Upload
trinhtram
View
221
Download
1
Embed Size (px)
Citation preview
Constraining the nature of E- and N-type components in the Baffin Island
picrites using olivine-hosted melt inclusions
Melissa Maisonneuve
Department of Earth & Planetary Sciences
McGill University
Montréal, Québec, Canada
December 2012
A thesis submitted to McGill University in partial fulfillment of the requirements
of the degree of Master of Science
© Melissa Maisonneuve 2012
ii
Abstract
The Baffin Island picrites are interpreted to represent primitive magmas
(up to ~22 wt % MgO) that are minimally changed since leaving their mantle
source and thus provide important insights into our understanding of high-MgO
primary magmas and the heterogeneity of their mantle sources. In this study of
olivine-hosted melt inclusions, the ratio of potassium to titanium (K/Ti) is used as
a probe for the mantle source as both these elements are incompatible in olivine
and plagioclase, K/Ti behaves in a similar manner to La/Sm and remains
unaffected by crystal fractionation. We define depleted glass compositions (N-
type) as those with K/Ti < 0.2 and enriched glass compositions (E-type) as those
with K/Ti > 0.2, based on an apparent population minimum in the melt inclusion
data set at ~ 0.2. Whereas N-type melt inclusions are hosted dominantly in the
higher-Fo content olivines (Fo89 to Fo87), the E-type melt inclusions are mostly
found in the lower-Fo content olivines (Fo87-Fo83), suggesting that the E-type
component was less magnesian than the N-type. Both E- and N-type melt
inclusions and pillow margin glasses are low in volatile contents, indicating that
both magmas were significantly degassed upon eruption. Higher overall Cl and F
contents in the E-type melt inclusions, however, may indicate that the E-type
magmas were slightly less degassed than the N-type. The variation in K/Ti
observed in the melt inclusions cannot be successfully modeled by crystal
fractionation of olivine and plagioclase, by contamination by continental crust,
nor by contamination by hydrothermally altered oceanic crust. Therefore, the E-
type and N-type components likely reflect small-scale heterogeneities in the
iii
mantle source. The similarity in composition between the melt inclusions and the
pillow margin glasses indicates that the melt inclusions were trapped immediately
before eruption. Melt inclusions in olivines from the same outcrop have restricted
K/Ti ratios (within ~0.1), whereas the two components are both present in single
hand specimens and in at least one sample within a single olivine phenocryst. This
indicates that the two components were present at least on the scale of tens of
centimetres (i.e., hand sample), and implies a fine-scale mixing of the two
magmas. We conclude that the E- and N-type magmas were distinct in the mantle
and partially homogenized in a shallow-level reservoir of less than 4 kilometers
depth.
iv
Résumé
Les picrites provenant de l'île de Baffin sont considérés comme
représentant de magmes primitifs (jusqu'à ~ 22% en poids de MgO) qui auront
étés peu changés depuis leur extraits de leur source mantellique et sont au cœur de
notre compréhension de magmes primaires contenant haute-MgO et les sources
mantelliques hétérogènes. Dans cette étude d’inclusions de fonte de silice piégés
en olivine, le rapport du potassium au titane (K/Ti) est utilisé comme analogue
d’enrichissement d’éléments de trace car ces deux éléments sont incompatibles en
olivine et plagioclase, K/Ti se comporte d'une manière similaire à La/Sm et cette
proportion est insensible à la cristallisation d’olivine et plagioclase. Nous
considérons des compositions de roche comme appauvri (« N-type ») quand leurs
rapports de K/Ti <0,2 et enrichies (« E-type ») quand leurs rapports de K/Ti> 0,2.
Cette limite est basée sur une population minimale d’inclusions de fonte apparente
~ 0,2. Alors que les inclusions de fonte N-type sont hébergés dans les olivines
avec un contenu de forstérite à partir de Fo89 à Fo87, les inclusions E-type se
trouvent principalement dans les olivines moins forstéritiques (Fo87-Fo83) ; cela
implique que le composant E-type était moins riche en Mg que le composant N-
type. Les deux types d’inclusions vitreuses et les bordures vitreuses des laves
cousinées sont faibles en matières volatiles, ce qui indique que les deux magmes
étaient significativement dégazé à l'éruption. Cependant, des contenus supérieurs
de Cl et F dans les inclusions magmatiques de type E peuvent indiquer que les
magmes de type E sont légèrement moins dégazés que type N. La variation de K /
Ti observée dans les inclusions vitreuses ne peut pas être modélisé avec succès
v
par la cristallisation fractionnée d'olivine et de plagioclase, ni par la contamination
par la croûte continentale, ni par la contamination par la croûte océanique subie
d’altération hydrothermale. Par conséquent, probablement que les variations de
composition de type E et de type N reflètent des petites hétérogénéités dans la
source mantellique. La similitude de composition entre les inclusions vitreuses et
les bordures vitreuses des laves cousinées, ainsi que des profils de composition
plats dans les olivines hébergeant à la fois des inclusions vitreuses de type E et de
type N, indiquent que les inclusions vitreuses ont été piégées immédiatement
avant l'éruption. Les inclusions vitreuses provenant des mêmes sites
geographiques ont des rapports de K/Ti restreints (~ 0,1), tandis que les deux
composants sont présents dans les échantillons à la main et dans au moins un
échantillon dans un seul phénocristal d'olivine. Ceci indique que les deux
composants sont présents au moins sur l'échelle de quelques dizaines de
centimètres (c.-à-échantillons à la main), et que les deux composants étaient
présents à petite échelle. Nous concluons que les magmes de type E et type N
étaient distincts dans le manteau et partiellement homogénéisé dans un réservoir
peu profond, moins de 4 kilomètres de profondeur.
vi
Preface
The following thesis presents original research by the author at the
Department of Earth and Planetary Sciences, McGill University. It is submitted in
a traditional thesis format, and is ultimately intended to form a manuscript to be
submitted to a peer-reviewed journal.
Sample cutting for thin section, sample crushing and grain picking,
microprobe analysis and ion microprobe analysis were performed by the author.
The author was responsible for writing the thesis. All new scientific data is the
responsibility of the author. Data acquisition, analysis and interpretation were
supervised by Professors Donald Francis and John Stix.
vii
Acknowledgements
Leaving the comforts of a small town in BC and settling into the big city
of Montréal was not a decision I took lightly and so I would first like to thank my
family for encouraging me to pursue my academic goals and to always challenge
myself, no matter how daunting the next step may be. In particular, I’d like to
acknowledge my mother for always pushing me to better myself through
academia. Knowledge truly is our greatest tool.
It is thanks to the generous financial support from the National Sciences
and Engineering Research Council (NSERC) of Canada that this project could be
completed. Additional financial support was graciously provided by R. Wares,
J.B. Lynch, L. Trottier and C. Reinhardt.
I would like to extend my deepest gratitude to Don Francis, my principal
supervisor, who inspired me early on to continue into the field of igneous
petrology. It is because if his vast knowledge and guidance that I’ve enjoyed the
journey to this point and have since learned that in geology one must “be explicit”
and ask questions. For his warm welcome into the Volcanology group and for
taking this project into a new and exciting direction, I would like to express my
thanks to John Stix, my co-supervisor. John’s ability to consider a problem from
all angles was an invaluable asset to this project and it has been my utmost
pleasure to work with him.
The data collection process is a long and complicated one- my many
thanks go to Lang Shi, for his 24-hour support and aid with the electron
viii
microprobe at McGill, and to Nobu Shimizu and Brian Monteleone, for their
knowledge, help and patience with the ion microprobe during my two week stay
at the Woods Hole Oceanographic Institution.
Both the Igneous Petrology and the Volcanology groups at McGill have
been incredibly helpful in offering advice regarding this project. Thank you in
particular to Michael Patterson, Dejan Mildragovic and Yumi Kitayama in the
Igneous Petrology group for our countless geochemical discussions and help with
computer modeling. I would also like to thank Marc-Antoine Longpré and Jason
Coumans for their help with the ion microprobe and volatile data correction.
Finally, I would like to extend my most heartfelt thanks to the Department
of Earth & Planetary Sciences (EPS) at McGill- the EPSers welcomed me with
open arms and became my second family. In particular, thank you to Anne
Kosowski, Kristy Thornton and Angela DiNinno for answering my million
questions and for organizing all the Departmental events, without which, we
would all go crazy. Thank you to George Panagiotidis for his help with sample
preparation and to Brigitte Dionne for her patience and aid with poster work and
computer support.
ix
Table of Contents
Abstract ................................................................................................................... ii
Résumé .................................................................................................................. iv
Preface .................................................................................................................... vi
Acknowledgements ............................................................................................... vii
Table of contents .................................................................................................... ix
List of figures ......................................................................................................... xi
List of tables .......................................................................................................... xii
List of appendices ................................................................................................ xiii
Section 1: General introduction………………...……………………………….1
Section 2: Introduction…………………………………………………………..7
Section 3: Geological setting……………………………………………………..8
Section 4: Methodology…………………………………….…………………..12
4.1 Major and minor elements…………………………………………...12
4.2 Volatile elements……………………………………………………..13
Section 5: Results……………………………………………………………….14
5.1 Petrography………………………………………………………….14
5.2 Olivine phenocrysts…………………………………………………..15
5.3 Pillow margin glass matrix…………………………………………..24
5.4 Melt inclusions……………………………………………………….25
Section 6: Discussion……………………………………………………………42
6.1 Comparison of melt inclusions and pillow margin glass matrix…….43
x
6.2 Contamination……………………………………………………….51
6.3 The nature of mixing of E- and N-type components………………….57
Section 7: Conclusions………………………………………………………….63
Section 8: Contributions to knowledge and future work…………………….64
References……………………………………………………………………….67
Tables……………………………………………………………………………77
Appendices………………………………………….…………...…………..…127
xi
List of figures
Figure 1. Map of North Atlantic Igneous Province (NAIP) and image of 10
Durban Island………………………………………………………..……………
Figure 2. Photomicrographs of olivine phenocrysts and melt inclusions………..17
Figure 3. Frequency distribution histogram of olivine aspect ratio……………...19
Figure 4. Frequency distribution histograms for olivine NiO concentration 22
and forsterite content and plot of olivine NiO vs. forsterite content………..…..
Figure 5. Olvine-melt inclusion traverses for FeO and MgO……………………27
Figure 6. Plot of Fe vs. Mg for E- and N-type melt inclusions…………………..29
Figure 7. Plot of melt inclusion Fe and Mg vs. host olivine forsterite content…..31
Figure 8. Plot of K/Ti vs. Mg for melt inclusions, pillow margin 34
glasses and whole rock compositions……………………………………………
Figure 9. Melt inclusion and pillow margin glass incompatible element 36
variation diagrams for K, Ti, Cl and F………………………………………….
Figure 10. Frequency distribution histograms for melt inclusion and 40
pillow margin glass volatile concentrations (CO2, Cl, F and S)……………….
Figure 11. Plot of melt inclusion K/Ti ratios grouped by outcrop……………….45
Figure 12. Plot of melt inclusion K/Ti ratios grouped by hand sample………….47
Figure 13. Plot of melt inclusion K/Ti ratios grouped by 49
individual host olivine phenocryst……………………………………………...
Figure 14. Plot of contamination model K/Ti ratios vs. Mg and Al……………..54
Figure 15. Plot of melt inclusion Cl/K vs. K/Ti………………………………….56
Figure 16. Plot of pillow margin glass matrix K/Ti ratios 59
against melt inclusion K/Ti ratios………………………………………………
Figure 17. Variation diagram for melt inclusion and pillow 61
margin glass CO2 vs. H2O, with modeled isobars……………………………...
xii
List of tables
Table 1. Olivine phenocryst geochemistry ……………………………………...77
Table 2. Pillow margin matrix glass geochemistry………………………………91
Table 3 Melt inclusion geochemistry……………………………………….…...93
Table 4. Olivine-melt inclusion-olivine traverse ……………………….………115
Table 5. Pillow margin matrix glass volatile chemistry …………………..…....118
Table 6. Melt inclusion volatile chemistry ………………………………….….120
Table 7. Geochemical models………………………...………….…………......124
xiii
List of appendices
Appendix 1. Supplementary methods information…………………………..…127
1.1 Geochemical modeling of crystal fractionation 127
and contamination………………………………………………
1.2 SIMS sample preparation……………………………………….129
1.3 Modeling crystallization depth estimation using 130
the SolEx program…………………………………………….
Appendix 2. Olivine volatile blanks …………………………………………..132
Appendix 3. P1326-2 glass standard composition …………..………………..134
Appendix 4. Electron microprobe detection limits ……………………………136
Appendix 5. Electron microprobe reproducibility……………………………..138
1
Section 1: General introduction
The abundance of basaltic rocks worldwide, particularly along mid-ocean ridges,
first indicated to earth scientists that these lavas could represent primary melts of
the Earth’s mantle (e.g., Engel et al. 1965). Based on field observations of
peridotite inclusions in basalts and on experimental petrology, the mantle source
for mid-ocean ridge basalts (MORBs) is thought to be primarily peridotitic or
eclogitic in composition (Kushiro & Kuno 1963). Ocean basalts contain relatively
high magnesium and iron contents (6-8 wt % MgO and 5-8 wt % FeO), for low
silica contents (49-50 wt % SiO2), and so have undergone only a small extent of
crystal fractionation of olivine, pyroxene and plagioclase before eruption. The
relatively unfractionated nature of these melts, compared to other igneous rocks
such as gabbros, as well as the proximity of basaltic melts to their mantle source
at spreading ridges has motivated earth scientists to use basalts as probes of upper
mantle chemistry.
Due to their generally uniform major element composition worldwide,
basalts were initially thought to originate from an upper mantle that was
homogeneous in chemistry and mineralogy (Kushiro & Kuno 1963). However,
highly variable incompatible element concentrations (such as K, Na, Ba, Sr and
Ti) and compositional mixing trends in basalts along spreading ridges (Hart et al.
1973; White & Schilling 1973) have hinted that there is compositional and
isotopic heterogeneity in the mantle source, at least to a scale of 1000s of
kilometers.
2
Globally, the origin of this mantle heterogeneity has been largely
attributed to several melting and crustal-generating events including before ~3.0
Ga and at ~2.8 Ga, ~1.8 Ga and ~0.7 Ga (Patchett et al. 1981). The large-scale
production of crust during these events partitioned the incompatible elements
(which prefer liquid to solid phases) preferentially into the crust and left the upper
mantle (and, consequently, the MORB-source) increasingly depleted in these
elements. Furthermore, the “enriched” oceanic crust that was produced eventually
subducted back into the mantle along with its cover of ocean sediments and at
depth was heated sufficiently to melt. This remelting depleted the subducted
crustal material in incompatible elements, and resulted in a complex “marble-
cake” or “plum-pudding” mantle structure, with regions of depleted, enriched and
moderately enriched compositions (Dupré & Allègre 1983; Allègre & Turcotte
1986; Phipps Morgan & Morgan 1999).
Variable melting of a “marble-cake” (or “plum-pudding”) mantle has
helped explain the highly variable incompatible element and isotopic contents
observed at some MORB locations, where the degree of melting is moderately
low, and the more homogeneous melts that are produced where spreading is fast
and large volumes of mantle are partially melted (for example, on the East Pacific
Rise; Allègre & Turcotte 1986). A numerical model using a three-component
heterogeneous mantle starting composition (enriched, pyroxenite and depleted
mantle) has also been used to argue that variable degrees of melting of the same
heterogeneous mantle, along with varying lithospheric thicknesses and mantle
flow rates, is successful in reproducing the variations in isotopic and incompatible
3
element composition observed in both ocean island basalts, without the need for a
mantle plume (e.g., Hawai’i), and in MORBs (Ito & Mahoney 2003; Ito &
Mahoney 2005).
It is becoming increasingly clear that mantle convection has been
inefficient in homogenizing large-scale domains of the upper mantle (Hofmann
2003). Large-scale chemical heterogeneities are thought to persist only until they
are mechanically “thinned out” in the mantle to the centimeter-scale; once these
regions are sufficiently thin, chemical diffusion becomes important and
homogenization begins (Allègre & Turcotte 1986; Stixrude & Lithgow-Bertelloni
2012). However, chemically distinct regions do remain in the upper mantle which
have not “thinned out”; for example, there is a sharp geochemical transition
between two mantle regions of different isotopic composition in the Australian-
Antarctic Discordance (AAD) indicating that little mixing has occurred, despite a
source age of 1.5 Ga (Rehkämper & Hofmann 1997; Kempton et al. 2002;
Hofmann 2003). This implies that the upper mantle in this region has remained
unmixed and relatively unchanged in over a billion years- no small feat when the
mantle is thought to overturn every 100-200 My (Stixrude & Lithgow-Bertelloni
2012).
The scale to which these mantle heterogeneities are present remains
unconstrained. Geochemical studies at the outcrop scale have yielded meters-wide
isotopic heterogeneities (10-20 m scale lengths; Reisberg & Zindler 1986) and
meter-scale estimates have been made using geochemical studies of ultramafic
xenoliths and isotopic diffusion in single mineral grains (Zindler & Hart 1986).
4
The discovery of these small-scale mantle heterogeneities has impacted the way
earth scientists model the geodynamic evolution of Earth’s mantle, resulting in a
present-day “mechanical mixture” mantle, rather than a “plum pudding” one (e.g.,
Ito & Mahoney 2003; Stixrude & Lithgow-Bertelloni 2012); in this former model,
the entire mantle is heterogeneous on all scales, from kilometers down to
centimeters.
Despite the development of increasingly intricate evolutionary models of
Earth’s mantle, there are still issues that arise when considering the scale of
mantle heterogeneity. Spatial resolution of deep mantle heterogeneity is poor and
limited to studies of seismic anisotropy, where seismic waves travel at different
velocities based on the direction in an anisotropic material. Deep mantle
anisotropic resolution is at best 10 km, although is more typically at the 200 km-
scale (Ritsema et al. 2007; Stixrude & Lithgow-Bertelloni 2012). Furthermore,
while these geophysical probes provide information on anisotropy, they do not
measure chemical composition; earth scientists must use experimental petrology
and knowledge of high-pressure phase transitions to correlate anisotropy with
compositional variability in the deep mantle (Stixrude & Lithgow-Bertelloni
2012).
While upper mantle compositional heterogeneity has been narrowed down
to 10’s of meters, the recent use of melt inclusions has been invaluable in
exploring even smaller-scale variability, down to a hand sample scale and even
grain scale. Melt inclusions are small blebs of magma trapped in crystals as they
form and are generally considered as “snapshots” into the chemical nature of the
5
magma, with the surrounding crystal acting as a physical barrier between the melt
inclusion and the surrounding melt (although studies demonstrate that some melt
inclusions are susceptible to post-entrapment modification [Gaetani & Watson
2000; Danyushevsky et al., 2000; Danyushevsky et al. 2002]). When magma is
erupted underwater, the outer edges of the lava are flash frozen and the melt
inclusions found in the crystals along these rims are turned to glass. With luck,
there is little to no alteration of these pillow rims so that the melt inclusions
remain fresh. Olivine-hosted melt inclusions from the FAMOUS basalts, along
the Mid-Atlantic Ridge, first provided evidence of small, hand sample-scale
chemical heterogeneity, indicating that enriched and depleted mid-ocean ridge
basalts (E- and N-MORB, respectively) exist in very close proximity in the
mantle (Shimizu 1998). Soon, similar scale isotopic and trace element
heterogeneities were also found in ocean island basalt (OIB) settings (Saal et al.
1998; Sobolev et al. 2000), indicating that small-scale mantle heterogeneity is
common globally. There remains, however, little information as to the range of
compositional heterogeneity at different scales within the same lava suite.
The picritic (olivine-rich) pillow lavas at Baffin Island are both fresh and
contain many olivines bearing glassy melt inclusions. They are among the highest
MgO lavas known (up to 22 wt % MgO) and are thought to have a composition
that reflects little crystal fractionation since leaving their mantle source. It is for
these reasons that the Baffin Island picrites are excellent samples to gain insight
into the spatial resolution of mantle heterogeneity and why they have been central
to an ongoing debate in the geological community regarding the existence of
6
high-MgO primary melts and the source of ancient isotopic signatures (Donaldson
& Brown 1977; Hart & Davis 1978; Clarke & O’Hara 1979; Francis 1985;
Robillard et al. 1992; Herzberg & O’Hara 2002; Stuart et al. 2003; Ellam &
Stuart 2004; Kent et al. 2004; Yaxley et al. 2004; Starkey et al. 2009; Dale et al.
2009).
The Baffin Island picrites contain the highest recorded terrestrial 3He/
4He
ratios (up to 49 times the atmospheric ratio; Stuart et al. 2003), suggesting that
these lavas could have originated from a mantle source that remained undegassed
relative to global MORB (mid-ocean ridge basalts) and OIB (ocean island
basalts). More recently, Jackson et al. (2010) revealed that the Baffin Island lavas
also have lead and neodymium isotopic ratios that are consistent with a primordial
mantle age, or 4.45-4.55 Ga. This implies the persistence of an ancient reservoir
that has remained distinct in the mantle for four and a half billion years and raises
many questions, not the least of which is, what is the geochemical nature of this
mantle source? Robillard et al. (1992) demonstrated that the Baffin Island lavas
have highly variable incompatible element concentrations, similar in range to N-
MORB and E-MORB and attributed this variability to small-scale chemical
heterogeneity in the source. Does this imply that the Earth’s primordial mantle
was also heterogeneous, similar to modern-day MORB? To what scale was this
heterogeneity present? The olivine-hosted melt inclusions from Baffin Island are
therefore central to our understanding of the nature of their mantle reservoir and
valuable insight can be gained by considering variations in melt inclusion
composition at different scales.
7
Section 2: Introduction
The Baffin Bay Volcanic Province erupted approximately 58 My ago, during the
rifting apart of Greenland and Baffin Island that formed Davis Strait. The Baffin
lavas are among the most primitive, MgO-rich Phanerozoic basalts known
(Francis 1985), with up to ~22 weight percent MgO. Because the lower lavas
were erupted subaqueously, the outer margins of their pillows have been flash-
frozen as glass. Within the rims of these pillows are olivine phenocrysts
containing blebs of trapped melt, or melt inclusions, which were similarly frozen
as glass. These can be used to investigate mantle processes that occur during the
history of the magma.
The picritic lavas from the North Atlantic Igneous Province (NAIP) have
been studied extensively over the last forty years with regards to the nature of
their source magmas and the geochemical processes which formed these lavas
(Donaldson & Brown 1977; Hart & Davis 1978; Clarke & O’Hara 1979; Francis
1985; Robillard et al. 1992; Herzberg & O’Hara 2002; Stuart et al. 2003; Ellam &
Stuart 2004; Kent et al. 2004; Yaxley et al. 2004; Starkey et al. 2009; Dale et al.
2009). Robillard et al. (1992) first discovered that the Baffin lavas were mixtures
of two mantle components. Robillard et al. (1992) defined one end-member as
depleted in incompatible elements, or N-type, and the other as relatively enriched
in incompatible elements, or E-type. Both N- and E-type components are present
and intermixed throughout the Baffin Island lavas. While significant progress has
been made in our understanding of the formation of the Baffin Island picrites and
the heterogeneous nature of their mantle source, several key questions remain. To
8
what extent are the two lava types, E- and N-type, mixed in the Baffin picrites? At
what scale is each type present, from the outcrop scale down to a single olivine
phenocryst? And what role, if any, has pre-eruptive contamination or post-
entrapment modification of melt inclusions played? We present in this paper the
results of a detailed study of the distribution of these two components at different
scales that shows that individual outcrops are dominantly E- or N-type, but both
magma types are present at the scale of tens of centimeters. We conclude that the
two magmas were mixed in a shallow reservoir shortly before eruption.
Section 3: Geological setting
The Baffin Bay volcanic province comprises a series of outcrops along the eastern
coast of Baffin Island from Cape Searle to Cape Dyer and on the western coast of
Greenland, between the Svartenhuk Peninsula and Disko Island (Fig. 1). The
Baffin Bay lavas are similar in age to lavas from East and West Greenland, the
Faeroe Islands, Northern Ireland and Western Scotland, collectively known as the
North Atlantic Tertiary Province (Clarke 1970). The North Atlantic Tertiary
Province is thought to be created by the upwelling of a mantle plume, associated
with the current Icelandic plume (Robillard et al. 1992); however, Gill et al.
(1995) have presented an alternative hypothesis in which Baffin Island and West
Greenland lavas were the products of a secondary plume not associated with
Iceland. Furthermore, some recent studies favour a source for the Baffin picrites
that is similar to North Atlantic mid-ocean ridge basalts (MORB), rather than a
plume (e.g. Stuart et al. 2003).
9
Figure 1 a Tectonic reconstruction of North Atlantic Igneous Province (NAIP) at
~55 Ma, modified from Saunders et al. (1997). Study area is indicated. b Image of
Cape Searle, looking north. The stratigraphy is representative of the successions
sampled at Padloping Island, Durban Island and Aki Point. The transition from
the lower pillows and pillow breccias (bottom ~300m) and the upper subaerial
flows (top ~450m) is shown by a solid line. Photograph courtesy of Don Francis.
10
a
b
Pillow lavas and breccias
Subaerial lava flows
Study
area
1000 km
N
11
The Tertiary lavas on Baffin Island are comprised almost entirely of
picrites to picritic basalts, while their counterparts on Greenland grade up-section
from picrites to plagioclase-bearing basalts, with minor nepheline-normative
trachytes (Clarke 1970). The Baffin lavas either lie unconformably on a
Precambrian gneissic basement or conformably on poorly-consolidated
Palaeogene terrestrial sediments (Francis 1985). The Precambrian basement
typically has a mineral assemblage of quartz-two feldspars-biotite-garnet-
muscovite, often with accessory apatite, zircon and/or magnetite, while the
sediments are generally quartz-rich sandstones and shales, indicative of deltaic
deposition (Clarke & Upton 1971). Individual lava flows are typically 3.5 meters
in thickness but range in places up to 35 meters. The flows are essentially
horizontal, but are locally disrupted by faulting and slumping (Clarke & Upton
1971), and the lava sequence thins inland from their maximum thickness along
seaside cliffs, where their stratigraphy is best exposed (Clarke & Upton 1971).
The sequence sampled on Padloping Island for this study is approximately
750 m thick with the bottom 300 m largely comprised of pillow basalts with
minor subaqueous massive flows and pillow breccias, while the upper 450 m are
mainly comprised of thin, subaerial flows with red, oxidized and ropy flow tops
(Fig. 1; Francis 1985). This stratigraphic sequence is characteristic of Baffin Bay
lavas in general (Clarke & Upton 1971). The picrites in this study were sampled
from northeastern Padloping Island (Lat. 67º10’N, Long. 62 º 25’W) by D.
Francis in 1985 and 2004 and are labeled as “PdXX” and “PIXX”, respectively.
The samples from Padloping Island in this paper have been previously studied by
Francis (1985), Robillard et al. (1992), Kent et al. (1998; 2004) and Yaxley et al.
12
(2004). Additional samples were collected by Francis in 2004 at Aki Point and
Durban Island, labeled “AkXX” and “DbXX”, respectively.
Section 4: Methodology
4.1 Major and minor elements
Polished thin sections with thicknesses of ~100 μm bearing glassy pillow
margins were used for petrography and major and minor element analysis by
electron microprobe. The major and minor elements in olivine phenocrysts, glass
margins and melt inclusions were analyzed using a JEOL 8900L scanning
electron microprobe at McGill University. The analyzing conditions for olivine
phenocrysts were 20 kV acceleration voltage, 30 nA beam current and a beam
diameter of 2 μm. Matrix glass and melt inclusion analyses were carried out with
a 15 kV acceleration voltage, 20 nA beam current and a 2 μm-diameter electron
beam. As sodium is a relatively volatile element, we monitored the intensity of the
Na signal for six minutes (longer than the total time per analysis) with the 2 μm-
diameter beam and confirmed that Na counts were constant and reliable under
these conditions. Peak counting times for olivine were 20s for Si, Mg, Mn, Fe and
Al, 50s for Ti and 60s for Ca and Ni. Peak count times for glass were 20s for Na,
Mg, Fe, K, Si, Al, Mg, P, Ti and Ca , 60s for Cr and 120s for Cl and S. Standards
were analyzed every 10-15 analyses to monitor analytical reproducibility.
Major and minor element concentrations in matrix glasses were calculated
as averages of 4-10 microprobe analyses, with outlier values (e.g. +/- 20% of any
major element) excluded. Melt inclusions were selected for microprobe analysis
13
on the basis of size and quality using a petrographic microscope, and were at least
60 μm in diameter in order to exclude compositional zonation adjacent to the
olivine walls of the inclusion. The melt inclusions selected in thin section
contained no visible cracks or shrinkage bubbles (N.B. bubbles were later
identified in grain mounts).
