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MY Camelopardalis

Binary star system in the constellation Camelopardalis From Wikipedia, the free encyclopedia

MY Camelopardalis
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MY Camelopardalis (MY Cam) is a binary star system located in the Alicante 1 open cluster, some 13 kly (4.0 kpc) away in the constellation Camelopardalis. It is one of the most massive known binary star systems and a leading candidate for a massive star merger. MY Cam is the brightest star in Alicante 1.[1]

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Artist's impression of MY Camelopardalis
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The system consists of two hot blue O-type stars with one component having a mass of 32 solar masses and the other 38 solar masses.

In 1998, the star was included in a list of suspected variable stars.[8] John Greaves and Patrick Wils proved that it is variable, in 2004.[9] It was given its variable star designation, MY Camelopardalis, in 2008.[10] MY Cam is a contact binary and eclipsing binary, with an orbital period of 1.2 days, and an orbital velocity of 1,000,000 km/h (280 km/s; 620,000 mph).[1] Both stars share a common envelope.[1]

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