File:2MASS Image of the Tarantula Nebula.jpg

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English: The Tarantula Nebula is one of the larger nebulae visible in the sky, which is a remarkable fact granted that it doesn't even lie within our own Galaxy! It is the dominant feature in our satellite galaxy the Large Magellanic Cloud (LMC), which is visible only from the Southern Hemisphere. This giant cloud is over 1000 light years across; if it were as close as the Orion Nebula, it would fill nearly half of the nighttime sky! It is one of the largest known star formation regions anywhere, and it's almost in our back yard.

At the core of the Tarantula nebula can be found the massive star cluster 30 Doradus, so compact that it was once thought to be a single supermassive star. The light from this cluster heats the surrounding gas, causing it to glow brightly.

This image mosaic covers a square region 40 arcminutes (2/3 of a degree) on a side, about the size of a pea held at arm's length. Some of the brighter stars in this image are local, foreground stars, while most of the fainter ones belong to the much more distant LMC. The clump of bright stars on the left side are one of many clusters recently formed in this region.
Date
Source http://www.ipac.caltech.edu/2mass/gallery/showcase/taran/index.html
Author 2MASS/T. Jarrett, R. Hurt

Copyright notice: http://www.ipac.caltech.edu/2mass/gallery/showcase/copyright.html

Licensing

Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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13 April 2003

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Date/TimeThumbnailDimensionsUserComment
current11:24, 8 May 2015Thumbnail for version as of 11:24, 8 May 20152,392 × 2,394 (1.23 MB)Jcpag2012cropped from the frame
19:16, 30 June 2011Thumbnail for version as of 19:16, 30 June 20112,500 × 2,550 (1.11 MB)Spitzersteph