Abstract:Multidimensional solid-state NMR spectroscopy is used to refine the identification and abundance determination of functional groups in insoluble organic matter (IOM) isolated from a carbonaceous chondrite (Murchison, CM2). It is shown that IOM is composed primarily of highly substituted single ring aromatics, substituted furan/pyran moieties, highly branched oxygenated aliphatics, and carbonyl groups. A pathway for producing an IOM-like molecular structure through formaldehyde polymerization is proposed and te… Show more
“…Relatively simple aldehydes such as formaldehyde and acetaldehyde can be found in molecular clouds, and may have been present in protoplanetary disks and primordial solar nebulae (e.g., Charnley, 2004;Tielens, 2005;Snyder, 2006;Dutrey et al, 1997). Formation of a formaldehyde polymer by aldol condensation has been emphasized for a possible origin of insoluble organic matter (IOM) in meteorites (Cody et al, 2011;Kebukawa et al, 2013). This study further indicates a contribution of aldol condensation products to soluble organic matter (SOM).…”
Section: Implications Of Alkylpyridine Occurrence To Chemical Evolutimentioning
“…Relatively simple aldehydes such as formaldehyde and acetaldehyde can be found in molecular clouds, and may have been present in protoplanetary disks and primordial solar nebulae (e.g., Charnley, 2004;Tielens, 2005;Snyder, 2006;Dutrey et al, 1997). Formation of a formaldehyde polymer by aldol condensation has been emphasized for a possible origin of insoluble organic matter (IOM) in meteorites (Cody et al, 2011;Kebukawa et al, 2013). This study further indicates a contribution of aldol condensation products to soluble organic matter (SOM).…”
Section: Implications Of Alkylpyridine Occurrence To Chemical Evolutimentioning
“…Their spectral patterns of aromatic/ olefinic carbon, aromatic ketone, and carboxyl carbon are typical of those observed from terrestrial coal (Cody et al 1998;Bassim et al 2012) and kerogen (Bernard et al 2012) and even extraterrestrial organic solids from chondritic meteorites and IDPs (e.g., Flynn et al 2003;Cody et al 2011). This does not necessarily imply that our category 3 particles are coal or chondritic organics, but the findings do suggest the presence of some form of heterogeneous macromolecule formed through chemical processing in a natural environment.…”
Section: Approach To Identify Category 3 Carbonaceous Particlesmentioning
confidence: 80%
“…; Ade et al 1992;Urquhart et al 1999), but it has been applied to a broad range of research areas. In cosmochemistry, STXM has been applied for organic chemical analyses of interplanetary dust particles (IDPs) (Flynn et al 2003(Flynn et al , 2013Busemann et al 2009), particles from Comet Wild 2 (Sanford et al 2006;Cody et al 2008a;De Gregorio et al 2010), acid-insoluble organic solids from chondritic meteorites (Cody et al 2008b, Cody et al 2011, and an Antarctic ultracarbonaceous micrometeorite (Yabuta et al 2013). Thus, an abundant database of XANES spectra for both terrestrial and extraterrestrial organic compounds is available for the chemical characterization of unknown carbonaceous samples.…”
Analyses with a scanning transmission x-ray microscope (STXM) using x-ray absorption near edge structure (XANES) spectroscopy were applied for the molecular characterization of two kinds of carbonaceous particles of unknown origin, termed category 3, which were collected from the Hayabusa spacecraft sample catcher. Carbon-XANES spectra of the category 3 particles displayed typical spectral patterns of heterogeneous organic macromolecules; peaks corresponding to aromatic/olefinic carbon, heterocyclic nitrogen and/or nitrile, and carboxyl carbon were all detected. Nitrogen-XANES spectra of the particles showed the presence of N-functional groups such as imine, nitrile, aromatic nitrogen, amide, pyrrole, and amine. An oxygen-XANES spectrum of one of the particles showed a ketone group. Differences in carbon-and nitrogen-XANES spectra of the category 3 particles before and after transmission electron microscopic (TEM) observations were observed, which demonstrates that the carbonaceous materials are electron beam sensitive. Calcium-XANES spectroscopy and elemental contrast mapping identified a calcium carbonate grain from one of the category 3 particles. No fluorine-containing molecular species were detected in fluorine-XANES spectra of the particles. The organic macromolecular features of the category 3 particles were distinct from commercial and/or biological 'fresh (non-degraded)' polymers, but the category 3 molecular features could possibly reflect degradation of contaminant polymer materials or polymer materials used on the Hayabusa spacecraft. However, an extraterrestrial origin for these materials cannot currently be ruled out.
“…Some meteorites and comets contain abundant organic matter of nonbiologic origin. How that matter forms and evolves is complex, and the work by Cody et al (30) reviews what we know about the processes that occur on small bodies that produce complex organic molecules. Finally, in acknowledgment of the fact that advances in cosmochemistry are highly technology-dependent, two papers are dedicated to the analytical methods themselves.…”
Cosmochemistry is the chemical analysis of extraterrestrial materials. This term generally is taken to mean laboratory analysis, which is the cosmochemistry gold standard because of the ability for repeated analysis under highly controlled conditions using the most advanced instrumentation unhindered by limitations in power, space, or environment. Over the past 40 y, advances in technology have enabled telescopic and spacecraft instruments to provide important data that significantly complement the laboratory data. In this special edition, recent advances in the state of the art of cosmochemistry are presented, which range from instrumental analysis of meteorites to theoretical-computational and astronomical observations.
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