stsci_2009-25ad September 9th, 2009
Credit: NASA, ESA, and the Hubble SM4 ERO Team
The supernova remnant, called N132D, resides in the Large Magellanic Cloud, a small companion galaxy of the Milky Way located 170,000 light-years away. The wispy, glowing, magenta structures in this NASA Hubble Space Telescope image are the remains of a star 10 to 15 times the mass of the Sun that we would have seen exploding as a supernova 3,000 years ago. The remnant's fast-moving gas is plowing into the surrounding gas of the galaxy, creating a supersonic shock wave in the surrounding medium and making the material glow. The Hubble visible-light image reveals, deep within the remnant, a crescent-shaped cloud of pink emission from hydrogen gas and soft purple wisps that correspond to regions of glowing oxygen. A dense background of colorful stars is also visible.
Provider: Space Telescope Science Institute
Image Source: https://hubblesite.org/contents/news-releases/2009/news-2009-25
Curator: STScI, Baltimore, MD, USA
Image Use Policy: http://hubblesite.org/copyright/
Detailed color mapping information coming soon...
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