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对Kuiper带天体动力学演化的数值模拟
引用本文:吴晓梅,孙勇.对Kuiper带天体动力学演化的数值模拟[J].山东师范大学学报(自然科学版),2007,22(1):63-65.
作者姓名:吴晓梅  孙勇
作者单位:泰山学院物理与电子科学系,271000,山东泰安;泰山医学院放射学系,271000,山东泰安
摘    要:鉴于无法找到描述Kuiper带天体动力学演化的分析解,本文采用数值模拟的方法,即通过数值积分,得到由太阳、海王星和Kuiper带天体组成的限制性三体问题中Kuiper带天体随时间演化的数值解.结果表明,经长期演化后,共振带中的一些天体的偏心率明显被激励;Kuiper带天体的轨道偏心率和倾角的激励程度和天体的初始轨道半长径、偏心率、倾角有关.

关 键 词:Kuiper带  轨道偏心率  轨道倾角  数值模拟
修稿时间:2006-08-16

NUMERICAL SIMULATION FOR DYNAMICAL EVOLVEMENT OF KUIPER BELT OBJECTS
Wu Xiaomei,Sun Yong.NUMERICAL SIMULATION FOR DYNAMICAL EVOLVEMENT OF KUIPER BELT OBJECTS[J].Journal of Shandong Normal University(Natural Science),2007,22(1):63-65.
Authors:Wu Xiaomei  Sun Yong
Institution:1. Department of Physics and Electronics, Taishan University, 271000, Taian, Shandong, China; 2. Department of Radiation, Taishan Medical College,271000, Taian, Shandong, China
Abstract:Numerical Solution for evolvement of KBOS with time in restricted three-body problem that only contain Sun,Neptune and Kuiper belt object.has been obtained.Results show that,after long-term evolution,some bodies' eccentricity in resonance region has been inspired.Orbital eccentricity and inclination's inspire degree are related to their initial orbital semimajor axis,eccentricity and inclination.
Keywords:kuiper belt  orbital eccentricity  orbital inclination  numerical simulation
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