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卡西尼-惠更斯号对土星系统的探索:13 年的发现之旅。

Cassini-Huygens' exploration of the Saturn system: 13 years of discovery.

机构信息

Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA.

出版信息

Science. 2019 Jun 14;364(6445):1046-1051. doi: 10.1126/science.aat3760.

Abstract

The Cassini-Huygens mission to Saturn provided a close-up study of the gas giant planet, as well as its rings, moons, and magnetosphere. The Cassini spacecraft arrived at Saturn in 2004, dropped the Huygens probe to study the atmosphere and surface of Saturn's planet-sized moon Titan, and orbited Saturn for the next 13 years. In 2017, when it was running low on fuel, Cassini was intentionally vaporized in Saturn's atmosphere to protect the ocean moons, Enceladus and Titan, where it had discovered habitats potentially suitable for life. Mission findings include Enceladus' south polar geysers, the source of Saturn's E ring; Titan's methane cycle, including rain that creates hydrocarbon lakes; dynamic rings containing ice, silicates, and organics; and Saturn's differential rotation. This Review discusses highlights of Cassini's investigations, including the mission's final year.

摘要

卡西尼-惠更斯任务对土星进行了近距离研究,包括其光环、卫星和磁层。卡西尼号飞船于 2004 年抵达土星,放下惠更斯探测器研究土星大小的卫星泰坦的大气层和表面,并在接下来的 13 年里绕土星运行。2017 年,当卡西尼号燃料不足时,它被有意在土星大气层中蒸发,以保护可能存在生命栖息地的海洋卫星土卫二和土卫六。任务发现包括土卫二南极的间歇泉,这是土星 E 环的来源;土卫六的甲烷循环,包括形成碳氢化合物湖泊的降雨;含有冰、硅酸盐和有机物的动态环;以及土星的差速旋转。本综述讨论了卡西尼号任务的调查亮点,包括任务的最后一年。

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