WebJan 29, 2010 · A white dwarf is supported by electron degeneracy pressure, a neutron star by neutron degeneracy pressure (go look those terms up for a quick physics lesson). 3. A white dwarf has a larger radius --about 600 times. 4. A neutron star has a stronger gravitational field -about 400,000 times. 5. Finally, neutron stars have higher temperatures … Web5,875 Likes, 20 Comments - O2P (@only__for__physics) on Instagram: "According to models of stellar evolution, certain types of stars need longer than the universe ha..."
White Dwarfs - Imagine the Universe!
WebWhite dwarfs typically have a radius just .01 times that of our own sun, but their mass is about the same. Stars like our sun fuse hydrogen in their cores into helium. White dwarfs … WebWhen a star like our Sun dies, it doesn’t explode into a supernova or collapse into a black hole. Instead, it gently sheds its outer layers, which form a beautiful cloud called a “planetary nebula”, while the dying star’s core becomes a white dwarf. cs workspace
White Dwarfs - New Mexico State University
WebAs the hydrogen runs out, a star with a similar mass to our sun will expand and become a red giant. When a high-mass star has no hydrogen left to burn, it expands and becomes a red supergiant. While most stars quietly fade away, the supergiants destroy themselves in a huge explosion, called a supernova. WebWhen all the nuclear reactions are over, a small star like the Sun may begin to contract under the pull of gravity. In this instance, the star becomes a white dwarf which fades and changes... WebWhite dwarfs have exhausted all their nuclear fuel and so have no residual nuclear energy sources. Their compact structure also prevents further gravitational contraction. The … earnings us companies