The crystalline complexes of Hamadan (Sanandaj–Sirjan zone, western Iran): metasedimentary Mesozoic sequences affected by Late Cretaceous tectono-metamorphic and plutonic events

The Hamadan area is characterised by various metamorphic rocks where the slates yielded Jurassic fossils. The entire column, representing the Mesozoic from at least the Jurassic to the Mid-Cretaceous, has been affected by tectono-metamorphic events and the emplacement of Late Cretaceous granitic rocks. A timing of these events is based on the ⁴⁰K–⁴⁰Ar ages carried mainly on separated amphiboles, biotites and muscovites, and interpreted as the ages of their isotopic closure. Results are ranging between 91 and 70 Ma. To cite this article: A. Baharifar et al., C. R. Geoscience 336 (2004).

Résumé

La région de Hamadan expose des roches métamorphiques dont les termes les moins transformés contiennent des fossiles jurassiques. Au cours du Crétacé supérieur, elle a été affectée par un événement tectono-métamorphique régional et elle a été le siège d'une activité plutonique. Les résultats des datations ⁴⁰K–⁴⁰Ar des amphiboles et des micas séparés des roches métamorphiques et plutoniques qui s'étagent entre 91 et 70 Ma montrent l'importance de ces événements et leur étalement au cours du Crétacé supérieur. Pour citer cet article : A. Baharifar et al., C. R. Geoscience 336 (2004).     

Répartition et utilisation stratigraphique des Bryozoaires du crétacé moyen (Aptien-Coniacien)

Bien que la durée stratigraphique de la plupart des Bryozoaires crétacés ne soit pas exacterment connue, beaucoup d'espèces caractérisent assez bien les différents étages. Au Crétacé inférieur, dont la faune bryozoologique est plus pauvre que celle du Crétacé supérieur, ce sont les Cyclostomata qui dominent encore, comme au Jurassique. A l'Aptien, citons Chisma, mais aussi Ceata, Meliceritites et Laterocavea apparus au Barrémien. La faune de l'Albien, un peu appauvrie et peu connue, n'a fourni que quelques genres nouveaux encroûtants de Cheilostomata anasca (Rhammatopora, Wilbertopora).Au Cénomanien commence l'explosion des Bryozoaires. Les Cheilostomata les plus anciennes, les Cribrimorpha, les genres “Biflustra”, Cellarinidra, Quadricellaria, Onychocella, “Rhagasostoma”, Stichomicropora, Aechmella et un grand nombre de Cyclostomata (Crisisina, Heterocrisina, Fascipora, Spirentalophora, Marssoniella, Amphimarssoniella, Umbrellina, Exidmonea, Corymbopora, Desmopora, Discocytis, Supercytis, Truncatulipora, etc.) apparaissent. Le Turonien est caractérisé par les genres Cyclostomes (Reticrisina, Bicavea, Homoeosolen), les Cheilostomes (Tylopora, Euritina, Fusicellaria, Reptolunulites) et par de nombreuses Cribrimorpha.Onychocella nerei et Membranipora perincerta sont caractéristiques du Coniacien où l'on trouve aussi les Lunulites et Pavolunulites. Le Coniacien, plus riche en espéces que le Turonien, contient de très nombreux genres et espèces qui se poursuivent dans les étages plus élevés (Santonien-Maastrichtien).This paper deals with the distribution and stratigraphic value of Mid-Cretaceous Bryozoa (Aptian-Coniacian). Research on Cretaceous bryozoa has been neglected during the last decades and knowledge of the stratigraphical range of many Upper Cretaceous genera and species is based mainly on the personal experience of the present author. Accordingly, the range of most species is not exactly known, and the results of these investigations are only preliminary. Many cyclostomate genera (such as Stomatopora, Proboscina, Diastopora, Berenicea and Entalophora) lack easy identifiable specific characteristics, and all the other genera which can be recognized only by their rare ovicells (gonozoids) (such as Plagioecia, Diaperoecia, Microecia, Mecynoecia, Spiropora, Heteropora or Ceriopora, Reptomulticava, Lichenopora and many others) are not particularly suitable as guide-fossils. On the other hand, many characteristic new species have not yet been described.The bryozoa of the Lower Cretaceous are similar to those of the Jurassic. Both are characterized by the absolute predominance of the Cyclostomata and a few very rare primitive Cheilostomata belonging to the encrusting membranimorph Anasca.The Barremo-Aptian fauna, known mainly from England (Faringdon, Berkshire) and eastern and southern France, is characterized by the first Eleidae (Meliceritidae) with Meliceritites and Foricula, the first Ceidae, Clausidae and Horneridae with Siphodictyum and Laterocavea, Chisma furcillatum is known only from the Aptian. Cheilostomata are rare and are represented solely by encrusting membranimorph genera (Rhammotopora, “Membranipora”). The poor Albian bryozoan fauna, although similar to that of the Aptian, is characterized by the appearance of primitive uniserial cheilostomate genera such as (?) Pyriporopsis, Charixa and the genus Wilbertopora. Erect precenomanian Cheilostomata are not known. Albian Bryozoa are little-known and relatively rare.Within the Cenomanian (the plenus-zone included) many new cyclostomate genera Fascipora, Umbrellina, Siphoniotyphlus, Crisisina, Heterocrisina, Discofascigera, Corymbopora, Marssoniella, Amphimarssoniella, Discocytis, Discotruncatulipora, Truncatulipora, Desmepora, Exidmonea, Meliceritella and numerous cheilostomate genera besides “Membranipora” mainly Aechmella, Onychocella, Stichomicropora and several cribrimorphs appear for the first time. The Cenomanian is also characterized by the first erect cheilostomate species such as Onychocella, “Biflustra” or “Vincularia” and the oldest articulated or radicelled cheilostomes (Cellarinidra, Quadricellaria).During the Turonian (excluding the plenus-zone), which is less abundant in Bryozoa than the Cenomanian, the cheilostomes increase (common genera are Onychocella, Euritina, “Rhagasostoma”, bilamellar membranimorphs and cribrimorphs, mainly Rhabdopora) and the first primitive Lunulitidae (Reptolunulites) occur. Among the cyclostomes, represented by numerous species of Meliceritites, Semielea, Foricula, Truncatulipora, Clausa, Petalopora, Heteropora and the first representatives of Homoesolen, Reticrisina, Tervia and Bicavea appear.Within the Coniacian, rich faunas are known from France and England. Although the Cyclostomata are still dominant until the Santonian, considerable progress in the evolution of the Cheilostomata was made mainly by the development of the onychocellids, the erect membranimorphs and the radiation of the different cribrimorph families and genera. The oldest free-living Lunulitidae with Lunulites and Pavolunulites are recorded from the Coniacian. Among the Cyclostomata, the appearance of the genera Diplosolen, Clypeina, Crisina, Filicrisina, Sulcocava, Ditaxia, Pachyteichopora and Cytis is noteworthy. The Coniacian bryozoan fauna is closely related to that of the Santonian and has clearly an Upper Cretaceous character.I refer to the text for comments on single species which may be supposed to be useful as guide-fossils for the Aptian-Coniacian stages.     