4.2 Volatile elements
Five samples (three depleted, one enriched, and one with both depleted
and enriched melt inclusions) with the highest sulfur concentrations analyzed by
electron microprobe were selected for secondary ion mass spectrometer (SIMS)
analysis (see Appendix 1.2 for sample preparation). The melt inclusions were
analysed on a Cameca IMS 1280 secondary ion mass spectrometer (SIMS) at
Woods Hole Oceanographic Institution (WHOI) for 12
C, 16
O1H,
19F,
30S and
35Cl,
ratioed against the 30
Si reference mass. These secondary ions were produced by a
primary 133
Cs+ beam with a 1.2-1.5 nA current and a 10 μm diameter. An electron
beam was used to compensate for the positive charge induced on the sample
surface by the primary ion beam. Before analysis, a 30 x 30 μm sample surface
area was rastered, and a mechanical aperture placed at the secondary ion image
plane was then used to analyze a 20 x 20 μm area of the melt inclusion surface,
after four minutes of pre-sputtering. Count times were 10 seconds for all
secondary ions including the 30
Si reference mass. Data were collected in blocks of
ten cycles (in which each cycle has one set of analyses for all secondary ions).
Calibration curves were generated using nine standard glasses of basaltic to
basaltic andesitic composition, and an external basaltic glass standard was
14
analyzed every 5-15 analyses to monitor analytical reproducibility (P1326-2,
Appendix 3).
In order to determine the background level of volatiles during SIMS
analysis, olivine phenocrysts from this study as well as olivine, spinel and
plagioclase phenocrysts being analyzed by other researchers during the same
period at WHOI were analyzed for their volatile contents. Averages (excluding
outliers) of the raw SIMS counts for each volatile element were created using the
full dataset in order to calculate representative background volatile levels. Raw
SIMS elemental counts were used for this purpose instead of the ratios because
spinel contains little Si; new elemental ratios were calculated using the average
SIMS counts for 12
C, 16
O1H,
19F,
30S and
35Cl and the average
30Si count. The
average background concentration of each volatile element was then determined
with these new average ratios using the calibration curves generated from
standards. The melt inclusion and pillow margin glass compositions were
corrected for background volatile levels by subtracting these average volatile
contents, and the error associated in all these steps was calculated.
Section 5: Results
5.1 Petrography
A total of twenty samples were used in this study, from sites on Padloping
Island (labelled “Pd” or “PI”), Durban Island (“Db”) and Aku Point (“Ak”). The
pillow lavas selected are well preserved and contain fresh glass, with only minor
alteration of olivine to orange palagonite along the outermost edges. The samples
15
are dominated by picrites, with olivine phenocryst abundances ranging from
<10% up to ~40%. Olivine crystals commonly occur as clusters of grains (Fig.
2a). Plagioclase microlites are commonly present in the glassy matrix of the
pillow margins, constituting up to ~5 modal percent, but typically <1%. Although
spinel is present in the Baffin Island samples analyzed by Yaxley et al. (2004),
there is no spinel in the glassy matrix of the pillow margins used in this study.
The silicate melt inclusions analyzed in this study are exclusively from the glassy
pillow margins, generally the outermost centimeter, where the inclusions are also
glassy. Melt inclusions deeper within the pillow are devitrified and were not
analyzed as they have undergone post-entrapment crystallization. The melt
inclusions range in diameter from ~10 to 100 μm, with the majority ≤ 70 μm, and
are generally oblate spheroids. Olivine rims up to ~5µm are present around the
low-MgO melt inclusions but are typically absent in the majority of the melt
inclusions with higher MgO (Fig. 2e). Shrinkage bubbles are commonly present in
the larger melt inclusions (i.e., greater than 60 µm in diameter), and may vary
from <5% up to ~30% of the total volume of the melt inclusion. Plagioclase,
spinel, and daughter minerals are occasionally present in glass melt inclusions, but
such melt inclusions have been excluded from our dataset.
5.2 Olivine phenocrysts
Individual olivine phenocrysts are typically euhedral and there is a range
in shape from elongate to equant (Figs. 2, 3). The phenocryst aspect ratios have a
unimodal distribution, with most phenocrysts sub-equant in shape (i.e., an aspect
16
Figure 2 a Olivine phenocrysts in clusters are indicated by white circles. b
Olivine phenocrysts occurring in a variety of crystal shapes within an individual
sample (PI-16). c,d Olivines hosting multiple melt inclusions. e A low-MgO (6.0
wt %) melt inclusion (PI12/1) with an olivine rim. f An 7.9 wt % MgO melt
inclusion (Ak11a/6) without an olivine rim. Scale bars of 100 µm are indicated.
17
f
a b
c d
e f
100 µm 100 µm
100 µm 100 µm
100 µm 100 µm
18
Figure 3 Histogram of the range in aspect ratios in olivine phenocrysts. Examples
of each crystal shape are shown.
19
0
20
40
60
80
100
120
1:1 1:2 1:3 1:4 1:5 1:6 1:7 1:8 1:9
Fre
qu
ency
Olivine crystal aspect ratio
Equant Sub-equant Tabular Elongate
20
ratio of 1:2; Fig. 3). For individual samples, the range of crystal shapes is more
restricted, with sub-equant and equant grains dominating in some samples and
tabular and elongate grains in others. Olivines with the average forsterite
composition in the suite (Fo87) range from sub-equant to elongate, with aspect
ratios extending to ~ 1:8. Although there is no clear correlation between the
presence of multiple melt inclusions and olivine crystal shape or forsterite
content, olivine phenocrysts containing low-MgO melt inclusions tend to be more
equant in shape, whereas olivines hosting melt inclusions with MgO contents
similar to those of the pillow margin glasses tend to be more elongate.
Olivine phenocrysts in the Baffin lavas range from < 100 µm to ~1.5 mm
in size, with an average phenocryst size of ~500 µm. They have a unimodal
forsterite distribution ranging from Fo83 to Fo89, with a mode about Fo87 (Fig. 4a)
and with two high-Fo olivines at Fo90 and Fo91. The forsterite content in
individual olivine phenocrysts is relatively constant with phenocrysts exhibiting
flat compositional profiles across the interiors with narrow normally zoned rims
(Francis 1985). The Ni content in the Baffin olivines also exhibits a prominent
mode at 0.35 wt %, but range from a low of 0.2 wt % NiO to a high of 0.45 wt %
NiO (Fig. 4b; Table 1). The Ni content in the olivines correlates positively with
the forsterite content (Fig. 4c).
The olivine rims that occur around the low-MgO melt inclusions (and very
few moderate- to higher-MgO melt inclusions) are identifiable in FeO profiles;
across Db15/13, for example, the Fe content increases from ~12 to ~13 wt % FeO
over a distance of ~10 µm and the Mg content decreases from 47 to 37 wt% MgO
21
Figure 4 a Frequency distribution histogram for the forsterite content of host
olivine phenocrysts. b Frequency distribution histogram for host olivine Ni
content (as wt % NiO). c The NiO content in the Baffin host olivine phenocrysts
versus the forsterite content.
22
0
20
40
60
80
100
120
140
80 82 84 86 88 90 92 94 98
Fre
qu
ency
Olivine forsterite content (% Fo)
a
0
20
40
60
80
100
120
140
160
0.00 0.10 0.15 0.20 0.25 0.30 0.35 0.40 0.45 0.50
Fre
qu
ency
NiO (wt %)
b
23
0.00
0.05
0.10
0.15
0.20
0.25
0.30
0.35
0.40
0.45
0.50
82 84 86 88 90 92 94
NiO
(w
t %
)
Olivine forsterite content (% Fo)
c
24
over a distance of 20 µm (Fig. 5). For the majority of the melt inclusions,
however, this rim is not present.
5.3 Pillow margin glass matrix
The Mg content of the pillow margin glasses is relatively restricted,
varying between 8.5 and 9.5 wt % MgO, with the Fe content varying between 9.3
and 11.1 wt % total Fe (Fig. 6; Table 2). The concentration of K and Ti in the
Baffin pillow margin glasses range, respectively, from 0.07 to ~0.23 wt % K2O
and from 0.9 to 1.7 wt % TiO2. The ratio of potassium to titanium in the pillow
margin glasses and melt inclusions is used as an analogue for incompatible
element enrichment, because both are incompatible in olivine and K/Ti is
insensitive to crystal fractionation (Yaxley et al. 2004; Kent 2008), behaving
similarly to La/Sm during magmatic processes, such as crystal fractionation and
partial melting (Robillard et al. 1992). The ratio of K/Ti in the pillow margin
glasses varies from 0.08 (Pd13 and Pd56) to 0.30 (PI17; Fig. 8), despite the
restricted range in major element composition such as Mg. A homogeneous glass
standard, used to determine microprobe analytical reproducibility, has a maximum
range in K/Ti from 0.178 to 0.218. This indicates that internal variability in the
microprobe analyses can account for ~ 0.017 in the ranges of pillow margin glass
and melt inclusion K/Ti (standard VG-2; Appendix 5).
The majority of pillow margin glasses are volatile poor, with sulfur,
chlorine and carbon dioxide concentrations all below 100 ppm (Figs. 9, 10; Table
5). Fluorine concentrations are generally ~100 ppm, but reach up to ~170 ppm in
PI17/18. The pillow margin glasses have H2O contents less than the background
25
volatile concentration of H2O (Table 5). Pillow margin glasses with the highest F
and Cl contents also have the highest K and Ti contents (Figs. 9, 10) and there is a
positive correlation between the F and the K contents (Fig. 9f).
5.4 Melt inclusions
The melt inclusion Mg contents range from 9 wt % MgO (8-12 cat %)
down to 3 wt % MgO (4 cat % Mg) in the low-MgO melt inclusions (Table 3),
and do not correlate with the forsterite content of the host olivines (Fig. 7a). The
Fe contents range from 8 to 11 wt % FeO* (6-8 cat %), with a strong peak at ~9
wt % FeO* (~7 cat %), and the Fe contents of E-type melt inclusions correlate
inversely with the forsterite content of the host olivines (Fig. 7b). The melt
inclusions found in the two high-Fo olivines (Fo > ~90) have approximately 8.7
wt % MgO (12 cat %), representing some of the most magnesian melt inclusions
in the Baffin suite, however, highly magnesian melt inclusions are also common
in olivines of ~Fo87, which is the average forsterite content (Fig. 7a). The Mg and
Fe contents of the melt inclusions are relatively constant across the centre of the
melt inclusions (~8.5 wt % MgO and ~9.5 wt % FeO in Db15/13; Fig. 5; Table 4),
but decrease towards the olivine boundary within a distance of ~15 µm in the
smaller melt inclusions (<60 µm diameter) and up to ~40 µm in the larger melt
inclusions (>100 µm diameter; Fig. 5). The Mg content decreases more than the
Fe content within this distance, down to ~6 wt % MgO, while the Fe content
decreases by ~ 0.5 wt % to ~9 wt % FeO (Fig. 5). The K/Ti ratio of the Baffin
melt inclusions ranges by more than an order of magnitude from 0.05 to 0.6 with a
26
Figure 5 a Iron and b magnesium traverses across a melt inclusion (open
diamonds), including host olivine phenocryst (solid diamonds) for a large, 130
µm diameter melt inclusion (Db15/13). There is a gradient across the olivine-melt
inclusion interface indicated with vertical dashed lines. Analyses are given in
Table 4.
27
6
7
8
9
10
11
12
13
14
0 50 100 150 200 250
FeO
(w
t %
)
Distance (µm)
Db15/13, Fo87.7 a
melt inclusion
0
10
20
30
40
50
60
0 20 40 60 80 100 120 140 160 180 200 220 240 260
MgO
(w
t %
)
Distance (µm)
Db15/13, Fo87.7 b
melt inclusion
?
28
Figure 6 Plots of Fe against Mg of N-type (solid diamonds) and E-type melt
inclusions (open diamonds), pillow margin matrix glasses (open circles), whole
rock analyses (open triangles) and olivine phenocrysts (solid squares): a The
variation in major element composition in the whole rocks, melt inclusions, and
pillow margin matrix glasses is controlled by the fractionation of olivine. b A
close-up of the melt inclusion and pillow margin glass data from a. While most
melt inclusions define a tight cluster at ~7 cat % Fe, a smaller population exhibit
decreasing Fe content with decreasing Mg. These are the melt inclusions which
have visible olivine rims, and may have experienced some re-equilibration. Whole
rock data are from Francis (1985) and Robillard et al. (1992).
29
0
10
20
30
40
50
60
0 10 20 30 40 50 60
Fe
(ca
t %
)
Mg (cat %)
N-type melt inclusion
E-type melt inclusion
Whole rock
Pillow margin matrix
Olivine
a
2
4
6
8
10
12
2 4 6 8 10 12 14
Fe
(cat
%)
Mg (cat %)
N-type melt inclusion
E-type melt inclusion
Pillow margin matrix
b
30
Figure 7 Plots of a Mg and b Fe in N-type (solid) and E-type (open) melt
inclusions against the forsterite content of the host olivine.
31
0
2
4
6
8
10
12
14
82 84 86 88 90 92
Mg
(ca
t %
)
Host olivine forsterite content (% Fo)
N-type melt inclusion
E-type melt inclusion
a
Pillow matrix glass
Olivine rim
crystallization
0
2
4
6
8
10
82 84 86 88 90 92
Fe
(ca
t %
)
Host olivine forsterite content (% Fo)
N-type melt inclusion
E-type melt inclusion
b
Pillow matrix glass
Fe-loss
32
population minimum at ~0.2. This value is taken as the boundary between “N-
type”, or depleted in incompatible elements, and “E-type”, or enriched in
incompatible elements, similar to the value used by Robillard et al. (1992).
Whereas both N- and E-type melt inclusions are found in olivine phenocrysts with
average forsterite contents (Fo87-Fo88), olivines hosting N-type melt inclusions
have Fo contents up to > Fo90, while olivines hosting E-type melt inclusions have
Fo contents as low as ~Fo83 (Fig. 7). Melt inclusions in lava pillow samples from
the same outcrop have a restricted range in K/Ti ratio, within ~0.1, over a range of
Mg contents, between ~6 to ~9 wt % MgO (8.5 to ~12 cat %; Fig. 11). Individual
samples (i.e., hand specimens) also have a restricted range in melt inclusion K/Ti
(Fig. 12). Melt inclusions within single olivine phenocrysts from all analyzed
samples except PI-17 typically have similar K/Ti ratios of N-type character which
vary by less than 0.05. By contrast, melt inclusions in sample PI17 are nearly
exclusively E-type with highly variable K/Ti ratios (from ~0.3 to ~0.7; Fig. 13).
There appears to be no correlation between the ratio of K/Ti and the distance of
the melt inclusion from the olivine crystal edge.
The volatile contents in the melt inclusions are similar to the pillow
margin matrix glasses, with most F contents below ~150 ppm, Cl below ~100
ppm, and H2O contents below the background volatile concentration (Fig. 10,
Table 6). Carbon dioxide concentrations, however, vary between <100 ppm up to
~2500 ppm and in a few multi-melt inclusions, CO2 varies by a factor of two or
more in single olivine phenocrysts. Sulfur contents are generally low at ~100
ppm, but reach between 300 and 800 ppm in several melt inclusions. Chlorine and
33
Figure 8 Plot of K/Ti vs. Mg (cation percent) for E- and N-type melt inclusions
(open and solid diamonds, respectively), pillow margin matrix glasses (open
circles) and whole rocks (open triangles). Whole rock data are from Francis
(1985) and Robillard et al. (1992).
34
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0 5 10 15 20 25 30 35 40
K/T
i
Mg (cat %)
N-type melt inclusion
E-type melt inclusion
Pillow margin matrix glass
Whole rock
35
Figure 9 Variation diagrams for incompatible elements a K and Ti, b Ti and Cl, c
F and Ti d K and Cl, e F and Cl f K and F. N-type melt inclusions shown as solid
diamonds, E-type melt inclusions as open diamonds, N-type pillow margin
glasses as solid circles and E-type pillow margin glasses as open circles.
Detection limits for minor elements are given in Appendix 4.
36
0.0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.5 0.6 0.7 0.8 0.9 1.0 1.1 1.2
K (
cat
%)
Ti (cat %)
E-type melt inclusion
E-type pillow margin matrix glass
N-type melt inclusion
N-type pillow margin matrix glass
a
0
50
100
150
200
250
300
350
400
450
0.5 0.6 0.7 0.8 0.9 1 1.1 1.2
Cl
(pp
m)
Ti (cat %)
N-type melt inclusion
N-type pillow margin matrix glass
E-type pillow margin matrix glass
E-type melt inclusion
b
37
0
50
100
150
200
250
300
350
0.5 0.6 0.7 0.8 0.9 1.0 1.1 1.2
F (
pp
m)
Ti (cat %)
N-type melt inclusion
E-type melt inclusion
E-type pillow margin matrix glass
N-type pillow margin matrix glass
c
0.00
0.05
0.10
0.15
0.20
0.25
0.30
0.35
0.40
0.45
0.50
0 50 100 150 200 250 300 350 400 450
K (
cat
%)
Cl (ppm)
N-type melt inclusion
E-type melt inclusion
N-type pillow margin glass
E-type pillow margin glass
d
38
0
50
100
150
200
250
0 20 40 60 80 100 120 140 160 180
F (
pp
m)
Cl (ppm)
N-type melt inclusion
E-type melt inclusion
N-type pillow margin glass
E-type pillow margin glass
e
0
0.05
0.1
0.15
0.2
0.25
0.3
0 50 100 150 200 250 300
K (
cat
%)
F (ppm)
N-type melt inclusion
N-type pillow margin glass
E-type pillow margin glass
E-type melt inclusion
f
39
Figure 10 Histograms of volatile concentrations in N-type melt inclusions (solid),
E-type melt inclusions (open), N-type pillow margin glasses (checkered) and E-
type pillow margin glasses (dotted) for a CO2 b F c S and d Cl.
40
0
2
4
6
8
10
12
14
16
0 200 400 600 800 1000 1200 1400 1600 1800 2000 2200 2400 2600
Fre
qu
ency
CO2 (ppm)
E-type pillow margin glass
N-type pillow margin glass
E-type melt inclusion
N-type melt inclusion
a)
0
2
4
6
8
10
12
0 20 40 60 80 100 120 140 160 180 200
Fre
qu
ency
F (ppm)
E-type pillow margin glass
N-type pillow margin glass
E-type melt inclusion
N-type melt inclusion
b)
41
0
2
4
6
8
10
12
14
16
0 100 200 300 400 500 600 700 800 900 1000
Fre
qu
ency
S (ppm)
E-type pillow margin glass
N-type pillow margin glass
E-type melt inclusions
N-type melt inclusions
c)
0
2
4
6
8
10
12
14
0 10 20 30 40 50 60 70 80 90 100 110 120 130 140 150 160 170
Fre
qu
ency
Cl (ppm)
E-type pillow margin glass
N-type pillow margin glass
E-type melt inclusions
N-type melt inclusions
d)
42
fluorine contents are systematically higher in E-type melt inclusions than N-type
(Figs. 9, 10). There is no clear correlation, however, between melt inclusion CO2
or S contents and relative enrichment (Fig. 10). The ratio of Cl/K, used to evaluate
the role of assimilation of hydrothermally-altered oceanic crust (Michael &
Cornell 1998), varies between ~0.002 and 0.1 (with one outlier at ~0.18) in the
Baffin Island melt inclusions, but the majority of the melt inclusions have a
restricted Cl/K ratio of less than 0.06 (Fig. 14). Several E-type melt inclusions
have Cl/K ratios slightly higher than 0.06 (Fig. 14).
As with the pillow margin glasses, there is a positive correlation between
the K, Cl and Ti contents in the melt inclusions, in both the E-type and N-type
melt inclusions (Fig. 9a, b, d). The fluorine contents are better correlated with the
Cl contents in the N-type melt inclusions than the E-type (Fig. 9e). The fluorine
contents are also weakly correlated with the K contents in both the E- and N-type
melt inclusions (Fig. 9f).
Section 6: Discussion
As the analytical reproducibility of glass K/Ti ratios is within 0.017, the ranges in
melt inclusion and pillow margin glass K/Ti observed in the Baffin Island picrites
are not a result of analytical error, but rather represent true variability in the
samples themselves. The variation in melt inclusion K/Ti indicates that both
compositional end-members were present at different scales ranging from meter-
wide outcrops down to centimeter-scale hand specimens to millimeter-scale
olivine and implies a fine-scale mixing but not complete homogenization of the
43
two magmatic components. Both N- and E-type melt inclusions are hosted in
olivines with flat compositional profiles (Francis 1985), suggesting that the two
types of melt inclusions were trapped in approximately the same magmatic
conditions, with the N-type melt inclusions hosted in the higher-Fo content
olivines and the E-type melt inclusions in the lower-Fo content olivines. The
overall low volatile contents in both N- and E-type melt inclusions, as well as the
adjacent pillow margin matrix glasses, indicates that the two magma types were
quite degassed at the time of melt inclusion entrapment.
6.1 Comparison of melt inclusions and pillow margin glasses
N-type melt inclusions are typically found in olivines in N-type pillow
margin glasses and E-type melt inclusions typically in olivines in E-type pillow
margin glasses (Fig. 15). For E-type glasses, melt inclusions show both higher
K/Ti and greater variability compared to pillow margin glasses. The similarity in
major element composition (Tables 2, 3) between the matrix glasses and melt
inclusions implies that there has not been significant olivine fractionation since
the entrapment of the melt inclusions. Francis (1985) has argued that the similar
composition of the melt inclusions and host glasses, along with the common
presence of plagioclase microlites, is an indication that the erupted liquids were
perched on the plagioclase saturation surface. This is best demonstrated in K/Ti-
Mg space in which a range of K/Ti values at almost constant Mg (Fig. 8)
represents the olivine-plagioclase cotectic defined by the arrival of individual
liquid compositions on the plagioclase saturation surface following olivine
44
Figure 11 A plot of the distribution in K/Ti at an outcrop scale for outcrop 1
(samples Ak11a, Ak12), outcrop 2 (Ak2), outcrop 3 (Db13, Db14, Db15), outcrop
4 (PI02c, PI3c, PI06c, PI07c, PI09c, PI10c), outcrop 5 (PI12, PI13c) and outcrop
6 (PI14, PI14c, PI15c, PI16, PI17, PI17c, PI18c, PI19c, PI23c).
45
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
K/T
i
Outcrop No.
N-type
E-type
1 2 3 4 5 6
46
Figure 12 Plot of the range in K/Ti in melt inclusions within different hand
samples.
47
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7K
/Ti
E-type
N-type
Pd
13
Pd
19
PI0
2
PI0
6
PI0
7
PI0
9
PI1
0
PI1
2
PI1
3
PI1
4
PI1
5
PI1
6
PI1
7
PI1
8
PI2
3
Db
13
Db
14
Db
15
Ak
2
Ak
11
a
Ak
12
Samples
48
Figure 13 Plot of K/Ti for multiple melt inclusions hosted within single olivine
phenocrysts. Dotted lines separate different samples.
49
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
Pd
13
/2
Pd
13
/i1
8
Pd
19
/i6
PI1
4/1
9
PI1
6/4
PI1
6/5
PI1
7/5
PI1
7/6
PI1
7/7
PI1
7/8
PI1
7/9
PI1
7/1
0
PI1
7/1
4
PI1
7/i
9
PI1
7/i
13
PI1
7/i
20
Db
14
/7
Db
15
/5
Db
15
/7
Db
15
/9
Db
15
/i2
6
AK
2/1
1
AK
2/1
3
AK
11
a/3
AK
12
/5
AK
12
/14
AK
12
/i2
K/T
i Larger Incl
Largest Incl
Smal ler incl
Smal les t Incl
E-type
N-type
50
crystallization. Crystal fractionation with or without plagioclase, however, cannot
explain the range of K/Ti values in this vertical trend while reproducing the major
element composition of the Baffin glasses. In particular, the aluminum content
increases with crystal fractionation, as not enough plagioclase crystalizes in the
model to sufficiently remove Al from the melt (i.e., 30% crystal fractionation
raises the K/Ti to 0.29 and Al to 30 wt% Al2O3; Table 7). This indicates that the
E-type melt inclusions have not merely evolved from the low-K/Ti, N-type melt
inclusions, but rather are sample a greater proportion of a distinct enriched E-type
component.
Danyushevsky et al. (2000; 2002) described a process of re-equilibration
in which melt inclusions lose iron to their host olivines and gain magnesium as
they cool in a process called “Fe-loss”. The primary experimental evidence for the
occurrence of Fe-loss is the presence of step-like FeO and MgO profiles across
olivine-melt inclusion boundaries, where, in as little as a few years, total
equilibration would occur in large olivine-hosted melt inclusions (e.g. >100 µm in
diameter), resulting in flat olivine and flat melt inclusion profiles and the absence
of Fe and Mg gradients across this boundary. Rather than step-like profiles, the
Baffin Island melt inclusions have 20-40 µm wide gradational zones adjacent to
their host olivine (Fig. 5). Melt inclusions which have experienced Fe-loss form a
trend of decreasing Fe with decreasing Mg (Fig. 6), at a constant host olivine Fo
content (Fig. 7b) and form the low-Mg edge of the data in K/Ti-Mg space (to ~3.5
cat %; Fig. 8). The spread from the MgO contents of the majority of melt
inclusions to the MgO contents of those that have undergone Fe-loss can be
explained by ~13% post-entrapment crystallization of olivine, and is interpreted to
51
represent the failure of plagioclase to nucleate in the melt inclusions. This excess
crystallization of olivine would produce a ~5 μm olivine rim on a 100 μm-
diameter spherical melt inclusion, consistent with those observed using the
electron microprobe (Fig. 2e). Olivine phenocrysts containing melt inclusions
with low MgO contents and olivine rims tend to be more equant in shape than
olivines hosting melt inclusions with MgO contents similar to those of the pillow
margin glasses, suggesting that the low-MgO melt inclusions reflect slower
olivine growth rates than the more elongated olivines. These slower growth rates
may have promoted Fe-loss during the excess crystallization of olivine. The
majority of the glass melt inclusions have Mg contents similar to those of the
pillow margin matrix glasses, however, indicating that the Fe-loss process is not a
significant problem in the majority of the Baffin Island melt inclusions.
6.2 Contamination
As the Baffin Island lavas were erupted through gneissic basement rock, it
is possible that the difference between the N- and E-type lavas is a result of
contamination with continental crust, where higher K abundances in the crust
could have raised the K/Ti ratios to produce the high values and variability in the
E-type melt. Yaxley et al. (2004) argued that up to 30% assimilation of granitic
crust could explain the compositional variation in at least some of the Baffin
Island lavas. To test this, we modeled the addition of the same granitic
contaminant (Baffin Island sample 95T-511 from Thériault et al. 2001) used by
Yaxley et al. (2004) to an N-type whole rock starting composition in an attempt to
replicate the E-type melt inclusion K/Ti ratios (Table 7). Whereas Yaxley et al.
52
(2004) performed simple two-component mixing calculations, we used both
MELTS (Asimow & Ghiorso 1998) and a thermodynamic crystal fractionation
model by Don Francis to simulate more realistic mixing conditions. We found that
as little as 10% assimilation of granite at 5% crystallization can reproduce the
K/Ti ratios of the least enriched E-type melt inclusions (i.e., K/Ti = 0.2). The
resulting Al contents, however, were unrealistically high (~ 20 cat % Al; Figure
14). This is likely a result of the fact that we modeled the end of crystal
fractionation at the onset of plagioclase crystallization (observed as microlites in
thin section) and thus not enough plagioclase had crystallized in the model to
sufficiently reduce the Al concentration. Since the assimilation of granite cannot
successfully reproduce the majority of K/Ti ratios in the E-type melt inclusions as
well as the major element compositions, contamination by granitic crust is not a
likely source for the E-type component.
The higher Cl contents of the E-type glasses suggest the possibility that
they have interacted with high-Cl fluids, such as seawater or brines. The Cl
contents in the E- and N-type melt inclusions, however, correlate positively with
the F contents (Fig. 9d), an incompatible element insensitive to seawater/brine
contamination. Another possibility is that contamination by hydrothermally-
altered oceanic crust produced the high chlorine-potassium ratios (Cl/K of 0.06-
0.08; Fig. 15) observed in the E-type melt inclusions (e.g. in PI17). The Cl/K
ratios of the E-type melt inclusions, however, are similar to those typical of E-
MORB (Cl/KE-MORB of 0.05-0.08; Michael & Cornell 1998). Using both MELTS
(Asimow & Ghiorso 1998) and our thermodynamic crystal fractionation model
(Don Francis), we tested the addition of a low-water (1 wt % H2O) and a higher-
53
Figure 14 Plot of K/Ti vs Mg (a) and K/Ti vs Al (b) for a representative number
of contamination models. In the legend, “OC” is oceanic crust. See Appendix 1.1
for details regarding modeling method.
