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Great Attractor - Wikipedia, the free encyclopedia

Great Attractor

From Wikipedia, the free encyclopedia

An image taken by the European Southern Observatory looking in the direction of the Great Attractor.
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An image taken by the European Southern Observatory looking in the direction of the Great Attractor.

The Great Attractor is a gravity anomaly in intergalactic space within the range of the Centaurus Supercluster which reveals the existence of a localised concentration of mass equivalent to tens of thousands of galaxies, observable by its effect on the motion of galaxies over a region hundreds of millions of light years across.

These galaxies are all redshifted, in accordance with the Hubble Flow, indicating that they are receding relative to us and to each other, but the variations in their redshift are sufficient to reveal the existence of the anomaly.

The phenomenon was first discovered in 1986 and lies at a distance of somewhere between 150 million and 250 million light years (the latter being the most recent estimate) from the Milky Way, in the direction of the Hydra and Centaurus constellations. That region of space is dominated by the Norma cluster (ACO 3627)[1], a massive cluster of galaxies, and contains a preponderance of large, old galaxies, many of which are colliding with their neighbours, and/or radiating large amounts of radio waves.

Attempts to further study the Great Attractor and other phenomena are hampered due to line of sight obstruction by its location in the zone of avoidance (the part of the night sky obscured by the Milky Way galaxy).

[edit] The Great Attractor in fiction

[edit] References

  1. ^ R. C. Kraan-Korteweg, in Lecture Notes in Physics 556, edited by D. Pageand J.G. Hirsch, p. 301 (Springer, Berlin, 2000).

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