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Revista Brasileira de Geofísica

Print version ISSN 0102-261X

Rev. Bras. Geof. vol.26 no.1 São Paulo Jan./Mar. 2008 

Geophysical and geochemical evidence for cold upper mantle beneath the Equatorial Atlantic Ocean



Susanna Eleonora SichelI; Sonia EsperançaII; Akihisa MotokiIII; Marcia MaiaIV; Mary F. HoranV; Peter SzatmariVI; Eliane da Costa AlvesVII; Sidney L.M. MelloVIII

IDepartamento de Geologia, LAGEMAR, Universidade Federal Fluminense, Brazil. E-mail:
IIDivision of Earth Sciences, National Science Foundation, Arlington, VA 22230, USA. E-mail:
IIIDepartamento de Mineralogia e Petrologia Ígnea, Universidade do Estado do Rio de Janeiro, Brazil. E-mail:
IVCNRS, UMR 6538 Domaines Océaniques, IUEM, Plouzané, France. E-mail:
VDTM-CIW, 5241 Broad Branch Rd, Washington DC, USA. E-mail:
VIIDepartamento de Geologia, LAGEMAR, Universidade Federal Fluminense, Brazil. E-mail:
VIIIDepartamento de Geologia, LAGEMAR, Universidade Federal Fluminense, Brazil. E-mail:




This paper presents geophysical and geochemical evidence for the possible existence of cold, subducted lithosphere beneath the Saint Paul Fracture Zone of the Equatorial Atlantic Ocean. The ocean floor along the fracture zone is characterized by a high percentage of abyssal peridotites. The abyssal peridotites were emplaced by tectonic uplift of the oceanic lithosphere. The top of the ridge is exposed at Saint Peter and Saint Paul islets. The Os isotopic composition of these abyssal peridotites indicate the presence of old depleted mantle material in this region with Re-depletion model ages (TRD) from 0.32 to 1.1Ga. Melt inclusions in plagioclase phenocrysts of the MORB close to this location have boninitic composition, suggesting that some basalts originated from low-degree mantle melting. The global tomography models show fast seismic velocities in the upper and lower mantle of the Equatorial Atlantic Ocean, consistent with the presence of cold subducted lithosphere. The range of Re-depletion model ages are consistent with paleo-reconstructions of plate motion, suggesting that the fossil subducted slab was formed during the closure of both the Iapetus and the Rheic oceans.

Keywords: Equatorial Atlantic Ocean, Saint Paul Fracture Zone, abyssal mantle, Re-Os isotope system, cold mantle, fossil subducted slab.


O presente trabalho mostra evidências geofísicas e geoquímicas para a possível existência de fragmentos frios do manto originados da placa subductada abaixo da Zona de Fratura de São Paulo no Oceano Atlântico Equatorial. A planície abissal desta área é caracterizada por uma abundância de rochas peridotíticas, com presença de poucas rochas basálticas originadas de baixo grau de fusão parcial. Arquipélago de São Pedro e São Paulo se localiza no topo de uma elevação morfológica com mais de 4000m de altura, constituída por peridotitos abissais, posicionados por um soerguimento tectônico da litosfera oceânica. A razão isotópica de Os dos peridotitos da Zona de Fratura de São Paulo indica a presença de materiais originados de antigo manto depletado nesta região com as idades modelo de 0.32 a 1.1Ga. As inclusões de magma trapeadas nos fenocristais de plagioclásio nos basalto da cadeia meso-oceânica pouco mais ao sul apresentam composição boninítica, típicas de zona de arco. Os modelos da tomografia mundial do manto demonstram alta velocidade sísmica tanto no manto superior quanto no inferior do Oceano Atlântico Equatorial, o que corrobora a interpretação da presença de placa subductada de baixa temperatura. As idades do modelo de depleção de Re dos peridotitos são consistentes com a reconstituição de movimento das placas, sugerindo que os fragmentos de placa fóssil subductada são provenientes do fechamento tanto do Oceano Iapetus como o do Oceano Rheic.

Palavras-chave: Oceano Atlântico Equatorial, Zona de Fratura de São Paulo, manto abissal, sistema isotópico Re-Os, manto frio, placa fóssil subductada.




