Titan Radar Mapper observations from Cassini's T3 fly-by.

Elachi, C; Wall, S; Janssen, M; Stofan, E; Lopes, R; Kirk, R; Lorenz, R; Lunine, J; Paganelli, F; Soderblom, L; Wood, C; Wye, L; Zebker, H; Anderson, Y; Ostro, S; Allison, M; Boehmer, R; Callahan, P; Encrenaz, P; Flamini, E; Francescetti, G; Gim, Y; Hamilton, G; Hensley, S; Johnson, W; Kelleher, K; Muhleman, D; Picardi, G; Posa, F; Roth, L; Seu, R; Shaffer, S; Stiles, B; Vetrella, S; West, R

Elachi, C; Wall, S; Janssen, M; Stofan, E; Lopes, R; Kirk, R; Lorenz, R; Lunine, J; Paganelli, F; Soderblom, L; Wood, C; Wye, L; Zebker, H; Anderson, Y; Ostro, S; Allison, M; Boehmer, R; Callahan, P; Encrenaz, P; Flamini, E; Francescetti, G; Gim, Y; Hamilton, G; Hensley, S; Johnson, W; Kelleher, K; Muhleman, D; Picardi, G; Posa, F; Roth, L; Seu, R; Shaffer, S; Stiles, B; Vetrella, S; West, R.

Afiliación

Elachi C; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109, USA.

Nature ; 441(7094): 709-13, 2006 Jun 08.

Article en En | MEDLINE | ID: mdl-16760968

RESUMEN

Cassini's Titan Radar Mapper imaged the surface of Saturn's moon Titan on its February 2005 fly-by (denoted T3), collecting high-resolution synthetic-aperture radar and larger-scale radiometry and scatterometry data. These data provide the first definitive identification of impact craters on the surface of Titan, networks of fluvial channels and surficial dark streaks that may be longitudinal dunes. Here we describe this great diversity of landforms. We conclude that much of the surface thus far imaged by radar of the haze-shrouded Titan is very young, with persistent geologic activity.

Buscar en Google

Añadir a Mi BVS

Imprimir

XML

PubMed Links

Colección: 01-internacional Base de datos: MEDLINE Idioma: En Revista: Nature Año: 2006 Tipo del documento: Article País de afiliación: Estados Unidos Pais de publicación: Reino Unido

Buscar en Google

Añadir a Mi BVS

Imprimir

XML

PubMed Links