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“neutron star”
1. The result of the collapse of the remnant from a supernova explosion: The mass of a neutron star exceeds the chandrasekhar limit, but is less than that required for gravity to continue the collapse down to a black hole.
2. A very small core of a "super-dense" star: A neutron star is composed mostly of neutrons (electrically neutral subatomic particles in the baryon family).
The "chandrasekhar limit" is the upper limit for the mass of a white dwarf star, beyond which the star collapses to a neutron star or a black hole. A star having a mass above this limit will continue to collapse to form a neutron star.
The name of the neutron star is derived from the fact that the object is so condensed that most of its material is in the form of neutrons.
It was named after Subrahmanyan Chandrasekhar (1910-1995), a U.S. astrophysicist.
Neutron stars are estimated to be so condensed that a fragment, the size of a sugar cube, would weigh as much as all the people on the Earth put together.
This entry is located in the following unit:
Astronomy and related astronomical terms
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