Labeled image of Abell 1758 system
Credit: X-ray: NASA/CXC/SAO/G.Schellenberger et al.; Optical:SDSS
Astronomers using data from NASA's Chandra X-ray Observatory and other telescopes have put together a detailed map of a rare collision between four galaxy clusters.
Eventually all four clusters — each with a mass of at least several
hundred trillion times that of the Sun — will merge to form one of the
most massive objects in the universe.
Galaxy clusters are the largest structures in the cosmos that are
held together by gravity. Clusters consist of hundreds or even thousands
of galaxies embedded in hot gas, and contain an even larger amount of
invisible dark matter. Sometimes two galaxy clusters collide, as in the case of the Bullet Cluster, and occasionally more than two will collide at the same time.
The new observations show a mega-structure being assembled in a
system called Abell 1758, located about 3 billion light-years from
Earth. It contains two pairs of colliding galaxy clusters that are
heading toward one another. Scientists first recognized Abell 1758 as a
quadruple galaxy cluster system in 2004 using data from Chandra and
XMM-Newton, a satellite operated by the European Space Agency (ESA).
Each pair in the system contains two galaxy clusters that are well on
their way to merging. In the northern (top) pair seen in the composite
image, the centers of each cluster have already passed by each other
once, about 300 to 400 million years ago, and will eventually swing back
around. The southern pair at the bottom of the image has two clusters
that are close to approaching each other for the first time.
X-rays
from Chandra are shown as blue and white, depicting fainter and
brighter diffuse emission, respectively. This new composite image also
includes an optical image from the Sloan Digital Sky Survey. The Chandra
data revealed for the first time a shock wave
— similar to the sonic boom from a supersonic aircraft — in hot gas
visible with Chandra in the northern pair's collision. From this shock
wave, researchers estimate two clusters are moving about 2 million to 3
million miles per hour (3 million to 5 million kilometers per hour),
relative to each other.
Chandra data also provide information about how elements heavier than
helium, the "heavy elements," in galaxy clusters get mixed up and
redistributed after the clusters collide and merge. Because this process
depends on how far a merger has progressed, Abell 1758 offers a
valuable case study, since the northern and the southern pairs of
clusters are at different stages of merging.
In the southern pair, the heavy elements are most abundant in the
centers of the two colliding clusters, showing that the original
location of the elements has not been strongly impacted by the ongoing
collision. By contrast, in the northern pair, where the collision and
merger has progressed further, the location of the heavy elements has
been strongly influenced by the collision. The highest abundances are
found between the two cluster centers and to the left side of the
cluster pair, while the lowest abundances are in the center of the
cluster on the left side of the image.
Collisions between clusters affect their component galaxies as well
as the hot gas that surrounds them. Data from the 6.5-meter MMT
telescope in Arizona, obtained as part of the Arizona Cluster Redshift
Survey, show that some galaxies are moving much faster than others,
probably because they have been thrown away from the other galaxies in
their cluster by gravitational forces imparted by the collision.
The team also used radio data from the Giant Metrewave Radio Telescope (GMRT), and X-ray data from ESA's XMM-Newton mission.
A paper describing these latest results by Gerrit Schellenberger,
Larry David, Ewan O'Sullivan, Jan Vrtilek (all from Center for
Astrophysics | Harvard & Smithsonian) and Christopher Haines
(Universidad de Atacama, Chile) was published in the September 1st, 2019
issue of The Astrophysical Journal, and is available online.
NASA's Marshall Space Flight Center manages the Chandra program. The
Smithsonian Astrophysical Observatory's Chandra X-ray Center controls
science and flight operations from Cambridge, Massachusetts.
Source: NASA’s Chandra X-ray Observatory
Fast Facts for Abell 1758
Scale: Image is about 16.7 arcmin (14 million light years) across.
Category: Groups & Clusters of Galaxies, Cosmology/Deep Fields/X-ray Background
Coordinates (J2000): RA 13h 32m 43.02s | Dec +50° 32´ 25.70"
Constellation: Canes Venatici
Observation Date: Aug 28, 2001
Observation Time: 56 hours 40 minutes (2 days 8 hours 40 minutes)
Obs. ID: 2213, 13997, 15538, 15540
Instrument: ACIS
References: Schellenberger G., et al, 2019, ApJ, 882, 59; arXiv:1907.10581
Color Code: X-ray: blue and white; Optical: yellow and pink
Distance Estimate: About 3.2 billion light years (z=0.28)
