The Size of Plume Heterogeneities Constrained by Marquesas Isotopic Stripes Catherine Chauvel, René C

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The Size of Plume Heterogeneities Constrained by Marquesas Isotopic Stripes Catherine Chauvel, René C The size of plume heterogeneities constrained by Marquesas isotopic stripes Catherine Chauvel, René C. Maury, Sylvain Blais, Eric Lewin, Hervé Guillou, Gérard Guille, Philippe Rossi, Marc-André Gutscher To cite this version: Catherine Chauvel, René C. Maury, Sylvain Blais, Eric Lewin, Hervé Guillou, et al.. The size of plume heterogeneities constrained by Marquesas isotopic stripes. Geochemistry, Geophysics, Geosys- tems, AGU and the Geochemical Society, 2012, 13 (1), pp.Q07005. 10.1029/2012GC004123. insu- 00720199 HAL Id: insu-00720199 https://hal-insu.archives-ouvertes.fr/insu-00720199 Submitted on 24 Jan 2013 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Article Volume 13, Number 1 12 July 2012 Q07005, doi:10.1029/2012GC004123 ISSN: 1525-2027 The size of plume heterogeneities constrained by Marquesas isotopic stripes Catherine Chauvel ISTerre, UMR 5275, CNRS, Université Grenoble 1, BP 53, FR-38041 Grenoble CEDEX 09, France ([email protected]) René C. Maury Domaines Océaniques, UMR 6538, Université de Brest, Université Européenne de Bretagne, CNRS, Institut Universitaire Européen de la Mer, Place N. Copernic, FR-29280 Plouzané, France Sylvain Blais Géosciences Rennes, UMR 6518, Université de Rennes 1, Université Européenne de Bretagne, CNRS, Campus de Beaulieu, Avenue du Général Leclerc, FR-35042 Rennes CEDEX, France Eric Lewin ISTerre, UMR 5275, CNRS, Université Grenoble 1, BP 53, FR-38041 Grenoble CEDEX 09, France Hervé Guillou UMR 8212, LSCE-IPSL/CEA-CNRS-UVSQ, Domaine du CNRS, 12 avenue de la Terrasse, FR-91198 Gif-sur-Yvette, France Gérard Guille Laboratoire de Géophysique, CEA-DASE, FR-91680 Bruyères-le-Chatel, France Philippe Rossi BRGM, SGN-CGF, 3 avenue Claude-Guillemin, BP 36009, FR-45060 Orléans CEDEX 2, France Marc-André Gutscher Domaines Océaniques, UMR 6538, Université de Brest, Université Européenne de Bretagne, CNRS, Institut Universitaire Européen de la Mer, Place N. Copernic, FR-29280 Plouzané, France [1] The scale and geometry of chemical and isotopic heterogeneities in the source of plumes have important scientific implications on the nature, composition and origin of plumes and on the dynamics of mantle mixing over time. Here, we address these issues through the study of Marquesas Islands, one of the Archipela- goes in Polynesia. We present new Sr, Nd, Pb, Hf isotopes as well as trace element data on lavas from several Marquesas Islands and demonstrate that this archipelago consists of two adjacent and distinct rows of islands with significantly different isotopic compositions. For the entire 5.5 Ma construction period, the northern islands, hereafter called the Ua Huka group, has had systematically higher 87Sr/86Sr and lower 206Pb/204Pb ratios than the southern Fatu Hiva group at any given 143Nd/144Nd value. The shape and curvature of mixing arrays preclude the ambient depleted MORB mantle as one of the mixing end-members. We believe therefore that the entire isotopic heterogeneity originates in the plume itself. We suggest that the two Marquesas isotopic stripes originate from partial melting of two adjacent fila- ments contained in small plumes or “plumelets” that came from a large dome structure located deep in ©2012. American Geophysical Union. All Rights Reserved. 1 of 23 Geochemistry Geophysics 3 CHAUVEL ET AL.: MARQUESAS ISOTOPIC STRIPES 10.1029/2012GC004123 Geosystems G the mantle under Polynesia. Low-degree partial melting under Marquesas and other “weak” Polynesian hot spot chains (Pitcairn-Gambier, Austral-Cook, Society) sample small areas of the dome and preserve source heterogeneities. In contrast, more productive hot spots build up large islands such as Big Island in Hawaii or Réunion Island, and the higher degrees of melting blur the isotopic variability of the plume source. Components: 14,000 words, 12 figures, 3 tables. Keywords: Marquesas; isotopes; ocean island; plume structure. Index Terms: 1025 Geochemistry: Composition of the mantle; 1030 Geochemistry: Geochemical cycles (0330); 1040 Geochemistry: Radiogenic isotope geochemistry. Received 23 February 2012; Revised 24 May 2012; Accepted 7 June 2012; Published 12 July 2012. Chauvel, C., R. C. Maury, S. Blais, E. Lewin, H. Guillou, G. Guille, P. Rossi, and M.-A. Gutscher (2012), The size of plume heterogeneities constrained by Marquesas isotopic stripes, Geochem. Geophys. Geosyst., 13, Q07005, doi:10.1029/ 2012GC004123. 