Share Email Print

Proceedings Paper

Submillimeter Wave Astronomy Satellite
Author(s): Volker Tolls; Gary J. Melnick; Alexander Dalgarno; Giovanni G. Fazio; John R. Stauffer; Patrick Thaddeus; Neal R. Erickson; Ron L. Snell; Paul F. Goldsmith; Martin Harwit; David J. Hollenbach; David G. Koch; David A. Neufeld; Rudolf T. Schieder; Gisbert F. Winnewisser
Format Member Price Non-Member Price
PDF $17.00 $21.00

Paper Abstract

The Submillimeter Wave Astronomy Satellite (SWAS) mission will study galactic star formation and interstellar chemistry. To carry out this mission, SWAS will survey dense (nH2 > 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 dominate 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. During its two-year mission, SWAS will observe giant and dark cloud cores with the goal of detecting to setting an upper limit on the water abundance of 3 X 10-6 (relative to H2) and on the molecular oxygen abundance of 2 X 10-6 (relative to H2). SWAS is designed to carry all elements of a ground based radiotelescope. The telescope is a highly efficient 54 X 68-cm off-axis Cassegrain antenna with an aggregate surface error less than or equal to 11 micrometers rms. The receiver system consists of two independent heterodyne receivers with second harmonic Schottky diode mixers, passively cooled to approximately equals 150 K. The spectrometer is a single acousto-optical spectrometer (AOS) with 1400 1-MHz channels enabling simultaneous observations of the H2O, O2, CI, and 13CO lines.

Paper Details

Date Published: 14 September 1994
PDF: 8 pages
Proc. SPIE 2268, Infrared Spaceborne Remote Sensing II, (14 September 1994); doi: 10.1117/12.185853
Show Author Affiliations
Volker Tolls, Harvard-Smithsonian Ctr. for Astrophysics (United States)
Gary J. Melnick, Harvard-Smithsonian Ctr. for Astrophysics (United States)
Alexander Dalgarno, Harvard-Smithsonian Ctr. for Astrophysics (United States)
Giovanni G. Fazio, Harvard-Smithsonian Ctr. for Astrophysics (United States)
John R. Stauffer, Harvard-Smithsonian Ctr. for Astrophysics (United States)
Patrick Thaddeus, Harvard-Smithsonian Ctr. for Astrophysics (United States)
Neal R. Erickson, Univ. of Massachusetts (United States)
Ron L. Snell, Univ. of Massachusetts (United States)
Paul F. Goldsmith, NAIC (United States)
Martin Harwit, National Air and Space Museum (United States)
David J. Hollenbach, NASA Ames Research Ctr. (United States)
David G. Koch, NASA Ames Research Ctr. (United States)
David A. Neufeld, Johns Hopkins Univ. (United States)
Rudolf T. Schieder, Univ. zu Koeln (Germany)
Gisbert F. Winnewisser, Univ. zu Koeln (Germany)

Published in SPIE Proceedings Vol. 2268:
Infrared Spaceborne Remote Sensing II
Marija S. Scholl, Editor(s)

© SPIE. Terms of Use
Back to Top