Lessons Learned From the Clementine Mission


3
Mission Implementation


TABLE 3.2 Clementine's Advanced Technology Components, Their Heritage, and Examples of Future Applications


Item Heritage Flown Before? Examples of
Subsequent Uses
Examples of Future Uses

Lightweight reaction wheel LOSAT-Xa (with different configuration) Yes (no information) GFO
R-3000, 32-bit
RISC Computer
Brilliant Eyes and
Brilliant Pebbles
flight test programs
No MSTI-3 Lewis, Clark
1750A Computer USAF spacecraft Yes: TAOS Milstar, NEAR, MGS IUS, MISR
GaAs/Ge Solar Arrays DOD applications
MSTI-1
Yes: classified
program
Mars Pathfinder, Soujourner,
TRACE, STRV-1B
Iridium, TRMM, GFO
Solid State Data Recorder Classified
applications
Yes (no information) NEAR, MGS Cassini, Lewis, Clark,
ACE, SBIR
Frangibolt Release
Mechanism
NRL (general
applications)
No TOMS, Mars Pathfinder STRV-2, SAPPHIRE,
Lewis, Clark
Single Pressure
Vessel Battery
Communications
satellite industry
No MGS Iridium, Lewis, Clark
Inertial Measurement Unit THAAD, LEAP No Derivative of instrument
on missiles flight test
program
Deep Space 1, LMLV,
DOD applications including
Apache helicopter
Data-compression Chipsa CNES program Cassini
Star TrackerBrilliant Pebbles
flight test program
Yes: early version
on BMDO suborbital flights
Bitsy, Mars Surveyor 1998
Orbiter and Lander
Ultraviolet/Visible Imager Brilliant Pebbles
flight test program
Yes: early version
on BMDO suborbital flights
High-Resolution
Imager/Lidar Receiver
Brilliant Pebbles
flight test program
Yes: early version on
BMDO suborbital flights
Laser Transmitter Brilliant Pebbles
flight test program
No
Near-Infrared Imager Space surveillance
applications
No
Long-wave Infrared Imager No No

NOTE: Abbreviations and acronyms are defined in the glossary.

aInformation on the data-compression chips could not be confirmed, but the entries are consistent with information presented by Jacques Blamont (Centre National d'Etudes Spatiales) at the July 1994 Clementine Engineering and Technology Workshop.

SOURCE: Information and choice of entries based on material initially supplied by Paul Regeon, Clementine program manager at the Naval Research Laboratory, and later updated with additional material supplied by Stewart Nozette and David Barnhart of the Clementine II team at the U.S. Air Force's Phillips Laboratory. Individual entries were confirmed and updated, whenever possible, by members of the relevant mission teams or the manufacturer of individual components.


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