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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…
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nebula pipe barnard 59 65 67 also 78 milky way known dark ophiuchus constellation apparent stem ldn 1773 300 60
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Pipe Nebula | Absolute magnitude (V) | – | 1.00 | infobox |
| Pipe Nebula | Apparent dimensions (V) | Pipe Stem 300′ × 60′ Pipe Bowl 200′ × 140′ | 1.00 | infobox |
| Pipe Nebula | Apparent magnitude (V) | – | 1.00 | infobox |
| Pipe Nebula | Constellation | Ophiuchus | 1.00 | infobox |
| Pipe Nebula | Declination | −26° 56′ | 1.00 | infobox |
| Pipe Nebula | Designations | Barnard 59, 65–67, & 78; LDN 1773; LDN 42 | 1.00 | infobox |
| Pipe Nebula | Distance | 600 to 700 ly (180 to 220 pc) | 1.00 | infobox |
| Pipe Nebula | Notable features | – | 1.00 | infobox |
| Pipe Nebula | Radius | – ly | 1.00 | infobox |
| Pipe Nebula | Right ascension | 17h 27m | 1.00 | infobox |
| Pipe Nebula | related to Gallery | The Milky Way | 0.60 | section |
| Pipe Nebula | related to Gallery | Sagittarius | 0.60 | section |
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