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: - -