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BRIAN KOBERLEIN, UNIVERSE TODAY
A white dwarf isn t your typical kind of star.
While main sequence stars such as our Sun fuse nuclear material in their cores to keep themselves from collapsing under their own weight, white dwarfs use an effect known as quantum degeneracy. The quantum nature of electrons means that no two electrons can have the same quantum state.
When you try to squeeze electrons into the same state, they exert a degeneracy pressure that keeps the white dwarf from collapsing.
But there is a limit to how much mass a white dwarf can have.
Subrahmanyan Chandrasekhar made a detailed calculation of this limit in 1930 and found that if a white dwarf has more mass than about 1.4 Suns, gravity will crush the star into a neutron star or black hole.
Your readers will wait for a proper production.
-Alex Parker
times.
As reported by The Washington Free Beacon, a newsroom racial reckoning’s collecting quite the following:
In a similar move, the New York Times Guild said in a memo last summer that the paper would move toward mirroring the city’s exact racial demographics in its newsroom. The guild claimed its concern with viewpoint diversity began a month before, with an op-ed written by Sen. Tom Cotton (R., Ark.) that black staff members said put them “in danger.”
[Read more about the Big Apple outlet’s Cottonmouth malady here.]
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