Prediction and reduction of space structure vibrations have become cri
tical issues over the last ten years. Motivating factors include optic
al systems with high stability requirements, large antennas, sensitive
micro gravity payloads, compatibility of flexible appendages with att
itude control, and large orbital infrastructure surviving. The experim
ent ''CASTOR'' (French acronym for ChAracterisation of STructures in O
Rbit) is dedicated to the identification of the structural dynamic mod
es of the MIR station and to the investigation of the dynamic behaviou
r-in zero g conditions-of a truss mock-up equipped with various passiv
e and active damping technologies. The measured modal parameters of MI
R are to be compared with the results of a finite element model analys
is. The differences between in-flight and on-ground dynamics of the tr
uss will be thoroughly analysed. This project has been conceived and i
s managed by CNES. The flight hardware will be delivered by the end of
1995, and the experimental work will be performed by a French cosmona
ut within the framework of the CASSIOPEE mission in June 1996. In the
first place, a comprehensive overview of CNES activities in the predic
tion of in-flight structural dynamics, and of similar experimental eff
orts found in literature will be discussed. Afterwards, the motivation
s behind the CASTOR experiment will be shown, followed by a full descr
iption of its equipment. The results of the ground tests and analyses,
and the in-orbit test plan will then be presented extensively. Partic
ular emphasis will be laid on the performances of the active damping s
ystems which will be validated in flight. In conclusion, the potential
re-utilisation of the experiment material within the framework of lat
er flights will be highlighted. (C) 1997 Elsevier Science Ltd.