This color image is constructed from multi-wavelength observations: Infrared observations from NASA’s Spitzer Space Telescope are shown in red; near-infrared and visible light captured by the Gemini Observatory atop Mauna Kea in Hawaii is green and blue; and radio light from the Combined Array for Research in Millimeter-wave Astronomy (CARMA), near Owens Valley in California, is purple.
In addition to galaxies, clusters also contain a reservoir of hot gas with temperatures in the tens of millions of degrees. CARMA was used to detect this gas and to determine the mass of this cluster.
Galaxy clusters are gravitationally bound groups of thousands of galaxies, which themselves each contain hundreds of billions of stars. The clusters grow bigger and bigger over time as they acquire new members.
How did these clusters evolve over time? What did they look like billions of years ago? To answer these questions, astronomers look back in time to our youthful universe. Because light takes time to reach us, we can see distant objects as they were in the past. For example, we are seeing the newfound galaxy cluster — called Massive Overdense Object (MOO) J1142+1527 — as it existed 8.5 billion years ago, long before Earth formed.
As light from remote galaxies makes its way to us, it becomes stretched to longer infrared wavelengths by the expansion of space. That’s where WISE and Spitzer help out.
For infrared space telescopes, picking out distant galaxies is like plucking ripe cherries from a cherry tree. In the infrared images produced by Spitzer, these distant galaxies stand out as red dots, while closer galaxies look white. Astronomers first combed through the WISE catalog to find candidates for clusters of distant galaxies. WISE cataloged hundreds of millions of objects in images taken over the entire sky from 2010 to 2011.
They then used Spitzer to narrow in on 200 of the most interesting objects in a project named the “Massive and Distant Clusters of WISE Survey” (MaDCoWS). Spitzer doesn’t observe the whole sky like WISE, but it can see more detail.
“It’s the combination of Spitzer and WISE that lets us go from a quarter billion objects down to the most massive galaxy clusters in the sky,” said Anthony Gonzalez of the University of Florida in Gainesville.
From these observations, MOO J1142+1527 jumped out as one of the most extreme.
The W.M. Keck Observatories and Gemini Observatory on Mauna Kea in Hawaii were used to measure the distance to the cluster at 8.5 billion light-years. Using data from the Combined Array for Research in Millimeter-wave Astronomy (CARMA) telescopes near Owens Valley in California, the scientists were then able to determine that the cluster’s mass is a quadrillion times that of our Sun, making it the most massive known cluster that far back in space and time.
MOO J1142+1527 may be one of only a handful of clusters of this heft in the early universe, according to the scientists’ estimates.
“Based on our understanding of how galaxy clusters grow from the very beginning of our universe, this cluster should be one of the five most massive in existence at that time,” said Peter Eisenhardt from NASA’s Jet Propulsion Laboratory in Pasadena, California.
In the coming year, the team plans to sift through more than 1,700 additional galaxy cluster candidates with Spitzer, looking for biggest of the bunch.
“Once we find the most massive clusters, we can start to investigate how galaxies evolved in these extreme environments,” said Gonzalez.
