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Ice in space: An experimental and theoretical investigationThe thermodynamics of water ice formation was experimentally investigated under a wide variety of conditions, including those of outer space. This information, and in particular, the lifetime of ice particles as a function of solar distance is an absolute requirement for proper interpretation of photometric profiles of comets. The sublimation of ice particles in a nonequilibrium situation was studied. An oscillating fiber microbalance was used to measure the sublimation rate of water droplets (which were suspended on a long quartz fiber which was oscillating in a vacuum chamber). The influence of particle size, surface temperature, and the index refraction from simulated solar radiation were studied in relation to ice formation. Also examined was the influence of impurities (clathrates) on ice formation. Windows in the vacuum chamber allowed the ice particles to be exposed to a 1 kilowatt xenon arc lamp which was used to simulate solar radiation. Ice is proposed as a possible energy source for comets, as amorphous water ice and ammonia in low temperature and pressure environments demonstrated a clear energy release upon warming. Motion pictures of ice formation were taken and photographs are shown.
Document ID
19760016029
Acquisition Source
Legacy CDMS
Document Type
Contractor Report (CR)
Authors
Patashnick, H. (Dudley Observatory Albany, NY, United States)
Rupprecht, G. (Dudley Observatory Albany, NY, United States)
Date Acquired
September 3, 2013
Publication Date
March 8, 1976
Subject Category
Astrophysics
Report/Patent Number
NASA-CR-144273
Accession Number
76N23117
Funding Number(s)
CONTRACT_GRANT: NAS8-30566
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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