SUMMARY: "Sakurai's Object" is a white dwarf star that surprised astronomers when if flared brightly in 1996. They originally thought it was a common nova explosion, but further observations have uncovered that the star has actually reignited its stellar furnace. Computer simulations predicted that it could be possible for leftover hydrogen to sink into the star and drive a new flash of hydrogen fusion. If the simulation is correct, the star will stay bright until around the year 2200.
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