Celestial hemisphere:  Southern  ·  Constellation: Ophiuchus (Oph)  ·  Contains:  13.76  ·  39 Oph A  ·  39 Oph B  ·  39 omi Oph  ·  44 Oph  ·  44 b Oph  ·  51 Oph  ·  51 c Oph  ·  914 Palisana  ·  B253  ·  B255  ·  B261  ·  B262  ·  B269  ·  B68  ·  B69  ·  B70  ·  B71  ·  B72  ·  B73  ·  B74  ·  B76  ·  B77  ·  HD155804  ·  HD155831  ·  HD156025  ·  HD156080  ·  HD156182  ·  HD156183  ·  HD156197  ·  And 97 more.
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Snake Nebula, Darius Kopriva
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Snake Nebula

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Snake Nebula, Darius Kopriva
Powered byPixInsight

Snake Nebula

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Description

The Snake Nebula (also known as Barnard 72) is a dark nebula in the Ophiuchus constellation. It is a small but readily apparent SP-shaped dust lane that snakes out in front of the Milky Way star clouds from the north-north-west edge of the bowl of the Pipe Nebula. Its thickness runs between 2′ and 3′ and runs around 6′ in the north-west / south-east orientation. A good view in a 4" to 6" telescope requires clear dark skies.

It is part of the much larger Dark Horse Nebula.

To the right of the Snake Nebula is Barnard 68. Below it is Barnard 69, Barnard 70, and Barnard 74.

A dark nebula or absorption nebula is a type of interstellar cloud, particularly molecular clouds, that is so dense that it obscures the visible wavelengths of light from objects behind it, such as background stars and emission or reflection nebulae. The extinction of the light is caused by interstellar dust grains located in the coldest, densest parts of molecular clouds. Clusters and large complexes of dark nebulae are associated with Giant Molecular Clouds. Isolated small dark nebulae are called Bok globules. Like other interstellar dust or material, things it obscures are only visible using radio waves in radio astronomy or infrared in infrared astronomy.

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Snake Nebula, Darius Kopriva

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Southern Hemisphere Astro