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Updated: Jan 7, 2026

Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
在太空飞船在低重力下着陆时,考虑到粘合力,预测细流石颗粒的散射
Masatsugu Otsuki1, Mitsuhisa Baba2, Takao Maeda3
1Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, 252-5210, Japan. otsuki.masatsugu@jaxa.jp.
未来的月球样本返回任务需要了解着陆期间的光岩粒子行为. 这项研究预测了从着陆台的粒子散射,以告知敏感设备的防护对策.
科学领域:
- 太空探索 太空探索
- 星球科学 星球科学
- 机器人技术 机器人技术 机器人技术
背景情况:
- 商业月球探测正在增加,日本计划火星月球样本返回任务.
- 长时间的月球着陆需要强大的系统,能够承受动态事件,而不是短暂的触摸和去任务.
- 在月球着陆期间,保护敏感设备免受 regolith 颗粒的冲击和粘附至关重要.
研究的目的:
- 为了预测由具有显著动能的着陆台散射的 regolith 颗粒的行为.
- 根据天体表面层特征,确定设备最不利的条件.
- 为规律反制措施提供建议,解决低重力测试中的挑战.
主要方法:
- 对在与着陆台撞击时的 regolith 颗粒行为进行分析.
- 模拟粒子散射动态,考虑着陆的动能 (几百焦耳).
- 评估天体表面层的特性,以确定不利的着陆条件.
主要成果:
- 预测的 regolith 粒子散射模式和速度.
- 确定对设备构成最高风险的着陆场景.
- 对观测设备的粒子粘附和碰撞效应的表征.
结论:
- 了解 regolith 动力学对于成功的长期登月至关重要.
- 特定的着陆地点特征可能会加剧颗粒散射的风险.
- 对抗措施的开发需要准确的预测模型,特别是对于低重力环境.
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