Geology and geochemistry of the Caxias gold deposit, and geochronology of the gold-hosting Caxias Microtonalite, São Luís Craton, northern Brazil

The Caxias gold deposit, located in the São Luís Craton, is hosted by a steeply dipping strike-slip shear zone crosscutting schists and a fine-grained, hydrothermally altered tonalite (Caxias Microtonalite). Petrography and whole-rock geochemistry have characterized both pelitic and mafic protoliths for the hosting schists. The Caxias Microtonalite shows major and trace element behavior compatible with modern calc-alkaline, metaluminous, subduction-related granitoids. Geochronological studies on the Caxias Microtonalite have defined a minimum crystallization age of 1985±4 Ma, obtained by single-zircon Pb evaporation, and Sm–Nd crustal residence age (T_DM) of 2.17 Ga, with Nd(T) +0.74, suggesting a juvenile protolith. The exact origin and role of the Caxias Microtonalite remain uncertain. It may be interpreted as representing either a late manifestation of the regionally dominant Tromaí magmatism, or a juvenile episode unrelated to this major magmatism. Rock, quartz veins, and saprolite geochemistry have shown that As, Sb, Ba, Rb, V, Cr, Co, and Ni, as well as Au, are useful elements that can be used in exploration for similar deposits in the region.     

Relics of eclogite facies assemblages in the Ceará Central Domain, NW Borborema Province, NE Brazil: Implications for the assembly of West Gondwana

The Borborema Province, in the NE of Brazil, is a rather complex piece in the Brazil–Africa puzzle as it represents the junction of the Dahomeyide/Pharusian, Central African, Araçuai and Brasilia fold belts located between the West-African/São Luis, Congo/São Francisco and Amazonas craton. The correlation between the Dahomeyides from W-Africa (Ghana, Benin, Togo, and Mali) and the Borborema Province involves the Médio Coreaú and Central Ceará domains. The inferred continuation of the main oceanic suture zone exposed in the Dahomeyides of W Africa is buried beneath the Phanerozoic Parnaíba Basin in Brazil (northwest of the Médio Coreaú domain) where some high density gravity anomalies may represent hidden remnants of an oceanic suture. In addition to this major suture a narrow, nearly continuous strip composed of mainly mafic pods containing relics of eclogite-facies assemblages associated with partially migmatized granulite-facies metapelitic gneisses has been found further east in the NW Borborema Province. These high pressure mafic rocks, interpreted as retrograded eclogites, are located between the Transbrasiliano Lineament and the Santa Quitéria continental arc and comprise primitive to evolved arc-related rocks with either arc- or MORB-type imprints that can indicate either deep subduction of oceanic lithosphere or roots of continental and oceanic magmatic arcs. Average peak P–T conditions under eclogite-facies metamorphism (T = 770 °C and P = 17.3 kbar) were estimated using garnet–clinopyroxene thermometry and Jd content in clinopyroxene. Transition to granulite-facies conditions, as well as later widespread re-equilibration under amphibolite facies, were registered both in the basic and the metapelitic rocks and suggest a clockwise P–T path characterized by an increase in temperature followed by strong decompression. A phenomenon possibly related to the exhumation of a highly thickened crust associated with the suturing of the Médio Coreaú and Central Ceará domains, two distinct crustal blocks separated by the Transbrasiliano Lineament.     

