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Updated: Jul 14, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
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Published on: November 15, 2013

混乱的起源在外太阳系的外部太阳系

Murray1, Holman

  • 1Canadian Institute for Theoretical Astrophysics, University of Toronto, 60 St. George Street, Toronto, Ontario M5S 3H8, Canada. Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA.

Science (New York, N.Y.)
|March 19, 1999
PubMed
概括

一个新的分析理论解决了太阳系稳定性争论,揭示了由于重叠共振的混乱木星行星轨道. 这种混乱的利亚普诺夫时间为1000万年,而天王星的动态寿命为100万亿年.

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