Chandra
Advanced X-ray Astrophysics Facility (AXAF), renamed Chandra X-ray
Observatory, as the nickname of Subrahmanyan Chandrasekhar, a nobel price
holder which studied evolution of stars.
Designed to observe X-rays from high energy regions of the universe, such as
hot gas in the remnants of exploded stars.
The launch was delayed several time, including in Jan 1999 when TRW reported
conductivity problems on multi-layered circuit boards.
The satellite is suffering from a build-up of grease on an optical filter in
front of one of Advanced CCD Imaging Spectrometer, blocking almost half the
light at some frequencies. A heater might be used in spring 2004 to bakeout the
lubricant.
http://xrtpub.harvard.edu/pub.html
http://asc.harvard.edu/
http://chandra.harvard.edu/
sat-index articles
Prime
contractor
|
TRW
|
Platform
|
|
Mass
at launch
|
5200
kg
|
Mass
in orbit
|
|
Dimension
|
15
m deployed
|
Solar
array
|
9
m span
|
Stabilization
|
|
DC
power
|
|
Design
lifetime
|
5
years
|
10 m focal length telescope
ACIS: camera with 10 X-ray CCD imagers based on
Astro D
technology
HRC: camera similar to
Rosat
technology