phoebe and Iapetus

by Cooper, N , Denk, T , Turtle, E , Giese, B , Neukum, G , Wagner, R , West, R , Dyudina, U , Grazier, K , Dawson, D. D , Murray, C. D , Helfenstein, P , Johnson, T. V , Beurle, K , Jacobson, R. A , Brahic, A , Veverka, J , Porco, C. C , Barbara, J , Perry, J , Squyres, S , Roatsch, T , Spitale, J , Thomas, P. C , Burns, J. A , McEwen, A , Tiscareno, M , Evans, M. W , Owen, W. M , Vasavada, A. R , Charnoz, S , Dones, L , Baker, E , Del Genio, A. D , Ingersoll, A. P

in Albedo / Analysis / Artificial satellites / Astronomical objects / Astronomy / Evidence / Extraterrestrial Environment / Fractions / Geologic Sediments / Iapetus (Satellite) / Ice / image analysis / Image resolution / Imaging / Impact craters / Mass wasting / Moons / Observations / Porosity / Research Articles and Reports / Satellites / Satellites (Astronomical bodies) / Saturn / Saturn (Planet) / Saturnian satellites / Scientific Concepts / Scientific imaging / Space exploration / space flight / Spacecraft / Spectrometer / Spectrometers / Topography / Water

2005

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Cassini Imaging Science: Initial Results on Phoebe and Iapetus

2005

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2005

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Journal Article

Cassini Imaging Science: Initial Results on Phoebe and Iapetus

Cooper, N,

Denk, T,

Turtle, E,

Giese, B,

Neukum, G,

Wagner, R,

West, R,

Dyudina, U,

Grazier, K,

Dawson, D. D,

Murray, C. D,

Helfenstein, P,

Johnson, T. V,

Beurle, K,

Jacobson, R. A,

Brahic, A,

Veverka, J,

Porco, C. C,

Barbara, J,

Perry, J,

Squyres, S,

Roatsch, T,

Spitale, J,

Thomas, P. C,

Burns, J. A,

McEwen, A,

Tiscareno, M,

Evans, M. W,

Owen, W. M,

Vasavada, A. R,

Charnoz, S,

Dones, L,

Baker, E,

Del Genio, A. D,

Ingersoll, A. P

2005

Overview

The Cassini Imaging Science Subsystem acquired high-resolution imaging data on the outer Saturnian moon, Phoebe, during Cassini's close flyby on 11 June 2004 and on Iapetus during a flyby on 31 December 2004. Phoebe has a heavily cratered and ancient surface, shows evidence of ice near the surface, has distinct layering of different materials, and has a mean density that is indicative of an ice-rock mixture. Iapetus's dark leading side (Cassini Regio) is ancient, heavily cratered terrain bisected by an equatorial ridge system that reaches 20 kilometers relief. Local albedo variations within and bordering Cassini Regio suggest mass wasting of ballistically deposited material, the origin of which remains unknown.

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Publisher

American Association for the Advancement of Science,The American Association for the Advancement of Science

Subject

Albedo

/ Analysis

/ Artificial satellites

/ Astronomical objects

/ Astronomy

/ Evidence

/ Extraterrestrial Environment