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neutron star

American  

noun

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


neutron star British  

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

"Collins English Dictionary — Complete & Unabridged" 2012 Digital Edition © William Collins Sons & Co. Ltd. 1979, 1986 © HarperCollins Publishers 1998, 2000, 2003, 2005, 2006, 2007, 2009, 2012

neutron star Scientific  
  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 Cultural  
  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.


Etymology

Origin of neutron star

First recorded in 1930–35

Example Sentences

Examples are provided to illustrate real-world usage of words in context. Any opinions expressed do not reflect the views of Dictionary.com.

See Examples For:

Many of the chemical elements found throughout the universe are forged during extreme cosmic events, including supernova explosions and neutron star mergers.

From Science Daily Jul. 8, 2026

Because this disk was likely tilted relative to the magnetar's spin, Einstein's theory predicts that the rapidly spinning neutron star would drag the surrounding fabric of space-time with it, producing a phenomenon called Lense-Thirring precession.

From Science Daily Jul. 6, 2026

"This work has the potential to explain the magnetic dynamics relevant in, for example, neutron star mergers and black hole formation, with direct applications to multimessenger astronomy," Tripathi says.

From Science Daily May 26, 2026

When a massive object such as a neutron star passes in front of a more distant star, its gravity bends and magnifies the background star's light.

From Science Daily May 15, 2026

For this mechanism to work, the unseen object has to be very small, like a white dwarf, neutron star, or black hole.

From "A Brief History of Time: And Other Essays" by Stephen Hawking

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