巨大的反射望远镜的反射镜以光学聚集来自天体的光，转往两部相机和两部摄谱仪。
The reflector telescope's mirror optics gather light from celestial objects and direct it to an array of cameras and spectrographs.
牛顿望远镜和反射折射望远镜都有一个次级反射镜(或称斜反射镜)，它们阻挡了一部分主反射镜的发射光。
Newtonian and catadioptric telescopes have secondary (or diagonal) mirrors that obstruct a small percentage of light from the primary mirror.
同时，这组反射镜将产生具有22.8米直径望远镜解析度的图象。
Together, the mirrors will produce images with a resolution of a 22.8-meter telescope.
借助平行光和双面反射镜，对分光计望远镜的视场角进行了分析和测量，并通过实验得出了结果。
With the help of the ray of equal rank and double-faced reflector, the telescopic visual angle of the spectrometer was analyzed and measured. And the conclusion was drawn.
这数据将输入功能强大的计算机处理，但所有这些将阐明的，只是望远镜和反射镜的距离。
That data will be fed into a powerful computer, but all it will tell is the distance between the telescope and the reflector.
这数据将输入功能强大的计算机处理，但所有这些将阐明的，只是望远镜和反射镜的距离。
That data will be fed into a powerful computer, but all it will tell is the distance between the telescope and the reflector.
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