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

被引:0
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作者
Jean-Pierre Lebreton
Olivier Witasse
Claudio Sollazzo
Thierry Blancquaert
Patrice Couzin
Anne-Marie Schipper
Jeremy B. Jones
Dennis L. Matson
Leonid I. Gurvits
David H. Atkinson
Bobby Kazeminejad
Miguel Pérez-Ayúcar
机构
[1] Research and Scientific Support Department,Scientific Project Department
[2] ESA Science Directorate,ESA Operations Directorate
[3] ESTEC,Jet Propulsion Laboratory
[4] ESOC,Department of Electrical and Computer Engineering
[5] Alcatel Alenia Space,Space Research Institute
[6] California Institute of Technology,undefined
[7] Joint Institute for VLBI in Europe,undefined
[8] University of Idaho,undefined
[9] Austrian Academy of Sciences,undefined
来源
Nature | 2005年 / 438卷
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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.
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页码:758 / 764
页数:6
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