Submillimeter-wave astronomy satellite

Gary J. Melnick

doi:10.1117/12.148072

15 July 1993 Submillimeter-wave astronomy satellite

Gary J. Melnick

Proceedings Volume 1874, Infrared and Millimeter-Wave Engineering; (1993) https://doi.org/10.1117/12.148072
Event: OE/LASE'93: Optics, Electro-Optics, and Laser Applications in Scienceand Engineering, 1993, Los Angeles, CA, United States

Abstract

The submillimeter wavelength range (100 micrometers <EQ (lambda) <EQ 1 mm) is exceptionally rich in atomic and molecular transitions that provide direct measures of the chemical composition, temperature, density, and cooling of the interstellar medium. In part, this is due to the fact that the most abundant oxygen- and carbon-bearing species as well as the most common hydrides have their lowest lying transitions within this wavelength region. However, because of the great abundance of many of these same species in our own atmosphere (e.g., H₂O and O₂), terrestrial absorption at submillimeter wavelengths is strong, rendering much of the sky inaccessible to ground- and even airborne observing platforms. In recognition of the scientific importance of the submillimeter range to astronomy and the limitations placed on its pursuit by the atmosphere, both NASA and ESA have embarked on ambitious programs to explore these wavelengths from space. The Submillimeter Wave Astronomy Satellite (SWAS), part of NASA's Small Explorer Program, is the first of these endeavors. During its planned 3-year lifetime, SWAS will survey dense ((eta) _H(2) > 10³ cm^-3) molecular clouds and cloud cores within our galaxy in five astrophysically important transitions of H₂O, H₂ ¹⁸O, O₂, CI, and ¹³CO. SWAS is scheduled for launch in 1995.

Citation Download Citation

Gary J. Melnick "Submillimeter-wave astronomy satellite", Proc. SPIE 1874, Infrared and Millimeter-Wave Engineering, (15 July 1993); https://doi.org/10.1117/12.148072

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KEYWORDS

Clouds

Receivers

Spectroscopy

Mirrors

Oxygen

Infrared radiation

Astronomy

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