Images by Date
Images by Category
Solar System
Stars
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
Multiwavelength
Sky Map
Constellations
3D Wall
Photo Blog
Top Rated Images
Image Handouts
Desktops
High Res Prints
Fits Files
Image Tutorials
Photo Album Tutorial
False Color
Cosmic Distance
Look-Back Time
Scale & Distance
Angular Measurement
Images & Processing
AVM/Metadata
Getting Hard Copies
Image Use Policy
Web Shortcuts
Chandra Blog
RSS Feed
Chandra Mobile
Chronicle
Email Newsletter
News & Noteworthy
Image Use Policy
Questions & Answers
Glossary of Terms
Download Guide
Get Adobe Reader
CID-42: Giant Black Hole Kicked Out of Home Galaxy
CID-42

  • A massive black hole is likely being ejected from its host galaxy according to new data from Chandra and other telescopes.

  • This galaxy is called CID-42 and is located about 4 billion light years from Earth.

  • Data from Chandra's High Resolution Camera pinpoints where the X-rays are coming from - an important clue.

  • A simulation is available to show what astronomers think is happening in this extraordinary galaxy.

The galaxy at the center of this image contains an X-ray source, CID-42, with exceptional properties. After combining data from several telescopes - including NASA's Chandra X-ray Observatory - researchers think that CID-42 contains a massive black hole being ejected from its host galaxy at several million miles per hour.

The main panel is a wide-field image of CID-42 and its surroundings taken by the Canada-French-Hawaii Telescope and the Hubble Space Telescope in optical light. The galaxy is located nearly 4 billion light years from Earth. The outlined box on the main panel represents the more localized view of CID-42 that is shown in the three separate boxes on the right-hand side of the graphic. At the top is an image from the Chandra X-ray Observatory. The X-ray emission is concentrated in a single source, corresponding to one of the two sources seen in deep observations by Hubble, which is shown in the middle inset box. The bottom inset shows how the X-rays align with the optical data in the two insets above.

The precise location of this source was recently obtained using Chandra's High Resolution Camera, giving an important clue in telling astronomers what is happening within this galaxy. Previous Chandra observations had detected a bright X-ray source likely caused by super-heated material around one or more supermassive black holes. However, they could not distinguish if the X-rays came from one or both of the optical sources because Chandra was not pointed directly at CID-42, giving an X-ray source that was less sharp than usual.


Simulation of Black Hole Ejection

The new data help to clarify the situation. Researchers think that CID-42 is the byproduct of two galaxies that have collided, producing the distinctive tail seen in the upper part of the optical image inset. A simulation by co-author Laura Blecha shows more details of how this spectacular event was thought to unfold.

When this galaxy collision occurred, the supermassive black holes in the center of each galaxy also collided. The two black holes then merged to form a single black hole, that recoiled from gravitational waves produced by the collision, giving the newly merged black hole a sufficiently large kick for it to eventually escape from the galaxy. In this scenario, the source with the X-rays is the black hole being ejected from the galaxy. The other optical source is thought to be the bright star cluster that was left behind at the center of the galaxy.

With the higher resolution Chandra data a new feature was discovered in CID-42, a small extension to the lower right of the source. This could be a jet from the black hole or stars forming near it.

There are two other possible, but less likely, explanations for the optical data detected in CID-42. Both would involve the presence of a second supermassive black hole in CID-42, requiring X-ray emission from a second source to be heavily obscured.

Fast Facts for CID-42:
Credit  X-ray: NASA/CXC/SAO/F.Civano et al; Optical: NASA/STScI; Optical (wide field): CFHT, NASA/STScI
Release Date  June 4, 2012
Scale  Wide field image is 1 arcmin (1 million light years), Zoom image is 3.7 arcsec across (60,000 light years)
Category  Quasars & Active Galaxies, Black Holes
Coordinates (J2000)  RA 10h 00m 29.06s | Dec +02 05' 31.33"
Constellation  Sextans
Observation Date  2011 Jan 26
Observation Time  22 hours 2 min
Obs. ID  12810
Instrument  ACIS
References Civano, F. et al, 2012 ApJ 752:49; arXiv:1205.0815
Distance Estimate  About 3.9 billion light years
Visitor Comments (8)

Perhaps something was missed. The ejected SMBH possibly interacted with two other SMBHs. Binary pairs tend to simply merge, depending on trajectory and velocity the presence of a third may better explain the image.

Posted by Robert A Dorrough on Tuesday, 09.30.14 @ 18:33pm


I think other sites should take chandra.harvard.edu as a model, very clean and excellent user friendly style and design. Let the content aside, you are an expert on this topic.

Posted by Delcie on Monday, 10.14.13 @ 17:18pm


I believe this is probably the most vital information in my situation. And I am glad reading your article. But should remark on few general things, The internet site style is perfect, the articles is actually excellent : Good job, cheers

Posted by Winstrol 2 mg on Sunday, 03.24.13 @ 06:30am


I believe the black hole is being pulled into another much bigger black hole. It is not being ejected instead think of it more like if our solar system were to lose speed and stop orbiting sagittarius A* we would no longer be able to escape its gravity and we would be pulled straight in.

Posted by Jon Canning on Friday, 09.28.12 @ 04:31am


Cavitation: new physics term for me though I observed it frequently.
Question: can gravity cavitate? I mean...to some degree its turbulence, but in the shape of a trail.

Posted by Jim Hinton on Wednesday, 06.6.12 @ 15:51pm


The video was very helpful in demonstrating what occurrs when two black holes collide.

Posted by Mariposa on Tuesday, 06.5.12 @ 22:58pm


Eventually, the ejected massive black hole would have no stars around it and cannot be seen in any light, X-ray or visible. How do we know how many of these solitary black holes are there in our universe?

Posted by S. Paul Pao on Tuesday, 06.5.12 @ 09:40am


Totally awesome! Thank you all for your work and bringing us into the universe of the unknown and your help in making it known.
Congrats and a big thank you.

Posted by Don Schipani on Monday, 06.4.12 @ 23:08pm


Leave Your Comment

Name:

Email:

Comments:


 
 

Rules

Rate This Image

Rating: 2.6/5
(252 votes cast)
Download & Share

Desktops

1024x768 - 329.6 kb
1280x1024 - 492.2 kb
1680x1050 - 592 kb
More Information
Press Room: CID-42
Blog: CID-42
More Images
X-ray Image of
CID-42
Jpg, Tif
X-ray

More Images
Animation & Video
Simulation of Black
Hole Ejection
Animation

More Animations
More Releases
CID-42
CID-42
(30 Jun 10)

Related Images
N3393
N3393
(10 Feb 09)

NGC 6240
NGC 6240
(06 Oct 09)

Related Information
Related Podcast
Top Rated Images
Eta Carinae

WASP-18

M82X-2




FaceBookTwitterYouTubeFlickr