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  • Journal article
    Emmerton S, Muxworthy AR, Sephton MA, Aldana M, Costanzo-Alvarez V, Bayona G, Williams Wet al., 2013,

    Correlating biodegradation to magnetization in oil bearing sedimentary rocks

    , GEOCHIMICA ET COSMOCHIMICA ACTA, Vol: 112, Pages: 146-165, ISSN: 0016-7037
  • Journal article
    Carter JN, Sephton MA, 2013,

    A Bayesian statistical assessment of representative samples for asteroidal or meteoritical material

    , Meteoritics & Planetary Science, Vol: 48, Pages: 976-996, ISSN: 1086-9379
  • Journal article
    Gilmour I, Gilmour M, Jolley D, Kelley S, Kemp D, Daly R, Watson Jet al., 2013,

    A high-resolution nonmarine record of an early Danian hyperthermal event, Boltysh crater, Ukraine

    , Geology
  • Journal article
    Sephton MA, 2013,

    Aromatic units from the macromolecular material in meteorites: Molecular probes of cosmic environments

    , Geochimica et Cosmochimica Acta, Vol: 107, Pages: 231-241, ISSN: 0016-7037
  • Journal article
    Wainipee W, Cuadros J, Sephton MA, Unsworth C, Gill MG, Strekopytov S, Weiss DJet al., 2013,

    The effects of oil on As(V) adsorption on illite, kaolinite, montmorillonite and chlorite

    , Geochimica et Cosmochimica Acta, Vol: 121, Pages: 487-502, ISSN: 0016-7037

    The effect of oil on As(V) adsorption on clay minerals has been investigated using batch experiments at low and high pH, NaCl concentration and oil contents. Four clay minerals were chosen because of their abundance in sediments and their different crystal chemistry: illite, kaolinite, montmorillonite, and chlorite. The values for pH were 4 and 8 and salt concentrations were 0.001 and 0.7 M NaCl to appreciate the effects of changing salinity, e.g from fresh water to seawater conditions. For the coating experiments, a well-characterised oil was used to survey the main effects of complex organic mixtures on adsorption and oil to clay mineral (w/w) ratios were 0.0325 and 0.3250. As(V) adsorption increased with increasing NaCl concentration, suggesting that the mechanisms of As(V) adsorption are related to the formation of inner-sphere complexes in which Na+ ions act as bridges between the clay surface and the As(V) anions. Cation bridging is also indicated by zeta potential measurements which show that higher NaCl concentrations along with the presence of As(V) can cause the clay particles and adsorbed ions to have a more negative overall charge. Adsorption is lower at higher pH due to the reduced number of positively charged sites on the edge of clay mineral layers. Oil coating reduces As(V) adsorption by decreasing the available surface area of clay minerals, except in the case of oil-coated montmorillonite, where surface area following dispersion in water is increased. The main variables controlling As(V) adsorption are surface area and surface charge density, as confirmed by a simplified quantitative model. These findings advance our ability to predict the effects of complex pollution events in various freshwater and marine settings.

  • Journal article
    Howard KT, Bailey MJ, Berhanu D, Bland PA, Cressey G, Howard LE, Jeynes C, Mathewman R, Martins Z, Sephton MA, Stolojan V, Verchovsky Set al., 2013,

    Biomass preservation in impact melt ejecta

    , Nature Geoscience

    Meteorites can have played a role in the delivery of life to Earth only if organic compounds are able to survive the high pressures and temperatures of an impact event. Although experimental impact studies have reported the survival of organics there are uncertainties in scaling experimental conditions to those of a meteorite impact on Earth and organic matter has not been found in highly shocked impact materials in a natural setting. Impact glass linked to the 1.2-km-diameter Darwin crater in western Tasmania is strewn over an area exceeding 400 km2 and is thought to have been ejected by a meteorite impact about 800 kyr ago into terrain consisting of rainforest and swamp. Here we use pyrolysis–gas chromatography–mass spectrometry to show that biomarkers representative of plant species in the local ecosystem—including cellulose, lignin, aliphatic biopolymer and protein remnants—survived the Darwin impact. We find that inside the impact glass the organic components are trapped in porous carbon spheres.We propose that the organic material was captured within impact melt and preserved when the melt quenched to glass, preventing organic decomposition since the impact. We suggest that organic material can survive capture and transport in products of extreme impact processing, at least for a Darwin-sized impact event.