Lateral variations in the temperature of the Earth's mantle havesignificant influence on the morphological and structural characteristics of mid-oceanic ridges. Hotspots, such as Iceland and Azores, induce excess axial morphologic elevation, with high magma production and consequently thickened crust. On the other hand, transform fault zones represent morphological depressions, with low magma production, and thin oceanic crust (Schilling et al., 1995; Thibaud et al., 1998). In some localities, serpentinized mantle peridotite is exposed directly on the abyssal surface, forming elliptic hills called "megamullion" (Tucholke et al., 1998, 2001; Ohara et al., 2001). These areas, so-called "cold spots", or "cold zones", are less common and little understood in comparison with hotspots. The best-known case is the Australian-Antarctic Discordance, called AAD, which probably reflects the presence of the cold, subducted lithosphere in the mantle (Gurnis et al., 1998; Ritzwoller et al., 2003), also called "megalith" (Fukao et al., 1994; Maruyama, 1994). A second probable cold spot lies in the equatorial region of the Atlantic Ocean.

The primary evidence for the presence of cold upper mantle beneath the Equatorial Mid-Atlantic Ridge comes from the structural analysis of the ridge axis morphology and the petrology of both basaltic and peridotitic rocks dredged from the area (Fig. 1; Gorini, 1981; Bonatti & Honnorez, 1970; Bonatti, 1990; Bonatti et al., 1993; Schilling et al., 1995). Deep axial domains are usually associated with colder mantle temperature, generally along the length of the transform fault. For example, the Australian-Antarctic Discordance is characterized by a depth anomaly of about 800 meters (Christie et al., 1998). In the Equatorial Atlantic Ocean, the deepest point is located at southern part of the Saint Paul transform fault fracture zone (Schilling et al., 1995), with depth anomaly of about 700 m. The basalt samples from the Equatorial Mid-Atlantic Ridge have different compositions from other parts of the mid-oceanic ridge system, and show a notable enrichment of incompatible elements. This phenomenon is attributed to melt enrichment derived from low degree of partial melts from a deeper but relatively colder upper mantle. Schilling et al. (1995) estimated that the temperature of this region may be 100 to 150ºC lower than other areas of normal Mid-Atlantic Ridge.



The geometry of the ridge axis at the Equatorial Mid-Atlantic Ridge is marked by one of the largest offsets of the whole Atlantic Ocean (Fig. 1). Cold barrier effects of the exceptionally long transform faults (Fox & Gallo, 1984) could be partially responsible for the low mantle temperature and consequent low melting rates. However, this factor is not enough to explain the entire reduction in temperature observed (Bonatti et al., 1993; Schilling et al., 1995). Moreover, numerical modelling suggests that the cold barrier effect is localized, extending only a few kilometres away from the ridge-transform intersection (Schilling et al., 1995).

Two models for the formation of the cold upper mantle have been suggested. Bonatti (1990) proposed the possible existence of downwelling of mantle flow in a broad area of the Equatorial Atlantic region. The cold mantle mass could have originated from sub-continental lithospheric blocks entrained in the upper mantle during the continental rifting of West-Gondwana and subsequent formation of the Atlantic Ocean. In an alternative model, Schilling et al. (1995) attributed the cold mantle to an accumulation of subducted oceanic lithosphere at the margin of the Iapetus and Rheic Oceans from the time of Pangea formation.

In order to constrain further the origin of the cold mantle of Equatorial Atlantic zone, this study combines geochemical and geophysical data of the area around Saint Paul transform faultfracture zone.



A suite of samples was collected from a large area around theSaint Paul Fracture Zone during a deep sea diving survey using the scientific submersible Nautile (Hekinian et al., 2000). Ten abyssal peridotitic rocks and one of basaltic dyke sample were selected for the analyses of major elements, trace elements (Table 1), including Re, Pt, and Os contents, and Os isotopic ratios (Table 2). The chemical analyses were performed at CNRS-Université de Bretagne Occidentale, France, following the protocol described in Cotten et al. (1995).





Samples for this study were collected in 7 of the 13 dives along the intra-transform ridges (Fig. 2), and from the North and the South Ridges of the Saint Peter Saint Paul massif. This massif is about 90 km long and 21 km wide at the 3000 m depth contour line, composed of two E-W trending ridges, called, respectively, North Ridge and South Ridge, forming an "S" shaped morphologic high (Hekinian et al., 2000). The highest point is on the North Ridge, exposing its top above the sea level as small islands. They are called officially by the Brazilian Government "Arquipélago de São Pedro e São Paulo".



