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31.
F. Wehland A. Stancu P. Rochette M.J. Dekkers E. Appel 《Physics of the Earth and Planetary Interiors》2005,153(4):181-190
Pyrrhotite bearing metamorphic limestones have recently experienced an increasing relevance in paleomagnetic research. Simple univectorial remanences document the metamorphic uplift, whereas more complex multicomponent pTRMs may constrain its age. For a successful application of the latter, it is important to estimate the degree of magnetic interactions to ensure the additivity of individual pTRM segments. We therefore have subjected the sized dispersed suite (<5-250 μm) of TTE pyrrhotite to FORC analysis and compared the result with remanence-based parameters like the ΔM or the irreversible susceptibility. This is used as a basis to evaluate the response of marly limestone samples from regionally metamorphic areas (Bourg d’Oisans, France) and contact-metamorphic aureoles (Elba, Italy; Skye, Scottland; Manaslu area, Nepal) to these techniques. The results show that the techniques are able to estimate the nature and - to a certain degree - the intensity of the magnetic interaction. The different dominant magnetic states of the assemblage can also be unravelled as well. Based on the remanence measurements of the TTE samples, a relationship between grain-size and the irreversible susceptibility is established in order to estimate the mean grain-size fraction in natural particle distribution. 相似文献
32.
Clment Suavet Pierre Rochette Myriam Kars Jrme Gattacceca Luigi Folco Ralph P. Harvey 《Polar Science》2009,3(2):100-109
Micrometeorites have been recovered from traps located at the summit of nunataks in the Transantarctic Mountains (TAM), Antarctica. They constitute the TAM micrometeorite collection. Micrometeorites accumulated by direct infall for hundreds of thousands of years. This long collection duration is confirmed by the wide range of weathering by dissolution of olivine in the stony micrometeorites from the TAM collection. A statistical study of the size distribution and frequency by type of this collection, and comparison with other Antarctic micrometeorite collections (the South Pole Water Well collection and the Walcott Névé collection), suggest that the TAM collection is essentially unbiased. Thanks to the very long exposure of the traps, large diameter (>1000 μm) micrometeorites are present in sufficiently large numbers to allow a statistically meaningful estimate of their size distribution in this size range for the first time. We found that the slope of the size distribution remains constant in the 100–1600 μm size range. Therefore, the size distribution of micrometeorites in this size range is controlled by a single process. 相似文献
33.
Hamed Pourkhorsandi Jrme Gattacceca Pierre Rochette Massimo D'Orazio Hojat Kamali Roberto de Avillez Sonia Letichevsky Morteza Djamali Hassan Mirnejad Vinciane Debaille A. J. Timothy Jull 《Meteoritics & planetary science》2019,54(8):1737-1763
We present for the first time a detailed report on the discovery of a new meteorite collection region in the Lut Desert, eastern–southeastern Iran, describing its geological, morphological, and climatic setting. Our search campaigns, alongside with the activity of meteorite hunters, yielded >200 meteorite finds. Here, we report on their classification, spatial distribution, and terrestrial weathering. All the collected meteorites are ordinary chondrites (OCs). The most abundant by far are the highly weathered paired H5 distributed in the northwest of Kalut area (central Lut, Kerman dense collection area). The second are well‐preserved paired L5 also found in Kalut region. A detailed study of the geochemistry and mineralogy of selected meteorites reveals significant effects of terrestrial weathering. Fe,Ni metal (hereafter simply metal) and troilite are transformed into Fe oxyhydroxides. A rather unusual type of troilite weathering to pyrite/marcasite is observed in most of the Lut Desert meteorites. Magnetic measurements and X‐ray diffractometry confirm the occurrence of terrestrial weathering products, with the dominance of maghemite, goethite, and hematite. Mobile elements, such as Li, Sr, Mo, Ba, Tl, Th, and U, are enriched with respect to fresh falls. Meanwhile, a decrease in the V, Cr, Co, Rb (and possibly Fe) due to terrestrial weathering is detectable. The total carbon and CaCO3 is higher than in samples from other hot deserts. The weathering effects observed in the Lut Desert OCs can be used as distinctive indicators to distinguish them from meteorites from other regions of the Earth. Measurements of terrestrial age (14C) show a range of 10–30 ka, which is in the range of ages reported for meteorites from other hot deserts except the Atacama Desert (Chile). Considering the high potential of the Lut Desert in meteorite preservation, systematic works should lead to the discovery of more samples giving access to interesting material for future studies. 相似文献
34.
