Supermassive Black Holes

Nicholas Mee
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Abstract

The Event Horizon Telescope (EHT) is aiming to image the event horizon of the supermassive black hole at the centre of our galaxy. Andrea Ghez has mapped out the orbits of stars around this supermassive black hole and deduced it has a mass of four million Suns. An even bigger supermassive black hole of six billion solar masses lies at the centre of the M87 Galaxy. Shep Doeleman has marshalled several of the world’s radio telescopes to form the EHT with the aim of imaging the event horizons of these black holes.
超大质量黑洞
事件视界望远镜(EHT)的目标是拍摄银河系中心超大质量黑洞的事件视界。安德里亚·盖兹绘制出了这个超大质量黑洞周围恒星的轨道,并推断出它的质量是400万个太阳的质量。M87星系的中心还有一个更大的超大质量黑洞,质量为60亿个太阳。谢普·多尔曼(Shep Doeleman)将世界上的几台射电望远镜组合在一起,形成EHT,目的是对这些黑洞的视界进行成像。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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