A balloon-borne 1 meter telescope for far-infrared astronomy
Giovanni G. Fazio, Douglas E. Kleinmann, R. W. Noyes, EDWARD L. WRIGHT, F. J. Low
Abstract
Giovanni G. Fazio, Douglas E. Kleinmann, R. W. Noyes, EDWARD L. WRIGHT, F. J. Low
Abstract
The flight of a balloon-borne one-meter telescope for infrared astronomy in the wavelength interval of 40 to 240 microns is discussed. The gyro-stabilized telescope mapped the intensity of the far infrared radiation from NGC 7538, Mars, the Orion Nebula, and W3 with a resolution of one minute and from selected regions of these sources with a resolution of 30 seconds. The infrared detection is described and its capabilities are analyzed. The instrumentation, orientation system, and modes of observation of the telescope are defined.
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The flight of a balloon-borne one-meter telescope for infrared astronomy in the wavelength interval of 40 to 240 microns is discussed. The gyro-stabilized telescope mapped the intensity of the far infrared radiation from NGC 7538, Mars, the Orion Nebula, and W3 with a resolution of one minute and from selected regions of these sources with a resolution of 30 seconds. The infrared detection is described and its capabilities are analyzed. The instrumentation, orientation system, and modes of observation of the telescope are defined.
Key concepts: Telescope, Infrared telescope, Physics, Astronomy, Infrared astronomy, Infrared, Remote sensing, Instrumentation (computer programming)