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The Apollo lunar surface water vapor event revisitedOn March 7, 1971, the first sunrise following the Apollo 14 mission, the Suprathermal Ion Detector Experiment (SIDE) deployed at the Apollo 14 site reported an intense flux of ions whose mass per charge was consistent with water vapor. The amount of water is examined, and the various acceleration processes, responsible for accelerating ions into the SIDE, are discussed. It is concluded that during most of the event the observed water vapor ions were accelerated by the negative lunar surface electric potential and, secondly, that this event was probably the result of mission associated water vapor, either from the LM ascent and descent stage rockets or from residual water in the descent stage tanks.
Document ID
19920030338
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Freeman, J. W., Jr.
(Rice University Houston, TX, United States)
Hills, H. K.
(NASA Goddard Space Flight Center; Hughes STX Corp. Greenbelt, MD, United States)
Date Acquired
August 15, 2013
Publication Date
November 1, 1991
Publication Information
Publication: Geophysical Research Letters
Volume: 18
ISSN: 0094-8276
Subject Category
Lunar And Planetary Exploration
Accession Number
92A12962
Distribution Limits
Public
Copyright
Other

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