Concepts for a large telescope in space with interferometric imaging

Details Concepts for a large telescope in space with interferometric imaging Concepts for a large telescope in space with interferometric imaging

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986aiaa.meetq....b&link_type=abstract

AIAA, Aerospace Sciences Meeting, 24th, Reno, NV, Jan. 6-9, 1986. 7 p.

Physics

Optics

Cassegrain Optics, Design Analysis, Interferometry, Reflecting Telescopes, Spaceborne Telescopes, Geosynchronous Orbits, High Resolution, Imaging Techniques, Mirrors

Scientific paper

A candidate for the successor to the Hubble Space Telescope is presented. The telescope is a traditional Cassegrain with a 10-meter diameter monolithic primary, passively cooled optics and a wavelength coverage from the far ultraviolet to mid-infrared. Diffraction-limited imagery is achieved in the visible and ultraviolet through interferometric techniques. The observatory is located in the geosynchronous orbit to minimize environmental constraints and increase observing efficiency.

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