Design and Optimizing an Interplanetary Trajectory of a Spacecraft to Mercury

IF 0.8 4区 物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS
O. S. Chernenko, I. A. Nikolichev
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Abstract

Throughout the exploration of the Solar System using spacecraft, Mercury has received less attention compared to Venus and Mars as the inner planet due to the inherent challenges of designing efficient trajectories in terms of both time and energy. A mission to Mercury requires a substantial reduction in the spacecraft’s heliocentric velocity, enabling its transfer into the inner Solar System. This trajectory optimization problem remains complex due to the interplay between gravitational influences, spacecraft constraints, and mission objectives. This study focuses on the development and optimization of interplanetary trajectories that minimize the total characteristic velocity (Δv) while meeting constraints on flight duration and flyby altitudes during gravity assist maneuvers. The proposed methodology incorporates gravity assist maneuvers near Earth, Venus, and Mercury, combined with deep space maneuvers (DSMs) for phasing and energy optimization. Two new trajectory designs are presented as examples, demonstrating improvements over traditional approaches by reducing mission duration by one year without exceeding the characteristic velocity budget of NASA’s MESSENGER mission. These results underscore the potential for further improvements in trajectory optimization through refined algorithms and expanded mission constraints. This work highlights the importance of integrating advanced computational techniques with modern propulsion technologies to enhance the feasibility of Mercury exploration. By addressing key challenges in mission design, it contributes to a growing framework for more efficient and scientifically productive missions to the innermost planet of the Solar System.

Abstract Image

设计和优化航天器到水星的行星际轨迹
在使用航天器探索太阳系的过程中,水星作为内行星受到的关注比金星和火星要少,因为在时间和能量方面设计有效的轨道是固有的挑战。前往水星的任务需要大幅降低航天器的日心速度,使其能够进入内太阳系。由于重力影响、航天器约束和任务目标之间的相互作用,这一轨迹优化问题仍然很复杂。本研究的重点是开发和优化行星际轨迹,使总特征速度最小化(Δv),同时满足重力辅助机动期间飞行时间和飞越高度的限制。所提出的方法结合了地球、金星和水星附近的重力辅助机动,结合深空机动(dsm)进行相位和能量优化。以两种新的轨道设计为例,展示了在不超过美国宇航局信使号任务的特征速度预算的情况下,将任务持续时间缩短一年的传统方法的改进。这些结果强调了通过改进算法和扩展任务约束进一步改进轨迹优化的潜力。这项工作强调了将先进的计算技术与现代推进技术相结合的重要性,以提高水星探测的可行性。通过解决任务设计中的关键挑战,它有助于建立一个不断增长的框架,以实现更高效、更科学地探索太阳系最深处行星的任务。
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来源期刊
Solar System Research
Solar System Research 地学天文-天文与天体物理
CiteScore
1.60
自引率
33.30%
发文量
32
审稿时长
6-12 weeks
期刊介绍: Solar System Research publishes articles concerning the bodies of the Solar System, i.e., planets and their satellites, asteroids, comets, meteoric substances, and cosmic dust. The articles consider physics, dynamics and composition of these bodies, and techniques of their exploration. The journal addresses the problems of comparative planetology, physics of the planetary atmospheres and interiors, cosmochemistry, as well as planetary plasma environment and heliosphere, specifically those related to solar-planetary interactions. Attention is paid to studies of exoplanets and complex problems of the origin and evolution of planetary systems including the solar system, based on the results of astronomical observations, laboratory studies of meteorites, relevant theoretical approaches and mathematical modeling. Alongside with the original results of experimental and theoretical studies, the journal publishes scientific reviews in the field of planetary exploration, and notes on observational results.
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