中子星很奇特!
瞧,我们就这么直说了。它们也没办法;当一颗恒星比我们的太阳更重,却只有一座城市那么大时,就会变成这样。中子星让我们得以接触地球上无法直接研究的极端条件。
以下是关于中子星的五个事实,它们表明中子星有时比科幻小说还要离奇!
1. 中子星以一声巨响开始生命
当一颗比我们的太阳更大、质量更高的恒星在生命末期耗尽燃料时,它的核心会坍缩,外层则在超新星爆发中被吹散。留下什么取决于原来恒星的质量。如果它大约是太阳质量的
2. Neutron stars contain the densest material that we can directly observe

While neutron stars’ dark cousins, black holes, might get all the attention, neutron stars are actually the densest material that we can directly observe. Black holes are hidden by their event horizon, so we can’t see what’s going on inside. However, neutron stars don’t have such shielding. To get an idea of how dense they are, one sugar cube of neutron star material would weigh about 1 trillion kilograms (or 1 billion tons) on Earth – about as much as a mountain. That is what happens when you cram a star with up to twice the mass of our Sun into a sphere the diameter of a city.
3. Neutron stars can spin as fast as blender blades
Some neutron stars, called pulsars, emit streams of light that we see as flashes because the beams of light sweep in and out of our vision as the star rotates. The fastest known pulsar, named PSR J1748-2446ad, spins 43,000 times every minute. That’s twice as fast as the typical household blender! Over weeks, months or longer, pulsars pulse with more accuracy than an atomic clock, which excites astronomers about the possible applications of measuring the timing of these pulses.
4. 中子星是已知最强的磁体
和太空中许多天体(包括地球)一样,中子星也有磁场。所有已知中子星的磁场都比地球强数十亿到数万亿倍,而一种被称为磁星的中子星,其磁场还能再强一千倍。这些极强的磁力会在磁星表面引发星震,撕裂星壳,并产生极其明亮的伽马射线闪光,已知这些闪光能穿越我们银河系数千光年,对地球高层大气造成可测量的变化。
5. 中子星的脉冲最初被认为可能是外星信号
嘀。嘀。嘀。脉冲星的发现始于1967年的一个谜团,当时天文学家接收到非常规律的射电闪光,却无法弄清是什么造成的。早期研究人员曾短暂考虑过这可能是外星文明信号的想法,这一解释后来被抛弃,但却留在了他们对最初天体的昵称中——LGM-1,暗指“小绿人”(后来它被重新命名为PSR B1919+21)。当然,现在科学家已经明白,脉冲星是旋转的中子星,发出覆盖很宽波长范围的光,我们将其探测为非常规律的脉冲——但最初的探测确实让观察者们一时摸不着头脑。
我们在国际空间站上的Neutron star Interior Composition Explorer (NICER)载荷正在为天文学家提供更多关于中子星的见解——helping us determine what is under the surface。
想了解更多关于中子星的知识吗?观看这个……
NASA’s Goddard Space Flight Center











