FUSE
Far Ultraviolet Spectroscopic Explorer
FUSE will access the wavelength below 1180 Angstroms (the
HST
STIS cutoff) with high resolution astronomical spectroscopy in the
far-ultraviolet spectral region. No long-term observatory since
Copernicus
(1972) has possessed this capability.
Total project cost: $171 million including $120 million for the satellite.
Funded by NASA. French and Canadian space agency share observation time. French
CNES paid 6 million EUR.
On 10 Dec 2001 the satellite went into safe mode when the second of 4 reaction
wheels stopped. In Feb 2002, partial usability was restored with the use of the
magnetic torquer. Full operations were restored in March 2002.
In July 2003 we learn that the gyroscopes are ageing and that software to
operate in gyroless mode was uploaded in April 2003. In this mode, the science
data is to remain the same quality.
On 27 Dec 2004 the third reaction wheel stopped. The satellite went into safe
mode. Observations resumed in November 2005 and were back to original quality
in Jan 2006. The control system has been modified again to use magnetic control
on two axes, which provides a tenuous but acceptable level of control.
Out
of service
|
Jul
2007
|
Cause
|
Last
reaction wheel failed
|
Decay
|
|
http://fuse.pha.jhu.edu/
sat-index articles
Prime
contractor
|
OSC
|
Platform
|
|
Mass
at launch
|
1360
kg
|
Mass
in orbit
|
|
Dimension
|
1.2
x 1.8 x 5.5 m
|
Solar
array
|
|
Stabilization
|
|
DC
power
|
|
Design
lifetime
|
3
years
|
Carries a telescope with 4 mirrors. It explores in the 912 to 1187 angstrom
range. The instrument is provided by the John Hopkins University.