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Development and Testing of an Engineering Model for an Asteroid Hopping Robot

机译:小行星跳跃机器人工程模型的开发与测试

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The science and origins of asteroids is deemed high priority in the Planetary Science Decadal Survey. Two of the main questions from the Decadal Survey pertain to what the "initial stages, conditions, and processes of solar system formation and the nature of the interstellar matter" that was present in the protoplanetary disk, as well as determining the "primordial sources for organic matter." Major scientific goals for the study of planetesimals are to decipher geological processes in SSSBs not determinable from investigation via in situ experimentation, and to understand how planetesimals contribute to the formation of planets. Ground based observations are not sufficient to examine SSSBs, as they are only able to measure what is on the surface of the body; however, in situ analysis allows for further, close up investigation as to the surface characteristics and the inner composure of the body. The Asteroid Mobile Imager and Geologic Observer (AMIGO) is a 1U stowed autonomous robot that can perform surface hopping on an asteroid with an inflatable structure. It contains science instruments to provide stereo context imaging, micro-imaging, seismic sensing, and electric field measurements. Multiple hopping robots are deployed as a team to eliminate single-point failure and add robustness to data collection. An on-board attitude control system consists of a thruster chip of diseretized micro-nozzles that provides hopping thrust and a reaction wheel for controlling the third axis. For the continued development of the robot, an engineering model is developed to test various components and algorithms. Three enabling technologies for the mission are tested. One of the primary components is the inflatable structure that enables context imaging, communication with a mother spacecraft, and solar collection. The other two components tests are for a small reaction wheel system and the MEMS thruster assembly. The inflatable, once properly deployed, is filled with helium to pro
机译:小行星的科学和起源在行星科学划分调查中被视为高度优先。二等调查中的两个主要问题涉及原文象盘中存在的“太阳系形成的初始阶段,条件和过程以及间隙物质的性质”,以及确定“原始来源有机物。”对行星研究的主要科学目标是在SSSBS的破译地质过程,而不是通过原位实验中的调查,并了解行星的形成如何促成行星的形成。基于地面的观察不足以检查SSSB,因为它们只能测量身体表面上的内容;然而,原位分析允许进一步彻底地接近表面特征和身体内部闭合的调查。小行星移动成像器和地质观察者(Amigo)是一个1U收起的自主机器人,可以在具有充气结构的小行星上进行表面跳跃。它包含科学仪器,提供立体声上下文成像,微观成像,地震传感和电场测量。多次跳跃机器人作为团队部署,以消除单点故障并为数据收集添加鲁棒性。板载姿态控制系统由脱臼微喷嘴的推进器芯片组成,其提供跳跃推力和用于控制第三轴的反作用轮。对于机器人的持续发展,开发了一种工程模型来测试各种组件和算法。测试了三种能够为特派团进行测试。其中一个主要组件是充气结构,其使上下文成像,与母宇宙飞船和太阳能集合进行通信。另外两个组件测试用于小反应轮系统和MEMS推进器组件。一旦妥善部署,充气,充满了氦气

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