Elemental, isotopic, and structural changes in Tagish Lake insoluble organic matter produced by parent body processes

Here, we present the results of a multitechnique study of the bulk properties of insoluble organic material (IOM) from the Tagish Lake meteorite, including four lithologies that have undergone different degrees of aqueous alteration. The IOM C contents of all four lithologies are very uniform and comprise about half the bulk C and N contents of the lithologies. However, the bulk IOM elemental and isotopic compositions vary significantly. In particular, there is a correlated decrease in bulk IOM H/C ratios and dD values with increasing degree of alteration—the IOM in the least altered lithology is intermediate between CM and CR IOM, while that in the more altered lithologies resembles the very aromatic IOM in mildly metamorphosed CV and CO chondrites, and heated CMs. Nuclear magnetic resonance (NMR) spectroscopy, C X-ray absorption near-edge (XANES), and Fourier transform infrared (FTIR) spectroscopy confirm and quantitate this transformation from CR-like, relatively aliphatic IOM functional group chemistry to a highly aromatic one. The transformation is almost certainly thermally driven, and probably occurred under hydrothermal conditions. The lack of a paramagnetic shift in 13 C NMR spectra and 1s-r* exciton in the C-XANES spectra, both typically seen in metamorphosed chondrites, shows that the temperatures were lower and/or the timescales were shorter than experienced by even the least metamorphosed type 3 chondrites. Two endmember models were considered to quantitatively account for the changes in IOM functional group chemistry, but the one in which the transformations involved quantitative conversion of aliphatic material to aromatic material was the more successful. It seems likely that similar processes were involved in producing the diversity of IOM compositions and functional group chemistries among CR, CM, and CI chondrites. If correct, CRs experienced the lowest temperatures, while CM and CI chondrites experienced similar more elevated temperatures. This ordering is inconsistent with alteration temperatures based on mineralogy and O isotopes.

[1]  George D. Cody,et al.  The origin and evolution of chondrites recorded in the elemental and isotopic compositions of their macromolecular organic matter , 2007 .

[2]  G. Cody,et al.  Establishing a molecular relationship between chondritic and cometary organic solids , 2011, Proceedings of the National Academy of Sciences.

[3]  Jacobsen,et al.  Soft X‐ray spectroscopy from image sequences with sub‐100 nm spatial resolution , 2000, Journal of microscopy.

[4]  George D. Cody,et al.  Solid-state ( 1 H and 13 C) nuclear magnetic resonance spectroscopy of insoluble organic residue in the Murchison meteorite: a self-consistent quantitative analysis , 2002 .

[5]  T. Tyliszczak,et al.  Quantitative organic and light‐element analysis of comet 81P/Wild 2 particles using C‐, N‐, and O‐μ‐XANES , 2008 .

[6]  M. Zolensky,et al.  Aqueous alteration on the hydrous asteroids - Results of EQ3/6 computer simulations , 1989 .

[7]  G. Socrates,et al.  Infrared and Raman characteristic group frequencies : tables and charts , 2001 .

[8]  H. Schobert,et al.  A New Method for Measuring the Graphite Content of Anthracite Coals and Soots , 2002 .

[9]  G. Cody,et al.  NMR studies of chemical structural variation of insoluble organic matter from different carbonaceous chondrite groups , 2005 .

[10]  L. Ley,et al.  A comparative analysis of a-C:H by infrared spectroscopy and mass selected thermal effusion , 1998 .

[11]  J. Rouzaud,et al.  High resolution TEM of chondritic carbonaceous matter: Metamorphic evolution and heterogeneity , 2012 .

[12]  E. Dartois,et al.  IRAS 08572+3915: constraining the aromatic versus aliphatic content of interstellar HACs , 2007 .

[13]  G. Huss,et al.  Presolar diamond, silicon carbide, and graphite in carbonaceous chondrites: implications for thermal processing in the solar nebula , 2003 .

[14]  Christopher D. K. Herd,et al.  Testing variations within the Tagish Lake meteorite—II: Whole‐rock geochemistry of pristine samples , 2014 .

[15]  S. Derenne,et al.  Extreme deuterium enrichment of organic radicals in the Orgueil meteorite: Revisiting the interstellar interpretation? , 2008 .

[16]  Larry R. Nittler,et al.  Characterization of insoluble organic matter in primitive meteorites by microRaman spectroscopy , 2007 .

