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MACS J1149.5+2233: A Fusion of Galaxy Clusters
MACS J1149.5+2233
MACS J1149.5+2233
MACS J1149.5+2233

  • The Frontier Fields is a project that combines long observations from multiple telescopes of galaxy clusters.

  • Galaxy clusters contain up to thousands of galaxies and vast reservoirs of hot gas embedded in massive clouds of dark matter.

  • Data from Chandra, Hubble, Spitzer and other telescopes are part of the Frontier Fields project.

  • This Frontier Fields galaxy cluster, known as MACS J1149.5+2233, is located about 5 billion light years from Earth.

MACS J1149.5+2233 (MACS J1149 for short) is a system of merging galaxy clusters located about 5 billion light years from Earth. This galaxy cluster was one of six that have been studied as part of the "Frontier Fields" project. This research effort included long observations of galaxy clusters with powerful telescopes that detected different types of light, including NASA's Chandra X-ray Observatory.

Astronomers are using the Frontier Fields data to learn more about how galaxy clusters grow via collisions. Galaxy clusters are enormous collections of hundreds or even thousands of galaxies and vast reservoirs of hot gas embedded in massive clouds of dark matter, invisible material that does not emit or absorb light but can be detected through its gravitational effects.

This new image of MACS J1149 combines X-rays from Chandra (diffuse blue), optical data from Hubble (red, green, blue), and radio emission from the Very Large Array (pink). The image is about four million light years across at the distance of MACS J1149.

The Chandra data reveal gas in the merging clusters with temperatures of millions of degrees. The optical data show galaxies in the clusters and other, more distant, galaxies lying behind the clusters. Some of these background galaxies are highly distorted because of gravitational lensing, the bending of light by massive objects. This effect can also magnify the light from these objects, enabling astronomers to study background galaxies that would otherwise be too faint to detect. Finally, the structures in the radio data trace enormous shock waves and turbulence. The shocks are similar to sonic booms, and are generated by the mergers of smaller clusters of galaxies.

NASA's Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program for NASA's Science Mission Directorate in Washington. The Smithsonian Astrophysical Observatory in Cambridge, Massachusetts, controls Chandra's science and flight operations.

Fast Facts for MACS J1149.5+2233:
Credit  X-ray: NASA/CXC/SAO; Optical: NASA/STScI; Radio: NSF/NRAO/AUI/VLA
Release Date  October 31, 2017
Scale  Image is 3.2 arcmin across (about 4.7 million light years)
Category  Groups & Clusters of Galaxies
Coordinates (J2000)  RA 11h 49m 36.3s | Dec 22° 23´ 58.1"
Constellation  Leo
Observation Date  8 pointings between Jun 2001 and Feb 2015
Observation Time  101 hours 30 min (4 days 5 hours 30 min)
Obs. ID  1656, 3589, 16238, 16239, 16306, 16582, 17595, 17596
Instrument  ACIS
Color Code  X-ray (Blue); Optical (Red, Green, Blue); Radio (Pink)
Radio
Optical
X-ray
Distance Estimate  About 5 billion light years
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