54
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
0 5 10 15 20 25 30
K/T
i
Mg (cat %)
+ 1% granite + 10% granite + 10% OC (1%H2O)
+ 20% OC (1%H2O) + 10% OC (5% H2O) + 50% OC (5% H2O)
50 % crystallized 35 30
25
20
15
10
5 1
a
E-type
N-type
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
15 17 19 21 23 25 27 29 31
K/T
i
Al (cat %)
+ 1% granite + 10% granite + 10% OC (1% H2O)
+ 20% OC (1% H2O) + 10% OC (5% H2O) + 50% OC (5% H2O)
50 35 30
25
20
15
10
5
1 % crystallized
b
E-type
N-type
55
Figure 15 Plot of Cl/K vs. K/Ti for all melt inclusions. The boundary between N-
and E-type melt inclusions is indicated with a vertical line and the upper limit of
mantle Cl/K ratios is indicated with a horizontal dashed line.
56
0.00
0.02
0.04
0.06
0.08
0.10
0.12
0.14
0.16
0.18
0.20
0.00 0.05 0.10 0.15 0.20 0.25 0.30 0.35 0.40
Cl/
K
K/Ti
Mantle
N-type E-type
57
water (5 wt % H2O) hydrothermally-altered oceanic crust composition to an N-
type starting composition in an attempt to reproduce the Cl/K ratios as well as the
K/Ti ratios of the E-type melt inclusions (Table 7). While as little as 10%
contamination of a hydrothermally-altered oceanic crust (of either water contents)
can reproduce a K/Ti ratio of 0.2, the corresponding Cl/K ratio is within accepted
mantle limits (0.03). Since the potassium contents increase more rapidly than the
Cl contents with additional assimilation, further contamination results in
progressively lower Cl/K ratios, below the Cl/K ratios observed in E-type glasses.
Chlorine levels in the contaminant would have to be unrealistically high,
approaching 0.1 wt % Cl before the Cl/K ratio surpasses normal mantle values.
Contamination by hydrothermally-altered oceanic crust therefore cannot
simultaneously reproduce the K/Ti ratios and Cl/K ratios in the majority of the
Baffin glasses. Contamination by granitic crust or by hydrothermally-altered
oceanic crust cannot successfully explain both the high K/Ti ratios and the Cl/K
ratios of the majority of the E-type melt inclusions as well as their major element
chemistry (i.e., the aluminum contents). Thus, the high Cl and F contents and
K/Ti and Cl/K ratios in the E-type melt inclusions are not likely the result of
crustal or brine/seawater contamination, but rather are characteristic of a distinct
E-type compositional end-member originating in the mantle.
6.3 The nature of mixing of N- and E-type components
Although Kent et al. (2004) identified four high-Fo olivines hosting E-
type melt inclusions, the majority of E-type melt inclusions are found in slightly
less magnesian olivines (down to Fo83), indicating that the E-type component was
58
Figure 16 Plot of pillow margin matrix K/Ti against the melt inclusion K/Ti ratios
from the same margins, with a 1:1 (dashed) line added for reference.
59
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7
Pil
low
ma
rgin
gla
ss K
/Ti
Melt inclusion K/Ti
E-type
N-type
60
Figure 17 Plot of the CO2 contents in the Baffin Island melt inclusions and pillow
margin glasses against the H2O contents. Since the H2O contents are lower than
background levels, the lowest water content the model would allow (~0.0001 wt
% H2O) was used to calculate the isobars and the CO2 contents essentially plot on
the Y-axis. a Plot of CO2 vs. H2O for melt inclusions and pillow margin glasses
(N-type pillow glasses are hidden by the E-type glasses, at [0, 0]). b Close-up of
a, below 1000 ppm CO2, where most melt inclusions and all the pillow margin
glasses occur.
61
0
500
1000
1500
2000
2500
3000
0 0.05 0.1
CO
2 (
pp
m)
H2O (wt%)
N-type melt inclusion
E-type melt inclusion
N-type pillow margin glass
E-type pillow margin glass
a
2 kbars
1 kbar
500 bars
250 bars
0
100
200
300
400
500
600
700
800
900
1000
0 0.05 0.1
CO
2 (
pp
m)
H2O (wt%)
N-type melt inclusion
E-type melt inclusion
N-type pillow margin glass
E-type pillow margin glass
1 kbar
500 bars
250 bars
b
62
likely low in MgO relative to the N-type magma. This E-type component appears
to be high in Cl and F contents, as both vary positively with the K/Ti ratios in the
E-type melt inclusions, but has similar CO2, H2O and S contents as the N-type
component. A majority of melt inclusions in the Baffin Island lavas are N-type,
suggesting that the N-type component is volumetrically dominant over the E-type
magma. The range in the level of enrichment in samples Pd19 and PI17 indicates
that the amount of E-type component was locally variable on the scale of a hand
specimen, and, in the case of PI17, on the scale of individual olivines. The greater
overall variability in melt inclusion K/Ti (up to ~0.6) compared to the K/Ti in
pillow margin glasses (from ~0.1-0.3; Fig. 16) implies a greater degree of
compositional heterogeneity during melt inclusion entrapment and only a partial
homogenization of the two magma components had occurred by the time of
eruption, as indicated by variable pillow glass K/Ti ratios. A relatively short time
interval with no significant crystal fractionation between melt inclusion
entrapment and eruption is required for the Baffin Island pillow glasses to retain a
composition similar to the melt inclusions.
The fact that many melt inclusions contain low volatile concentrations
similar to those of the host pillow margin glasses indicates that the melt inclusions
were trapped after both E- and N-type magmas were degassed. Water
concentrations in the melt inclusions cannot be accurately determined from our
SIMS results, but we can assume that the H2O contents in the pillow margin
glasses and melt inclusions are below background levels (e.g., below ~0.1 wt%
H2O). This could indicate either that the source for the Baffin lavas is lower in
water contents than the MORB-source (MORB water concentrations range from
63
0.05-0.6 wt % H20; Michael 1995; Danyushevsky 2001), or that the melts that
produced these picrites degassed vigorously prior to melt inclusion entrapment.
Alternatively, the Baffin melt inclusions may have been trapped with higher
initial H2O concentrations, but have since undergone diffusive loss of H+, as H+ is
known to diffuse rapidly through olivine from melt inclusions (e.g. Demouchy &
Mackwell 2006; Chen et al. 2011; Gaetani et al. 2012).
Since the water contents in the melt inclusions and pillow margin glasses
are lower than the background volatile level during analysis, we cannot apply the
CO2-H2O SolEx barometric model by Witham et al. (2011) directly. However, as
this model is not very sensitive to changes in H2O, we can estimate that for the
range of CO2 contents observed in the melt inclusions and the very low water
contents (see Appendix 1.3), crystallization could have occurred over a range of
depths less than 4 km (< 1 kbar, Fig. 17). A shallow mixing model explains the
similarity in the compositions and volatile contents between the melt inclusions
and pillow glasses and is consistent with the regional extensional regime present
during the separation of Greenland and Baffin Island; this extensional
environment could have promoted shallow-level pooling of upwelling mantle
material, and allowed for the E- and N-type magmas to hybridize.
Section 7: Conclusions
Melt inclusions hosted in olivine from the Baffin Island picrites indicate the
presence of two distinct components: a low K/Ti, high Mg and relatively degassed
N-type end-member and a high K/Ti, low Mg and less degassed E-type end-
64
member. The variation in K/Ti observed in the melt inclusions cannot be
successfully modeled by crystal fractionation of olivine and plagioclase, by
contamination by continental crust, nor by contamination by hydrothermally
altered oceanic crust. The positive correlation between F and Cl contents in the
melt inclusions renders interaction with seawater unlikely as a source for the E-
type component. We therefore conclude that the E-type and N-type components
reflect small-scale heterogeneities in the mantle source. Melt inclusions from the
same outcrop are dominantly either E- or N-type, with restricted K/Ti ratios;
however, both components are present in at least two single hand specimens and
within a single olivine phenocryst in one of them. The two components were thus
mixed on the scale of tens of centimetres (i.e., hand sample) and perhaps even on
the scale of millimetres. The similarity in major element composition and the
degassed nature of both the pillow margin glasses and melt inclusions indicates
the mixing of E- and N-type magmas and the entrapment of the melt inclusions
occurred in a shallow (less than 4 km deep) reservoir, immediately prior to
eruption. The shallow depth of mixing likely reflects the extensional environment
in which these lavas formed, during the rifting of Baffin Island and Greenland and
formation of Baffin Bay.
Section 8: Contributions to knowledge and future work
Research of the Baffin Island picrites has recently focused on their origins from a
primordial, undegassed mantle source (Stuart et al. 2003; Jackson et al. 2010) and
further work is needed to better characterize this ancient reservoir, to better
65
understand how a geochemically distinct source in the mantle can remain
unmixed for billions of years. Before this can be done, the geochemistry of the
olivine-hosted melt inclusions at Baffin Island has to be better characterized.
Robillard et al. (1992) first recognized the two-component mixing (an enriched E-
type with a depleted N-type component) that has occurred to produce the array of
incompatible element compositions in the Baffin Island lavas. This study has built
upon this and other previous work, enhancing our understanding of the nature of
these two components and characterising the scale to which each component is
present.
E-type melt inclusions are generally found in olivines of lower forsterite
content than N-type melt inclusions and therefore the E-type component was
likely lower in Mg than the N-type. This study presents the first set of volatile
concentrations for the Baffin Island lavas and it is determined that, while both E-
and N-type glasses are low in volatile contents, the E-type melt inclusions and
pillow margin glasses contain slightly higher F and Cl contents. It is concluded
that, while both E- and N-type components were relatively degassed soon before
eruption and at the time of melt inclusion formation, the E-type end-member was
less degassed. Both E- and N-type components are present at the outcrop scale
and at the hand sample scale. In one case, both melt inclusions types are present in
a single olivine. It is therefore determined that the two compositional end-
members were present at the scale of centimeters and, in one sample, to the scale
of a single olivine phenocryst. This implies a fine-scale mixing of the two
components in the mantle reservoir. If the mantle source for the Baffin Island
66
picrites is primordial, this further implies that the early Earth’s mantle was already
as heterogeneous as modern-day mid-ocean ridge basalts.
Future research could focus on obtaining new helium, lead and
neodymium data and determining if the N- and E-type components each have
distinct isotopic signatures. Valuable insight into the heterogeneous nature of this
primordial mantle reservoir would be gained if it could be determined whether
both compositional end-members are from this ancient reservoir or if one has
remained for billions of years, mixing later with a more modern mantle
component. The fine-scale mixing described in this study suggests that there is an
intimate link between the two components and it would further our understanding
of the Baffin Island source if this issue could be resolved.
67
References
Allègre, C.J. & Turcotte, D.L. (1986) Implications of a two-component marble-
cake mantle. Nature, 323: 123-127.
Asimow, P.D. & Ghiorso, M.S. (1998) Algorithmic modifications extending
MELTS to calculate subsolidus phase relations. American Mineralogist, 83:
1127-1132.
Barnes, J.D. & Cisneros, M. (2012) Mineralogical control on the chlorine isotope
composition of altered oceanic crust. Chemical Geology, 326-327: 51-60.
Chen, Y., Provost, A., Schiano, P. & Cluzel, N. (2011) The rate of water loss from
olivine-hosted melt inclusions. Contributions to Mineralogy and Petrology,
162(3): 625-636.
Clarke, D.B. & O’Hara, M.J. (1979) Nickel, and the existence of high-MgO
liquids in nature. Earth and Planetary Science Letters, 44: 153-158.
Clarke, D.B. & Upton, B.G.J. (1971) Tertiary basalts of Baffin Island: field
relations and tectonic setting. Canadian Journal. of Earth Sciences, 8: 248-
258.
68
Dale, C.W., Pearson, D.G., Starkey, N.A., Stuart, F.M., Ellam, R.M., Larsen,
L.M., Fitton, J.G. & Macpherson, C.G. (2009) Osmium isotopes in North
Atlantic picrites with extreme 3He/
4He ratios: implications for the nature of
high 3He/
4He mantle and the Os isotope composition of the convecting
mantle. Earth and Planetary Science Letters, 278(3-4): 267-277.
Danyushevsky, L.V. (2001) The effect of small amounts of H2O on crystallisation
of mid-ocean ridge and backarc basin magmas. Journal of Volcanology and
Geothermal Research, 110: 265-280.
Danyushevsky, L.V., Della-Pasqua, F.N. & Sokolov, S. (2000) Re-equilibration
of melt inclusions trapped by magnesian olivine phenocrysts from
subduction-related magmas: petrological implications. Contributions to
Mineralogy and Petrology, 138: 68-83.
Danyushevsky, L.V., Sokolov, S. & Falloon, T.J. (2002) Melt Inclusions in
Olivine Phenocrysts: Using Diffusive Re-equilibration to Determine the
Cooling History of a Crystal, with Implications for the Origin of Olivine-
phyric Volcanic Rocks. Journal of Petrology, 43(9): 1651-1671.
Demouchy, S. & Mackwell, S. (2006) Mechanisms of hydrogen incorporation and
diffusion in iron-bearing olivine. Physics and Chemistry of Minerals, 5(33):
347-355.
69
Donaldson, C.H. (1976) An Experimental Investigation of Olivine Morphology.
Contributions to Mineralogy and Petrology, 57: 187-213.
Donaldson, C.H. & Brown, R.W. (1977) Refractory megacrysts and magnesium-
rich melt inclusions within spinel in oceanic tholeities- indicators of magma
mixing and parental magma composition. Earth and Planetary Science
Letters, 37: 81-89.
Dupré, B. & Allègre, C.J. (1983) Pb-Sr isotope variation in Indian Ocean basalts
and mixing phenomena. Nature, 303: 142-146.
Ellam, R.M. & Stuart, F.M. (2004) Coherent He-Nd-Sr isotope trends in high
3He/
4He basalts: implications for a common reservoir, mantle heterogeneity
and convection. Earth and Planetary Science Letters, 228: 511-523.
Engel, A.E.J., Engel, C.G. & Havens, R.G. (1965) Chemical Characteristics of
Oceanic Basalts and the Upper Mantle. Geological Society of America
Bulletin, 76: 719-734.
Francis, D. (1985) The Baffin Bay lavas and the value of picrites as analogues of
primary magmas. Contributions to Mineralogy and Petrology, 89: 144-155.
Gaetani, G.A. & Watson, E.B. (2000) Open system behavior of olivine-hosted
melt inclusions. Earth and Planetary Science Letters, 183: 27-41.
70
Gaetani, G. A., O’Leary, J. A., Shimizu, N., Bucholz, C. E. & Newville, M.
(2012) Rapid reequilibration of H2O and oxygen fugacity in olivine-hosted
melt inclusions. Geology, 40(10): 915-918.
Gill, R.C.O., Holm, P.M. & Nielsen, T.F.D. (1995) Was a short-lived Baffin Bay
plume active prior to initiation of the present Icelandic plume? Clues from
the high-Mg picrites of West Greenland. Lithos, 34: 27-39.
Hart, S.R., Schilling, J.-G. & Powell, J.L. (1973) Basalts from Iceland and Along
the Reykjanes Ridge: Sr Isotope Geochemistry. Natural Physical Science,
246: 104-107.
Hart, S.R. & Davis, K.E. (1978) Nickel partitioning between olivine and silicate
melt. Earth and Planetary Science Letters, 40: 203-219.
Herzberg, C. & O’Hara, M.J. (2002) Plume-associated ultramafic magmas of
Phanerozoic age. Journal of Petrology, 43(10): 1857-1883.
Hofmann, A.W. (2003) Sampling Mantle Heterogeneity through Oceanic Basalts:
Isotopes and Trace Elements. Treatise on Geochemistry,2: 61–101.
71
Ito, G. & Mahoney, J.J. (2003) Flow and melting of a heterogeneous mantle: 1.
Method and importance to the geochemistry of ocean island and mid-ocean
ridge basalts. Earth and Planetary Science Letters, 230: 29-46.
Ito, G. & Mahoney, J.J. (2005) Flow and melting of a heterogeneous mantle: 2.
Implications for a chemically nonlayered mantle. Earth and Planetary
Science Letters, 230: 47-63.
Jackson, M.G., Carlson, R.W., Kurz, M.D., Kempton, P.D., Francis, D. &
Blusztajn, J. (2010) Evidence for the survival of the oldest terrestrial mantle
reservoir. Nature, 466: 853-856.
Jamtveit, B., Brooker, R., Brooks, K., Lotte, M.L. & Pedersen, T. (2001) The
water content of olivines from the North Atlantic Volcanic Province. Earth
and Planetary Science Letters, 186: 401-415.
Kelley, K.A., Plank, T., Ludden, J. & Stuadigel, H. (2003) Composition of altered
oceanic crust at ODP Sites 801 and 1149. Geochemistry, Geophysics,
Geosystems, 4, 8910, doi: 10.1029/2002GC000435.
Kempton, P. D., Pearce, J. A., Barry, T. L., Fitton, J. G., Langmuir, C. H. &
Christie, D. M. (2002) Sr–Nd–Pb–Hf isotope results from ODP Leg 187:
evidence for mantle dynamics of the Australian-Antarctic Discordance and
72
origin of the Indian MORB source. Geochemistry, Geophysics, Geosystems,
3, 1074, doi: 10.29/2002GC000320.
Kent, A.J.R., Stolper, E.M., Francis, D., Woodhead, J., Frei, R. & Eiler, J. (2004)
Mantle heterogeneity during the formation of the North Atlantic Igneous
Province: constraints from trace element and Sr-Nd-Os-O isotope
systematics of Baffin Island picrites. Geochemistry, Geophysics,
Geosystems, 5, Q11004, doi:10.1029/2004GC000743.
Kent, A.J.R (2008) Melt Inclusions in Basaltic and Related Volcanic Rocks.
Reviews in Mineralogy & Geochemistry, 69: 273-331.
Kushiro, I. & Kuno, H. (1963) Origin of Primary Basalt Magmas and
Classification of Basaltic Rocks. Journal of Petrology, 4(1): 75-89.
Michael, P. (1995) Regionally distinctive sources of depleted MORB: Evidence
from trace elements and H2O. Earth and Planetary Science Letters, 131:
301-320.
Michael, P.J. & Cornell, W.C. (1998) Influence of spreading rate and magma
supply on crystallization and assimilation beneath mid-ocean ridges:
Evidence from chlorine and major element chemistry of mid-ocean ridges.
Journal of Geophysical Research, 108(B8): 18,325-18,356.
73
Nielsen, R.L, & Dungan, M.A. (1983) Low pressure mineral-melt equilibria in
natural anhydrous mafic systems. Contributions to Mineralogy and
Petrology, 84(4): 310-326.
Patchett, P.J., Kouvo, O., Hedge, C.E. & Tatsumoto, M. (1981) Evolution of
Continental Crust and Mantle Heterogeneity: Evidence from Hf Isotopes.
Contributions to Mineralogy and Petrology, 78: 279-297.
Phipps Morgan, J. & Morgan, W.J. (1999) Two-stage melting and the
geochemical evolution of the mantle: a recipe for mantle plum-pudding.
Earth and Planetary Science Letters, 170: 215-239.
Rehkämper, M. & Hofmann, A. W. (1997) Recycled ocean crust and sediment in
Indian Ocean MORB. Earth and Planetary Science Letters, 147: 93–106.
Reisberg, L. & Zindler, A. (1986) Extreme isotopic variations in the upper
mantle: evidence from Ronda. Earth and Planetary Science Letters, 81: 29-
45.
Ritsema, J, McNamara. A.K. & Bull, A.L. (2007) Tomographic filtering of
geodynamic models: implications for model interpretation and large-scale
mantle structure. Journal of Geophysical Research, 112, B01303,
doi:10.1029/2006JB004566
74
Saal, A.E., Hart, S.R., Shimizu, N., Hauri, E.H. & Layne, G.D. (1998) Pb Isotopic
Variability in Melt Inclusions from Oceanic Island Basalts, Polynesia.
Science, 282: 1481-1484.
Saunders, A.D., Fitton, J.G., Kerr, A.C., Norry, M.J. & Kent, R.W. (1997) The
North Atlantic Igneous Province. In: Mahoney, J.J. & Coffin, M.F. (eds)
Large Igneous Provinces: Continental, Oceanic and Planetary Flood
Volcanism. Geophysical Monograph, American Geophysical Union, 100: 45-
93.
Shimizu, N. (1998) The geochemistry of olivine-hosted melt inclusions in a
FAMOUS basalt ALV519-4-1. Physics of the Earth and Planetary Interiors,
107: 183-201.
Sobolev, A.V., Hofmann, A.W. & Nikogosian, I. (2000) Recycled oceanic crust
observed in ‘ghost plagioclase’ within the source of Mauna Loa lavas.
Nature, 404: 986-990.
Starkey, N.A., Stuart, F.M., Ellam, R.M., Fitton, J.G., Basu, S. & Larsen, L.M.
(2009) Helium isotopes in early Iceland plume picrites: Constraints on the
composition of high 3He/
4He mantle. Earth and Planetary Science Letters,
277: 91-100.
75
Stixrude, L. & Lithgow-Bertelloni, C. (2012) Geophysics of Chemical
Heterogeneity in the Mantle. Annual Review of Earth and Planetary
Sciences, 40: 569-595.
Stuart, F.M., Lass-Evans, S., Fitton, J.G. & Ellam, R.M. (2003) High 3He/
4He
ratios in picritic basalts from Baffin Island and the role of a mixed reservoir
in mantle plumes. Nature, 424: 57-59.
Thériault, R.J., St-Onge, M.R.& Scott, D.J. (2001) Nd isotopic and geochemical
signature of the Paleoproterozoic Trans-Hudson Orogen, southern Baffin
Island, Canada: implications for the evolution of eastern Laurentia.
Precambrian Research, 108:113–138.
White, W.M. & Schilling, J.-G. (1978) The nature and origin of geochemical
variation in Mid-Atlantic Ridge basalts from the Central North Atlantic.
Geochimica et Cosmochimica Acta, 42: 1501-1516.
Witham, F., Blundy, J., Kohn, S., Lesne, P., Dixon, J., Churakov, S. &
Botcharnikov, R. (2012) SolEx: A model for mixed COHSCl-volatile
solubilities and exsolved gas compositions in basalt. Computers &
Geosciences, 45: 87-97.
Yaxley, G.M., Kamenetsky, V.S., Kamenetsky, M., Norman, M.D & Francis, D.
(2004) Origins of compositional heterogeneity in olivine-hosted melt
76
inclusions from the Baffin Island picrites. Contributions to Mineralogy and
Petrology, 148: 426-442.
Zindler, A.& Hart, S. (1986) Chemical geodynamics. Annual Review of Earth and
Planetary Sciences, 14: 493–571.
77
Table 1 Olivine phenocryst geochemistry and geometry. Major and minor
elements analyzed by electron microprobe. Uncertainty was below 1% for major
elements, checked by analyzing standards. All Fe as FeO*. Concentrations are
averages of three to ten analyses.
