Looking at Old Stars in New Ways: Gravitational Waves Help Us See Inside a Neutron Star
You might have heard the stories: neutron stars are so dense that one teaspoon would weigh about a billion tons on Earth. These stars were once not so different from our Sun, generally about 4 to 8 times more massive. But when these stars run out of fuel to burn, they have a supernova explosion, and eject their outer layers – and in this particular case, the ejected outer layers formed what we now call our beautiful Crab Nebula (see photo). The inner part of the star, with no more fuel, collapse ...
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