Cassini radar views the surface of Titan

被引：194

作者：

Elachi, C

Wall, S

Allison, M

Anderson, Y

Boehmer, R

Callahan, P

Encrenaz, P

Flamini, E

Franceschetti, G

Gim, Y

Hamilton, G

Hensley, S

Janssen, M

Johnson, W

Kelleher, K

Kirk, R

Lopes, R

Lorenz, R

Lunine, J

Muhleman, D

Ostro, S

Paganelli, F

Picardi, G

Posa, F

Roth, L

Seu, R

Shaffer, S

Soderblom, L

Stiles, B

Stofan, E

Vetrella, S

West, R

Wood, C

Wye, L

Zebker, H

机构：

[1] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA

[2] NASA, Goddard Inst Space Studies, New York, NY 10025 USA

[3] Observ Paris, F-75014 Paris, France

[4] Agenzia Spaziale Italiana, I-00198 Rome, Italy

[5] Fac Ingn, I-80125 Naples, Italy

[6] US Geol Survey, Flagstaff, AZ 86001 USA

[7] Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA

[8] CALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA

[9] Univ Roma La Sapienza, I-00184 Rome, Italy

[10] Politecn Bari, INFM, I-70126 Bari, Italy

[11] Politecn Bari, Dipartimento Interateneo Fis, I-70126 Bari, Italy

[12] Proxemy Res, Laytonville, MD 20882 USA

[13] Planetary Sci Inst, Tucson, AZ 85719 USA

[14] Stanford Univ, Stanford, CA 94305 USA

来源：

SCIENCE | 2005年 / 308卷 / 5724期

关键词：

D O I：

10.1126/science.1109919

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

The Cassini Titan Radar Mapper imaged about 1% of Titan's surface at a resolution of similar to 0.5 kilometer, and larger areas of the globe in lower resolution modes. The images reveal a complex surface, with areas of low relief and a variety of geologic features suggestive of dome-like volcanic constructs, flows, and sinuous channels. The surface appears to be young, with few impact craters. Scattering and dielectric properties are consistent with porous ice or organics. Dark patches in the radar images show high brightness temperatures and high emissivity and are consistent with frozen hydrocarbons.

引用

页码：970 / 974

页数：5

共 27 条

[1] Radar detection of Iapetus [J].