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Lunar laser ranging by optical transponder collocated with VLBI radio sources on the moon

机译:月球激光通过光学应答器与月球上的VLBI无线电源并沉淀

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The lunar laser ranging (LLR) has been dependent on the retro-reflectors placed on the Moon since the past three decades before. In spite of the technical improvement, regular observations are performed by a limited number of stations due to the weak echo. To allow more opportunities for observations, it is most effective to place modern device on the Moon. Since a Japanese second lunar probe is planned to be launched in 2006, the ideas are collected for scientific purposes. It is described here that an optical transponder on the Moon would enhance the possibility of LLR observations to a large degree. It is also proposed to have three radio sources on the Moon to determine the angular component perpendicular to the Earth-Moon vector and librations. One of the most important scientific targets for the proposed mission is a relativistic experiment which was not attained by a conventional LLR.
机译:月球激光测距(LLR)一直依赖于自过去三十年以来以来放置在月球上的复古反射器。尽管有技术改进,但由于弱回声,通过有限数量的车站进行定期观察。为了允许更多的观察机会,将现代设备放在月球上最有效。由于计划在2006年开展日本的第二次月球探针,因此收集了这些想法以获得科学目的。这里描述了月球上的光学应答器将增强LLR观察的可能性在很大程度上。还提出了在月球上有三个无线电源来确定垂直于地球矢量和守计的角分量。拟议任务最重要的科学目标之一是一种相对论的实验,常规LLR未获得。

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