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Kepler Beyond Planets: Finding Exploding Stars (Type Ia Supernova from a White Dwarf Merger)

NASA/JPL-Caltech2018-03-26

NASA

NASA
Washington, DC, United States

This frame from an animation shows the merger of two white dwarfs. A white dwarf is an extremely dense remnant of a star that can no longer burn nuclear fuel at its core. This is another way that a "type Ia" supernova occurs.

Stellar explosions forge and distribute materials that make up the world in which we live, and also hold clues to how fast the universe is expanding. By understanding supernovae, scientists can unlock mysteries that are key to what we are made of and the fate of our universe. But to get the full picture, scientists must observe supernovae from a variety of perspectives, especially in the first moments of the explosion. That's really difficult -- there's no telling when or where a supernova might happen next.

An animation is available at https://photojournal.jpl.nasa.gov/catalog/PIA22353

Details

  • Title: Kepler Beyond Planets: Finding Exploding Stars (Type Ia Supernova from a White Dwarf Merger)
  • Creator: NASA/JPL-Caltech
  • Date Created: 2018-03-26
  • Rights: JPL
  • Album: kboggs

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