Chandra X-ray Observatory (AXAF) Processing - KSC Video Feeds
Views of Chandra X-ray Observatory (AXAF) in VPF
Chandra is one of NASA's great observatories. In energy sensing range it
falls between the Hubble
Space Telescope (HST) and the Gamma Ray Observatory (GRO).
This facility will be available to scientists in the United States and
to the international astronomical community over an anticipated
mission lifetime of at least 5 years. The objective of AXAF is to make
astrophysical observations in the 0.09 to 10.0 keV energy range in
order to
- determine the nature of celestial objects from normal stars to quasars
- understand the nature of physical processes which take place in and between astronomical objects
- understand the history and evolution of the universe
Chandra X-ray Observatory (AXAF) is scheduled for launch in July of 1999 on Space Shuttle Columbia (STS-93) and an IUS upper stage , and will be placed in a highly elliptical orbit (10,000 x 140,000km) at 28.5
degrees initial inclination.
Chandra X-ray Observatory (AXAF) Newsroom Home Page
Chandra X-ray Observatory Center Home Page
Other KSC Live Video Feeds
Kennedy Space Center Home page