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VLT takes most detailed infrared image of the Carina Nebula

This nebula is a perfect laboratory for astronomers studying the violent births and early lives of stars.
RELATED TOPICS: STARS | NEBULAE | VERY LARGE TELESCOPE
Carina-Nebula
This broad panorama of the Carina Nebula, a region of massive star formation in the southern skies, was taken in infrared light using the HAWK-I camera on ESO’s Very Large Telescope. Many previously hidden features, scattered across a spectacular celestial landscape of gas, dust and young stars, have emerged. Credit: ESO/T. Preibisch
Deep in the heart of the southern Milky Way lies a stellar nursery called the Carina Nebula. It is about 7,500 light-years from Earth in the constellation Carina the Keel. This cloud of glowing gas and dust is one of the closest incubators of massive stars to Earth and includes several of the brightest and heaviest stars known. One of them, the mysterious and highly unstable star Eta (η) Carinae, was the second brightest star in the entire night sky for several years in the 1840s, and it is likely to explode as a supernova in the near future — by astronomical standards. The Carina Nebula is a perfect laboratory for astronomers studying the violent births and early lives of stars.

Although this nebula is spectacular in normal visible-light pictures, many of its secrets are hidden behind thick clouds of dust. To penetrate this veil, a European team of astronomers led by Thomas Preibisch from the University Observatory in Munich, Germany, has used the power of the European Southern Observatory’s (ESO) Very Large Telescope (VLT) along with an infrared-sensitive camera called HAWK-I. Hundreds of individual images have been combined to create this picture, which is the most detailed infrared mosaic of the nebula ever taken and one of the most dramatic images ever created by the VLT. It shows not only the brilliant massive stars, but also hundreds of thousands of much fainter stars that were previously invisible.

The dazzling star Eta Carinae itself appears at the lower left of the new picture. It is surrounded by clouds of gas that are glowing under the onslaught of fierce ultraviolet radiation. Across the image, there are also many compact blobs of dark material that remain opaque even in the infrared. These are the dusty cocoons in which new stars are forming.

Over the past few million years, this region of the sky has formed large numbers of stars both individually and in clusters. The bright star cluster close to the center of the picture is called Trumpler 14. Although this object is seen well in visible light, many more fainter stars can be seen in this infrared view. And toward the left side of the image, a small concentration of stars that appear yellow can be seen. This grouping was seen for the first time in this new data from the VLT — these stars cannot be seen in visible light at all. This is just one of many new objects revealed for the first time in this spectacular panorama.

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