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- Electron degeneracy pressureBecause the material in a white dwarf no longer undergoes fusion reactions, it lacks a heat source to support it against gravitational collapse. Instead, it is supported only by electron degeneracy pressure, causing it to be extremely dense.en.wikipedia.org/wiki/White_dwarf
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White dwarf - Wikipedia
Because the material in a white dwarf no longer undergoes fusion reactions, it lacks a heat source to support it against gravitational collapse. Instead, it is supported only by electron degeneracy pressure, causing it to be extremely dense. See more
A white dwarf is a stellar core remnant composed mostly of electron-degenerate matter. A white dwarf is very dense: in an Earth sized volume, it packs a mass that is comparable to the Sun. No nuclear fusion takes place in a … See more
Although white dwarfs are known with estimated masses as low as 0.17 M☉ and as high as 1.33 M☉, the mass distribution is strongly peaked at 0.6 M☉, and the majority lie between … See more
The first white dwarf discovered was in the triple star system of 40 Eridani, which contains the relatively bright main sequence See more
White dwarfs are thought to represent the end point of stellar evolution for main-sequence stars with masses from about 0.07 to 10 M☉. The … See more
A white dwarf's stellar and planetary system is inherited from its progenitor star and may interact with the white dwarf in various ways. There … See more
Wikipedia text under CC-BY-SA license White Dwarfs Facts, Information and Photos - National …
White dwarfs are stars that have burned up all of the hydrogen they once used as nuclear fuel. But not all white dwarfs will spend many millennia cooling their heels. Those in a binary star...
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Mar 4, 2022 · White dwarfs contain approximately the mass of the sun but have roughly the radius of Earth, according to Cosmos, the astronomy encyclopedia from Swinburne University in Australia. This makes...
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Jul 16, 2020 · For stars smaller than this, when they run out of hydrogen the helium in their cores is able to support itself through the weird quantum mechanical effect known as degeneracy pressure, whereas...
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Apr 25, 2023 · White dwarfs are the hot, dense remnants of long-dead stars. They are stellar cores, left behind when stars exhaust their fuel supplies and blow their gases into space.
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Jan 30, 2003 · White dwarfs are compact objects supported by degenerate-electron pressure. Newly formed white dwarfs are surrounded by emission nebulae called ``planetary nebulae''.
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