Argiles et zéolites dans l'altération d'un volcan bouclier en milieu tropical (Le Piton des Neiges,La Réunion)

The drilling of a gallery through the Roche-Écrite massif (Reunion Island) allowed to sample the old formations of the ‘Piton des Neiges’ volcano. The mineralogical study of the alteration products of the formations showed significant variations of the zeolites/clay minerals ratio depending on the location of the rocks in the volcano. The abundance of zeolites in the formation near the surface hydrographic network or the underground water drainage system seems to be due to the physicochemical processes favouring zeolites in more open systems in their competition with secondary clays. To cite this article: L. Bret et al., C. R. Geoscience 335 (2003).     

Identifying the origin of groundwater and flow processes in complex landslides affecting black marls: insights from a hydrochemical survey

The Super‐Sauze mudslide is a persistently active slow‐moving landslide occurring in the black marl outcrops of the French South Alps. It has been intensively studied since the early 1990s. Geotechnical, geomorphological, geophysical and hydrological investigations have led to a better understanding of the processes governing the landslide motion. Water ?ows inside the system have been proven to have a major impact. To look closer at the processes involved and especially to gain a better idea of the origin and pathways of the waters, a hydrochemical study was carried out from May 2003 to May 2004. The groundwater was sampled during ?ve ?eld campaigns spread uniformly over the year. Groundwater from a network of boreholes was collected as well as spring waters from the fractured bedrock (in situ black marl) and from the moraine aquifer above the landslide. Results showed that the groundwater chemistry could not be fully explained by rainfall recharge or simple water–matrix equilibrium. A contribution of saline waters coming from the bottom of a thrust sheet overhanging the landslide was required to get the observed high mineralization. On a ?ow line, the hydrochemical evolution was related to both soil–matrix equilibrium and deep water sources coming up to the surface by means of major faults, the bedding planes and the schistosity. Hydrochemical anomalies made it possible to point out such contributions locally. It was shown that water chemistry and landslide activity were closely related. This hydrochemical investigation also enabled us to better de?ne the hydrosystem limits.Copyright © 2006 John Wiley & Sons, Ltd.     

The effect of compression on noble gas solubility in silicate melts and consequences for degassing at mid-ocean ridges

The effect of compression on noble gas solubility in silicate melts is still badly understood due to a lack of theoretical guidance. In the experimental literature, noble gases dissolving in liquid silicates are found to concentrate almost linearly with increasing pressure up to several tens of kbar, suggesting that Henry’s law could be valid up to very high pressures, although this law stipulates that the gaseous phase in contact with the liquid must be ideal. Recently, new experiments dealing with the dissolution of argon in synthetic and natural silicate melts have pointed out that the evolution of concentration with pressure exhibits a departure from linearity in the 50-100 kbar range, leading either to a levelling off or to a sudden collapse of the argon concentration above 50 kbar. Here, we investigate by means of liquid state physics how volatile species dissolve into silicate melts under pressure. We use a hard sphere model (the reference fluid in liquid state physics) to describe silicate melts and gas at high pressures. One of our main results is that, when pressure increases, the concurrent compaction of gas and melt explains the almost-linear behaviour of the noble gas concentration up to several tens of kbars, before melt compaction dominates and concentration either levels off or decreases gradually in the 50-100 kbar range. In spite of the existence of a quasi-linear regime over a large pressure range, our work disqualifies the use of the Henry law when dealing with high pressures. The implication of these findings to provide an understanding of degassing at mid-ocean ridges is next investigated. Applying our model to the scenario where CO₂ vesicle generation occurs in the magma at mantle depths during its ascent from melting regions, we evaluate magma vesicularity as well as noble gas concentrations in the basalt melt and in vesicles as a function of pressure at depth. It is stressed that the variable and usually strong noble gas elemental fractionation observed in mid-ocean ridge basalts can be explained by assuming a sequence of several vesiculation stages interrupted by vesicle loss during magma ascent.     

The late Pan-African intracontinental linear fold belt of the Eastern Hoggar (Central Sahara,Algeria): geology,structural development,U/Pb geochronology,tectonic implications for the Hoggar shield

The structural development of the Tiririne Belt, located in the eastern Hoggar, central Sahara, Algeria has been entirely controlled by a high-strain, now vertical, N—S-trending zone, along which metamorphism and deformation gradually appear to the north in the Tiririne Formation, a clastic unit up to 8000 m thick whose sedimentological environment is described. U/Pb geochronology on zircons from a pretectonic sill within the Tiririne Formation indicates a pre-660 Ma depositional age. This intracontinental belt has been formed during the ‘late Pan-African’, as shown by the 604 and 585 Ma U/Pb zircon ages obtained on syn- to late-kinematic granitic phases from a circular pluton emplaced in the belt (using λ₈ = 0.155125 · 10^?9 y^?1 and λ₅ = 0.98485 · 10^?9 y^?1). The tectonic implications are discussed in the light of the structural and geochronological data. They suggest an eastwards younging of the peak of Pan-African deformation towards the East-Saharan craton, which has been stable for more than 660 Ma.     

