Somewhere in the range of 170,000 light-years away in the heavenly body of Dorado, somewhere down in the heart of the Tarantula Nebula, is a group of extremely youthful, splendid stars. The R136 bunch, as it is somewhat unromantically known, has a surprisingly high rate of star arrangement.
It’s bright to the point that it creates most of the vitality that makes the Tarantula Nebula, around 1,900 light-years over, unmistakable from Earth.
The vitality these stars radiate, be that as it may, is for the most part in the bright range. So a global group of researchers drove by Paul Crowther at the University of Sheffield in the UK utilized the bright spatial determination capacity of the Hubble Space Telescope’s Imaging Spectrograph to examine.
“The capacity to recognize bright light from such an incredibly packed district into its segment parts, determining the marks of individual stars, was just made conceivable with the instruments on board Hubble,” Crowther said in an announcement.
What the researchers found was unprecedented. Inside the group are many stars more than 50 times the mass of the sun, and nine huge beasts more than 100 times the mass of the sun. What’s more, it’s not all simply mass, either: Together, the stars are 30 million times brighter than the sun.
Four of these stars were already known, discovered by Crowther and his team in 2010, measuring over 150 solar masses. Up until that point, 150 sunlight based masses was thought to be as far as possible for how huge stars could get. This new overview opens up new open doors for concentrate how these inestimable leviathans structure, since it’s still an immense riddle.
However, the nine stars are still not the most massive stars in the universe. That record still goes to a star in the cluster called R136a1, which clocks in at 256 solar masses.
If you want a wallpaper-sized version of the photo of R136, you can find them here.