“The night has a thousand eyes, and the day but one;
Yet the light of the bright world dies with the dying sun.” -Francis William Bourdillon
When we look for the brightest, bluest, most massive individual stars, we’re restricted to looking nearby, since it’s impossible to resolve individual stars at distances that extend much beyond our own galaxy. So how surprising is it, then, when the most massive stars we’ve ever found aren’t in our own galaxy, nor in any of the monster galaxies we’ve found nearby, but in a small, satellite dwarf of our own: the Large Magellanic Cloud?
The tidal disruption of the Milky Way causes a huge spike in star formation among the neutral gas, and has led to an incredibly rich region of new stars, including dozens of stars over 50 solar masses, nine over 100, four over 150 and the most massive one, R136a1, coming in at an incredible 250 times the mass of our Sun. It’s the most massive collection of hot, young stars in the entire known Universe.