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Eagle Nebula (IC 4703) and M16 star cluster in Snake - The Eagle nebula in...

Eagle Nebula (IC 4703) and M16 star cluster in Snake - The Eagle nebula in Serpens - Eagle Nebula (IC 4703) an
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Medium 1024 × 695 px 87 × 59 mm 1.0 MB

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IMAGE number
PIX4620009
Image title
Eagle Nebula (IC 4703) and M16 star cluster in Snake - The Eagle nebula in Serpens - Eagle Nebula (IC 4703) and M16 star cluster in Snake. The M16 star cluster is a cluster of young stars distant from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. These stars are much warmer than the Sun and can be 30 times more massive. Image obtained with a telescope 61 cm in diameter. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are often associated recent star formation. This example is about 7000 light years distant. Image taken with a 24 - inch telescope
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Eagle Nebula (IC 4703) and M16 star cluster in Snake - The Eagle nebula in Serpens - Eagle Nebula (IC 4703) and M16 star cluster in Snake. The M16 star cluster is a cluster of young stars distant from 7000 years - light, formed about 2 million years ago in the Eagle nebula, IC 4703. These stars are much warmer than the Sun and can be 30 times more massive. Image obtained with a telescope 61 cm in diameter. Messier 16 is a cluster of young stars which formed about 2 million years ago from the gas and dust which still surrounds them. Brilliant blue stars of this type are much hotter than the Sun and can be up to thirty times more massive. The dark intrusions visible across the face of the nebula are condensations of dusty material which might one day collapse into yet more stars, should they survive the radiation from the bright stars, which is gradually etching them away. Bright red regions of photo - ionised hydrogen such as M16 are usually found in the spiral arms of galaxies and are often associated recent star formation. This example is about 7000 light years distant. Image taken with a 24 - inch telescope

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Photo © MLSC/Univ.of Arizona/Novapix / Bridgeman Images
Image keywords
astronomy / snake / reptile / animal / 2008 / snake / eagle / star / astronomy / photography / snakes / star / star cluster / Novapix / star cluster / astronomy / Open Clusters / Open Cluster / star formation / Star Training / nebula / Emission Nebula / Nebula emission / nebula / Diffused Nebula / Broadcast Nebula / eagle

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