Astrophotonics: The next wave in observational cosmology

J. Bland-Hawthorne
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Abstract

Modern astronomy is on the verge of another revolution. The largest optical/infrared telescopes, with diameters up to 10m, are soon to be overtaken by 25-42m behemoths. The most compelling science goals are the detection of faint light from extrasolar planets in orbit around nearby stars and, at the other extreme, the detection of the first star-forming systems in the early universe which is the focus of this talk. The design and construction of the next generation of astronomical instruments presents us with a major challenge. The astronomical community must embrace new technological avenues, in particular, astrophotonics. I will show the PIMMS concept, a new approach to astronomical instruments which has application across many applied sciences. I will also feature a new instrument concept GNOSIS that will see first light in 2011.
天文光子学:观测宇宙学的下一波浪潮
现代天文学即将迎来另一场革命。直径达10米的最大光学/红外望远镜很快将被25-42米的庞然大物所取代。最引人注目的科学目标是探测在附近恒星轨道上的太阳系外行星发出的微弱光,在另一个极端,探测早期宇宙中第一个恒星形成系统这是这次演讲的重点。下一代天文仪器的设计和建造给我们提出了一个重大挑战。天文学界必须接受新的技术途径,特别是天文光子学。我将展示PIMMS概念,这是一种应用于许多应用科学的天文仪器的新方法。我还将介绍一种新的仪器概念GNOSIS,它将在2011年首次亮相。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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