南極亮星巡天望遠鏡BSST

南极亮星巡天望远镜（BBST）主镜口径30cm，对角线视场4.8度，含有7个滤光片，观测波段为0.36~1.01μm。计划充分利用南极地区的优良台址条件，寻找出一批短周期（几天）和中短周期（几十天到一个月）轨道上的太阳系外行星。该望远镜在丽江站试观测初步结果显示，南极亮星巡天望远镜像质优秀，在R波段120秒曝光观测极限星等17.5，信噪比20；V波段120秒曝光极限星等16，信噪比40。

2016年4月1日，经过十几天艰苦的安装调试之后，"南极亮星巡天望远镜"（简称BSST）在中国南极中山站正式初光，用BSST望远镜拍摄了杜鹃座47球状星团，效果非常理想，这标志着BSST正式在南极中山站投入实际观测。

BSST的最终安装地点是南极昆仑站(S80º25'01" E77º06'58")，因为过去十几年的研究结果表明，南极昆仑站由于其独特的地理位置，非常适合于光学天文观测，如极佳的视宁度、低的大气边界层、连续黑夜等。从2008年开始，我国天文学家陆续在南极昆仑站从事天文设备的安装和天文观测。实际的台址监测和望远镜观测结果表明了昆仑站台址的优越性。但是南极昆仑站自然环境恶劣，最低温度达到了-80°C，海拔4087米，这对望远镜的正常稳定运行影响极大。针对南极恶劣的环境条件，对BSST望远镜的各个系统进行了优化设计并进行了严苛的试验，顺利完成各项功能。

The telescope mount is from astrophysics 1600GTO

BSST

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