description E0102 Overview
E0102, formally designated 1E 0102.2-7219, is a young, oxygen-rich supernova remnant located in the Small Magellanic Cloud, a dwarf galaxy orbiting the Milky Way. Estimated to be approximately 2,000 years old, it is the brightest X-ray source in its host galaxy and has been extensively studied by instruments like the Chandra X-ray Observatory. The remnant features a distinct, expanding ring of ejected material that provides crucial data on the mechanics of massive stellar explosions. It is primarily observed by astrophysicists researching shock physics and the chemical enrichment of galaxies.
help E0102 FAQ
How old is the supernova remnant E0102?
E0102 is estimated to be approximately 2,000 years old. It is a young, oxygen-rich supernova remnant located in the Small Magellanic Cloud.
Is E0102 a bright object in its host galaxy?
Yes, it is the brightest X-ray source in its host galaxy. It is located in the Small Magellanic Cloud, which is a dwarf galaxy orbiting the Milky Way.
What is the formal designation for the nebula E0102?
Its formal designation is 1E 0102.2-7219. It is a young, oxygen-rich supernova remnant located in the Small Magellanic Cloud.
Where is the nebula E0102 located?
E0102 is located in the Small Magellanic Cloud, a dwarf galaxy orbiting the Milky Way. It is estimated to be roughly 2,000 years old and is the brightest X-ray source in its galaxy.
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