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首页> 外文会议>Symposium of the International Academy of Astronautics, Oct 2-6, 2000, Rio de Janeiro, Brazil >SPACE DEBRIS OBSERVATIONS AT THE BISEI SPACEGUARD CENTER
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SPACE DEBRIS OBSERVATIONS AT THE BISEI SPACEGUARD CENTER

机译：在BISEI SPACEGUARD中心进行的空间碎片观测

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We are currently constructing a 0.5-meter and a 1-meter telescopes that will operate in tandem to detect and track Near Earth Objects (NEOs) and Space debris. The telescopes have a single flat-plane Cassegrain focus, are optimized for a specific range of wavelengths of light, a small focal ratio with a wide field of view, and hold a single multi-chip CCD camera as their only observational instrument. Because these telescopes are designed for a specific type of observation, the costs of the telescopes are greatly reduced compared to similar sized multipurpose telescopes system. Field sizes are 2 and 3 degree for the 0.5 m and 1.0 m telescopes, respectively. Using the half meter telescope, we started to make test observations from February 1, 2000, and detected known and unknown GEOs and LEOs. The telescope performance developed from February to August is shown in this paper. Some interesting results obtained are also and expected prospects of one meter telescope starting its observation in December are explained.
机译：我们目前正在建造一个0.5米和1米望远镜，这两个望远镜将协同工作，以检测和跟踪近地物体（NEO）和太空碎片。这些望远镜具有一个单一的平面Cassegrain焦距，针对特定波长范围的光进行了优化，具有较小的焦比和宽广的视场，并装有一个多芯片CCD相机作为其唯一的观测仪器。因为这些望远镜是为特定类型的观察而设计的，所以与类似尺寸的多用途望远镜系统相比，望远镜的成本大大降低了。 0.5 m和1.0 m望远镜的视场大小分别为2度和3度。我们从2000年2月1日开始使用半米望远镜进行测试观察，并检测到已知和未知的GEO和LEO。本文显示了从2月到8月开发的望远镜性能。还获得了一些有趣的结果，并解释了从12月开始观测的一米望远镜的预期前景。

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