Supernova Remnant DEM L71
Several thousand years ago, a star some 160,000 light-years away from us exploded, scattering stellar shrapnel across the sky. The exploding star was a white dwarf located in the Large Magellanic Cloud, one of our nearest neighboring galaxies. After swelling to approximately one and a half times the size of the sun, the star became unstable and ignited as a Type Ia supernova. The supernova remnant pictured here, known as DEM L71, formed when a white dwarf reached the end of its life and ripped itself apart, ejecting a superheated cloud of debris in the process. Slamming into the surrounding interstellar gas, this stellar shrapnel gradually diffused into the separate fiery filaments of material seen scattered across this skyscape.
Credits: ESA/Hubble & NASA, Y. Chu