月球熔岩管探测任务热环境分析

Stefano Pescaglia, R. Barbieri, Giuseppe Bortolato, P. Maggiore, P. Messidoro, R. Vittori
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摘要

月球纳米无人机(LuNaDrone)是一种能够在月球近地表环境下自主飞行的小型航天器,其主要应用是探测月球凹坑以探测月球熔岩管的潜在开口。在整个任务的各个阶段,航天器必须处理几个热环境,其中,月球表面的操作对热控制设计至关重要。有意义的热分析需要对地面和飞行中的热环境和航天器进行正确的建模。在“热桌面”中实施的拟议建模方法旨在对整个表面操作和飞行段入射到航天器表面的辐射热通量进行初步评估,以便定性地验证飞行演习模型的实施并确定最关键的热情景。从阿波罗17号和月球勘测轨道器的温度数据出发,设计了月球表面和月球坑的热模型,并以Mare Tranquillitatis坑为例对其进行了表征。为了评估航天器上的热流,已经建立了一个12U测试箱的模型,利用热桌面的组装和符号功能来实现热模型中的飞行演习。分析是在三个不同的当地时间和四个基本方向上进行的。结果表明建模方法如何正确地允许在热模型中执行飞行演习。无论当地时间或航天器方向如何,结果表明,最关键的辐射情景不是飞行段中的一个,而是发射阶段,即推进剂几乎完全耗尽,航天器发现自己处于月球表面的高辐射环境之后。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Analysis of the thermal environment in the LuNaDrone exploration mission of lunar lava tubes
Lunar Nano Drone (LuNaDrone) is a small spacecraft capable of performing autonomous flight in the lunar near-surface environment, whose primary application is a mission of exploration of lunar pits to detect potential openings to lunar lava tubes. Throughout the phases of this mission, the spacecraft has to deal with several thermal environments and among these, the lunar surface operations can be critical for the thermal control design. A meaningful thermal analysis requires correct modelling of both the thermal environment and the spacecraft, on the ground and in flight. The proposed modelling approach, implemented in Thermal Desktop, aims to provide a preliminary evaluation of the radiative thermal fluxes incident on the spacecraft faces throughout the surface operations and flight segments, in order to qualitatively validate the flight manoeuvres model implementation and to identify the most critical thermal scenario. Starting from temperature data of Apollo 17 and Lunar Reconnaissance Orbiter, a thermal model was designed for the lunar surface and for a lunar pit, characterizing them for the Mare Tranquillitatis Pit case. A 12U test box has been modelled in order to evaluate heat fluxes on the spacecraft, exploiting Thermal Desktop's Assembly and Symbols features to implement the flight manoeuvres in the thermal model. The analyses were performed for three different local times and four cardinal directions approaches to the pit. The results showed how the modelling approach correctly allows the implementation of flight manoeuvres in the thermal model. Regardless of local time or spacecraft orientation, the results show that the most critical radiative scenario is not one of the flight segments, but the transmission phase, after the propellant has been almost completely depleted and the spacecraft finds itself in a highly radiative environment on the lunar surface.
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