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Dive into the research topics where Renaud Merle is active.

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Featured researches published by Renaud Merle.


Journal of the Geological Society | 2009

Evidence of multi-phase Cretaceous to Quaternary alkaline magmatism on Tore-Madeira Rise and neighbouring seamounts from 40Ar/39Ar ages

Renaud Merle; Fred Jourdan; Andrea Marzoli; Paul R. Renne; Marion Grange; Jacques Girardeau

Abstract: The Tore–Madeira Rise is a seamount chain located 300 km off the Portugal and Morocco coasts attributed to hotspot activity. U–Pb ages of lavas from the northern and central Tore–Madeira Rise range between 103 and 80.5 Ma whereas 40Ar/39Ar ages from the central and southern Tore–Madeira Rise yield ages ranging from 94.5 to 0.5 Ma. We performed new 40Ar/39Ar measurements to better understand the geodynamic history of the Tore–Madeira Rise. Plagioclase ages from the Bikini Bottom and Torillon seamounts suggest ages of >90 Ma and ≥60 Ma, respectively. Amphiboles from the Seine seamount yield an age of 24.0 ± 0.8 Ma. Biotites from lavas of the Ashton seamount give ages of 97.4 ± 1.1 Ma and 97.8 ± 1.1 Ma. The geochronological database available on the Tore–Madeira Rise has been filtered on statistical criteria to eliminate unreliable ages. The resulting database reveals three pulses of alkaline magmatism on the Tore–Madeira Rise at 103–80.5 Ma, at c. 68 Ma and between 30 Ma and the present. The magmatism was continuous from 103 Ma until c. 68 Ma and from c. 30 Ma until the present on the Tore–Madeira Rise, the surrounding seamounts and the Portugal coast. We suggest that the space–time distribution of this magmatism results from the interaction between a wide thermal anomaly emitting magmatic pulses and the complex motion of the Iberian plate. Supplementary material: A detailed Ar measurements dataset is available at http://www.geolsoc.org.uk/SUP18359.


Geological Society of America Bulletin | 2015

Neoproterozoic to early Paleozoic extensional and compressional history of East Laurentian margin sequences: The Moine Supergroup, Scottish Caledonides

Peter A. Cawood; R. A. Strachan; Renaud Merle; Ian L. Millar; Staci Loewy; Ian W. D. Dalziel; Peter D. Kinny; Fred Jourdan; Alexander A. Nemchin; James N. Connelly

Neoproterozoic siliciclastic-dominated sequences are widespread along the eastern margin of Laurentia and are related to rifting associated with the breakout of Laurentia from the supercontinent Rodinia. Detrital zircons from the Moine Supergroup, NW Scotland, yield Archean to early Neoproterozoic U-Pb ages, consistent with derivation from the Grenville-Sveconorwegian orogen and environs and accumulation post–1000 Ma. U-Pb zircon ages for felsic and associated mafi c intrusions confi rm a widespread pulse of extension-related magmatism at around 870 Ma. Pegmatites yielding U-Pb zircon ages between 830 Ma and 745 Ma constrain a series of defor ma tion and metamorphic pulses related to Knoydartian orogenesis of the host Moine rocks. Additional U-Pb zircon and monazite data, and 40 Ar/ 39 Ar ages for pegmatites and host gneisses indicate high-grade metamorphic events at ca. 458–446 Ma and ca. 426 Ma during the Caledonian orogenic cycle. The presence of early Neoproterozoic silici clastic sedimentation and deformation in the Moine and equivalent successions around the North Atlantic and their absence along strike in eastern North America refl ect contrasting Laurentian paleogeography during the breakup of Rodinia. The North Atlantic realm occupied an external location on the margin of Laurentia, and this region acted as a locus for accumulation of detritus (Moine Supergroup and equivalents) derived from the Grenville-Sveconorwegian orogenic welt, which developed as a consequence of collisional assembly of Rodinia. Neoproterozoic orogenic activity corresponds with the inferred development of convergent platemargin activity along the periphery of the supercontinent. In contrast in eastern North America, which lay within the internal parts of Rodinia, sedimentation did not commence until the mid-Neoproterozoic (ca. 760 Ma) during initial stages of supercontinent fragmentation. In the North Atlantic region, this time frame corresponds to a second pulse of extension represented by units such as the Dalradian Supergroup, which unconformably overlies the predeformed Moine succession.


