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
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
More Information
Quasars & Active Galaxies
X-ray Astronomy Field Guide
Quasars & Active Galaxies
Questions and Answers
Quasars & Active Galaxies
Chandra Images
Quasars & Active Galaxies
Related Podcasts
Tour: Unexpectedly Calm and Remote Galaxy Cluster Discovered
Download Image

More Information

More Images
X-ray Production by Compton Scattering of Microwave Background
(Credit: NASA/CXC/M.Weiss)


Related Images
GB1508+5714:
Most Distant X-Ray Jet Yet Discovered Provides Clues To Big Bang


GB1508+5714
Credit: NASA/CXC/A.Siemiginowska et al.; Illustration: NASA/CXC/M.Weiss

The Chandra image of the quasar GB1508+5714 (inset) reveals a jet of high-energy particles that extends more than 100,000 light years from the supermassive black hole powering the quasar. At a distance of 12 billion light years from Earth, this is the most distant jet ever detected. The discovery of this jet is especially significant because it provides astronomers with a way to measure the intensity of the cosmic background radiation about one billion years after the Big Bang.

Quasars are thought to be galaxies that harbor an active central supermassive black hole fueled by infalling gas and stars. This accretion process is often observed to be accompanied by powerful high-energy jets, which is depicted in the artist's illustration.

As the electrons in the jet fly away from the quasar at near the speed of light, they move through the sea of cosmic background radiation left over from the hot early phase of the universe. When a fast-moving electron collides with one of these background photons, it can boost the photon's energy up into the X-ray band.

The observed X-ray brightness of the jet, which depends on the power in the electron beam and the intensity of the background radiation, is consistent with the predictions of the standard Big Bang model. The jet's brightness also implies that enormous amounts of energy were deposited in the outer regions of the host galaxy of the quasar at a very early stage. This energy input could have had a profound effect on the evolution of the galaxy by triggering the formation of stars, or inhibiting the accretion of matter from intergalactic space.

Fast Facts for GB1508+5714:
Credit  NASA/CXC/A.Siemiginowska et al.; Illustration: NASA/CXC/M.Weiss
Scale  Image (inset) is 9 arcsec per side.
Category  Quasars & Active Galaxies
Coordinates (J2000)  RA 15h 10m 02.90s | Dec +57° 02´ 43.40"
Constellation  Draco
Observation Dates  June 10, 2001
Observation Time  25 hours
Obs. IDs  2241
Color Code  Intensity
Instrument  ACIS
Also Known As QSO 1508+5714
References A. Siemiginowska et al. 2003 Astrophys. Journal Letters (in press); also astro-ph/0310241; W. Yuan et al; 2003 Monthly Notices Roy. Astron. Soc. (in press); astro-ph/0309318 C. Cheung astro-ph/0310733
Distance Estimate  12 billion light years (redshift z = 4.3)
Release Date  November 17, 2003