One of the most identifiable nebulae in the sky, the Horsehead Nebula in Orion, is part of a large, dark, molecular cloud. Also known as Barnard 33, the unusual shape was first discovered on a photographic plate in the late 1800s. The red glow originates from hydrogen gas predominantly behind the nebula, ionized by the nearby bright star Sigma Orionis. The darkness of the Horsehead is caused mostly by thick dust, although the lower part of the Horsehead's neck casts a shadow to the left. Streams of gas leaving the nebula are funneled by a strong magnetic field. The featured image was taken with the large 3.6-m Canada-France-Hawaii Telescope in Hawaii, USA.
The Horsehead Nebula Newsletter
By Staff | Last Modified on: 2018-04-11 10:05:01 | Hits: 74