This NASA Hubble Space Telescope image of Abell 3192 holds two independent galaxy clusters. ESA/Hubble & NASA, G. Smith, H. Ebeling, D. Coe
This Hubble image features a massive cluster of brightly
glowing galaxies, first identified as Abell 3192. Like all galaxy
clusters, this one is suffused with hot gas that emits powerful X-rays, and it
is enveloped in a halo of invisible dark matter. All this unseen material
– not to mention the many galaxies visible in this image – comprises such a
huge amount of mass that the galaxy cluster noticeably curves spacetime around
it, making it into a gravitational lens. Smaller galaxies behind the
cluster appear distorted into long, warped arcs around the cluster’s edges.
The galaxy cluster is in the
constellation Eridanus, but the question of its distance from Earth is a more
complicated one. Abell 3192 was originally documented in the 1989 update of the
Abell catalog of galaxy clusters that was first published in 1958. At that
time, Abell 3192 was thought to comprise a single cluster of galaxies,
concentrated at a single distance. However, further research revealed something
surprising: the cluster’s mass seemed to be densest at two distinct points
rather than one.
It was subsequently shown that the
original Abell cluster is actually comprised of two independent galaxy clusters
– a foreground group around 2.3 billion light-years from Earth, and another
group at the greater distance of about 5.4 billion light-years from our planet.
The more distant galaxy cluster, included in the Massive Cluster Survey as MCS
J0358.8-2955, is central in this image. The two galaxy groups are thought to
have masses equivalent to around 30 trillion and 120 trillion times the mass of
the Sun, respectively. Both of the two largest galaxies at the center of this
image are part of MCS J0358.8-2955; the smaller galaxies you see here, however,
are a mixture of the two groups within Abell 3192.
Text credit: European Space Agency
Source: Hubble Views a Double Cluster of Glowing Galaxies - NASA Science
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