| Abell 1689 | |
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The yellow galaxies in this image belong to the cluster itself, however, the red and blue distorted streaks are background galaxies gravitationally lensed by the cluster. Some of the lensed galaxies are over 13 billion light years (4000 megaparsec) distant. The lensing zone itself is 2 million light years (0.60 megaparsec) across.
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| Observation data (Epoch J2000) | |
| Constellation(s) | Virgo |
| Right ascension | 13h 11m 34.2s[1] |
| Declination | -01° 21′ 56″ |
| Richness class | 4[2] |
| Bautz-Morgan type | II-III[2] |
| Redshift | 0.1832[1] |
| Distance (co-moving) |
754 Mpc (2,459 Mly) h−1 0.705 [1] |
| X-ray flux | (14.729 ± 8.1%)×10−11 erg s-1 cm-2 (0.1—2.4 keV)[1] |
| See also: Galaxy groups and clusters, List of galaxy clusters | |
Abell 1689 is a galaxy cluster in the constellation Virgo. It is one of the biggest and most massive galaxy clusters known and acts as a gravitational lens, distorting the images of galaxies that lie behind it.[3]
As of February 2008, one of the lensed galaxies, A1689-zD1, was the most distant galaxy found.[4][5]
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Coordinates:
13h 11m 34.2s, −01° 21′ 56″
| Astronomical catalogs | ||
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| Abell: | Abell 1684 - Abell 1685 - Abell 1686 - Abell 1687 - Abell 1688 - Abell 1689 - Abell 1690 - Abell 1691 - Abell 1692 - Abell 1693 - Abell 1694 | |
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