Verifying mirror technology for NGST with a space-qualified, cryogenic 3.5 m mirror

Research output: Chapter in Book/Report/Conference proceedingConference contribution

1 Scopus citations

Abstract

A cryogenic 3.5 m mirror is being developed which weighs 140 kg, that could be incorporated into a telescope and launched to a high orbit by the Shuttle or number of other vehicles. Such a space mission would complement those already planned for scaled down tests of the unfolding of the next generation space telescope (NGST) mirror segments and the sunshade. Much would be learned by running the mirror at cryogenic temperature, with a new infrared array to make preliminary observations in the 2-4 μm dark sky window and a charge coupled devices to check optical image quality.

Original languageEnglish (US)
Title of host publicationEuropean Space Agency, (Special Publication) ESA SP
PublisherESA
Pages181-188
Number of pages8
VolumeSP-429
Publication statusPublished - Oct 1998
EventProceedings of the 1998 34th Liege International Astrophysics Colloquium - Liege, Belgium
Duration: Jun 15 1998Jun 18 1998

Other

OtherProceedings of the 1998 34th Liege International Astrophysics Colloquium
CityLiege, Belgium
Period6/15/986/18/98

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ASJC Scopus subject areas

  • Aerospace Engineering

Cite this

Angel, J. R. P., & Burge, J. H. (1998). Verifying mirror technology for NGST with a space-qualified, cryogenic 3.5 m mirror. In European Space Agency, (Special Publication) ESA SP (Vol. SP-429, pp. 181-188). ESA.