The Crab and the Jellyfish

Nicholas Mee
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Abstract

Supernova explosions have been recorded as guest stars for thousands of years, but their true nature was only revealed in the twentieth century, largely through the work of Baade and Zwicky. Following Hubble’s determination of the distance to the Andromeda Galaxy, Baade and Zwicky established a new class of extremely bright stellar outburst that they named supernovae. They realized that such explosions in distant galaxies were comparable to the occasional guest star reported in the historical records including stars recorded by Tycho and Kepler. We now know that very large stars that have consumed their nuclear fuel may explode and produce a supernova. The star may be completed destroyed in the eruption or its core may collapse to form a neutron star or black hole.
螃蟹和水母
几千年来,超新星爆炸一直被记录为客座恒星,但它们的真实性质直到20世纪才被揭示出来,主要是通过巴德和兹威基的工作。在哈勃确定了仙女座星系的距离之后,巴德和兹威基建立了一类新的极其明亮的恒星爆发,他们将其命名为超新星。他们意识到,在遥远的星系中,这种爆炸与历史记录中偶尔报告的客星相当,包括第谷和开普勒记录的恒星。我们现在知道,非常大的恒星在耗尽核燃料后可能会爆炸并产生超新星。恒星可能在喷发中完全毁灭,或者它的核心可能坍缩形成中子星或黑洞。
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