Astronomers have discovered “monster” stars whose size and brightness exceed what many scientists thought was possible
Found within two young star clusters, NGC 3603 and RMC 136a, the stars weigh up to 300 times the mass of the Sun, a figure which doubles the previously accepted limit of solar mass.
A researcher at the University of Sheffield discovered the stars using the European Southern Observatory's (ESO) Very Large Telescope.
The biggest star found, R136a1 within the R136a cluster, has a current mass of 265 solar masses, and is thought its birthweight was as much as 320 times that of the Sun.
It is also the most luminous star ever found, close to 10 million times that of the Sun.
If R136a1 replaced the Sun at the centre of our solar system, it would outshine our star by as much as the Sun currently outshines the Moon.
The team of international astronomers was led by Paul Crowther, professor of astrophysics from the University of Sheffield's Department of Physics and Astronomy.
Professor Crowther said: “Unlike humans, these stars are born heavy and lose weight as they age.
Being a little over a million-years-old, the most extreme star R136a1 is already “middle-aged” and has undergone an intense weight loss programme, shedding a fifth of its initial mass over that time, or more than fifty solar masses.
“Owing to the rarity of these monsters, I think it is unlikely that this new record will be broken any time soon.” Due to the short lives of these very rare, high mass stars, it remained a challenge for astronomers to identify how they originated, he said.