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STIS Chemically Analyzes the Ring Around SN 1987a (IRAS 05240-6948 , Large Magellanic Cloud , LMC , SN 1987A) — image from the Hubble Space Telescope

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STIS Chemically Analyzes the Ring Around SN 1987a

May 12, 1997 · ESA/Hubble · IRAS 05240-6948 , Large Magellanic Cloud , LMC , SN 1987A · Dorado

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The ring formed 30, 000 years before the star exploded and so is a fossil record of the final stages of the star's existence. The light from the supernova heated the gas in the ring so that it now glows at temperatures from 5, 000 to 25, 000 degrees Kelvin.