The Formation and Stability of Carbonic Acid on Outer Solar System Bodies
The radiation chemistry, thermal stability, and vapor pressure of solid-phase carbonic acid (H2CO3) have been studied with mid-infrared spectroscopy. A new procedure for measuring this molecule's radiation stability has been used to obtain intrinsic IR band strengths and half-lives for radiolyt...
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ftnasantrs:oai:casi.ntrs.nasa.gov:20090033103 2023-05-15T15:52:10+02:00 The Formation and Stability of Carbonic Acid on Outer Solar System Bodies Hudson, R. L. Peeters, Z. Moore, M. H. Lewis, Ariel Unclassified, Unlimited, Publicly available [2009] application/pdf http://hdl.handle.net/2060/20090033103 unknown Document ID: 20090033103 http://hdl.handle.net/2060/20090033103 Copyright, Distribution as joint owner in the copyright CASI Space Sciences (General) 2009 ftnasantrs 2018-06-09T22:58:22Z The radiation chemistry, thermal stability, and vapor pressure of solid-phase carbonic acid (H2CO3) have been studied with mid-infrared spectroscopy. A new procedure for measuring this molecule's radiation stability has been used to obtain intrinsic IR band strengths and half-lives for radiolytic destruction. Results are compared to literature values. We report, for the first time, measurements of carbonic acid's vapor pressure and its heat of sublimation. We also report the first observation of a chemical reaction involving solid-phase carbonic acid. Possible applications of these findings are discussed, with an emphasis on the outer Solar System. Other/Unknown Material Carbonic acid NASA Technical Reports Server (NTRS) |
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Open Polar |
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NASA Technical Reports Server (NTRS) |
op_collection_id |
ftnasantrs |
language |
unknown |
topic |
Space Sciences (General) |
spellingShingle |
Space Sciences (General) Hudson, R. L. Peeters, Z. Moore, M. H. Lewis, Ariel The Formation and Stability of Carbonic Acid on Outer Solar System Bodies |
topic_facet |
Space Sciences (General) |
description |
The radiation chemistry, thermal stability, and vapor pressure of solid-phase carbonic acid (H2CO3) have been studied with mid-infrared spectroscopy. A new procedure for measuring this molecule's radiation stability has been used to obtain intrinsic IR band strengths and half-lives for radiolytic destruction. Results are compared to literature values. We report, for the first time, measurements of carbonic acid's vapor pressure and its heat of sublimation. We also report the first observation of a chemical reaction involving solid-phase carbonic acid. Possible applications of these findings are discussed, with an emphasis on the outer Solar System. |
author |
Hudson, R. L. Peeters, Z. Moore, M. H. Lewis, Ariel |
author_facet |
Hudson, R. L. Peeters, Z. Moore, M. H. Lewis, Ariel |
author_sort |
Hudson, R. L. |
title |
The Formation and Stability of Carbonic Acid on Outer Solar System Bodies |
title_short |
The Formation and Stability of Carbonic Acid on Outer Solar System Bodies |
title_full |
The Formation and Stability of Carbonic Acid on Outer Solar System Bodies |
title_fullStr |
The Formation and Stability of Carbonic Acid on Outer Solar System Bodies |
title_full_unstemmed |
The Formation and Stability of Carbonic Acid on Outer Solar System Bodies |
title_sort |
formation and stability of carbonic acid on outer solar system bodies |
publishDate |
2009 |
url |
http://hdl.handle.net/2060/20090033103 |
op_coverage |
Unclassified, Unlimited, Publicly available |
genre |
Carbonic acid |
genre_facet |
Carbonic acid |
op_source |
CASI |
op_relation |
Document ID: 20090033103 http://hdl.handle.net/2060/20090033103 |
op_rights |
Copyright, Distribution as joint owner in the copyright |
_version_ |
1766387445436252160 |