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Bullet Cluster: Searching for Primordial Antimatter
Bullet Cluster

This view of the Bullet Cluster, located about 3.8 billion light years from Earth, combines an image from NASA's Chandra X-ray Observatory with optical data from the Hubble Space Telescope and the Magellan telescope in Chile. This cluster, officially known as 1E 0657-56, was formed after the violent collision of two large clusters of galaxies. It has become an extremely popular object for astrophysical research, including studies of the properties of dark matter and the dynamics of million-degree gas.

In the latest research, the Bullet Cluster has been used to search for the presence of antimatter leftover from the very early Universe. Antimatter is made up of elementary particles that have the same masses as their corresponding matter counterparts - protons, neutrons and electrons - but the opposite charges and magnetic properties.

The optical image shows the galaxies in the Bullet Cluster and the X-ray image (red) reveals how much hot gas has collided. If some of the gas from either cluster has particles of antimatter, then there will be annihilation between the matter and antimatter and the X-rays will be accompanied by gamma rays.

The observed amount of X-rays from Chandra and the non-detection of gamma rays from NASA's Compton Gamma Ray Observatory show that the antimatter fraction in the Bullet Cluster is less than three parts per million. Moreover, simulations of the Bullet Cluster merger show that these results rule out any significant amounts of antimatter over scales of about 65 million light years, an estimate of the original separation of the two colliding clusters.

Fast Facts for Bullet Cluster:
Credit  X-ray: NASA/CXC/CfA/M.Markevitch et al.; Optical: NASA/STScI; Magellan/U.Arizona/D.Clowe et al.
Release Date  October 30, 2008
Scale  Image is 6.7 arcmin across.
Category  Groups & Clusters of Galaxies
Coordinates (J2000)  RA 06h 58m 37.9s | Dec -55° 57´ 00.00"
Constellation  Carina
Observation Date  08/10/2004 - 08/25/2008
Observation Time  140 hours
Obs. ID  5355-58, 5361, 4984-86
Instrument  ACIS
Color Code  X-ray: Pink; Optical: White/Orange;
Distance Estimate  About 3.8 billion light years
distance arrow
Visitor Comments (1)

Good evening. Please can you inform the apparent magnitude of the cluster? Thanks.

Posted by Jaqueline de Souza Valdemiro Campos on Saturday, 10.15.16 @ 00:30am

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