Charophytes du Crétacé moyen et données nouvelles sur l'Evolution des Clavatoracées

La découverte de nouveaux gisements dans le Sud de la France révèle la persistance, dans le Cénomanien, d'Embergerella cruciata, Atopochara restricta et A. brevicellis (Clavatoraceae). Une parenté entre les genres Embergerella (Barrémien-Cénomanien) et Septorella (Maastrichtien) est envisagée sur la base d'une nouvelle interprétation de la structure de l'utricule. Pour la première fois, des représentants de la famille des Characeae sont décrits dans le Cénomanien: Peckisphaera revesti n. sp. et le Turonien: Mesochara fusiformis n. sp. Indications biostratigraphiques: dans l'état actuel des connaissances sur les flores de Charophytes du Crétacé moyen, seul le Cénomanien est bien caractérisé, par A. multivolvis à laquelle s'ajoute maintenant une nouvelle association de quatre espèces; l'Albien et le Turonien, pour lesquels des précisions sont apportées, restent toutefois encore mal individualisés.The discovery of new localities in the South of France shows that Embergerella cruciata, Atopochara restricta and A. brevicellis (Clavatoraceae) continued into the Cenomanian. A relationship between the genera Embergerella (Barremian-Cenomanian) and Septorella (Maastrichtian) is suggested on the basis of a new interpretation of the structure of the utricle. Representatives of the family Characeae are described for the first time, Peckisphaera revesti n. sp. in the Cenomanian and Mesochara fusiformis n. sp. in the Turonian. Biostratigraphic information: in the present state of knowledge of Middle Cretaceous Charophyte floras, only the Cenomanian is well characterized, by A. multivolvis to which is now added a new association of four species. Although new information is presented on the Albian and Turonian, they are still inadequately understood.     

The copper–gold and gold deposits of the Neoproterozoic Mara Rosa magmatic arc, central Brazil

Mineral exploration in the Neoproterozoic Goiás Magmatic Arc, central Brazil, dates back to the beginning of the 1970s. The Goiás Magmatic Arc extends for more than 1000 km in the western and northern parts of Goiás, into Tocantins, and disappears under the Phanerozoic Parnaíba Basin. Two main areas of Neoproterozoic juvenile crust, the Arenópolis and the Mara Rosa arcs, are identified. They lie in the southern and northern sectors of the Goiás Arc, respectively, and are relatively well studied.The Goiás Magmatic Arc dominantly comprises tonalitic/dioritic orthogneisses and narrow NNE-striking volcano-sedimentary belts. Recent U–Pb zircon data indicate crystallization of the tonalite protoliths in two main episodes: the older between ca. 890 and 790 Ma and the younger at 670–600 Ma. Nd isotopic data indicate the very primitive nature of the original magmas, with T_DM model ages mostly within the interval between 0.9 and 1.0 Ga and _Nd(T) values between +3.0 and +4.6. In the Chapada–Mara Rosa area, the supracrustal rocks form three individual NNE belts, known as the eastern, central and western belts, separated from each other by metatonalites/metadiorites.Gold and Cu–Au deposits of the Mara Rosa area occur in four main associations: (i) Au–Ag–Ba (e.g., Zacarias), which are interpreted as stratiform, disseminated volcanogenic deposits, (ii) Cu–Au (e.g., Chapada) which has been interpreted either as volcanogenic or as a porphyry-type deposit, (iii) Au-only deposits (e.g., Posse), interpreted as an epigenetic disseminated deposit controlled by a mesozonal shear zone and (iv) Au–Cu–Bi (e.g., the Mundinho occurrence), which are considered as vein-type deposits controlled by magnetite-rich diorites.The gold and Cu–Au deposits located within the Goiás Magmatic Arc can be spatially and temporally related to the magmatic evolution of a collisional belt or, in other words, to an orogenic gold deposit model. These models are based on the continuous evolution of collisional plates, which can be subdivided into four stages with distinct magmatic characteristics: (i) subduction stage, (ii) syntectonic collisional magmatism stage, (iii) post-tectonic collisional magmatism stage and (iv) post-orogenic extension stage.     

K–Ar and Ar/Ar ages of dikes emplaced in the onshore basement of the Santos Basin, Resende area, SE Brazil: implications for the south Atlantic opening and Tertiary reactivation

New K–Ar and ⁴⁰Ar/³⁹Ar data of tholeiitic and alkaline dike swarms from the onshore basement of the Santos Basin (SE Brazil) reveal Mesozoic and Tertiary magmatic pulses. The tholeiitic rocks (basalt, dolerite, and microgabbro) display high TiO₂ contents (average 3.65 wt%) and comprise two magmatic groups. The NW-oriented samples of Group A have (La/Yb)_N ratios between 15 and 32.3 and range in age from 192.9±2.2 to 160.9±1.9 Ma. The NNW-NNE Group B samples, with (La/Yb)_N ratios between 7 and 16, range from 148.3±3 to 133.9±0.5 Ma. The alkaline rocks (syenite, trachyte, phonolite, alkaline basalts, and lamprophyre) display intermediate–K contents and comprise dikes, plugs, and stocks. Ages of approximately 82 Ma were obtained for the lamprophyre dikes, 70 Ma for the syenite plutons, and 64–59 Ma for felsic dikes. Because Jurassic–Early Cretaceous basic dikes have not been reported in SE Brazil, we might speculate that, during the emplacement of Group A dikes, extensional stresses were active in the region before the opening of the south Atlantic Ocean and coeval with the Karoo magmatism described in South Africa. Group B dikes yield ages compatible with those obtained for Serra Geral and Ponta Grossa magmatism in the Paraná Basin and are directly related to the breakup of western Gondwana. Alkaline magmatism is associated with several tectonic episodes that postdate the opening of the Atlantic Ocean and related to the upwelling of the Trindade plume and the generation of Tertiary basins southeast of Brazil. In the studied region, alkaline magmatism can be subdivided in two episodes: the first one represented by lamprophyre dykes of approximately 82 Ma and the second comprised of felsic alkaline stocks of approximately 70 Ma and associated dikes ranging from 64 to 59 Ma.

