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Infrared emission associated with chemical reactions on Shuttle and SIRTF surfacesThe infrared intensities which would be observed by the Shuttle Infrared Telescope Facility (SIRTF), and which are produced by surface chemistry following atmospheric impact on SIRTF and the shuttle are estimated. Three possible sources of reactants are analyzed: (1) direct atmospheric and scattered contaminant fluxes onto the shuttle's surface; (2) direct atmospheric and scattered contaminant fluxes onto the SIRTF sunshade; and (3) scattered fluxes onto the cold SIRTF mirror. The chemical reactions are primarily initiated by the dominent flux of reactive atomic oxygen on the surfaces. Using observations of the optical glow to constrain theoretical parameters, it is estimated for source (1) that the infrared glow on the SIRTF mirror will be comparable to the zodiacal background between 1 and 10 micron wavelengths. It is speculated that oxygen reacts with the atoms and the radicals bound in the organic molecules that reside on the shuttle and the Explorer surfaces. It is concluded that for source (2) that with suitable construction, a warm sunshade will produce insignificant infrared glow. It is noted that the atomic oxygen flux on the cold SIRTF mirror (3) is insufficient to produce significant infrared glow. Infrared absorption by the ice buildup on the mirror is also small.
Document ID
19840014447
Acquisition Source
Legacy CDMS
Document Type
Technical Memorandum (TM)
Authors
Hollenbach, D. J.
(NASA Ames Research Center Moffett Field, CA, United States)
Tielens, Alexander G. G. M.
(NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
September 4, 2013
Publication Date
March 1, 1984
Subject Category
Space Sciences (General)
Report/Patent Number
A-9595
NASA-TM-85875
NAS 1.15:85875
Accession Number
84N22515
Funding Number(s)
PROJECT: RTOP 188-41-23-01
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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