A submillimeter mission for the 1990s: SMMM

Astronomy and Astrophysics – Astronomy

Scientific paper

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Bolometers, Explorer Satellites, Fabry-Perot Spectrometers, Spaceborne Astronomy, Spaceborne Telescopes, Spacecraft Design, Spectroscopic Telescopes, Submillimeter Waves, Heterodyning, Josephson Junctions, Line Spectra, Mission Planning, Radio Receivers, Sis (Superconductors)

Scientific paper

The detailed design and science rationale for the Explorer or submillimeter moderate mission (SMMM) is presented. Equipped with a 4 m class telescope, the SMMM mission follows the Explorer submillimeter wave astronomy satellite (SWAS) mission, equipped with a 55 cm diameter telescope, and precedes the Large Deployable Reflector (LDR) mission with a 210 m telescope. The submillimeter spectroscopy and far infrared continuum studies of all these missions are carried out using ambient temperature telescopes. The instrumentation of SMMM is cooled to liquid helium temperatures and includes a high resolution spectrometer using superconductor insulator superconductor (SIS) receivers for the 300 to 600 micrometer band. A Fabry-Perot spectrometer with an array of bolometer detectors is used for the 100 to 300 micrometer band and an array of bolometers is used for continuum studies in the 100 to 800 micrometer band.

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