Composition of The Universe and the Stellar Life Cycle Flashcards Quizlet
What Is A White Dwarf Quizlet. A white dwarf's faint luminosity comes from the emission of residual thermal energy; Click the card to flip 👆.
No fusion takes place in a white dwarf. If one white dwarf collides with another or pulls too much matter from its nearby star, the white dwarf can explode. Web white dwarfs term 1 / 27 luminosity, temp, radius, density click the card to flip 👆 definition 1 / 27 low luminosity high temp => small radius high density click the card to flip 👆 flashcards learn test match created by stellare terms in this set (27) luminosity, temp, radius, density low luminosity high temp => small radius high density What is a white dwarfs composition? A white dwarf is very dense: Web a white dwarf is what's left after a star the size of our sun has run out of fuel. Web a white dwarf is a) the exposed core of a dead star, supported by electron degeneracy pressure. Web what is a white dwarf? C) a hot but very small main sequence star with a mass of less than 1.4 solar masses. Click the card to flip 👆.
Degeneracy pressure arises in white dwarfs from closely packed electrons. Also called a degenerate dwarf. What is a white dwarfs composition? A white dwarf is very dense: Degeneracy pressure what is degeneracy pressure? Web what is a white dwarf? Sets found in the same folder cosmic microwave background 4 terms adrianmoldovan facts about the universe 4 terms Degeneracy pressure arises in white dwarfs from closely packed electrons. B) the exposed core of a dead star, supported by neutron degeneracy pressure. Web white dwarfs term 1 / 27 luminosity, temp, radius, density click the card to flip 👆 definition 1 / 27 low luminosity high temp => small radius high density click the card to flip 👆 flashcards learn test match created by stellare terms in this set (27) luminosity, temp, radius, density low luminosity high temp => small radius high density C) a hot but very small main sequence star with a mass of less than 1.4 solar masses.
