An important example of the gravitational lens effect is the Einstein ring phenomenon illustrated at right. According to general relativity, gravity causes a deflection of light by the gravitational field of a massive body. In this case a galaxy bends the light emanating from a galaxy that is directly behind it, focusing the otherwise divergent light into a visible ring.
引力透镜效应的一个重要例子是图中所示的爱因斯坦环现象。根据广义相对论,重力会使光因 massive body 的引力场而发生偏折。在这种情况下,一个星系会弯曲来自其后方另一个星系的光,将原本发散的光聚焦成一个可见的环。 This image was made by the Hubble Space Telescope and is credited to L. J. King
(U. Manchester, NICMOS, HST, NASA). The formal designation of the more distant galaxy is B1938+666. The ring is described as being 1 arcsecond across as observed from Earth's vicinity, but tens of thousands of light years across in size. The foreground galaxy must be almost perfectly aligned to provide a circular ring of light like this example.
这张图像由哈勃太空望远镜制作,版权归属于L. J. King(曼彻斯特大学,NICMOS,HST,NASA)。更遥远的星系正式名称为B1938+666。环的直径在地球附近观测时为1角秒,但在实际尺寸上却达到数万光年。前景星系必须几乎完美对齐,才能产生如本例所示的圆形光环。
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