Submillimeter Wave Astronomy Satellite


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SCIENCE OBJECTIVES

By observing spectral lines emanating from dense molecular clouds, SWAS will:

  • Determine the composition of interstellar clouds
  • Establish the means by which they cool as they collapse and form planets
INSTRUMENT
Orbit Average Power: 59 W (includes heater power)
Primary Mirror: 68 x 58 cm polished aluminum
Receiver: 490 - 550 GHz
CCD Imager: 1400-pixel, each pixel @1MHz
  • Off-axis Cassegrain telescope - Ball
  • Submillimeter Wave Receiver Subsystem - Millitech
  • Acousto-Optical Spectrometer - University of Cologne

MISSION FACTS
Mission Duration: 2 years
Orbit: 600 x 600 km, 70° inclination
Spacecraft Weight/Power: 397 lbs./270 W
Instrument Weight: 225 lbs.
Launch Vehicle: Pegasus XL
Launch Site: Western Range/Vandenberg AFB
Launch Date: December 2, 1998

SPACECRAFT
SMEX Computer System: 80386/80387 processor, 88 MBytes solid-state recorder, 1553 Data Bus
Communication System: S-Band transponder, 2 Kbps uplink, 1.8 Mbps downlink
Attitude Control System: 8085 processor, analog acquisition, 3-axis pointer, zero-momentum biased, Elevation on-source pointing accuracy 38 arc-seconds Azimuth on-source pointing accuracy 19 arc-minutes
SMEX Power Electronics: Direct Energy Transfer, full-array shunting, V/T and AHI battery charge control
Mechanical Structure: Machined aluminum
Battery: 21 Ah "Super" Nickel Cadmium
Solar Arrays: Gallium Arsenide solar cells, body-mounted and deployed panels 600 W BOL power
ACS Actuators: 4 reaction/momentum wheels 3 magnetic torque rods
ACS Sensors: 3-axis magnetometer, 3 inertial gyros, 1 high accuracy CCD star tracker, 1 digital Sun sensor, 6 coarse Sun sensors, 1 bright object sensor

Latest Mission Information
Launch Site
Smithsonian Astrophysical Observatory
Mission Operations
Swas Schedules:
SWAS Re-integration
SWAS R-Day

The Science

The SWAS instrument is a submillimeter wave telescope that incorporates dual heterodyne radiometers and an acousto-optical spectrometer to investigate the composition of dense interstellar clouds. The instrument weighs 102 kg and attaches to the top of the spacecraft structure as a single module. The total observatory mass is 288 kg. The SWAS mission will operate in a 600 km circular orbit with a 70° inclination.

SWAS is a three-axis-stabilized, stellar-pointed observatory with a pointing accuracy of 38 arcseconds and jitter less than 19 arcseconds. The spacecraft will typically point the science instrument at 3-5 targets per orbit. Target selection is constrained so that the solar arrays always face within ±15° of the Sun, except during eclipse. The Principal Investigator will generate the observation timeline and select the navigation guide stars. Using this timeline, the spacecraft, without ground intervention, will "nod" from an on-source target position to an off-source instrument calibration position up to three degrees away under 15 seconds. This nodding occurs approximately every 40 seconds. Attitude control, including pointing and nodding, is accomplished by using three magnetic-torquer coils, one digital Sun sensor, six coarse Sun sensors, four reaction wheels, one magnetometer, three inertial gyros and a high accuracy CCD star tracker. The Attitude Control System (ACS) uses the Spacecraft Computer System (SCS) processor to perform closed loop attitude determination and control.

Four deployable, fixed solar panels and one body-mounted panel contain 3.4 m2 of solar cells and provide 230 W of orbital average power that is distributed to the spacecraft and instrument. The orbit average power consumption of the spacecraft hardware is 150 W. The instrument consumes 59 W.

The data system for the SWAS mission contains 110 Mbps of bulk memory. It utilizes the MIL-STD-1553 data bus to communicate with the subsystems and the instrument. Instrument data is collected at approximately 12 Kbps average rate. Dual quadrifilar antennas are used for ground communications. The stored data is transferred to the ground at 1.8 Mbps. Commands are uplinked at 2 Kbps.


Author: Jim Watzin (jim.watzin@gsfc.nasa.gov)
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The last time this page was updated was 11/19/97.