Some parts of Saint Peter Saint Paul North Ridge crop out above sea level forming 5 islets (Fig.3). This is the only locality in which serpentinized mantle peridotite of megamullion(Motoki et al., 2008). Because of the alteration problem, the samples were selected based on freshness. They were analysed with high priority because they have highest contents of Os and are best situated to present the mantle-derived residual material than may yield geochemical information regarding the underlyingmantle evolution. Os is highly compatible in mantle assemblages and has a notable contrast with Re partitions into the melt. Episodes of mantle melting therefore, slow or stop the ingrowths of radiogenic 187Os over time, and allow the Re-Os isotope system to be used to constrain the depletion history of the mantle (Shirey & Walker, 1998).



Determination of reliable geochemical information of the abyssal peridotite is not easy because of seawater alteration and serpentinization, hydrothermal fluid interaction at high and low temperatures, and potential contamination by ocean floor sediment. The major element composition indicates high loss-on-ignition (Table 1), as expected from the intensity of serpentinization. Snow & Dick (1995) showed that some major elements, such as Mg, can be removed during alteration on the seafloor. Mével (2003) stated that the serpentinization has little effect on most elements except for CaO, and that the MgO loss would take place only in low temperature weathering conditions of lessthan 100ºC.

Figure 4 shows Re, Os, and Pt variations with MgO contents. The Re and Os abundances have almost no correlation to MgO, although Re addition during the serpentinization or hydrothermal alteration is possible. It is unlikely that these processes would add Os to the mantle peridotite. Likewise, the Pt contents appear to have no correlation with MgO, indicating that Pt is also little influenced by seafloor alteration. The peridotite samples have high MgO concentrations that are not clearly correlated with CaO, which is a highly mobile element during alteration. These observations indicate that the major element composition of these peridotite samples was not significantly affected by serpentinization or hydrothermal alteration even at low temperature. Therefore, the major and trace element variations may reflect directly thechemical characteristics of the oceanic mantle. For instance, the samples of Saint Paul Fracture Zone have lower Al2O3 and CaO contents than the peridotitic rocks of the Kane Fracture Zone. These differences in major element composition are possibly a reflection of oceanic mantle chemical heterogeneities between above-mentioned areas.



It is noteworthy that sample SP 06-01 has low SiO2 and MgO, but high Al2O3 and FeO. This sample was extracted from a dyke and possibly represents a vein formed by the interaction of melts or fluids derived from peridotite in the oceanic lithosphere. This interpretation is consistent with high Ti, V and Sc contents, low Cr and Ni, and less radiogenic Os isotopic ratio of this sample (Tables 1-2). Therefore, this sample is excluded from the diagrams for peridotite samples.

An inverse correlation between Os and Al2O3 contents is generally observed in residual phases of melting events. Figure 5 shows variations of Re, Os, Pt contents, and of 187Re/188Os and 187Os/188Os with Al2O3 (wt%). The absence of clear correlation between the platinum group elements and a melt-depletion proxy, such as AlO, indicates that the peridotite samples are not the result of a single melt-depletion event. The highest Os concentrations of the Saint Paul peridotites are projected on the range of the abyssal peridotites of the Kane Fracture Zone (Brandon et al., 2000). These values are reasonable for a depleted mantle source.



Many samples of the Saint Paul Fracture Zone have lower Re and Os but similar Pt contents than those of the Kane Fracture Zone. One sample with a radiogenic Os isotopic ratio has high Pt, low Os, and low Re contents (Fig. 6). The lower Os and Re contents of the Saint Paul Fracture Zone relative to the Kane Fracture Zone indicate distinct chemical characteristics of the oceanic mantle lithosphere between these fracture zones. The Os isotopic variation of the Saint Paul Fracture Zone samples can be explained by the contamination of approximately 40 to 50% of sediments or infiltration of 30 to 40% of amphibolite veins (Fig. 6B). However,neither of these two models is consistent with the observed low Re contents of the peridotite samples, because sediments and amphibolite are typically enriched in Re relative to mantle assemblages (Fig. 6C).