  • Report
    Mustard JF, Adler M, Allwood A, Bass DS, Beaty DW, Bell JF, Brinckerhoff WB, Carr M, Des Marais DJ, Drake B, Edgett KS, Eigenbrode J, Elkins-Tanton LT, Grant JA, Milkovich SM, Ming D, Moore C, Murchie S, Onstott TC, Ruff SW, Sephton MA, Steele A, Treiman Aet al., 2013,

    Report of the Mars 2020 Science Definition Team

    , Report of the Mars 2020 Science Definition Team, Publisher: Mars Exploration Analysis Group (MEPAG)
  • Journal article
    Montgomery W, Court RW, Rees AC, Sephton MAet al., 2013,

    High temperature reactions of water with heavy oil and bitumen: insights into aquathermolysis chemistry during steam-assisted recovery

    , Fuel, Vol: 113, Pages: 426-426, ISSN: 0016-2361

    To better understand the hot water-mediated organic transformation process (aquathermolysis) that occurs during the steam-assisted recovery of heavy oils and bitumen we have performed a series of experiments that subject a heavy oil to progressively higher temperatures and pressures in the presence of liquid water. As temperature and pressure increases, from ambient conditions to 300 °C and 1250 psig (8.6 MPa), a floating oil (flotate) is generated and is composed of mostly aliphatic hydrocarbons that appear to be generated at the expense of polars and asphaltenes. Analyses of hopane maturity parameters for the flotate indicate lower temperatures than the starting material suggesting the liberation of hopanes and, therefore, other hydrocarbons, from asphaltenes. Infrared spectra confirm changes in overall organic constitution as the relative abundance of hydrocarbons to oxygen-containing functional groups increases in the flotate. At the highest temperatures and pressures (325 °C, 1750 psig (13.8 MPa)) the flotate is at a maximum relative amount, the untransformed heavy oil is at a minimum and significant amounts of methane are generated indicating the onset of cracking. Steam-assisted recovery of heavy oil, therefore, leads to changes in the chemical constitution of a number of chemical fractions generating a lighter oil and gases that must be taken into account when planning field operations for production.

  • Conference paper
    Montgomery W, Sephton MA, Court RW, Watson JS, Zeng H, Rees Aet al., 2013,

    Quantitative Laboratory Assessment Of Aquathermolysis Chemistry During Steam-assisted Recovery Of Heavy Oils And Bitumen, With A Focus On Sulfur

    , SPE Heavy Oil Conference, Publisher: Society of Petroleum Engineers

    The production of gaseous sulfur-containing species during the steam-assisted recovery of heavy oil and bitumen presents problems owing to their toxicity, corrosion properties and odor. In order to quantitatively study aquathermolysis sulfur chemistry during the thermal (steam-assisted) recovery of heavy oils we have subjected a well-characterized and sulfur-rich bitumen core sample to 150 - 325°C and 70 - 1740 psia (0.48 - 12 MPa) conditions in the continued presence of liquid water for 24 hours. The reaction products include gases, oil flotate, oil sinkate, water-soluble products, and water- insoluble residues. All have been studied with a variety of analytical techniques, including FTIR spectroscopy, chromatographic fractionation (SARA analysis), GC-FPD and GC-MS. Moreover, these techniques have been extended to analysis of the asphaltene fractions. Results suggest that some in-situ upgrading of the oil occurs under these conditions; additionally, gaseous hydrogen sulfide is released at temperatures at and above 250 °C. Variations in the relative abundances of solubility classes and chemical fractions imply that the source of sulfur is via the thermal degradation of resins and/or asphaltenes. The experimental methods, results and quantification approach discussed herein will be useful to support the development of models for engineering design of facilities for the steam-assisted recovery of heavy oils and bitumen.

