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How big do stellar explosions get?

机译:恒星爆炸有多大?

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摘要

We thought we knew how powerful supernova explosions could be. We also thought that supernovae and γ -ray bursts were unrelated. One extraordinary supernova is making us re-examine these Ideas. Supernovae are the explosive death throes of massive stars, and they produce the elements that the Earth and you and I are made of. In a 'core-collapse' supernova — one of two main types — the star's core becomes so large that it collapses. The mass of electrons and nuclei becomes compressed into a neutron star, a tiny ball of neutrons about ten kilometres across; that releases a vast amount of gravitational energy into the surrounding material, blowing it outwards. For a few weeks a single star becomes as bright as a galaxy of 100 billion ordinary stars. Supernovae release their energy in many forms: neutrinos, the kinetic energy of the debris, optical light and radio waves.
机译:我们以为我们知道超新星爆炸的强大程度。我们还认为超新星爆发与γ射线爆发无关。一个非凡的超新星正在使我们重新审视这些想法。超新星是巨大恒星爆炸性的死亡喉咙,它们产生了地球和你我组成的元素。在“核塌陷”超新星(两种主要类型之一)中,恒星的核变得如此之大,以至于坍塌。电子和核的质量被压缩成一个中子星,这是一个横跨十公里的微小中子球。它将大量的引力能量释放到周围的材料中,并将其向外吹散。几周之内,一颗恒星变得像一千亿颗普通恒星一样明亮。超新星以多种形式释放其能量:中微子,碎片的动能,光和无线电波。

著录项

  • 来源
    《Nature》 |1998年第6703期|p.635-636|共2页
  • 作者

    Eddie Baron;

  • 作者单位
  • 收录信息 美国《科学引文索引》(SCI);美国《工程索引》(EI);美国《生物学医学文摘》(MEDLINE);美国《化学文摘》(CA);
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 自然科学总论;
  • 关键词

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