Geology | 2015

Age and geochemistry of magmatism on the oceanic Wallaby Plateau and implications for the opening of the Indian Ocean

Hugo K.H. Olierook; Renaud Merle; Fred Jourdan; Keith N. Sircombe; Geoff Fraser; Nicholas E. Timms; Gabriel Nelson; Kelsie A. Dadd; Laurent Kellerson; Irina Borissova

The temporal relationship between tectonic and volcanic activity on passive continental margins immediately before and after the initiation of mid-ocean ridge spreading is poorly understood because ...


Journal of the Geological Society | 2012

Provenance of the Highland Border Complex: constraints on Laurentian margin accretion in the Scottish Caledonides

Peter A. Cawood; Renaud Merle; R. A. Strachan; P. W. G. Tanner

Contrasting tectonic models for the Highland Border Complex in the Scottish Caledonides view it either as part of the rifted Laurentian margin of the Iapetus Ocean or as an oceanic terrane. Detrital zircon data from sandstones of the complex yield age peaks at 2.8–2.6, 1.3 and 1.1–1.0 Ga and minor peaks at c. 1.7–1.9 Ga. These characteristics compare closely with those of the upper Dalradian Supergroup of the adjacent Grampian terrane, and with the record of eastern Laurentia. The data are also consistent with the Laurentian provenance indicated by palaeontological evidence from the complex, and field evidence for continuity with the Dalradian Supergroup. Detrital ages for the Cambrian Salterella Grit of the Caledonian foreland compare with those for approximately age-equivalent sandstones from the Highland Border Complex. Both were contemporaneous with the regressive Hawke Bay event, accounting for similarities in provenance, and further linking the Highland Border Complex to Laurentia. The Grampian terrane was being uplifted and shedding detritus throughout the Ordovician and Silurian. The absence of this event from the detrital zircon records of either the Midland Valley or Southern Upland terranes suggests that these blocks cannot have been in their current location relative to the Grampian terrane before the end of the Silurian. Supplementary material: The complete analytical dataset and cathodoluminescence images are available at http://www.geolsoc.org.uk/SUP18531.


Australian Journal of Earth Sciences | 2015

Paleodrainage and fault development in the southern Perth Basin, Western Australia during and after the breakup of Gondwana from 3D modelling of the Bunbury Basalt

Hugo K.H. Olierook; Nicholas E. Timms; Renaud Merle; Fred Jourdan; P. Wilkes

The evolution of faults and paleodrainage patterns on the southwestern Australian passive margin during and after the breakup of Gondwana in the Early Cretaceous remains poorly understood. This contribution investigates the fault and paleodrainage evolution in the southern Perth Basin with the use of the ‘Bunbury Basalt’, the only lava flows known to be synchronous with continental breakup. New aeromagnetic data have been integrated with well intersections and outcrop constraints to establish the first 3D model of the Bunbury Basalt. The model reveals that flows are up to 100 m thick and are predominantly confined to two north–south-trending paleovalleys and their tributaries situated in the Bunbury Trough in the southern Perth Basin. The Donnybrook Paleovalley flow ponded in a paleovalley proximal to the Darling Fault and is truncated by the two later flows within the Bunbury Paleovalley, which is positioned centrally in the Bunbury Trough. Offsets of the Bunbury Basalt have been used to identify new northeast- and northwest-trending faults in the southern Perth Basin, and broad folding is interpreted as a consequence of drag into the Darling and Busselton faults. The model has been used to determine post-basalt net displacements for the Darling and Busselton faults of 370 and 210 m, respectively, and <175 m for the northeast and northwest-trending faults. The source vents for the Bunbury Basalt were probably located at extensional jogs at intersections between the Darling Fault and subordinate oblique faults. These results challenge the views on longstanding quiescence of the post-breakup western Australian passive margin.


