Museum dHistoire Naturelle de Geneva
Museum dHistoire Naturelle de Geneva
Meister C.,Museum DHistoire Naturelle de Geneva |
Schirolli P.,Museo di Science Naturali di Brescia |
Dommergues J.-L.,University of Burgundy
Rivista Italiana di Paleontologia e Stratigrafia | Year: 2017
This work provides a more precise up-to-date biostratigraphical framework of the Early Jurassic ammonite succession of the Brescian Prealps with more than seventy taxa for the Sinemurian, Pliensbachian and basal Toarcian corresponding to a about 30 horizons or faunal assemblages rather well correlable with the NW European standard zonation. These results are supported with already published data, new data from recent ield investigations, revised contributions of different authors and with the study of the historical collection of the Museum of Natural Sciences of Brescia (Northern Italy). The biohorizons are referred to the Lower Jurassic carbonate series of the Brescian Prealps, cropping out between the eastern surroundings of Brescia (Botticino-Serle), to the East, and the Lake Iseo, to the West. This area was located in the eastern border of the wide Lombardian Basin, a part of the southern continental passive margin subjected to the Jurassic rifting, preceding the Neo-Tethys opening.
Hollier J.,Museum dHistoire Naturelle de Geneva
Revue Suisse de Zoologie | Year: 2017
The Muséum d'histoire naturelle de Genève contains type specimens of nine species of parasitic marine isopods, all described in the 19th century. These are enumerated and the current nomenclatural combination is given.
Meister C.,Museum dHistoire naturelle de Geneva |
Dommergues J.-L.,University of Burgundy |
Rocha R.B.,New University of Lisbon
Bulletin of Geosciences | Year: 2012
The lowermost Portuguese Pliensbachian is characterized by the association of Apoderoceras dunrobinense Spath, Tragophylloceras numismale (Quenstedt) and Vicininodiceras aff. mouterdei Donovan. This ammonite fauna indicates the lower part of the Jamesoni Chronozone (lower to middle Taylori Subchronozone). Thanks to the numerous specimens collected, the ontogeny and variability of A. dunrobinense Spath, could also be investigated. The paleogeographical distribution of these ammonites underlines the close connections between the Lusitanian Basin and the Euroboreal seas during the Early Pliensbachian.
Popova O.,Russian Academy of Sciences |
Borovicka J.,Czech Republic Astronomical Institute |
Hartmann W.K.,Planetary Science Institute |
Spurny P.,Czech Republic Astronomical Institute |
And 3 more authors.
Meteoritics and Planetary Science | Year: 2011
We have assembled data on 13 cases of meteorite falls with accurate tracking data on atmospheric passage. In all cases, we estimate the bulk strength of the object corresponding to its earliest observed or inferred fragmentation in the high atmosphere, and can compare these values with measured strengths of meteorites in the taxonomic class for that fall. In all 13 cases, the strength corresponding to earliest observed or inferred fragmentation is much less than the compressive or tensile strength reported for that class of stony meteorites. Bulk strengths upon atmospheric entry of these bodies are shown to be very low, 0.1 to approximately 1MPa on first breakup, and maximal strength on breakup as 1-10MPa corresponding to weak and "crumbly" objects, whereas measured average tensile strength of the similar meteorite classes is about 30MPa. We find a more random relation between bulk sample strength and sample mass than is suggested by a commonly used empirical power law. We estimate bulk strengths on entry being characteristically of the order of 10-1-10-2 times the tensile strengths of recovered samples. We conclude that pre-entry, meter-scale interplanetary meteoroids are typically highly fractured or in some cases rubbly in texture, presumably as a result of their parent bodies' collisional history, and can break up under stresses of a few megapascals. The weakness of some carbonaceous objects may result from very porous primordial accretional structures, more than fractures. These conclusions have implications for future asteroid missions, sample extraction, and asteroid hazard mitigation. © The Meteoritical Society, 2011.
Hardy C.,CNRS Biogeosciences Laboratory |
Fara E.,CNRS Biogeosciences Laboratory |
Laffont R.,CNRS Biogeosciences Laboratory |
Dommergues J.-L.,CNRS Biogeosciences Laboratory |
And 2 more authors.
PLoS ONE | Year: 2012
Conservation biologists and palaeontologists are increasingly investigating the phylogenetic distribution of extinctions and its evolutionary consequences. However, the dearth of palaeontological studies on that subject and the lack of methodological consensus hamper our understanding of that major evolutionary phenomenon. Here we address this issue by (i) reviewing the approaches used to quantify the phylogenetic selectivity of extinctions and extinction risks; (ii) investigating with a high-resolution dataset whether extinctions and survivals were phylogenetically clustered among early Pliensbachian (Early Jurassic) ammonites; (iii) exploring the phylogenetic and temporal maintenance of this signal. We found that ammonite extinctions were significantly clumped phylogenetically, a pattern that prevailed throughout the 6.6 Myr-long early Pliensbachian interval. Such a phylogenetic conservatism did not alter - or may even have promoted - the evolutionary success of this major cephalopod clade. However, the comparison of phylogenetic autocorrelation among studies remains problematic because the notion of phylogenetic conservatism is scale-dependent and the intensity of the signal is sensitive to temporal resolution. We recommend a combined use of Moran's I, Pearson's φ and Fritz and Purvis' D statistics because they highlight different facets of the phylogenetic pattern of extinctions and/or survivals. © 2012 Hardy et al.
Bachmann O.,University of Washington |
Deering C.D.,University of Washington |
Deering C.D.,University of Wisconsin - Oshkosh |
Ruprecht J.S.,Lamont Doherty Earth Observatory |
And 3 more authors.