P. Rochette R. Ala P. Beck G. Brocard A. J. Cavosie V. Debaille B. Devouard F. Jourdan B. Mougel F. Moustard F. Moynier S. Nomade G. R. Osinski B. Reynard J. Cornec 《Meteoritics & planetary science》2019,54(4):880-901
The circa 14 km diameter Pantasma circular structure in Oligocene volcanic rocks in Nicaragua is here studied for the first time to understand its origin. Geomorphology, field mapping, and petrographic and geochemical investigations all are consistent with an impact origin for the Pantasma structure. Observations supporting an impact origin include outward‐dipping volcanic flows, the presence of former melt‐bearing polymict breccia, impact glass (with lechatelierite and low H2O, <300 ppm), and also a possible ejecta layer containing Paleozoic rocks which originated from hundreds of meters below the surface. Diagnostic evidence for impact is provided by detection in impact glass of the former presence of reidite in granular zircon as well as coesite, and extraterrestrial ε54Cr value in polymict breccia. Two 40Ar/39Ar plateau ages with a combined weighted mean age of 815 ± 11 ka (2 σ; P = 0.17) were obtained on impact glass. This age is consistent with geomorphological data and erosion modeling, which all suggest a rather young crater. Pantasma is only the fourth exposed crater >10 km found in the Americas south of N30 latitude, and provides further evidence that a significant number of impact craters may remain to be discovered in Central and South America. 相似文献
35.
W. Zylberman Y. Quesnel P. Rochette G. R. Osinski C. Marion J. Gattacceca 《Meteoritics & planetary science》2017,52(10):2147-2165
Haughton is a ~24 Myr old midsize (apparent diameter 23 km) complex impact structure located on Devon Island in Nunavut, Canada. The center of the structure shows a negative gravity anomaly of ?12 mGal coupled to a localized positive magnetic field anomaly of ~900 nT. A field expedition in 2013 led to the acquisition of new ground magnetic field mapping and electrical resistivity data sets, as well as the first subsurface drill cores down to 13 m depth at the top of the magnetic field anomaly. Petrography, rock magnetic, and petrophysical measurements were performed on the cores and revealed two different types of clast‐rich polymict impactites: (1) a white hydrothermally altered impact melt rock, not previously observed at Haughton, and (2) a gray impact melt rock with no macroscopic sign of alteration. In the altered core, gypsum is present in macroscopic veins and in the form of intergranular selenite associated with colored and zoned carbonate clasts. This altered core has a natural remanent magnetization (NRM) four to five times higher than materials from the other core but the same magnetic susceptibility. Their magnetization is still higher than the surrounding crater‐fill impact melt rocks. X‐ray fluorescence data indicate a similar proportion of iron‐rich phases in both cores and an enrichment in silicates within the altered core. In addition, alternating‐field demagnetization results show that one main process remagnetized the rocks. These results support the hypothesis that intense and possibly localized post‐impact hydrothermal alteration enhanced the magnetization of the clast‐rich impact melt rocks by crystallization of magnetite within the center of the Haughton impact structure. Subsequent erosion was followed by in situ concentration in the subsurface leading to large magnetic gradient on surface. 相似文献
36.
Modification of REE distribution of ordinary chondrites from Atacama (Chile) and Lut (Iran) hot deserts: Insights into the chemical weathering of meteorites 
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下载免费PDF全文 Hamed Pourkhorsandi Massimo D'Orazio Pierre Rochette Millarca Valenzuela Jérôme Gattacceca Hassan Mirnejad Brad Sutter Aurore Hutzler Maria Aboulahris 《Meteoritics & planetary science》2017,52(9):1843-1858
The behavior of rare earth elements (REEs) during hot desert weathering of meteorites is investigated. Ordinary chondrites (OCs) from Atacama (Chile) and Lut (Iran) deserts show different variations in REE composition during this process. Inductively coupled plasma–mass spectrometry (ICP‐MS) data reveal that hot desert OCs tend to show elevated light REE concentrations, relative to OC falls. Chondrites from Atacama are by far the most enriched in REEs and this enrichment is not necessarily related to their degree of weathering. Positive Ce anomaly of fresh chondrites from Atacama and the successive formation of a negative Ce anomaly with the addition of trivalent REEs are similar to the process reported from Antarctic eucrites. In addition to REEs, Sr and Ba also show different concentrations when comparing OCs from different hot deserts. The stability of Atacama surfaces and the associated old terrestrial ages of meteorites from this region give the samples the necessary time to interact with the terrestrial environment and to be chemically modified. Higher REE contents and LREE‐enriched composition are evidence of contamination by terrestrial soil. Despite their low degrees of weathering, special care must be taken into account while working on the REE composition of Atacama meteorites for cosmochemistry applications. In contrast, chondrites from the Lut desert show lower degrees of REE modification, despite significant weathering signed by Sr content. This is explained by the relatively rapid weathering rate of the meteorites occurring in the Lut desert, which hampers the penetration of terrestrial material by forming voluminous Fe oxide/oxyhydroxides shortly after the meteorite fall. 相似文献
37.
