Pipe Nebula (Darius Kopriva)

Celestial hemisphere: Southern · Constellation: Ophiuchus (Oph) · Contains: 3 Sgr · 39 Oph A · 39 Oph B · 42 Oph) · 44 Oph · 51 Oph · The star 2 Sgr · The star 38 Oph · The star Garafsa (θ Oph · The star b Oph · The star c Oph · The star ο Oph A · The star ο Oph B

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Pipe Nebula

Revision title: High Resolution

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Pipe Nebula

Revision title: High Resolution

This is a 4 panel mosaic of the Pipe Nebula. All 4 panels have an exposure time of about 5 hours.

The Pipe Nebula (also known as Barnard 59, 65–67, and 78) is a dark nebula in the Ophiuchus constellation and a part of the Dark Horse Nebula. It is a large but readily apparent smoking pipe-shaped dust lane that obscures the Milky Way star clouds behind it. Clearly visible to the naked eye in the Southern United States under clear dark skies, but it is best viewed with 7× binoculars.

The nebula has two main parts: the Pipe Stem with an opacity of 6 which is composed of Barnard 59, 65, 66, and 67 (also known as LDN 1773)

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Title: High Resolution

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Southern Hemisphere Astro

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Astrometry.net job	5953960
PixInsight job	25M8CKTNDJHRF17VTCC2RXS6CAC4J7J8
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PixInsight stage	PLATE_SOLVING_IMAGE

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Pipe Nebula

Revision title: High Resolution

Pipe Nebula

Revision title: High Resolution

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Pipe Nebula

Revision title: High Resolution

Pipe Nebula

Revision title: High Resolution

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