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Extreme ultraviolet survey experiment MA-083A grazing incidence telescope sensitive to radiation in the 5- to 100-nanometer band was flown in the Apollo service module. On 10 nighttime revolutions, the command and service module was maneuvered to point the instrument at 30 different stellar targets for periods of 1 to 20 minutes, thus constituting the first sensitive search for extreme ultraviolet radiation from nonsolar sources. Several hours of supplementary data were also obtained during nighttime orbits when other experiments in the scientific instrument module bay were operating. Preliminary analysis of a small fraction of the total data indicates the definite detection of a strong source of extreme ultraviolet radiation during observations made during revolution 109. The source is located in Coma Berencies. The suggested optical identification is the white dwarf HZ 43. If this association is correct, the star has the highest temperature of any known white dwarf. Regardless of the optical identification, however, this object is the first nonsolar source to be detected in the extreme ultraviolet band.
Document ID
19760015990
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Bowyer, S.
(California Univ. Berkeley, CA, United States)
Margon, B.
(California Univ. Berkeley, CA, United States)
Lampton, M.
(California Univ. Berkeley, CA, United States)
Paresce, F.
(California Univ. Berkeley, CA, United States)
Stern, R.
(California Univ. Berkeley, CA, United States)
Date Acquired
August 8, 2013
Publication Date
February 1, 1976
Publication Information
Publication: NASA. Lyndon B. Johnson Space Center Apollo-Soyuz Test Project
Subject Category
Space Radiation
Accession Number
76N23078
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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