78
Oli
vin
e p
hen
ocr
yst
s
S
amp
le
Pd
13
/1
Pd
13
/2
Pd
13
/3
Pd
13
/4
Pd
13
/5
Pd
13
/6
Pd
13
/7
Pd
13
/8
Pd
13
/9
Pd
13
/10
Pd
13
/11
Pd
13
/i1
2
Pd
13
/i1
5
Pd
13
/i1
8
(wt
%)
SiO
2
39
.25
39
.07
39
.28
39
.28
38
.86
39
.02
39
.20
39
.53
39
.25
39
.51
39
.16
39
.90
39
.84
40
.63
TiO
2
0.0
0
0.0
1
0.0
1
0.0
0
0.0
0
0.0
1
0.0
0
0.0
2
0.0
1
0.0
2
0.0
0
0.0
0
0.0
1
0.0
0
Al 2
O3
0.0
6
0.0
6
0.0
7
0.0
5
0.0
4
0.0
7
0.0
5
0.1
1
0.0
9
0.0
7
0.0
4
0.0
5
0.0
5
0.0
6
FeO
*
11
.00
10
.98
11
.29
10
.99
10
.91
11
.92
11
.20
11
.27
11
.25
10
.93
10
.82
11
.11
11
.13
11
.13
Mn
O
0.1
7
0.1
8
0.1
8
0.1
6
0.1
7
0.1
9
0.1
7
0.1
7
0.1
7
0.1
7
0.1
7
0.1
8
0.1
8
0.1
7
MgO
4
7.5
5
47
.29
47
.35
47
.47
47
.35
46
.95
47
.43
47
.51
47
.33
47
.63
47
.60
47
.48
47
.27
47
.70
CaO
0
.33
0.3
3
0.3
2
0.3
3
0.3
3
0.3
2
0.3
2
0.3
3
0.3
2
0.3
2
0.3
1
0.3
2
0.3
2
0.3
3
NiO
0
.34
0.3
3
0.3
2
0.3
4
0.3
4
0.3
2
0.3
3
0.3
2
0.3
3
0.3
3
0.3
5
0.3
3
0.3
4
0.3
3
Cr 2
O3
0.0
7
0.0
8
0.0
6
0.0
6
0.0
6
0.0
6
0.0
4
0.0
7
0.0
8
0.0
7
0.0
5
0.0
0
0.0
0
0.0
0
To
tal
98
.77
98
.33
98
.88
98
.69
98
.05
98
.86
98
.73
99
.33
98
.82
99
.05
98
.49
99
.36
99
.12
10
0.3
5
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
Si
32
.34
32
.33
32
.36
32
.41
32
.23
32
.22
32
.33
32
.44
32
.37
32
.46
32
.33
32
.71
32
.75
33
.03
Ti
0.0
0
0.0
1
0.0
1
0.0
0
0.0
0
0.0
1
0.0
0
0.0
1
0.0
0
0.0
1
0.0
0
0.0
0
0.0
0
0.0
0
Al
0.0
6
0.0
6
0.0
6
0.0
5
0.0
4
0.0
6
0.0
4
0.1
1
0.0
8
0.0
6
0.0
4
0.0
4
0.0
5
0.0
6
Fe
7.5
8
7.6
0
7.7
8
7.5
8
7.5
7
8.2
3
7.7
3
7.7
4
7.7
6
7.5
1
7.4
7
7.6
2
7.6
5
7.5
6
Mn
1.0
5
1.1
1
1.1
0
1.0
3
1.0
6
1.1
6
1.0
6
1.0
4
1.0
4
1.0
5
1.0
5
1.0
9
1.1
1
1.0
4
Mg
58
.41
58
.34
58
.15
58
.38
58
.55
57
.78
58
.31
58
.12
58
.19
58
.35
58
.58
58
.04
57
.93
57
.80
Ca
0.2
9
0.2
9
0.2
8
0.2
9
0.2
9
0.2
9
0.2
9
0.2
9
0.2
9
0.2
8
0.2
7
0.2
8
0.2
8
0.2
9
Ni
0.2
2
0.2
2
0.2
1
0.2
2
0.2
2
0.2
1
0.2
2
0.2
1
0.2
2
0.2
2
0.2
3
0.2
2
0.2
2
0.2
2
Cr
0.0
4
0.0
5
0.0
4
0.0
4
0.0
4
0.0
4
0.0
2
0.0
4
0.0
5
0.0
4
0.0
3
0.0
0
0.0
0
0.0
0
Fo
con
ten
t (%
) 8
8.5
8
8.5
8
8.2
8
8.5
8
8.6
8
7.5
8
8.3
8
8.3
8
8.2
8
8.6
8
8.7
8
8.4
8
8.3
8
8.4
L
on
g a
xis
(x1
0-6
m)
31
8
50
0
95
0
45
0
14
57
41
1
61
9
21
0
23
0
38
9
10
62
S
ho
rt a
xis
(x1
0-6
m)
22
7
31
5
69
3
26
0
11
00
15
0
46
9
18
0
19
0
36
7
67
5
A
spec
t ra
tio
1
.4
1.6
1
.4
1.7
1
.3
2.7
1
.3
1.2
1
.2
1.1
1
.6
79
Oli
vin
e p
hen
ocr
yst
s co
nti
nu
ed
S
amp
le
Pd
19
/1
Pd
19
/2
Pd
19
/3
Pd
19
/4
Pd
19
/5
Pd
19
/7
Pd
19
/8
Pd
19
/9
Pd
19
/13
Pd
19
/14
Pd
19
/i3
a P
d19
/i5
Pd
19
/i6
Pd
19
/i8
(wt
%)
SiO
2
40
.20
40
.08
40
.07
40
.12
39
.97
40
.33
39
.51
39
.42
38
.69
39
.47
40
.21
39
.84
39
.85
40
.11
TiO
2
0.0
0
0.0
0
0.0
0
0.0
0
0.0
1
0.0
0
0.0
0
0.0
0
0.0
2
0.0
1
0.0
0
0.0
0
0.0
0
0.0
1
Al 2
O3
0.0
9
0.0
7
0.0
4
0.0
5
0.0
6
0.0
5
0.0
5
0.0
7
0.0
8
0.0
4
0.0
4
0.0
5
0.0
6
0.0
6
FeO
*
11
.02
11
.06
11
.11
11
.28
11
.27
11
.46
14
.42
13
.59
14
.63
13
.68
11
.34
11
.42
12
.31
11
.97
Mn
O
0.1
6
0.1
6
0.1
6
0.1
7
0.1
9
0.1
9
0.2
2
0.2
1
0.2
2
0.2
1
0.1
7
0.1
6
0.1
9
0.1
8
MgO
4
7.9
9
47
.71
47
.93
47
.55
47
.56
47
.83
44
.84
45
.38
44
.52
45
.76
47
.31
47
.02
46
.70
46
.70
CaO
0
.33
0.3
3
0.3
3
0.3
5
0.3
4
0.3
4
0.3
5
0.3
3
0.3
5
0.3
4
0.3
3
0.3
3
0.3
4
0.3
6
NiO
0
.34
0.3
3
0.3
3
0.3
3
0.3
3
0.3
2
0.2
1
0.2
4
0.2
1
0.2
3
0.3
2
0.3
3
0.3
1
0.3
1
Cr 2
O3
0.0
3
0.0
4
0.0
5
0.0
3
0.0
0
0.0
0
0.0
0
0.0
0
To
tal
10
0.1
4
99
.73
99
.97
99
.84
99
.72
10
0.5
3
99
.63
99
.29
98
.77
99
.78
99
.72
99
.14
99
.75
99
.69
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
Si
32
.70
32
.76
32
.66
32
.77
32
.65
32
.70
32
.73
32
.67
32
.34
32
.53
32
.92
32
.82
32
.71
32
.93
Ti
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
1
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
Al
0.0
9
0.0
6
0.0
4
0.0
5
0.0
6
0.0
5
0.0
5
0.0
7
0.0
8
0.0
4
0.0
4
0.0
4
0.0
6
0.0
6
Fe
7.5
0
7.5
6
7.5
7
7.7
1
7.7
0
7.7
7
9.9
9
9.4
2
10
.22
9.4
3
7.7
7
7.8
7
8.4
5
8.2
2
Mn
1.0
1
0.9
7
0.9
8
1.0
7
1.1
5
1.1
7
1.4
0
1.2
9
1.3
9
1.3
1
1.0
3
1.0
1
1.1
5
1.0
9
Mg
58
.20
58
.13
58
.24
57
.90
57
.92
57
.81
55
.37
56
.07
55
.47
56
.21
57
.75
57
.74
57
.13
57
.17
Ca
0.2
8
0.2
9
0.2
8
0.3
0
0.2
9
0.3
0
0.3
1
0.3
0
0.3
1
0.3
0
0.2
9
0.2
9
0.3
0
0.3
2
Ni
0.2
3
0.2
2
0.2
2
0.2
1
0.2
2
0.2
1
0.1
4
0.1
6
0.1
4
0.1
5
0.2
1
0.2
2
0.2
0
0.2
1
Cr
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
2
0.0
2
0.0
3
0.0
2
0.0
0
0.0
0
0.0
0
0.0
0
Fo
con
ten
t (%
) 8
8.6
8
8.5
8
8.5
8
8.3
8
8.3
8
8.2
8
4.7
8
5.6
8
4.4
8
5.6
8
8.1
8
8.0
8
7.1
8
7.4
L
on
g a
xis
(x1
0-6
m)
11
88
35
6
16
11
18
96
57
6
56
8
28
2
41
4
44
6
30
0
64
0
S
ho
rt a
xis
(x1
0-6
m)
88
8
25
0
73
7
10
07
25
6
25
9
17
6
22
1
30
0
22
5
30
0
A
spec
t ra
tio
1
.3
1.4
2
.2
1.9
2
.3
2.2
1
.6
1.9
1
.5
1.3
2
.1
80
Oli
vin
e p
hen
ocr
yst
s co
nti
nu
ed
S
amp
le
Pd
19
/i1
1
Pd
19
/i1
3
Pd
56
/1
Pd
56
/2
PI1
2/1
P
I12
/2
PI1
2/3
P
I12
/4
PI1
2/6
P
I12
/7
PI1
2/8
P
I12
/9
PI1
4/1
P
I14
/2
(wt
%)
SiO
2
40
.30
40
.88
39
.93
42
.26
39
.14
39
.03
39
.19
39
.40
39
.20
39
.24
39
.15
39
.35
40
.36
40
.47
TiO
2
0.0
0
0.0
0
0.0
1
0.3
5
0.0
1
0.0
1
0.0
2
0.0
0
0.0
0
0.0
1
0.0
1
0.0
1
0.0
1
0.0
1
Al 2
O3
0.0
5
0.0
3
0.0
8
2.8
9
0.0
5
0.0
3
0.0
3
0.0
5
0.0
6
0.0
3
0.0
3
0.0
4
0.0
7
0.0
6
FeO
*
11
.42
7.1
7
13
.99
12
.14
16
.31
15
.90
16
.36
14
.10
14
.08
15
.09
16
.18
15
.67
10
.97
10
.95
Mn
O
0.1
7
0.1
0
0.2
2
0.1
9
0.2
5
0.2
4
0.2
3
0.2
1
0.2
2
0.2
2
0.2
6
0.2
3
0.1
7
0.1
7
MgO
4
7.3
5
50
.38
45
.83
39
.12
43
.79
44
.05
44
.01
45
.74
45
.68
45
.09
43
.93
44
.66
48
.03
48
.06
CaO
0
.33
0.2
7
0.3
4
2.8
3
0.3
8
0.3
6
0.3
8
0.3
3
0.3
4
0.3
4
0.3
9
0.3
6
0.3
3
0.3
3
NiO
0
.33
0.4
3
0.2
5
0.2
6
0.1
8
0.2
1
0.1
8
0.2
5
0.2
5
0.2
2
0.1
9
0.2
1
0.3
3
0.3
4
Cr 2
O3
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
To
tal
99
.95
99
.26
10
0.6
5
10
0.0
4
10
0.1
2
99
.84
10
0.4
0
10
0.0
9
99
.82
10
0.2
3
10
0.1
3
10
0.5
3
10
0.2
8
10
0.3
9
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
Si
32
.92
33
.13
32
.66
35
.49
32
.47
32
.41
32
.44
32
.40
32
.31
32
.34
32
.43
32
.41
32
.77
32
.82
Ti
0.0
0
0.0
0
0.0
1
0.2
2
0.0
1
0.0
1
0.0
1
0.0
0
0.0
0
0.0
0
0.0
1
0.0
1
0.0
1
0.0
0
Al
0.0
5
0.0
3
0.0
7
2.8
6
0.0
5
0.0
3
0.0
3
0.0
5
0.0
6
0.0
3
0.0
3
0.0
4
0.0
7
0.0
6
Fe
7.8
0
4.8
6
9.5
7
8.5
3
11
.31
11
.04
11
.32
9.7
0
9.7
1
10
.40
11
.21
10
.79
7.4
5
7.4
3
Mn
1.0
5
0.6
0
1.3
4
1.2
1
1.5
6
1.5
2
1.4
4
1.3
3
1.3
4
1.3
6
1.6
0
1.4
6
1.0
6
1.0
7
Mg
57
.67
60
.86
55
.88
48
.97
54
.14
54
.53
54
.30
56
.07
56
.12
55
.41
54
.26
54
.84
58
.14
58
.11
Ca
0.2
9
0.2
4
0.3
0
2.5
4
0.3
4
0.3
2
0.3
3
0.2
9
0.3
0
0.3
0
0.3
4
0.3
1
0.2
8
0.2
9
Ni
0.2
2
0.2
8
0.1
6
0.1
7
0.1
2
0.1
4
0.1
2
0.1
6
0.1
6
0.1
5
0.1
3
0.1
4
0.2
2
0.2
2
Cr
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
Fo
con
ten
t (%
) 8
8.1
9
2.6
8
5.4
8
5.2
8
2.7
8
3.2
8
2.7
8
5.3
8
5.3
8
4.2
8
2.9
8
3.6
8
8.6
8
8.7
L
on
g a
xis
(x1
0-6
m)
59
0
15
20
66
3
13
3
23
7
12
3
63
3
27
8
12
6
17
1
16
9
10
0
11
00
Sh
ort
axis
(x1
0-6
m)
53
0
13
3
15
0
83
12
6
10
0
54
7
15
7
96
10
0
98
75
74
3
Asp
ect
rati
o
1
.1
11
.4
4.4
1
.6
1.9
1
.2
1.2
1
.8
1.3
1
.7
1.7
1
.3
1.5
81
Oli
vin
e p
hen
ocr
yst
s co
nti
nu
ed
Sam
ple
P
I14
/4
PI1
4/5
P
I14
/6
PI1
4/7
P
I14
/8
PI1
4/9
P
I14
/10
PI1
4/1
1
PI1
4/1
2
PI1
4/1
3
PI1
4/1
4
PI1
4/1
5
PI1
4/1
6
PI1
4/1
7
(wt
%)
SiO
2
39
.66
39
.87
39
.79
39
.64
39
.76
39
.84
39
.53
40
.04
39
.87
39
.28
39
.32
39
.34
39
.44
39
.04
TiO
2
0.0
0
0.0
0
0.0
1
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
1
0.0
0
0.0
1
0.0
1
0.0
0
0.0
0
Al 2
O3
0.0
9
0.0
9
0.0
6
0.0
9
0.0
7
0.0
4
0.0
9
0.0
5
0.0
5
0.0
6
0.0
5
0.0
8
0.1
0
0.0
4
FeO
*
12
.20
11
.85
11
.34
11
.78
11
.43
12
.13
12
.00
11
.04
10
.82
12
.08
11
.29
12
.03
12
.56
11
.49
Mn
O
0.1
8
0.1
7
0.1
7
0.1
8
0.1
8
0.1
8
0.1
8
0.1
6
0.1
7
0.1
7
0.1
7
0.1
7
0.1
9
0.1
6
MgO
4
7.3
8
47
.40
47
.81
48
.09
47
.64
47
.30
46
.94
47
.95
48
.17
47
.38
48
.13
47
.19
46
.93
47
.92
CaO
0
.35
0.3
4
0.3
3
0.3
4
0.3
3
0.3
4
0.3
4
0.3
1
0.3
1
0.3
6
0.3
4
0.3
4
0.3
6
0.3
2
NiO
0
.30
0.3
2
0.3
4
0.3
2
0.3
2
0.3
1
0.3
2
0.3
4
0.3
5
0.3
1
0.3
3
0.3
2
0.3
0
0.3
2
Cr 2
O3
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
To
tal
10
0.1
7
10
0.0
5
99
.86
10
0.4
3
99
.73
10
0.1
4
99
.40
99
.89
99
.75
99
.64
99
.63
99
.48
99
.88
99
.30
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
Si
32
.36
32
.55
32
.47
32
.16
32
.48
32
.52
32
.50
32
.65
32
.50
32
.19
32
.10
32
.31
32
.30
32
.00
Ti
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
1
0.0
1
0.0
0
0.0
0
Al
0.0
8
0.0
9
0.0
6
0.0
8
0.0
6
0.0
4
0.0
9
0.0
5
0.0
5
0.0
6
0.0
5
0.0
8
0.0
9
0.0
4
Fe
8.3
2
8.0
9
7.7
4
7.9
9
7.8
1
8.2
8
8.2
5
7.5
3
7.3
7
8.2
8
7.7
1
8.2
6
8.6
0
7.8
8
Mn
1.1
0
1.0
7
1.0
7
1.1
0
1.1
2
1.0
9
1.1
2
1.0
1
1.0
4
1.0
6
1.0
5
1.0
7
1.2
0
1.0
1
Mg
57
.63
57
.69
58
.15
58
.16
58
.02
57
.56
57
.53
58
.27
58
.53
57
.89
58
.58
57
.77
57
.29
58
.57
Ca
0.3
1
0.2
9
0.2
9
0.2
9
0.2
9
0.3
0
0.3
0
0.2
7
0.2
7
0.3
2
0.2
9
0.3
0
0.3
1
0.2
8
Ni
0.2
0
0.2
1
0.2
2
0.2
1
0.2
1
0.2
0
0.2
1
0.2
2
0.2
3
0.2
0
0.2
1
0.2
1
0.2
0
0.2
1
Cr
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
Fo
con
ten
t (%
) 8
7.4
8
7.7
8
8.3
8
7.9
8
8.1
8
7.4
8
7.5
8
8.6
8
8.8
8
7.5
8
8.4
8
7.5
8
6.9
8
8.1
L
on
g a
xis
(x1
0-6
m)
32
1
27
1
36
8
26
3
35
8
23
6
40
0
79
3
18
14
26
1
14
31
29
2
23
3
52
6
Sh
ort
axis
(x1
0-6
m)
25
7
17
1
22
1
16
8
23
2
18
6
30
0
52
7
91
4
17
1
80
0
10
8
80
47
4
Asp
ect
rati
o
1.2
1
.6
1.7
1
.6
1.5
1
.3
1.3
1
.5
2.0
1
.5
1.8
2
.7
2.9
1
.1
82
Oli
vin
e p
hen
ocr
yst
s co
nti
nu
ed
S
amp
le
PI1
4/1
8
PI1
4/1
9
PI1
6/1
P
I16
/2
PI1
6/3
P
I16
/4
PI1
6/5
P
I17
/1
PI1
7/2
P
I17
/3
PI1
7/4
P
I17
/5
PI1
7/6
P
I17
/7
(wt
%)
SiO
2
39
.59
39
.53
40
.11
40
.22
40
.60
40
.13
40
.15
40
.04
39
.84
38
.01
39
.94
39
.86
39
.84
40
.00
TiO
2
0.0
1
0.0
0
0.0
0
0.0
1
0.0
4
0.0
0
0.0
0
0.0
0
0.0
1
0.0
0
0.0
1
0.0
1
0.0
1
0.0
1
Al 2
O3
0.0
6
0.0
5
0.0
7
0.0
6
0.8
1
0.0
6
0.0
5
0.0
5
0.0
7
0.3
6
0.0
7
0.0
9
0.0
5
0.0
8
FeO
*
11
.59
11
.22
9.8
2
10
.99
11
.59
11
.50
11
.06
11
.86
12
.71
12
.81
12
.77
12
.72
12
.55
12
.67
Mn
O
0.1
7
0.1
7
0.1
5
0.1
8
0.1
8
0.1
7
0.1
8
0.1
8
0.2
0
0.2
0
0.2
0
0.2
0
0.1
8
0.1
9
MgO
4
7.9
3
48
.10
48
.52
47
.95
46
.22
47
.65
48
.02
47
.62
46
.81
44
.23
46
.72
47
.10
47
.32
46
.96
CaO
0
.33
0.3
3
0.3
0
0.3
2
0.7
4
0.3
3
0.3
3
0.3
3
0.3
4
0.3
8
0.3
4
0.3
3
0.3
4
0.3
3
NiO
0
.32
0.3
3
0.3
6
0.3
5
0.3
1
0.3
2
0.3
4
0.3
4
0.3
2
0.2
9
0.3
0
0.3
0
0.3
1
0.3
0
Cr 2
O3
0.0
0
0.0
0
To
tal
99
.98
99
.73
99
.33
10
0.0
7
10
0.4
8
10
0.1
6
10
0.1
3
10
0.4
2
10
0.3
0
96
.28
10
0.3
4
10
0.5
9
10
0.6
0
10
0.5
4
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
Si
32
.27
32
.25
32
.74
32
.72
33
.12
32
.69
32
.64
32
.56
32
.52
32
.43
32
.62
32
.43
32
.41
32
.58
Ti
0.0
0
0.0
0
0.0
0
0.0
0
0.0
3
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
1
0.0
0
Al
0.0
6
0.0
5
0.0
6
0.0
5
0.7
8
0.0
6
0.0
5
0.0
5
0.0
7
0.3
6
0.0
7
0.0
9
0.0
5
0.0
8
Fe
7.9
0
7.6
5
6.7
1
7.4
8
7.9
1
7.8
3
7.5
2
8.0
7
8.6
8
9.1
4
8.7
2
8.6
6
8.5
4
8.6
3
Mn
1.0
4
1.0
4
0.9
4
1.0
8
1.0
9
1.0
7
1.0
9
1.0
8
1.2
5
1.2
6
1.2
1
1.2
1
1.1
1
1.1
8
Mg
58
.24
58
.51
59
.05
58
.15
56
.22
57
.86
58
.19
57
.73
56
.97
56
.26
56
.88
57
.13
57
.39
57
.03
Ca
0.2
9
0.2
8
0.2
6
0.2
8
0.6
5
0.2
8
0.2
8
0.2
9
0.3
0
0.3
4
0.3
0
0.2
8
0.3
0
0.2
9
Ni
0.2
1
0.2
1
0.2
4
0.2
3
0.2
0
0.2
1
0.2
2
0.2
2
0.2
1
0.2
0
0.2
0
0.1
9
0.2
0
0.2
0
Cr
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
Fo
con
ten
t (%
) 8
8.1
8
8.4
8
9.8
8
8.6
8
7.7
8
8.1
8
8.6
8
7.7
8
6.8
8
6.0
8
6.7
8
6.8
8
7.0
8
6.9
L
on
g a
xis
(x1
0-6
m)
50
0
65
8
15
00
12
67
84
6
72
3
60
0
75
0
63
0
44
1
68
3
81
7
76
2
18
18
Sh
ort
axis
(x1
0-6
m)
36
4
50
0
50
0
82
2
38
5
38
5
43
3
45
0
40
0
22
9
30
8
60
0
40
5
60
0
Asp
ect
rati
o
1.4
1
.3
3.0
1
.5
2.2
1
.9
1.4
1
.7
1.6
1
.9
2.2
1
.4
1.9
3
.0
83
Oli
vin
e p
hen
ocr
yst
s co
nti
nu
ed
S
amp
le
PI1
7/8
P
I17
/9
PI1
7/1
0
PI1
7/1
1
PI1
7/1
3
PI1
7/1
4
PI1
7/1
6
PI1
7/1
8
PI1
7/1
9
PI1
7/2
1
PI1
7/2
2
PI1
7/2
3
PI1
7/i
1
PI1
7/i
2
(wt
%)
SiO
2
40
.03
39
.97
39
.97
39
.84
39
.92
39
.70
39
.76
39
.81
39
.82
39
.81
39
.21
39
.89
39
.93
39
.85
TiO
2
0.0
1
0.0
1
0.0
0
0.0
1
0.0
0
0.0
0
0.0
1
0.0
1
0.0
1
0.0
1
0.0
2
0.0
1
0.0
1
0.0
0
Al 2
O3
0.0
7
0.0
8
0.0
7
0.0
4
0.0
7
0.0
3
0.0
7
0.0
4
0.0
9
0.0
6
0.0
4
0.0
5
0.0
6
0.0
4
FeO
*
12
.56
12
.56
12
.09
13
.03
11
.75
12
.69
12
.70
11
.80
12
.64
12
.53
15
.70
12
.42
12
.89
12
.67
Mn
O
0.1
8
0.1
9
0.1
7
0.2
0
0.1
8
0.2
0
0.2
0
0.1
8
0.2
0
0.2
0
0.2
5
0.1
9
0.1
8
0.1
9
MgO
4
6.9
6
47
.03
47
.08
46
.42
47
.32
46
.68
46
.51
47
.10
46
.55
46
.87
44
.38
46
.88
46
.05
45
.92
CaO
0
.33
0.3
3
0.3
2
0.3
4
0.3
2
0.3
3
0.3
4
0.3
3
0.3
3
0.3
4
0.3
0
0.3
3
0.3
3
0.3
4
NiO
0
.30
0.3
0
0.3
2
0.2
7
0.3
3
0.3
0
0.2
9
0.3
3
0.3
0
0.3
0
0.2
6
0.3
1
0.2
9
0.3
0
Cr 2
O3
0.0
0
0.0
0
To
tal
10
0.4
5
10
0.4
8
10
0.0
3
10
0.1
5
99
.88
99
.92
99
.89
99
.60
99
.95
10
0.1
1
10
0.1
6
10
0.0
8
99
.75
99
.31
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
Si
32
.66
32
.57
32
.69
32
.63
32
.63
32
.54
32
.61
32
.65
32
.63
32
.54
32
.41
32
.62
32
.89
32
.94
Ti
0.0
1
0.0
1
0.0
0
0.0
0
0.0
0
0.0
0
0.0
1
0.0
0
0.0
1
0.0
0
0.0
1
0.0
0
0.0
0
0.0
0
Al
0.0
7
0.0
8
0.0
7
0.0
4
0.0
7
0.0
3
0.0
7
0.0
4
0.0
8
0.0
5
0.0
4
0.0
5
0.0
6
0.0
4
Fe
8.5
7
8.5
6
8.2
7
8.9
2
8.0
3
8.7
0
8.7
1
8.0
9
8.6
7
8.5
6
10
.85
8.5
0
8.8
8
8.7
6
Mn
1.1
0
1.1
7
1.0
8
1.2
5
1.1
1
1.2
1
1.2
6
1.1
2
1.2
5
1.2
4
1.5
4
1.1
9
1.1
5
1.1
8
Mg
57
.11
57
.13
57
.40
56
.68
57
.67
57
.04
56
.85
57
.59
56
.87
57
.11
54
.70
57
.15
56
.54
56
.59
Ca
0.2
9
0.2
9
0.2
8
0.3
0
0.2
8
0.2
9
0.3
0
0.2
9
0.2
9
0.3
0
0.2
7
0.2
9
0.2
9
0.3
0
Ni
0.2
0
0.2
0
0.2
1
0.1
8
0.2
1
0.2
0
0.1
9
0.2
2
0.2
0
0.2
0
0.1
7
0.2
0
0.1
9
0.2
0
Cr
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
Fo
con
ten
t (%
) 8
6.9
8
7.0
8
7.4
8
6.4
8
7.8
8
6.8
8
6.7
8
7.7
8
6.8
8
7.0
8
3.4
8
7.1
8
6.4
8
6.6
L
on
g a
xis
(x1
0-6
m)
10
09
30
00
80
0
28
4
92
5
21
85
69
2
46
2
15
00
13
50
34
5
18
24
44
0
Sh
ort
axis
(x1
0-6
m)
46
4
45
0
53
3
18
4
64
2
44
6
50
8
26
2
20
0
17
8
27
3
48
6
13
0
Asp
ect
rati
o
2.2
6
.7
1.5
1
.5
1.4
4
.9
1.4
1
.8
7.5
7
.6
1.3
3
.8
3
.4
84
Oli
vin
e p
hen
ocr
yst
s co
nti
nu
ed
Sam
ple
P
I17
/i5
PI1
7/i
8
PI1
7/i
9
PI1
7/i
10
PI1
7/i
13
PI1
7/i
14
PI1
7/i
18
PI1
7/i
19
PI1
7/i
20
Db
13
/1
Db
13
/2
Db
13
/3
Db
13
/4
Db
13
/5
(wt
%)
SiO
2
39
.94
40
.03
39
.93
39
.55
40
.08
39
.90
39
.92
39
.83
39
.87
40
.30
40
.24
40
.65
40
.32
40
.33
TiO
2
0.0
1
0.0
1
0.0
0
0.0
1
0.0
1
0.0
0
0.0
1
0.0
1
0.0
2
0.0
1
0.0
1
0.0
0
0.0
1
0.0
1
Al 2
O3
0.0
5
0.0
4
0.0
7
0.0
7
0.0
5
0.0
6
0.0
5
0.0
3
0.1
0
0.0
7
0.0
7
0.0
6
0.0
6
0.0
7
FeO
*
12
.75
12
.49
12
.63
11
.33
12
.39
12
.04
12
.25
12
.58
13
.03
13
.02
12
.79
11
.56
11
.71
11
.59
Mn
O
0.1
8
0.1
8
0.1
9
0.1
7
0.1
8
0.1
8
0.1
7
0.1
9
0.1
9
0.2
1
0.1
9
0.1
8
0.1
9
0.1
8
MgO
4
6.0
3
46
.33
46
.08
47
.01
46
.34
46
.50
46
.54
46
.46
45
.80
46
.22
47
.00
48
.21
47
.55
47
.77
CaO
0
.33
0.3
3
0.3
2
0.3
3
0.3
2
0.3
2
0.3
3
0.3
3
0.4
2
0.3
8
0.3
5
0.3
3
0.3
4
0.3
4
NiO
0
.30
0.3
0
0.3
0
0.3
3
0.3
0
0.3
2
0.3
0
0.3
0
0.2
9
0.2
9
0.3
0
0.3
2
0.3
2
0.3
4
Cr 2
O3
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
T
ota
l 9
9.5
9
99
.71
99
.51
98
.81
99
.67
99
.32
99
.58
99
.74
99
.71
10
0.5
0
10
0.9
5
10
1.3
1
10
0.4
9
10
0.6
3
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
Si
32
.94
32
.94
32
.92
32
.65
32
.98
32
.89
32
.85
32
.74
32
.88
32
.93
32
.67
32
.72
32
.76
32
.70
Ti
0.0
0
0.0
1
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
1
0.0
1
0.0
1
0.0
0
0.0
0
0.0
0
0.0
0
Al
0.0
5
0.0
4
0.0
7
0.0
7
0.0
5
0.0
6
0.0
5
0.0
3
0.0
9
0.0
7
0.0
7
0.0
6
0.0
6
0.0
7
Fe
8.7
9
8.6
0
8.7
1
7.8
2
8.5
3
8.3
0
8.4
3
8.6
5
8.9
8
8.9
0
8.6
8
7.7
8
7.9
5
7.8
6
Mn
1.1
4
1.0
9
1.1
7
1.0
9
1.0
9
1.1
2
1.0
8
1.1
5
1.1
8
1.2
8
1.1
9
1.0
8
1.1
4
1.1
0
Mg
56
.58
56
.84
56
.65
57
.85
56
.86
57
.14
57
.09
56
.93
56
.29
56
.30
56
.89
57
.86
57
.58
57
.75
Ca
0.2
9
0.2
9
0.2
8
0.2
9
0.2
9
0.2
8
0.2
9
0.2
9
0.3
7
0.3
3
0.3
1
0.2
9
0.3
0
0.3
0
Ni
0.2
0
0.2
0
0.2
0
0.2
2
0.2
0
0.2
1
0.2
0
0.2
0
0.1
9
0.1
9
0.1
9
0.2
1
0.2
1
0.2
2
Cr
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
Fo
con
ten
t (%
) 8
6.6
8
6.9
8
6.7
8
8.1
8
7.0
8
7.3
8
7.1
8
6.8
8
6.2
8
6.4
8
6.8
8
8.1
8
7.9
8
8.0
L
on
g a
xis
(x1
0-6
m)
61
0
61
0
61
0
11
5
19
4
27
9
45
6
56
9
Sh
ort
