脉冲星
【正文快照】: 脉冲星(Pulsars)是一种致密天体,是中等质量的恒星演化到晚期经超新星爆发后的遗迹.
脉冲中子星
科学家最新发现一个天然的「星际导航系统,要由「脉冲中子星(pulsars)的协助,宇宙飞船能在任何地点定位,而且误差不会超过五公里! (.
A pulsar (short for pulsating radio star) is a highly magnetized, rotating neutron star that emits a beam of electromagnetic radiation. This radiation can only be observed when the beam of emission is pointing toward the Earth, much the way a lighthouse can only be seen when the light is pointed in the direction of an observer, and is responsible for the pulsed appearance of emission. Neutron stars are very dense, and have short, regular rotational periods. This produces a very precise interval between pulses that range from roughly milliseconds to seconds for an individual pulsar.The precise periods of pulsars make them useful tools. Observations of a pulsar in a binary neutron star system were used to indirectly confirm the existence of gravitational radiation. The first extrasolar planets were discovered around a pulsar, PSR B1257+12. Certain types of pulsars rival atomic clocks in their accuracy in keeping time.
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