Journal of the Geological Society | 2012

Occurrence of inherited supra-subduction zone mantle in the oceanic lithosphere as inferred from mantle xenoliths from Dragon Seamount (southern Tore–Madeira Rise)

Renaud Merle; Mary-Alix Kaczmarek; E.J. Tronche; Jacques Girardeau

Spinel-bearing peridotite and pyroxenite xenoliths dredged from the Dragon Seamount (southern Tore–Madeira Rise, West Iberia and Morocco margin) give an insight into the composition of the underlying lithosphere. These xenoliths are devoid of evidence of strong host lava–peridotite interaction and re-equilibration or late impregnation in the plagioclase facies. The spinels and pyroxenes from the Dragon peridotites have compositions distinct from those of both lherzolites and harzburgites from the Iberia margin and the Mid-Atlantic Ridge. They display a highly depleted composition, in particular, high Cr-number, up to 0.63 in the spinels, consistent with a melting degree between 12 and 19%. Because of the strong chemical similarities between the Tore–Madeira Rise, Newfoundland peridotites, and peridotites from supra-subduction zones, we propose that the Dragon peridotites formed in a similar context. The pyroxenites display a cumulate texture and are probably a high-temperature–high-pressure cumulate formed by fractional crystallization from a melt. The Tore–Madeira Rise peridotites may represent a former mantle wedge in an oceanic arc, later included into the continental lithosphere and finally tectonically disseminated within the lithosphere during the rifting of the Newfoundland–Iberia continental lithosphere. As a consequence, rifting processes may produce heterogeneities in the oceanic lithosphere and influence isotopic compositions of ocean island basalt-type lavas during plume–lithosphere interactions, as inferred for the southern Tore–Madeira Rise. Supplementary material: Further information on the analytical results is available at http://www.geolsoc.org.uk/SUP18512.


Journal of Petrology | 2017

Mt Bambouto Volcano, Cameroon Line: Mantle Source and Differentiation of Within-plate Alkaline Rocks

Renaud Merle; Andrea Marzoli; F. T. Aka; J. M. Chiaradia; Laurie Reisberg; F. Castorina; Fred Jourdan; Paul R. Renne; J. N’ni; J. B. Nyobe

The Late Cretaceous–Quaternary Cameroon Volcanic Line (CVL) is a 1600 km long chain of volcanoes that straddles the continent–ocean boundary and extends from the Gulf of Guinea to the interior of t ...


Archive | 2018

The Central Atlantic Magmatic Province (CAMP): A Review

Andrea Marzoli; Sara Callegaro; Jacopo Dal Corso; Joshua H.F.L. Davies; Massimo Chiaradia; Nassrrdine Youbi; Hervé Bertrand; Laurie Reisberg; Renaud Merle; Fred Jourdan

The Central Atlantic magmatic province (CAMP) consists of basic rocks emplaced as shallow intrusions and erupted in large lava flow fields over a land surface area in excess of 10 million km2 on the supercontinent Pangaea at about 201 Ma. The peak activity of the CAMP straddled the Triassic-Jurassic boundary and probably lasted less than 1 million years, while late activity went on for several Ma more into the Sinemurian. Emission of carbon and sulfur from the CAMP magmas and from intruded sediments probably caused extinctions at the end-Triassic. Intrusive rocks are represented by isolated dykes up to 800 km-long, by dense dyke swarms and by extremely voluminous sills and a few layered intrusions. Lava fields were erupted as short-lived pulses and can be traced over distances of several hundred km within sedimentary basins. They consist of either compound or simple pahoehoe flows. Globally, the intrusive and effusive rocks are estimated to represent an original magmatic volume of at least 3 million km3. Herein we subdivide the CAMP basalts for the first time into six main geochemical groups, five represented by low-Ti and one by high-Ti rocks. Except for one low-Ti group, which is ubiquitous throughout the entire province, all other groups occur in relatively restricted areas and their compositions probably reflect contamination from the local continental lithosphere. Major and trace elements and Sr-Nd-Pb-Os isotopic compositions indicate that the basaltic magmas had an enriched composition compared to Mid-Ocean Ridge basalts and different from Atlantic Ocean Island basalts. The enriched composition of CAMP basalts is only in part attributable to crustal contamination. It also probably requires subducted upper and lower continental crust material that enriched the shallow upper mantle from which CAMP basalts were generated. A contribution from a deep mantle-plume is not required by geochemical and thermometric data, but it remains unclear what other possible heat source caused mantle melting on the scale required to form CAMP.


