Seconds after impact: Insights into the thermal history of impact ejecta from diffusion between lechatelierite and host glass in tektites and experiments

1Catherine A.Macris, 1Paul D.Asimow, 2James Badro, 1John M.Eiler, 3Youxue Zhang, 1Edward M.Stolper
Geochimica et Cosmochimica Acta (in Press) Link to Article [https://doi.org/10.1016/j.gca.2018.08.031]
1Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, 91125, USA
2Institut de Physique du Globe de Paris, Paris, France
3Earth and Environmental Sciences, University of Michigan, Ann Arbor, MI, 48109, USA
Copyright Elsevier

Tektites contain inclusions of lechatelierite, nearly pure SiO2 glass formed by quenching of quartz grains melted during hypervelocity impacts. We report the discovery in a tektite of chemically zoned boundary layers (ca 20 μm) between lechatelierite and host felsic glass. These boundary layers in tektites formed by chemical diffusion between molten silica inclusions (quenched to lechatelierite on cooling) and surrounding felsic melt. We reproduced the details of these boundary layers via experiments on mixtures of powdered natural tektite plus quartz grains heated to 1800-2400 ˚C for 1-120 s using an aerodynamic levitation laser heating furnace. The results of these experiments were used to provide quantitative constraints on possible thermal histories of the natural sample.

The experiments successfully reproduced all major aspects of the concentration profiles from the natural sample including diffusion length scale, strong asymmetry of the concentration profiles with respect to the Matano plane (due to the strong concentration dependence of the diffusivities of all oxides on SiO2 content), similarities in lengths of the diffusive profiles (due to control by the diffusion of SiO2 on the diffusivity of the other oxides), and differences in the shapes of the profiles among the oxides (including a maximum in the diffusion profile of K2O due to uphill diffusion). The characteristic lengths of all non-alkali oxide profiles are proportional to t from which diffusivities and activation energies can be derived; these results are consistent with measurements in melts with lower SiO2 contents and at lower temperatures reported in the literature. We also fit the experimental profiles of SiO2 and Al2O3 using simple formulations of the dependence of their diffusivities on SiO2 content and temperature, yielding results similar to those obtained from the t dependence of the characteristic profile lengths.

The quantitative characterization of diffusion in boundary layers based on our experiments allow us to set limits on the thermal history of the natural tektite in which the boundary layers were discovered. If the interdiffusion between the silica and felsic melts occurred at constant temperature, the duration of heating experienced by the natural tektite we studied depends on temperature; possible solutions include heating at ∼2000 °C for ∼70 s, -2400 °C for ∼3 seconds. We also explored non-isothermal, asymptotic cooling histories; for a maximum temperature of 2400 °C, a characteristic cooling time scale of ∼50 s is implied, whereas, for 2000 °C, the time scale is ∼1400 s. Further, a maximum temperature of ∼2360 °C yields an effective diffusive time scale of ∼5 s, a cooling time scale of ∼90 s, and a cooling rate at the glass transition temperature of ∼5 °C/s; results that are consistent with independent estimates of cooling time scales for ∼1 cm clasts (Xu and Zhang, 2002), as well as cooling rates at the glass transition temperature (Wilding et al., 1996) – thus satisfying all currently available relevant data. More complex T-t paths are possible and can also be modeled using our experimental results and compared with and used as tests of the accuracy of physical models of tektite-forming impact events.

Baddeleyite as a widespread and sensitive indicator of meteorite bombardment in planetary crusts

1,2,3White, L.F., 1Darling, J.R., 4Moser, D.E., 5Cayron, C., 4Barker, I., 1Dunlop, J., 2,3Tait, K.T.
Geology 46, 719-722 Link to Article [DOI: 10.1130/G45008.1]
1School of Earth and Environmental Sciences, University of Portsmouth, Portsmouth, United Kingdom
2Department of Natural History, Royal Ontario Museum, 100 Queens Park, Toronto, ON, Canada
3Deparment of Earth Sciences, University of Toronto, Toronto, ON, Canada
4Department of Earth Sciences, University of Western Ontario, London, Canada
5Laboratory of ThermoMechanical Metallurgy (LMTM), École Polytechnique Fédérale de Lausanne (EPFL), Rue de la Maladière, 71b, Neuchâtel, Switzerland

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Chondrules as direct thermochemical sensors of solar protoplanetary disk gas

