An overview of the Chandra mission and goals, Chandra's namesake, top 10 facts.
Classroom activities, printable materials, interactive games & more.
Overview of X-ray Astronomy and X-ray sources: black holes to galaxy clusters.
All Chandra images released to the public listed by date & by category
Current Chandra press releases, status reports, interviews & biographies.
A collection of multimedia, illustrations & animations, a glossary, FAQ & more.
A collection of illustrations, animations and video.
Chandra discoveries in an audio/video format.
Q&A: Chandra Mission

Q:
Can Chandra calculate red shift data of objects?

A:
NGC 4151
HETG Spectrum
of NGC 4151
GRB 991216
ACIS Spectrum
of GRB 991216
Yes. The ability of the transmission gratings on Chandra to make fine distinctions between the energies of the X-rays from an object makes it possible to identify sharp peaks or lines in the spectrum due to ions of oxygen, silicon, iron, etc. if they are present. By comparing the observed energy or wavelength of these peaks with the corresponding values observed in the laboratory, the red shift can be measured. A rough measurement (within 5 or 10%) of the red shift can be made with the Advanced CCD Imaging Spectrometer (ACIS) without the gratings. In practice the red shifts determined by Chandra are used as a confirmation of the red shifts measured by optical telescopes. A notable exception is the red shift measured from the X-ray afterglow of the gamma ray burst GRB 991216.


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