  • Journal article
    Matthewman R, Martins Z, Sephton MA, 2013,

    Type IV kerogens as analogues for organic macromolecular materials in aqueously altered carbonaceous chondrites

    , Astrobiology, Vol: 13, Pages: 324-333, ISSN: 1531-1074
  • Journal article
    Sephton MA, James RH, Fehr MA, Bland PA, Gounelle Met al., 2013,

    Lithium isotopes as indicators of meteorite parent body alteration

    , Meteoritics & Planetary Science, Vol: 48, Pages: 872-878, ISSN: 1086-9379

    Hydrothermal processing on planetesimals in the early solar system produced new mineral phases, including those generated by the transformation of anhydrous silicates into their hydrated counterparts. Carbonaceous chondrites represent tangible remnants of such alteration products. Lithium isotopes are known to be responsive to aqueous alteration, yet previously recognized variability within whole rock samples from the same meteorite appears to complicate the use of these isotopes as indicators of processing by water. We demonstrate a new way to use lithium isotopes that reflects aqueous alteration in carbonaceous chondrites. Temperature appears to exert a control on the production of acetic acid-soluble phases, such as carbonates and poorly crystalline Fe-oxyhydroxides. Temperature and degree of water-rock interaction determines the amount of lithium isotope fractionation expressed as the difference between whole rock and acetic acid-leachable fractions. Using these features, the type 1 chondrite Orgueil (d7Li(whole rock) = 4.3&; D7Li(acetic-whole) = 1.2&) can be distinguished from the type 2 chondrites Murchison (d7Li(whole rock) = 3.8; D7Li(acetic whole) = 8.8&) and carbonate-poor Tagish Lake (d7Li(whole rock) = 4.3; D7Li(acetic-whole) = 9.4&). This initial study suggests that lithium isotopes have the potential to reveal the role of liquid water in the early solar system.

  • Journal article
    Sephton MA, 2013,

    Pyrolysis, spectroscopy and extraterrestrial organic matter

    , SpectroscopyEurope, Vol: 25, Pages: 6-11, ISSN: 0966-0941
  • Journal article
    Sephton MA, Court RW, Lewis JM, Wright MC, Gordon PRet al., 2013,

    Selecting samples for Mars sample return: Triage by pyrolysis-FTIR

    , Planetary and Space Science, Vol: 78, Pages: 45-51, ISSN: 0032-0633

    A future Mars Sample Return mission will deliver samples of the red planet to Earth laboratories for detailed analysis. A successful mission will require selection of the best samples that can be used to address the highest priority science objectives including assessment of past habitability and evidence of life. Pyrolysis is a commonly used method for extracting organic information from rocks but is most often coupled with complex analytical steps such as gas chromatography and mass spectrometry. Pyrolysis-Fourier transform infrared spectroscopy is a less resource demanding method that still allows sample characterization. Here we demonstrate how pyrolysis-Fourier transform infrared spectroscopy could be used to triage samples destined to return to Earth, thereby maximising the scientific return from future sample return missions.

  • Journal article
    Sephton MA, Hazen RM, 2013,

    On the origins of deep hydrocarbons

    , Reviews in Mineralogy & Geochemistry, Vol: 75, Pages: 449-465, ISSN: 1529-6466

    Deep deposits of hydrocarbons, including varied reservoirs of petroleum and natural gas,represent the most economically important component of the deep carbon cycle. Yet despitetheir intensive study and exploitation for more than a century, details of the origins of somedeep hydrocarbons remain a matter of vocal debate in some scientific circles. This long andcontinuing history of controversy may surprise some readers, for the biogenic origins of “fossilfuels”—a principle buttressed by a vast primary scientific literature and established as textbookorthodoxy in North America and many other parts of the world—might appear to be settled fact.Nevertheless, conventional wisdom continues to be challenged by some scientists.The principal objectives of this chapter are: (1) to review the overwhelming evidence for thebiogenic origins of most known deep hydrocarbon reservoirs; (2) to present equally persuasiveexperimental, theoretical, and field evidence that components of some deep hydrocarbondeposits appear to have an abiotic origin; and (3) to suggest future studies that might help toachieve a more nuanced resolution of this sometimes polarized topic.

