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The central part of the Tarantula Nebula, including the massive star cluster R136 (above center), stands out in this mosaic of Hubble Space Telescope images.
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The biggest star-forming region in the local universe, the Tarantula Nebula also ranks among the most stunning sights astronomy.com said.
Northern Hemisphere skywatchers gush about the beauty of the Orion Nebula, a sight that warms observers' hearts during cold winter nights. Those who live in the Southern Hemisphere rave with even greater gusto about the intricate splendor of the Eta Carinae Nebula. Yet neither of these stellar nurseries, as spectacular as they are, come close to matching the Tarantula Nebula.
The Tarantula resides in the Large Magellanic Cloud (LMC), an irregular satellite galaxy to the Milky Way. While the Orion and Eta Carinae nebulae are a couple of thousand light-years away, the Tarantula is a whopping 170,000 light-years distant.
Yet, despite its great range, the Tarantula glows brightly enough to be seen with the naked eye. Observers in the Southern Hemisphere can glimpse it on the outskirts of the LMC, in the southeastern corner of the constellation Doradus.
The massive complex spans 1,000 light-years, making it the biggest stellar nursery in the local universe. In fact, if this huge network of stars, gas, and dust replaced the Orion Nebula, it would cover a quarter of the sky and shine so dazzlingly you could see it in daylight.
One of the two recently released images shows the nebula's tangled central regions as seen by the Amateur astronomer Danny LaCrue recently sifted through this data and found that 15 exposures taken with the telescope's Wide Field and Planetary Camera 2 could be combined into a dramatic mosaic.
LaCrue used the ESA/ESO/NASA Photoshop FITS Liberator, which he downloaded from the Spacetelescope.org web site, to work with the format of Hubble's images.
The mosaic reveals wispy tendrils of gas and dust interlaced with hot, luminous stars. Just above the image's center lies R136, a rich cluster of stars that formed from the dense gas cloud. The cluster contains hundreds of stars, some up to 100 times as massive as the Sun and with surface temperatures 10 times the Sun's.
Prodigious amounts of ultraviolet radiation from these stars ionize the surrounding gas, causing it to glow. The brightest patches of nebulosity extending from the cluster somewhat resemble the legs of a spider, hence the nebula's name.
The entangled filaments on the nebula's outskirts more closely resemble a spider's cobweb. This was the target for astronomers using the 2.2-meter telescope of the European Southern Observatory (ESO) in La Silla, Chile. They took an image of the northeastern corner of the Tarantula that extends into the more barren areas just beyond.
The red color in the ESO image results from excited hydrogen atoms, and the green is emission from oxygen atoms that have lost two electrons. The radiation from the hot stars in R136, which lies beyond the lower-right corner of the image, knocks off those electrons. Because the intensity of radiation rises closer to the cluster, the color turns more yellow there.