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The five-hundred-meter Aperture Spherical radio Telescope (FAST) project

机译:五百米孔径球面射电望远镜(FAST)项目

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Five-hundred-meter Aperture Spherical radio Telescope (FAST) is a Chinese mega-science project to build the largest single dish radio telescope in the world. Its innovative engineering concept and design pave a new road to realize a huge single dish in the most effective way. FAST also represents Chinese contribution in the international efforts to build the square kilometer array (SKA). Being the most sensitive single dish radio telescope, FAST will enable astronomers to jump-start many science goals, such as surveying the neutral hydrogen in the Milky Way and other galaxies, detecting faint pulsars, looking for the first shining stars, hearing the possible signals from other civilizations, etc. The idea of sitting a large spherical dish in a karst depression is rooted in Arecibo telescope. FAST is an Arecibo-type antenna with three outstanding aspects: the karst depression used as the site, which is large to host the 500-meter telescope and deep to allow a zenith angle of 40 degrees; the active main reflector correcting for spherical aberration on the ground to achieve a full polarization and a wide band without involving complex feed systems; and the light-weight feed cabin driven by cables and servomechanism plus a parallel robot as a secondary adjustable system to move with high precision. The feasibility studies for FAST have been carried out for 14 years, supported by Chinese and world astronomical communities. Funding for FAST has been approved by the National Development and Reform Commission in July of 2007 with a capital budget ~ 700 million RMB. The project time is 5.5 years from the commencement of work in March of 2011 and the first light is expected to be in 2016. This review intends to introduce the project of FAST with emphasis on the recent progress since 2006. In this paper, the subsystems of FAST are described in modest details followed by discussions of the fundamental science goals and examples of early science projects.
机译:五百米孔径球面射电望远镜是一项中国的大型科学项目,旨在建造世界上最大的单碟射电望远镜。其创新的工程理念和设计为以最有效的方式实现巨大的单碟铺平了道路。 FAST也代表了中国在建立平方公里阵列(SKA)的国际努力中的贡献。作为最敏感的单碟射电望远镜,FAST将使天文学家能够启动许多科学目标,例如调查银河系和其他星系中的中性氢,探测微弱的脉冲星,寻找第一颗闪亮的恒星,听到可能的信号。在喀斯特洼地中坐一个大的球形盘的想法根植于Arecibo望远镜。 FAST是一种Arecibo型天线,具有三个突出方面:喀斯特洼地作为场地,大面积容纳500米望远镜,而深处则允许40度的天顶角;有源主反射器可校正地面上的球差,以实现全极化和宽带,而无需复杂的馈电系统;轻巧的进料室由电缆和伺服机构驱动,再加上并联机器人作为辅助可调系统,可以高精度移动。在中国和世界天文界的支持下,FAST的可行性研究已经进行了14年。 FAST的资金已由国家发展和改革委员会于2007年7月批准,资金预算约为7亿元人民币。该项目从2011年3月开始工作起的时间为5.5年,预计将在2016年首次亮相。本次审查旨在介绍FAST项目,重点是2006年以来的最新进展。在本文中,子系统对FAST的描述不大详细,随后讨论了基础科学目标和早期科学项目的示例。

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