Resumo

Novos dados K–Ar e ⁴⁰Ar/³⁹Ar de enxames de diques toleíticos e alcalinos localizados no embasamento onshore da Bacia de Santos (SE Brasil) apontam para diferentes pulsos magmáticos ocorridos entre o Jurássico e o Terciário. Os diques de rochas toleíticas (basalto, diabásio e microgabro), são mais velhos, exibem altos teores de TiO₂ (3,65% peso na média) e podem ser subdivididos em dois grupos magmáticos. O Grupo A aflora a norte da Bacia de Resende, compreende diques orientados na direção NW, com razões (La/Yb)_N entre 15 e 32,3, e idades entre 192.9±2.2 e 160.9±1.9 Ma. O Grupo B aflora a sul e a leste da Bacia de Resende, engloba diques orientados na direção NNW e NNE, com razões (La/Yb)_N entre 7 e 16, e idades obtidas entre 148.3±3 e 133.9±0.5 Ma. As rochas alcalinas (sienito, traquito, fonolito, basalto alcalino e lamprófiro) possuem teores médios de K, e afloram como diques, plugs e stocks.. As idades obtidas são de ca. 82 Ma para os diques lamprofíricos, de ca. 70 Ma para os plugs sieníticos, e entre 64 e 59 Ma para os diques félsicos. Como estas idades Jurássicas para diques toleíticos ainda não foram descritas para a região sudeste do Brasil, pode-se especular que durante o emplacement dos diques do GrupoA o cenário tectônico indicaria esforços extensionais anteriores à abertura do Oceano atlântico Sul, e contemporânea ao derrame basáltico do Karoo na África do Sul. Já os diques do Grupo B são contemporâneos ao magmatismo Serra Geral e ao enxame de diques de Ponta Grossa, e portanto este episódio está diretamente relacionado à separação entre o Brasil e África no Cretáceo. O magmatismo alcalino está associado a diversos episódios tectônicos que sucedem à abertura do Oceano Atlântico Sul e que resultaram no desenvolvimento das Bacias terciárias do sudeste brasileiro. Está provavelmente relacionado à chegada da Pluma de Trindade e as idades obtidas para a região em estudo indicam que o magmatismo lamprofírico é mais antigo (ca. 82 Ma), seguido pelos plútons sieníticos (ca. 70 Ma) e diques associados (64 a 59 Ma.)     

Les Bélemnites

Dans la partie moyenne du Crétacé, les bélemnites définissent deux grandes provinces en Europe, toutes deux occupées, jusqu'au Cénomanien moyen, par les Belemnopseidae. Puis les bélemnites disparaissent de la province mésogéenne tandis qu'en Europe du Nord leur évolution se poursuit avec les Belemnitellidae.The belemnites of the middle part of the Cretaceous define two broad provinces in Europe: a Mesogean Province to the south, characterized by representatives of the Belemnopseidae up to the Middle Cenomanian (after which belemnites disappeared from this province) and a North European Province, belonging to the “boreal realm”, in which Belemnopseidae occur up to Middle Cenomanian and Belemnitellidae from the beginning of the Cenomanian.     

