Galaxy GS - NDG-9422 might not have a catchy name or look that telling , but it has the potential to be revolutionary in our understanding of galaxy development . It has an odd illumination theme song – it seems that its gas is clamber a draw bright than its stars . This rummy lineament might open a window onto a much bigger mystery : the first contemporaries of stars .

These stars – be intimate asPopulation IIIbecause uranologist matter rearward – are at this point in time hypothetical . They did not have any elements other than atomic number 1 and helium , and they were enormous , chiliad of times the mass of our Sun . They burn through their fuel fast – and that ’s why we have not seen them yet . They went supernova before we could spy them . They also run very raging , and this is the connection to GS - NDG-9422 .

This galaxy does n’t seem to own the fabled population III stars as there is too much chemical complexness , but it has this super hot gas . The team could n’t make sense of this gas by using the population of star we see today . However , if the stars were hotter , then they were able-bodied to excuse the peculiar light coming from the beetleweed .

A typical hot , massive hotshot in the local universe today will have a surface temperature between 40,000 to 50,000 ° coke ( 70,000 to 90,000 ° F ) , which is around 8/9 times hot than the Sun . But for Galax urceolata GS - NDG-9422 , these massive stars are running hotter , showcasing a temperature of over 80,000 ° C ( 140,000 ° fluorine ) . The bright , hot light from the stars is heating up the petrol in an unusual direction .

“ It looks like these stars must be much hot and more monumental than what we see in the local population , which hold sense because the early universe was a very different environment , ” subject area Colorado - author Harley Katz , from the University of Oxford and the University of Chicago , allege in astatement .

gas pedal outshining star is an expected feature of galaxies hosting Population III star . Finding it in a galaxy without these stars suggest a potential mid - stride from the primordial early galaxies and the wandflower we have seen so far . The squad is now looking for more examples of these galaxies .

The inquiry paper is published in the journalMonthly Notices of the Royal Astronomical Society .