• Medientyp: E-Artikel
  • Titel: Organic Syntheses During the Impact of a Comet with a Gaseous Planet
  • Beteiligte: Guaita, Cesare; Crippa, Roberto; Manzini, Federico
  • Erschienen: Cambridge University Press (CUP), 1997
  • Erschienen in: International Astronomical Union Colloquium, 161 (1997), Seite 189-195
  • Sprache: Englisch
  • DOI: 10.1017/s0252921100014706
  • ISSN: 0252-9211
  • Schlagwörter: General Engineering
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  • Beschreibung: <jats:title>Abstract</jats:title><jats:p>A large amount of CO has been detected above many SL9/Jupiter impacts. This gas was never detected before the collision. So, in our opinion, CO was released from a parent compound during the collision. We identify this compound as POM (polyoxymethylene), a formaldehyde (HCHO) polymer that, when suddenly heated, reformes monomeric HCHO. At temperatures higher than 1200°K HCHO cannot exist in molecular form and the most probable result of its decomposition is the formation of CO. At lower temperatures, HCHO can react with NH3 and/or HCN to form high UV-absorbing polymeric material. In our opinion, this kind of material has also to be taken in to account to explain the complex evolution of some SL9 impacts that we observed in CCD images taken with a blue filter.</jats:p>
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