Uwe Glahn
September 7th, 2020, 07:33 PM
IC 5146 = LBN 424 = Sh 2-125
Cons: Cygnus
RA: 21 53 29
Dec: +47 16 01
Size: 12'
The history of our OOTW started 1893/1894 when Max Wolf and E.E. Barnard discovered this nebula independently on a photo plate (a 6" lens each). Our expert contributor Steve G. brings more light in the history in a thread here in 2015 (http://www.deepskyforum.com/showthread.php?759-About-the-name-Cocoon-Nebula).
The "special feature" here is its galactic position within a massive molecular cloud. The strong star formation makes the nebula not unique but interesting for visual observer. That means we can observe a central Open Star Cluster (Cr 470) surrounded by a nebula (Cocoon) which shows signs of emission, refection and absorption. As a nice addition, especially for smaller aperture we find the large Dark Nebula Barnard 168
Physically the distance of the whole complex is around 3000ly away. High resolution spectral analyses let the nebula classify in a crossover stadium between a reflection and emission case. The central star cluster consists of around 100 young stars up to 12mag.
Most easiest detail in telescopes or even smaller binoculars is the long dark structure B 168 which can be seen as a thin, nearly 2° long streak. The Cocoon is much more difficult and even mid size telescopes can have trouble with it when the sky is not transparent enough. Best filters are UHC and Hß.
photo of IC 5146 + B 168 by Fabian Neyer (larger (http://www.starpointing.com/ccd/cocoonlarge1.html))
3995
sketch of IC 5146: 27", 113x, Hß, NELM 6m5+
3996
As always, give it a go and let us know.
Cons: Cygnus
RA: 21 53 29
Dec: +47 16 01
Size: 12'
The history of our OOTW started 1893/1894 when Max Wolf and E.E. Barnard discovered this nebula independently on a photo plate (a 6" lens each). Our expert contributor Steve G. brings more light in the history in a thread here in 2015 (http://www.deepskyforum.com/showthread.php?759-About-the-name-Cocoon-Nebula).
The "special feature" here is its galactic position within a massive molecular cloud. The strong star formation makes the nebula not unique but interesting for visual observer. That means we can observe a central Open Star Cluster (Cr 470) surrounded by a nebula (Cocoon) which shows signs of emission, refection and absorption. As a nice addition, especially for smaller aperture we find the large Dark Nebula Barnard 168
Physically the distance of the whole complex is around 3000ly away. High resolution spectral analyses let the nebula classify in a crossover stadium between a reflection and emission case. The central star cluster consists of around 100 young stars up to 12mag.
Most easiest detail in telescopes or even smaller binoculars is the long dark structure B 168 which can be seen as a thin, nearly 2° long streak. The Cocoon is much more difficult and even mid size telescopes can have trouble with it when the sky is not transparent enough. Best filters are UHC and Hß.
photo of IC 5146 + B 168 by Fabian Neyer (larger (http://www.starpointing.com/ccd/cocoonlarge1.html))
3995
sketch of IC 5146: 27", 113x, Hß, NELM 6m5+
3996
As always, give it a go and let us know.