[17]  F. Robert,et al.  The concentration and isotopic composition of hydrogen, carbon and nitrogen in carbonaceous meteorites☆ , 1982 .

[18]  D. Brownlee,et al.  Diverse forms of primordial organic matter identified in interplanetary dust particles , 2012 .

[19]  R. Stroud,et al.  Testing variations within the Tagish Lake meteorite—I: Mineralogy and petrology of pristine samples , 2014 .

[20]  G. Cody,et al.  Deuterium enrichments in chondritic macromolecular material—Implications for the origin and evolution of organics, water and asteroids , 2010 .

[21]  R. Redmayne Coal: , 1936, Nature.

[22]  Christopher D. K. Herd,et al.  Soluble organic compounds in the Tagish Lake meteorite , 2014 .

[23]  M. Sephton Aromatic units from the macromolecular material in meteorites: Molecular probes of cosmic environments , 2013 .

[24]  A. Brearley Aqueous alteration and brecciation in Bells, an unusual, saponite-bearing, CM chondrite , 1995 .

[25]  Adrian J. Brearley,et al.  The Action of Water , 2006 .

[26]  Ronald A. Nieman,et al.  The Organic Content of the Tagish Lake Meteorite , 2001, Science.

[27]  F. R. Krueger,et al.  The organic component in dust from comet Halley as measured by the PUMA mass spectrometer on board Vega 1 , 1987, Nature.

[28]  S. Epstein,et al.  Relic interstellar grains in Murchison meteorite , 1984, Nature.

[29]  A. Westphal,et al.  Carbon investigation of two Stardust particles: A TEM, NanoSIMS, and XANES study , 2008 .

[30]  M. Zolensky,et al.  Spatial distribution of organic matter in the Bells CM2 chondrite using near‐field infrared microspectroscopy , 2010 .

[31]  L. Nittler,et al.  Presolar SiC abundances in primitive meteorites by NanoSIMS raster ion imaging of insoluble organic matter , 2009 .

[32]  J. Rouzaud,et al.  Precursor and metamorphic condition effects on Raman spectra of poorly ordered carbonaceous matter in chondrites and coals , 2009 .

[33]  Michael E. Zolensky,et al.  Mineralogy of Tagish Lake: An ungrouped type 2 carbonaceous chondrite , 2002 .

[34]  George J. Flynn,et al.  FTIR and Raman analyses of the Tagish Lake meteorite: Relationship with the aliphatic hydrocarbons observed in the Diffuse Interstellar Medium , 2004 .

[35]  G. Flynn,et al.  The origin of organic matter in the solar system: Evidence from the interplanetary dust particles , 2003 .

[36]  C. Alexander Re‐examining the role of chondrules in producing the elemental fractionations in chondrites , 2005 .

[37]  R. Hoffman Structure Determination of Organic Compounds , 2005 .

[38]  J. Eiler,et al.  Temperatures of aqueous alteration and evidence for methane generation on the parent bodies of the CM chondrites , 2007 .

[39]  G. Cody,et al.  Ultra-primitive interplanetary dust particles from the comet 26P/Grigg–Skjellerup dust stream collection , 2009 .

[40]  N. Johnson,et al.  A Self-Perpetuating Catalyst for the Production of Complex Organic Molecules in Protostellar Nebulae , 2008, Proceedings of the International Astronomical Union.

[41]  G. Flynn,et al.  Fine‐grained dust rims in the Tagish Lake carbonaceous chondrite: Evidence for parent body alteration , 2002 .

[42]  Ian A. Franchi,et al.  Light dement geochemistry of the Tagish Lake CI2 chondrite: Comparison with CI1 and CM2 meteorites , 2002 .

[43]  S. Messenger Identification of molecular-cloud material in interplanetary dust particles , 2000, Nature.

[44]  R. Bowden,et al.  The classification of CM and CR chondrites using bulk H, C and N abundances and isotopic compositions , 2013 .

[45]  R. Bowden,et al.  The Classification of CM and CR Chondrites Using Bulk H Abundances and Isotopes , 2012 .

[46]  Christopher D. K. Herd,et al.  Unusual nonterrestrial l‐proteinogenic amino acid excesses in the Tagish Lake meteorite , 2012 .

[47]  L. Bonal,et al.  Determination of the petrologic type of CV3 chondrites by Raman spectroscopy of included organic matter , 2006 .

[48]  G. Cody,et al.  The insoluble carbonaceous material of CM chondrites: A possible source of discrete organic compounds under hydrothermal conditions , 2007 .

