Abstract
Fabrication of a 92cm diameter light-weight F/2 paraboloid vacuum ultraviolet telescope mirror to be utilized on an early Spacelab Mission for investigation of ultraviolet emissions from galaxies, stars, planets and comets from 900 Å to 2,000 Å will be discussed. Dr. William G. Fastie, of The Johns Hopkins University, will be Principal Investigator.
© 1980 Optical Society of America
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