axis
(x1
0-6
m)
53
0
25
0
25
0
73
11
9
23
8
15
0
33
1
Asp
ect
rati
o
1.2
2
.4
2.4
1
.6
1.6
1
.2
3.0
1
.7
85
Oli
vin
e p
hen
ocr
yst
s co
nti
nu
ed
S
amp
le
Db
13
/6
Db
13
/7
Db
13
/8
Db
14
/1
Db
14
/3
Db
14
/4
Db
14
/5
Db
14
/6
Db
14
/7
Db
14
/9
Db
14
/10
Db
14
/12
Db
14
/13
Db
14
/14
(wt
%)
SiO
2
40
.13
40
.14
40
.70
40
.23
40
.03
40
.00
40
.22
40
.07
39
.51
40
.04
40
.14
40
.02
39
.99
39
.98
TiO
2
0.0
1
0.0
0
0.0
0
0.0
1
0.0
1
0.0
1
0.0
1
0.0
1
0.0
1
0.0
0
0.0
1
0.0
0
0.0
1
0.0
1
Al 2
O3
0.0
5
0.0
4
0.0
9
0.0
6
0.0
7
0.0
9
0.0
7
0.0
7
0.1
4
0.0
8
0.0
5
0.0
4
0.0
7
0.0
7
FeO
*
12
.39
12
.07
8.6
5
11
.84
11
.96
12
.14
11
.82
12
.19
12
.06
12
.21
12
.07
12
.55
12
.15
12
.19
Mn
O
0.1
9
0.1
9
0.1
4
0.1
8
0.1
9
0.1
9
0.1
8
0.1
9
0.1
9
0.1
8
0.1
9
0.0
0
0.1
9
0.1
8
MgO
4
6.9
4
47
.03
49
.78
47
.26
47
.08
46
.58
47
.32
47
.34
46
.82
47
.37
47
.43
47
.10
47
.39
47
.29
CaO
0
.34
0.3
4
0.3
0
0.3
4
0.3
4
0.3
4
0.3
4
0.3
4
0.3
4
0.3
5
0.3
3
0.0
1
0.3
4
0.3
4
NiO
0
.30
0.3
1
0.4
3
0.3
2
0.3
2
0.3
3
0.3
2
0.3
1
0.3
1
0.3
1
0.3
1
0.3
8
0.3
3
0.3
1
Cr 2
O3
To
tal
10
0.3
6
10
0.1
3
10
0.0
9
10
0.2
3
99
.99
99
.67
10
0.2
9
10
0.5
4
99
.37
10
0.5
6
10
0.5
1
10
0.1
0
10
0.4
7
10
0.3
7
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
Si
32
.74
32
.77
32
.83
32
.80
32
.71
32
.86
32
.77
32
.57
32
.49
32
.56
32
.63
33
.04
32
.52
32
.58
Ti
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
1
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
1
Al
0.0
5
0.0
4
0.0
9
0.0
5
0.0
7
0.0
9
0.0
7
0.0
7
0.1
3
0.0
8
0.0
4
0.0
4
0.0
7
0.0
6
Fe
8.4
5
8.2
4
5.8
4
8.0
8
8.1
8
8.3
4
8.0
6
8.2
9
8.2
9
8.3
1
8.2
0
8.6
7
8.2
6
8.3
1
Mn
1.1
7
1.2
0
0.8
3
1.1
4
1.2
0
1.1
6
1.1
3
1.1
9
1.1
9
1.1
2
1.1
4
0.0
2
1.1
8
1.1
0
Mg
57
.09
57
.23
59
.87
57
.43
57
.35
57
.03
57
.47
57
.37
57
.39
57
.42
57
.48
57
.97
57
.45
57
.44
Ca
0.3
0
0.3
0
0.2
6
0.2
9
0.3
0
0.3
0
0.3
0
0.3
0
0.3
0
0.3
1
0.2
9
0.0
1
0.3
0
0.3
0
Ni
0.2
0
0.2
1
0.2
8
0.2
1
0.2
1
0.2
2
0.2
1
0.2
0
0.2
1
0.2
1
0.2
0
0.2
5
0.2
2
0.2
1
Cr
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
Fo
con
ten
t (%
) 8
7.1
8
7.4
9
1.1
8
7.7
8
7.5
8
7.2
8
7.7
8
7.4
8
7.4
8
7.4
8
7.5
8
7.0
8
7.4
8
7.4
L
on
g a
xis
(x1
0-6
m)
75
7
76
2
34
5
42
1
15
00
no
in
cl
63
3
76
5
12
67
47
6
11
71
45
6
32
4
40
0
Sh
ort
axis
(x1
0-6
m)
48
6
43
1
26
2
37
9
53
3
38
3
48
2
40
0
44
1
61
4
18
7.5
2
27
35
8
Asp
ect
rati
o
1.6
1
.8
1.3
1
.1
2.8
1.7
1
.6
3.2
1
.1
1.9
2
.4
1.4
1
.1
86
Oli
vin
e p
hen
ocr
yst
s co
nti
nu
ed
S
amp
le
Db
14
/15
Db
15
/1
Db
15
/2
Db
15
/3
Db
15
/4
Db
15
/5
Db
15
/6
Db
15
/7
Db
15
/8
Db
15
/9
Db
15
/10
Db
15
/11
Db
15
/12
Db
15
/13
(wt
%)
SiO
2
39
.83
40
.00
40
.74
40
.77
40
.31
40
.34
40
.16
40
.16
39
.95
40
.29
40
.16
39
.89
39
.97
40
.42
TiO
2
0.0
1
0.0
1
0.0
1
0.0
0
0.0
1
0.0
1
0.0
1
0.0
0
0.0
0
0.0
0
0.0
1
0.0
1
0.0
1
0.0
0
Al 2
O3
0.1
0
0.1
1
0.0
8
0.1
2
0.0
7
0.0
8
0.0
8
0.0
6
0.0
9
0.0
3
0.0
8
0.0
7
0.0
6
0.0
7
FeO
*
12
.16
12
.10
12
.79
11
.87
12
.40
11
.96
12
.54
12
.32
12
.56
12
.14
12
.03
12
.32
12
.46
11
.87
Mn
O
0.1
8
0.1
9
0.2
0
0.1
9
0.1
8
0.1
9
0.2
0
0.2
0
0.2
0
0.2
0
0.2
0
0.1
8
0.2
0
0.1
9
MgO
4
6.9
1
46
.19
46
.31
47
.22
46
.68
47
.52
46
.98
46
.95
46
.77
47
.21
46
.96
46
.92
46
.82
47
.55
CaO
0
.35
0.3
4
0.3
7
0.3
3
0.3
4
0.3
4
0.3
3
0.3
4
0.3
3
0.3
4
0.3
4
0.3
3
0.3
5
0.3
3
NiO
0
.31
0.3
2
0.2
8
0.3
2
0.3
0
0.3
2
0.3
1
0.3
1
0.3
1
0.3
1
0.3
1
0.3
1
0.3
0
0.3
2
Cr 2
O3
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
To
tal
99
.85
99
.27
10
0.7
7
10
0.8
3
10
0.2
9
10
0.7
5
10
0.6
2
10
0.3
4
10
0.2
1
10
0.5
2
10
0.0
8
10
0.0
3
10
0.1
7
10
0.7
5
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
Si
32
.64
33
.01
33
.20
33
.07
32
.95
32
.71
32
.68
32
.75
32
.64
32
.77
32
.80
32
.64
32
.66
32
.76
Ti
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
1
0.0
0
Al
0.0
9
0.1
0
0.0
7
0.1
1
0.0
6
0.0
8
0.0
8
0.0
6
0.0
8
0.0
3
0.0
8
0.0
7
0.0
6
0.0
6
Fe
8.3
3
8.3
5
8.7
2
8.0
5
8.4
7
8.1
1
8.5
4
8.4
0
8.5
8
8.2
6
8.2
1
8.4
3
8.5
2
8.0
4
Mn
1.1
0
1.1
9
1.2
4
1.1
8
1.1
3
1.1
5
1.2
2
1.2
2
1.2
2
1.2
0
1.2
4
1.1
4
1.2
2
1.1
8
Mg
57
.31
56
.82
56
.26
57
.10
56
.88
57
.45
56
.99
57
.07
56
.98
57
.24
57
.17
57
.23
57
.04
57
.46
Ca
0.3
1
0.3
0
0.3
2
0.2
9
0.3
0
0.2
9
0.2
9
0.3
0
0.2
9
0.2
9
0.2
9
0.2
9
0.3
1
0.2
9
Ni
0.2
1
0.2
1
0.1
8
0.2
1
0.2
0
0.2
1
0.2
0
0.2
0
0.2
1
0.2
0
0.2
0
0.2
1
0.2
0
0.2
1
Cr
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
Fo
con
ten
t (%
) 8
7.3
8
7.2
8
6.6
8
7.6
8
7.0
8
7.6
8
7.0
8
7.2
8
6.9
8
7.4
8
7.4
8
7.2
8
7.0
8
7.7
L
on
g a
xis
(x1
0-6
m)
54
7
50
0
12
9
58
3
38
3
74
1
39
5
71
9
41
0
59
1
75
0
91
3
28
6
20
50
Sh
ort
axis
(x1
0-6
m)
16
0
14
6
93
36
7
20
0
32
4
20
5
26
9
21
9
34
5
70
0
66
3
14
6
10
00
Asp
ect
rati
o
3.4
3
.4
1.4
1
.6
1.9
2
.3
1.9
2
.7
1.9
1
.7
1.1
1
.4
2.0
2
.1
87
Oli
vin
e p
hen
ocr
yst
s co
nti
nu
ed
S
amp
le
Db
15
/i7
Db
15
/i10
Db
15
/i12
Db
15
/i14
Db
15
/i18
Db
15
/i26
Ak2
/1
Ak2
/2
Ak2
/3
Ak2
/4
Ak2
/6
Ak2
/7
Ak2
/8
Ak2
/9
(wt
%)
SiO
2
39
.95
40
.04
40
.22
40
.17
40
.09
40
.17
39
.81
40
.14
39
.88
39
.75
40
.07
39
.96
40
.00
39
.85
TiO
2
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
1
0.0
1
0.0
1
0.0
0
0.0
1
0.0
0
0.0
0
0.0
1
0.0
0
Al 2
O3
0.0
6
0.0
6
0.0
5
0.0
4
0.0
4
0.0
7
0.1
0
0.0
5
0.0
8
0.0
8
0.0
7
0.0
9
0.0
6
0.0
7
FeO
*
12
.56
12
.27
12
.24
12
.18
12
.16
12
.53
12
.22
12
.07
12
.20
12
.00
12
.04
12
.18
12
.49
12
.15
Mn
O
0.2
2
0.1
9
0.2
0
0.1
8
0.1
7
0.2
0
0.2
0
0.1
8
0.1
9
0.1
9
0.1
8
0.1
9
0.2
0
0.1
9
MgO
4
6.1
0
46
.86
46
.77
47
.21
46
.39
46
.18
46
.53
47
.11
46
.94
46
.91
46
.89
47
.11
46
.90
46
.98
CaO
0
.32
0.3
3
0.3
3
0.3
3
0.3
3
0.3
5
0.3
5
0.3
4
0.3
4
0.3
4
0.3
3
0.3
4
0.3
6
0.3
4
NiO
0
.30
0.3
0
0.3
1
0.3
1
0.3
1
0.2
9
0.3
2
0.3
1
0.3
1
0.3
1
0.3
1
0.3
1
0.2
9
0.3
2
Cr 2
O3
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
To
tal
99
.51
10
0.0
5
10
0.1
1
10
0.4
2
99
.50
99
.78
99
.54
10
0.1
9
99
.95
99
.59
99
.88
10
0.1
8
10
0.3
1
99
.89
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
Si
32
.89
32
.76
32
.88
32
.71
33
.04
33
.02
32
.72
32
.77
32
.63
32
.62
32
.82
32
.62
32
.64
32
.61
Ti
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
1
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
1
0.0
0
Al
0.0
5
0.0
5
0.0
4
0.0
4
0.0
4
0.0
6
0.1
0
0.0
4
0.0
8
0.0
7
0.0
6
0.0
9
0.0
6
0.0
7
Fe
8.6
5
8.3
9
8.3
7
8.2
9
8.3
8
8.6
2
8.4
0
8.2
4
8.3
5
8.2
4
8.2
5
8.3
1
8.5
3
8.3
1
Mn
1.3
5
1.1
5
1.2
2
1.1
4
1.0
6
1.2
1
1.2
4
1.1
0
1.1
7
1.1
7
1.1
3
1.1
5
1.2
1
1.1
9
Mg
56
.58
57
.15
56
.99
57
.32
56
.98
56
.59
57
.02
57
.34
57
.27
57
.39
57
.25
57
.33
57
.05
57
.32
Ca
0.2
8
0.2
9
0.2
9
0.2
9
0.2
9
0.3
1
0.3
1
0.2
9
0.3
0
0.3
0
0.2
9
0.3
0
0.3
2
0.3
0
Ni
0.2
0
0.2
0
0.2
0
0.2
0
0.2
1
0.1
9
0.2
1
0.2
0
0.2
0
0.2
0
0.2
0
0.2
1
0.1
9
0.2
1
Cr
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
Fo
con
ten
t (%
) 8
6.7
8
7.2
8
7.2
8
7.4
8
7.2
8
6.8
8
7.2
8
7.4
8
7.3
8
7.4
8
7.4
8
7.3
8
7.0
8
7.3
L
on
g a
xis
(x1
0-6
m)
45
0
43
0
57
0
57
0
27
0
15
0
36
2
51
7
23
8
10
92
34
7
59
5
15
0
10
00
Sh
ort
axis
(x1
0-6
m)
40
0
35
0
49
0
30
0
22
0
11
0
24
3
23
3
14
6
43
8
26
0
31
9
93
20
9
Asp
ect
rati
o
1.1
1
.2
1.2
1
.9
1.2
1
.4
1.5
2
.2
1.6
2
.5
1.3
1
.9
1.6
4
.8
88
Oli
vin
e p
hen
ocr
yst
s co
nti
nu
ed
S
amp
le
Ak2
/10
Ak2
/11
Ak2
/12
Ak2
/13
Ak2
/14
Ak1
1a/
3
Ak1
1a/
4
Ak1
1a/
5
Ak1
1a/
6
Ak1
2/1
A
k1
2/2
A
k1
2/3
A
k1
2/4
A
k1
2/5
(wt
%)
SiO
2
40
.12
39
.99
39
.87
39
.86
40
.03
39
.63
39
.79
39
.67
39
.62
40
.11
39
.96
39
.99
39
.93
39
.87
TiO
2
0.0
0
0.0
1
0.0
1
0.0
0
0.0
1
0.0
0
0.0
0
0.0
0
0.0
1
0.0
0
0.0
0
0.0
0
0.0
0
0.0
1
Al 2
O3
0.0
9
0.0
4
0.0
7
0.0
5
0.0
4
0.0
7
0.0
4
0.0
5
0.1
0
0.1
0
0.0
5
0.0
6
0.0
5
0.0
5
FeO
*
11
.97
12
.16
11
.87
11
.95
12
.02
12
.20
12
.18
11
.99
12
.10
12
.08
12
.11
12
.08
12
.16
12
.23
Mn
O
0.1
8
0.1
8
0.1
8
0.1
8
0.1
9
0.1
8
0.1
8
0.1
9
0.1
8
0.1
7
0.1
9
0.1
9
0.1
9
0.1
8
MgO
4
7.3
9
47
.26
47
.35
47
.13
47
.17
47
.27
47
.15
47
.55
47
.11
47
.09
47
.20
47
.24
46
.91
46
.92
CaO
0
.34
0.3
4
0.3
3
0.3
3
0.3
4
0.3
4
0.3
5
0.3
3
0.3
4
0.3
5
0.3
4
0.3
4
0.3
4
0.3
5
NiO
0
.32
0.3
1
0.3
1
0.3
2
0.3
2
0.3
1
0.3
2
0.3
2
0.3
1
0.3
2
0.3
1
0.3
1
0.3
1
0.3
0
Cr 2
O3
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
To
tal
10
0.4
1
10
0.2
8
99
.99
99
.83
10
0.1
2
10
0.0
1
10
0.0
2
10
0.1
0
99
.77
10
0.2
2
10
0.1
7
10
0.2
2
99
.88
99
.90
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
Si
32
.64
32
.60
32
.56
32
.63
32
.66
32
.40
32
.53
32
.34
32
.45
32
.76
32
.60
32
.62
32
.69
32
.65
Ti
0.0
0
0.0
0
0.0
0
0.0
0
0.0
1
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
Al
0.0
9
0.0
3
0.0
7
0.0
5
0.0
4
0.0
7
0.0
4
0.0
5
0.0
9
0.1
0
0.0
5
0.0
6
0.0
5
0.0
5
Fe
8.1
5
8.2
9
8.1
1
8.1
8
8.2
0
8.3
4
8.3
3
8.1
7
8.2
9
8.2
5
8.2
6
8.2
4
8.3
2
8.3
8
Mn
1.1
4
1.1
2
1.1
1
1.1
3
1.2
0
1.0
9
1.1
4
1.1
6
1.1
3
1.0
6
1.1
8
1.1
5
1.2
0
1.1
4
Mg
57
.48
57
.45
57
.65
57
.51
57
.39
57
.60
57
.46
57
.79
57
.53
57
.33
57
.41
57
.44
57
.25
57
.28
Ca
0.3
0
0.3
0
0.2
9
0.2
9
0.2
9
0.2
9
0.3
0
0.2
9
0.2
9
0.3
0
0.3
0
0.3
0
0.3
0
0.3
0
Ni
0.2
1
0.2
0
0.2
0
0.2
1
0.2
1
0.2
1
0.2
1
0.2
1
0.2
1
0.2
1
0.2
0
0.2
1
0.2
0
0.2
0
Cr
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
Fo
con
ten
t (%
) 8
7.6
8
7.4
8
7.7
8
7.5
8
7.5
8
7.4
8
7.3
8
7.6
8
7.4
8
7.4
8
7.4
8
7.5
8
7.3
8
7.2
L
on
g a
xis
(x1
0-6
m)
27
0
40
5
59
3
50
0
14
60
40
0
28
7
65
7
38
8
10
00
33
0
40
9
51
2
10
00
Sh
ort
axis
(x1
0-6
m)
14
3
26
7
32
1
23
2
63
0
18
9
16
9
32
9
16
5
20
5
20
5
12
6
22
4
65
0
Asp
ect
rati
o
1.9
1
.5
1.8
2
.2
2.3
2
.1
1.7
2
.0
2.4
4
.9
1.6
3
.2
2.3
1
.5
89
Oli
vin
e p
hen
ocr
yst
s co
nti
nu
ed
S
amp
le
Ak1
2/6
A
k1
2/7
A
k1
2/8
A
k1
2/9
A
k1
2/1
0
Ak1
2/1
1
Ak1
2/1
2
Ak1
2/1
3
Ak1
2/1
4
Ak1
2/1
5
Ak1
2/1
6
Ak1
2/i
2
Ak1
2/i
4
Ak1
2/i
6
(wt
%)
SiO
2
39
.92
39
.66
39
.77
39
.70
39
.78
39
.75
39
.74
39
.85
39
.52
39
.77
39
.63
40
.11
40
.04
40
.04
TiO
2
0.0
1
0.0
1
0.0
1
0.0
1
0.0
1
0.0
0
0.0
1
0.0
0
0.0
0
0.0
0
0.0
0
0.0
1
0.0
0
0.0
1
Al 2
O3
0.0
9
0.0
8
0.0
7
0.0
6
0.0
5
0.1
2
0.1
1
0.0
6
0.0
9
0.0
8
0.0
8
0.0
3
0.0
7
0.0
6
FeO
*
12
.06
12
.11
12
.14
12
.20
12
.22
12
.05
12
.14
11
.98
12
.33
11
.96
12
.19
12
.11
12
.04
12
.16
Mn
O
0.1
9
0.1
8
0.1
9
0.1
8
0.1
7
0.1
9
0.1
8
0.1
8
0.2
0
0.1
8
0.1
7
0.1
9
0.1
9
0.1
8
MgO
4
7.0
9
47
.14
47
.17
47
.20
46
.94
47
.09
47
.13
47
.32
46
.81
47
.14
47
.13
46
.64
47
.07
46
.56
CaO
0
.35
0.3
3
0.3
4
0.3
5
0.3
4
0.3
3
0.3
3
0.3
3
0.3
5
0.3
4
0.3
5
0.3
3
0.3
4
0.3
4
NiO
0
.31
0.3
1
0.3
1
0.3
1
0.3
1
0.3
1
0.3
2
0.3
2
0.3
1
0.3
2
0.3
2
0.3
1
0.3
1
0.3
1
Cr 2
O3
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
To
tal
10
0.0
1
99
.82
10
0.0
0
10
0.0
1
99
.83
99
.84
99
.97
10
0.0
4
99
.61
99
.78
99
.87
99
.73
10
0.0
7
99
.66
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
Si
32
.63
32
.47
32
.49
32
.46
32
.62
32
.53
32
.50
32
.54
32
.42
32
.57
32
.46
32
.92
32
.71
32
.90
Ti
0.0
1
0.0
0
0.0
1
0.0
1
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
1
Al
0.0
9
0.0
8
0.0
6
0.0
6
0.0
5
0.1
1
0.1
0
0.0
6
0.0
9
0.0
8
0.0
7
0.0
3
0.0
7
0.0
6
Fe
8.2
4
8.2
9
8.2
9
8.3
4
8.3
8
8.2
5
8.3
0
8.1
8
8.4
6
8.1
9
8.3
5
8.3
1
8.2
3
8.3
6
Mn
1.1
7
1.1
4
1.1
8
1.1
0
1.0
7
1.1
7
1.1
4
1.1
1
1.2
6
1.1
1
1.0
6
1.1
7
1.1
6
1.1
3
Mg
57
.37
57
.53
57
.46
57
.53
57
.37
57
.45
57
.45
57
.61
57
.25
57
.55
57
.54
57
.06
57
.33
57
.04
Ca
0.3
1
0.2
9
0.3
0
0.3
0
0.3
0
0.2
9
0.2
9
0.2
9
0.3
1
0.3
0
0.3
0
0.2
9
0.3
0
0.3
0
Ni
0.2
0
0.2
0
0.2
0
0.2
1
0.2
1
0.2
0
0.2
1
0.2
1
0.2
0
0.2
1
0.2
1
0.2
1
0.2
0
0.2
0
Cr
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
Fo
con
ten
t (%
) 8
7.4
8
7.4
8
7.4
8
7.3
8
7.3
8
7.4
8
7.4
8
7.6
8
7.1
8
7.5
8
7.3
8
7.3
8
7.5
8
7.2
L
on
g a
xis
(x1
0-6
m)
38
2
52
4
11
00
21
5
18
3
24
8
28
5
37
5
20
9
26
9
25
0
68
0
64
0
S
ho
rt a
xis
(x1
0-6
m)
16
2
32
4
34
0
15
3
11
9
10
4
15
6
38
0
10
6
19
3
19
8
19
0
12
0
A
spec
t ra
tio
2
.4
1.6
3
.2
1.4
1
.5
2.4
1
.8
1.0
2
.0
1.4
1
.3
3.6
5
.3
90
Oli
vin
e p
hen
ocr
yst
s co
nti
nu
ed
Sam
ple
A
k1
2/i
7
Ak1
2/i
9
Ak1
2/i
11
Ak1
2/i
16
Ak1
2/i
24
(wt
%)
S
iO2
40
.15
40
.29
40
.29
39
.98
39
.60
TiO
2
0.0
0
0.0
0
0.0
1
0.0
1
0.0
0
Al 2
O3
0.1
0
0.0
5
0.0
8
0.0
9
0.0
1
FeO
*
12
.02
12
.23
12
.14
11
.91
11
.98
Mn
O
0.1
9
0.1
9
0.1
7
0.1
8
0.1
9
MgO
4
6.4
8
46
.54
46
.97
46
.88
46
.35
CaO
0
.33
0.3
4
0.3
4
0.3
4
0.3
3
NiO
0
.31
0.3
0
0.3
0
0.3
1
0.3
1
Cr 2
O3
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
To
tal
99
.57
99
.95
10
0.2
9
99
.70
98
.78
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
S
i 3
3.0
1
33
.02
32
.89
32
.79
32
.79
Ti
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
Al
0.1
0
0.0
5
0.0
7
0.0
9
0.0
1
Fe
8.2
7
8.3
8
8.2
9
8.1
7
8.2
9
Mn
1.1
7
1.2
0
1.0
7
1.1
1
1.1
8
Mg
56
.97
56
.85
57
.17
57
.33
57
.21
Ca
0.2
9
0.3
0
0.3
0
0.3
0
0.3
0
Ni
0.2
0
0.2
0
0.2
0
0.2
1
0.2
1
Cr
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
Fo
con
ten
t (%
) 8
7.3
8
7.2
8
7.3
8
7.5
8
7.3
Lo
ng a
xis
(x1
0-6
m)
18
0
48
0
S
ho
rt a
xis
(x1
0-6
m)
13
0
37
0
A
spec
t ra
tio
1.4
1.3
91
Table 2 Pillow margin matrix glass geochemistry. Major and minor elements
analyzed by electron microprobe. Uncertainty was below 1% for major elements,
checked by analyzing standards. All Fe as FeO*. Concentrations are averages of
at least five analyses.
92
Pil
low
mar
gin
mat
rix g
lass
Sam
ple
P
d13
Pd
19
v1
Pd
19
v2
Pd
56
PI1
6
PI1
7v1
PI1
7v2
PI1
7i
Db
13
Db
14
Db
15
Db
15
i A
k2
A
k1
1a
Ak1
2
Ak1
2i
Typ
e
N
N
N
N
N
E
E
E
N
N
N
N
N
N
N
N
(wt
%)
SiO
2
48
.41
48
.68
48
.42
49
.21
48
.61
48
.46
49
.12
49
.35
49
.50
49
.02
49
.64
49
.02
49
.23
49
.23
49
.28
48
.53
MgO
8.4
9
9.0
2
9.2
7
9.3
7
9.0
3
9.3
8
8.4
9
8.4
3
8.6
9
8.7
3
8.7
4
8.7
0
9.2
6
9.2
3
9.1
1
9.0
2
Mn
O
0
.26
0.1
7
0.1
6
0.2
2
0.1
7
0.2
0
0.1
8
0.1
5
0.1
7
0.1
7
0.1
7
0.1
8
0.1
6
0.1
6
0.1
5
0.1
6
CaO
17
.54
13
.58
13
.39
15
.29
13
.45
13
.06
13
.18
13
.29
13
.67
13
.59
13
.67
13
.61
13
.39
13
.47
13
.52
13
.43
FeO
*
10
.09
9.5
5
9.4
4
10
.11
9.4
5
11
.15
9.6
8
9.7
5
9.9
1
9.8
2
9.7
7
9.7
2
9.3
4
9.4
4
9.4
5
9.3
0
Al 2
O3
11
.44
15
.04
15
.12
11
.93
15
.03
12
.84
14
.45
14
.71
14
.76
14
.72
14
.71
14
.89
15
.57
15
.61
15
.58
15
.82
TiO
2
1
.24
1.1
1
1.0
9
1.6
6
1.0
6
1.4
6
1.1
9
1.3
6
1.2
1
1.1
8
1.1
5
1.2
1
0.9
4
0.9
4
0.9
7
1.0
4
Na 2
O
1
.52
2.5
3
2.3
8
2.5
7
2.5
9
2.7
6
2.5
9
1.9
5
1.8
4
2.4
8
1.8
5
1.9
4
1.7
4
1.7
6
1.7
7
1.8
5
K2O
0.0
6
0.0
8
0.0
7
0.0
8
0.0
8
0.1
8
0.2
1
0.2
3
0.1
0
0.0
8
0.1
0
0.1
0
0.0
9
0.0
9
0.0
9
0.0
9
P2O
5
0.0
3
0.1
0
0.1
1
0.2
9
0.0
9
0.1
3
0.1
1
0.1
0
0.1
0
0.2
1
0.1
1
0.1
0
0.1
8
C
r 2O
3
0.0
7
0.0
5
0.0
4
0.0
6
0.0
5
0.0
6
0.0
4
To
tal
9
9.2
2
99
.86
99
.45
10
0.7
2
99
.57
99
.62
99
.20
99
.30
99
.97
99
.91
10
0.0
8
99
.42
99
.91
10
0.1
0
10
0.2
0
99
.32
Cl
(pp
m)
10
75
47
38
70
17
20
20
45
S (
pp
m)
0
6
47
35
14
63
69
81
80
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
S
i 4
4.9
5
44
.41
44
.37
44
.61
44
.43
44
.39
45
.22
45
.73
45
.51
44
.83
45
.59
45
.23
45
.15
45
.05
45
.12
44
.74
Mg
11
.75
12
.27
12
.66
12
.66
12
.30
12
.81
11
.65
11
.65
11
.91
11
.91
11
.97
11
.97
12
.67
12
.60
12
.44
12
.40
Mn
1.8
1
1.1
9
1.1
2
1.5
2
1.2
0
1.3
7
1.2
2
1.0
8
1.1
8
1.1
7
1.1
8
1.2
4
1.1
1
1.1
4
1.0
7
1.0
9
Ca
17
.45
13
.28
13
.15
14
.86
13
.17
12
.82
12
.99
13
.19
13
.47
13
.32
13
.45
13
.45
13
.16
13
.21
13
.26
13
.27
Fe
7.8
3
7.2
8
7.2
3
7.6
6
7.2
3
8.5
4
7.4
5
7.5
5
7.6
2
7.5
1
7.5
0
7.5
0
7.1
6
7.2
3
7.2
4
7.1
7
Al
12
.52
16
.17
16
.33
12
.75
16
.19
13
.86
15
.68
16
.06
15
.99
15
.87
15
.93
16
.19
16
.83
16
.83
16
.82
17
.19
Ti
0.8
7
0.7
7
0.7
5
1.1
3
0.7
3
1.0
0
0.8
2
0.9
5
0.8
4
0.8
1
0.8
0
0.8
4
0.6
5
0.6
4
0.6
7
0.7
2
Na
2.7
4
4.4
7
4.2
2
4.5
1
4.5
9
4.9
0
4.6
3
3.5
1
3.2
9
4.4
0
3.3
0
3.4
7
3.0
9
3.1
2
3.1
4
3.3
1
K
0.0
7
0.0
9
0.0
8
0.0
9
0.0
9
0.2
1
0.2
5
0.2
7
0.1
1
0.1
0
0.1
1
0.1
2
0.1
1
0.1
0
0.1
0
0.1
1
P
0.0
2
0.0
7
0.0
8
0.2
2
0.0
7
0.1
0
0.0
9
0.0
0
0.0
8
0.0
8
0.1
6
0.0
0
0.0
8
0.0
8
0.1
4
0.0
0
Cr
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
5
0.0
0
0.0
0
0.0
4
0.0
3
0.0
4
0.0
4
0.0
4
0.0
3
K/T
i
0.0
8
0.1
2
0.1
1
0.0
8
0.1
2
0.2
1
0.3
0
0.2
9
0.1
3
0.1
2
0.1
4
0.1
4
0.1
7
0.1
6
0.1
6
0.1
5
93
Table 3 Melt inclusion geochemistry. Major and minor elements analyzed by
electron microprobe. Uncertainty was below 1% for major elements, checked by
analyzing standards. All Fe as FeO*.
