NGC 6334, The Cat’s Paw Nebula image
This image of emission nebula NGC6334 (the Cat’s Paw Nebula), a star-forming region in the constellation Scorpius, was taken in 2007 using the Mosaic-2 imager on the Blanco 4-meter telescope at Cerro Tololo Inter-American Observatory. The colors of the nebula are reddened by intervening dust in the plane of the Milky Way galaxy. The image was taken as part of a continuing campaign of public-release images using both NOAO 4-meter telescopes. Credit: T.A. Rector/University of Alaska Anchorage, T. Abbott and NOIRLab/NSF/AURA

NGC 6334 is one of the most active areas of massive star formation in our galaxy. The nebula hides newly formed bright blue stars, each of which has a mass nearly ten times that of our Sun and was born within the last few million years. While theoretically visible from Italy, where I live, these are a classic deep-sky pair in the Southern Hemisphere. In this shot, taken remotely from Chile, they were at zenith in the best possible conditions to capture their details and those of the Milky Way centre clouds surrounding them.

Looking rather like a cosmic feline foot protruding outwards from among the stars, NGC 6334 is also known as the Cat’s Paw Nebula or the Bear Claw Nebula, making it one of many Nebulae That Look Like Animals.

NGC 6334 may contain tens of thousands of stars, many of them concealed deep within the nebula’s dust. The nebula also contains a vast supply of material needed for star formation, roughly equal to a mass of 200,000 Suns.

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