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neutron
1. An uncharged elementary particle that has a mass nearly equal to that of the proton and is present in all known atomic nuclei except the hydrogen nucleus.
2. A neutral hadron that is stable in the atomic nucleus but decays into a protron, an electron and an antineutrino with a mean life of 12 minutes outside the nucleus. Neutronics exist in all atomic nuclei except normal hydrogen. Reported in 1932 by James Chadwick.
2. A neutral hadron that is stable in the atomic nucleus but decays into a protron, an electron and an antineutrino with a mean life of 12 minutes outside the nucleus. Neutronics exist in all atomic nuclei except normal hydrogen. Reported in 1932 by James Chadwick.
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neutron
An atomic particle having high mass but no electrical charge.
Neutrons are present in the nuclei of all atoms except hydrogen.
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Astronomy and related astronomical terms
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“neutron”
neutron star
1. The result of the collapse of the remnant from a supernova explosion if its mass 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 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.
Its name derives from the fact that the object is so condensed that most of its material is in the form of neutrons.
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
(page 17)