Smaller sized stars such as white dwarfs– ultradense outstanding remains that form when sunlike stars exhaust all of their nuclear fuel– do not have the gravity and density to produce this iron.”As white overshadows cool down over the next few trillion years, theyll grow dimmer, eventually freeze strong, and become black dwarf stars that no longer shine,” Caplan stated. Its mindbogglingly far in the future,” he said.He found that the most enormous black dwarfs will take off first, followed by less and less enormous stars up until there are none left, which he expects will be in about 10 ^ 3,2000 years.

Smaller sized stars such as white overshadows– ultradense stellar remains that form when sunlike stars exhaust all of their nuclear fuel– dont have the gravity and density to produce this iron.”As white dwarfs cool down over the next few trillion years, theyll grow dimmer, eventually freeze solid, and end up being black dwarf stars that no longer shine,” Caplan said. Caplan calculated that the first of these “black dwarf supernovas” will explode in about 10 to the 1,1000 th years– a practically inconceivably big number. Its mindbogglingly far in the future,” he said.He discovered that the most massive black dwarfs will explode first, followed by less and less enormous stars until there are none left, which he expects will be in about 10 ^ 3,2000 years. “Black dwarf supernova may be the last fascinating thing to happen in the universe.

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