11:5:09 Black Holes and Milky Way

11:5:09 Black Holes and Milky Way - BlackHoles,MilkyWay...

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Black Holes, Milky Way 05/11/2009 08:35:00 Neutron Star A neutron star is the ball of neutrons left behind by a massive-star supernova Degeneracy pressure of neutrons supports a star Electron degeneracy pressure goes away because electrons combine with  protons, making neutrons and neutrinos Neutrons collapse to center, forming a  neutron star Black Holes A black hole is an object whose gravity is so powerful that not even light can  escape it In more detail, so dense that gravity is so strong that anything in it would need  to be moving faster than the speed of light to escape. Cant happen, so  nothing can get out. The “surface” of a black hole is the radius at which the escape velocity equals  the speed of light o Known as the even horizon o Nothing can escape from within the event horizon because nothing can  go faster than light
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11:5:09 Black Holes and Milky Way - BlackHoles,MilkyWay...

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