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
Imaging telescope or lens:Teleskop Service TS Photoline 107mm f/6.5 Super-Apo
Imaging camera:ZWO ASI1600MM-Cool
Guiding telescope or lens:Celestron OAG Deluxe
Guiding camera:QHYCCD QHY5III174
Focal reducer:Riccardi Reducer/Flattener 0.75x
Filters:Baader Planetarium Ha 1.25" 7nm , Baader Planetarium OIII 1.25" 8.5nm , Astrodon O-III 36mm - 5nm , Astrodon S-II 36mm - 5nm , Astrodon R Gen.2 E-series 36mm , Astrodon G Gen.2 E-series 36mm , Astrodon B Gen.2 E-series 36mm , Astrodon HA 36mm - 5nm , Baader Planetarium SII 1.25" 8nm
Astrodon B Gen.2 E-series 36mm: 15x5" (gain: 200.00) -20C bin 1x1
Astrodon G Gen.2 E-series 36mm: 15x5" (gain: 200.00) -20C bin 1x1
Astrodon HA 36mm - 5nm: 56x300" (gain: 200.00) -20C bin 1x1
Baader Planetarium Ha 1.25" 7nm: 50x120" (gain: 200.00) -20C bin 1x1
Baader Planetarium Ha 1.25" 7nm: 25x180" (gain: 200.00) -20C bin 1x1
Astrodon O-III 36mm - 5nm: 21x300" (gain: 200.00) -20C bin 1x1
Baader Planetarium OIII 1.25" 8.5nm: 17x120" (gain: 200.00) -20C bin 1x1
Astrodon R Gen.2 E-series 36mm: 15x5" (gain: 200.00) -20C bin 1x1
Astrodon S-II 36mm - 5nm: 15x300" (gain: 200.00) -20C bin 1x1
Baader Planetarium SII 1.25" 8nm: 16x180" (gain: 200.00) -20C bin 1x1
Integration: 12.0 hours
Avg. Moon age: 16.28 days
Avg. Moon phase: 73.22%
Astrometry.net job: 2281894
RA center: 0h 3' 35"
DEC center: +67° 8' 52"
Pixel scale: 2.931 arcsec/pixel
Orientation: -0.883 degrees
Field radius: 1.155 degrees
Locations: Berga Resort, Berga, Barcelona, Spain
Data source: Backyard
NGC 7822 is a young star forming complex in the constellation of Cepheus.
The complex encompasses the emission region designated Sharpless 171, and the young cluster of stars named Berkeley 59.
The complex is believed to be some 800-1000 pc distant (3,000 light years), with the younger components aged no more than a few million years.
The complex also includes one of the hottest stars discovered within 1 kpc of the Sun, namely BD+66 1673, which is an eclipsing binary system consisting of an O5V that exhibits a surface temperature of nearly 45000 K and a luminosity ~100,000 times that of the Sun.
The star is one of the primary sources illuminating the nebula and shaping the complex's famed pillars of creation-type formations, the elephant trunks.
(Description credits: Wikipedia)
|You have no new notifications.|
This page or operation is not available at the moment, because AstroBin is in READ ONLY mode. For more information, please check out our Twitter feed: https://twitter.com/AstroBin_com
This feature is only offered at higher membership levels.
Would you be interested in upgrading? AstroBin is a very small business and your support would mean a lot!
Such limitation improves the website as a whole by discouraging people from creating fake accounts to like their own images. Thank you for understanding!
Currently, your AstroBin index is 0.00.