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|Garching bei München, Germany – July 29, 2009: Using different state-of-the-art techniques on ESO's Very Large Telescope, two independent teams of astronomers have obtained the sharpest ever views of the supergiant star Betelgeuse. They show that the star has a vast plume of gas almost as large as our|
Solar System and a gigantic bubble boiling on its surface.
These discoveries provide important clues to help explain
how these mammoths shed material at such a tremendous rate.
Betelgeuse – the second brightest star in the constellation of Orion (the Hunter) – is a red supergiant, one of the biggest stars known, and almost 1000 times larger than our Sun. It is also one of the most luminous stars known, emitting more light than 100 000 Suns. Such extreme properties foretell the demise of a short-lived stellar king. With an age of only a few million years, Betelgeuse is already nearing the end of its life and is soon doomed to explode as a supernova. When it does, the supernova should be seen easily from Earth, even in broad daylight.
Red supergiants still hold several unsolved mysteries. One of them is just how these behemoths shed such
tremendous quantities of material –
about the mass of the Sun – in only 10 000 years.
Two teams of astronomers have used
Very Large Telescope (VLT)
and the most advanced technologies to take a closer look at the gigantic star.
Their combined work suggests that an answer
to the long-open mass-loss question may well be at hand.
The first team used the adaptive optics instrument,
combined with a so-called “lucky imaging” technique,
to obtain the sharpest ever image of Betelgeuse, even with Earth’s turbulent,
image-distorting atmosphere in the way.
With lucky imaging,
only the very sharpest exposures are chosen and then combined
to form an image much sharper than a single, longer exposure would be.
The resulting NACO images almost reach the theoretical limit of sharpness attainable for an 8-metre telescope. The resolution is as fine as 37 milliarcseconds, which is roughly the size of a tennis ball on the International Space Station (ISS), as seen from the ground.
“Thanks to these outstanding images, we have detected a large plume of gas extending into space from the surface of Betelgeuse,” says Pierre Kervella from the Paris Observatory, who led the team. The plume extends to at least six times the diameter of the star, corresponding to the distance between the Sun and Neptune.
“This is a clear indication that the whole outer shell of the star is not shedding matter evenly in all directions,” adds Kervella. Two mechanisms could explain this asymmetry. One assumes that the mass loss occurs above the polar caps of the giant star, possibly because of its rotation. The other possibility is that such a plume is generated above large-scale gas motions inside the star, known as convection – similar to the circulation of water heated in a pot.
Image of the supergiant star Betelgeuse obtained with the NACO adaptive optics instrument on ESO’s Very Large Telescope.
The use of NACO combined with a so-called “lucky imaging” technique,
allowed the astronomers to obtain the sharpest ever image of Betelgeuse,
even with Earth’s turbulent, image-distorting atmosphere in the way.
The resolution is as fine as 37 milliarcseconds, which is roughly the size of a tennis ball on the International Space Station (ISS), as seen from the ground. The image is based on data obtained in the near-infrared, through different filters.
The field of view is about half an arcsecond wide.
North is up, East is left.
Image: © ESO / P. Kervella
To arrive at a solution, astronomers needed to probe the behemoth in still finer detail.
To do this Keiichi Ohnaka from the
Max Planck Institute for Radio Astronomy
in Bonn, Germany, and his colleagues used interferometry.
Very Large Telescope Interferometer,
which combines the light from three
the astronomers obtained observations as sharp as those of a giant,
virtual 48-metre telescope.
With such superb resolution, the astronomers were able to detect indirectly details
four times finer still than the amazing
images had already allowed
(in other words,
the size of a marble on the ISS,
as seen from the ground).
“Our AMBER observations are the sharpest observations of any kind ever made of Betelgeuse. Moreover, we detected how the gas is moving in different areas of Betelgeuse’s surface – the first time this has been done for a star other than the Sun”, says Ohnaka.
The AMBER observations revealed that the gas in Betelgeuse's atmosphere is moving vigorously up and down, and that these bubbles are as large as the supergiant star itself. Their unrivalled observations have led the astronomers to propose that these large-scale gas motions roiling under Betelgeuse’s red surface are behind the ejection of the massive plume into space.
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. 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”.
P. Kervella, T. Verhoelst, S.T. Ridgway, G. Perrin, S. Lacour, J. Cami and X. Haubois,
"The close circumstellar environment of Betelgeuse – Adaptive optics spectro-imaging in the near-IR with VLT/NACO," Astron. and Astrophys. (accepted) (ArXiv e-print)
K. Ohnaka, K.-H. Hofmann, M. Benisty, A. Chelli, T. Driebe, F. Millour, R. Petrov, D. Schertl, Ph. Stee, F. Vakili and G. Weigelt, "Spatially resolving the inhomogeneous structure of the dynamical atmosphere of Betelgeuse with VLTI/AMBER," Astron. and Astrophys. (accepted) (ArXiv e-print)
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