SKYLAB ultraviolet stellar astronomy experiment S019

Details SKYLAB ultraviolet stellar astronomy experiment S019 SKYLAB ultraviolet stellar astronomy experiment S019

Apr 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977apopt..16..973o&link_type=abstract

Applied Optics, vol. 16, Apr. 1977, p. 973-977.

Astronomy and Astrophysics

Astronomy

1

Skylab Program, Spaceborne Astronomy, Stellar Spectrophotometry, Ultraviolet Spectrometers, Absorption Spectra, Calcium Fluorides, Lens Design, Lithium Fluorides, Mirrors, Photographic Film, Prisms, Reflecting Telescopes, Spectral Line Width, Ultraviolet Spectroscopy

Scientific paper

An objective-prism stellar spectrograph of 15-cm aperture was flown on all three Skylab missions. The wavelength region from 1300 A to 5000 A was covered by a special optical system containing a combination of reflecting telescope optics, a CaF2 objective prism, and an achromatized field-corrector lens system of CaF2 and LiF. Observations of 188 star fields, each covering 4.0 x 5.0 deg of arc, were conducted at the Skylab antisolar airlock with the aid of an articulated mirror system which allowed acquisition within a 30 by 360 deg band of the sky.

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