Chandra Spies Structure of Huge X-Ray Jets

Space Science News home
Chandra Spies Structure of Huge X-Ray Jets
Extended X-Ray Jet in Nearby Galaxy
Reveals Energy Source
October
26, 1999: NASA's Chandra X-ray Observatory has made an extraordinary
image of Centaurus A, a nearby galaxy noted for its explosive
activity. The image shows X-ray jets erupting from the center
of the galaxy over a distance of 25,000 light years. Also detected
are a group of X-ray sources clustered around the nucleus, which
is believed to harbor a supermassive black hole. The X-ray jets
and the cluster of sources may be a byproduct of a titanic collision
between galaxies several hundred million years ago.
Right: Centaurus A as viewed from the Chandra X-Ray
Observatory shows two x-ray jets extending from a galactic center
thought to be home to a huge black hole at the center. The image
links to a 540x533-pixel,
138 KB JPG. Or, click here for a 2250x2221-pixel,
3.6MB TIFF. Image credit: NASA and Chandra Science Center
"This image is great," said Dr. Ethan Schreier of
the Space Telescope Science Institute, "For twenty years
we have been trying to understand what produced the X rays seen
in the Centaurus A jet. Now we at last know that the X-ray emission
is produced by extremely high energy electrons spiraling around
a magnetic field." Schreier explained that the length and
shape of the X-ray jet pinned down the source of the radiation.
The entire length of the X-ray jet is comparable to the diameter
of the Milky Way Galaxy.
Other features of the image excite scientists. "Besides
the jets, one of the first things I noticed about the image was
the new population of sources in the center of the galaxy,"
said Dr. Christine Jones from the Harvard-Smithsonian Center
for Astrophysics. "They are grouped in a sphere around the
nucleus, which must be telling us something very fundamental
about how the galaxy, and the supermassive black hole in the
center, were formed."
December 3: Mars Polar Lander nears touchdown December 2: What next, Leonids? November 30: Polar Lander Mission Overview November 30: Learning how to make a clean sweep in space |
![]() | ![]() | ![]() | ![]() |
Photo:2 MASS | Photo:AURA/NOAO/NSF | Photo:NASA/CXC/SAO | Photo:NRAO/AUI |
Above: Centaurus A as viewed in four different spectra. The brilliant jet so visible in the x-ray is perpendicular to the apparent plane of the galaxy in visible or infrared. See the Chandra X-Ray Observatory Center's What Do These Images Tell Us page for more information.
Astronomers have accumulated evidence with optical and infrared
telescopes that Centaurus A collided with a small spiral galaxy
several hundred million years ago. This collision is believed
to have triggered a burst of star formation and supplied gas
to fuel the activity of the central black hole.
According to Dr. Giuseppina Fabbiano, of Harvard-Smithsonian,
"The Chandra image is like having a whole new laboratory
to work in. Now we can see the main jet, the counter jet, and
the extension of the jets beyond the galaxy. It is gorgeous in
the detail it reveals," she said.
Dr. Allyn Tennnant of NASA's Marshall Space Flight Center agreed.
"It's incredible, being able to see all that structure in
the jet," he said. "We have one fine X-ray telescope."
![]() Sign up for our EXPRESS SCIENCE NEWS delivery |
The Chandra X-ray image of Centaurus A, made with the High Resolution Camera, shows a bright source in the nucleus of the galaxy at the location of the suspected supermassive black hole. The bright jet extending out from the nucleus to the upper left is due to explosive activity around the black hole that ejects matter at high speeds from the vicinity of the black hole. A "counter jet" extending to the lower right can also be seen. This jet is probably pointing away from us, which accounts for its faint appearance.
One of the most intriguing features of supermassive black holes is that they do not suck up all the matter that falls within their sphere of influence. Some of the matter falls inexorably toward the black hole, and some explodes away from the black hole in high-energy jets that move at near the speed of light. The presence of bright X-ray jets in the Chandra image means that electric fields are continually accelerating electrons to extremely high energies over enormous distances. Exactly how this happens is a major puzzle that Chandra may help to solve.
Dr. Stephen Murray of the Harvard-Smithsonian Center for Astrophysics is the principal investigator for the High Resolution Camera. NASA's Marshall Space Flight Center in Huntsville, AL, manages the Chandra program. TRW, Inc., Redondo Beach, CA, is the prime contractor for the spacecraft. The Smithsonian's Chandra X-ray Center controls science and flight operations from Cambridge, MA.
Web LinksXrayastronomy.com,
science
news from the Chandra X-Ray Observatory
Chandra X-ray Observatory
Center home
page, with links to education, news, and technical pages.
Chandra news from Marshall Space
Flight Center
Chandra
Project Science is
managed at NASA/Marshall, has links to individual instruments
and the prime contractor.
X-ray astrophysics
branch at
NASA/Marshall conducts a broad range of research and technology
work, as well as supporting the Chandra X-ray Observatory.
More Space Science Headlines - NASA research on the web
NASA's Office of Space Sciencepress releases and other news related to NASA and astrophysics
More
Headlines| For more information,
please contact: Dr. John M. Horack , Director of Science Communications | Author: Dave Dooling Curator: Bryan Walls NASA Official: M. Frank Rose |




