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Tarantula Nebula (NGC 2070) in the river bream - The Tarantula Nebula, around the 30...

Tarantula Nebula (NGC 2070) in the river bream - The Tarantula Nebula, around the 30 Dor cluster - The Tarantu
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Medium 819 × 1024 px 69 × 87 mm 1.5 MB

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IMAGE number
PIX4618255
Image title
Tarantula Nebula (NGC 2070) in the river bream - The Tarantula Nebula, around the 30 Dor cluster - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Image obtained with Siding Spring's 3.9m telescope. This object is the only extra - galactic nebula which can be seen with the unaided eye. It is a faint patch of light at the eastern end of the Large Magellanic Cloud, 170,000 light years distant. A small telescope reveals narrow spindly tendrils of glowing gas which have been likened to the legs of a spider. The 'body' of the spider is the bright nebula seen at the centre of the photograph, while at its core is an extremely dense clump of very hot stars, until recently thought to a single, unusually massive star known as 30 Doradus. The very hot stars of 30 Dor are responsible for making the nebula visible
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Image description

Tarantula Nebula (NGC 2070) in the river bream - The Tarantula Nebula, around the 30 Dor cluster - The Tarantula Nebula (or 30 Bream) is the largest star-forming region of the Great Magellan Cloud. It is located 170,000 light years ago in the constellation Dorado (southern hemisphere). At the center of this nebula, the open cluster of R136 stars, clusters of hot and massive stars. Image obtained with Siding Spring's 3.9m telescope. This object is the only extra - galactic nebula which can be seen with the unaided eye. It is a faint patch of light at the eastern end of the Large Magellanic Cloud, 170,000 light years distant. A small telescope reveals narrow spindly tendrils of glowing gas which have been likened to the legs of a spider. The 'body' of the spider is the bright nebula seen at the centre of the photograph, while at its core is an extremely dense clump of very hot stars, until recently thought to a single, unusually massive star known as 30 Doradus. The very hot stars of 30 Dor are responsible for making the nebula visible

Photo credit
Photo © Anglo-Australian Observatory/David Malin Images/Novapix / Bridgeman Images
Image keywords
astronomy / star / astronomy / photography / aao / 1984 / dorado / sea bream / r136 / mail / star / star cluster / Novapix / star cluster / astronomy / Open Clusters / South Hemisphere / Open Cluster / southern hemisphere / Large Magellan Cloud / large magellanic cloud / Young Star / Massive Star / Massive Star / Young Star / star formation / Star Training / nebula / nebula / Diffused Nebula / Broadcast Nebula / Ngc 2070 / tarantula / 30 doradus / Tarentula

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