SWAS
Submillimeter Wave Astronomy Satellite, also called SMEX 3
The SWAS mission is an outgrowth of the scientific interest in the exploration
of the submillimeter wavelength region for astronomy. SWAS will be a
pioneering step in submillimeter astronomy in space. The SWAS mission is
designed to study molecular clouds in the galactic plane, providing a mini and
full survey of the clouds, leading towards the development of maps. It will
also perform quick-look chemistry on the structure and content of these
molecular clouds, and will research extragalactic sources.
After being desactivated in 2004, the satellite was reactivated in Jun 2005 to
monitor comet Tempel 1 after its impact with Deep Impact. It should be
desactivated again in Aug 2005.
http://sunland.gsfc.nasa.gov/smex/swas/
http://cfa-www.harvard.edu/cfa/oir/Research/swas.html
sat-index articles
Prime
contractor
|
|
Platform
|
|
Mass
at launch
|
288
kg
|
Payload
mass
|
102
kg
|
Dimension
|
|
Solar
array
|
|
Stabilization
|
3-axis
|
DC
power
|
230
W
|
Design
lifetime
|
2
years
|
Telemetry: 2215 MHz (realtime: 18.75 kbps, playback: 1.8 Mbps), 5 W
transmitter
Command: 2039.65 MHz (2 kbps)
The instrument consists of an off-axis Cassegrain telescope, receiver,
Acousto-Optical Spectrometer (AOS), instrument control electronics (ICE) and a
thermal control subsystem.
The satellite has a 0.6m telescope with a 490 to 550 GHz submillimeter receiver
and an acousto-optical spectrometer.