Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aas...203.3819f&link_type=abstract
American Astronomical Society Meeting 203, #38.19; Bulletin of the American Astronomical Society, Vol. 35, p.1263
Astronomy and Astrophysics
Astronomy
Scientific paper
The next generation of optical/IR telescopes will require large numbers of co-phased mirror segments. Therefore, some form of replication technology is desirable to reduce costs. Eletroforming has the advantage that it is a commercially developed technology for replication, and the technology has been widely used for making X-ray mirrors (e.g. XMM-Newton). Composite materials are appealing, since a great deal of development work has been done with composites as well. There are 3 areas that need to be addressed: replication with minimal stress so as to produce a high quality figure; attachment of support of the mirror segment so as to maintain the figure quality; thermal control requirements. Here we present a discussion of the requirements that lead us to select replication as the fabrication technology and the advantages of replication. We report on our first results of making a concave and flat mirrors.
This work was funded by a NASA Space Grant to Illinois, Ball Aerospace, Northwestern University, NASA Contract NAS1-03007, an AFOSR Contract F4620-C-0073, and a NASA Grant NAG5-03069.
Baker Daniel
Echt J.
Farber Miriam
Graham Michael E.
Ulmer Melville P.
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