Sharpless 252 – Monkey Head Nebula

The Monkey Head Nebula is an open cluster embedded in a bright emission nebula in the constellation Orion, located about 7,270 light-years away, and reaches its annual culmination at astronomical midnight and is best observed late December.

The Monkey Head Nebula, also cataloged as NGC 2175, is an open star cluster wrapped in a glowing region of ionized hydrogen that makes it a rewarding target for wide-field astrophotography. With an apparent magnitude of 6.8, the cluster itself is bright, while the surrounding nebulosity rewards long exposures and narrowband filters that isolate the hydrogen-alpha signal. Its distinctive shape, reminiscent of a primate’s face, emerges most clearly in image stacks that reveal the sculpted pillars and dark lanes carved into the gas. Because the object spans a generous area of sky, short-to-medium focal lengths and camera sensors with a wide field are ideal for framing the full structure.

Names and Catalog numbers

  • Monkey Head Nebula
  • NGC 2175
  • Sh2-252 (Sharpless 252)
  • LBN 854
  • LBN 190.10+00.58

Position and the cosmic neighborhood

The Monkey Head Nebula lies in the constellation Orion at a right ascension of 06h 09m 39s and a declination of +20° 29′ 12″, placing it in the northern reaches of one of the winter sky’s richest regions. This part of Orion sits near the border with Gemini, in a stretch of the Milky Way dense with star-forming clouds and young stellar associations. For astrophotographers, its high declination keeps it well-placed for northern-hemisphere observers, and the surrounding field offers a colorful backdrop of stars and faint nebulosity that enriches any wide-field composition. The object is also known under designations including NGC 2175, Sh2-252, and LBN 854.

Nice to Know

  • Despite being classified as an open cluster, NGC 2175 is best known for the vivid emission nebula surrounding it, which gives the region its famous monkey-face appearance.
  • At magnitude 6.8, the cluster is bright enough to hint at in modest optics, yet the surrounding gas demands long exposures to fully reveal its detail.
  • The nebula carries multiple catalog identities, appearing as Sh2-252, LBN 854, and LBN 190.10+00.58 in addition to its NGC number.
  • Its location deep within the Milky Way band of Orion makes it a favorite subject for narrowband imaging, where hydrogen-alpha data brings out the sculpted pillars and dark structures.

Brightness, distance and size

The object has an apparent magnitude of 6.8 mag, it lies about 7,270 light-years from Earth.

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