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Delta
Successfully Launches IMAGE
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A
Boeing Delta 2 7326 rocket successfully launched
NASA's IMAGE satellite at 12:34 p.m. PST (2034:43
UTC) March 25 from Vandenberg’s SLC 2W launch pad. NASA's
Imager for Magnetopause-to-Aurora Global Exploration (IMAGE)
spacecraft will operate in a highly elliptical orbit around the
Earth's poles. During its two-year research mission, the satellite
will take images of the planet's magnetosphere.
The total cost for the IMAGE mission, including satellite
(US$82 M),
Delta 2 launch (US$50 M), and two years of operations (US$21.5 M) is about US$154
million. IMAGE is NASA’s first Medium-class Explorer (MIDEX)
mission.
The initial
parking orbit was reported to be near perfect, with an apogee of 1076
km (581 nmi), a perigee of 185 km (99.9 nmi) and an orbital
inclination at the desired 93.9°.
The mission orbit will
have an
apogee of 45,922 km, with a perigee of 1000 km. The initial apogee
will be at 40 degrees north latitude. During the first year of the
two-year mission, the apogee will precess from 40 to 90 degrees
north latitude, that is, to a position directly over the north
pole; it will continue to precess until it returns to ~40 degrees
by the end of the mission. Because of the Earth's annual motion
about the Sun, IMAGE will be able to view each local time from
apogee twice during the mission. IMAGE will complete one orbit
every 14.2 hours.
The Southwest
Research Institute (SRI), San Antonio, Texas, leads the IMAGE
science mission for NASA. Lockheed
Martin Missiles and Space, Sunnyvale, Calif. built the IMAGE
spacecraft under contract to SRI. The
IMAGE observatory is a spin-stabilized spacecraft that, at launch,
measured 2.25 m (7.4 ft) in diameter and 1.52 m (4.99 ft) in
height and weighed 494 kg (1087 lbm). On orbit, the
antennas aboard IMAGE will extend 10.1 m (33 ft) parallel to the
spin axis and 249.9 m (820 ft) in four directions perpendicular to
the spin axis. The
satellite has the form of a regular octagon. Arrays of
high-efficiency, dual-junction gallium-arsenide solar cells
attached to the spacecraft's eight side and two end panels provide
power to the scientific instruments and subsystems, which together
will require an orbit-averaged power of 250 Watts. When the
spacecraft is in eclipse, power is provided by a Super
Nickel-Cadmium battery. IMAGE has a nominal spin period of 2
minutes (a spin rate of 0.5 ± 0.01 rpm); its spin axis is
perpendicular to the orbital plane.
The Principal
Investigator of the mission is Dr. James Burch of the Southwest
Research Institute. IMAGE uses six state-of- the-art instruments
along with a data processor. The instruments and their developers
are:
- High
Energy Neutral Atom (HENA) imager, developed by Johns Hopkins
University Applied Physics Laboratory, Laurel, MD
- Medium
Energy Neutral Atom (MENA) imager, developed by SRI
- Low
Energy Neutral Atom (LENA) imager, developed by NASA Goddard
- Extreme
Ultraviolet (EUV) imager, developed by the University of
Arizona, Tucson
- Far
Ultraviolet (FUV) imager, developed by the University of
California at Berkeley
- Radio
Plasma Imager (RPI), developed by the University of
Massachusetts at Lowell
- Central
Instrument Data Processor (CIDP) developed by SRI
More Information:
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2000 SPACEandTECH
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