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土星重力场和环质量的测量及其意义。

Measurement and implications of Saturn's gravity field and ring mass.

机构信息

Department of Mechanical and Aerospace Engineering, Sapienza Università di Roma, Rome 00184, Italy.

Department of Astronomy, University of California, Berkeley, Berkeley, CA 94720, USA.

出版信息

Science. 2019 Jun 14;364(6445). doi: 10.1126/science.aat2965. Epub 2019 Jan 17.

Abstract

The interior structure of Saturn, the depth of its winds, and the mass and age of its rings constrain its formation and evolution. In the final phase of the Cassini mission, the spacecraft dived between the planet and its innermost ring, at altitudes of 2600 to 3900 kilometers above the cloud tops. During six of these crossings, a radio link with Earth was monitored to determine the gravitational field of the planet and the mass of its rings. We find that Saturn's gravity deviates from theoretical expectations and requires differential rotation of the atmosphere extending to a depth of at least 9000 kilometers. The total mass of the rings is (1.54 ± 0.49) × 10 kilograms (0.41 ± 0.13 times that of the moon Mimas), indicating that the rings may have formed 10 to 10 years ago.

摘要

土星的内部结构、风速的深度以及其环的质量和年龄限制了它的形成和演化。在卡西尼号任务的最后阶段,该航天器在距离云层顶部 2600 到 3900 公里的高度之间潜入行星及其最内层的环之间。在这六次穿越中,监测了与地球的无线电链路,以确定行星的引力场和环的质量。我们发现土星的重力偏离了理论预期,需要大气的差动旋转延伸到至少 9000 公里的深度。环的总质量为(1.54 ± 0.49)×10 千克(比月球土卫一的质量小 0.41 ± 0.13 倍),这表明这些环可能在 10 到 10 年前形成。

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