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VISTA captures celestial cat's hidden secrets

The view of NGC 6334 in the infrared is strikingly different from that in visible light. With the dust obscuring the view far less, scientists can learn more about how these stars form and develop in their first few million years of life.
Provided by ESO, Garching, Germany
NGC 6334
VISTA's infrared view of the Cat's Paw Nebula.
ESO
April 21, 2010
The Cat's Paw Nebula (NGC 6334) is a huge stellar nursery, the birthplace of hundreds of massive stars. In a magnificent new European Southern Observatory's (ESO) image taken with the Visible and Infrared Survey Telescope for Astronomy (VISTA) at the Paranal Observatory in Chile, the glowing gas and dust clouds obscuring the view are penetrated by infrared light, and some of the Cat's hidden young stars are revealed.

Toward the heart of the Milky Way, 5,500 light-years from Earth in the constellation Scorpius the Scorpion, the Cat's Paw Nebula stretches across 50 light-years. In visible light, hot young stars, creating strange reddish shapes that give the object its nickname, illuminate gas and dust. A recent image by ESO's Wide Field Imager (WFI) at the La Silla Observatory captured this visible light view in great detail. NGC 6334 is one of the most active nurseries of massive stars in our galaxy.

VISTA, the latest addition to ESO's Paranal Observatory in the Chilean Atacama Desert, is the world's largest survey telescope. It works at infrared wavelengths, seeing right through much of the dust that is such a beautiful but distracting aspect of the nebula and revealing objects hidden from the sight of visible light telescopes. Visible light tends to be scattered and absorbed by interstellar dust, but the dust is nearly transparent to infrared light.

VISTA has a main mirror that is 4.1 meters across, and it is equipped with the largest infrared camera on any telescope. It shares the spectacular viewing conditions with ESO's Very Large Telescope (VLT), which is located on the nearby summit. With this powerful instrument at their command, astronomers were keen to see the birth pains of the big young stars in the Cat's Paw Nebula, some nearly 10 times the mass of the Sun. The view in the infrared is strikingly different from that in visible light. With the dust obscuring the view far less, they can learn more about how these stars form and develop in their first few million years of life. VISTA's wide field of view allows the whole star-forming region to be imaged in one shot with greater clarity than ever before.

The VISTA image is filled with countless stars of our Milky Way Galaxy overlaid with spectacular tendrils of dark dust that are seen here fully for the first time. The dust is sufficiently thick in places to block even the near-infrared radiation to which VISTA's camera is sensitive. In many of the dusty areas, such as those close to the center of the picture, features that appear orange are apparent — evidence of otherwise hidden active young stars and their accompanying jets. Further out, though, slightly older stars are laid bare to VISTA's vision, revealing the processes taking them from their first nuclear fusion along the unsteady path of the first few million years of their lives.

The VISTA telescope is now embarking on several big surveys of the southern sky that will take years to complete. The telescope's large mirror, high-quality images, sensitive camera, and huge field of view make it by far the most powerful infrared survey telescope on Earth. As this striking image shows, VISTA will keep astronomers busy analyzing data they could not have otherwise acquired.
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