A researcher at the University of Sheffield has discovered the most massive stars ever found, using the European Southern Observatory´s (ESO) Very Large Telescope. 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 team of international astronomers led by Paul Crowther, Professor of Astrophysics from the University of Sheffield´s Department of Physics and Astronomy, used the ESO Very Large Telescope and data from the NASA/ESA (European Space Agency) Hubble Space Telescope to study the two clusters of stars. The research, which is funded by the STFC (Science and Technologies Funding Council) may provide an answer to the question as to how massive stars can be.
NGC 3603 is located 22,000 light-years away from the Sun, and is a cosmic factory within which stars form quickly from the nebula´s ring of gas and dust. RMC 136a (more commonly known as R136a), another cluster of young, hot stars, is found within the Tarantula nebula, itself within the Large Magellanic Cloud, a neighboring galaxy to the Milky Way.
Stars with surface temperatures of over 40,000 C – more than seven times hotter than the Sun – were found, measuring tens of times larger and millions of times brighter. Many of these stars were born with a greater mass than they now posses, losing weight through very powerful winds, and models suggest that several were born in excess of 150 solar masses.
The most massive star ever found, R136a1 within the R136a cluster, has a current mass of 265 solar masses, and it 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 ten million times that of the Sun. Within R136, only four stars out of an estimated 100,000 stars in the cluster weighed more than 150 solar masses at birth, yet they account for nearly half of the solar wind and radiation in the entire cluster.
In NGC 3603, two stars in a binary system were measured, to validate the models used. The stars A1, B and C in the cluster were all estimated to have weighed above or close to 150 solar masses at birth.
Such massive stars have the potential of creating exceptionally bright "pair instability supernovae" at the end of the lives, blowing themselves completing apart without any remnants, and dispersing up to ten solar masses of iron into their surroundings.
Professor Paul 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 remains a challenge for astronomers to identify how they originated. Paul Crowther added: "Either they were born so big or smaller stars merged together to produce them."
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. Raphael Hirschi, from Keele University, added: "Its high mass would reduce the length of the Earth´s year to three weeks, and it would bathe the Earth in incredibly intense ultraviolet radiation, rendering life on our planet impossible."
Notes for Editors: The work is presented within an article titled `The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150M stellar mass limit´ in The Monthly Notices of the Royal Astronomical Society, Paul Crowther et al).
The star A1 in NGC 3603 is a double star, with an orbital period of 3.77 days. The two stars in the system have, respectively, 120 and 92 times the mass of the Sun, which means that they have formed as stars weighing, respectively, 148 and 106 solar masses.
The team is composed of Paul A. Crowther, Richard J. Parker, and Simon P. Goodwin (University of Sheffield, UK), Olivier Schnurr (University of Sheffield and Astrophysikalisches Institut Potsdam, Germany), Raphael Hirschi (Keele University, UK), and Norhasliza Yusof and Hasan Abu Kassim (University of Malaya, Malaysia). Funding for the research was provided by the UK Science and Technology Research Council (STFC)
ESO, the European Southern Observatory, is the foremost intergovernmental astronomy organisation in Europe and the world´s most productive astronomical observatory. It is supported by 14 countries: Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world´s most advanced visible-light astronomical observatory and VISTA, the world´s largest survey telescope. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a 42-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become "the world´s biggest eye on the sky".
For further information please contact: Kyle Christie, Media Relations Assistant, on 0114 2229852 or email k.christie@sheffield.ac.uk
