TY - JOUR A1 - Quirico, E. A1 - Moroz, Liubov V. A1 - Schmitt, B. A1 - Arnold, Gabriele A1 - Faure, M. A1 - Beck, P. A1 - Bonal, L. A1 - Ciarniello, M. A1 - Capaccioni, F. A1 - Filacchione, G. A1 - Erard, S. A1 - Leyrat, C. A1 - Bockelee-Morvan, D. A1 - Zinzi, A. A1 - Palomba, E. A1 - Drossart, P. A1 - Tosi, F. A1 - Capria, M. T. A1 - De Sanctis, M. C. A1 - Raponi, A. A1 - Fonti, S. A1 - Mancarella, F. A1 - Orofino, V. A1 - Barucci, A. A1 - Blecka, M. I. A1 - Carlson, R. A1 - Despan, D. A1 - Faure, A. A1 - Fornasier, S. A1 - Gudipati, M. S. A1 - Longobardo, A. A1 - Markus, K. A1 - Mennella, V. A1 - Merlin, F. A1 - Piccioni, G. A1 - Rousseau, B. A1 - Taylor, F. T1 - Refractory and semi-volatile organics at the surface of comet 67P/Churyumov-Gerasimenko: Insights from the VIRTIS/Rosetta imaging spectrometer JF - Icarus : international journal of solar system studies N2 - The VIRTIS (Visible, Infrared and Thermal Imaging Spectrometer) instrument aboard the Rosetta spacecraft has performed extensive spectral mapping of the surface of comet 67P/Churyumov-Gerasimenko in the range 0.3-5 mu m. The reflectance spectra collected across the surface display a low reflectance factor over the whole spectral range, two spectral slopes in the visible and near-infrared ranges and a broad absorption band centered at 3.2 mu m. The first two of these characteristics are typical of dark small bodies of the Solar System and are difficult to interpret in terms of composition. Moreover, solar wind irradiation may modify the structure and composition of surface materials and there is no unequivocal interpretation of these spectra devoid of vibrational bands. To circumvent these problems, we consider the composition of cometary grains analyzed in the laboratory to constrain the nature of the cometary materials and consider results on surface rejuvenation and solar wind processing provided by the OSIRIS and ROSINA instruments, respectively. Our results lead to five main conclusions: (i) The low albedo of comet 67P/CG is accounted for by a dark refractory polyaromatic carbonaceous component mixed with opaque minerals. VIRTIS data do not provide direct insights into the nature of these opaque minerals. However, according to the composition of cometary grains analyzed in the laboratory, we infer that they consist of Fe-Ni alloys and FeS sulfides. (ii) A semi-volatile component, consisting of a complex mix of low weight molecular species not volatilized at T similar to 220 K, is likely a major carrier of the 3.2 p.m band. Water ice contributes significantly to this feature in the neck region but not in other regions of the comet. COOH in carboxylic acids is the only chemical group that encompasses the broad width of this feature. It appears as a highly plausible candidate along with the NH4+ ion. (iii) Photolytic/thermal residues, produced in the laboratory from interstellar ice analogs, are potentially good spectral analogs. (iv) No hydrated minerals were identified and our data support the lack of genetic links with the CI, CR and CM primitive chondrites. This concerns in particular the Orgueil chondrite, previously suspected to have been of cometary origin. (v) The comparison between fresh and aged terrains revealed no effect of solar wind irradiation on the 3.2 mu m band. This is consistent with the presence of efficient resurfacing processes such as dust transport from the interior to the surface, as revealed by the OSIRIS camera. (C) 2016 Elsevier Inc. All rights reserved. KW - Comets KW - Organic chemistry KW - Infrared observations KW - Meteorites KW - Spectrophotometry Y1 - 2016 U6 - https://doi.org/10.1016/j.icarus.2016.02.028 SN - 0019-1035 SN - 1090-2643 VL - 272 SP - 32 EP - 47 PB - Elsevier CY - San Diego ER - TY - JOUR A1 - Uba, Cornelius Eji A1 - Hasler, Claude-Alain A1 - Buatois, Luis A. A1 - Schmitt, Axel K. A1 - Plessen, Birgit T1 - Isotopic, paleontologic, and ichnologic evidence for late Miocene pulses of marine incursions in the central Andes N2 - Recognition of an inferred Miocene marine incursion affecting areas from Colombia through Peru and Bolivia and into Argentina is essential to delineate the South American Seaway. In Bolivia, corresponding strata of inferred marine origin have been assigned to the late Miocene Yecua Formation. We carried out high-resolution delta C-13 and delta O-18 isotopic studies on 135 in situ carbonates from 3 outcrops, combined with detailed