M87 as Black Hole CandidateM87作为黑洞候选
The case for identifying an object as a black hole sometimes takes the form of eliminating other possible explanations for its behavior. Shown below is an image captured by the Wide Field and Planetary Camera of the Hubble Space Telescope. It is a portion of the active galaxy M87 showing a spiral of hot gas at its center. The inset at upper left shows the central region. Measurements by the space telescope indicate that the central disc is rotating so rapidly that a black hole is likely the energy source. Further evidence comes from the brilliant relativistic jet of electrons seen as a diagonal line at lower right. This also points to a black hole "engine" to supply that kind of energy in that small a volume of space. The volume from which the energy emanates is no larger than our solar system. Models of the phenomena indicate a black hole at the center of M87 with as much as 3 billion solar masses. 将一个天体认定为黑洞有时会以排除其行为的其他可能解释的形式出现。下图是哈勃太空望远镜宽场和行星相机拍摄的图像。这是一幅活跃星系M87的图像,显示其中心有螺旋状的高温气体。左上角的插图显示了中心区域。空间望远镜的测量结果表明,中心盘的旋转速度如此之快,很可能黑洞是其能量来源。进一步的证据来自右下角看到的明亮的相对论电子喷流,这表明一个黑洞“引擎”能够在此如此小的体积空间内提供这种类型的能量。能量来源的体积不超过我们的太阳系。现象模型表明,M87中心有一个多达30亿倍太阳质量的黑洞。
![]() M87位于室女座,距离地球约5000万光年。NASA图像。 |
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