Répartition des Bivalves (sans inocérames ou rudistes) dans le Crétacé moyen

Parmi les Bivalves, les groupes dont les coquilles ont une assez forte teneur en calcite, se retrouvent très fréquemment dans les dépôts du Crétacé. En général, il s'agit de Ptériomorphes, et au Crétacé moyen particulièrement d'huîtres (Ostreacea), de peignes (Pectinidés s.l.), de Spondylidés, de limes (Limidés), de plicatules et d'Anomidés.Le rapport présenté ici reprend assez complètement les Limidés et les Pectinidés d'Europe, d'Afrique du Nord et du Texas; pour les huîtres une sélection a été faite en essayant d'y inclure des espèces utilisées en stratigraphie. Je me suis basée uniquement sur des examplaires étudiés personnellement. Certains ont été récoltés sur le terrain, mais la majeure partie a étéétudiée dans les collections de nombreux musées d'Europe et d'Amérique du Nord—les énumérer serait fastidieux et la liste n'en est pas incluse. Cependant l'objectivité scientifique m'oblige à préciser que les données pour le domaine tempéré d'Europe et pour la Téthys du Texas sont plus nombreuses que celles obtenues pour le domaine mésogéen d'Europe et d'Afrique du Nord; surtout, dans une partie des collections téthysiennes que j'ai pu étudier les indications stratigraphiques manquaient de précision; ceci pourrait expliquer certaines anomalies dans les résultats.Les subdivisions stratigraphiques utilisées sont celles présentées pour le WG9 du MCE.Au Crétacé moyen les Ptériomorphes se différencient partiellement entre les domaines téthysien et tempéré-boréal. De l'Albien au Turonien les dépôts présumés boréaux sont relativement rares; ils se retrouvent cependant à Bornholm, en U.R.S.S., et dans certains dépôts du Cénomanien supérieur du bassin anglo-parisien (Plenus marls) comme il a été démontré par Jefferies (1962).Les Ptériomorphes les mieux connus se trouvent dans le domaine tempéré. La diversité des faciès et les adaptations à ces faciès par les groupes étudiés, peuvent expliquer le grand nombre d'espèces reconnues (une liste des faunes est donnée).Among the Pelecypods, the groups with rich calcite shells are abundant in the Cretaceous deposits. In general, they belong to the Pteriomorphia and, especially in the middle Cretaceous, to oysters (Ostreacea), Pectinids s.l., Spondylacea, Limacea, Plicatula and Anomiacea.This report resumes the study of Limacea and Pectinids of Europe, North Africa and Texas. From among the oysters a selection has been made, trying to include species with a stratigraphical use. I have based my work only on specimens studied personally. Some of them were collected in the field, but most were studied in the collections of numerous European and North American Museums. I cannot enumerate all these forms, and the list is not included. Nevertheless, for scientific objectivity it must be specified that the data from the European temperate realm and from the Tethyan Texas are more abundant than those from the European and North African mesogean realms. Above all, a part of the Tethyan collections studied shows a lack of stratigraphical precision, which could explain some anomalies in the results.Stratigraphical subdivisions used are those of the WG 9 of the MCE.During the middle Cretaceous the Pteriomorphia are differentiated between the Tethyan and the temperate-boreal realms. From Albian to Turonian, the presumed boreal deposits are relatively rare; they still exist in Bornholm, the U.S.S.R. and in some upper Cenomanian deposits from the anglo-Paris Basin (Plenus marls), as was proved by Jefferies (1962).The well known Pteriomorphia are in the temperate realm. The variety of the facies and the adaptations to these facies for the groups studied can explain the great number of recognized species (a list of the fauna is given).     

Un Pachyerymnoceras arabique dans le Callovien supérieur du Dahar (Sud tunisien), nouvel élément de datation du membre Ghomrassène (formation Tataouine) ; corrélations avec l'Arabie Saoudite et le Moyen-Orient

The first ammonite discovered at the base of the Ghomrassène Member of the Tataouine Formation belongs to a species of Pachyerymnoceras from the Latest Callovian (Solidum Zone) of the Arabian province. The underlying Krechem el Miit Member is also dated Late Callovian, with a fauna of Pachyerymnoceras from the Lower Athleta Zone in Algeria. The associated faunas (echinids, brachiopods) are the same, as well as the faunas of the overlying Ksar Haddada Member, which is dated also Late Callovian, referring to the brachiopods faunal succession in Saudi Arabia. Correlations with other areas in Tunisia, Saudi Arabia and Middle East underline the same sedimentary evolution during a second-order transgressive half-cycle. To cite this article: R. Enay et al., C. R. Geoscience 334 (2002) 1157–1167.

Résumé

La première ammonite découverte à la base du membre Ghomrassène de la formation Tataouine est un Pachyerymnoceras de la partie supérieure du Callovien supérieur (Zone à Solidum) de la province arabique. Le membre Krechem el Miit sous-jacent est aussi daté du Callovien supérieur par des Pachyerymnoceras connus dans la partie inférieure de la Zone à Athleta en Algérie. La faune associée (échinides, brachiopodes) est la même que celle du membre Ksar Haddada sus-jacent, daté également du Callovien supérieur par référence à la succession des brachiopodes en Arabie Saoudite. Les corrélations avec les autres régions de Tunisie, l'Arabie Saoudite et le Moyen-Orient mettent en évidence une même évolution sédimentaire au cours d'un demi-cycle transgressif de deuxième ordre. Pour citer cet article : R. Enay et al., C. R. Geoscience 334 (2002) 1157–1167.     

The pegmatites of the Nova Era–Itabira–Ferros pegmatite district and the emerald mineralisation of Capoeirana and Belmont (Minas Gerais, Brazil): geochemistry and Rb–Sr dating

The chemical composition and Rb–Sr ages of mica, feldspar, and whole rock samples from the emerald mineralisation of Capoeirana and Belmont, from emerald-barren pegmatites and of the Borrachudos granitic gneiss, Monlevade banded and granitic gneisses from the area of Nova Era–Itabira–Ferros (Minas Gerais, Brazil) as well as from the Guanhães gneiss (Minas Gerais, Brazil) have been determined. The Borrachudos granitic and Monlevade banded gneiss with connected pegmatitic schlieren and pegmatite veins, as well as the Guanhães gneiss, got their actual textures and mineralogical composition at about 1.9 Ga in the context of the Transamazonic tectonothermal event.The Monlevade banded gneiss belongs to a volcano-metasedimentary greenstone belt sequence, which is the typical country rock of the emerald occurrences. The main emerald-forming event at Belmont and Capoeirana was a metasomatic reaction of Be-rich anatectic pegmatites with Cr-rich ultrabasic rocks during the Transamazonic event. At Capoeirana, K–feldspar-bearing Be-rich pegmatites were transformed during the emerald-forming process into plagioclase–quartz rocks. Rb–Sr ages on biotite of about 480 Ma from the emerald mineralisation result from the rejuvenation of Transamazonic biotite by the Brasiliano event.The widespread macroscopically unmetamorphosed pegmatites of the study area formed in the Brasiliano event at 477±14 Ma. These pegmatites resulted to be emerald-barren although the differentiation degree, as given by diagrams such as Cs vs. K/Rb for muscovite and K–feldspar, starts from ceramic and ends with Be pegmatites. Some pegmatites display a marked internal differentiation.