sedimentologic, paleontologic, and ichnologic analysis. Four less negative delta C-13 excursion levels were recorded that coincide well with beds containing marine body (barnacle) and trace (Ophiomorpha) fossils. These strata are interbedded with red-green beds containing mudcracks, plant roots, gypsum, and trace fossils of the continental Scoyenia ichnofacies. Our data are significant in that they show for the first time four possible short-lived marine incursions in the Bolivian central Andes during the late Miocene. The result is constrained by a new U-Pb date of 7.17 +/- 0.34 Ma at the top of Yecua strata. Y1 - 2009 UR - http://geology.gsapubs.org/ U6 - https://doi.org/10.1130/G30014a.1 SN - 0091-7613 ER - TY - JOUR A1 - Toy, Virginia Gail A1 - Sutherland, Rupert A1 - Townend, John A1 - Allen, Michael J. A1 - Becroft, Leeza A1 - Boles, Austin A1 - Boulton, Carolyn A1 - Carpenter, Brett A1 - Cooper, Alan A1 - Cox, Simon C. A1 - Daube, Christopher A1 - Faulkner, D. R. A1 - Halfpenny, Angela A1 - Kato, Naoki A1 - Keys, Stephen A1 - Kirilova, Martina A1 - Kometani, Yusuke A1 - Little, Timothy A1 - Mariani, Elisabetta A1 - Melosh, Benjamin A1 - Menzies, Catriona D. A1 - Morales, Luiz A1 - Morgan, Chance A1 - Mori, Hiroshi A1 - Niemeijer, Andre A1 - Norris, Richard A1 - Prior, David A1 - Sauer, Katrina A1 - Schleicher, Anja Maria A1 - Shigematsu, Norio A1 - Teagle, Damon A. H. A1 - Tobin, Harold A1 - Valdez, Robert A1 - Williams, Jack A1 - Yeo, Samantha A1 - Baratin, Laura-May A1 - Barth, Nicolas A1 - Benson, Adrian A1 - Boese, Carolin A1 - Célérier, Bernard A1 - Chamberlain, Calum J. A1 - Conze, Ronald A1 - Coussens, Jamie A1 - Craw, Lisa A1 - Doan, Mai-Linh A1 - Eccles, Jennifer A1 - Grieve, Jason A1 - Grochowski, Julia A1 - Gulley, Anton A1 - Howarth, Jamie A1 - Jacobs, Katrina A1 - Janku-Capova, Lucie A1 - Jeppson, Tamara A1 - Langridge, Robert A1 - Mallyon, Deirdre A1 - Marx, Ray A1 - Massiot, Cécile A1 - Mathewson, Loren A1 - Moore, Josephine A1 - Nishikawa, Osamu A1 - Pooley, Brent A1 - Pyne, Alex A1 - Savage, Martha K. A1 - Schmitt, Doug A1 - Taylor-Offord, Sam A1 - Upton, Phaedra A1 - Weaver, Konrad C. A1 - Wiersberg, Thomas A1 - Zimmer, Martin T1 - Bedrock geology of DFDP-2B, central Alpine Fault, New Zealand JF - New Zealand journal of geology and geophysics : an international journal of the geoscience of New Zealand, the Pacific Rim, and Antarctica ; NZJG N2 - During the second phase of the Alpine Fault, Deep Fault Drilling Project (DFDP) in the Whataroa River, South Westland, New Zealand, bedrock was encountered in the DFDP-2B borehole from 238.5–893.2 m Measured Depth (MD). Continuous sampling and meso- to microscale characterisation of whole rock cuttings established that, in sequence, the borehole sampled amphibolite facies, Torlesse Composite Terrane-derived schists, protomylonites and mylonites, terminating 200–400 m above an Alpine Fault Principal Slip Zone (PSZ) with a maximum dip of 62°. The most diagnostic structural features of increasing PSZ proximity were the occurrence of shear bands and reduction in mean quartz grain sizes. A change in composition to greater mica:quartz + feldspar, most markedly below c. 700 m MD, is inferred to result from either heterogeneous sampling or a change in lithology related to alteration. Major oxide variations suggest the fault-proximal Alpine Fault alteration zone, as previously defined in DFDP-1 core, was not sampled. KW - Alpine Fault KW - New Zealand KW - scientific drilling KW - mylonite KW - cataclasite Y1 - 2017 U6 - https://doi.org/10.1080/00288306.2017.1375533 SN - 0028-8306 SN - 1175-8791 VL - 60 IS - 4 SP - 497 EP - 518 PB - Taylor & Francis CY - Abingdon ER - TY - JOUR A1 - del Papa, C. A1 - Hongn, Fernando D. A1 - Powell, J. A1 - Payrola, P. A1 - Do Campo, M. A1 - Strecker, Manfred A1 - Petrinovic, I. A1 - Schmitt, A. K. A1 - Pereyra, R. T1 - Middle Eocene-Oligocene broken-foreland evolution in the Andean Calchaqui Valley, NW Argentina: insights from stratigraphic, structural and provenance studies JF - BASIN RESEARCH N2 - Two end-member models have been proposed for the Paleogene Andean foreland: a simple W-E migrating foreland model and a broken-foreland model. We present new stratigraphic, sedimentological and structural data from the Paleogene Quebrada de los Colorados (QLC) Formation, in the Eastern Cordillera, with which to test these two different models. Basin-wide unconformities, growthstrata and changes in provenance