Contributions to Mineralogy and Petrology | Year: 2012
Multiple eruptions of silicic magma (dacite and rhyolites) occurred over the last ~3 My in the Kos-Nisyros volcanic center (eastern Aegean sea). During this period, magmas have changed from hornblende-biotite-rich units with low eruption temperatures (≤750-800°C; Kefalos and Kos dacites and rhyolites) to hotter, pyroxene-bearing units (>800-850°C; Nisyros rhyodacites) and are transitioning back to cooler magmas (Yali rhyolites). New whole-rock compositions, mineral chemistry, and zircon Hf isotopes show that these three types of silicic magmas followed the same differentiation trend: they all evolved by crystal fractionation and minor crustal assimilation (AFC) from parents with intermediate compositions characterized by high Sr/Y and low Nb content, following a wet, high oxygen fugacity liquid line of descent typical of subduction zones. As the transition between the Kos-Kefalos and Nisyros-type magmas occurred immediately and abruptly after the major caldera collapse in the area (the 161 ka Kos Plateau Tuff; KPT), we suggest that the efficient emptying of the magma chamber during the KPT drew out most of the eruptible, volatile-charged magma and partly solidified the unerupted mush zone in the upper crust due to rapid unloading, decompression, and coincident crystallization. Subsequently, the system reestablished a shallow silicic production zone from more mafic parents, recharged from the mid to lower crust. The first silicic eruptions evolving from these parents after the caldera collapse (Nisyros units) were hotter (up to >100°C) than the caldera-forming event and erupted from reservoirs characterized by different mineral proportions (more plagioclase and less amphibole). We interpret such a change as a reflection of slightly drier conditions in the magmatic column after the caldera collapse due to the decompression event. With time, the upper crustal intermediate mush progressively transitioned into the cold-wet state that prevailed during the Kefalos-Kos stage. The recent eruptions of the high-SiO 2 rhyolite on Yali Island, which are low temperature and hydrous phases (sanidine, quartz, biotite), suggest that another large, potentially explosive magma chamber is presently building under the Kos-Nisyros volcanic center. © 2011 Springer-Verlag.
Giese J.,University of Bern |
Berger A.,Copenhagen University |
Schreurs G.,University of Bern |
Gnos E.,Museum dhistoire naturelle de Geneva
Precambrian Research | Year: 2011
In central southern Madagascar the crystalline basement is composed of mid-crustal rocks which have experienced polycyclic deformation and metamorphism coupled with repeated granitoid magmatism at the Neoproterozoic-Phanerozoic boundary. Based on the integration of in situ U-Th-Pb dating of monazite and structural relationships, two distinct phases of major ductile deformation, the Andreaba and Ihosy phases can be distinguished in central southern Madagascar. Both these deformation phases occur between ~550 and 520. Ma. Coeval with, and outlasting deformation, granitic plutons and dykes were emplaced. HT/HP granulite facies metamorphism (M1), including migmatisation and anatexis of the crust started at ~585. Ma and lasted until at least ~500. Ma. Monazite growth between 480 and 450. Ma postdates major ductile deformation and might be related to a second, HT/MP metamorphism (M2), indicating that the whole crustal section remained in a mid-crustal position. Metamorphic overprinting related to M2 is spatially limited and is heterogeneously distributed in central southern Madagascar. Newly developed M2 mineral assemblages are preferentially found in areas featuring Ihosy phase vertical foliation planes. Very often these structures show brittle/ductile or brittle overprint and might be considered as preferred pathways for fluid flow, thus localising metamorphic overprint. © 2011 Elsevier B.V.
Hollier A.,Museum dHistoire Naturelle de Geneva |
Hollier J.,Museum dHistoire Naturelle de Geneva
Archives of Natural History | Year: 2013
The nineteenth-century Swiss entomologist Henri de Saussure is probably better known today as the father of linguist Ferdinand de Saussure than as a scientist in his own right. In this context, it is his personality rather than his work that has attracted attention, encouraged by the availability of letters and diaries in which he expresses himself openly on personal matters. This paper presents an overview of his life that includes analysis of his scientific contribution in order to give a more balanced assessment. Examination of his publications confirms his importance as a taxonomist, and shows interesting trends in his approach. He was also notable for his cultivation of a wide network of collaborators and for the way he used his status to enhance the collections of the Museum d'histoire naturelle de Geneve. © The Society for the History of Natural History.
Hollier J.,Museum dHistoire Naturelle de Geneva |
Hollier A.,Museum dHistoire Naturelle de Geneva
Bulletin of the British Ornithologists' Club | Year: 2016
The cousins Louis-Albert Necker and Henri de Saussure exemplify the contribution to the study of birds made by non-specialists in the first half of the 19th century, during the period when ornithology was just emerging as a scientific discipline. Necker undertook local field observations and published some of the earliest detailed information on the birds of Switzerland, especially the Geneva region, and both men were important contributors to the Museum d'histoire naturelle de Geneve in ways characteristic of their time: via the donation of private collections or the procurement of exotic specimens through scientific expeditions.
Dirickx H.G.,Museum dHistoire Naturelle de Geneva
Revue Suisse de Zoologie | Year: 2010
So far, three species of the tribe Bacchini have been recorded from Madagascar. A review of the known species is given, including a redescription of Ptileuria (pBaccha) nigroscutata Enderlein, 1938. Five new species are described from the island: A. similis sp. n., A.fumosa sp. n., A. madecassa sp. n., A. obscura sp. n. and A. subflava sp. n. A brief historical account of the taxonomy of the Bacchini, in particular with regard to the status of Allobaccha is presented.