| Abell 1689 | |
|---|---|
| Hubble view of galaxy cluster Abell 1689. It combines both visible and infrared data, with a combined exposure time of over 34 hours. [1] | |
| Observation data (Epoch J2000) | |
| Constellation(s) | Virgo |
| Right ascension | 13h 11m 34.2s [2] |
| Declination | −01° 21′ 56″ |
| Richness class | 4 [3] |
| Bautz–Morgan classification | II-III [3] |
| Redshift | 0.1832 [2] |
| Distance | 754 Mpc (2,459 Mly) h−1 0.705 [2] |
| X-ray flux | (14.729 ± 8.1%)×10−11 erg s−1 cm−2 (0.1–2.4 keV) [2] |
Abell 1689 is a galaxy cluster in the constellation Virgo over 2.3 billion light-years away.
Abell 1689 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. [4] It has the largest system of gravitational arcs ever found. [5]
Abell 1689 shows over 160,000 globular clusters, the largest population ever found. [6]
There is evidence of merging and gases in excess of 100 million degrees. [5] The very large mass of this cluster makes it useful for the study of dark matter and gravitational lensing. [7] [8]
At the time of its discovery in 2008, one of the lensed galaxies, A1689-zD1, was the most distant galaxy found. [9] [10]