As big as old

As big as old https://blogger.googleusercontent.com/img/b/R29vZ2xl/AVvXsEi6e_kUlNMK80ZhzuIzxVuC6h8xqmjqMWeybXs0hHgvo2bGk1uMHhfCezaqraBDMEyAsjj8IiYcafEntTBhdGrJnqTgq_fMy9gsId2EKOpGnyLwIaTHX0zXnPncgfYsMnIx5fXUvxvHCvk/w1200-h630-p-k-no-nu/PIA20052.jpg

As big as old


In a very remote region of the cosmos, astronomers have found a giant cluster of galaxies thanks to observations carried out by the Spitzer Space Telescope and the WISE probe (Wide-field Infrared Survey Explorer). This great cluster, keeps its thousands of galaxies gravitationally united and grows as they incorporate new members.

To find this cluster the scientists analyzed the WISE catalog with the aim of finding candidates for distant galaxy clusters. Then, using Spitzer's data, they reduced the most interesting objects to 200 in a project called MaDCoWS (Massive and Distant Clusters of WISE Survey).

Image 1: MOO galaxy cluster J1142 + 1527. The red galaxies in the center make up the heart of this cluster. Credits: NASA / JPL-Caltech / Gemini / CARMA.

"It's the combination of Spitzer and WISE that has allowed us to reduce from 250,000 objects to just the most massive galaxy clusters," said Anthony Gonzalez, of the University of Florida (United States) and main author of the article that includes this investigation.

Once centered in the large cluster, called MOO J1142 + 1527, the telescopes of the W.M. Keck Observatory and the Gemini Observatory to measure the distance that separated us from it, being 8,500 million light years. Also, using the set of telescopes CARMA (Combined Array for Research in Millimeter-wave Astronomy), scientists were able to determine that the mass of the cluster is a billion billion (10 ^ 15) times that of our Sun, thus becoming the most massive galaxy cluster known and farthest from us.

Image 2: The graph on the left shows a 10 'x 10' region of the MOO cluster J1142 + 1527 obtained from the WISE data. The inner box shows a 3.5 'x 3.5' region centered on the cluster that corresponds to the graph on the right, based on the observation made by Spitzer. In both graphs the red dots mark individual locations of galaxies obtained with WISE. Credits: A.H. Gonzalez et al., 1015, ApJ, 812 L40.

"Based on our understanding of how galaxy clusters grow at the beginning of our universe, this group must be one of the five most massive of those moments," says Peter Eisenhardt, WISE project scientist at the JPL (Jet Propulsion Laboratory) of NASA in California (United States) and co-author of the article that exposes the investigation. Next year, more than 1,700 candidates for galaxy clusters will be analyzed with Spitzer to find the largest of the group.

One piece of information to reflect on is that the light that comes from this cluster shows us what it was like 8,500 million years ago, long before our solar system was formed.

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This research has been published in the journal Astrophysical Journal Letters in an article entitled "The massive and distant clusters of WISE Survey: MOO J1142 + 1527, at 10 ^ 15 M⊙ galaxy cluster at z = 1.19", by A.H. Gonzalez et al.

The team that has carried out the research consists of Anthony H. Gonzalez (Department of Astronomy, University of Florida, United States), Bandon Decker (Department of Physics and Astronomy, University of Missouri, United States), Mark Brodwin (Department of Physics and Astronomy, University of Missouri, United States), Peter RM Isehardt (Jet Propulsion Laboratory, California Institute of Technology, United States), Daniel P. Marrone (Steward Observatory, University of Arizona, United States), S.A. Stanford (Department of Physics, University of California, United States, Institute of Geophysics and Planetary Physics, Lawrence Livermore National Laboratory, United States), Daniel Stern (Jet Propulsion Laboratory, California Institute of Technology, United States), Dominika Wylezalek (Department of Physics and Astronomy, Johns Hopkins University, United States), Greg Aldering (Physics Division, Lawrence Berkeley National Laboratory, United States), Zubair Abdulla (Department of Astronomy and Astrophysics, University of Chicago, United States, Kavli Institute for Cosmological Physics, University of Chicago, United States), Kyle Boone (Physics Division, Lawrence Berkeley National Laboratory, United States, Department of Physics, University of California Berkeley, United States), John Carlstrom (Department of Astronomy and Astrophysics, University of Chicago, United States; Kavli Institute for Cosmological Physics, University of Chicago, United States), Parker Fagrelius (P hysics Division, Lawrence Berkeley National Laboratory, United States; Department of Physics, University of California Berkeley, United States), Daniel P. Gettings (Department of Astronomy, University of Florida, United States), Christopher H. Greer (Steward Observatory, University of Arizona, United States), Brain Hayden (Physics Division, Lawrence Berkeley National Laboratory, United States, Space Sciences Lab, University of California Berkeley, United States), Erik M. Leitch (Department of Astronomy and Astrophysics, University of Chicago, United States, Kavli Institute for Cosmological Physics, University of Chicago , United States), Yen-Ting Lin (Institute of Astronomy and Astrophysics, Academia Sinica, Taiwan), Adam B. Mantz (Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, United States, Department of Physics, Stanford University, United States ), Stephen Muchovej (California Institute of Technology, Owens Valley Radio Observatory, United States, California Institute of Technology, Department of Astronomy, United States), Saul Perlmutter (Physics Division, Lawrence Berkeley National Laboratory, United States; Department of Physics, University of California Berkeley, United States) and Gregory R. Zeimann (Department of Astronomy and Astrophysics, Pennsylvania State University, United States).
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