Celestial hemisphere:  Northern  ·  Constellation: Cepheus (Cep)  ·  Contains:  HD216102  ·  HD216380  ·  HD216425  ·  HD216532  ·  HD216629  ·  HD216658  ·  HD216711  ·  HD216898  ·  HD216926  ·  HD217035  ·  HD217061  ·  HD217086  ·  HD217099  ·  HD217297  ·  HD217312  ·  HD217463  ·  HD217657  ·  HD217730  ·  HD217872  ·  HD217966  ·  LBN 524  ·  LBN 527  ·  LBN 529  ·  LDN 1215  ·  LDN 1216  ·  LDN 1218  ·  LDN 1220  ·  PK110+01.1  ·  Sh2-155
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Caldwell 9 / SH2-155, Joe Matthews
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Caldwell 9 / SH2-155

Getting plate-solving status, please wait...
Caldwell 9 / SH2-155, Joe Matthews
Powered byPixInsight

Caldwell 9 / SH2-155

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Description

Last night was another good night for imaging, so I decided to try and get in two targets, both of which I haven't imaged before, Caldwell 9 or SH2-155 was my second image which I started at 01:30 and finished at 04:00.  I am going to try and do better with this image on the next clear night.

Sh2-155 (also designated Caldwell 9, 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 starHD 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

The name "Cave Nebula" was coined for this object by Patrick Moore, presumably derived from photographic images showing a curved arc of emission nebulosity corresponding to a cave mouth. The name was also used earlier to refer to another brighter but unrelated reflection nebula in Cepheus known as Ced 201  or VdB 152,  positioned at R.A.: 22h 13m 27s Dec.: +70° 15′ 18″ (2000). The name's application to Sh2-155 has come into vogue through the nebula's inclusion in Moore's Caldwell catalogue  as object Caldwell 9. (SIMBAD lists the name for Ced 201, but not for Sh2-155.)
@information from Wikipedia

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