Barnard 72 “ Snake Nebula”
Ophiuchus · 9 - 29 / 7/2013 · Takahashi FSQ ED
About the target
The Snake Nebula (also known as Barnard 72) is a dark nebula (opens in a new tab) in the Ophiuchus constellation (opens in a new tab). It is a small but readily apparent S-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 (opens in a new tab). 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 (opens in a new tab).
To the right side of the Snake Nebula is found Barnard 68 (opens in a new tab). Below it are found Barnard 69, Barnard 70, and Barnard 74.
Text from Wikipedia.
© Nikos Paschalis
Observing log
- Object
- Barnard 72 - Snake Nebula
- Constellation
- Ophiuchus
- Distance + Ap. Magnitude
- 650 Light Years - 6.5
- Date + Time
- 9 - 29 / 7/2013
- Location
- Remote imaging from iTelescope.net - Sliding spring Australia
- Optics
- Takahashi FSQ ED
- Tools
- ACP
- Camera
- SBIG STL 11000M
- Exposure Time
- LRGB: L= 18X300 sec -RGB 6 X 600 (each)
- More Details
- Environment Temperature: ---- Camera Temperature -30 °C
- Mount
- Paramount ME
- Guiding
- Off axis guided
- Processing Details
- Photoshop, Maxim, CCDsoft
- Notes
- Weather: - - Transparence: - - Humidity: - -
