Currently, scientific space missions based on interferometric optical and infrared
astronomical instruments are under development in the United States as well as in Europe.
These instruments require optical path length accuracy in the order of a few nanometres
across structural dimensions of several metres. This puts extreme demands on static and
dynamic structural stability. It is expected that actively controlled, adaptive structures will
increasingly have to be used for these satellite applications to overcome the limits of passive
structural accuracy.
Based on the evaluation of different piezo-active concepts, analysis and design of an
adaptive lightweight satellite mirror primarily made of carbon fibre reinforced plastic with
embedded piezoceramic actuators for shape control is described. Simulation of global
mirror performance takes different wavefront sensors and controls for several cases of
loading into account. Extensive finite-element optimization of various structural details was
performed while testing of active sub-components served as a basis for a final update of
finite-element models. Local material properties of sub-assemblies or geometry effects at the
edges of the structure were investigated with respect to their impact on mirror
performance.
The major result of the analysis was the lay-out of the adaptive mirror and the specific
design of embedded piezoceramic actuators. Manufacture of structural components and
successfully completed mirror integration is described. The paper concludes with an outline
of testing, and space qualification of the demonstrator of an actively controllable
lightweight satellite mirror currently under way.