首页> 外文会议>9th Symposium on space resource utilization 2016 >Near-Infrared Monitoring of Volatiles in Frozen Lunar Simulants While Drilling
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Near-Infrared Monitoring of Volatiles in Frozen Lunar Simulants While Drilling

机译:钻井时冷冻月球模拟物中挥发物的近红外监测

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In Situ Resource Utilization (ISRU) focuses on using local resources for mission consumables. The approach can reduce mission cost and risk. Lunar polar volatiles, e.g. water ice, have been detected via remote sensing measurements and represent a potential resource for both humans and propellant. The exact nature of the horizontal and depth distribution of the ice remains to be documented in situ. NASA's Resource Prospector mission (RP) is intended to investigate the polar volatiles using a rover, drill, and the RESOLVE science package. RP component level hardware is undergoing testing in relevant lunar conditions (cryovacuum). In March 2015 a series of drilling tests were undertaken using the Honeybee Robotics RP Drill, Near-Infrared Volatile Spectrometer System (NIRVSS), and sample capture mechanisms (SCM) inside a 'dirty' thermal vacuum chamber at the NASA Glenn Research Center. The goal of these tests was to investigate the ability of NIRVSS to monitor volatiles during drilling activities and assess delivery of soil sample transfer to the SCMs in order to elucidate the concept of operations associated with this regolith sampling method. Ten soil samples were captured over the course of two tests at pressures of 10~(-7)-10~(-5) Torr and soil temperatures were 203° to 213° K and ≈93° K for tests 1 and 2, respectively. Each sample was obtained from a depth of 30 to 40 cm within a cryogenically frozen layered bed of NU-LHT-3M lunar regolith simulant. The simulant was doped with 0.1 and 0.2 wt.% water in the upper ~16 cm, for test 1 and 2 respectively, and ~5 wt.% of water below, for both tests, with the two layers separated by aluminum foil. For each sample the drilling sequence consisted of insertion and extraction of the drill to 10, 20, 30, and 40 cm depths, and after the final depth the sample was delivered to the SCM. NIRVSS acquired spectra and images during the drilling sequence and these are the focus of the discussion here. NIRVSS spectra exhibit spectral features associated with water ice after the drill penetrated the aluminum barrier, and especially on extraction from 20 cm depth. These spectral features can be temporally correlated with measurements of the evolved water from the surface during the drilling sequence and images document the growth and evolution of the cuttings pile deposited by the drill. The spectra and images also document some anomalous behavior associated with the refilling of an existing hole due to the constraints imposed by the confined dimensions of the chamber.
机译:原位资源利用(ISRU)重点是将本地资源用于任务消耗品。该方法可以减少任务成本和风险。月球极性挥发物,例如水冰是通过遥感测量发现的,对人类和推进剂都是潜在的资源。冰的水平和深度分布的确切性质仍有待现场记录。 NASA的Resource Prospector任务(RP)旨在使用流动站,钻探和RESOLVE科学软件包研究极性挥发物。 RP组件级硬件正在相关的月球环境(冷冻)下进行测试。 2015年3月,在美国国家航空航天局格伦研究中心的“脏”热真空室内使用Honeywell Robotics RP钻机,近红外挥发性光谱仪系统(NIRVSS)和样品捕获机构(SCM)进行了一系列钻探测试。这些测试的目的是调查NIRVSS在钻井活动期间监测挥发物的能力,并评估将土壤样品转移至SCM的能力,以阐明与这种碎屑取样方法相关的操作概念。在两次测试过程中,在10〜(-7)-10〜(-5)Torr的压力下捕获了十个土壤样品,测试1和2的土壤温度分别为203°至213°K和≈93°K 。在NU-LHT-3M月球重石模拟物的低温冷冻分层床中,从30至40 cm的深度获得每个样品。对于试验1和2,分别在上部〜16 cm处用0.1和0.2 wt。%的水掺杂模拟物,对于两种试验,在下面分别用〜5 wt。%的水掺杂,两层用铝箔隔开。对于每个样品,钻孔顺序包括将钻头插入和拔出至10、20、30和40 cm的深度,并且在最终深度之后,将样品输送到SCM。 NIRVSS在钻井过程中获取了光谱和图像,这些是这里讨论的重点。 NIRVSS光谱显示出钻头穿透铝屏障后与水冰相关的光谱特征,尤其是在从20 cm深度提取时。这些光谱特征可以在时间上与在钻探序列期间从表面释放的水的测量相关,并且图像记录由钻头沉积的钻屑桩的生长和演变。光谱和图像还记录了由于腔室尺寸受限而产生的与重新填充现有孔相关的一些异常行为。

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