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1.
Noun (astrophysics term): the small, highly-dense stellar body remaining after the nova detonation of a "main sequence" star, typically Earth-sized in overall dimension, but displacing a gravitational mass equivalent to that of the Earth's Sun.
Astrophysicists now calculate that white dwarf stars may account for as much as 6% of all the known stars in our quadrant of the Milky Way galaxy.
by speedog July 13, 2010

Words related to white dwarf

black hole