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CHEMGE-15681; No of Pages 18<br />

ARTICLE IN PRESS<br />

Chemical Geology xxx (2009) xxx–xxx<br />

Contents lists available at ScienceDirect<br />

Chemical Geology<br />

journal homepage: www.elsevier.com/locate/chemgeo<br />

Geochemical and p<strong>et</strong>rographic evidence for magmatic impregnation in the oceanic<br />

lithosphere at Atlantis Massif, Mid-Atlantic Ridge (IODP Hole U1309D, 30°N)<br />

Marion Drouin a,1 , Marguerite Godard a, ⁎, Benoit Ildefonse a , Olivier Bruguier a , Carlos J. Garrido b<br />

a Géosciences Montpellier, CNRS & Université Montpellier 2, F-34095 Montpellier cedex5, France<br />

b Instituto Andaluz de Ciencias de la Tierra (IACT), CSIC & UGR, Facultad de Ciencias, Fuentenueva sn. 18002 Granada, Spain<br />

article<br />

info<br />

abstract<br />

Article history:<br />

Received 9 June 2008<br />

Received in revised form 22 December 2008<br />

Accepted 24 February 2009<br />

Available online xxxx<br />

Editor: D.B. Dingwell<br />

Keywords:<br />

Troctolite<br />

<strong>LA</strong>-<strong>ICP</strong>-<strong>MS</strong><br />

Olivine<br />

Integrated Ocean Drilling Program<br />

Mid-ocean ridge<br />

Impregnated mantle<br />

IODP Hole U1309D (Atlantis Massif, Mid-Atlantic Ridge 30°N) is the second deepest hole drilled into slow<br />

spread gabbroic lithosphere. It comprises 5.4% of olivine-rich troctolites (~N70% olivine), possibly the most<br />

primitive gabbroic rocks ever drilled at mid-ocean ridges. We present the result of an in situ trace element<br />

study carried out on a series of olivine-rich troctolites, and neighbouring troctolites and gabbros, from<br />

olivine-rich intervals in Hole U1309D. Olivine-rich troctolites display poikilitic textures; coarse-grained<br />

subhedral to medium-grained rounded olivine crystals are included into large undeformed clinopyroxene<br />

and plagioclase poikiloblasts. In contrast, gabbros and troctolites have irregularly seriate textures, with highly<br />

variable grain sizes, and locally poikilitic clinopyroxene oikocrysts in troctolites. Clinopyroxene is high Mg#<br />

augite (Mg# 87 in olivine-rich troctolites to 82 in gabbros), and plagioclase has anorthite contents ranging<br />

from 77 in olivine-rich troctolites to 68 in gabbros. Olivine has high forsterite contents (82–88 in olivine-rich<br />

troctolites, to 78–83 in gabbros) and is in Mg–Fe equilibrium with clinopyroxene. Clinopyroxene cores and<br />

plagioclase are depl<strong>et</strong>ed in trace elements (e.g., Yb cpx ~5–11×Chondrite), they are in equilibrium with the<br />

same MORB-type melt in all studied rock-types. These compositions are not consistent with the progressively<br />

more trace element enriched (evolved) compositions expected from olivine rich primitive products to gabbros in<br />

a MORB cumulate sequence. They indicate that clinopyroxene and plagioclase crystallized concurrently, after<br />

melts having the same trace element composition, consistent with crystallization in an open system with a<br />

buffered magma composition. The slight trace element enrichments and lower Cr contents observed in<br />

clinopyroxene rims and interstitial grains results from crystallization of late-stage differentiated melts, probably<br />

indicating the closure of the magmatic system. In contrast to clinopyroxene and plagioclase, olivine is not in<br />

equilibrium with MORB, but with a highly fractionated depl<strong>et</strong>ed melt, similar to that in equilibrium with<br />

refractory oceanic peridotites, thus possibly indicating a mantle origin. In addition, textural relationships suggest<br />

that olivine was in <strong>par</strong>t assimilated by the basaltic melts after which clinopyroxene and plagioclase crystallized<br />

(impregnation). These observations suggest a complex crystallization history in an open system involving<br />

impregnation by MORB-type melt(s) of an olivine-rich rock or mush. The documented magmatic processes<br />

suggest that olivine-rich troctolites were formed in a zone with large magmatic transfer and accumulation, similar<br />

to the mantle-crust transition zone documented in ophiolites and at fast spreading ridges.<br />

© 2009 Elsevier B.V. All rights reserved.<br />

1. Introduction<br />

Slow spreading ridges (full-spreading rate b50 mm/yr), such as the<br />

Mid Atlantic Ridge (MAR), represent about half of Earth's mid-ocean<br />

ridges. In contrast to the layered fast-spread crust (Penrose Conference<br />

<strong>par</strong>ticipants, 1972; Ildefonse <strong>et</strong> al., 2007b), slow-spread crust is highly<br />

h<strong>et</strong>erogeneous with, at least in some places, discr<strong>et</strong>e gabbroic bodies<br />

intruded into serpentinized peridotites (e.g., Lagabrielle and Cannat,<br />

⁎ Corresponding author.<br />

E-mail address: Marguerite.Godard@gm.univ-montp2.fr (M. Godard).<br />

1 Present address: Laboratoire Géosciences Reunion, Institut de Physique du Globe de<br />

Paris, Université de la Réunion, UMR 7154, CNRS, 15 avenue René Cassin, BP 7151, F-97715<br />

Saint Denis messag CEDEX 9, La Réunion, France.<br />

1990; Cannat, 1993, 1996; Canales <strong>et</strong> al., 2000; Carlson, 2001). Ocean<br />

Drilling has provided deep access to gabbroic rocks emplaced at depth<br />

in this type of h<strong>et</strong>erogeneous lithosphere in various oceanic core<br />

complexes (Ildefonse <strong>et</strong> al., 2007a).<br />

During IODP Expeditions 304 and 305 (Blackman <strong>et</strong> al., 2006;<br />

Ildefonse <strong>et</strong> al., 2006), a 1415.5 m deep hole was drilled at 30°N near<br />

the Mid-Atlantic Ridge (Fig.1). IODP Hole U1309D is the second deepest<br />

hole in slow-spread lithosphere, after ODP Hole 735B on the Southwest<br />

Indian Ridge (Dick <strong>et</strong> al., 2000). Hole U1309D is almost exclusively made<br />

of gabbroic rocks (Blackman <strong>et</strong> al., 2006). Com<strong>par</strong>ed to ODP Hole 735B<br />

and other drilled gabbroic series, IODP Hole U1309D gabbroic rocks<br />

comprise a relatively large proportion of olivine-rich lithologies. The<br />

most olivine rich ones (~N70%) were grouped as olivine-rich troctolites,<br />

and represent 5.4% of the rocks recovered at Hole U1309D (Blackman<br />

0009-2541/$ – see front matter © 2009 Elsevier B.V. All rights reserved.<br />

doi:10.1016/j.chemgeo.2009.02.013<br />

Please cite this article as: Drouin, M., <strong>et</strong> al., Geochemical and p<strong>et</strong>rographic evidence for magmatic impregnation in the oceanic lithosphere at<br />

Atlantis Massif, Mid-Atlantic Ridge (IODP Hole U1309D, 30°N), Chemical Geology (2009), doi:10.1016/j.chemgeo.2009.02.013

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