Benefits, Costs, and Cooperation in Greenhouse Gas Abatement

Abatement cost and benefit projections through 2100are computed, assembled and interpreted with respectto various levels of emission reduction. Mathematicalexpressions describing regional costs and benefits asa function of abatement strategy are developed. Usingthese data and expressions, optimal abatementstrategies are defined for noncooperative andcooperative (Pareto optimal) policies. Thecooperative solution calls for an average emissionsreduction of 16.6 percent over the 1990–2100 period,as compared to 5.8 percent in the noncooperative case. Achieving the cooperative solution would require sidepayments to China and potentially to the U.S., as wellas stringent (though beneficial) restrictions onnon-OECD countries. It is argued that Paretooptimality is technically achievable but possiblyinfeasible in the real world.     

Report on the 4th International Meeting of the IUGS Lower Cretaceous Ammonite Working Group, the “Kilian Group” (Dijon, France, 30th August 2010)

The 4th Kilian Group meeting (Dijon, France, 30th August 2010) focused on the Aptian and Albian Stages. For the Aptian, a two-fold division of the stage was adopted for the Mediterranean area with a boundary between the Dufrenoyia furcata and Epicheloniceras martini Zones. The main changes to the zonal scheme concern the Lower Aptian with: the introduction of a Deshayesites luppovi Subzone in the upper part of the Deshayesites oglanlensis Zone; the replacement of Deshayesites weissi by Deshayesites forbesi as new index-species of the second interval zone; the introduction of a Roloboceras hambrovi Subzone in the upper part of the D. forbesi Zone; and the subdivision of the D. furcata Zone into the D. furcata and Dufrenoyia dufrenoyi Subzones. For the Albian, the upper part of the Douvilleiceras mammillatum Zone (Lower Albian) is now characterized by a Lyelliceras pseudolyelli Subzone. The main amendments concern the Upper Albian. The base of this substage is defined by the base of the Dipoloceras cristatum Zone. Above it, the Upper Albian zonal scheme comprises in stratigraphic order the Mortoniceras pricei, Mortoniceras inflatum, Mortoniceras fallax, Mortoniceras rostratum, Mortoniceras perinflatum and Arrhaphoceras briacensis Zones.     

Metamorphosed calcium‐aluminum‐rich inclusions in CK carbonaceous chondrites

CK chondrites are the only group of carbonaceous chondrites with petrologic types ranging from 3 to 6. Although CKs are described as calcium‐aluminum‐rich inclusion (CAI)‐poor objects, the abundance of CAIs in the 18 CK3–6 we analyzed ranges from zero to approximately 16.4%. During thermal metamorphism, some of the fine‐grained CAIs recrystallized as irregular assemblages of plagioclase + Ca‐rich pyroxene ± olivine ± Ca‐poor pyroxene ± magnetite. Coarse‐grained CAIs display zoned spinel, fassaite destabilization, and secondary grossular and spinel. Secondary anorthite, grossular, Ca‐rich pyroxene, and spinel derive from the destabilization of melilite, which is lacking in all CAIs investigated. The Al‐Mg isotopic systematics measured in fine‐ and coarse‐grained CAIs from Tanezrouft (Tnz) 057 was affected by Mg redistribution. The partial equilibration of Al‐Mg isotopic signatures obtained in the core of a coarse‐grained CAI (CG1‐CAI) in Tnz 057 may indicate a lower peak temperature for Mg diffusion of approximately 540–580 °C, while grossular present in the core of this CAI indicates a higher temperature of around 800 °C for the metamorphic event on the parent body of Tnz 057. Excluding metamorphic features, the similarity in nature and abundance of CAIs in CK and CV chondrites confirms that CVs and CKs form a continuous metamorphic series from type 3 to 6.     

Optical spectroscopy of X-Mega targets – II. The massive double-lined O-type binary HD 93205

A new high-quality set of orbital parameters for the O-type spectroscopic binary HD 93205 has been obtained combining échelle and coudé CCD observations. The radial velocity orbits derived from the He  ii λ 4686 Å (primary component) and He  i λ 4471 Å (secondary component) absorption lines yield semi-amplitudes of 133±2 and 314±2 km s⁻¹ for each binary component, resulting in minimum masses of 31 and 13 M_⊙ ( q =0.42) . We also confirm for the binary components the spectral classification of O3 V+ O8 V previously assigned. Assuming for the O8 V component a 'normal' mass of 22–25 M_⊙ we would derive for the primary O3 V a mass of 'only' 52–60 M_⊙ and an inclination of about 55° for the orbital plane. We have also determined for the first time a period of apsidal motion for this system, namely 185±16 yr using all available radial velocity data sets of HD 93205 (from 1975 to 1999). Phase-locked variations of the X-ray emission of HD 93205 consisting of a rise of the observed X-ray flux near periastron passage are also discussed.     

The Basel 1356 earthquake: which fault produced it?

The 1356 Basel earthquake was the strongest event to have shaken NW Europe in the last thousand years. The peculiar location of this historical event makes it possible to relate it to normal faulting along the edges of the Rhine Graben, as well as to reverse faulting along the Jura frontal thrust or to fault reactivation within the Hercynian basement. Alternate hypotheses are discussed and their implications compared taking into account available structural data and results of the morphotectonic study performed in the epicentral area. This study combines field observations with the analysis of SPOT satellite imagery, aerial photographs, and detailed topography. It is concluded that the Basel earthquake most probably reactivated a basement fault (reverse or wrench fault) beneath the shallow-depth aseismic detachment that underlies the Jura Mountains.