This image shows a pair of colossal stars, WR 25 and Tr16-244, located within the open cluster Trumpler 16. This cluster is embedded within the Carina Nebula, an immense cauldron of gas and dust that lies approximately 7,500 light-years from Earth in the constellation of Carina. Larger image (new window)
Hubble spies gigantic stars
27 Nov 2008
Two of our Galaxy's most massive stars have been scrutinised in an impressive view by the Hubble Space Telescope. They have, until recently, been shrouded in mystery, but the new image shows them in greater detail than ever before.
The image shows a pair of colossal stars, known as WR 25 and Tr16-244, located within the open cluster Trumpler 16. The cluster is embedded within the Carina Nebula, an immense cauldron of gas and dust that lies approximately 7,500 light-years from Earth.
The Carina Nebula contains several ultra-hot stars, including these two star systems and the famous blue star Eta Carinae, which has the highest luminosity yet confirmed.
As well as producing incredible amounts of heat, these stars are also very bright, emitting most of their radiation in the ultraviolet part of the spectrum and appearing blue in colour. They are so powerful that they burn through their hydrogen fuel faster than other types of stars, leading to a 'live fast, die young' lifestyle.
WR 25 is the brightest, situated near the centre of the image. The neighbouring Tr16-244 is the third brightest, just to the upper left of WR 25. The second brightest, to the left of WR 25, is a low-mass star located much closer to the Earth than the Carina Nebula but in the same line of sight.
Stars like WR 25 and Tr16-244 are relatively rare compared to other, cooler types. They interest astronomers because they are associated with gas clouds where stars are being born, and influence the structure and evolution of galaxies.
WR 25 is likely to be the most massive and interesting of the two. Its true nature was revealed two years ago when an international group of astronomers led by Roberto Gamen, then at the Universidad de La Serena in Chile, discovered that it was actually at least two stars very close together. The more massive is a 'Wolf-Rayet star' and may weigh more than 50 times the mass of our Sun. It is losing mass rapidly through powerful stellar winds that have expelled the majority of its outermost hydrogen-rich gas layers, while its more mundane companion star is probably about half as massive as the Wolf-Rayet star, and orbits around it once every 208 days.
Massive stars are usually formed in compact star clusters. Often the individual stars are so physically close to each other that it is very difficult to resolve them through telescopes as separate objects.
In the WR 25 star system, two of the stars are so close to each other that they usually look like a single object—but Hubble's Advanced Camera for Surveys shows them as two.
The new Hubble observations have revealed that the Tr16-244 system is actually a triple star. Two of the stars are so close to each other that they look like a single object, but Hubble's Advanced Camera for Surveys shows them as two (see the image at left). The third star takes tens or hundreds of thousands of years to orbit the other two. The brightness and close proximity of the individual components of such massive double and triple star systems makes it particularly challenging to discover the properties of massive stars.
WR 25 and Tr16-244 are the likely sources of radiation that is causing a giant gas globule within the Carina Nebula to slowly evaporate away into space, while possibly inducing the formation of new stars within it. The radiation is also thought to be responsible for the globule's interesting shape, prominently featured in earlier Hubble images, which looks like a hand with a 'defiant' finger pointing towards WR 25 and Tr16-244.
These new observations were obtained by a team including astronomers from US, Chilean, Spanish, and Argentine institutions and led by Jesus Maiz Apellaniz from the Instituto de Astrofisica de Andalucia in Spain. They are using Hubble as well as ground-based observatories in Spain, Chile, and Argentina to build a comprehensive catalogue of observations of all the massive stars in the Galaxy that are detectable at visible wavelengths.
Adapted from information issued by NASA, ESA and Jesus Maiz Apellaniz (Instituto de Astrofisica de Andalucia, Spain).
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