The geochemistry and the injection mechanism of hypovolcanic ring dykes have been extensively studied, but such is not the
case for their internal fabric. The Tertiary Western Red Hills epigranites of the Isle of Skye are a classic example of such
intrusions. Using anisotropy of magnetic susceptibility measurements, we present the first structural data of their internal
magmatic fabric. The magnetic foliations, equated with the magmatic flow planes, have strikes which roughly follow the walls
of the different intrusions. They dip steeply toward the convex wall of each intrusion. The lineations, or maximal magnetic
susceptibility axes, generally have shallow plunges, except in the latest granite intrusion. These structures appear to be
related to the compressional deformation of each intrusion toward the end of its crystallization. This shortening would be
a consequence of a radial and compressive stress field acting after each injection of magma. This radial stress field is interpreted
as the effect of high magma pressures originating from the acid magma chamber underlying the ring-dyke complex at a shallow
depth.
Received: 10 October 1995 / Accepted: 4 June 1997 相似文献
38.
N. S. Bezaeva D. D. Badyukov M. A. Nazarov P. Rochette J. Feinberg 《Geochemistry International》2013,51(7):568-574
This paper presents the distribution of magnetic susceptibility, χ0, in fragments of the Chelyabinsk ordinary chondrite (LL5, S4, W0, fall of February 15, 2013) from the collection of the Vernadsky Institute of Geochemistry and Analytical Chemistry, Russian Academy of Sciences, and results obtained by standard magnetic techniques for the meteorite material, including thermomagnetic analysis, measurements of natural remanent magnetization (NRM) and saturation isothermal remanent magnetization (SIRM), as well as the spectra of their alternating field demagnetization at amplitudes up to 170 mT, measurements of hysteresis loops and back-field remanence demagnetization curves at temperatures from 10 K to 700°C etc. The mean logχ0 values for the light-colored (main) lithology of the meteorite material and impact-melt breccia from our collection are 4.54 ± 0.10 (n = 66) and 4.65 ± 0.09 (n = 38) (×10?9 m3/kg), respectively. According to international magnetic classification of meteorites, Chelyabinsk falls within the range of LL5 chondrites. The mean metal content was estimated from the saturation magnetization, M s, of the light- and dark-colored lithologies as 3.7 and 4.1 wt %, respectively. Hence, the dark lithology is richer in metal. The metal grains are multidomain at room temperature and show low coercive force, B c (<2 mT) and remanent coercive force, B cr (15–23 mT). The thermomagnetic analyses of the samples showed that the magnetic properties of the Chelyabinsk meteorite are controlled mainly by taenite and kamacite at temperatures >75 K. In the temperature range below 75 K, magnetic properties are controlled by chromite; the magnetic hardness of the samples is maximal at 10 K and equals to 606 and 157 mT for the light- and dark-colored lithologies, respectively. 相似文献
39.
La fabrique magnétique du flysch dauphinois (Alpes francaises) : origine et application quantitative
RésuméLes propriétés magnétiques des schistes, grès et calcaires du flysch eocène de la zone dauphinoise ont été étudiées en relation avec la minéralogie et la structure de ces roches. La susceptibilité magnétique en champ faible est principalement due au paramagnétisme des phyllosilicates (illite et chlorite).L’anisotropie de susceptibilité correspond à un ellipsoïde aplati qui présente les caractéristiques suivantes : un axe minimal perpendiculaire à la schistosité et un axe maximal parallèle soit à une linéation d’intersection soit à la direction d’étirement maximal.On présente un modèle mathématique simple permettant d’utiliser le taux d’anisotropie magnétique pour quantifier l’orientation préférentielle des phyllosilicates. Ce modèle testé sur les niveaux les plus phylliteux du flysch donne des résultats en bon accord avec ceux de la goniometrie de texture. Les possibilités et les avantages de cette méthode structure-logique quantitative sont discutés. 相似文献
40.