One source of error is refraction, the bending of light beams as they pass through air layers of different temperature and pressure.
误差的一个来源是折射,即光束通过不同温度和压力的空气层时发生的弯曲现象。
If a large object passes in front of a more distant background star, it may act as a lens, bending and distorting the light of that star so that it may appear to brighten significantly.
如果一个体积足够大的星体从一个距离很远的恒星前面经过,那么会产生透镜效果,使那个恒星的光线产生弯曲或变形,这样就能很清楚的看到这个星体。
In this method, when one star passes in front of another, as seen from Earth, the nearer star's gravity ACTS like a lens, bending and magnifying the more distant star's light.
当天文学家用这种方法从地球上观测到一颗恒星在另一颗恒星前“走过”时,距地球较近的这颗恒星的重力就如同一个镜头,将较远的那颗恒星的光弯曲并放大。
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