The regional nanosatellite constellation modelling formation by a piggyback launch from different spaceports

A. Spiridonov, V. Baranova, V. Saetchnikov, Dmitrii Ushakov
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Abstract

The roadmap for constructing a regional nanosatellite constellation using the piggyback launch according to Chinese provider information has developed. For nanosatellite constellation formation to a specific purpose, it is necessary to analyse existing constellation operated similar tasks. Therefore, the software module for the Spire Global constellation orbital construction analysis was developed. The construction of Spire Global nanosatellites constellation based on orbital parameters database in the two-line element set format, satellite constellation databases and the developer site was analysed. A launch from the International Space Station and a piggyback launch were used for constellation formation. Nanosatellite deployment schemes, orbital parameters and flight parameters are investigated launches from the Taiyuan and Jiuquan Satellite Launch Centers with orbit inclination about 90°, that best correspond to the passes over Minsk (ϕ = 53°54′27″ N, λ = 27°33′52″ E) are analysed. The method of nanosatellite orbit preflight prediction at a passing launch has been developed. It involves a finding the nanosatellite state vector in the first flight day and at the time of constellation mission operate start. The launch time, satellite launch center coordinates, launch vehicle type, orbit inclination and altitude (period) are used in the method. In addition, the launch history and the satellite motion dynamics analysis on similar orbits is carried out. It was found that five launches are enough to organise a regional nanosatellite constellation with average radio visibility interruption time of at least 36 min with a maximum value of 85 min.
区域纳米卫星星座的建模形成由一个背驮式发射从不同的航天发射场
根据中国提供的信息,已经制定了使用背驮式发射构建区域纳米卫星星座的路线图。为了使纳米卫星星座形成具有特定的用途,有必要对现有星座运行的类似任务进行分析。为此,开发了Spire Global星座轨道结构分析软件模块。分析了基于双线元集格式轨道参数数据库、卫星星座数据库和开发站点的Spire Global纳米卫星星座建设。一次从国际空间站发射,一次背驮式发射用于星座形成。研究了纳米卫星的部署方案、轨道参数和飞行参数,分别在轨道倾角约为90°的太原和酒泉卫星发射中心发射,分析了最符合明斯克上空(ϕ = 53°54′27″N, λ = 27°33′52″E)的方案。提出了一种纳米卫星通过发射时的飞前轨道预测方法。它涉及到首飞日和星座任务开始运行时纳米卫星状态向量的求值。该方法使用了发射时间、卫星发射中心坐标、运载火箭类型、轨道倾角和高度(周期)。此外,还对卫星的发射历史和相似轨道上的卫星运动动力学进行了分析。研究发现,五次发射足以组织一个区域纳米卫星星座,平均无线电能见度中断时间至少为36分钟,最大值为85分钟。
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