The same argument is valid for contamination of the peridotites by MORBs, as most basaltic melts also have high Re contents. In addition to the depletion in Os and Re contents, the end-member with radiogenic Os isotopic composition has high Pt contents. The process that led to the depletion in Re and Os appears to be also capable of concentrating Pt. The radiogenic nature of this end member is a good indication that this mantle component is ancient. A study of mantle xenoliths from arc settings has shown that the oxidizing conditions of the mantle wedge above the subduction zones favors the removal of Re and Os from mantle assemblages (Brandon et al., 1996). Although it is not known how Pt would behave in similar conditions, it is possible that these chemical characteristics are inherited from an old subduction event.

The range of Os isotopic compositions obtained for this suite of rocks is large (187Os/188Os varies from 0.11988 to 0.14804) butthe majority of the samples has gOs values that are equal to or below chondritic values. These data cannot be explained simply by melt extraction from a fertile MORB mantle with homogeneous Os isotopic composition, and reinforce previous results by others indicating a sub-chondritic average for abyssal peridotites (Martin, 1991; Roy-Barman & Allègre, 1994; Snow & Reisberg, 1995). The sub-chondritic Os isotopic composition of most of these peridotites also cannot be explained by interaction of the mantle assemblage with abyssal sediments that are significantly more radiogenic than the MORB mantle (Roy-Barman et al., 1998) or primitive upper mantle. Two peridotite samples have significantly higher Os concentrations and more radiogenic Os isotopic ratios. These characteristics could be attributed to possible assimilation of sediments and interaction of enriched melts orfluids (Fig. 7).



The chondritic to sub-chondritic Os isotopic composition of most Saint Paul Fracture Zone peridotites contrasts with models of Os isotopic evolution of the primitive upper mantle as constrained by spinel lherzolites from continental environments that support a more chondritic value for the bulk upper mantle (Meisel et al., 1996, 2001). Model ages for Re-depletion for the sub-chondritic samples are in the range of 320 Ma to 1,100 Ma, being classified into three groups:

1) Middle Proterozoic, about 1,100 Ma (SP 04-01, SP 12-12);

2) Late Proterozoic, 870 Ma (SP 09-02, SP 06-01); and

3) Carboniferous, 330 Ma (SP 03-06, SP 08-02, SP 13-13).

These ages might record depletion events of the abyssal peridotiteand consequent old oceanic crust formation.

This range of depletion model ages for the sampled mantle rocks is consistent with three different hypotheses:

1) Os isotopic composition of the MORB mantle is more unradiogenic than previously thought;

2) Abyssal peridotites entrained pieces of old continental lithosphere delaminated during the opening of the Atlantic Ocean; and

3) Abyssal peridotites inherited unradiogenic Os from depleted portions of fossil subducted slab, or megaliths.

The first hypothesis is less consistent with available data on chromite obtained from ophiolite sequences that have crystallised during oceanic lithosphere formation (Walker, 1989), and the limited but robust set of Os isotopic compositions of primitive basaltic rocks from oceanic environments (Lassiter & Hauri, 1998). These data indicate that the MORB source, although somewhat heterogeneous, has probably a chondritic to slightly super-chondritic Os isotope ratio.

The second and third hypotheses can be supported by the Re-Os isotopic composition presented. The sub-continental lithosphere along the Atlantic Ocean margins in the equatorial region is much older than Pan-African (1.1-0.9 Ga). However, the age of melt depletion related to the formation of oceanic lithosphere, and its subsequent subduction during the closing of the Iapetus Sea in this region match better the Re-depletion model ages of the analysed peridotitic rocks.

The Os isotopic ratios of the Saint Paul Fracture Zone samples are not correlated with their 187Re/188Os ratio and can beattributed to possible late Re mobilisation (Fig.7). The data set shows a positive correlation between 187Os/188Os and Pt/Os (Fig.8). The same relationship was observed in the abyssal peridotites from Kane Fracture Zone (Brandon et al., 2000). In the Saint Paul Fracture Zone, Pt and Os concentrations also appear to be positively correlated, and the samples with higher Pt/Os ratios also have lower overall concentrations of these two platinumgroup elements.