1. Introduction limited set of samples collected during reconnais- sance sampling in the early 1970s by R.A. Duncan, R. Brousse, H. Craig and H.G. Barsczus, and during a [2] The considerable isotopic heterogeneity in plume-related basalts is attributed to processes such single dredging cruise on Marquesas seamounts as (i) chemical heterogeneity of mantle plumes at [Desonie et al., 1993]. All these studies focused on depth [Kerr et al., 1995], (ii) entrainment of sur- the origin of the isotopic diversity and they did not rounding asthenospheric mantle materials [Hart use recently developed high-precision isotopic anal- et al., 1992] or (iii) plume-lithosphere interac- yses to investigate potential relationships with a tions [Saunders et al., 1992]. There is ongoing plume track or changes in source compositions as a debate about the relative importance of the three function of time or distance to the presumed location processes in the genesis of basaltic magmas from of the active plume. Iceland [Chauvel and Hémond, 2000; Fitton et al., [4] The Marquesas archipelago has also been the 2003; Thirlwall et al., 2004; Kokfelt et al., 2006], object of great interest for geophysical studies, the Galapagos [White et al., 1993; Hoernle et al., 2000; particularly since McNutt and coworkers [McNutt, Blichert-Toft and White, 2001; Saal et al., 2007], 1998; McNutt and Bonneville, 2000] discovered Afar [Furman et al., 2006; Beccaluva et al., 2009; that French Polynesia was built on top of a large Daoud et al., 2010] and Hawaii [Yang et al., 2003; topographic height attributed to the so-called Frey et al., 2005; Fekiacova et al., 2007]. In par- Polynesian Superswell. Its existence is usually ticular, differences in lead isotopes between the Kea thought to be linked to the presence of a large and Loa trends in Hawaii have been attributed to a region of hot material rising from deep in the bilateral asymmetry of the plume [Abouchami et al., mantle [Davaille, 1999; Romanowicz and Gung, 2005; Farnetani and Hofmann, 2009, 2010]. 2002; Courtillot et al., 2003; Montelli et al., 2006] but the way these observations relate to [3] Large isotopic variations in Marquesas basalts have been known for decades [Vidal et al., 1984; geochemical constraints remains unsolved. Duncan et al., 1986; Dupuy et al., 1987; Vidal et al., [5] Here we reexamine the scale of isotopic varia- 1987; Woodhead, 1992; Desonie et al., 1993; Caroff tions using high-precision Sr, Nd, Hf and Pb iso- et al., 1995; Le Dez et al., 1996; Castillo et al., topic measurements obtained on a large set of new 2007] and have been attributed to (i) a concentri- samples that were collected and dated during the cally zoned structure of the Marquesas plume first detailed geological mapping of Marquesas [Duncan et al., 1986], (ii) small-scale hetero- Islands. We demonstrate the existence of isotopic geneities within the plume [Dupuy et al., 1987; stripes different from those suggested recently by Vidal et al., 1987; Le Dez et al., 1996] or (iii) plume- Huang et al. [2011] and we propose that they lithosphere interactions [Duncan et al., 1986; originate from small-scale heterogeneities located Woodhead, 1992; Desonie et al., 1993; Caroff et al., within elongated filaments in rising plumelets 1995]. These models were primarily based on a 2of23 Geochemistry Geophysics 3 CHAUVEL ET AL.: MARQUESAS ISOTOPIC STRIPES 10.1029/2012GC004123 Geosystems G Figure 1. Location map of Marquesas Islands. The bathymetry comes from the global altimetry data set of Smith and Sandwell [1997]. Shades of purple denote depths of 5,000 to 4,000 m; shades of blue, depths of 4,000 to 2,000 m and shades of orange, depths less than 2,000 m. The main trend of the Marquesas chain is N40W. Current Pacific plate motion is 10.5 cm/yr at N65W, corresponding to the line shown in white and labeled plate movement. This line is also the line separating the two groups of islands as shown in Figures 4 and 5. In Hiva Oa, the line is located on the south- western side of the island in the Taaoa Bay (see Figure S1 for more details). MFZ: Marquesas Fracture Zone. coming from a large dome structure. Further com- anomalously shallow given its age [Crough and parison with other ocean islands suggests that weak Jarrard, 1981] and the so-called “Marquesas plume-derived islands such as Polynesia are ideal swell” has been interpreted as resulting from uplift sites to determine the scale of plume hetero- due to a rising mantle plume [Crough and Jarrard, geneities while strong plume-derived islands such 1981]. However, the crustal thickness reaches 15– as Hawaii are the best choices to establish the 20 km below the central part of the Archipelago average composition of plumes. [Filmer et al., 1993; Caress et al., 1995], and the swell could also result from the buoyancy of such a thick basaltic crust [McNutt and Bonneville, 2000]. 2. Geological Setting of the Marquesas The origin of the crustal thickening was attributed Archipelago either to (i) Plio-Quaternary underplating of plume magmas just below the Moho [Caress et al., 1995; [6] The ca.
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