Recently, astronomers have observed a white dwarf that is creating a colorful shockwave as it moves through space.
About White Dwarf:
It is the stellar core left behind after a dying star has exhausted its nuclear fuel and expelled its outer layers to form a planetary nebula.
Characteristics of White dwarfs:
It no longer support nuclear fusion reactions that generate energy, but they are still extremely hot.
Size and Mass: A typical white dwarf is half as massive as the Sun, yet only slightly bigger than Earth.
This makes white dwarfs one of the densest collections of matter, surpassed only by neutron stars.
Composition: A newly born white dwarf consists of helium, carbon, and oxygen nuclei, swimming in a sea of highly energetic electrons.
Unlike most other stars that are supported against their own gravitation by normal gas pressure, white dwarf stars are supported by the degeneracy pressure of the electron gas in their interior.
Degeneracy pressure is the increased resistance exerted by electrons composing the gas, as a result of stellar contraction.
Unless it is accreting matter from a nearby star, the white dwarf cools down over the next billion years or so.
It is predicted that they would ultimately form ‘black dwarfs’, although the Universe is likely not old enough for any black dwarfs to exist yet.
The luminosity of white dwarfs can be used by astronomers to measure how long-ago star formation began in a particular region.
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