Toshiki P. Tanaka, Oikawa, Takuto, Keeni Shruti, Iida, Teruhito, Kazuya Yoshida, John Walker · 2026 · arXiv (Cornell University)
DOI: 10.48550/arxiv.2610.28127 · cited by 3 works (OpenAlex) · open-access PDF
研究は、HAKUTO Rover Flight Model(FM)の熱インターフェイス設計に焦点を当て、最終的な熱真空実験を使用してその評価に焦点を当てた。最初は、分析熱モデルが開発され、ロバーを6つの異なる放射表面に分けました。ロバーの表面温度は、太陽放射流に対する方向性と、月の放射線、太陽アルベド、および月の規律からの導力などの他の熱因子に基づいて決定されました。これらの熱源の影響を考慮して、航空技術とソーラーパネルの角度のための適切な設置場所は、ロバーの熱性能と電力生成を最適化するために決定され、ロバーの質量が4kg未満であることを保証しました。初期的な熱分析
Machine translation (Meta M2M100); the English original follows.
The research focuses on the thermal interface design of the HAKUTO Rover Flight Model (FM) and its evaluation using the final thermal vacuum experiment. Initially, an analytical thermal model was developed, dividing the rover into six distinct radiating surfaces. The surface temperature of the rover was then determined based on its orientation relative to the solar radiative flux, as well as other thermal factors such as lunar radiation, solar albedo, and conduction from the lunar regolith. By considering the impact of these heat sources, suitable mounting locations for the avionics and the angle of the solar panels were determined to optimize the rover's thermal performance and power generation while ensuring the rover's mass remained under 4 kg. After the preliminary thermal analysis, numerical computational simulations were conducted to further elaborate on the thermal response of the final HAKUTO Rover FM design, which was then verified through a thermal balance test in a vacuum environment.
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Topics: Astrobiology, Control (management), Computer science, Geology, Remote sensing, Aeronautics
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