Primitive Lower Mantle in the Hawaiian Plume? Evidence from
Correlated Os-Pb-Sr-Nd Isotopes in Picrites
Marc Norman1, Vickie Bennett2 and Tezer Esat2
1GEMOC, School of Earth Sciences, Macquarie University, North Ryde NSW 2109 Australia.
2Research School of Earth Sciences, Australian National University,
Canberra ACT 0200 Australia
Abstract - PGE abundances and Os isotopic compositions
provide important constraints on processes of planetary differentiation,
including core formation, melt extraction, and crustal recycling.
We have determined Re and Os abundances and Os isotopic compositions
for a suite of picritic basalts from the Hawaiian plume to investigate
the nature and composition of the deep mantle of the Earth. These
data may provide a window through the late accretionary veneer
which established near-chondritic relative abundances of PGE in
the upper mantle, and constrain models for the origin and early
evolution of the Earth. Sr, Nd, and Pb isotopic compositions of
Hawaiian tholeiites indicate mixing of two mantle sources [1,
2]. One of these components is isotopically similar to depleted
mantle, and the other is similar to that predicted for the primitive
mantle. Os isotopic compositions are well correlated with the
other isotopic systems, with 187Os/186Os Å 1.09 in the depleted
component, and 187Os/186Os Å 1.21 in the "primitive"
component, requiring a long-term history with super-chondritic
Re/Os. Although crustal recycling can introduce high Re/Os components
into the mantle, the trends of the picrite data are better matched
by mixing of two mantle components. The upper mantle of the Earth
apparently has had near-chondritic Re/Os since at least 3.8 Ga,
suggesting long-term isolation of the upper and lower mantle.
Introduction - The Hawaiian plume is the largest, hottest,
longest-lived mantle plume currently active on the Earth [3,4].
Tomography indicates a source for the Hawaiian plume in the lower
mantle, below the 670 km transition zone [5]. Sr, Nd, Pb, and
noble gas isotopic compositions of Hawaiian basalts show that
at least two components with distinct long-term histories are
present within the plume [1,2,4,6] and fluid dynamics experiments
[7] suggest it is reasonable to consider these components as potentially
reflecting upper and lower mantle compositions. To investigate
the nature of these mantle components, a suite of picrites from
7 major volcanic centres (Koolau, Hualalai, Kohala, Mauna Kea,
Mauna Loa, Kilauea, and Loihi), representing 3 million years of
plume activity, were analyzed for major element, trace element,
and Sr-Nd-Pb-Os isotopic compositions. Picrites are ideal for
such a study as they are the best candidates for near-primary
magmas. Hawaiian picrites apparently erupt preferentially from
deeper in the volcanic plumbing than more typical subaerial tholeiites
[3, 8], and have largely escaped the complexities introduced by
the higher level magma chambers [9]. Picrites, therefore, should
provide a clearer picture of source variations within the Hawaiian
plume.
Results - The excellent correlations between the isotopic
and trace element compositions of the picrites are consistent
with mixing of two source components (Fig. 1). One component
in the Hawaiian plume has Sr, Nd, and Pb isotopic compositions
similar, but not identical to, those of Pacific MORB, and this
component is most reasonably interpreted as predominantly depleted
upper mantle [1,2] (Fig. 2). Depleted compositions are
best expressed at Kilauea and Loihi. The second component has
Sr, Nd, and Pb isotopic compositions close to those predicted
for the primitive mantle, and predominates at Koolau [1,2], Lanai
[10] and Kahoolawe [11] (Fig. 2).
Os isotopic compositions of the picrites are well-correlated with
those of Sr, Nd, and especially Pb (Fig. 3), with 187Os/186Os
ranging from 1.09 in lavas from Kilauea to 1.21 in samples from
Koolau. Although crustal recycling can produce elevated Os isotopic
compositions in the mantle, the Os-Pb picrite arrays are better
fit by mixtures of two mantle components with subequal Pb/Os (Fig.
3). 187Os/186Os values of Hawaiian picrites require a time-integrated
super-chondritic Re/Os for the "primitive" lower mantle
component of these picrites, at least 60% higher than chondritic
if the fractionation occurred 4.5 billion years ago. In contrast,
the compositions of abyssal peridotites and mantle xenoliths show
that the upper mantle has evolved with a near-chondritic Re/Os
(187Os/186Os = 1.06 today), consistent with the relative abundances
of other PGE in the upper mantle [12], and near-chondritic Re/Os
apparently has been a feature of the upper mantle of the Earth
since at least 3.8 Ga [13]. If the "primitive" component
of the Hawaiian plume does represent the lower mantle, the isotopic
compositions of Hawaiian basalts imply long-term isolation of
the upper and lower mantle.
[1] Stille et al. (1986) GCA 50, 2303-2319.
[2] Roden et al., (1994) GCA 58, 1431-1440.
[3] Garcia et al. (1995) AGU Geophys. Monograph: Mauna Loa, in press.
[4] Kurz (1993) Phil. Trans. R. Soc. Lond. A342, 91-103.
[5] Romanowicz (1994) EPSL 128, 113-121.
[6] Honda et al. (1991) Nature 349, 149-151.
[7] Griffiths and Campbell (1990) EPSL 99, 66-78.
[8] Ryan (1987) Geochem. Soc. Spec. Pub. 1, 259-287
[9] Clague (1995) J. Petrology 36, 299-349.
[10] West et al. (1992) CPM 112, 520-542.
[11] Leeman et al. (1994) CMP 116, 62-77
[12] Capobianco et al. (1993) JGR 98, 5433-5443.
[13] Bennett et al. (1995) Eos Spring AGU, and in prep.
Figures available from Marc Norman.
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