Great Rift (astronomy)

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Image of the Great Rift - a dusty lane that stretches from the constellation Cygnus to Sagittarius.

In astronomy, the Great Rift (sometimes called the Dark Side, Dark Rift, or, less commonly, Dark River) is a series of overlapping, non-luminous, molecular dust clouds that are located between the Solar System and the Sagittarius Arm of the Milky Way Galaxy at a distance of about 100 parsecs or about 300 light years (2×1015 miles or 3×1015 kilometers) from Earth. The clouds are estimated to contain about 1 million solar masses of plasma and dust.[1]

Properties[edit]

To the naked eye, the Great Rift appears as a dark lane that divides the bright band of the Milky Way lengthwise, through about one-third of its extent, and is flanked by lanes of numerous stars.[1]

Starting at the constellation of Cygnus, where it is known as the Cygnus Rift or Northern Coalsack, the Great Rift stretches to Aquila; to Ophiuchus, where it broadens out; to Sagittarius, where it obscures the Galactic Center; and finally to Centaurus. One of the most important regions it obscures is the Cygnus OB2 association, a large cluster of young stars and one of the largest regions of star formation near Earth. A similar dark band can be seen in edge-on distant galaxies, such as NGC 891 in Andromeda.[2]

Gallery[edit]

See also[edit]

Notes[edit]

  1. ^ a b Great Rift: Dark area in the Milky Way 2010 EarthSky Communications. Accessed June 2010
  2. ^ Pitts, Sam. "NGC 891 Edge on Galaxy (HV19)". Sams Astro. Retrieved 2009-04-25. 

References[edit]