Contains:NGC 7822
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NGC7822-HA-Meade triplet-ASI 1600 MM-Pro, 




    

        Adel Kildeev
NGC7822-HA-Meade triplet-ASI 1600 MM-Pro

NGC7822-HA-Meade triplet-ASI 1600 MM-Pro

Technical card

Resolution: 4183x3335

Dates: July 12, 2018

Frames: Astronomik 12nm H-Alpha Ha: 3x600" (gain: 139.00) -18C bin 1x1

Integration: 0.5 hours

Darks: ~3

Flats: ~7

Avg. Moon age: 28.80 days

Avg. Moon phase: 0.60%

Astrometry.net job: 2142656

RA center: 0.804 degrees

DEC center: 67.156 degrees

Pixel scale: 1.630 arcsec/pixel

Orientation: 49.741 degrees

Field radius: 1.211 degrees

Locations: Home observatory, Toronto, Ontario, Canada

Data source: Backyard

Description

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, 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. Wikipedia (c)

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Starminer68
Adel Kildeev
License: None (All rights reserved)
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NGC7822-HA-Meade triplet-ASI 1600 MM-Pro, 




    

        Adel Kildeev

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Narrowband imaging
ZWO ASI1600MM