indicate deposition of the QLC Formation in a tectonically active basin. Both west- and east-vergent structures, rooted in the basement, controlled the deposition and distribution of the QLC Formation from the Middle Eocene to the Early Miocene. The provenance analysis indicates that the main source areas were basement blocks, like the Paleozoic Oire Eruptive Complex, uplifted during Paleogene shortening, and that delimits the eastern boundary of the present-day intraorogenic Puna plateau. A comparison of the QLC sedimentary basin-fill pattern with those of adjacent Paleogene basins in the Puna plateau and in the Santa Barbara System highlights the presence of discrete depozones. These reflect the early compartmentalization of the foreland, rather than a stepwise advance of the deformation front of a thrust belt. The early Tertiary foreland of the southern central Andes is represented by a ca. 250-km-wide area comprising several deformation zones (Arizaro, Macon, Copalayo and Calchaqui) in which doubly vergent or asymmetric structures, rooted in the basement, were generated. Hence, classical foreland model is difficult to apply in this Paleogene basin; and our data and interpretation agree with a broken-foreland model. Y1 - 2013 U6 - https://doi.org/10.1111/bre.12018 SN - 0950-091X SN - 1365-2117 VL - 25 IS - 5 SP - 574 EP - 593 PB - WILEY-BLACKWELL CY - HOBOKEN ER - TY - JOUR A1 - Pingel, Heiko A1 - Mulch, Andreas A1 - Alonso, Ricardo N. A1 - Cottle, John A1 - Hynek, Scott A. A1 - Poletti, Jacob A1 - Rohrmann, Alexander A1 - Schmitt, Axel K. A1 - Stockli, Daniel F. A1 - Strecker, Manfred T1 - Surface uplift and convective rainfall along the southern Central Andes (Angastaco Basin, NW Argentina) JF - Earth & planetary science letters N2 - Stable-isotopic and sedimentary records from the orogenic Puna Plateau of NW Argentina and adjacent intermontane basins to the east furnish a unique late Cenozoic record of range uplift and ensuing paleoenvironmental change in the south-central Andes. Today, focused precipitation in this region occurs along the eastern, windward flanks of the Eastern Cordillera and Sierras Pampeanas ranges, while the orogen interior constitutes high-elevation regions with increasingly arid conditions in a westward direction. As in many mountain belts, such hydrologic and topographic gradients are commonly mirrored by a systematic relationship between the oxygen and hydrogen stable isotope ratios of meteoric water and elevation. The glass fraction of isotopically datable volcanic ash intercalated in sedimentary sequences constitutes an environmental proxy that retains a signal of the hydrogen-isotopic composition of ancient precipitation. This isotopic composition thus helps to elucidate the combined climatic and tectonic processes associated with topographic growth, which ultimately controls the spatial patterns of precipitation in mountain belts. However, between 25.5 and 27 degrees S present-day river-based hydrogen isotope lapse rates are very low, possibly due to deep-convective seasonal storms that dominate runoff. If not accounted for, the effects of such conditions on moisture availability in the past may lead to misinterpretations of proxy-records of rainfall. Here, we present hydrogen-isotope data of volcanic glass (delta Dg), extracted from 34 volcanic ash layers in different sedimentary basins of the Eastern Cordillera and the Sierras Pampeanas. Combined with previously published delta Dg records and our refined U-Pb and (U-Th)/He zircon geochronology on 17 tuff samples, we demonstrate hydrogen-isotope variations associated with paleoenvironmental change in the Angastaco Basin, which evolved from a contiguous foreland to a fault-bounded intermontane basin during the late Mio-Pliocene. We unravel the environmental impact of Mio-Pliocene topographic growth and associated orographic effects on long-term hydrogen-isotope records of rainfall in the south-central Andes, and potentially identify temporal variations in regional isotopic lapse rates that may also apply to other regions with similar topographic boundary conditions. (C) 2016 Elsevier B.V. All rights reserved. KW - hydrogen stable isotopes KW - volcanic glass KW - paleoaltimetry KW - NW-Argentine Andes KW - orographic barrier uplift KW - convective rainfall Y1 - 2016 U6 - https://doi.org/10.1016/j.epsl.2016.02.009 SN - 0012-821X SN - 1385-013X VL - 440 SP - 33 EP - 42 PB - Elsevier CY - Amsterdam ER -