94
Mel
t in
clu
sion
s
S
amp
le
Pd
13
/1
Pd
13
/2.1
P
d13
/2.2
P
d13
/3
Pd
13
/4
Pd
13
/6
Pd
13
/7.1
P
d13
/8
Pd
13
/10
Pd
13
/i1
2
Pd
13
/i1
5
Pd
13
/i1
8.1
P
d13
/i1
8.2
P
d19
/1
Typ
e
N
N
N
N
N
E
N
N
N
N
N
N
N
N
(wt
%)
SiO
2
51
.69
52
.06
50
.94
50
.74
51
.56
51
.57
51
.30
50
.93
51
.04
51
.48
49
.92
50
.03
50
.05
49
.36
MgO
2.5
6
2.6
5
2.9
2
3.6
4
3.0
6
4.9
6
3.5
7
2.9
6
3.7
5
4.1
1
4.2
1
4.1
2
3.2
9
7.2
7
Mn
O
0
.12
0.1
4
0.1
9
0.1
1
0.1
3
0.1
1
0.1
2
0.1
1
0.1
1
0.1
2
0.1
3
0.1
8
0.1
4
0.1
8
CaO
16
.93
16
.56
16
.95
16
.52
16
.01
15
.57
16
.52
16
.71
16
.32
16
.00
15
.79
16
.11
16
.21
14
.26
FeO
*
5.5
2
5.8
7
6.1
4
7.3
9
6.7
6
6.6
5
7.1
4
6.8
9
7.5
1
7.3
3
7.0
9
7.9
2
6.9
4
9.5
4
Al 2
O3
19
.09
19
.63
18
.62
18
.12
18
.82
17
.93
18
.05
18
.55
18
.03
17
.94
17
.80
17
.29
17
.93
15
.95
TiO
2
1
.21
1.4
0
1.2
2
1.3
7
1.3
5
1.0
0
1.3
2
1.2
9
1.2
9
1.5
3
1.2
3
1.3
9
1.2
8
1.1
6
Na 2
O
2
.17
2.2
7
1.9
8
1.9
6
2.2
3
2.2
4
1.9
4
2.0
1
1.9
9
2.1
0
1.9
3
1.9
7
2.0
2
2.8
6
K2O
0.1
4
0.1
1
0.1
1
0.1
5
0.1
1
0.1
2
0.1
1
0.1
2
0.1
2
0.1
1
0.1
4
0.1
1
0.1
3
0.0
7
P2O
5
0.1
4
0.1
3
0.1
1
0.1
4
0.1
1
0.1
5
0.1
1
0.1
3
0.1
2
0.0
7
Cr 2
O3
0.0
6
0.0
4
0.0
9
0.0
7
T
ota
l
99
.71
10
0.9
8
99
.34
10
0.2
1
10
0.2
9
10
0.3
7
10
0.2
1
99
.83
10
0.3
8
10
0.7
9
98
.31
99
.30
98
.15
10
0.7
1
Cl
(pp
m)
10
0
50
80
70
50
40
50
40
20
29
21
23
12
S
(pp
m)
45
3
30
0
22
0
36
16
0
52
72
28
8
11
2
77
10
2
38
5
10
2
C
atio
ns
pro
po
rtio
ns
(100
cat
ion
s)
S
i 4
8.2
8
47
.97
47
.64
47
.25
47
.89
47
.51
47
.75
47
.66
47
.44
47
.53
47
.16
46
.86
47
.49
44
.81
Mg
3.5
6
3.6
4
4.0
7
5.0
6
4.2
4
6.8
2
4.9
6
4.1
2
5.2
0
5.6
6
5.9
2
5.7
5
4.6
5
9.8
4
Mn
0.8
4
0.9
4
1.3
1
0.7
9
0.8
9
0.7
6
0.8
1
0.8
1
0.8
0
0.8
6
0.9
4
1.2
5
1.0
3
1.2
3
Ca
16
.95
16
.35
16
.99
16
.48
15
.93
15
.36
16
.48
16
.75
16
.25
15
.82
15
.98
16
.17
16
.48
13
.87
Fe
4.3
1
4.5
2
4.8
0
5.7
6
5.2
6
5.1
2
5.5
6
5.3
9
5.8
3
5.6
6
5.6
0
6.2
1
5.5
0
7.2
4
Al
21
.02
21
.31
20
.53
19
.88
20
.61
19
.47
19
.80
20
.46
19
.75
19
.52
19
.82
19
.08
20
.05
17
.06
Ti
0.8
5
0.9
7
0.8
6
0.9
6
0.9
4
0.6
9
0.9
2
0.9
1
0.9
0
1.0
6
0.8
7
0.9
8
0.9
2
0.7
9
Na
3.9
2
4.0
5
3.5
9
3.5
4
4.0
2
4.0
0
3.5
0
3.6
4
3.5
9
3.7
7
3.5
3
3.5
7
3.7
2
5.0
3
K
0.1
7
0.1
3
0.1
4
0.1
8
0.1
2
0.1
4
0.1
3
0.1
5
0.1
4
0.1
3
0.1
7
0.1
3
0.1
5
0.0
8
P
0.1
1
0.1
0
0.0
9
0.1
1
0.0
9
0.1
2
0.0
9
0.1
0
0.0
9
0.0
0
0.0
0
0.0
0
0.0
0
0.0
5
Cr
0.0
5
0.0
3
0.0
7
0.0
5
K
/Ti
0
.19
0.1
4
0.1
6
0.1
9
0.1
3
0.2
1
0.1
4
0.1
6
0.1
6
0.1
2
0.1
9
0.1
3
0.1
7
0.1
0
Cl/
K
0.0
6
0.0
4
0.0
6
0.0
4
0.0
4
0.0
3
0.0
4
0.0
3
0.0
1
0.0
2
0.0
1
0.0
2
0.0
1
0.0
0
95
Mel
t in
clu
sion
s co
nti
nu
ed
S
amp
le
Pd
19
/2
Pd
19
/4
Pd
19
/5
Pd
19
/7
Pd
19
/8
Pd
19
/9
Pd
19
/13
Pd
19
/i3
a
Pd
19
/i6
.1
Pd
19
/i6
.2
Pd
19
/i1
1
Pd
56
/1
Pd
56
/2
PI1
2/1
P
I12
/2
Typ
e
N
N
N
N
E
E
E
N
N
N
N
N
N
E
E
(wt
%)
S
iO2
49
.12
49
.12
49
.71
49
.55
51
.02
51
.28
50
.87
49
.94
50
.95
50
.42
50
.88
49
.84
49
.40
48
.45
47
.82
MgO
5.9
0
6.4
6
4.9
6
4.7
7
2.9
1
3.2
0
2.8
1
3.3
9
3.0
2
3.1
1
4.0
0
6.1
3
7.5
2
5.9
8
7.5
2
Mn
O
0
.16
0.1
9
0.1
8
0.1
4
0.1
4
0.0
9
0.1
6
0.1
5
0.1
8
0.1
7
0.0
8
0.1
8
0.1
6
0.1
5
0.1
9
CaO
15
.04
14
.90
15
.78
15
.68
15
.73
15
.84
15
.34
16
.53
16
.43
16
.85
17
.14
13
.93
13
.29
14
.21
13
.40
FeO
*
8.6
3
8.9
5
9.3
4
8.0
9
8.5
7
8.2
1
8.8
7
7.6
7
7.4
4
7.8
1
6.1
7
10
.49
10
.19
11
.06
10
.82
Al 2
O3
16
.29
16
.11
16
.80
16
.92
17
.13
17
.57
17
.56
17
.20
17
.24
17
.46
18
.25
14
.84
14
.75
14
.45
15
.12
TiO
2
1
.23
1.1
4
1.2
5
1.2
6
1.4
8
1.1
9
1.2
0
1.5
7
1.2
0
1.1
0
1.3
1
1.5
8
1.5
5
1.6
1
1.2
9
Na 2
O
2
.28
2.2
5
2.5
3
2.3
4
2.2
0
1.8
3
2.4
7
1.9
5
2.1
5
2.1
1
2.1
7
3.2
9
3.2
6
1.9
5
1.9
7
K2O
0.0
7
0.0
9
0.0
8
0.0
8
0.1
9
0.2
2
0.2
2
0.1
2
0.0
8
0.1
1
0.1
4
0.1
7
0.1
7
0.2
2
0.2
0
P2O
5
0.1
1
0.1
1
0.0
5
0.1
6
0.1
6
0.1
3
0.1
6
0.1
5
0.1
5
0.1
3
0.1
2
Cr 2
O3
0.0
8
0.0
6
0.0
3
0.0
6
0.0
4
0.0
3
To
tal
9
8.8
4
99
.33
10
0.6
6
98
.98
99
.67
99
.84
99
.92
98
.63
98
.82
99
.23
10
0.2
4
10
0.6
0
10
0.4
4
98
.29
98
.54
Cl
(pp
m)
13
0
12
0
14
0
64
15
23
1
20
0
20
0
S (
pp
m)
27
6
88
9
78
9
11
2
9
15
1
1
16
0
19
6
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
Si
45
.82
45
.45
45
.63
46
.35
47
.95
48
.32
47
.57
47
.27
48
.01
47
.33
47
.16
45
.55
44
.99
45
.97
44
.77
Mg
8.2
1
8.9
1
6.7
8
6.6
5
4.0
8
4.4
9
3.9
2
4.7
9
4.2
5
4.3
5
5.5
2
8.3
6
10
.22
8.4
6
10
.50
Mn
1.1
5
1.3
4
1.2
4
0.9
6
1.0
1
0.6
6
1.1
3
1.1
0
1.2
8
1.1
9
0.5
8
1.2
2
1.1
1
1.1
1
1.3
1
Ca
15
.03
14
.78
15
.51
15
.72
15
.84
15
.99
15
.37
16
.76
16
.59
16
.95
17
.02
13
.64
12
.96
14
.45
13
.44
Fe
6.7
3
6.9
3
7.1
7
6.3
3
6.7
3
6.4
7
6.9
3
6.0
7
5.8
6
6.1
3
4.7
9
8.0
2
7.7
6
8.7
7
8.4
7
Al
17
.90
17
.57
18
.17
18
.65
18
.98
19
.51
19
.36
19
.18
19
.15
19
.32
19
.94
15
.98
15
.83
16
.15
16
.69
Ti
0.8
7
0.7
9
0.8
6
0.8
9
1.0
4
0.8
4
0.8
4
1.1
2
0.8
5
0.7
8
0.9
1
1.0
8
1.0
6
1.1
5
0.9
1
Na
4.1
2
4.0
4
4.5
0
4.2
4
4.0
1
3.3
4
4.4
8
3.5
7
3.9
2
3.8
4
3.9
1
5.8
4
5.7
6
3.5
8
3.5
7
K
0.0
9
0.1
0
0.0
9
0.0
9
0.2
3
0.2
7
0.2
6
0.1
4
0.0
9
0.1
3
0.1
6
0.2
0
0.1
9
0.2
6
0.2
4
P
0.0
8
0.0
9
0.0
4
0.1
2
0.1
3
0.1
1
0.1
2
0.0
0
0.0
0
0.0
0
0.0
0
0.1
2
0.1
1
0.1
0
0.1
0
Cr
0.0
6
0.0
5
0.0
2
0.0
5
K/T
i
0.1
0
0.1
3
0.1
1
0.1
0
0.2
2
0.3
2
0.3
1
0.1
2
0.1
1
0.1
6
0.1
8
0.1
8
0.1
8
0.2
3
0.2
6
Cl/
K
0.0
0
0.0
0
0.0
0
0.0
0
0.0
6
0.0
4
0.0
5
0.0
5
0.0
2
0.0
2
0.0
0
0.0
0
0.0
0
0.0
8
0.0
8
96
Mel
t in
clu
sion
s co
nti
nu
ed
S
amp
le
PI1
2/3
P
I12
/4
PI1
2/6
P
I12
/7
PI1
2/8
P
I12
/9
PI1
4/1
P
I14
/2
PI1
4/4
P
I14
/5
PI1
4/6
P
I14
/7
PI1
4/8
P
I14
/9
PI1
4/1
1
Typ
e
E
E
E
E
E
E
N
N
N
N
N
N
N
N
N
(wt
%)
S
iO2
48
.73
48
.26
48
.61
48
.38
49
.52
48
.64
48
.82
49
.25
48
.57
48
.50
48
.72
48
.49
48
.43
48
.34
49
.24
MgO
6.3
0
6.5
6
6.0
3
5.5
4
5.6
4
6.1
7
6.9
0
6.8
3
6.7
5
8.0
3
8.3
6
8.3
9
8.6
8
8.5
0
8.7
3
Mn
O
0
.20
0.1
8
0.1
8
0.2
1
0.2
0
0.2
1
0.1
5
0.1
6
0.1
5
0.1
7
0.1
4
0.1
0
0.1
4
0.1
5
0.1
6
CaO
13
.78
14
.10
14
.66
14
.39
14
.44
14
.15
14
.35
14
.76
14
.64
14
.25
14
.10
14
.06
14
.08
13
.87
13
.41
FeO
*
11
.30
9.6
5
10
.28
11
.07
11
.03
10
.62
8.6
6
9.0
4
9.2
5
10
.00
8.6
2
9.0
2
8.8
3
9.4
4
8.2
2
Al 2
O3
14
.27
15
.81
15
.69
15
.80
14
.26
15
.51
16
.07
16
.16
16
.20
15
.34
15
.68
15
.71
15
.57
15
.28
15
.52
TiO
2
1
.57
1.2
8
1.3
1
1.2
4
1.6
0
1.3
6
1.1
6
1.2
0
1.1
0
1.1
9
1.1
6
1.1
6
1.1
2
1.1
8
1.0
4
Na 2
O
2
.05
2.0
0
1.9
1
1.9
9
2.0
7
1.9
8
2.8
7
2.7
9
1.8
7
1.7
4
1.8
0
1.8
0
1.8
3
1.7
6
1.9
4
K2O
0.2
1
0.2
1
0.1
8
0.2
0
0.2
1
0.1
9
0.0
8
0.0
6
0.1
0
0.0
9
0.1
0
0.1
1
0.1
2
0.0
9
0.1
1
P2O
5
0.1
4
0.1
6
0.1
4
0.1
5
0.1
4
0.1
5
0.1
1
0.0
8
0.1
2
0.1
0
0.1
3
0.0
9
0.1
0
0.0
9
0.1
2
Cr 2
O3
0.0
6
0.0
4
0.0
6
0.0
8
0.0
5
0.0
6
0.0
8
0.0
7
0.0
6
0.0
5
0.0
7
0.0
7
0.0
8
To
tal
9
8.6
4
98
.35
99
.29
99
.19
99
.20
99
.12
99
.16
10
0.3
3
98
.86
99
.51
98
.99
99
.01
99
.01
98
.78
98
.62
Cl
(pp
m)
20
0
17
0
40
0
15
0
19
0
18
5
10
35
20
10
10
20
10
S (
pp
m)
10
0
31
2
82
4
50
8
13
6
31
8
13
6
66
48
0
13
6
19
2
66
23
2
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
Si
45
.89
45
.32
45
.52
45
.35
46
.48
45
.47
45
.04
44
.96
45
.41
44
.93
45
.26
45
.12
44
.90
45
.00
45
.69
Mg
8.8
4
9.1
8
8.4
1
7.7
4
7.8
9
8.5
9
9.4
9
9.2
9
9.4
1
11
.09
11
.58
11
.63
12
.00
11
.79
12
.08
Mn
1.4
1
1.3
0
1.2
6
1.4
8
1.4
3
1.4
9
1.0
3
1.1
3
1.0
3
1.1
8
1.0
1
0.7
2
0.9
6
1.0
8
1.1
0
Ca
13
.90
14
.18
14
.71
14
.46
14
.52
14
.17
14
.19
14
.44
14
.67
14
.15
14
.03
14
.01
13
.99
13
.83
13
.33
Fe
8.9
0
7.5
8
8.0
5
8.6
8
8.6
6
8.3
0
6.6
8
6.9
0
7.2
4
7.7
5
6.7
0
7.0
2
6.8
5
7.3
5
6.3
8
Al
15
.84
17
.50
17
.32
17
.46
15
.77
17
.09
17
.47
17
.39
17
.85
16
.75
17
.17
17
.23
17
.01
16
.77
16
.98
Ti
1.1
1
0.9
0
0.9
2
0.8
7
1.1
3
0.9
6
0.8
0
0.8
3
0.7
7
0.8
3
0.8
1
0.8
1
0.7
8
0.8
2
0.7
2
Na
3.7
4
3.6
4
3.4
7
3.6
1
3.7
7
3.5
8
5.1
3
4.9
4
3.4
0
3.1
3
3.2
5
3.2
5
3.2
8
3.1
7
3.5
0
K
0.2
5
0.2
6
0.2
2
0.2
4
0.2
5
0.2
2
0.0
9
0.0
6
0.1
2
0.1
1
0.1
1
0.1
3
0.1
4
0.1
1
0.1
3
P
0.1
1
0.1
3
0.1
1
0.1
2
0.1
1
0.1
2
0.0
8
0.0
6
0.0
9
0.0
8
0.1
0
0.0
7
0.0
8
0.0
7
0.0
9
Cr
K
/Ti
0
.22
0.2
8
0.2
4
0.2
8
0.2
2
0.2
3
0.1
1
0.0
8
0.1
6
0.1
3
0.1
4
0.1
6
0.1
8
0.1
3
0.1
8
Cl/
K
0.0
8
0.0
7
0.1
8
0.0
6
0.0
8
0.0
8
0.0
0
0.0
0
0.0
1
0.0
3
0.0
2
0.0
1
0.0
1
0.0
2
0.0
1
97
Mel
t in
clu
sion
s co
nti
nu
ed
Sam
ple
P
I14
/13
PI1
4/1
4
PI1
4/1
5
PI1
4/1
6
PI1
4/1
7
PI1
4/1
8
PI1
4/1
9.1
P
I14
/19.2
P
I16
/1
PI1
6/2
P
I16
/3
PI1
6/4
.1
PI1
6/4
.2
PI1
6/5
.1
Typ
e
N
N
N
N
N
N
N
N
N
N
N
N
N
N
(wt
%)
SiO
2
48
.98
48
.63
48
.90
48
.40
48
.38
49
.10
49
.09
49
.69
49
.02
49
.33
49
.29
49
.84
49
.01
49
.77
MgO
6.3
2
7.9
0
7.3
6
8.7
9
8.1
9
6.5
7
5.3
5
5.1
1
9.2
5
8.1
4
7.8
0
6.5
0
7.0
7
7.4
7
Mn
O
0
.15
0.1
3
0.1
5
0.1
6
0.1
0
0.1
6
0.1
6
0.1
5
0.1
6
0.1
8
0.1
9
0.1
7
0.1
9
0.1
6
CaO
15
.04
14
.12
14
.42
13
.57
14
.24
14
.41
15
.32
15
.54
13
.14
14
.06
14
.11
14
.20
14
.33
14
.15
FeO
*
9.0
0
9.1
7
8.7
2
9.6
6
9.9
1
9.6
8
8.0
7
7.9
9
9.5
9
9.6
7
9.7
4
9.2
8
9.6
9
9.9
9
Al 2
O3
15
.88
15
.62
16
.15
15
.12
15
.46
15
.91
16
.94
17
.10
15
.24
15
.31
15
.48
16
.34
15
.76
15
.95
TiO
2
1
.10
1.2
9
1.1
3
1.2
1
1.1
9
1.2
1
1.2
4
1.2
1
1.0
3
1.0
9
1.1
4
1.1
7
1.2
3
1.0
9
Na 2
O
1
.77
1.8
5
1.8
2
1.7
9
1.7
6
1.8
5
1.8
5
1.9
1
2.7
5
2.7
8
2.7
3
3.1
7
2.7
8
3.1
3
K2O
0.0
9
0.1
0
0.1
0
0.0
9
0.0
9
0.1
0
0.1
0
0.1
0
0.0
7
0.0
6
0.0
7
0.0
9
0.0
8
0.0
7
P2O
5
0.1
1
0.0
9
0.1
0
0.0
9
0.1
3
0.1
0
0.1
2
0.1
0
0.1
1
0.1
0
0.0
6
0.0
8
0.1
0
0.0
9
Cr 2
O3
0.0
6
0.0
6
0.0
7
0.0
6
0.0
7
0.0
4
0.0
9
0.0
6
To
tal
9
8.5
3
98
.96
98
.92
98
.93
99
.54
99
.15
98
.39
98
.98
10
0.3
5
10
0.5
5
10
0.6
0
10
0.8
5
10
0.2
3
10
1.8
7
Cl
(pp
m)
30
25
43
50
20
50
50
40
S (
pp
m)
15
2
30
35
8
69
60
18
0
96
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
S
i 4
6.0
4
45
.28
45
.54
44
.94
44
.93
45
.85
46
.24
46
.55
44
.43
44
.70
44
.76
45
.19
44
.76
44
.64
Mg
8.8
6
10
.97
10
.22
12
.16
11
.35
9.1
4
7.5
1
7.1
3
12
.50
10
.99
10
.56
8.7
9
9.6
3
9.9
8
Mn
1.0
8
0.9
4
1.0
5
1.1
2
0.7
2
1.1
2
1.1
4
1.0
6
1.0
8
1.2
1
1.2
9
1.1
8
1.2
9
1.1
0
Ca
15
.15
14
.09
14
.40
13
.50
14
.17
14
.42
15
.46
15
.60
12
.76
13
.65
13
.73
13
.80
14
.03
13
.60
Fe
7.0
7
7.1
4
6.7
9
7.5
0
7.7
0
7.5
6
6.3
6
6.2
6
7.2
7
7.3
3
7.3
9
7.0
4
7.4
0
7.4
9
Al
17
.59
17
.14
17
.73
16
.54
16
.92
17
.51
18
.80
18
.89
16
.27
16
.35
16
.57
17
.46
16
.96
16
.86
Ti
0.7
8
0.9
0
0.7
9
0.8
4
0.8
3
0.8
5
0.8
8
0.8
5
0.7
1
0.7
4
0.7
8
0.8
0
0.8
4
0.7
4
Na
3.2
3
3.3
3
3.2
9
3.2
2
3.1
7
3.3
6
3.3
9
3.4
7
4.8
3
4.8
9
4.8
0
5.5
7
4.9
3
5.4
4
K
0.1
0
0.1
2
0.1
2
0.1
0
0.1
1
0.1
2
0.1
2
0.1
1
0.0
8
0.0
7
0.0
8
0.1
0
0.0
9
0.0
8
P
0.0
8
0.0
7
0.0
8
0.0
7
0.1
0
0.0
8
0.1
0
0.0
8
0.0
8
0.0
8
0.0
5
0.0
6
0.0
8
0.0
7
Cr
K/T
i
0.1
3
0.1
3
0.1
5
0.1
2
0.1
3
0.1
4
0.1
4
0.1
3
0.1
1
0.1
0
0.1
0
0.1
3
0.1
1
0.1
2
Cl/
K
0.0
3
0.0
2
0.0
4
0.0
5
0.0
2
0.0
4
0.0
4
0.0
4
0.0
0
0.0
0
0.0
0
0.0
0
98
Mel
t in
clu
sion
s co
nti
nu
ed
Sam
ple
P
I16
/5.2
P
I17
/3
PI1
7/5
.1
PI1
7/5
.2
PI1
7/6
.1
PI1
7/6
.2
PI1
7/7
.1
PI1
7/7
.2
PI1
7/8
.1
PI1
7/8
.2
PI1
7/9
.1
PI1
7/9
.2
PI1
7/1
0.1
P
I17
/10.2
Typ
e
N
E
E
E
E
E
E
E
E
E
E
E
E
E
(wt
%)
SiO
2
49
.76
49
.34
49
.77
49
.26
49
.35
49
.11
48
.92
48
.95
49
.18
49
.65
49
.32
48
.82
50
.93
50
.49
MgO
8.9
7
7.1
4
8.3
8
8.0
2
8.4
4
8.4
0
8.5
8
8.1
6
8.3
6
7.0
5
8.0
3
7.4
3
7.9
9
7.7
4
Mn
O
0
.17
0.1
4
0.1
7
0.1
4
0.1
9
0.1
4
0.1
8
0.1
3
0.1
7
0.1
4
0.1
8
0.1
9
0.1
4
0.1
7
CaO
14
.67
13
.86
13
.21
12
.35
13
.15
13
.19
13
.04
13
.01
13
.06
13
.39
13
.46
13
.57
12
.42
13
.60
FeO
*
8.6
0
9.7
4
9.7
7
9.0
5
9.6
3
8.7
5
9.8
0
9.0
0
9.3
7
8.7
7
9.8
5
9.4
3
8.0
1
8.4
1
Al 2
O3
15
.57
14
.71
15
.08
15
.64
14
.84
15
.93
14
.89
16
.15
14
.98
16
.56
14
.80
15
.64
15
.88
15
.88
TiO
2
1
.11
1.1
9
1.2
8
1.3
4
1.2
7
1.1
1
1.2
1
1.1
0
1.1
2
1.0
1
1.2
1
1.0
3
1.1
4
1.1
2
Na 2
O
2
.74
3.3
7
3.5
8
3.8
7
3.4
4
3.3
9
3.4
0
3.4
2
3.4
2
3.8
1
3.3
4
3.3
0
3.0
4
2.6
3
K2O
0.0
4
0.2
0
0.2
2
0.4
1
0.2
1
0.1
9
0.2
3
0.1
9
0.2
0
0.2
0
0.1
9
0.1
9
0.4
1
0.2
2
P2O
5
0.1
1
0.1
1
0.1
1
0.1
4
0.1
1
0.1
0
0.1
1
0.1
0
0.1
4
0.1
2
0.1
5
0.1
0
0.1
5
0.1
4
Cr 2
O3
To
tal
1
01.7
3
99
.79
10
1.5
5
10
0.2
3
10
0.6
3
10
0.3
0
10
0.3
6
10
0.1
9
10
0.0
0
10
0.7
1
10
0.5
2
99
.69
10
0.1
2
10
0.3
8
Cl
(pp
m)
S (
pp
m)
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
S
i 4
4.4
5
45
.20
44
.48
44
.52
44
.47
44
.38
44
.20
44
.35
44
.60
44
.75
44
.64
44
.52
46
.27
45
.92
Mg
11
.94
9.7
6
11
.16
10
.81
11
.33
11
.31
11
.55
11
.02
11
.30
9.4
7
10
.83
10
.10
10
.82
10
.49
Mn
1.1
4
0.9
8
1.1
3
0.9
2
1.2
8
0.9
8
1.2
5
0.8
9
1.1
7
0.9
6
1.2
1
1.3
0
0.9
9
1.1
5
Ca
14
.04
13
.61
12
.65
11
.96
12
.70
12
.77
12
.62
12
.63
12
.69
12
.93
13
.06
13
.25
12
.09
13
.25
Fe
6.4
2
7.4
6
7.3
1
6.8
4
7.2
6
6.6
2
7.4
0
6.8
2
7.1
1
6.6
1
7.4
5
7.1
9
6.0
9
6.3
9
Al
16
.40
15
.88
15
.88
16
.66
15
.76
16
.96
15
.85
17
.24
16
.01
17
.59
15
.79
16
.80
17
.01
17
.02
Ti
0.7
5
0.8
2
0.8
6
0.9
1
0.8
6
0.7
5
0.8
2
0.7
5
0.7
6
0.6
9
0.8
2
0.7
1
0.7
8
0.7
7
Na
4.7
4
5.9
8
6.2
1
6.7
9
6.0
1
5.9
3
5.9
6
6.0
0
6.0
2
6.6
6
5.8
7
5.8
3
5.3
6
4.6
4
K
0.0
4
0.2
3
0.2
5
0.4
7
0.2
4
0.2
2
0.2
6
0.2
2
0.2
3
0.2
3
0.2
1
0.2
2
0.4
8
0.2
5
P
0.0
8
0.0
8
0.0
8
0.1
1
0.0
9
0.0
7
0.0
8
0.0
8
0.1
0
0.0
9
0.1
2
0.0
8
0.1
2
0.1
1
Cr
K/T
i
0.0
5
0.2
8
0.2
9
0.5
2
0.2
8
0.2
9
0.3
2
0.2
9
0.3
1
0.3
4
0.2
6
0.3
1
0.6
1
0.3
3
Cl/
K
99
Mel
t in
clu
sion
s co
nti
nu
ed
Sam
ple
P
I17
/10.3
P
I17
/11
PI1
7/1
3
PI1
