Physics
Scientific paper
Dec 2004
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004agufmsa13a1127h&link_type=abstract
American Geophysical Union, Fall Meeting 2004, abstract #SA13A-1127
Physics
7831 Laboratory Studies, 6008 Composition, 6020 Ice, 6045 Physics And Chemistry Of Materials, 6060 Radiation And Spectra
Scientific paper
Radio and IR observations have revealed that a rich organic chemistry exists in comets and in a variety of interstellar regions. Among the organic molecules detected are acids, alcohols, aldehydes, ketones, and nitriles. The simplest sugar, glycolaldehyde, has been reported (Hollis et al., ApJ, 2000, 540, L107), as has an amino acid, glycine (Kuan et al., ApJ, 2003, 593, 848; but see Hollis et al., ApJ, 2003, 588, 353). Gas-phase reactions to produce many of these molecules are not well understood, and solid-phase chemistry is thought to make an important contribution. To better understand organic chemistry in cold cosmic environments, we have performed photo- and radiation chemical experiments on icy materials at 10 - 100 K. Gas-phase molecules are frozen in a vacuum chamber, and then exposed to either MeV protons or vacuum-UV photons to mimic cosmic-ray bombardment or cosmic-UV exposure, respectively. Changes in ice composition are followed in situ with IR spectroscopy. In this AGU presentation we will describe our latest results for glycolaldehyde, as well as a few prebiological organics. Solid-state IR spectra and reaction pathways will be presented, and predictions will be made for the chemical composition of selected Solar System objects. -- This research is funded through NASA's Planetary Atmospheres and SARA programs, and through the NASA Astrobiology Program under RTOP 344-53-51-01 to M. J. Mumma (NASA GSFC).
Gerakines Perry A.
Hudson Reggie L.
Moore Marla H.
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