Sh2-155 · Cave Nebula
| Chinese name | 洞穴星云 |
|---|---|
| Type | Emission nebula |
| Constellation | Cep |
| RA | 22h57m |
| Dec | +62° |
| Apparent magnitude | 7.7ᵐ |
| Hemisphere | Northern |
| Best season | Autumn |
| Difficulty | Moderate |
| Focal length | 中长焦 800–1200mm |
About
The Cave Nebula (Sh2-155) lies about 2,400 light-years away in Cepheus, named for a curved dark dust band that frames a cave-like opening against bright red hydrogen gas. Sitting on the edge of the large Cepheus B molecular cloud, it is an active H II star-forming region whose bright rim is an ionization front excited by radiation from nearby hot stars, with young stars and protostars embedded within. The nebula combines red emission and blue reflection components, rich in color and layered structure. Of relatively low surface brightness, it suits medium-to-long focal narrowband exposures, making it a rewarding autumn Cepheus target.