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Sh2-155 Cave Nebula in the Hubble Palette, 





    
        

            Douglas J Struble
Sh2-155 Cave Nebula in the Hubble Palette

Sh2-155 Cave Nebula in the Hubble Palette

Technical card

Resolution: 6000x4800

Dates:Aug. 16, 2016Aug. 13, 2017Aug. 17, 2017July 10, 2018July 14, 2018July 17, 2018

Frames:
Astrodon Ha 5nm: 96x240" (gain: 139.00) -20C bin 1x1
Astrodon Ha 5nm: 111x120" (gain: 201.00) -20C bin 1x1
Astrodon OIII 3nm: 142x240" (gain: 139.00) -20C bin 1x1
Astrodon OIII 3nm: 325x120" (gain: 201.00) -20C bin 1x1
Astrodon SII 3nm: 61x240" (gain: 139.00) -20C bin 1x1
Astrodon SII 3nm: 132x120" (gain: 201.00) -20C bin 1x1

Integration: 38.9 hours

Darks: ~50

Flats: ~50

Bias: ~250

Avg. Moon age: 15.20 days

Avg. Moon phase: 37.44%

Bortle Dark-Sky Scale: 6.67

Astrometry.net job: 2157262

RA center: 344.430 degrees

DEC center: 62.627 degrees

Pixel scale: 0.358 arcsec/pixel

Orientation: 20.734 degrees

Field radius: 0.382 degrees

Locations: Backyard Red Zone Observatory, Taylor, MI, Michigan, United States

Data source: Backyard

Description

Sh2-155 (also designated Sharpless 155 or S155) is a diffuse nebula in the constellation Cepheus, within a larger nebula complex containing emission, reflection, and dark nebulosity. It is widely known as the Cave Nebula, though that name was applied earlier to Ced 201, a different nebula in Cepheus. Sh2-155 is an ionized H II region with ongoing star formation activity, at an estimated distance of 725 parsecs (2400 light-years) from Earth.

Sh2-155 was first noted as a galactic emission nebula in 1959 in the extended second edition of the Sharpless catalogue, being a part of the much larger Cep OB3 Association. Although Sh2-155 is relatively faint for amateur observation, some of its structure may be seen visually through a moderately sized telescope under dark skies.

Sh2-155 lies at the edge of the Cepheus B cloud (part of the Cepheus molecular cloud), and is ionized by young stars from the Cep OB3 association. It has been suggested that radiation from the hot O-type star HD 217086 is compressing the region, triggering the formation of a new generation of stars. A study of the region's young stellar objects by the Chandra X-ray Observatory and Spitzer Space Telescope shows a progression of stellar ages in front of the cloud, supporting the hypothesis of triggered star-formation.

Comments

Author

dugstruble
Douglas J Struble
License: None (All rights reserved)
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Revisions

  • Sh2-155 Cave Nebula in the Hubble Palette, 





    
        

            Douglas J Struble
    Original
  • Final
    Sh2-155 Cave Nebula in the Hubble Palette, 





    
        

            Douglas J Struble
    B

Sky plot

Sky plot

Histogram

Sh2-155 Cave Nebula in the Hubble Palette, 





    
        

            Douglas J Struble