7/1
4.1
P
I17
/14.2
P
I17
/14.3
P
I17
/14.4
P
I17
/16
PI1
7/1
7
PI1
7/1
8
PI1
7/1
9
PI1
7/2
2
PI1
7/2
3
PI1
7/i
1
Typ
e
E
E
E
E
E
E
E
E
E
E
E
E
E
E
(wt
%)
SiO
2
51
.51
49
.83
50
.90
49
.65
49
.23
49
.65
49
.01
49
.59
49
.64
49
.83
50
.04
48
.63
50
.18
49
.23
MgO
7.9
9
8.1
3
7.5
7
8.4
3
8.4
7
8.5
3
8.1
2
8.6
2
7.7
1
7.2
9
7.1
4
7.5
3
6.2
5
8.2
7
Mn
O
0
.17
0.1
4
0.1
5
0.1
4
0.1
6
0.1
3
0.1
8
0.1
6
0.1
3
0.2
0
0.2
0
0.2
0
0.1
2
0.1
7
CaO
12
.34
13
.56
14
.32
13
.03
13
.32
13
.28
12
.81
13
.35
14
.06
13
.90
13
.89
13
.53
13
.95
13
.94
FeO
*
8.1
2
8.9
7
8.8
4
9.2
2
9.1
4
9.7
8
9.6
1
9.5
9
8.3
2
9.8
8
9.6
6
9.6
6
8.2
2
9.6
5
Al 2
O3
16
.15
15
.22
16
.17
15
.73
15
.60
14
.86
14
.68
14
.53
16
.15
14
.66
14
.81
14
.46
16
.48
15
.94
TiO
2
1
.10
1.1
1
0.9
9
1.2
0
1.1
3
1.1
8
1.2
2
1.1
7
1.0
8
1.2
5
1.1
9
1.1
5
1.1
9
1.1
2
Na 2
O
3
.13
2.5
2
2.3
7
2.6
9
2.6
3
2.5
3
2.2
9
2.5
2
2.5
5
2.5
9
2.6
7
2.3
4
2.6
6
1.8
7
K2O
0.3
8
0.1
9
0.1
3
0.2
8
0.1
6
0.1
7
0.2
0
0.2
0
0.1
7
0.1
8
0.1
7
0.1
9
0.1
8
0.1
5
P2O
5
0.1
0
0.0
7
0.1
0
0.1
9
0.1
1
0.1
2
0.0
9
0.1
5
0.1
4
0.1
4
0.1
3
0.0
9
0.1
0
C
r 2O
3
0.0
4
To
tal
1
00.9
9
99
.74
10
1.5
4
10
0.5
4
99
.94
10
0.2
2
98
.21
99
.86
99
.94
99
.90
99
.90
97
.78
99
.33
10
0.4
7
Cl
(pp
m)
25
S (
pp
m)
26
8
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
S
i 4
6.3
2
45
.73
45
.98
45
.11
44
.92
45
.40
45
.71
45
.40
45
.43
45
.75
45
.92
45
.56
46
.44
45
.05
Mg
10
.72
11
.13
10
.20
11
.41
11
.52
11
.63
11
.29
11
.76
10
.51
9.9
7
9.7
7
10
.51
8.6
3
11
.28
Mn
1.1
4
0.9
4
1.0
3
0.9
4
1.1
0
0.8
7
1.2
6
1.1
1
0.9
3
1.3
8
1.3
5
1.4
4
0.8
7
1.1
6
Ca
11
.89
13
.33
13
.86
12
.68
13
.02
13
.01
12
.80
13
.09
13
.78
13
.67
13
.66
13
.59
13
.83
13
.67
Fe
6.1
1
6.8
8
6.6
8
7.0
0
6.9
7
7.4
8
7.4
9
7.3
4
6.3
7
7.5
9
7.4
1
7.5
7
6.3
6
7.3
9
Al
17
.12
16
.46
17
.21
16
.84
16
.77
16
.02
16
.14
15
.68
17
.42
15
.86
16
.02
15
.97
17
.97
17
.19
Ti
0.7
5
0.7
7
0.6
8
0.8
2
0.7
7
0.8
1
0.8
5
0.8
0
0.7
4
0.8
7
0.8
2
0.8
1
0.8
3
0.7
7
Na
5.4
5
4.4
8
4.1
5
4.7
3
4.6
6
4.4
9
4.1
4
4.4
7
4.5
3
4.6
0
4.7
4
4.2
5
4.7
8
3.3
2
K
0.4
4
0.2
2
0.1
5
0.3
2
0.1
9
0.2
0
0.2
4
0.2
4
0.1
9
0.2
1
0.2
0
0.2
3
0.2
1
0.1
7
P
0.0
8
0.0
6
0.0
8
0.1
4
0.0
9
0.0
9
0.0
7
0.1
1
0.1
1
0.1
1
0.1
0
0.0
7
0.0
8
0.0
0
Cr
0.0
3
K/T
i
0.5
9
0.2
9
0.2
2
0.3
9
0.2
4
0.2
5
0.2
8
0.3
0
0.2
6
0.2
5
0.2
5
0.2
8
0.2
5
0.2
2
Cl/
K
100
Mel
t in
clu
sion
s co
nti
nu
ed
Sam
ple
P
I17
/i2
PI1
7/i
5
PI1
7/i
9.1
P
I17
/i9
.2
PI1
7/i
13
.1
PI1
7/i
13
.2
PI1
7/i
14
PI1
7/i
18
a P
I17
/i19
PI1
7/i
20
.1
PI1
7/i
20
.2
Db
13
/1
Db
13
/3
Db
13
/5.1
Typ
e
E
E
E
N
E
E
E
E
E
E
E
N
N
N
(wt
%)
SiO
2
49
.07
49
.54
49
.09
50
.31
49
.06
49
.54
51
.20
50
.18
49
.93
49
.58
49
.20
49
.29
49
.47
49
.02
MgO
6.2
3
5.6
0
7.4
9
8.0
0
7.3
5
7.5
8
4.6
2
6.7
4
5.5
6
6.1
3
5.8
2
8.4
9
7.7
9
7.1
1
Mn
O
0
.17
0.1
6
0.1
8
0.1
0
0.2
1
0.1
9
0.1
1
0.1
9
0.1
6
0.1
3
0.1
9
0.2
0
0.1
9
0.1
1
CaO
14
.71
15
.08
14
.07
13
.96
14
.18
13
.97
14
.98
14
.76
14
.86
14
.75
14
.71
13
.70
14
.65
14
.86
FeO
*
9.1
2
8.7
7
9.6
7
8.9
8
9.9
1
10
.30
7.7
9
8.6
0
9.0
3
8.9
3
9.3
9
10
.05
9.0
1
8.6
7
Al 2
O3
15
.87
16
.82
15
.49
15
.96
14
.70
14
.50
17
.16
16
.18
16
.91
16
.59
16
.39
14
.68
15
.97
15
.98
TiO
2
1
.26
1.2
3
0.9
9
1.1
0
1.3
8
1.3
2
1.1
3
1.2
6
1.4
0
1.1
4
1.1
6
1.1
6
1.1
0
1.2
3
Na 2
O
1
.85
1.8
9
1.8
9
1.9
6
1.8
4
1.8
2
2.3
6
1.9
7
2.0
5
1.9
7
1.9
0
1.8
6
1.6
9
1.8
0
K2O
0.1
8
0.2
0
0.1
2
0.1
1
0.2
1
0.2
3
0.1
4
0.1
7
0.2
4
0.1
9
0.2
0
0.1
1
0.0
9
0.0
9
P2O
5
0.0
9
0.0
7
0.1
1
Cr 2
O3
0.0
5
0.0
7
0.0
6
0.0
3
0.0
2
0.0
6
0.0
5
0.0
5
0.0
4
0.0
6
0.0
5
T
ota
l
98
.56
99
.40
99
.17
10
0.6
7
98
.88
99
.53
99
.69
10
0.1
8
10
0.2
5
99
.52
99
.09
99
.68
10
0.0
8
99
.07
Cl
(pp
m)
54
36
28
16
15
9
79
27
51
82
60
64
S
(pp
m)
14
5
85
41
2
43
7
24
0
56
51
5
38
8
19
0
16
0
16
3
C
atio
ns
pro
po
rtio
ns
(100
cat
ion
s)
S
i 4
6.0
6
46
.20
45
.62
46
.12
45
.73
45
.98
47
.71
46
.16
46
.17
46
.15
45
.97
45
.41
45
.45
45
.78
Mg
8.7
2
7.7
8
10
.38
10
.94
10
.21
10
.48
6.4
1
9.2
5
7.6
6
8.5
1
8.1
1
11
.67
10
.67
9.9
1
Mn
1.2
4
1.1
2
1.2
7
0.7
2
1.4
7
1.3
3
0.7
8
1.3
1
1.1
1
0.9
2
1.3
2
1.4
0
1.3
1
0.7
6
Ca
14
.79
15
.06
14
.01
13
.71
14
.16
13
.89
14
.95
14
.55
14
.72
14
.71
14
.73
13
.52
14
.42
14
.87
Fe
7.1
6
6.8
4
7.5
1
6.8
8
7.7
2
8.0
0
6.0
7
6.6
1
6.9
8
6.9
5
7.3
3
7.7
5
6.9
2
6.7
8
Al
17
.56
18
.49
16
.96
17
.25
16
.14
15
.86
18
.85
17
.54
18
.43
18
.20
18
.05
15
.94
17
.29
17
.59
Ti
0.8
9
0.8
6
0.6
9
0.7
6
0.9
7
0.9
2
0.7
9
0.8
7
0.9
7
0.8
0
0.8
2
0.8
0
0.7
6
0.8
6
Na
3.3
7
3.4
1
3.4
1
3.4
8
3.3
3
3.2
8
4.2
7
3.5
1
3.6
7
3.5
5
3.4
4
3.3
2
3.0
1
3.2
6
K
0.2
2
0.2
4
0.1
4
0.1
3
0.2
5
0.2
7
0.1
7
0.2
0
0.2
8
0.2
3
0.2
4
0.1
3
0.1
0
0.1
0
P
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
7
0.0
6
0.0
9
Cr
0.0
4
0.0
5
0.0
4
0.0
2
0.0
2
0.0
5
0.0
3
0.0
3
0.0
3
0.0
4
0.0
4
K
/Ti
0
.24
0.2
8
0.2
0
0.1
7
0.2
5
0.2
9
0.2
1
0.2
3
0.2
9
0.2
9
0.3
0
0.1
6
0.1
4
0.1
2
Cl/
K
101
Mel
t in
clu
sion
s co
nti
nu
ed
Sam
ple
D
b1
3/6
D
b1
3/7
D
b1
3/8
.2
Db
14
/1
Db
14
/3
Db
14
/5.2
D
b1
4/6
D
b1
4/7
.1
Db
14
/7.2
D
b1
4/9
D
b1
4/1
0.2
D
b1
4/1
2
Db
14
/13
Db
14
/14
Typ
e
N
N
N
N
N
N
N
N
N
N
N
N
N
N
(wt
%)
SiO
2
49
.35
48
.98
50
.14
49
.16
48
.77
48
.56
49
.44
48
.55
49
.37
49
.14
48
.28
48
.36
47
.93
49
.10
MgO
8.6
0
7.7
3
8.6
2
7.6
1
7.4
5
8.4
7
8.6
0
8.1
2
8.4
9
6.3
2
8.1
0
8.7
1
8.6
2
8.1
6
Mn
O
0
.12
0.1
9
0.1
3
0.1
6
0.1
8
0.1
6
0.1
5
0.1
6
0.1
7
0.1
1
0.1
8
0.1
5
0.1
2
0.1
6
CaO
13
.90
14
.36
14
.45
14
.47
14
.89
14
.05
13
.67
14
.53
13
.88
15
.18
14
.06
13
.72
13
.67
13
.79
FeO
*
10
.18
10
.25
6.2
9
8.9
0
9.0
5
9.2
2
9.7
7
9.0
3
9.7
6
9.1
6
9.7
7
9.4
7
9.1
3
9.1
9
Al 2
O3
14
.91
14
.61
16
.70
16
.10
16
.07
15
.86
14
.99
16
.03
14
.96
16
.30
15
.82
15
.97
15
.99
16
.11
TiO
2
1
.13
1.3
5
1.1
8
1.0
8
1.0
6
1.0
9
1.2
1
1.1
6
1.2
6
1.1
6
1.2
0
1.0
9
1.1
0
1.0
5
Na 2
O
1
.82
1.7
7
1.9
2
2.3
7
2.3
1
2.4
0
2.5
9
2.3
8
2.3
3
2.3
6
2.0
9
2.5
1
2.3
8
2.4
2
K2O
0.1
0
0.0
8
0.1
0
0.0
6
0.0
6
0.0
6
0.0
7
0.0
7
0.0
8
0.0
5
0.0
9
0.0
7
0.0
9
0.0
4
P2O
5
0.0
9
0.1
0
0.1
0
0.1
3
0.0
7
0.1
2
0.1
2
0.1
1
0.1
3
0.1
0
0.1
3
0.0
8
0.0
7
0.1
0
Cr 2
O3
To
tal
1
00.2
2
99
.43
99
.83
10
0.0
5
99
.91
99
.99
10
0.6
1
10
0.1
3
10
0.4
2
99
.90
99
.71
10
0.1
1
99
.09
10
0.1
2
Cl
(pp
m)
S (
pp
m)
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
S
i 4
5.4
1
45
.45
45
.92
45
.00
44
.69
44
.35
44
.95
44
.34
45
.02
45
.44
44
.38
44
.08
44
.20
44
.84
Mg
11
.80
10
.70
11
.77
10
.38
10
.18
11
.53
11
.66
11
.05
11
.55
8.7
1
11
.10
11
.84
11
.85
11
.11
Mn
0.8
6
1.3
5
0.8
9
1.1
2
1.2
6
1.1
0
1.0
1
1.0
7
1.1
8
0.7
7
1.2
7
1.0
0
0.8
6
1.0
7
Ca
13
.71
14
.28
14
.17
14
.19
14
.62
13
.75
13
.32
14
.22
13
.56
15
.04
13
.85
13
.40
13
.51
13
.50
Fe
7.8
4
7.9
5
4.8
2
6.8
1
6.9
3
7.0
4
7.4
3
6.9
0
7.4
4
7.0
8
7.5
1
7.2
2
7.0
4
7.0
1
Al
16
.17
15
.98
18
.03
17
.37
17
.36
17
.07
16
.07
17
.26
16
.08
17
.77
17
.14
17
.16
17
.38
17
.34
Ti
0.7
8
0.9
4
0.8
1
0.7
4
0.7
3
0.7
5
0.8
3
0.7
9
0.8
6
0.8
1
0.8
3
0.7
4
0.7
7
0.7
2
Na
3.2
5
3.1
8
3.4
1
4.2
1
4.1
0
4.2
4
4.5
6
4.2
1
4.1
1
4.2
4
3.7
3
4.4
3
4.2
5
4.2
9
K
0.1
2
0.0
9
0.1
1
0.0
7
0.0
7
0.0
7
0.0
8
0.0
8
0.0
9
0.0
6
0.1
0
0.0
8
0.1
0
0.0
5
P
0.0
7
0.0
8
0.0
8
0.1
0
0.0
5
0.0
9
0.0
9
0.0
9
0.1
0
0.0
8
0.1
0
0.0
6
0.0
5
0.0
7
Cr
K/T
i
0.1
5
0.1
0
0.1
4
0.1
0
0.1
0
0.1
0
0.1
0
0.1
0
0.1
1
0.0
8
0.1
2
0.1
0
0.1
3
0.0
7
Cl/
K
102
Mel
t in
clu
sion
s co
nti
nu
ed
Sam
ple
D
b1
4/1
5
Db
15
/1
Db
15
/2
Db
15
/3
Db
15
/4
Db
15
/5.1
D
b1
5/5
.2
Db
15
/5.3
D
b1
5/6
D
b1
5/7
.1
Db
15
/7.2
D
b1
5/8
D
b1
5/9
.1
Db
15
/9.2
Typ
e
N
N
N
N
N
N
N
N
N
N
N
N
N
N
(wt
%)
SiO
2
49
.27
49
.59
48
.74
48
.77
48
.73
49
.19
48
.92
48
.97
48
.80
49
.04
48
.78
49
.15
48
.45
48
.50
MgO
6.8
3
5.4
5
5.2
1
7.1
4
6.5
0
5.8
7
4.8
2
5.6
1
6.3
8
6.5
0
6.4
5
6.6
5
7.8
9
7.8
9
Mn
O
0
.13
0.1
8
0.2
1
0.1
1
0.1
7
0.1
7
0.1
9
0.1
4
0.1
4
0.1
4
0.1
4
0.1
9
0.1
4
0.1
8
CaO
14
.54
15
.13
15
.42
14
.86
15
.01
15
.43
15
.65
15
.34
14
.95
15
.03
15
.14
14
.84
14
.40
14
.36
FeO
*
8.7
5
9.6
1
9.3
4
8.9
9
9.4
9
9.1
9
9.1
1
8.8
7
9.5
0
9.3
9
9.0
6
10
.23
9.3
9
9.4
1
Al 2
O3
16
.71
15
.75
16
.41
15
.89
16
.09
16
.58
16
.97
16
.17
16
.14
16
.04
15
.86
15
.13
15
.61
15
.74
TiO
2
1
.13
1.3
0
1.1
8
1.3
0
1.1
9
1.1
8
1.2
0
1.1
8
1.2
5
1.0
8
1.2
8
1.3
2
1.2
0
1.1
2
Na 2
O
2
.39
2.0
2
1.8
1
1.8
4
1.7
5
1.8
4
1.9
5
1.8
2
1.8
2
1.8
5
1.7
8
1.9
0
1.7
4
1.8
1
K2O
0.0
8
0.1
1
0.1
0
0.0
8
0.0
9
0.1
0
0.0
9
0.0
9
0.0
8
0.0
9
0.0
8
0.0
8
0.0
8
0.0
7
P2O
5
0.0
8
0.1
0
0.1
2
0.1
0
0.1
1
0.1
2
0.1
1
0.1
0
0.0
8
0.0
7
0.1
1
0.0
9
0.0
7
0.1
0
Cr 2
O3
0.0
7
0.0
8
0.0
5
0.0
6
0.0
7
0.0
8
0.0
6
0.0
7
0.0
4
0.1
3
0.0
7
0.0
6
0.0
7
To
tal
9
9.9
1
99
.33
98
.67
99
.17
99
.22
99
.79
99
.23
98
.39
99
.25
99
.30
98
.85
99
.65
99
.09
99
.31
Cl
(pp
m)
65
70
20
40
40
10
40
40
40
50
35
20
50
S (
pp
m)
58
19
6
16
2
15
8
21
0
60
4
17
6
21
6
14
4
17
2
18
20
2
16
8
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
S
i 4
5.3
4
46
.36
45
.82
45
.50
45
.48
45
.68
45
.82
46
.25
45
.61
45
.73
45
.80
45
.65
45
.11
44
.91
Mg
9.3
7
7.6
0
7.3
0
9.9
3
9.0
4
8.1
2
6.7
3
7.8
9
8.8
9
9.0
3
9.0
3
9.2
1
10
.95
10
.89
Mn
0.9
0
1.2
4
1.4
8
0.8
1
1.1
8
1.2
1
1.3
1
0.9
7
1.0
0
0.9
9
0.9
7
1.3
5
0.9
8
1.2
8
Ca
14
.34
15
.15
15
.53
14
.85
15
.01
15
.35
15
.70
15
.52
14
.97
15
.02
15
.23
14
.77
14
.37
14
.25
Fe
6.7
3
7.5
2
7.3
4
7.0
2
7.4
1
7.1
4
7.1
3
7.0
0
7.4
2
7.3
2
7.1
2
7.9
5
7.3
2
7.2
9
Al
18
.12
17
.35
18
.18
17
.47
17
.70
18
.14
18
.73
18
.00
17
.77
17
.63
17
.54
16
.57
17
.13
17
.18
Ti
0.7
9
0.9
1
0.8
3
0.9
1
0.8
3
0.8
3
0.8
4
0.8
4
0.8
8
0.7
6
0.9
0
0.9
2
0.8
4
0.7
8
Na
4.2
6
3.6
6
3.3
0
3.3
3
3.1
7
3.3
2
3.5
4
3.3
3
3.2
9
3.3
5
3.2
3
3.4
2
3.1
5
3.2
5
K
0.1
0
0.1
3
0.1
2
0.1
0
0.1
0
0.1
2
0.1
0
0.1
1
0.1
0
0.1
1
0.0
9
0.0
9
0.0
9
0.0
9
P
0.0
6
0.0
8
0.0
9
0.0
8
0.0
8
0.0
9
0.0
9
0.0
8
0.0
6
0.0
6
0.0
9
0.0
7
0.0
6
0.0
8
Cr
0.0
5
0.0
6
0.0
4
0.0
5
0.0
5
0.0
6
0.0
4
0.0
5
0.0
3
0.1
0
0.0
5
0.0
4
0.0
5
K/T
i
0.1
2
0.1
4
0.1
4
0.1
1
0.1
2
0.1
4
0.1
2
0.1
3
0.1
1
0.1
4
0.1
0
0.1
0
0.1
1
0.1
1
Cl/
K
0
.05
0.0
6
0.0
2
0.0
4
0.0
3
0.0
1
0.0
4
0.0
4
0.0
4
0.0
5
0.0
4
0.0
2
0.0
6
103
Mel
t in
clu
sion
s co
nti
nu
ed
Sam
ple
D
b1
5/1
0
Db
15
/11
Db
15
/12
Db
15
/13
Db
15
/i7
Db
15
/i10
Db
15
/i12
Db
15
/i18
D
b1
5/i
26
.1
Ak2
/1
Ak2
/2
Ak2
/3
Ak2
/4.1
A
k2
/4.2
Typ
e
N
N
N
N
N
N
N
N
N
N
N
N
N
N
(wt
%)
SiO
2
48
.76
48
.83
48
.61
48
.69
50
.59
48
.33
49
.54
49
.38
47
.80
48
.28
48
.36
48
.41
48
.17
48
.30
MgO
8.1
4
6.9
7
7.3
6
8.2
4
3.9
5
4.7
3
4.8
8
7.6
3
7.3
3
8.6
2
9.1
6
8.5
9
9.3
8
9.2
2
Mn
O
0
.20
0.1
8
0.1
5
0.1
5
0.1
7
0.2
1
0.1
9
0.1
6
0.1
0
0.1
7
0.1
4
0.1
6
0.1
7
0.2
4
CaO
14
.01
14
.57
14
.41
13
.80
16
.17
15
.49
15
.69
14
.52
14
.42
13
.74
13
.09
13
.83
13
.37
13
.26
FeO
*
10
.05
9.9
8
10
.03
9.4
9
8.1
3
8.9
8
8.8
0
9.2
0
9.3
0
9.3
5
9.7
4
9.8
4
9.3
3
9.7
8
Al 2
O3
14
.87
15
.08
15
.09
15
.26
17
.62
16
.79
17
.07
16
.05
15
.88
16
.06
15
.55
15
.91
15
.67
15
.45
TiO
2
1
.24
1.2
0
1.2
7
1.2
0
1.0
1
1.2
2
1.2
0
0.8
9
1.1
6
0.9
8
1.0
4
0.9
6
0.9
9
0.8
5
Na 2
O
1
.83
1.8
5
1.8
2
1.8
6
2.2
0
1.9
6
1.9
3
1.7
5
1.8
6
1.8
0
1.7
3
1.8
1
1.8
0
1.7
6
K2O
0.0
8
0.0
9
0.0
8
0.1
0
0.1
2
0.1
0
0.1
1
0.1
0
0.1
0
0.0
9
0.0
9
0.1
0
0.0
9
0.0
9
P2O
5
0.1
0
0.0
9
0.1
1
0.0
9
0.0
6
0.0
5
0.0
5
0.0
7
0.0
4
Cr 2
O3
0.0
6
0.0
6
0.0
7
0.0
7
0.0
4
0.0
5
0.0
8
0.0
3
0.0
7
0.0
7
0.1
0
0.0
5
0.0
5
0.0
3
To
tal
9
9.3
5
98
.91
99
.02
98
.97
10
0.1
7
97
.94
99
.53
99
.74
98
.03
99
.29
99
.09
99
.71
99
.12
99
.04
Cl
(pp
m)
20
20
30
3
50
30
23
30
23
40
20
0
30
10
S (
pp
m)
3
40
50
68
80
1
23
0
83
11
2
71
23
6
12
0
84
83
68
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
S
i 4
5.1
3
45
.63
45
.41
45
.27
46
.93
45
.72
46
.18
45
.58
45
.10
44
.59
44
.82
44
.57
44
.41
44
.45
Mg
11
.23
9.7
1
10
.25
11
.42
5.4
6
6.6
8
6.7
8
10
.50
10
.31
11
.87
12
.65
11
.78
12
.89
12
.65
Mn
1.4
3
1.2
8
1.0
8
1.0
8
1.1
7
1.5
0
1.3
1
1.1
5
0.6
9
1.1
7
1.0
1
1.1
2
1.1
9
1.6
7
Ca
13
.90
14
.59
14
.43
13
.75
16
.07
15
.70
15
.67
14
.36
14
.57
13
.59
13
.00
13
.64
13
.21
13
.08
Fe
7.7
8
7.8
0
7.8
4
7.3
8
6.3
1
7.1
0
6.8
6
7.1
0
7.3
4
7.2
2
7.5
5
7.5
8
7.2
0
7.5
2
Al
16
.22
16
.61
16
.61
16
.73
19
.26
18
.72
18
.75
17
.46
17
.66
17
.48
16
.99
17
.26
17
.03
16
.76
Ti
0.8
6
0.8
5
0.8
9
0.8
4
0.7
0
0.8
7
0.8
4
0.6
2
0.8
2
0.6
8
0.7
3
0.6
6
0.6
9
0.5
9
Na
3.2
9
3.3
5
3.3
0
3.3
5
3.9
5
3.5
9
3.4
8
3.1
3
3.4
0
3.2
2
3.1
1
3.2
3
3.2
2
3.1
4
K
0.1
0
0.1
1
0.1
0
0.1
2
0.1
4
0.1
2
0.1
3
0.1
1
0.1
2
0.1
1
0.1
1
0.1
1
0.1
1
0.1
0
P
0.0
8
0.0
7
0.0
9
0.0
7
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
4
0.0
4
0.0
4
0.0
6
0.0
3
Cr
0.0
4
0.0
5
0.0
5
0.0
5
0.0
3
0.0
4
0.0
6
0.0
2
0.0
5
0.0
5
0.0
8
0.0
3
0.0
4
0.0
2
K/T
i
0.1
1
0.1
3
0.1
1
0.1
4
0.2
0
0.1
4
0.1
5
0.1
8
0.1
5
0.1
6
0.1
5
0.1
7
0.1
6
0.1
7
Cl/
K
0.0
2
0.0
2
0.0
3
0.0
0
0.0
4
0.0
3
0.0
2
0.0
3
0.0
2
0.0
4
0.0
2
0.0
0
0.0
3
0.0
1
104
Mel
t in
clu
sion
s co
nti
nu
ed
Sam
ple
A
k2
/6
Ak2
/7
Ak2
/8
Ak2
/9
Ak2
/10
Ak2
/11
.1
Ak2
/11
.2
Ak2
/12
Ak2
/13
.1
Ak2
/13
.2
Ak2
/14
AK
11
a/3
.1
AK
11
a/3
.2
AK
11
a/4
Typ
e
N
N
N
N
N
N
N
N
N
N
N
N
N
N
(wt
%)
SiO
2
48
.29
49
.13
48
.43
49
.73
48
.51
49
.19
49
.48
49
.13
49
.16
49
.24
49
.14
47
.88
48
.00
48
.73
MgO
8.7
9
7.6
6
6.8
3
4.9
8
6.5
7
6.2
5
6.3
9
5.0
3
4.6
1
4.6
1
5.0
8
7.8
9
8.0
3
6.3
7
Mn
O
0
.17
0.2
3
0.1
5
0.1
5
0.1
5
0.1
9
0.1
8
0.1
4
