Extremely lightweight space telescope mirrors with integrated active figure control.

Computer Science

Scientific paper

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Space Telescopes: Optical Design, Space Telescopes: Mirrors

Scientific paper

A concept for an extremely light weight primary mirror for a large space telescope is proposed. The mirror uses a sandwich structure composed of aluminum faceplates with an aluminum foam core. Modal analysis indicates that a fundamental frequency of 100 Hz can be obtained for a 6 meter diameter mirror with a tapered back and having a total mass of about 3500 kg. An array of thermal actuators embedded in the mirror corrects for figure errors.

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