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Numerical Simulation of Dynamical Evolution of the Solar System over 5 Billion Years

Numerical Simulation of Dynamical Evolution of the Solar System over 5 Billion Years
太阳系50亿年来动力学演化的数值模拟
批准号:
04640277
负责人:
KINOSHITA Hiroshi
金额:
$1.6万
依托单位国家:
日本
项目类别:
Grant-in-Aid for General Scientific Research (C)
财政年份:
1992
资助国家:
日本
项目状态:
已结题
起止时间:
1992 至 1994

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中文摘要
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英文摘要
Planetary motions are said to be chaotic in the sense that the maximum Lyapunov exponent is positive.So far the longest integration up to now, over 845 million years (42 Pluto's Lyapunov times) , does not show any indication of a gross instability in the motion of Pluto.We carried out the numerical integration of Pluto over the age of the solar system (5.5 billion years both towards the past and the future) . This integration also did not give any indication of chaotic evolution of Pluto.The divergences of Keplerian elements of a nearby trajectory at first grow limearly with the time and then start to increase exponentially.The exponential divergences stop at about 420 million years and saturate.The exponential divergneces are suppressed by the following three resoncnaces that Pluto has :1) Pulto is in the 3 : 2 mean motion resonance with Neptune.2) The argument of perihelion librates around 90 degrees and its period is 3.8 Myr.The dominant periodic variations of the eccentricity and the inclination are synchronized with the libration of the argument of perihelion.3) Moreover the longitude of Pluto's node referred to the longitude of Neptune's node circulates and the period of this circulation is equal to the period of the libration of the argument of Perihelion (a secondary resonance) .In order to investigate how Pluto evolves to the present stable state of three resonance lockings, we have to take account of a non-conservative mechanism in the earlsy stage of the solar system.
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K.Tanikawa and Y.Yamaguchi: Toward the Understanding of Chaos : Towards the Harnessing of Chaos, ed M.Yamaguchi. Elsevier, 409-412 (1994)
K.Tanikawa 和 Y.Yamaguchi:走向对混沌的理解:走向混沌的利用,M.Yamaguchi 编辑。
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通讯作者:
K.Tanikawa: "Stable and Unstable Manifolds Asymptotic to the Outermost KAM Curve" Journ.Math.Analys.Appl.166. 529-539 (1992)
K.Tanikawa:“渐近到最外层 KAM 曲线的稳定和不稳定流形”Journ.Math.Analys.Appl.166。
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通讯作者:
H. Kinoshita: "Motion of the Orbital Plane of a Satellite due to a Secular Change of the Obliquity of its Mother Planet" Celestial Mechanics and Dynamical Astronomy. 57. 359-368 (1993)
H. Kinoshita:“由于其母行星倾角的长期变化而导致卫星轨道平面的运动”天体力学和动力天文学。
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