The composition of parental liquids to mid-ocean ridge basaltic rocks is controlled by source characteristics such as pressure, temperature, bulk mantle composition, degree of partial melting, and the presence of volatile species. Mid-ocean ridge primary magmas are generally basaltic and the freshest samples can be obtained from volcanic glass in abyssal pillow lavas that have cooled rapidly to prevent extensive fractionation, and are the best chemical proxies for their original source composition. The melt inclusions trapped within plagioclase phenocrysts in this glass can provide important information about their parental melt because they were isolated from later processes, such as magma mixing and crystallisation fractionation. However, their composition could be modified by post-entrapment recrystallisation of the host crystal, such as mineral growth. In order to evaluate the extent of host mineral crystallisation, it is important to note the relationship between the composition of the inclusion and the host mineral, zoning, or internal heterogeneity, which would provide a strong argument for the host mineral recrystallisation. Once host recrystallisation has been evaluated, the melt inclusion composition can be adjusted back to its original entrapment composition.

Sichel (1990) presented the analyses of the melt inclusions in plagioclase phenocrysts and their host minerals, obtained from dredged samples of Mid-Atlantic Ridge (EN61-2D; latitude 2º24'S). A group of plagioclase crystals appears to be in equilibrium with the MORB matrix glass. However, the range in anorthite content for the plagioclase phenocrysts that contain melt inclusions goes up to An90, which can be interpreted as representing a more primitive melt composition than the matrix glass.The Mg# (Mg/Mg+Fe) of these primitive melt inclusions are 69-70. Table 3 shows major and trace element compositions of the matrix glass and representative melt inclusions.



The high MgO, high SiO2 and enriched LREE of the melt inclusions are consistent with a boninitic composition. Boninite is a primary high-magnesia andesitic magma generated from the partial melting of young and hot oceanic crust in the presence of H2O, generally in subduction zones (Crawford et al., 1989; Tatsumi & Maruyama, 1989). Such melting conditions are present only in certain localities of arcs in which ridge subduction takes place. The presence of melt inclusions of boninitic composition in plagioclase phenocrysts in volcanic glasses from the Mid-Atlantic Ridge is consistent with melt contribution to MORBs from magmas generated from melting of slab material at depth.



The topographic and mantle Bouguer anomaly (Fig. 9) sections across the Mid-Atlantic Ridge show a topographic low and a high Bouguer anomaly in the Equatorial Atlantic area in comparison with the other regions.



The attenuation Q model for seismic waves (Romanowicz & Gung, 2002; Gung & Romanowicz, 2004) demonstrates high Q values around the Mid-Atlantic Ridge of this region, implyingcooler than normal mantle temperatures (Fig.10). This surface anomaly corresponds to a high-Q body located in the lower part of the upper mantle. Global whole mantle tomographic models (Boschi & Dziewonski, 1999; Ritsema & Van Heijst, 2000; Becker & Boschi, 2002) also show significantly high seismic velocities beneath the Equatorial Mid-Atlantic Ridge (Fig. 11).





Although global tomographic models have generally low resolution at the surface (half-wavelength of ~ 1000 km), both the S and P models show high velocities in the upper mantle near the equatorial area. A notable characteristic of these whole-mantle seismological models is that the high velocity zone observed for the upper mantle apparently continues into the lower mantle.A similar phenomenon is observed in the present day subduction zones. This geophysical evidence is consistent with the presence of fossil subducted slab fragments in the mantle.

High seismic velocities of the mantle in areas in which subduction is no longer active are attributed to the presence of old slab fragments (Steinberger, 2000). The cold slab pieces can contribute to maintain the low temperature in upper mantle long after the end of subduction. This low mantle temperature could decrease the magma production at the ridge axis, resulting in thinner crust and thicker lithosphere. The cold upper mantle would result in a highly segmented ridge axis system at greater depth, as is observed in the Australian-Antarctic Discordance.



