HD 93129A is one of the most luminous stars in the Milky Way. This very young blue hypergiant is an O-type hypergiant located about 7500 light-years from Earth in the bright nebula NGC 3372, the same nebula that harbors other super luminous stars, like Eta Carinae. HD 93129A is actually the brighter member of a binary system that, with its dimmer companion—also an O3 Ia supergiant (HD 93129B)—has an overall mass of 200 solar masses.