Abstract

Foram determinadas as composições químicas e as idades Rb–Sr de mica branca, feldspato potássico e de rochas totais das mineralizações de esmeraldas de Capoeirana e Belmont, de pegmatitos sem esmeraldas e dos gnaisses Borrachudos, Monlevade e Guanhães da região de Nova Era–Itabira–Ferros (Minas Gerais, Brazil). Os gnaisses graníticos Borrachudos, os gnaisses bandados Monlevade, seus respectivos pegmatitos e veios/schlieren pegmatóides, e os gnaisses Guanhães, adquiriram suas texturas e composições mineralógicas atuais há cerca de 1.9 Ga no contexto do evento Transamazônico.As rochas regionais encaixantes típicas das ocorrências de esmeraldas são os gnaisses Monlevade que pertencem a uma sequência metavulcano-sedimentar de tipo greenstone belt. O evento principal de formação de esmeraldas em Belmont e Capoeirana foi uma reação metassomática dos pegmatitos anatéticos ricos em Be com rochas ultrabásicas ricas em Cr durante o evento Transamazônico em torno de 1.9 Ga. Em Capoeirana nesse contexto os pegmatitos com feldspato potássico ricos em Be foram transformados em rochas de plagioclasio–quartzo. As idades Rb–Sr de cerca de 480 Ma de minerais das mineralizações de esmeralda resultaram da reequilibração de biotitas e feldspatos Transamazônicos durante o evento Brasiliano.Os pegmatitos não-metamórficos e sem esmeralda da região estudada foram formados no evento Brasiliano há 477±14 Ma. O grau de diferenciação dos pegmatitos, estudado em diagramas indicadores específicos como por exemplo Cs vs. K/Rb de micas brancas e feldspatos potássicos, varia desde pegmatitos cerámicos até muscovita-pegmatitos, à pegmatitos de metais raros e até berilíferos. Alguns dos pegmatitos apresentam marcante diferenciação interna.     

Use of two-dimensional electric resistivity and ground penetrating radar for archaeological prospecting at the ancient capital of Egypt

Two-dimensional (2-D) resistivity and ground penetrating radar (GPR) surveys facilitate tracing of buried archaeological relics at the archaeological site of the Tell El Rabi'a, southwestern Cairo. These surveys also provide information on variations in depth of the groundwater table, which affect both exhumed and buried archaeological remains. The 2-D electrical resistivity profiles obtained show some high anomalies (up to 6900 Ω m). Based upon on-site calibration at partly exhumed sites, such anomalies are interpreted as pillar crowns and wall-like structures of hard limestone of the Hathour temple. The low background resistivities are interpreted to represent riverine deposits with differing moisture (or saturation) characteristics. The results of the GPR survey show three forms of high-amplitude radar anomalies, denoted as “P, H and R”. The “P” anomalies have semi-hyperbolic shapes, which suggest the presence of thin buried walls. The second, near-horizontal group of anomalies, “H”, may be either due to the presence of thick buried walls or arise from coincidental parallel alignment of survey lines with buried linear structures. The third group of GPR anomalies “R” is composed of chaotic reflections, and interpreted to depict buried stone-filled chambers. Some un-exhumed parts of the study area show weak radar reflections with occasional highly attenuated radar signals. These phenomena are ascribed to differing compaction and moisture characteristics of riverine soil layers. Recommendations with regard to archaeological site-excavation, preservation of archaeological relics, and soil conservation are submitted.     

First U–Pb SHRIMP age of the Hauterivian stage, Neuquén Basin, Argentina

A high-resolution ion-microprobe (SHRIMP) U–Pb zircon age from a tuff layer intercalated in the ammonoid bearing sedimentary succession of the Neuquén Basin in Argentina provides a robust geochronologic date to add to the absolute ages and to improve the relative chronology of the Early Cretaceous Hauterivian stage. The tuff layer appears interbedded between shales of the upper member (Agua de la Mula) of the Agrio Formation within the Spitidiscus riccardii ammonoid zone (base of the Late Hauterivian) yielding a date of 132.5 ± 1.3 Ma. This date confirms and supports an accurate correlation between the ammonoid biostratigraphy of the Neuquén Basin with the Western Mediterranean Province of the Tethys during the Early Cretaceous and matches with the most recently published time scale. It also casts doubts on the validity of K–Ar ages on glauconite-grains recently reported from the Lower Cretaceous of the Vocontian Basin of France.     

