Using Hubbles images we can see that Abell 3192 is a vast and radiant collection of galaxies. What makes this cosmic assembly so intriguing is the presence of dark matter surrounding it and the emission of powerful X rays from clusters of hot gas. These visible and invisible elements combine to create an amount of mass that actually warps space time itself through gravitational lensing. This creates a sight where smaller galaxies located behind Abell 3192 appear stretched and distorted into elongated arcs around the clusters edge.
Now lets dive deeper into the specifics of Abell 3192. Initially researchers believed it was a concentrated cluster of galaxies within the Eridanus constellation. However further investigations revealed a discovery; there are actually two distinct locations with denser masses. This means that Abell 3192 is now recognized as a dual cluster phenomenon.
These two individual galaxy clusters are positioned at depths, in space.
One of the clusters is located about 2.3 billion years away and is positioned in front of Abell 3192. The other cluster, MCS J0358.8 2955 is away at a distance of approximately 5.4 billion light years and holds a central position in the observed image. These two clusters have a combined mass, estimated to be around 150 trillion times the mass of our Sun. The larger galaxies seen in the center of the image belong to MCS J0358.8 2955 while the smaller galaxies are a mix from both groups within the Abell 3192 complex.
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