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Evidence for first polymer in Comet Halley: PolyoxymethyleneThe RPA2-Positive Ion Cluster Composition Analyzer (PICCA) on the Giotto spacecraft detected 5 mass peaks with regular spacing of 15 amu up to approximately 120 amu. Starting at 45 amu, the peaks decrease in intensity with increasing mass. Within their half-width they are in good agreement with dissociation products of formaldehyde polymer (POM). A production sequence in which cosmic radiation formed POM from water and carbon monoxide on grains that were aggregated into cometesimals is suggested. Other polymers, possibly containing CN, may also exist. Observations suggest that at least some of the H-, C-, and O-containing dust particles detected by the Particle Impact Analyzer (PIA) on board the Giotto spacecraft and its equivalent on the VEGA-1 and -2 spacecraft contain POM. The properties of POM are consistent with many of the unexpected observations in the coma.
Document ID
19880012522
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Huebner, W. F.
(Southwest Research Inst. San Antonio, TX., United States)
Boice, D. C.
(Southwest Research Inst. San Antonio, TX., United States)
Sharp, C. M.
(Los Alamos National Lab. NM., United States)
Korth, A.
(Max-Planck-Inst. fuer Aeronomie Katlenburg-Lindau (Germany, F.R.), United States)
Lin, R. P.
(California Univ. Berkeley., United States)
Mitchell, D. L.
(California Univ. Berkeley., United States)
Reme, H.
(Centre d'Etude Spatiale des Rayonnements Toulouse, France)
Date Acquired
September 5, 2013
Publication Date
September 1, 1987
Publication Information
Publication: ESA, Proceedings of the International Symposium on the Diversity and Similarity of Comets
Subject Category
Lunar And Planetary Exploration
Accession Number
88N21906
Funding Number(s)
CONTRACT_GRANT: CNES-1212
CONTRACT_GRANT: NASW-3375
CONTRACT_GRANT: BMFT-01-OF-85057
Distribution Limits
Public
Copyright
Other

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