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作 者:Xiangyuan Zeng Giovanni Vulpetti Christian Circi
机构地区:[1]School of Automation,Beijing Institute of Technology,Beijing,100081,China [2]International Academy of Astronautics,Paris,75116,France [3]Sapienza University of Rome,Rome,00138,Italy
出 处:《Astrodynamics》2019年第1期1-15,共15页航天动力学(英文)
基 金:the National Natural Science Foundation of China(No.11602019);the Young Elite Scientist Sponsorship Program by CAST(2016QNRC001);The Excellent Young Teachers Program of Beijing Institute of Technology(2015YG0605)is acknowledged as well.Autho。
摘 要:The set of the orbital angular-momentum reversal,or H-reversal,sailcraft trajectory was born as a type of unconventional precursor interstellar mission trajectory by using highperformance solar sails.Starting from an outline of the H-reversal sail trajectory,this paper mainly focuses on the 2D reversal-mode solution to the general solar-photon sail motion equations.The feasible region for H-reversal trajectories in fixed sail attitude angles is illustrated.Some interesting applications of the H-reversal trajectory are presented in detail to show its advantages.As a special case,a precursor interstellar probe can be delivered with a constant sail orientation in the H-reversal trajectory to be compared with the direct-motion sail flyby of the Sun.Of importance are the heliocentric periodic orbits in double H-reversal modes,obtained via both fixed and time-varying sail attitude angles.Two more applications involving H-reversal trajectories are discussed in terms of asteroid deflection and transfer trajectory to rectilinear orbits.Finally,some items of the mathematics behind the 3D motion-reversal trajectories are summarized.
关 键 词:solar-photon sailing sailcraft lightness number orbital H-reversal mode
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