From Hubble: “NASA’s Great Observatories Weigh Massive Young Galaxy Cluster”

NASA Hubble Telescope

Hubble

January 7, 2016
CONTACT

Megan Watzke
Chandra X-ray Center, Cambridge, Massachusetts
617-496-7998
mwatzke@cfa.harvard.edu

Ray Villard
Space Telescope Science Institute, Baltimore, Maryland
410-338-4514
villard@stsci.edu

Whitney Clavin
Jet Propulsion Laboratory, Pasadena, California
818-354-4673
whitney.clavin@jpl.nasa.gov

Mark Brodwin
University of Missouri, Kansas City, Missouri
brodwinm@umkc.edu

Temp 1
Hubble, Chandra, Spitzer Composite of Massive Galaxy Cluster IDCS J1426.5+3508

Temp 2
HST Image of Massive Galaxy Cluster IDCS J1426.5+3508

Temp 3
Compass and Scale Image of Massive Galaxy Cluster IDCS J1426.5+3508

Astronomers have used data from three of NASA’s Great Observatories to make the most detailed study yet of an extremely massive young galaxy cluster. This rare galaxy cluster, which is located 10 billion light-years from Earth, is almost as massive as 500 trillion suns. This object has important implications for understanding how these megastructures formed and evolved early in the universe.

The galaxy cluster, called IDCS J1426.5+3508 (IDCS 1426 for short), is so far away that the light detected is from when the universe was roughly a quarter of its current age. It is the most massive galaxy cluster detected at such an early age.

First discovered by the Spitzer Space Telescope in 2012, IDCS 1426 was then observed using the Hubble Space Telescope and the Keck Observatory to determine its distance.

NASA Spitzer Telescope
NASA/Spitzer

Keck Observatory
Keck Observatory Interior
Keck Observatory

Observations from the Combined Array for Millimeter-wave Astronomy indicated it was extremely massive.

Caltech Combined Array for Millimeter Astronomy
Caltech/Combined Array for Millimeter-wave Astronomy

New data from the Chandra X-ray Observatory confirm the galaxy cluster mass and show that about 90 percent of the mass of the cluster is in the form of dark matter, a mysterious substance detected so far only through its gravitational pull on normal matter composed of atoms.

NASA Chandra Telescope
NASA/Chandra

“We are really pushing the boundaries with this discovery,” said Mark Brodwin of the University of Missouri at Kansas City, who led the study. “As one of the earliest massive structures to form in the universe, this cluster sets a high bar for theories that attempt to explain how clusters and galaxies evolve.”

Galaxy clusters are the largest objects in the universe bound together by gravity. Because of their sheer size, scientists think it should take several billion years for them to form. The distance of IDCS J1426 means astronomers are observing it when the universe was only 3.8 billion years old, implying that the cluster is seen at a very young age.

The data from Chandra reveal a bright knot of X-rays near the middle of the cluster, but not exactly at its center. This overdense core has been dislodged from the cluster center, possibly by a merger with another developing cluster 500 million years prior. Such a merger would cause the X-ray-emitting, hot gas to slosh around like wine in a glass that is tipped from side to side.

“Mergers with other groups and clusters of galaxies should have been more common so early in the history of the universe,” said co-author Michael McDonald of the Massachusetts Institute of Technology in Cambridge, Massachusetts. “That appears to have played an important part in this young cluster’s rapid formation.”

Aside from this cool core, the hot gas in the rest of the cluster is very smooth and symmetric. This is another indication that IDCS 1426 formed very rapidly. In addition, astronomers found possible evidence that the abundance of elements heavier than hydrogen and helium in the hot gas is unusually low. This suggests that this galaxy cluster might still be in the process of enriching its hot gas with these elements as supernovae create heavier elements and blast them out of individual galaxies.

“The presence of this massive galaxy cluster in the early universe doesn’t upset our current understanding of cosmology,” said co-author of Anthony Gonzalez of the University of Florida in Gainesville, Florida. “It does, however, give us more information to work with as we refine our models.”

Evidence for other massive galaxy clusters at early times has been found, but none of these matches IDCS 1426, with its combination of mass and youth. The mass determination used three independent methods: a measurement of the mass needed to confine the hot X-ray-emitting gas to the cluster, the imprint of the cluster’s gaseous mass on the cosmic microwave background radiation [CMB], and the observed distortions in the shapes of galaxies behind the cluster, which are caused by the bending of light from the galaxies by the gravity of the cluster.

CMB Planck ESA
CMB per ESA/Planck

ESA Planck
ESA/Planck

These results were presented at the 227th American Astronomical Society meeting being held in Kissimmee, Florida. A paper describing these results has been accepted for publication in The Astrophysical Journal and is available online. NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program for NASA’s Science Mission Directorate in Washington, D.C. The Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, controls Chandra’s science and flight operations. The Spitzer Space Telescope is managed by NASA’s Jet Propulsion Laboratory in Pasadena, California. The Spitzer Science Center at the California Institute of Technology in Pasadena conducts science operations. The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency. NASA’s Goddard Space Flight Center manages the telescope. The Space Telescope Science Institute (STScI) in Baltimore, Maryland, conducts Hubble science operations. STScI is operated for NASA by the Association of Universities for Research in Astronomy in Washington, D.C.

Data Description:

The HST data were taken from the following proposals: 11663 : M. Brodwin (University of Missouri, Kansas City), P. Eisenhardt (JPL), A. Stanford (UC Davis/LLNL), D. Stern (JPL), L. Moustakas (JPL), A. Dey (NOAO), B. Jannuzi (University of Arizona/NOAO), and A. Gonzalez (University of Florida, Gainesville);

12203: A. Stanford (UC Davis/LLNL), M. Brodwin (University of Missouri, Kansas City), A. Gonzalez (University of Florida, Gainesville), A. Dey (NOAO), D. Stern (JPL), G. Zeimann (Penn State University), and P. Eisenhardt and L. Moustakas (JPL);

and 12994: A. Gonzalez (University of Florida, Gainesville), M. Brodwin (University of Missouri, Kansas City), A. Stanford (UC Davis/LLNL), J. Rhodes and D. Stern (JPL), P. Eisenhardt (JPL), C. Fedeli (University of Florida), G. Zeimann (Penn State University), A. Dey (NOAO), and D. Marrone (University of Arizona).

The science team includes M. Brodwin (University of Missouri, Kansas City), M. McDonald (MIT), A. Gonzalez (University of Florida, Gainesville), A. Stanford (UC Davis/LLNL), P. Eisenhardt and D. Stern (JPL), and G. Zeimann (Penn State University).
Instruments/Filters:
ACS/WFC F606W (V)
ACS//WFC F814W(I)
WFC3/IR F160W (H)

NASA Hubble ACS
ACS

NASA Hubble WFC3
WFC3

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The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency. NASA’s Goddard Space Flight Center manages the telescope. The Space Telescope Science Institute (STScI), is a free-standing science center, located on the campus of The Johns Hopkins University and operated by the Association of Universities for Research in Astronomy (AURA) for NASA, conducts Hubble science operations.

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