Titan's surface before Cassini

被引：27

作者：

Lorenz, RD ^{[1
]}

Lunine, JI ^{[1
]}

机构：

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

来源：

PLANETARY AND SPACE SCIENCE | 2005年 / 53卷 / 05期

关键词：

ADAPTIVE OPTICS; TROPOSPHERIC CLOUDS; PHYSICAL-PROPERTIES; AEROSOL ANALOGS; SPACE-TELESCOPE; MU-M; ATMOSPHERE; RADAR; IMAGES; METHANE;

D O I：

10.1016/j.pss.2004.06.004

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We review current understanding of Titan's surface, synthesizing a paradigm from Earth-based radar observations and near-infrared surface maps, together with reanalysis of Voyager data and results from published theoretical models. Based on these we suggest that Titan has a varied landscape with a variety of tectonic and erosive features indicative of geologic activity, and an impact crater population reflective of the dense atmosphere. (c) 2005 Elsevier Ltd. All rights reserved.

引用

页码：557 / 576

页数：20

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