NASA Videograb: Type Ia Supernova.This animation shows the explosion of a white dwarf, an extremely dense remnant of a star that can no longer burn nuclear fuel at its core. In this "type Ia" supernova, white dwarf's gravity steals material away from a nearby stellar companion. When the white dwarf reaches an estimated 1.4 times the current mass of the Sun, it can no longer sustain its own weight, and blows up. Credit: NASA/JPL-Caltech https://exoplanets.nasa.gov/resources/2172/type-ia-supernova/
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Fastest star in the galaxy clocked at 2285 kilometres per second

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NASA Videograb: Type Ia Supernova.This animation shows the explosion of a white dwarf, an extremely dense remnant of a star that can no longer burn nuclear fuel at its core. In this "type Ia" supernova, white dwarf's gravity steals material away from a nearby stellar companion. When the white dwarf reaches an estimated 1.4 times the current mass of the Sun, it can no longer sustain its own weight, and blows up. Credit: NASA/JPL-Caltech https://exoplanets.nasa.gov/resources/2172/type-ia-supernova/

The white dwarf on the right is stealing matter from a neighbouring star. It will eventually explode as a type Ia supernova, propelling its companion away

NASA/JPL-Caltech

Two white dwarfs rocketing through space are the fastest free-moving stars that we know about and they could explain how some supernovae form.

Type Ia supernovae are so reliably bright that astronomers use them as measuring sticks for assessing how far away distant stars and galaxies are. These supernovae tend to occur when a white dwarf siphons off matter from a neighbouring star and starts …

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