HETE 2
High-Energy Transient Experiment
This satellite was funded to replace
HETE
which was lost right after launch. The launch site was chosen because it is
optimum for equatorial orbits. The mission control center was in Cape Canaveral
and communication channels were setup for remote control.
It will carry out the first multiwavelength study of gamma-ray bursts with UV,
X-ray, and gamma-ray instruments mounted on a single, compact spacecraft. A
unique feature of the HETE mission is its capability to localize GRBs with ~10
arc second accuracy, in near real time aboard the spacecraft, and to transmit
these positions directly to a network of receivers at existing ground-based
observatories, enabling rapid, sensitive follow-up studies in the radio, IR,
and optical bands.
http://nis-www.lanl.gov/nis-projects/hete/
http://space.mit.edu/HETE/
sat-index articles
Prime
contractor
|
MIT
|
Platform
|
|
Mass
at launch
|
123
kg
|
Mass
in orbit
|
|
Dimension
|
|
Solar
array
|
|
Stabilization
|
|
DC
power
|
|
Design
lifetime
|
|
Build
by
|
CESR
(France)
|
Instrument
type
|
NaI(Tl);
cleaved
|
Energy
range
|
6
keV to > 1 MeV
|
Timing
resolution
|
4
ms
|
Spectral
resolution
|
~40%
@ 6 keV; ~7% @ 662 keV
|
Effective
area
|
120
cm^2
|
Sensitivity
(10 sigma)
|
3
x 10^-8 erg/cm**2/s for 8-1000 keV
|
FOV
|
~
2 pi sr
|
Angular
resolution
|
~
1 sr
|
Build
by
|
RIKEN
(Japan) and Los Alamos
|
Instrument
type
|
Coded
Mask with Position Sensitive Proportional Counter
|
Energy
range
|
2
to 25 keV
|
Timing
resolution
|
1
ms
|
Spectral
resolution
|
~15%
@ 6 keV
|
Effective
area
|
200
cm^2 (each of 2 units)
|
Sensitivity
(10 sigma)
|
8
x 10^-9 erg/cm^2/s for 2-10 keV
|
FOV
|
~
2 sr (combined)
|
Angular
resolution (1 sigma)
|
+-6
arcmin
|
Build
by
|
MIT
CSR
|
Instrument
type
|
4
CCD20 Detectors, 2 optical CCD22
|
Energy
range
|
500
eV to 14 keV
|
Timing
resolution
|
1
s
|
Spectral
resolution
|
46
eV @ 525 eV, 129 eV @ 5.9 keV
|
Effective
area
|
6.1x6.1
cm^2 (each of 2 units)
|
FOV
|
~0.91
sr
|
Dimension
|
10
cm x 10 cm x 17.5 cm
|
The spacecraft hardware and software is being developed by Aeroastro (USA).
Downlink frequencies: 137.963, 2255.5 & 2272 MHz