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Birthday · November 26, 2008

The Horsehead Nebula in Orion

November 26, 2008

In the time it took you to read this, the Earth moved another thousand miles through space. You are not standing still. You never have been.

The Horsehead Nebula in Orion

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APOD published November 26, 2008. Credit: Adam Block. A publication-date match, not a photo taken on your date. Independent of NASA.

Behind the image

The Horsehead Nebula in Orion

Original APOD · November 26, 2008

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. A blue reflection nebula dubbed NGC 2023 surrounds the bright star at the lower left. 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. Bright spots in the Horsehead Nebula's base are young stars just in the process of forming. Light takes about 1500 years to reach us from the Horsehead Nebula. The above image was taken earlier this month with a 0.6-meter telescope at the Mt. Lemmon SkyCenter in Arizona, USA.

Image credit: Adam Block

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