neutron star

noun

1. an extremely dense, compact star composed primarily of neutrons, especially the collapsed core of a supernova.

neutron star

noun

1. a star that has collapsed under its own gravity to a diameter of about 10 to 15 km. It is composed mostly of neutrons, has a mass of between 1.4 and about 3 times that of the sun, and a density in excess of 10 ¹⁷ kilograms per cubic metre

neutron star

1. A celestial object consisting of an extremely dense mass of neutrons, formed at the core of a supernova, where electrons and nuclei are compressed together so intensely by the force of gravity that protons and electrons merge together into neutrons. Though their mass is close to that of the Sun, the density of neutron stars is much higher—about 3 × 10 ¹¹ kilograms per cubic centimeter (by comparison, the density of steel is 7.7 grams per cubic centimeter). Neutron stars are typically about 10 km across, and rotate very rapidly. Due to the spinning of electrically charged protons and electrons at their surfaces, their rotation gives rise to strong magnetic fields. The existence of neutron stars was predicted in the 1930s but was not confirmed until the discovery of the first pulsar in 1967.

2. See more at pulsar

neutron star

1. A star about the size of the Earth, made almost entirely of neutrons. It is the end product of the evolution of some stars larger than the sun.

Word History and Origins

Origin of neutron star¹

First recorded in 1930–35

Example Sentences

The neutron star system produces an unusually dense outflow that challenges current ideas about how these winds form and how they reshape their surroundings.

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This discrepancy led many to favor another explanation: ancient, fast-spinning neutron stars known as millisecond pulsars.

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Light emitted from reinvigorated, old neutron stars that spin quickly -- called millisecond pulsars -- could also explain the existing gamma ray map, measurements and signal signature.

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These waves can originate from powerful cosmic events such as supernovae, merging black holes, and colliding neutron stars.

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The night sky contains remarkably precise "cosmic clocks": pulsars, which are dense neutron stars that emit radio pulses at steady intervals, ticking like perfectly timed metronomes.

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