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POST: A Polar Stratospheric Telescope for the Antarctic

Published online by Cambridge University Press:  25 April 2016

Michael A. Dopita ,
Holland C. Ford ,
John Bally  and
Pierre Bely
Michael A. Dopita
Affiliation:
Mount Stromlo and Siding Spring Observatories, Institute of Advanced Studies, Australian National University, Private Bag, Weston Creek PO, ACT 2611, Australia. [email protected]
Holland C. Ford
Affiliation:
Johns Hopkins University, Baltimore, MD 21218, USA
John Bally
Affiliation:
Astrophysical, Planetary, and Atmospheric Sciences Department, University of Colorado, Boulder, CO 80309, USA
Pierre Bely
Affiliation:
Space Telescope Science Institute, Baltimore, MD 21218, USA
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Abstract

The tropopause, typically at 16 to 18 km altitude at the lower latitudes, dips down to only 8 km in the polar regions, allowing access to the cold, dry and nonturbulent lower stratosphere by tethered aerostats. These can float as high as 12 km, have long operating lifetimes, and are extremely reliable. In contrast to free-flying balloons, they can stay on station for weeks at a time, and payloads can be safely recovered for maintenance and adjustment and relaunched in a matter of hours. We propose to use such a platform, located first near Fairbanks, Alaska, and later in the Antarctic, to operate a new-technology 4 m telescope with diffraction-limited performance in the near infrared. Thanks to the low ambient temperature (~200 K), thermal emission from the optics is of the same order as that of the zodiacal light in the 2–3 μm band. Since this wavelength interval is the darkest part of the zodiacal light spectrum from optical wavelengths to 100 μm, the combination of high-resolution images and a very dark sky make it the spectral region of choice for observing galaxies, QSOs and clusters of galaxies at the formation epoch of galaxies.

Keywords

Antarctic astronomyatmospheric effectsballoonsinfrared: generaltelescopes
Type
The First JACARA International Antarctic Astronomy Meeting
Information
Publications of the Astronomical Society of Australia , Volume 13 , Issue 1 , January 1996 , pp. 48 - 59
Copyright
Copyright © Astronomical Society of Australia 1996

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