29 Jan 2026
NGC1333 is a very active region of star formation in the Perseus molecular cloud. It was first discovered by Eduard Schonfeld in 1855 and is a bright reflection nebula in the western portion of the Perseus molecular cloud. The star BD +30◦549 illuminates NGC 1333 and was found to be a B8 spectral type. It is approximately 1000 light years away and is about 15 light years in diameter.
NGC 1333
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