| Abell 2744 | |
|---|---|
| Abell 2744, nicknamed Pandora's Cluster. The galaxies in the cluster make up less than five percent of its mass. The gas (around 20 percent) is so hot that it shines only in X-rays (coloured red in this image). The distribution of invisible dark matter (making up around 75 percent of the cluster's mass) is coloured here in blue. | |
| Observation data (Epoch J2000) | |
| Constellation | Sculptor |
| Right ascension | 00h 14m 19.51s [1] |
| Declination | −30° 23′ 19.18″ [1] |
| Richness class | 3 [2] |
| Bautz–Morgan classification | III [2] |
| Redshift | 0.30800 [3] |
| Distance | 1,221 Mpc (3,982 Mly) h−1 0.705 [3] |
| X-ray flux | (5.805 ± 4.7%)×10−13 erg s−1 cm−2 (0.1–2.4 keV) [3] |
| Other designations | |
| Pandora's Cluster | |
Abell 2744, nicknamed Pandora's Cluster, is a giant galaxy cluster resulting from the simultaneous pile-up of at least four separate, smaller galaxy clusters that took place over a span of 350 million years, and is located approximately 4 billion light years from Earth. [1] The galaxies in the cluster make up less than five percent of its mass. [1] The gas (around 20 percent) is so hot that it shines only in X-rays. [1] Dark matter makes up around 75 percent of the cluster's mass. [1]
This cluster also shows a radio halo along with several other Abell clusters. It has a strong central halo, along with an extended tail, which could either be relic radiation, or an extension of the central halo. [4]
Renato Dupke, a member of the team that discovered the Cluster, explained the origin of the name in an interview: "We nicknamed it ‘Pandora's Cluster’ because so many different and strange phenomena were unleashed by the collision." [5]
This section may incorporate text from a large language model .(January 2026) |
In February 2023, the James Webb Space Telescope (JWST) provided an unprecedented deep-field view of Abell 2744 as part of the Ultradeep NIRSpec and NIRCam Observations before the Epoch of Reionization (UNCOVER) program. This observation revealed approximately 50,000 sources of near-infrared light, showcasing the cluster's complex structure and its role as a powerful gravitational lens. The combined mass of the merging galaxy clusters creates a natural magnification effect, allowing astronomers to observe much more distant galaxies in the early universe by using the cluster as a cosmic magnifying glass. [6] [7] [8] Further studies utilizing ultra-deep X-ray observations from the Chandra X-ray Observatory have detailed the disruption of cool cores in the three X-ray luminous subclusters of Abell 2744. These findings confirm the presence of a shock to the northwest and suggest a complex merger history involving a head-on north-south merger approximately 0.5–0.6 billion years ago, followed by the first infall of a northwest subcluster. [9] Additionally, the gravitational lensing effect of Abell 2744 has facilitated the discovery of some of the most distant galaxies observed to date. Notably, UNCOVER-z13 and UNCOVER-z12 are high-redshift Lyman-break galaxies identified behind the cluster, with redshifts of 13 and 12.393, respectively.
A 2025 analysis further examined the UNCOVER imaging to identify the positions and shapes of starburst galaxies in the Abell 2744 cluster. The analysis studied the shape of galaxies unobscured by cosmic dust by viewing images in the emission spectrum of polycyclic aromatic hydrocarbons (PAH), compounds which are associated with high rates of star formation. [10] The analysis found that almost all the star-forming galaxies in the cluster were in low-density areas on the outer edges of the cluster, suggesting star-forming galaxies are quenched as they fall into the cluster and ram pressure strips them of gas and dust. [11]