The existence of plate fragments in the Equatorial Atlantic region may be related to the numerous episodes of subduction that occurred during the assembly of Pangea (Blakey, 2004; Scotese, 2004) that spanned more than 200 million years. Several convergent margins were active in this region since the Late Cambrian. The equatorial area may have corresponded to a region of subduction during two collision events of Gondwana and Laurentia: 1) prior to the closing of the Iapetus Ocean (Fig.12A) in the Ordovician, about 460 Ma; and 2) prior to closing of the Rheic Ocean (Fig. 12B), in the Carboniferous and Permian, about 300 Ma (Dalziel, 1997). The Carboniferous Re-Os model ages of about 330Ma fit well the Rheic Ocean closure event. The present positions of these subduction zones relative to the South American continental block are far from the present Equatorial Atlantic Ocean. If their positions are referenced relative to the fixed locations of hotspots, however, they are located in the present Equatorial Atlantic region. Therefore, convergent margins could have accumulated fossil slabs in the upper mantle below the present position of the Equatorial Atlantic Ocean.



Schilling et al. (1995) previously suggested that closing of the western block of Pangea prior to 300 Ma was a possible origin for fragmentary blocks of oceanic lithosphere trapped in the upper mantle, which were remobilized upward during the subsequent rifting of Pangea and opening of the Atlantic Ocean (Fig.13). An additional factor that could have contributed fragments of subducted lithosphere to the upper mantle is the shear movement that may have been active between Early and Late Permian along this margin of Pangea (Muttoni et al., 2003).



A similar process was proposed for the Australian-Antarctic Discordance cold spot that, like the Equatorial Atlantic, has thin crust and a topographic low (Gurnis et al., 1998). The seismic tomography similarly revealed a high velocity anomaly in the mantle, interpreted as low mantle temperatures of this area that resulted from fragments of an ancient slab (Ritzwoller et al., 2003).This slab is probably linked to a convergent margin that was active until about 100 million years ago. Although the Australian-Antarctic Discordance presents much stronger anomalies than the Equatorial Atlantic, we suggest that similar processes may have occurred in both areas.



The Os isotopic ratios recorded in the abyssal peridotites, the degree of depletion of basalts and peridotites, the ridge axial morphology, and the high seismic mantle velocities support the existence of anomalous cold mantle material beneath the Equatorial Atlantic region. The Re depletion model ages and palaeo-reconstructions of the area both point to an event in thePalaeozoic, probably the closing of the Iapetus Sea. Entrainment of subducted depleted mantle materials during the formation of the Atlantic oceanic lithosphere could have imparted the non-radiogenic Os signature to the abyssal peridotites in this region.

Further evidence of subducted components beneath the Equatorial Atlantic region comes from the trace element and isotopic composition of tholeiitic basalts from intra-transform ridges within the St. Paul Fracture Zone. These samples show elevated Ce/Pb ratios, and 87Sr/86Sr isotopic ratios that plot towards the HIMU component of the oceanic array (Hemond et al., 2002), geochemical characteristics that are commonly interpreted to be inherited from ancient recycled oceanic crust.

The intense stretching of the lithosphere during the rifting and opening of the Equatorial Atlantic region might have induced delamination of the old continental lithosphere. The presence of cold continentally derived lithospheric fragments in the upper mantle could effectively reduce the average mantle temperature, thus yielding low melting rates and high seismic velocities at higher levels in the mantle. However, the high seismic velocities observed into the lower mantle in this region are more easily explained by the presence of a subducted slab than by delamination and downwelling of large blocks of subcontinental lithosphere.

It is speculated that the subduction at the margin of the Rheic Ocean until 300 million years ago provided the fossil slab mass around the present day position of the Equatorial Atlantic region relative to hotspots. Such cold slab material can be seen in a high velocity zone in the lower mantle on the tomographic image. Although the subducted lithosphere could have been created in a divergent period prior to 460 million years ago, the younger age estimates seem to be more consistent with the depletion model ages obtained with the Re-Os system.



Combined geochemistry on abyssal peridotites from the Saint Paul Fracture Zone, recent whole mantle tomographic models, and kinematic palaeo-reconstructions indicate that low mantle temperatures in the Equatorial Atlantic Ocean result from fragments of a subducted slab in the upper mantle. The presence of Mg-SiO2 rich melt inclusions with LREE enrichment in MORB samples is consistent with the suggestion that the underlying oceanic mantle in the Equatorial Atlantic has chemical heterogeneities that are characteristic of those in arc settings. The colder lower mantle temperatures seen in global tomography models may have been induced by the detached cold slab fragments. These could also have the effect of cooling the upper mantle while maintaining a downwelling flow even without active present day subduction. Fragments of the subducted plate that were detached during earlier subduction could have melted or been entrained in the upper mantle, yielding the osmium isotopic compositions observed in the abyssal peridotites.



