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Contains:  NGC 7762, NGC 7822
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Ced 214 / NGC 7822, 


            Steven Bellavia
Ced 214 / NGC 7822

Ced 214 / NGC 7822

Technical card

Resolution: 3600x4800

Dates:Sept. 19, 2019

Astronomik 6nm OIII: 24x300" (gain: 120.00) -15C bin 1x1
Optolong 7nm Ha 2": 32x300" (gain: 120.00) -15C bin 1x1

Integration: 4.7 hours

Darks: ~30

Flats: ~30

Flat darks: ~30

Avg. Moon age: 19.61 days

Avg. Moon phase: 75.73%

Bortle Dark-Sky Scale: 4.00

Mean SQM: 20.40

Mean FWHM: 5.50

Temperature: 12.00 job: 2931036

RA center: 23h 59' 37"

DEC center: +67° 38' 16"

Pixel scale: 1.994 arcsec/pixel

Orientation: 355.190 degrees

Field radius: 1.661

Data source: Backyard


NGC 7822 and Cederblad 214 (Sh2-171) form a large molecular cloud and star forming region in the constellation of Cepheus. This is the center of the "Cosmic Question Mark". NGC 7822 forms the faint northern arch at the top of the image, while Cederblad 214 is the brighter nebula towards the bottom. This field of view is filled with a multitude of young stars born from the hydrogen gas in the cloud. These young stars also form several clusters within the nebula. The cluster Berkeley 59 is located at the heart of Cederblad 214, while NGC 7762 is towards the upper right of the ring.
Within Cederblad 214 is one of the hottest known stars in our stellar neighborhood. With a temperature of almost 45,000 degrees Kelvin, BD+66 1673 is over 100,000 times more luminous than our own Sun. Also contained within Cederblad 214 are numerous Bok globules - areas of of condensing gas from which young protostars are created.



Steven Bellavia
License: None (All rights reserved)

Sky plot

Sky plot


Ced 214 / NGC 7822, 


            Steven Bellavia