Cookie consent

AstroBin saves small pieces of text information (cookies) on your device in order to deliver better content and for statistical purposes. You can disable the usage of cookies by changing the settings of your browser. By browsing AstroBin without changing the browser settings, you grant us permission to store that information on your device.

I agree
Contains:  The star εCha, The star πCha, The star δ2Cha, The star δ1Cha, The star γCha
Getting plate-solving status, please wait...
Mosaic out of 6 images - Molecular Clouds in the Central part of Constellation Chameleon., 





    
        

            oldwexi
Mosaic out of 6 images - Molecular Clouds in the Central part of Constellation Chameleon.

Mosaic out of 6 images - Molecular Clouds in the Central part of Constellation Chameleon.

Technical card

Imaging camera:SBIG ST11000 ST11K

Mount:Paramount-ME Paramount ME

Guiding telescope or lens:Takahashi FSQ-106N Tak 106

Guiding camera:SBIG ST11000 ST11K

Software:PixInsight

Filters:BlueGreenRed

Resolution: 2376x2587

Dates:March 27, 2015

Frames: 190x300"

Integration: 15.8 hours

Avg. Moon age: 7.55 days

Avg. Moon phase: 51.73%

Astrometry.net job: 1476455

RA center: 170.556 degrees

DEC center: -78.355 degrees

Pixel scale: 7.003 arcsec/pixel

Orientation: -177.794 degrees

Field radius: 3.416 degrees

Locations: SidingSprings Itelescope Farm, Siding Springs, Australia

Data source: Amateur hosting facility

Remote source: iTelescope

Description

Mosaic out of 5 images - Molecular Clouds in Constellation Chameleon

The southern constellation of Chamaeleon (at a distance of ∼160 - 180 pc) contains one of the nearest groups of dark clouds.
There are 3 main complexes. Cha I, Cha II and Cha III.
This mosaic shows in the upper right corner the dark cloud complex
Chameleon I, which extends down to the lower left where it reaches the
border of dark cloud complex Chameleon III which i show in another picture
in my gallery of astrobin.

The "Chamaeleon I" complex is a place of young low mass stars, resulting in various reflection nebulae - IC 2631, and the blue nebula Ced 111 and the white reflection nebula Ced 110.
The obscuring mass of thick brown dust in the upper right region absorbs the blue light of distant stars making them appear much redder than they actually are. This process of interstellar reddening also changes the light of galaxies behind, reducing the blue light of these distant galaxies.

Image Details:
Resolution ........ 8.665 arcsec/pix
Rotation .......... 2.434 deg
Focal ............. 530.27 mm
Pixel size ........ 22.27 um
Field of view ..... 4d 37' 16.0" x 5d 1' 57.6"
Image center ...... RA: 11 22 14.263 Dec: -78 21 16.57
Image bounds:
top-left ....... RA: 12 01 35.174 Dec: -75 44 18.08
top-right ...... RA: 10 46 48.203 Dec: -75 34 47.01
bottom-left .... RA: 12 17 10.083 Dec: -80 42 11.57
bottom-right ... RA: 10 23 22.726 Dec: -80 27 43.93

Exposures:
Using a SBIG ST11K on a Takahashy FSQ 106 with 530 mm focal length on a Paramount ME mount.

All images were exposed remotely on the T12 of Siding Spring iTelescop Farm.
During 2015 and 2016

Comments

Author

oldwexi
oldwexi
License: None (All rights reserved)
2364
Like

Sky plot

Sky plot

Histogram

Mosaic out of 6 images - Molecular Clouds in the Central part of Constellation Chameleon., 





    
        

            oldwexi