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Deposition of metal films on an ionic liquid as a basis for a lunar telescope

机译:金属膜在离子液体上的沉积作为月球望远镜的基础

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An optical/infrared telescope of 20-100 m aperture located on the Moon would be able to observe objects 100 to 1,000 times fainter than the proposed next generation of space telescopes. The infrared region of the spectrum is particularly important for observations of objects at redshifts z > 7. The apparent simplicity and low mass of a liquid mirror telescope, compared with a traditional pointable glass mirror, suggest that the concept should be considered further. A previously proposed liquid mirror telescope, based upon a spinning liquid metallic alloy, is not appropriate for infrared applications, which will require a liquid below 130 K. Here we report the successful coating of an ionic liquid with silver. The surface is smooth and the silver coating is stable on a timescale of months. The underlying ionic liquid does not evaporate in a vacuum and remains liquid down to a temperature of 175K. Given that there are ~10~6 simple and ~10~(18) ternary ionic liquids, it should be possible to synthesize liquids with even lower melting temperatures.
机译:位于月球上的孔径为20-100 m的光学/红外望远镜将能够观测到比拟议的下一代太空望远镜微弱100至1,000倍的物体。光谱的红外区域对于观察红移z> 7的物体尤为重要。与传统的点状玻璃镜相比,液体镜望远镜的明显简单性和低质量建议应进一步考虑该概念。先前提出的基于旋转的液态金属合金的液体镜望远镜不适用于红外应用,因为红外应用将需要低于130 K的液体。在此,我们报道了成功的离子液体镀银技术。表面光滑,并且银涂层在数月的时间内都是稳定的。下方的离子液体不会在真空中蒸发,而会保持液体状态直至175K。考虑到存在〜10〜6种简单的离子液体和〜10〜(18)三元离子液体,应该有可能以更低的熔融温度合成液体。

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