Supernova remnant N132D

Supernova remnant N132D
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In this pointillist image of supernova remnant N132D, the pink sections correspond to hydrogen gas, while the traces of purple correspond to regions of oxygen. These 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," NASA says.

September 11, 2009 9:49 AM PDT

Photo by: NASA, ESA, and the Hubble SM4 ERO Team

| Caption by: Jonathan Skillings

 

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