Paper
30 January 2003 Ultra-lightweight 4-meter segmented composite mirrors for extremely large telescopes
Author Affiliations +
Abstract
Presented is a lightweight mirror compatible with the extremely large telescopes being proposed. The mirror exhibits an areal density of less than 12 kg/m2, which is the same relative areal density as the primary mirrors on the 100-meter Robert Byrd Radio Telescope. The panels can be fabricated in 2.5-meters diameter with traceability to 4-meters. Presented are preliminary results of a set of large demonstrator mirrors, their characteristics and traceability to producing 4-meter low-cost and easily fabricated mirror segments for large telescopes.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Robert C. Romeo and Peter C. Chen "Ultra-lightweight 4-meter segmented composite mirrors for extremely large telescopes", Proc. SPIE 4840, Future Giant Telescopes, (30 January 2003); https://doi.org/10.1117/12.459865
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Mirrors

Composites

Large telescopes

Telescopes

Spherical lenses

Glasses

Optical fibers

RELATED CONTENT

Variable-curvature mirrors for the VLTI
Proceedings of SPIE (July 24 1998)
Precision thermal control trades for telescope systems
Proceedings of SPIE (August 28 1998)
Composite technology for lightweight optical mirrors
Proceedings of SPIE (July 01 1990)
UltraLITE glass/composite hybrid mirror
Proceedings of SPIE (July 28 2000)
Large Optical Generator
Proceedings of SPIE (December 09 1983)

Back to Top