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
NGC 4151: An Active Black Hole in the "Eye of Sauron"
NGC 4151
NGC 4151
NGC 4151

  • NGC 4151 is a spiral galaxy with an actively growing supermassive black hole at its center.

  • This composite image of NGC 4151 contains X-rays from Chandra (blue), optical data (yellow), and radio emission (red).

  • The structure has been dubbed "The Eye of Sauron" by astronomers due to its resemblance to the character in "The Lord of the Rings" movies.

This composite image shows the central region of the spiral galaxy NGC 4151, dubbed the "Eye of Sauron" by astronomers for its similarity to the eye of the malevolent character in "The Lord of the Rings". In the "pupil" of the eye, X-rays (blue) from the Chandra X-ray Observatory are combined with optical data (yellow) showing positively charged hydrogen ("H II") from observations with the 1-meter Jacobus Kapteyn Telescope on La Palma. The red around the pupil shows neutral hydrogen detected by radio observations with the NSF's Very Large Array. This neutral hydrogen is part of a structure near the center of NGC 4151 that has been distorted by gravitational interactions with the rest of the galaxy, and includes material falling towards the center of the galaxy. The yellow blobs around the red ellipse are regions where star formation has recently occurred.

A recent study has shown that the X-ray emission was likely caused by an outburst powered by the supermassive black hole located in the white region in the center of the galaxy. Evidence for this idea comes from the elongation of the X-rays running from the top left to the bottom right and details of the X-ray spectrum. There are also signs of interactions between a central source and the surrounding gas, particularly the yellow arc of H II emission located above and to the left of the black hole.

Two different scenarios to explain the X-ray emission have been proposed. One possibility is that the central black hole was growing much more quickly about 25,000 years ago (in Earth's time frame) and the radiation from the material falling onto the black hole was so bright that it stripped electrons away from the atoms in the gas in its path. X-rays were then emitted when electrons recombined with these ionized atoms.

The second possibility also involved a substantial inflow of material into the black hole relatively recently. In this scenario the energy released by material flowing into the black hole in an accretion disk created a vigorous outflow of gas from the surface of the disk. This outflowing gas directly heated gas in its path to X-ray emitting temperatures. Unless the gas is confined somehow, it would expand away from the region in less than 100,000 years. In both of these scenarios, the relatively short amount of time since the last episode of high activity by the black hole may imply such outbursts occupy at least about 1% of the black hole's lifetime.

NGC 4151 is located about 43 million light years away from the Earth and is one of the nearest galaxies that contains an actively growing black hole. Because of this proximity, it offers one of the best chances of studying the interaction between an active supermassive black hole and the surrounding gas of its host galaxy. Such interaction, or "feedback", is recognized to play a key role in the growth of supermassive black holes and their host galaxies. If the X-ray emission in NGC 4151 originates from hot gas heated by the outflow from the central black hole, it would be strong evidence for feedback from active black holes to the surrounding gas on galaxy scales. This would resemble the larger scale feedback, observed on galaxy cluster scales, from active black holes interacting with the surrounding gas, as seen in objects like the Perseus Cluster.

These results were published in the August 20, 2010 issue of The Astrophysical Journal Letters. The authors were Junfeng Wang and Giuseppina Fabbiano from the Harvard Smithsonian Center for Astrophysics (CfA), Guido Risaliti from CfA and INAF-Arcetri Observatory, in Firenze, Italy, Martin Elvis from CfA, Carole Mundell from Liverpool John Moores University in Birkenhead, UK, Gaelle Dumas and Eva Schinnerer from the Max Planck Institute for Astrophysics in Heidelberg, Germany, and Andreas Zezas, from CfA and the University of Crete in Greece.

Fast Facts for NGC 4151:
Credit  X-ray: NASA/CXC/CfA/J.Wang et al.; Optical: Isaac Newton Group of Telescopes, La Palma/Jacobus Kapteyn Telescope, Radio: NSF/NRAO/VLA
Release Date  March 10, 2011
Scale  Image is 3 arcmin across (about 37,540 light years across)
Category  Quasars & Active Galaxies
Coordinates (J2000)  RA 12h 10m 32.60s | Dec +39° 24' 20.40"
Constellation  Canes Venatici
Observation Date  March 27th and 29th, 2008
Observation Time  55 hours 33 min (2 days 7 hours 33 min )
Obs. ID  9217, 9218
Instrument  ACIS
References Wang, J. et al. (2011), ApJ, 729, 75; Wang, J et al. (2010) ApJ, 719, L208; Wang, J. et al. (2009), ApJ, 704, 1195
Color Code  X-ray (Blue); Optical (Yellow); Radio (Red)
Radio
Optical
X-ray
Distance Estimate  About 43 million light years
Visitor Comments (8)

Spectroscopically Resolved Sub-parsec Orbit of a Supermassive Binary Black Hole in NGC 4151 :
http://arxiv.org/abs/1209.4524

Posted by Edi Bon on Sunday, 10.14.12 @ 10:22am


It would be interesting to add a gamma ray image from Fermi telescope.

Posted by DavidM on Tuesday, 10.18.11 @ 17:41pm


This is a great place to come to so much information with such exactness.

Posted by rick on Saturday, 07.16.11 @ 17:47pm


Send more photos.

Posted by Charles Watson on Thursday, 05.5.11 @ 14:51pm


Apparently, from what I have been reading on the subject of Black Holes, there are more galaxies with one than galaxies without them.
Most interesting article. Educational as always.
Marvin L. S.

Posted by Marvin L S on Friday, 03.11.11 @ 20:31pm


I am still impressed by the advances in astronomy. It is hard to comprehend the vastness of knowledge.

Posted by Mark Milhous on Thursday, 03.10.11 @ 21:55pm


Looking back some many light years ago, I was Steve Murray Joe Swider, and Gerry Austin's PLANNER on the design and development of the Chandra HRC Program. What a program, even today, I am thrilled when I receive daily news of our journey into deep space. Awesome, I have since gone into a hard earned retirement. Hello, to all of my friends including Harold T. NASA Blood Still Runs Thru My Veins.
Gene Talford, Newburyport, MA

Posted by Gene Talford on Thursday, 03.10.11 @ 20:16pm


Try photographing the black hole with many kind's of sodium filters and spinning rapidly slow-light gels and see what slowed down photons respond like.

Posted by peter grant on Thursday, 03.10.11 @ 19:09pm


Leave Your Comment

Name:

Email:

Comments:


 
 

Rules

Rate This Image

Rating: 2.7/5
(396 votes cast)
Download & Share

Desktops

1024x768 - 314 kb
1280x1024 - 434.2 kb
1680x1050 - 548.1 kb
More Information
Blog: NGC 4151
Zoom: NGC 4151
More Images
X-ray Image of
NGC 4151
Jpg, Tif
X-ray

More Images
Animation & Video
Multiwavelength view of NGC 4151
animation

More Animations
More Releases
NGC 4151
NGC 4151
(05 Jun 00)

Related Images
NGC 1068
NGC 1068
(03 Mar 10)

NGC 1068
NGC 1068
(09 Jul 03)

NGC 5548
NGC 5548
(17 Feb 00)

Related Information
Related Podcast
Top Rated Images
Eta Carinae

WASP-18

M82X-2




FaceBookTwitterYouTubeFlickr