Changement de faunes de bryozoaires dans le Valanginien supérieur des Alpes-de-Haute-Provence. Parallélisme avec la crise observée dans le Jura à la même époque

Dans le Valanginien supérieur (Marnes à Toxaster et Grande Lumachelle) des Alpes-de-Haute-Provence, la succession de deux faunes de bryozoaires est observée. Parmi les causes du changement de faune, le remplacement d'un fond vaseux en eau calme (Marnes à Toxaster) par un fond sableux coquillier en eau assez agitée (Grande Lumachelle) est certainement important. Cependant, ces modifications résultent elles-mêmes d'événements plus généraux.Le changement de faune peut être comparé à celui qui intervient dans le Jura au début de la zone à Trinodosum. La faune des Marnes à Toxaster (zone à Verrucosum) montre certaines des espèces caractéristiques de la “faune 1” du Jura et, de plus, les deux mêmes espèces dominantes. Le milieu de vasière des Marnes à Toxaster, opposé à celui de plate-forme carbonatée du Jura, entraîne seulement un appauvrissement spécifique. Quant à la faune de la grande Lumachelle, elle est absolument semblable à la “faune 2” récoltée dans les Marnes à bryozoaires et le Calcaire à Alectryonia du Jura.Ce parallélisme des deux faunes avec celles du Jura, malgré les différences de faciès sédimentaire, montre que le changement de faune, maintenant reconnu sur près de 400 km, résulte d'une même cause principale. Ainsi, l'hypothèse d'un refroidissement que j'ai proposée pour le Jura semble pouvoir être étendue à la Provence.The change of bryozoan fauna in the upper Valanginian of the Alpes-de-Haute-Provence. Parallelism with the crisis observed in the Jura at the same time.In the upper Valanginian (Marnes à Toxaster and Grande Lumachelle) of the Alpes-de-Haute-Provence, the succession of two bryozoan faunas is observed. Among the reasons for the change of fauna, the replacement of a muddy bottom in calm water (Marnes à Toxaster) by a sandy-shelly bottom in rather agitated water (Grande Lumachelle) is certainly important, but these modifications are the result of more general events. The change of fauna could be compared with the one that took place at the beginning of the Trinodosum Zone in the Jura. The fauna of the Marnes à Toxaster (Verrucosum Zone) shows some characteristic species of the “faune 1” of the Jura and, moreover, the same two dominating species. The muddy basin environment of the Marnes à Toxaster, unlike the carbonate platform environment in the Jura, involves only a specific impoverishment. As for the fauna of the Grande Lumachelle, it is totally identical to the “faune 2” found in the Marnes à bryozoaires and the Calcaire à Alectryonia of the Jura.This parallelism of the two faunas with those of the Jura, in spite of the differences of sedimentary facies, shows the change of the fauna now observed over about 400 km, has the same principal cause. Thus it seems possible to extend the cooling hypothesis I have proposed for the Jura, to Provence.     

Offneria arabicanov. sp. (rudiste, Caprinidae) de l''Aptien inférieur du Jebel Madar (Sultanat d''Oman)

Offneria arabicanov. sp. (rudiste, Caprinidae) est caractérisé par la simplicité de l'architecture de la valve supérieure, bien exprimée par la forme subrectangulaire des canaux où les planchers sont relativement rares, et le faible développement des tabulae. La valve inférieure est beacoup plus complexe, ce qui traduit un taux d'evolution différencié des deux valves. L'espèce a été) trouvée dans l'Aptien inférieur (Formation Shuaiba) du Jebel Madar, dans l'avant pays des nappes des Montagnes d'Oman. Son organisation la rattache au groupe des formes arabo-africaines. A côté de ses caractères évolutifs, elle est intéressante par son potentiel biostratigraphique et paléobiologéographique.

Abstract

Offneria arabicanov. sp. (rudist, Caprinidae) is characterized by the simplicity of the upper valve, well expressed by the subrectangular shape of the canals where horizontal partitions are relatively rare, and the weak development of the tabulae. The lower valve is far more complex, which means distinctive evolutionary rates for the two valves. The species was found in the Lower Aptian (Shuaiba Formation) of the Jebel Madar, in the foreland of the Oman Mountain nappes. By its overall organisation it belongs to the Arabo-African group of species. Besides its evolutionary characters this form is interesting because of its biostratigraphic and palaeobiogeographic potential.     

Mise en evidence par le paleomagnetisme d'une importante rotation antihoraire des Vosges meridionales entre le Viseen terminal et le Westphalien superieur

The volcano-sedimentary formations from the southern Vosges are subdivided in two main series: a lower Visean series characterized by a volcanism of spilite-keratophyre type, and an upper Visean series which includes a normal volcanic association of shoshonitic tendency. Paleomagnetic study of 50 sites sampled in both series, but mostly in the upper one, yields three types of directions of characteristic magnetizations. The first type corresponds to Tertiary and Quaternary remagnetizations with low apparent blocking temperatures (350°–500°C, titano-maghemites?). The second group is formed by remagnetizations which have taken place during late Carboniferous-early Permian times, and which show high blocking temperatures of magnetite and mostly titano-haematites. The mean direction is D = 16°, I = 7°, α₉₅ = 9° for 13 sites, (λ = 43°N, φ = 165°E). The last group is represented by primary magnetizations of latest Visean age and post-Sudetic remagnetizations, with blocking temperatures of magnetite and haematite. The mean direction D = 323°, I = −17°, α₉₅ = 9° for 18 sites, (λ = 25°N, φ = 228°E), deviates from about 60° from the theoretical direction, calculated with the early Carboniferous, European pole position. This deviation is interpreted as resulting from a counterclockwise rotation of the southern Vosges between late Visean and Westphalian times. One consequence may be the formation of the variscan “V”, due to the anticlockwise rotation of the eastern branch of the chain. The northwesterly directions show a variation of the inclinations which may indicate that the rotation was preceded by a relatively significant drift of the Vosges to the north.

