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Public release date: 20-Feb-2013[ | E-mail |
Share ] Contact: Richard Hook
rhook@eso.org
49-893-200-6655
ESO
New infrared VISTA image of NGC 6357
Located around 8000 light-years away in the constellation of Scorpius (The Scorpion), NGC 6357 -- sometimes nicknamed the Lobster Nebula [1] due to its appearance in visible-light images -- is a region filled with vast clouds of gas and tendrils of dark dust. These clouds are forming stars, including massive hot stars which glow a brilliant blue-white in visible light.
This image uses infrared data from ESO's Visible and Infrared Survey Telescope for Astronomy (VISTA) at the Paranal Observatory in Chile. It is just a small part of a huge survey called VISTA Variables in the Via Lactea (VVV) that is imaging the central parts of the Galaxy (eso1242 - http://www.eso.org/public/news/eso1242/). The new picture presents a drastically different view to that seen in visible-light images -- such as the image taken with the 1.5-metre Danish telescope at La Silla -- as infrared radiation can penetrate much of the covering of dust that shrouds the object [2].
One of the bright young stars in NGC 6357, known as Pismis 24-1, was thought to be the most massive star known -- until it was found to actually be made up of at least three huge bright stars, each with a mass of under 100 times that of our Sun. Even so, these stars are still heavyweights -- some of the most massive in our Milky Way. Pismis 24-1 is the brightest object in the Pismis 24 star cluster, a bunch of stars that are all thought to have formed at the same time within NGC 6357.
VISTA is the largest and most powerful survey telescope ever built, and is dedicated to surveying the sky in infrared light. The VVV survey is scanning the central bulge and some of the plane of our galaxy to create a huge dataset that will help astronomers to discover more about the origin, early life, and structure of the Milky Way.
Parts of NGC 6357 have also been observed by the NASA/ESA Hubble Space Telescope (heic0619a - http://www.spacetelescope.org/images/heic0619a/) and ESO's Very Large Telescope (eso1226a - http://www.eso.org/public/images/eso1226a/). Both telescopes have produced visible-light images of various parts of this region -- comparing these images with this new infrared image above shows some striking differences. In the infrared the large plumes of red-hued material are much reduced, with tendrils of pale, purple gas stretching out from the nebula in different areas.
###
Notes
[1] The informal name of Lobster Nebula is also sometimes given to the spectacular star-forming region Messier 17 (eso0925 - http://www.eso.org/public/news/eso0925/), although that object is more often called the Omega Nebula.
[2] Infrared observations can reveal features that cannot be seen in visible-light pictures, for example because an object is too cold, obscured by thick dust, or is very distant, meaning that its light has been stretched towards the red end of the spectrum by the expansion of the Universe.
More information
ESO is the foremost intergovernmental astronomy organisation in Europe and the world's most productive ground-based astronomical observatory by far. It is supported by 15 countries: Austria, Belgium, Brazil, 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 two survey telescopes. VISTA works in the infrared and is the world's largest survey telescope and the VLT Survey Telescope is the largest telescope designed to exclusively survey the skies in visible light. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning the 39-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become "the world's biggest eye on the sky".
Links
Contacts
Richard Hook
ESO, La Silla, Paranal, E-ELT & Survey Telescopes Press Officer
Garching bei Mnchen, Germany
Tel: +49 89 3200 6655
Cell: +49 151 1537 3591
Email: rhook@eso.org
[ | E-mail | Share ] ?
AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert! system.
Public release date: 20-Feb-2013[ | E-mail |
Share ] Contact: Richard Hook
rhook@eso.org
49-893-200-6655
ESO
New infrared VISTA image of NGC 6357
Located around 8000 light-years away in the constellation of Scorpius (The Scorpion), NGC 6357 -- sometimes nicknamed the Lobster Nebula [1] due to its appearance in visible-light images -- is a region filled with vast clouds of gas and tendrils of dark dust. These clouds are forming stars, including massive hot stars which glow a brilliant blue-white in visible light.
This image uses infrared data from ESO's Visible and Infrared Survey Telescope for Astronomy (VISTA) at the Paranal Observatory in Chile. It is just a small part of a huge survey called VISTA Variables in the Via Lactea (VVV) that is imaging the central parts of the Galaxy (eso1242 - http://www.eso.org/public/news/eso1242/). The new picture presents a drastically different view to that seen in visible-light images -- such as the image taken with the 1.5-metre Danish telescope at La Silla -- as infrared radiation can penetrate much of the covering of dust that shrouds the object [2].
One of the bright young stars in NGC 6357, known as Pismis 24-1, was thought to be the most massive star known -- until it was found to actually be made up of at least three huge bright stars, each with a mass of under 100 times that of our Sun. Even so, these stars are still heavyweights -- some of the most massive in our Milky Way. Pismis 24-1 is the brightest object in the Pismis 24 star cluster, a bunch of stars that are all thought to have formed at the same time within NGC 6357.
VISTA is the largest and most powerful survey telescope ever built, and is dedicated to surveying the sky in infrared light. The VVV survey is scanning the central bulge and some of the plane of our galaxy to create a huge dataset that will help astronomers to discover more about the origin, early life, and structure of the Milky Way.
Parts of NGC 6357 have also been observed by the NASA/ESA Hubble Space Telescope (heic0619a - http://www.spacetelescope.org/images/heic0619a/) and ESO's Very Large Telescope (eso1226a - http://www.eso.org/public/images/eso1226a/). Both telescopes have produced visible-light images of various parts of this region -- comparing these images with this new infrared image above shows some striking differences. In the infrared the large plumes of red-hued material are much reduced, with tendrils of pale, purple gas stretching out from the nebula in different areas.
###
Notes
[1] The informal name of Lobster Nebula is also sometimes given to the spectacular star-forming region Messier 17 (eso0925 - http://www.eso.org/public/news/eso0925/), although that object is more often called the Omega Nebula.
[2] Infrared observations can reveal features that cannot be seen in visible-light pictures, for example because an object is too cold, obscured by thick dust, or is very distant, meaning that its light has been stretched towards the red end of the spectrum by the expansion of the Universe.
More information
ESO is the foremost intergovernmental astronomy organisation in Europe and the world's most productive ground-based astronomical observatory by far. It is supported by 15 countries: Austria, Belgium, Brazil, 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 two survey telescopes. VISTA works in the infrared and is the world's largest survey telescope and the VLT Survey Telescope is the largest telescope designed to exclusively survey the skies in visible light. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning the 39-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become "the world's biggest eye on the sky".
Links
Contacts
Richard Hook
ESO, La Silla, Paranal, E-ELT & Survey Telescopes Press Officer
Garching bei Mnchen, Germany
Tel: +49 89 3200 6655
Cell: +49 151 1537 3591
Email: rhook@eso.org
[ | E-mail | Share ] ?
AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert! system.
Source: http://www.eurekalert.org/pub_releases/2013-02/e-std021813.php
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