[49]  R. Schultz,et al.  Infrared absorption spectroscopy. , 1971, American Industrial Hygiene Association journal.

[50]  Rhonda M. Stroud,et al.  Origin and Evolution of Prebiotic Organic Matter As Inferred from the Tagish Lake Meteorite , 2011, Science.

[51]  R. Bowden,et al.  Carbonate abundances and isotopic compositions in chondrites , 2013 .

[52]  Koji Nakanishi,et al.  Infrared Absorption Spectroscopy , 1977 .

[53]  I. Franchi,et al.  Carbon and nitrogen in carbonaceous chondrites: Elemental abundances and stable isotopic compositions , 2006 .

[54]  H. Naraoka,et al.  Elemental and isotope behavior of macromolecular organic matter from CM chondrites during hydrous pyrolysis , 2009 .

[55]  S. Epstein,et al.  Interstellar organic matter in meteorites , 1983 .

[56]  J. Rouzaud,et al.  Structure, composition, and location of organic matter in the enstatite chondrite Sahara 97096 (EH3) , 2012, 1502.00216.

[57]  D. Mittlefehldt Geochemistry of the ungrouped carbonaceous chondrite Tagish Lake, the anomalous CM chondrite Bells, and comparison with CI and CM chondrites , 2002 .

[58]  L. Bonal,et al.  Organic matter and metamorphic history of CO chondrites , 2007 .

[59]  J. Kerridge Isotopic composition of carbonaceous-chondrite kerogen: evidence for an interstellar origin of organic matter in meteorites , 1983 .

[60]  M. Zolensky,et al.  CM chondrites exhibit the complete petrologic range from type 2 to 1. [Abstract only] , 1994 .

[61]  P. Hoppe,et al.  Interstellar Chemistry Recorded in Organic Matter from Primitive Meteorites , 2006, Science.

[62]  G. Cody,et al.  Correlated microanalysis of cometary organic grains returned by Stardust , 2011 .

[63]  E. Anderson,et al.  Interferometer-controlled scanning transmission X-ray microscopes at the Advanced Light Source. , 2003, Journal of synchrotron radiation.

[64]  François Robert,et al.  Enrichment of deuterium in insoluble organic matter from primitive meteorites: A solar system origin? , 2006 .

[65]  Andrew Steele,et al.  Organics Captured from Comet 81P/Wild 2 by the Stardust Spacecraft , 2006, Science.

[66]  R. Kagi,et al.  Clay catalysis of aromatic hydrogen-exchange reactions , 1982 .

[67]  C. T. Pillinger,et al.  Aromatic moieties in meteoritic macromolecular materials: analyses by hydrous pyrolysis and δ13C of individual compounds , 2000 .

[68]  P G Brown,et al.  The fall, recovery, orbit, and composition of the Tagish Lake meteorite: a new type of carbonaceous chondrite. , 2000, Science.

[69]  C. Pillinger,et al.  The origin of chondritic macromolecular organic matter: A carbon and nitrogen isotope study , 1998, Meteoritics & planetary science.

[70]  E. Quirico,et al.  Metamorphic grade of organic matter in six unequilibrated ordinary chondrites , 2003 .

[71]  R. Bowden,et al.  The Provenances of Asteroids, and Their Contributions to the Volatile Inventories of the Terrestrial Planets , 2012, Science.

[72]  Chris Jacobsen,et al.  The nature of molecular cloud material in interplanetary dust , 2004 .

[73]  G. Cody,et al.  Compositional diversity in insoluble organic matter in type 1, 2 and 3 chondrites as detected by infrared spectroscopy , 2011 .

[74]  Emmanuel Dartois,et al.  Mid-infrared study of the molecular structure variability of insoluble organic matter from primitive chondrites , 2013 .

[75]  H. Naraoka,et al.  A different behavior of hydrogen isotope exchange in aqueous solutions between two PAH isomers (fluoranthene and pyrene) , 2003 .

[76]  G. Cody,et al.  Organic thermometry for chondritic parent bodies , 2008 .

[77]  Weifu Guo Carbonate clumped isotope thermometry: Application to carbonaceous chondrites & effects of kinetic isotope fractionation , 2009 .

[78]  L. Nittler,et al.  Isotopic anomalies in organic nanoglobules from Comet 81P/Wild 2: Comparison to Murchison nanoglobules and isotopic anomalies induced in terrestrial organics by electron irradiation , 2010 .