Analysis of Earth-Uranus Direct-Transfer Trajectory for Optimal Delta-V Using Lambert’s Problem

Gisa Geoson Suseela, Yadu Krishnan Sukumarapillai, Hariprasad Thimmegowda, Pavan Kalyan Devaiah, M. Nagendra, Tamore Silviya Dhiraj
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Abstract

: The Ice Giants may become a sought-after destination in the coming decades as researchers aim to have a better awareness of our Solar system- its origins and growth. The interplanetary trajectory optimization is an important aspect of the analysis of a mission to Uranus. This study investigates possible interplanetary paths to Uranus in the 2022-2030 timeframe. It provides a preliminary estimate of fuel consumption in units of ∆V for various mission durations. A variety of approaches can be used to travel from Earth to another planet. It is conceivable to use a direct transfer route with two engine burns, one at a parking orbit around the Earth and the other to capture around the target planet. This article emphasizes a direct transfer trajectory analysis towards Uranus using Lambert’s problem. Different lambert arcs were considered for the direct transfer. Variations of excess velocities at arrival and departure for various time-of-flight were obtained. The ceiling of the time-of-flight was fixed as 16.5 years by performing a Hohmann transfer. The minimum ∆V was obtained for various time-of-flight ranging from 8.5 years to 16.5 years. The ideal ∆V obtained during the fixed timeframe lies between 6.87 km/s and 7.98 km/s. The minimum value of ∆V was observed for the time-of-flight of 13.5 years.
用Lambert问题分析最优Delta-V的地球-天王星直接传递轨迹
当前位置在未来的几十年里,由于研究人员的目标是更好地了解我们的太阳系——它的起源和发展,冰巨人可能会成为一个受欢迎的目的地。行星际轨道优化是分析天王星任务的一个重要方面。这项研究调查了2022-2030年间可能到达天王星的行星际路径。它提供了不同任务期间以∆V为单位的燃料消耗量的初步估计。从地球到另一个星球旅行可以使用多种方法。可以想象使用两个发动机燃烧的直接转移路线,一个在地球周围的停车轨道上,另一个在目标行星周围捕获。本文着重利用朗伯问题对天王星的直接转移轨迹进行分析。采用不同的朗伯弧线进行直接传递。得到了不同飞行时间到达和离开时的超速度的变化。通过执行霍曼转移,将飞行时间上限定为16.5年。最小∆V在8.5 ~ 16.5年的不同飞行时间范围内得到。在固定时间内得到的理想∆V介于6.87 km/s和7.98 km/s之间。在飞行时间为13.5年时,观测到∆V的最小值。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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