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Author > Underhill, A. B. 

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Title: The large space telescope instrumentation.
Author(s): Underhill, A. B.
Abstract: Aspects of the Large Space Telescope project (LST) as it is developing at the Goddard Space Flight Center are presented and a brief discussion is given of the types of observing program that might be handled. The special characteristics of an LST are large light-gathering power, good spectral efficiency from 900 A to 5 microns, near diffraction limited performance, launch by the space shuttle into a low orbit like that of the Orbiting Astronomical Observatories, and a lifetime of at least 10 years. A basic set of instruments to be used with the telescope might include on-axis cameras with broad-band filter response, an imaging spectrograph, a low-resolution spectrograph, a high-resolution spectrograph, spectrum scanners, narrow-band photometers, interferometers for use in the near infrared, polarimeters for use in the ultraviolet, and provision for measuring the time variations of the light from astronomical objects on a scale of milli-seconds as well as on a scale of minutes, hours, days, and weeks.
NASA Center: Goddard Space Flight Center
Publication Date: Feb 1, 1972
Document Source: Other Sources
No Digital Version Available: Go to Tips On Ordering
Document ID: 19720042015
Accession ID: 72A25681
Publication Information: Number of Pages = 7
Keywords: NASA PROGRAMS; SPACEBORNE ASTRONOMY; TELESCOPES; CONFERENCES; LIGHT (VISIBLE RADIATION); REFLECTING TELESCOPES; SYSTEMS ENGINEERING; ULTRAVIOLET RADIATION;
Notes: (Symposium on Advanced Electronic Systems for Astronomy, Santa Cruz, Calif., Aug. 31-Sept. 2, 1971.) Astronomical Society of the Pacific, Publications, vol. 84, Feb. 1972, p. 84-90.
Accessibility: Unclassified; Copyright; Unlimited; Publicly available;
Updated/Added to NTRS: 2004-11-03

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