设置在月球的巨大的光学干涉法望远镜阵列，将探测太阳系周围其他星球，而且对它们的环境特征和是否具备生存条件进行分析。
Very large optical interferometry telescope arrays on the Moon will not only detect planets around other stars, but also analyze their atmospheres and characterize their habitability.
但是光学望远镜只能在清晰视觉条件下工作，所以受气候和大气干扰限制。
But the telescopes only perform during clear conditions and are limited by weather and atmospheric interferences.
在进行电子光学计算之前，必须先界定边界条件。
The boundary conditions should be defined before the electron optics computation.
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