An overview of the descent and landing of the Huygens probe on Titan

被引:167
作者
Lebreton, JP [1 ]
Witasse, O
Sollazzo, C
Blancquaert, T
Couzin, P
Schipper, AM
Jones, JB
Matson, DL
Gurvits, LI
Atkinson, DH
Kazeminejad, B
Pérez-Ayúcar, M
机构
[1] European Space Agcy, Estec, Sci Directorate, Res & Sci Support Dept, NL-2200 AG Noordwijk, Netherlands
[2] European Space Agcy, Estec, Sci Directorate, Sci Project Dept, NL-2200 AG Noordwijk, Netherlands
[3] ESOC, ESA Operat Directorate, D-64293 Darmstadt, Germany
[4] Alcatel Alenia Space, F-06156 Cannes La Bocca, France
[5] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[6] Joint Inst VLBI Europe, NL-7990 AA Dwingeloo, Netherlands
[7] Univ Idaho, Dept Elect & Comp Engn, Moscow, ID 83844 USA
[8] Austrian Acad Sci, Space Res Inst, A-8042 Graz, Austria
基金
美国国家科学基金会;
关键词
D O I
10.1038/nature04347
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
Titan, Saturn's largest moon, is the only Solar System planetary body other than Earth with a thick nitrogen atmosphere. The Voyager spacecraft confirmed that methane was the second-most abundant atmospheric constituent in Titan's atmosphere, and revealed a rich organic chemistry, but its cameras could not see through the thick organic haze. After a seven-year interplanetary journey on board the Cassini orbiter, the Huygens probe was released on 25 December 2004. It reached the upper layer of Titan's atmosphere on 14 January and landed softly after a parachute descent of almost 2.5 hours. Here we report an overview of the Huygens mission, which enabled studies of the atmosphere and surface, including in situ sampling of the organic chemistry, and revealed an Earth-like landscape. The probe descended over the boundary between a bright icy terrain eroded by fluvial activity - probably due to methane - and a darker area that looked like a river- or lake-bed. Post-landing images showed centimetre-sized surface details.
引用
收藏
页码:758 / 764
页数:7
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