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Stability Analysis of Coupled Orbit–Attitude Dynamics Around Asteroids Using Finite-Time Lyapunov Exponents

机译:基于有限时间Lyapunov指数的小行星周围轨道-姿态耦合动力学的稳定性分析

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摘要

This paper investigates coupled orbit-attitude dynamics around asteroids subject to solar radiation pressure and gravity irregularities. The solutions of sun-synchronous orbits with sun-tracking attitude motion are analytically derived, and their stability is evaluated by applying linearization and averaging. To validate the analytical solutions, numerical simulations are performed based on nonlinear coupled orbit-attitude equations of motion. In addition, the nonlinear stability of such coupled motion is analyzed using finite-time Lyapunov exponents. It is demonstrated that the sun-synchronous orbit-attitude coupled motions exhibit long-term stability under certain conditions, and thus, these motions are promising options for asteroid missions.
机译:本文研究了受到太阳辐射压力和重力不规则作用的小行星周围的轨道-高度耦合动力学。通过解析推导了太阳同步轨道与太阳跟踪姿态运动的解,并通过线性化和求平均值来评估它们的稳定性。为了验证解析解,基于运动的非线性耦合轨道-高度方程进行了数值模拟。另外,使用有限时间李雅普诺夫指数分析了这种耦合运动的非线性稳定性。结果表明,太阳同步轨道-姿态耦合运动在某些条件下具有长期稳定性,因此,这些运动是小行星飞行任务的有希望的选择。

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  • 来源
    《Journal of guidance, control, and dynamics》 |2019年第6期|1289-1305|共17页
  • 作者单位

    Japan Aerosp Explorat Agcy JAXA, Chuo Ku, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2525210, Japan;

    Japan Aerosp Explorat Agcy JAXA, Chuo Ku, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2525210, Japan;

    Japan Aerosp Explorat Agcy JAXA, Chuo Ku, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2525210, Japan;

    Japan Aerosp Explorat Agcy JAXA, Chuo Ku, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2525210, Japan;

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