The senior author is grateful to Roger Hekinian and Thierry Juteau for their mentorship and support during the cruise and to IFREMER for their support of the St. Paul Cruise of N/O Nadir and the Nautile. She also thanks Marcus Aguiar Gorini who offered her the unique opportunity for participating in the dives on the NAUTILE submersible in the St. Paul Transform Fault Zone. Richard Walker generously provided access to the Isotopic Geochemistry Laboratory of University of Maryland-College Park where the isotopic analyses were performed. This project received financial support of CAPES/COFECUB, program of the Brazilian Government (project 220/97 and 415/03); PETROBRAS/CENPES, Brazilian Petroleum Company (Project: Origem e Evolução das Rochas Mantélicas do Arquipélago de São Pedro e São Paulo); IUEM - Université de Bretagne Occidentale, France; CNRS-INSU, France. The field trip to the island and chemical analyses were supported by the project Nos.480023/2004-2 and 557309/2005-0 of the Brazilian Government, SECIRM/CNPq.



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Recebido em 14 setembro, 2007 / Aceito em 24 janeiro, 2008
Received on September 14, 2007 / Accepted on January 24, 2008




Susanna Eleonora Sichel. B.Sc. in Geology at Universidade Federal do Rio de Janeiro (UFRJ), Brazil, with an additional specialization at the University of Clausthal-Zellerfeld, Germany. M.Sc. in Geology at UFRJ and Ph.D. in Oceanography at the Graduate School of Oceanography of the University of Rhode Island, USA. Currently Professor in the Department of Geology of Universidade Federal Fluminense (LAGEMAR/UFF).

Sonia Esperança. B.A. in Geology at Rice University, M.Sc. in Earth Sciences at the Hebrew University of Jerusalem, and Ph.D. in Geology at Arizona State University. Held a number of faculty and staff appointments at Monash and Deakin Universities in Australia, and Old Dominion University and the University of Maryland-College Park in the United States. Currently manages the Petrology and Geochemistry program in the Division of Earth Sciences at the National Science Foundation, USA.

Akihisa Motoki. B.Sc. and M.Sc. in Geology at the Faculty of Science, Kobe University, Japan. Ph.D. in Geology at the Instituto de Geociências, Universidade de São Paulo, Brazil. Since 1983, has been Professor in the Department of Mineralogy and Petrology at the Universidade do Estado do Rio de Janeiro.

Marcia Maia. B.Sc. in Oceanography at the Universidade do Estado do Rio de Janeiro, Doctorate in Sciences in Geophysics at the Université de Paris XI, Orsay, and the Habilitation à Diriger des Recherches from the Université de Bretagne Occidentale. Currently, is research faculty in the CNRS - Institut Universitaire Européen de la Mer, Université de Bretagne Occidentale, Plouzané, France.

Mary F. Horan. B.A. in Geology at Rice University, Houston, Texas, USA and M.Sc. in Geochemistry at the State University of New York at Stony Brook. Employed as the Geochemistry Laboratory Manager in the Department of Terrestrial Magnetism of the Carnegie Institution of Washington, Washington DC, USA.

Peter Szatmari. M.Sc. (Diplomarbeit) in Geology at the Eotvos University in Budapest, Hungary, and Ph.D. at the Grant Institute of Geology at the University of Edinburgh, U.K. Worked in the U.S. at the International Salt company, Princeton University and as an independent consultant. Worked as consultant and geologist for Petrobras since 1973.

Eliane da Costa Alves. B.Sc. in Geology at Universidade Federal do Rio de Janeiro, M.Sc. at Universidade Federal do Rio Grande do Sul, and Ph.D. in Geology and Geophysics at Universidade Federal do Rio de Janeiro. Currently Professor in the Department of Geology/LAGEMAR of the Instituto de Geociências, Universidade Federal Fluminense.

Sidney Luiz Matos Mello. Graduated in Geology at Universidade Federal do Rio de Janeiro, Brazil. M.Sc. in Geology at Universidade Federal do Rio de Janeiro. Ph.D. in Marine Geology and Geophysics at the School of Earth Sciences of the University of Leeds, UK. Working as Professor in the Department of Geology, Universidade Federal Fluminense, Brazil.

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