Astronomers witness birth of Milky Way's most massive star
Scientists have observed in unprecedented detail the birth of a massive star within a dark cloud core about 10,000 light years from Earth. The team used the new ALMA (Atacama Large Millimetre/submillimetre Array) telescope in Chile -- the most powerful radio telescope in the world -- to view the stellar womb which, at 500 times the mass of the Sun and many times more luminous, is the largest ever seen in our galaxy.
The researchers say their observations -- to be published in the journal Astronomy and Astrophysics -- reveal how matter is being dragged into the centre of the huge gaseous cloud by the gravitational pull of the forming star -- or stars -- along a number of dense threads or filaments.
"The remarkable observations from ALMA allowed us to get the first really in-depth look at what was going on within this cloud," said lead author Dr Nicolas Peretto, from Cardiff University. "We wanted to see how monster stars form and grow, and we certainly achieved our aim. One of the sources we have found is an absolute giant -- the largest protostellar core ever spotted in the Milky Way!
"Even though we already believed that the region was a good candidate for being a massive star-forming cloud, we were not expecting to find such a massive embryonic star at its centre. This cloud is expected to form at least one star 100 times more massive than the Sun and up to a million times brighter. Only about one in 10,000 of all the stars in the Milky Way reach that kind of mass."
Different theories exist as to how these massive stars form but the team's findings lend weight to the idea that the entire cloud core begins to collapse inwards, with material raining in towards the centre to form one or more massive stars.
Co-author Professor Gary Fuller, from The University of Manchester, said: "Not only are these stars rare, but their births are extremely rapid and childhood short, so finding such a massive object so early in its evolution in our Galaxy is a spectacular result.
"Our observations reveal in superb detail the filamentary network of dust and gas flowing into the central compact region of the cloud and strongly support the theory of global collapse for the formation of massive stars."
The University of Manchester hosts the Science and Technology Facilities Council (STFC)-funded support centre for UK astronomers using ALMA, where the observations were processed.
Team member Dr Ana Duarte-Cabral, from the Université de Bordeaux, said: "Matter is drawn into the centre of the cloud from all directions but the filaments are the regions around the star that contain the densest gas and dust and so these distinct patterns are generated."
Dr Peretto added: "We managed to get these very detailed observations using only a fraction of ALMA's ultimate potential. ALMA will definitely revolutionise our knowledge of star formation, solving some current problems, and certainly raising new ones."
Source: Manchester University
- Big Baby: Astronomers Zoom In on Birth of Very Massive Starfrom Scientific AmericanThu, 11 Jul 2013, 13:00:23 EDT
- Telescope captures birth of Milky Way's most massive star yet seenfrom UPIWed, 10 Jul 2013, 18:30:14 EDT
- Dark Cloud Is Creating A Monster Star | Videofrom Space.comWed, 10 Jul 2013, 8:00:35 EDT
- Astronomers witness birth of Milky Way's most massive starfrom Science DailyWed, 10 Jul 2013, 7:00:28 EDT
- Astronomers witness birth of Milky Way's most massive starfrom PhysorgWed, 10 Jul 2013, 5:30:27 EDT
Latest Science NewsletterGet the latest and most popular science news articles of the week in your Inbox! It's free!
Check out our next project, Biology.Net
From other science news sites
Popular science news articles
- Possible extragalactic source of high-energy neutrinos
- Screening method uncovers drugs that may combat deadly antibiotic-resistant bacteria
- Discovery of a fundamental limit to the evolution of the genetic code
- New tech uses hardware, software to train dogs more efficiently
- Three potentially habitable worlds found around nearby ultracool dwarf star