The Pistol and LBV 1806-20 are the brightest stars today because they are the most massive, around 150 or 200 solar masses. Their lifespan is directly proportional to their mass and inversely proportional to their energy output. We expect them to live only about one 200,000th as long as our own sun's main sequence life of 10,000,000,000 years. These heavyweights will therefore shine perhaps as little as 50,000 years.<br /><br />Amazingly enough they are not the most massive stars there ever were. In the first few years after the big bang all stars were composed of hydrogen, helium, and lithium only. They had no heavy metals because these would be created by the deaths of these early stars. Also, the gas clouds that these first stars formed in were extremely more massive than the gas clouds within galaxies that exist today. Finally, these gas clouds were much warmer than their present-day counterparts.<br /><br />These three factors together mean that some of these very first Population III Stars were as much as 100,000 times as massive as our sun. It is hard to calculate their luminiosity because you have to extrapolate three orders of magnitude beyond the available data. If there is a knee in the log line, meaning that the line curves and we don't know it, then our estimate will be wrong.<br /><br />That being said, when a star 100 times more massive than our sun, then it is a million times brighter. This is a rough cubic relationship. Extend that three more zeros for a star 100,000 times as massive as our sun and you get a star that is a quadrillion times brighter (1,000,000,000,000,000 or 10<sup>15</sup> L). Since it has 100,000 times as much mass to start with, it will burn through it's main sequence lifespan in a ten billionth the time our sun does, just about one year.<br /><br />It won't last long, but it makes one hell of a night light while it's lit.