Images by Date
Images by Category
Solar System
Stars
Exoplanets
White Dwarfs
Supernovas
Neutron Stars
Black Holes
Milky Way Galaxy
Normal Galaxies
Quasars
Galaxy Clusters
Cosmology/Deep Field
Miscellaneous
Images by Interest
Space Scoop for Kids
4K JPG
Multiwavelength
Sky Map
Constellations
Photo Blog
Top Rated Images
Image Handouts
Desktops
Fits Files
Visual descriptions
Image Tutorials
Photo Album Tutorial
False Color
Cosmic Distance
Look-Back Time
Scale & Distance
Angular Measurement
Images & Processing
AVM/Metadata
Image Use Policy
Web Shortcuts
Chandra Blog
RSS Feed
Chronicle
Email Newsletter
News & Noteworthy
Image Use Policy
Questions & Answers
Glossary of Terms
Download Guide
Get Adobe Reader
Chandra Spots a Mega-Cluster of Galaxies in the Making
Abell 1758
Abell 1758

  • A mega-merger of four galaxy clusters in Abell 1758 has been observed by Chandra and other telescopes.

  • Abell 1758 contains two pairs of galaxy clusters, each with hundreds of galaxies embedded in large amounts of hot gas and unseen dark matter.

  • Eventually these two pairs of clusters will collide to form one of the most massive objects in the Universe.

  • The X-rays from Chandra helped astronomers estimate how fast one pair of clusters were moving toward each other.

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.

Labeled Image of Abell 1758
Labeled image of Abell 1758 system.

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.

 

Fast Facts for Abell 1758:
Credit  X-ray: NASA/CXC/SAO/G.Schellenberger et al.; Optical:SDSS
Release Date  October 24, 2019
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
Optical
X-ray
Distance Estimate  About 3.2 billion light years (z=0.28)
distance arrow
Rate This Image

Rating: 3.7/5
(168 votes cast)
Download & Share

More Information
More Images
X-ray Image of
Abell 1758
Jpg, Tif
X-ray

More Images
Animation & Video
A Tour of a Collision Between Four Galaxy Clusters in Abell 1758
animation

More Animations
More Releases
Abell 1758
Abell 1758
(30 Aug 10)

Related Images
Merging clusters Abell 399 and Abell 401

Galaxy Cluster Abell 2142
Abell 2142
(28 Sep 18)


Related Information
Related Podcast
Top Rated Images
Brightest Cluster Galaxies

Timelapses: Crab Nebula and Cassiopeia A

Chandra Releases 3D Instagram Experiences




FaceBookTwitterYouTubeFlickr