Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. Wray 17-96 is a very luminous star in the Scorpius constellation, about 15,000 light-years (4.6 kpc) away. Likely a luminous blue variable (LBV), it has an absolute bolometric magnitude of –10.9 (1.8 million solar units), making it one of the most luminous stars known. Wray 17-96 is also notable for its gas hull, once thought to be a planetary nebula.

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