<title>Submillimeter-wave astronomy satellite: science objectives and instrument description</title>

Abstract

The Submillimeter Wave Astronomy Satellite (SWAS) mission is dedicated to the study of star formation and interstellar chemistry. To carry out this mission, SWAS will survey dense [n(H2) greater than 103 cm-3) molecular clouds within our galaxy in either the ground-state or a low- lying transition of five astrophysically important species: H2O, H218O, O2, CI, and 13CO. By observing these lines SWAS will: (1) test long-standing theories that predict that these species are the dominant coolants of molecular clouds during the early stages of their collapse to form stars and planets; and (2) supply heretofore missing information about the abundance of key species central to the chemical models of dense interstellar gas. SWAS will employ two independent Schottky barrier diode mixers, passively cooled to approximately 170 K, coupled to a 53 X 68-cm off- axis Cassegrain antenna with an aggregate surface error less than or equal to 11 micrometer rms. During its baseline two- year mission, SWAS will observe giant and dark cloud cores with the goal of detecting or setting an upper limit on the water and molecular oxygen abundance of 3 X 10-6 (relative to H2). In addition, advantage will be taken of SWAS's relatively large beamsize of 3.3 X 4.2 arcminutes at 557 GHz and 3.8 X 4.8 arcminutes at 492 GHz to obtain large-area (approximately 1 degree X 1 degree) maps of giant and dark clouds in the 13CO and CI lines. With the use of a 1.4 GHz bandwidth acousto-optical spectrometer, SWAS will have the ability to simultaneously observe the H2O, H218O, O2, CI, and 13CO lines. All measurements will be conducted with a velocity resolution of less than 1 km s-1.© (1998) COPYRIGHT SPIE--The International Society for Optical Engineering. Downloading of the abstract is permitted for personal use only.