  • Journal article
    Sephton MA, Sims MR, Court RW, Luong D, Cullen DCet al., 2013,

    Searching for biomolecules on Mars: Considerations for Operation of a Life Marker Chip instrument

    , Planetary and Space Science, Vol: 86, Pages: 66-74, ISSN: 0032-0633

    The search for life on Mars requires instruments that detect organic matter and discriminate between potential sources. One such instrument is the Life Marker Chip that recognizes small molecules which are characteristic of particular organic provenances. The use of an antibody-based detection system requires the delivery of small organic compounds in a suitable solvent. Dedicated extraction protocols have been developed partly through the use of a Life Marker Chip breadboard system. Techniques which provide the strong diagnostic potential of the Life Marker Chip necessitate specific extraction protocols and appropriate sample types. Clay mineral-rich rocks are attractive targets owing to their i) association with liquid water, ii) propensity for organic matter and clay mineral co-deposition following transport from a wide hinterland, and iii) relatively large surface area and therefore potential for trapping/adsorption of organic materials. The most appropriate target organic compounds are the hydrocarbon-dominated lipids that can be highly diagnostic and have relatively high preservation potentials. The sample sites on Mars and sample preparation steps that are needed for successful detection require careful consideration. In this paper we explore the scientific results that may be obtained through the operation of a Life Marker Chip instrument on Mars.

  • Journal article
    Court RW, Sephton MA, 2012,

    Extrasolar planets and false atmospheric biosignatures: The role of micrometeoroids

    , PLANETARY AND SPACE SCIENCE, Vol: 73, Pages: 233-242, ISSN: 0032-0633
  • Journal article
    Lomax BH, Fraser WT, Harrington G, Blackmore S, Sephton MA, Harris NBWet al., 2012,

    295 A novel palaeoaltimetry proxy based on spore and pollen wall chemistry

    , 日本花粉学会会誌, Vol: 58, Pages: 133-134, ISSN: 0387-1851
  • Book chapter
    Emmerton S, Muxworthy AR, Sephton MA, 2012,

    Magnetic characterization of oil sands at Osmington Mills and Mupe Bay, Wessex Basin, UK

    , Remagnetization and Chemical Alteration of Sedimentary Rocks, Editors: Elmore, Muxworthy, Aldana, Mena, Elmore, Muxworthy, Aldana, Mena, London, Publisher: Geological Society, Pages: 189-198
  • Book chapter
    Watson JS, 2012,

    Application of GC × GC–TOFMS to the Characterization of Extraterrestrial Organic Matter

    , Mass Spectrometry Handbook, Editors: Lee, Publisher: Wiley, ISBN: 9780470536735
  • Journal article
    Court RW, Sephton MA, 2012,

    Insights into the nature of cometary organic matter from terrestrial analogues

    , International Journal of Astrobiology, Vol: 11, Pages: 83-92, ISSN: 1473-5504

    The nature of cometary organic matter is of great interest to investigations involving the formation and distribution of organic matter relevant to the origin of life. We have used pyrolysis–Fourier transform infrared (FTIR) spectroscopy to investigate the chemical effects of the irradiation of naturally occurring bitumens, and to relate their products of pyrolysis to their parent assemblages. The information acquired has then been applied to the complex organic matter present in cometary nuclei and comae. Amalgamating the FTIR data presented here with data from published studies enables the inference of other comprehensive trends within hydrocarbon mixtures as they are progressively irradiated in a cometary environment, namely the polymerization of lower molecular weight compounds; an increased abundance of polycyclic aromatic hydrocarbon structures; enrichment in 13C; reduction in atomic H/C ratio; elevation of atomic O/C ratio and increase in the temperature required for thermal degradation. The dark carbonaceous surface of a cometary nucleus will display extreme levels of these features, relative to the nucleus interior, while material in the coma will reflect the degree of irradiation experienced by its source location in the nucleus. Cometary comae with high methane/water ratios indicate a nucleus enriched in methane, favouring the formation of complex organic matter via radiation-induced polymerization of simple precursors. In contrast, production of complex organic matter is hindered in a nucleus possessing a low methane/water ration, with the complex organic matter that does form possessing more oxygen-containing species, such as alcohol, carbonyl and carboxylic acid functional groups, resulting from reactions with hydroxyl radicals formed by the radiolysis of the more abundant water. These insights into the properties of complex cometary organic matter should be of particular interest to both remote observation and space missions involving in situ an

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