1,2Libourel, G., 3Portail, M.
Science Advances 4, eaar3321 Link to Article [DOI: 10.1126/sciadv.aar3321]
1Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, UMR 7293 Lagrange, Boulevard de l’Observatoire, CS34229, Nice Cedex 4, France
2Hawai‘i Institute of Geophysics and Planetology, School of Ocean, Earth Science and Technology, University of Hawai‘i, Mānoa, Honolulu, HI, United States
3Université Côte d’Azur, CNRS–Centre de Recherches sur l’Hétéro-Epitaxie et ses Applications, Sophia Antipolis, Rue Bernard Grégory, Valbonne, France

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Results of mineralogical and petrological research of new samples on the Pułtusk meteorite at the 150th anniversary of the fall [Wyniki badań mineralogicznych i petrologicznych nowych okazów meteorytu Pułtusk w 150 rocznicȩ spadku]

1Przylibski, T.A.,1Łuszczek, K.
Przeglad Geologiczny 66, 368-378 Link to Article [DOI: 10.3390/min8060240]
1Wydział Geoinżynierii, Górnictwa i Geologii, Politechnika Wrocławska, Wybrzeże S. Wyspiańskiego 27, Wrocław, Poland

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Nitrogen abundance and isotope analysis of silicate glasses by secondary ionization mass spectrometry

1Füri, E.,1Deloule, E., 1,2Dalou, C.
Chemical Geology 493, 327-337 Link to Article [DOI: 10.1016/j.chemgeo.2018.06.008]
1Centre de Recherches Pétrographiques et Géochimiques, UMR 7358, CNRS-UL, 15 rue Notre Dame des Pauvres, BP20, Vandoeuvre-lès-Nancy Cedex, France
2University of Minnesota, Department of Earth Sciences, 108 Pillsbury Hall, Minneapolis, MN, United States

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Chemical-petrographic types and shock metamorphism of 184 Grove Mountains equilibrated ordinary chondrites

1Dai, D., 1,2Liu, S. 1,2Liu, X.
Minerals 8, 240 Link to Article [DOI: 10.3390/min8060240]
1Institute of Geology, Hunan University of Science and Technology, Xiangtan, China
2Hunan Provincial Key Laboratory of Shale Gas Resource Utilization, Xiangtan, China


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Shock heterogeneity and shock history of the recently found ordinary Csátalja chondrite in Hungary

1Kereszturi, A., 2Fintor, K.,3Gyollai, I., 4Kereszty, Z., 3Szabo, M., 5,6Szalai, Z., 2Walter, H.
Geological Quarterly 62, 433-446 Link to Article [doi: 10.7306/gq.1416]
1Research Centre for Astronomy and Earth Sciences, Konkoly Thege Miklos Astronomical Institute, Konkoly Thege Miklósút 15–17, Budapest, Hungary
2University of Szeged, Vulcano Petrology and Geochemistry Research Group, Department of Mineralogy, Geochemistry and Petrology, Hungary
3Research Centre for Astronomy and Earth Sciences, Institute for Geological and Geochemical Research, Hungary

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The vanadium isotopic composition of L ordinary chondrites

1,2Xue, Y., 3Li, C.-H., 3Qi, Y., 1,2Zhang, C., 1,2Miao, B., 3Huang, F.
Acta Geochimica 37, 501-508 Link to Article [DOI
https://doi.org/10.1007/s11631-018-0279-2]
1Institution of Meteorites and Planetary Materials Research, Guilin University of Technology, Guilin, China
2Key Laboratory of Planetary Geological Evolution at Universities of Guangxi Province, Guilin University of Technology, Guilin, China
3Key Laboratory of Crust-Mantle Materials and Environments, School of Earth and Space Sciences, University of Science and Technology of China, Hefei, China

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Shock-Induced Olivine-Ringwoodite Transformation in the Shock Vein of Chondrite GRV053584

1,2Feng Yin, 3,4Zhiwei Liao, 1,5Andrew Hursthouse, 2Deqiu Dai
Minerals 8, 139 Link to Article [https://doi.org/10.3390/min8040139]
1Hunan Provincial Key Laboratory of Shale Gas Resource Utilization, Hunan University of Science and Technology, Xiangtan 411201, China
2Department of Geology, Hunan University of Science and Technology, Xiangtan 411201, China
3College of Resources and Environmental Science, Chongqing University, Chongqing 400044, China
4State Key Laboratory of Coal Mine Disaster Dynamics and Control, Chongqing University, Chongqing 400044, China
5School of Science and Sport, University of the West of Scotland, Paisley PA1 2BE, UK

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