Monster "El Gordo" Galaxy Cluster is Bigger Than Thought
Scientists first announced the discovery of El Gordo with Chandra
and ground-based optical telescopes in 2012. They determined that El Gordo is
the most massive, the hottest, and gives off the most X-rays of any known galaxy
cluster at its distance or beyond.
New data from the Hubble Space Telescope suggests El Gordo weighs as much as
3 million billion times the mass of our Sun. This is about 43 percent higher
than the original estimate based on the X-ray data and dynamical studies.
The new Hubble study determined that most of the mass is hidden away as dark matter. The
location of the dark matter is mapped out in this composite in blue. Because dark matter
doesn't emit any radiation, astronomers instead precisely measure how its
gravity warps the images of far background galaxies like a funhouse mirror. This
allowed them to come up with a mass estimate for the cluster. Chandra's X-ray
data are shown in pink and these have been overlaid on optical data from Hubble
that shows the individual galaxies in the cluster as well as stars in the field
of view.
The X-ray image of El Gordo reveals a distinct cometary appearance. Along with the optical data,
this shows that El Gordo is, in fact, the site of two galaxy clusters running
into one another at several million miles per hour. This and other
characteristics make El Gordo akin to the well-known object called the Bullet Cluster, which
is located almost 4 billion light years closer to Earth.
As with the Bullet Cluster, there is evidence that normal matter, mainly
composed of hot, X-ray bright gas, has been wrenched apart from the dark matter
in El Gordo. The hot gas in each cluster was slowed down by the collision, but
the dark matter was not.
NASA's Marshall Space Flight Center in Huntsville, Ala., manages the Chandra
program for NASA's Science Mission Directorate in Washington. The
Smithsonian Astrophysical Observatory in Cambridge, Mass., controls Chandra's
science and flight operations.
Image credit: NASA, ESA, J. Jee (Univ. of California, Davis), J. Hughes
(Rutgers Univ.), F. Menanteau (Rutgers Univ. & Univ. of Illinois,
Urbana-Champaign), C. Sifon (Leiden Obs.), R. Mandelbum (Carnegie Mellon Univ.),
L. Barrientos (Univ. Catolica de Chile), and K. Ng (Univ. of California,
Davis)
NASA
Guillermo Gonzalo Sánchez Achutegui
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