White Dwarf Binaries
1 year ago
5
White dwarf stars are dense stellar remnants that can orbit very close to other stars. Sometimes they siphon matter from their companion. The buildup of this matter can trigger a nova explosion on the surface of the white dwarf, releasing a ton of energy. These novas can happen repeatedly over a long period of time. The buildup may also cause a Type Ia supernova, which is a much larger explosion that completely destroys the white dwarf.
Graphics: SpaceEngine
Other Animations: 1st: ESO/M. Kornmesser; 2nd & 3rd: NASA/JPL-Caltech
Music: Brandenburg Concerto No.6 in B-flat major, BWV 1051
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