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DISCORD BETWEEN GAIA AND SELENE: WHY SELENOTHERMAL ENERGY IS INSUFFICIENT FOR ELECTRICAL POWER GENERATION

机译:盖亚和硒之间的矛盾:为什么亚热能不足以发电

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During the year 2012, the German Aerospace Center (DLR) has, in the framework of the internal Competition of Visions, investigated the possibility of using residual lunar heat, dubbed selenothermal energy, for electrical power generation by application of e.g. Rankine or Stirling processes. The initial idea was mainly based on the fact that the lunar subsurface region has an increased temperature (250 K) in comparison to the surface (ca. 120 K during lunar night) and therefore a heat reservoir that could potentially be used for energy production during the lunar night, where lack of solar illumination prevents usage of solar cells. Preliminary results have been previously published on the 63~(rd) IAC in Naples. More review, calculation and testing has however shown that the heat flow within the lunar soil cannot support power generation in a way or amount meaningful for a lunar infrastructure or mission. Initial calculations estimated the available heat flow to about 4 W/m~2, which has to be corrected downwards by a factor of 100 following the more detailed research. In this paper the details of this research will be elaborated, explaining new calculations and the reasons for the divergence of the initial calculations and the more recent ones. It will be shown how the data review led to the conclusion that selenothermal energy cannot be used in the desired way analogously to geothermal energy.
机译:在2012年期间,德国航空航天中心(DLR)在内部视觉竞争的框架下,研究了利用月球余热(被称为硒热能)通过应用例如太阳能发电的可能性。朗肯或斯特林工艺。最初的想法主要基于以下事实:月球地下区域的温度比地面(月球夜间大约120 K)升高(250 K),因此蓄热器可能在下半年产生能量在阴暗的夜晚,缺乏太阳光会阻止太阳能电池的使用。初步结果先前已在那不勒斯的第63届IAC上发表。然而,更多的审查,计算和测试表明,月球土壤中的热流无法以对月球基础设施或任务有意义的方式或数量支持发电。初步计算估计可用热流量约为4 W / m〜2,在进行更详细的研究后,必须将其向下修正100倍。在本文中,将详细阐述这项研究的细节,解释新的计算方法以及初始计算方法与最新计算方法之间出现差异的原因。将显示数据审查如何得出结论:不能以与地热能类似的理想方式使用硒热能。

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