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FIRST (far-infrared and submillimeter space telescope): a major scientific project of ESA

机译:第一(远红外线和淹没望远镜):ESA的一个主要科学项目

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As one of the four Cornerstones of its scientific program 'Horizon 2000', the European Space Agency ESA is studying a Far Infrared and Submillimeter Space Telescope (FIRST). FIRST will open to astronomical observations the 100 $mu@m to 1mm spectral region, virtually unexplored with a sub-arcmin angular resolution. The 3 - 4 m diameter telescope will be diffraction limited at $lambda $EQ 300 $mu@m or less. The fabrication of a single dish of composite materials is considered as the baseline. The expected life time of this system in orbit is five years or more. The Model Payload, defined in order to allow a realistic system study and an evaluation of the possible scientific return, is composed of two focal instruments. The Multifrequency heterodyne spectrometer will give a very high spectral resolution in the 400 to 630 $mu@m wavelength range and around 300 $mu@m. The Far Infrared Receiver will be an imaging spectrometer covering the 100 - 400 $mu@m range with spectral resolutions ranging from 5 to 10$+4$/ obtained with a set of Fabry-Perot interferometers and filters. FIRST is expected to give unprecedented information on the physics, chemistry and dynamics of interstellar, circumstellar, planetary and cometary gas and dust. Extragalactic physics and deep surveys of cosmological interest will also benefit from this project.
机译:欧洲航天局ESA作为其科学计划“Horizo​​ n 2000”的四个基石之一,正在研究一个远红外和淹没的空间望远镜(第一)。首先将开放到天文观察100 $ MU @ M到1mm光谱区域,几乎未探测到子弧分角分辨率。 3 - 4米直径望远镜将是$ Lambda $ EQ 300 $ MU @ M或更低的衍射限制。一盘复合材料的制造被认为是基线。该系统在轨道中的预期终生时间是五年或更长时间。定义的模型有效载荷,以允许逼真的系统研究和对可能的科学回归的评估,由两个焦点仪器组成。多频外差距光谱仪将在400到630 $ MU @ M波长范围内提供非常高的光谱分辨率,约为300 $ MU @ M。远红外接收器将是覆盖100 - 400 $ MU @ M系列的成像光谱仪,频谱分辨率范围为5至10 $ + 4 $ /获得,具有一组法布里 - 珀罗干涉仪和过滤器。首先,预计将提供有关星际,外形,行星,行星和灰尘和灰尘的物理,化学和动态的前所未有的信息。近似术物理和深度调查宇宙学兴趣也将受益于此项目。

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