Résumé

Les terrains volcano-sédimentaires des Vosges méridionales se subdivisent en deux séries principales: la série du Viséen inférieur caractérisée par un volcanisme du type spilite-kératophyre et la série du Viséen supérieur qui comporte une association volcanique normale à tendance shoshonitique. L'étude paléomagnétique de 50 sites échantillonnés dans les deux séries, avec une prédominance dans la série supérieure, met en évidence trois types de directions d'aimantations caractéristiques, Le premier type correspond à des réaimantations d'áge Tertiaire à Quaternaire, à températures de blocage apparentes basses (350°–500°C, titano-maghemites?). Le second groupe est f'orme par des réaimantations mises en place au Carbonifère supérieur-Permien inférieur, à température de blocage haute de magnétite et surtout de titanohématites. La direction moyenne est D = 16°, I = 7°, α₉₅ = 9° pour 13 sites. (λ = 43°N, φ = 165°E). Le dernier groupe est représenté par des aimantations primaires, d'âge Viséen supérieur et des réaimantations post phase Sudète II, à température de blocage de magnetite et d'hématite. La direction moyenne D = 323°, I = −17°, α₉₅ = 9° pour 18 sites (λ = 25 °N, φ = 228°E), dévie de prés de 60° de la direction théorique calculée à partir du pôle européen au Carbonifère inférieur. Cette déviation est interprétée comme résultant d'une rotation antihoraire des Vosges méridionales entre le Viséen supérieur et le Westphalien. Une des conséquences en serait la formation du “V” varisque. par suite de la rotation antihoraire de la branche orientale de la chaîne. Les directions nord-ouest présentent une variation en inclinaison qui semble indiquer que la rotation antihoraire était précédée par une dérive relativement importante des Vosges vers le Nord.     

Répartitions comparées de foraminifères planctoniques du Crétacé moyen dans la téthys et la mer boréale par rapport à une zonéologie macropaléontologique

Cette note donne une présentation des résultats obtenus par le Groupe de Travail européen des foraminifères planctoniques de 1976 à 1978.The results obtained by the European MCE working group on planktic foraminifera are summarized. A total of 49 species were revised, referable to the genera Planomalina, Rotalipora, Hedbergella, Whiteinella, Archaeoglobigerina, Praeglobotruncana, Dicarinella and Marginotruncana.     

Regional shear variation in relation to diapirism and folding

Regional structural trends in the Lévézou area (southern Massif Central, France) delineate an antiformal structure. Deformed granitoids display changes along strike in S---C plane relationships, and therefore in sense of shear. These variations are interpreted to be strain accommodation features that developed during the diapiric emplacement and folding of the granitoid sheets, and so cannot be used as kinematic indicators on a regional scale.     

La prévision du climat : de l'échelle saisonnière à l'échelle décennale

The atmosphere and the ocean are subject to many dynamical instabilities, which limit the time during which their behaviour can be deterministically forecasted. At longer timescales, the atmosphere can be predicted at best using statistical methods, as a response to external forcing linked to sea- and land-surface anomalies. Climate being defined as the mean of atmospheric states, it appears that it can be predicted up to a few months in advance, which is the characteristic time of the so-called slow components of the climate system. Forecasting can sometimes be extended to longer time ranges, especially when the coupled ocean–atmosphere system exhibits internal variability modes, with characteristic times of a few years. Seasonal climate forecasting is most often based upon Monte-Carlo simulations, where the various realisations correspond to slightly different initial conditions. The present sate-of-the-art in Europe (ECMWF) and/or in the USA (IRI) allows to forecast such major phenomena, as El Niño, up to six months in advance. Finally, some parameters may exhibit predictability at still longer time-ranges (inter-annual to decadal), but only for certain regions. The example of electricity production is used to underline the potentially large economical benefit of seasonal climate forecasting. To cite this article: J.-C. André et al., C. R. Geoscience 334 (2002) 1115–1127.

Résumé

L'atmosphère et l'océan sont le siège d'instabilités dynamiques, qui limitent la durée pendant laquelle il est possible d'en prévoir l'évolution de façon déterministe. Au-delà, l'atmosphère n'est plus prévisible, au mieux, que de façon statistique, en fonction du forçage externe qu'exerce(nt) sur elle l'océan et/ou la surface des continents. Le climat (au sens d'une moyenne des états atmosphériques) se révèle ainsi prévisible jusqu'à des échéances temporelles de quelques mois, échelle de temps caractéristique des composantes dites « lentes » du système climatique. La prévision peut s'étendre à des échéances parfois plus longues, dans le cas où le système couplé océan–atmosphère posséderait des modes de variabilité temporelle de périodes caractéristiques de quelques années. La prévision climatique saisonnière est très souvent construite à partir de simulations de type Monte-Carlo, avec des ensembles de réalisations utilisant des conditions initiales légèrement différentes. Dans l'état actuel de ces prévisions, qu'elles soient réalisées en Europe (CEPMMT) ou aux États-Unis (IRI), il est possible de prévoir environ six mois à l'avance un certain nombre de phénomènes climatiques, en particulier ceux liés aux épisodes dits « El Niño », pour lesquels l'amplitude des variations est suffisamment importante. Il existe, par ailleurs, une prévisibilité à encore plus longue échéance (inter-annuelle à décennale), mais seulement pour certains paramètres et certaines régions. L'exemple de la production d'électricité montre l'importance économique potentielle très grande de la prévision climatique saisonnière. Pour citer cet article : J.-C. André et al., C. R. Geoscience 334 (2002) 1115–1127.