Australian Journal of Earth Sciences | 2018

Geochronology of the Tore-Madeira Rise seamounts and surrounding areas: a review

Renaud Merle; Fred Jourdan; Jacques Girardeau

ABSTRACT We present new 40Ar/39Ar data for two of the Tore-Madeira Rise (TMR) volcanic seamounts. A sample from Tore East seamount on the northern part of the TMR yielded an ultra-precise age of 80.50 ± 0.13 Ma (2σ) that is similar within uncertainties to a published age obtained by U–Pb TIMS technique on titanites and zircons extracted from Tore NW seamount. Another sample from Isabelle seamount, located on the southern part of the TMR failed to produce a plateau age but yielded a minimum age estimate of >85 Ma. We filtered the published ages available on the TMR, the surrounding seamounts and the massifs of southwest Portugal to better understand the origin of this magmatic province. Together with this dataset, our new data suggest that: (1) a hypothetical Madeira hot-spot track spanning from Serra de Monchique on the continent to Madeira Archipelago is difficult to reconcile with the occurrence of several seamounts geographically located within or very close to this alleged hot-spot track yet being much older than the age predicted by the age trend.(2) The geographical distribution and age pattern of the TMR and surrounding areas magmatism are still best explained by the interaction of a mantle melting anomaly emitting magma pulses and the different motion phases of the Iberia plate since 103 Ma.


Journal of Petrology | 2018

The Kalkarindji Large Igneous Province, Australia: Petrogenesis of the Oldest and Most Compositionally Homogenous Province of the Phanerozoic

Bryant Ware; Fred Jourdan; Renaud Merle; Massimo Chiaradia; Kyle Hodges

The Kalkarindji Large Igneous Province (LIP) is a Middle Cambrian (511 Ma) continental flood basalt (CFB) province located in northern and central–west Australia that has been linked to an extinction event at the Early–Middle Cambrian boundary. The extent of this LIP has been esti- mated at about 2·1 x 106km2, with exposures in Western Australia, Northern Territory, Queensland and South Australia. Major and trace element datasets reveal geochemical charac- teristics typical for continental flood basalts (CFBs) including: tholeiitic affinity; an enrichment in incompatible elements, in particular, large-ion lithophile elements (LILE); enrichment of light rare earth elements (LREE) compared to heavy rare earth elements (HREE) relative to N-MORB; nega- tive Nb and Ta anomalies in normalized extended element patterns. Here we present the first comprehensive geochemical investigation of the Kalkarindji CFB province. The Kalkarindji CFBs are geochemically homogeneous, low-Ti basaltic andesites, with a nearly complete lack of basalts as defined using a total-alkalis vs silica diagram. All of the rocks analysed for Sr, Nd, Pb isotopic ratios display enriched initial (t 1⁄4 511 Ma) isotopic compositions (143Nd/144Ni 1⁄4 0·511928– 0·511981; 87Sr/86Sri 1⁄4 0·70917–0·71029; 206Pb/204Pbi 1⁄4 18·105–18·843; 207Pb/204Pbi 1⁄4 15·726–15·805; 208Pb/204Pbi 1⁄4 38·374–39·208). Crustal assimilation models are interpreted to suggest that the geo- chemical characteristics, as well as the homogenous composition across the entire province, cannot be explained by continental crust contamination. Therefore, the enriched isotopic ratios (particularly the extremely high 207Pb/204Pbi and elevated 208Pb/204Pbi for moderate 206Pb/204Pbi), coupled with relative depletions in Nb and Ta concentrations, indicate the involvement of an an- cient enriched lithospheric-like component in the genesis of the Kalkarindji CFB. We propose a model in which the source region was affected by an enrichment event at around 2·5 Ga (possibly through the addition of subducted sediments). Decompression melting and mantle warming (focused by edge driven convection) allowed melting of the fertile mantle to generate the Kalkarindji CFB province at c. 511 Ma.

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