0.1
3
0.1
6
0.1
5
0.1
5
0.1
5
0.2
1
CaO
13
.75
14
.01
14
.91
14
.64
14
.66
14
.92
14
.88
15
.55
15
.62
15
.52
15
.49
14
.21
14
.17
14
.90
FeO
*
9.5
8
8.9
4
9.5
9
8.4
6
9.3
1
9.2
6
9.5
3
8.8
0
8.3
9
8.6
9
9.0
2
9.4
0
9.3
5
9.5
3
Al 2
O3
15
.64
16
.07
16
.12
17
.68
16
.13
16
.82
16
.94
17
.22
17
.64
17
.33
17
.17
15
.90
15
.81
16
.43
TiO
2
0
.93
0.8
9
0.9
9
1.0
1
0.9
2
1.1
0
0.9
5
1.0
8
1.0
7
1.0
6
1.0
4
0.8
5
0.8
9
1.1
7
Na 2
O
1
.66
1.8
2
1.6
8
2.0
7
1.7
8
1.8
0
1.8
4
1.8
2
1.8
7
1.8
3
1.8
2
1.7
1
1.7
5
1.8
6
K2O
0.1
0
0.0
8
0.0
9
0.1
0
0.0
8
0.1
0
0.0
9
0.0
9
0.1
0
0.1
1
0.0
9
0.1
0
0.0
9
0.1
0
P2O
5
0.1
0
0.0
8
0.0
8
0.0
6
0.1
1
0.0
8
0.0
6
0.0
6
0.1
0
0.0
9
0.0
6
0.0
9
0.0
8
0.0
8
Cr 2
O3
0.0
8
0.0
6
0.0
5
0.0
5
0.0
9
0.0
7
0.1
0
0.0
5
0.0
4
0.0
8
0.0
5
0.0
7
0.0
8
0.0
5
To
tal
9
9.1
6
99
.02
98
.96
99
.11
98
.51
99
.83
10
0.4
9
99
.04
98
.82
98
.79
99
.16
98
.41
98
.59
99
.45
Cl
(pp
m)
70
0
35
0
20
20
30
25
60
30
30
0
0
10
S (
pp
m)
23
6
19
6
16
8
76
4
85
2
25
6
25
2
24
0
37
2
24
8
19
6
76
0
74
8
92
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
S
i 4
4.7
2
45
.47
45
.30
46
.55
45
.66
45
.55
45
.52
46
.11
46
.28
46
.35
46
.07
44
.86
44
.87
45
.20
Mg
12
.14
10
.56
9.5
2
6.9
5
9.2
2
8.6
3
8.7
6
7.0
4
6.4
7
6.4
7
7.0
9
11
.01
11
.19
8.8
1
Mn
1.1
8
1.5
8
1.0
4
1.0
8
1.0
4
1.3
2
1.2
6
1.0
2
0.9
5
1.1
7
1.0
5
1.0
5
1.0
5
1.4
9
Ca
13
.64
13
.89
14
.94
14
.68
14
.78
14
.80
14
.66
15
.64
15
.75
15
.66
15
.56
14
.27
14
.19
14
.81
Fe
7.4
2
6.9
2
7.5
0
6.6
2
7.3
3
7.1
7
7.3
4
6.9
0
6.6
1
6.8
4
7.0
7
7.3
7
7.3
1
7.4
0
Al
17
.07
17
.53
17
.77
19
.50
17
.90
18
.35
18
.37
19
.05
19
.57
19
.23
18
.97
17
.56
17
.42
17
.96
Ti
0.6
5
0.6
2
0.6
9
0.7
1
0.6
5
0.7
6
0.6
6
0.7
7
0.7
6
0.7
5
0.7
3
0.6
0
0.6
3
0.8
2
Na
2.9
8
3.2
7
3.0
5
3.7
5
3.2
5
3.2
3
3.2
8
3.3
2
3.4
1
3.3
3
3.3
0
3.1
0
3.1
8
3.3
4
K
0.1
2
0.1
0
0.1
1
0.1
2
0.0
9
0.1
2
0.1
1
0.1
1
0.1
1
0.1
3
0.1
1
0.1
1
0.1
0
0.1
2
P
0.0
8
0.0
6
0.0
6
0.0
5
0.0
9
0.0
6
0.0
4
0.0
5
0.0
8
0.0
7
0.0
5
0.0
7
0.0
6
0.0
6
Cr
0.0
6
0.0
4
0.0
4
0.0
3
0.0
7
0.0
5
0.0
7
0.0
4
0.0
3
0.0
6
0.0
4
0.0
5
0.0
6
0.0
3
K/T
i
0.1
8
0.1
6
0.1
5
0.1
6
0.1
4
0.1
6
0.1
6
0.1
4
0.1
5
0.1
7
0.1
5
0.1
9
0.1
6
0.1
4
Cl/
K
0.0
6
0.0
0
0.0
3
0.0
0
0.0
2
0.0
2
0.0
3
0.0
2
0.0
5
0.0
2
0.0
3
0.0
0
0.0
0
0.0
1
105
Mel
t in
clu
sion
s co
nti
nu
ed
Sam
ple
A
K1
1a/
5
AK
11
a/6
A
K1
2/1
A
K1
2/2
A
K1
2/3
A
K1
2/4
A
K1
2/5
.1
AK
12
/5.2
A
K1
2/5
.3
AK
12
/6
AK
12
/7
AK
12
/8
AK
12
/9
AK
12
/10
Typ
e
N
N
N
N
N
N
N
N
N
N
N
N
N
N
(wt
%)
SiO
2
48
.62
48
.17
47
.90
48
.60
48
.42
48
.23
47
.92
48
.50
47
.92
48
.37
48
.31
48
.44
48
.19
48
.37
MgO
7.4
2
7.6
0
7.0
2
6.4
3
7.9
2
7.5
8
7.6
5
7.6
7
7.5
1
8.4
9
8.7
9
8.6
7
8.5
5
8.5
7
Mn
O
0
.18
0.2
0
0.1
5
0.1
5
0.1
5
0.1
8
0.1
6
0.1
8
0.2
0
0.1
9
0.1
3
0.1
6
0.1
3
0.1
5
CaO
14
.56
14
.53
15
.06
15
.31
14
.52
14
.65
14
.75
14
.45
14
.96
14
.22
14
.01
14
.04
13
.92
13
.79
FeO
*
9.0
6
9.4
0
9.7
1
9.1
3
9.3
3
10
.12
9.7
8
9.6
7
9.7
8
9.3
9
9.0
4
9.1
9
9.3
4
9.3
6
Al 2
O3
16
.40
16
.16
15
.93
16
.33
15
.89
15
.55
15
.72
15
.86
15
.84
15
.82
16
.05
15
.94
15
.83
15
.78
TiO
2
0
.95
1.0
6
1.0
2
1.0
1
1.0
0
1.0
2
1.1
1
0.9
6
1.0
8
0.9
6
0.9
0
1.1
2
1.0
9
1.0
2
Na 2
O
1
.77
1.7
3
1.6
3
1.6
8
1.6
1
1.6
1
1.6
0
1.7
0
1.5
9
1.7
0
1.7
5
1.8
0
1.7
8
1.7
1
K2O
0.1
1
0.1
0
0.1
0
0.0
7
0.0
7
0.0
9
0.0
9
0.1
0
0.0
8
0.0
9
0.0
8
0.0
9
0.1
1
0.0
9
P2O
5
0.0
5
0.0
7
0.0
7
0.0
9
0.0
5
0.0
5
0.0
8
0.0
9
0.0
8
0.0
9
0.0
9
0.0
9
0.0
6
0.0
3
Cr 2
O3
0.0
9
0.0
6
0.0
8
0.0
7
0.0
7
0.0
7
0.0
6
0.0
9
0.0
7
0.0
6
0.0
5
0.0
6
0.0
7
0.0
5
To
tal
9
9.2
5
99
.15
98
.78
98
.92
99
.09
99
.16
98
.98
99
.32
99
.15
99
.57
99
.25
99
.71
99
.28
98
.97
Cl
(pp
m)
0
25
20
30
10
0
0
20
20
17
0
0
40
10
S (
pp
m)
22
4
25
2
38
4
15
4
25
8
16
25
6
20
4
18
4
73
9
22
0
40
8
75
2
20
0
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
S
i 4
5.0
6
44
.69
44
.91
45
.52
45
.07
44
.90
44
.71
44
.99
44
.56
44
.62
44
.70
44
.59
44
.70
44
.90
Mg
10
.25
10
.51
9.8
2
8.9
8
10
.99
10
.52
10
.65
10
.61
10
.40
11
.68
12
.13
11
.90
11
.82
11
.86
Mn
1.2
8
1.3
8
1.0
6
1.0
4
1.0
2
1.2
4
1.1
5
1.2
8
1.3
8
1.3
0
0.8
8
1.1
4
0.9
4
1.0
6
Ca
14
.46
14
.44
15
.13
15
.36
14
.48
14
.61
14
.75
14
.36
14
.91
14
.05
13
.89
13
.85
13
.84
13
.72
Fe
7.0
2
7.2
9
7.6
1
7.1
5
7.2
7
7.8
8
7.6
3
7.5
0
7.6
1
7.2
5
6.9
9
7.0
8
7.2
5
7.2
6
Al
17
.92
17
.67
17
.60
18
.02
17
.43
17
.07
17
.28
17
.34
17
.36
17
.20
17
.50
17
.29
17
.31
17
.27
Ti
0.6
6
0.7
4
0.7
2
0.7
1
0.7
0
0.7
2
0.7
8
0.6
7
0.7
6
0.6
7
0.6
2
0.7
7
0.7
6
0.7
1
Na
3.1
8
3.1
1
2.9
7
3.0
5
2.9
1
2.9
1
2.8
9
3.0
6
2.8
7
3.0
5
3.1
3
3.2
1
3.2
1
3.0
7
K
0.1
3
0.1
1
0.1
2
0.0
9
0.0
9
0.1
1
0.1
0
0.1
2
0.1
0
0.1
1
0.0
9
0.1
0
0.1
3
0.1
1
P
0.0
4
0.0
6
0.0
6
0.0
7
0.0
4
0.0
4
0.0
6
0.0
7
0.0
6
0.0
7
0.0
7
0.0
7
0.0
5
0.0
3
Cr
0.0
6
0.0
4
0.0
6
0.0
5
0.0
5
0.0
5
0.0
4
0.0
6
0.0
5
0.0
4
0.0
4
0.0
5
0.0
5
0.0
4
K/T
i
0.1
9
0.1
5
0.1
7
0.1
2
0.1
3
0.1
6
0.1
3
0.1
8
0.1
3
0.1
6
0.1
4
0.1
3
0.1
7
0.1
5
Cl/
K
0.0
0
0.0
2
0.0
2
0.0
3
0.0
1
0.0
0
0.0
0
0.0
2
0.0
2
0.0
2
0.0
0
0.0
0
0.0
3
0.0
1
106
Mel
t in
clu
sion
s co
nti
nu
ed
Sam
ple
A
K1
2/1
1
AK
12
/13
AK
12
/14
.1
AK
12
/14
.2
AK
12
/15
AK
12
/16
AK
12
/i4
.1
AK
12
/i7
A
K1
2/i
9
AK
12
/i1
1
AK
12
/i1
6
AK
12
/i2
4
PI0
2c
PI0
2c
Typ
e
N
N
N
N
N
N
N
N
N
N
N
N
N
N
(wt
%)
SiO
2
48
.38
48
.28
48
.63
48
.53
48
.15
48
.49
50
.39
48
.37
48
.93
49
.39
48
.68
48
.77
48
.87
48
.64
MgO
9.0
7
8.5
5
8.8
6
9.0
5
8.8
5
8.8
1
5.2
4
6.7
2
7.2
3
7.3
9
8.1
9
8.5
0
8.4
8
8.4
4
Mn
O
0
.14
0.1
6
0.1
6
0.1
3
0.1
3
0.1
9
0.1
5
0.1
2
0.1
9
0.1
5
0.2
4
0.1
8
0.1
8
0.1
7
CaO
13
.68
13
.98
13
.53
13
.39
13
.69
13
.82
15
.34
14
.94
14
.88
14
.76
14
.21
13
.98
13
.46
13
.80
FeO
*
9.4
8
9.2
3
9.3
8
9.1
6
9.0
1
9.3
2
8.8
8
9.4
9
9.7
5
9.5
4
9.5
0
9.1
4
9.9
8
9.0
1
Al 2
O3
15
.91
16
.22
15
.90
15
.83
16
.13
15
.75
17
.13
16
.49
16
.15
16
.45
15
.88
15
.90
15
.44
15
.77
TiO
2
1
.00
1.1
2
0.9
5
0.9
6
0.9
4
0.9
3
1.0
4
0.9
6
1.0
5
0.9
4
0.9
4
0.8
8
1.2
0
1.1
4
Na 2
O
1
.78
1.7
9
1.7
8
1.7
7
1.7
9
1.6
8
1.9
0
1.7
6
1.6
7
1.8
3
1.6
9
1.7
8
1.9
3
1.9
0
K2O
0.0
9
0.0
9
0.0
9
0.1
0
0.0
9
0.0
8
0.0
8
0.0
7
0.0
9
0.0
7
0.0
8
0.0
8
0.1
2
0.1
1
P2O
5
0.0
8
0.0
8
0.0
8
0.0
7
0.0
9
0.0
4
0.1
0
0.1
4
Cr 2
O3
0.0
8
0.0
8
0.0
8
0.0
5
0.0
7
0.0
4
0.0
8
0.0
7
0.0
4
0.0
6
0.0
6
0.0
7
To
tal
9
9.7
3
99
.62
99
.48
99
.11
99
.04
99
.18
10
0.2
9
99
.18
10
0.0
3
10
0.6
4
99
.51
99
.31
99
.77
99
.11
Cl
(pp
m)
20
0
10
30
40
0
15
5
20
13
18
20
S (
pp
m)
24
4
16
8
12
8
28
0
44
0
16
4
12
0
12
1
16
1
15
1
19
9
15
0
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
S
i 4
4.5
3
44
.49
44
.82
44
.92
44
.62
44
.76
46
.69
45
.26
45
.13
45
.29
44
.81
45
.00
44
.94
44
.95
Mg
12
.44
11
.74
12
.17
12
.49
12
.22
12
.12
7.2
4
9.3
7
9.9
4
10
.11
11
.24
11
.68
11
.62
11
.63
Mn
0.9
5
1.0
9
1.1
4
0.9
4
0.9
3
1.3
5
1.0
3
0.8
1
1.3
3
1.0
3
1.6
5
1.2
6
1.2
8
1.1
8
Ca
13
.50
13
.80
13
.36
13
.28
13
.59
13
.67
15
.23
14
.98
14
.70
14
.50
14
.01
13
.82
13
.26
13
.67
Fe
7.3
0
7.1
1
7.2
3
7.0
9
6.9
8
7.1
9
6.8
8
7.4
3
7.5
2
7.3
1
7.3
1
7.0
5
7.6
7
6.9
6
Al
17
.26
17
.61
17
.27
17
.27
17
.61
17
.13
18
.70
18
.19
17
.56
17
.77
17
.22
17
.29
16
.73
17
.18
Ti
0.6
9
0.7
8
0.6
6
0.6
7
0.6
5
0.6
4
0.7
2
0.6
7
0.7
3
0.6
5
0.6
5
0.6
1
0.8
3
0.7
9
Na
3.1
8
3.2
0
3.1
7
3.1
8
3.2
1
3.0
1
3.4
1
3.2
0
2.9
8
3.2
6
3.0
1
3.1
9
3.4
4
3.4
1
K
0.1
0
0.1
1
0.1
0
0.1
1
0.1
1
0.1
0
0.1
0
0.0
9
0.1
1
0.0
8
0.0
9
0.0
9
0.1
4
0.1
3
P
0.0
6
0.0
6
0.0
6
0.0
5
0.0
7
0.0
3
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
8
0.1
1
Cr
0.0
6
0.0
6
0.0
6
0.0
4
0.0
5
0.0
3
0.0
6
0.0
5
0.0
3
0.0
4
0.0
4
0.0
5
K/T
i
0.1
4
0.1
4
0.1
6
0.1
7
0.1
7
0.1
5
0.1
4
0.1
3
0.1
5
0.1
3
0.1
4
0.1
5
0.1
7
0.1
6
Cl/
K
0.0
2
0.0
0
0.0
1
0.0
3
0.0
4
0.0
0
0.0
2
0.0
1
0.0
2
0.0
2
0.0
2
0.0
2
107
Mel
t in
clu
sion
s co
nti
nu
ed
Sam
ple
P
I02
c P
I02
c P
I02
c P
I3c
PI0
6c
PI0
6c
PI0
6c
PI0
6c
PI0
6c
PI0
6c
PI0
6c
PI0
6c
PI0
6c
PI0
6c
PI0
6c
PI0
6c
PI0
6c
PI0
6c
Typ
e
N
E
N
N
E
N
E
N
N
E
N
E
N
N
N
N
E
E
(wt
%)
SiO
2
48
.91
48
.55
48
.64
48
.94
49
.20
49
.20
49
.05
48
.54
48
.61
48
.91
48
.76
49
.25
48
.91
48
.76
48
.48
48
.82
48
.91
48
.71
MgO
8.0
6
8.3
3
8.6
2
7.4
8
7.1
1
7.4
8
7.7
5
7.7
0
7.9
9
7.8
6
7.9
8
8.1
0
8.0
4
7.9
7
7.9
4
8.1
3
7.9
1
7.9
8
Mn
O
0
.17
0.1
5
0.1
9
0.1
5
0.1
6
0.1
4
0.1
7
0.1
8
0.1
9
0.1
7
0.1
7
0.1
5
0.1
5
0.1
5
0.1
7
0.1
7
0.1
7
0.1
8
CaO
14
.08
13
.73
13
.51
13
.97
14
.38
14
.17
14
.12
14
.08
13
.92
14
.01
13
.87
13
.84
13
.87
13
.68
13
.87
13
.92
13
.97
13
.79
FeO
*
9.2
1
10
.22
10
.09
10
.00
8.8
6
8.8
3
9.1
2
8.8
1
8.7
7
8.9
5
8.7
8
8.7
3
8.9
6
8.7
6
8.6
9
8.8
5
8.7
3
8.7
9
Al 2
O3
15
.80
15
.47
15
.39
15
.28
16
.08
15
.89
15
.81
15
.61
15
.71
15
.72
15
.67
15
.84
15
.64
15
.56
15
.81
15
.76
15
.67
15
.63
TiO
2
1
.18
1.1
1
1.1
2
1.2
1
1.2
7
1.2
7
1.1
8
1.1
9
1.1
9
1.2
2
1.1
5
1.2
0
1.2
1
1.2
7
1.2
0
1.2
1
1.1
5
1.1
9
Na 2
O
1
.92
1.8
9
1.8
6
1.8
0
2.0
1
1.9
2
1.9
7
1.9
1
2.0
2
1.9
7
1.9
8
2.0
1
2.0
2
1.9
5
1.9
7
2.0
1
2.0
0
1.9
9
K2O
0.1
2
0.1
6
0.1
2
0.0
8
0.1
5
0.1
2
0.1
4
0.1
3
0.1
4
0.1
5
0.1
2
0.1
7
0.1
4
0.1
4
0.1
4
0.1
4
0.1
5
0.1
7
P2O
5
0.1
0
0.0
8
0.0
9
0.1
0
0.1
0
0.1
1
0.1
1
0.0
9
0.0
9
0.0
8
0.1
1
0.1
3
0.1
6
0.1
0
0.1
4
0.0
8
0.0
9
0.0
8
Cr 2
O3
To
tal
9
9.5
5
99
.69
99
.63
99
.01
99
.32
99
.13
99
.42
98
.24
98
.63
99
.04
98
.59
99
.42
99
.10
98
.34
98
.41
99
.09
98
.75
98
.51
Cl
(pp
m)
S (
pp
m)
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
S
i 4
5.0
8
44
.80
44
.77
45
.68
45
.59
45
.71
45
.31
45
.33
45
.10
45
.31
45
.33
45
.44
45
.30
45
.53
45
.15
45
.13
45
.40
45
.29
Mg
11
.07
11
.46
11
.83
10
.41
9.8
2
10
.36
10
.67
10
.72
11
.05
10
.86
11
.06
11
.14
11
.10
11
.09
11
.02
11
.20
10
.95
11
.06
Mn
1.2
1
1.0
6
1.3
1
1.0
4
1.1
2
0.9
8
1.1
9
1.2
7
1.3
3
1.1
9
1.2
0
1.0
5
1.0
5
1.0
6
1.2
0
1.1
9
1.1
9
1.2
7
Ca
13
.90
13
.57
13
.32
13
.97
14
.28
14
.11
13
.97
14
.09
13
.84
13
.91
13
.82
13
.68
13
.77
13
.69
13
.84
13
.79
13
.89
13
.74
Fe
7.1
0
7.8
9
7.7
7
7.8
1
6.8
7
6.8
6
7.0
5
6.8
8
6.8
0
6.9
3
6.8
3
6.7
4
6.9
4
6.8
4
6.7
7
6.8
4
6.7
8
6.8
3
Al
17
.16
16
.82
16
.70
16
.81
17
.56
17
.40
17
.21
17
.18
17
.18
17
.17
17
.17
17
.22
17
.07
17
.12
17
.35
17
.17
17
.14
17
.13
Ti
0.8
2
0.7
7
0.7
8
0.8
5
0.8
9
0.8
9
0.8
2
0.8
4
0.8
3
0.8
5
0.8
0
0.8
3
0.8
4
0.8
9
0.8
4
0.8
4
0.8
0
0.8
3
Na
3.4
3
3.3
8
3.3
2
3.2
6
3.6
1
3.4
6
3.5
3
3.4
6
3.6
3
3.5
4
3.5
7
3.6
0
3.6
3
3.5
3
3.5
6
3.6
0
3.6
0
3.5
9
K
0.1
4
0.1
9
0.1
4
0.0
9
0.1
8
0.1
4
0.1
6
0.1
5
0.1
7
0.1
8
0.1
4
0.2
0
0.1
7
0.1
7
0.1
7
0.1
7
0.1
8
0.2
0
P
0.0
8
0.0
6
0.0
7
0.0
8
0.0
8
0.0
9
0.0
9
0.0
7
0.0
7
0.0
6
0.0
9
0.1
0
0.1
3
0.0
8
0.1
1
0.0
6
0.0
7
0.0
6
Cr
K/T
i
0.1
7
0.2
4
0.1
8
0.1
1
0.2
0
0.1
6
0.2
0
0.1
9
0.2
0
0.2
1
0.1
8
0.2
4
0.2
0
0.1
9
0.2
0
0.2
0
0.2
2
0.2
4
Cl/
K
108
Mel
t in
clu
sion
s co
nti
nu
ed
Sam
ple
P
I06
c P
I06
c P
I06
c P
I06
c P
I07
c P
I07
c P
I07
c P
I07
c P
I07
c P
I07
c P
I07
c P
I07
c P
I07
c P
I07
c P
I07
c P
I09
c P
I09
c P
I09
c
Typ
e
E
E
N
N
E
N
N
N
E
E
N
E
N
E
E
N
N
E
(wt
%)
SiO
2
49
.74
49
.08
48
.86
48
.78
49
.08
48
.80
49
.09
48
.90
48
.87
48
.63
48
.71
48
.87
48
.80
48
.93
48
.76
48
.87
49
.20
49
.60
MgO
6.4
5
8.0
1
7.9
5
7.7
5
8.4
3
7.5
9
6.8
5
6.7
8
7.6
7
7.9
1
8.2
0
7.8
8
7.8
6
8.3
5
8.2
1
7.5
1
8.2
2
8.3
2
Mn
O
0
.19
0.1
7
0.1
7
0.2
0
0.1
8
0.2
0
0.1
7
0.1
8
0.1
8
0.1
7
0.1
8
0.1
6
0.1
9
0.1
7
0.1
8
0.2
0
0.1
4
0.1
5
CaO
14
.36
13
.58
14
.03
13
.80
13
.87
14
.11
14
.59
14
.48
13
.93
13
.88
13
.59
13
.71
13
.80
13
.81
13
.56
14
.25
13
.44
13
.75
FeO
*
9.6
0
10
.00
9.9
6
9.8
6
8.9
7
10
.27
9.8
6
10
.02
10
.39
10
.33
10
.13
9.8
5
10
.09
9.0
8
10
.21
10
.16
9.4
5
9.6
3
Al 2
O3
15
.12
15
.45
15
.39
15
.25
15
.57
15
.06
15
.46
15
.67
15
.31
15
.25
15
.23
15
.31
15
.38
15
.51
15
.35
15
.12
15
.94
15
.43
TiO
2
1
.30
1.1
3
1.1
8
1.2
3
1.2
8
1.1
8
1.1
9
1.2
9
1.2
1
1.2
0
1.1
4
1.2
0
1.2
0
1.1
4
1.1
4
1.1
6
1.2
4
1.1
5
Na 2
O
2
.12
1.9
5
1.9
1
1.8
6
2.0
1
1.8
6
1.7
9
1.8
4
1.9
2
1.8
8
1.8
9
1.9
1
1.8
5
1.9
7
1.9
3
1.6
8
1.9
8
1.8
5
K2O
0.1
9
0.1
5
0.1
3
0.1
3
0.1
7
0.1
1
0.1
2
0.1
2
0.1
4
0.1
5
0.1
2
0.1
5
0.1
3
0.1
4
0.1
4
0.1
1
0.1
2
0.1
5
P2O
5
0.1
9
0.1
2
0.0
7
0.0
8
0.1
0
0.1
3
0.1
5
0.1
0
0.1
2
0.0
9
0.1
1
0.1
3
0.0
6
0.1
4
0.1
3
0.0
6
0.1
0
0.1
1
Cr 2
O3
To
tal
9
9.2
6
99
.64
99
.65
98
.94
99
.66
99
.30
99
.27
99
.38
99
.75
99
.49
99
.30
99
.16
99
.36
99
.24
99
.61
99
.12
99
.84
10
0.1
4
Cl
(pp
m)
S (
pp
m)
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
S
i 4
6.2
6
45
.30
45
.11
45
.33
45
.09
45
.27
45
.74
45
.49
45
.14
45
.03
45
.08
45
.38
45
.19
45
.17
44
.97
45
.46
45
.28
45
.56
Mg
8.9
4
11
.02
10
.94
10
.74
11
.54
10
.50
9.5
1
9.4
0
10
.56
10
.92
11
.31
10
.91
10
.85
11
.49
11
.29
10
.41
11
.28
11
.39
Mn
1.3
4
1.1
9
1.1
9
1.4
1
1.2
3
1.3
7
1.1
9
1.2
5
1.2
7
1.1
8
1.2
6
1.1
2
1.3
0
1.2
0
1.2
8
1.4
3
1.0
0
1.0
7
Ca
14
.31
13
.43
13
.88
13
.74
13
.65
14
.03
14
.57
14
.43
13
.79
13
.77
13
.48
13
.64
13
.69
13
.66
13
.40
14
.20
13
.25
13
.53
Fe
7.4
7
7.7
2
7.6
9
7.6
6
6.8
9
7.9
7
7.6
8
7.8
0
8.0
3
8.0
0
7.8
4
7.6
5
7.8
1
7.0
1
7.8
7
7.9
0
7.2
7
7.4
0
Al
16
.57
16
.80
16
.75
16
.70
16
.86
16
.47
16
.98
17
.18
16
.67
16
.64
16
.61
16
.75
16
.79
16
.87
16
.68
16
.58
17
.29
16
.70
Ti
0.9
1
0.7
8
0.8
2
0.8
6
0.8
8
0.8
2
0.8
3
0.9
0
0.8
4
0.8
4
0.7
9
0.8
4
0.8
4
0.7
9
0.7
9
0.8
1
0.8
6
0.7
9
Na
3.8
2
3.4
9
3.4
2
3.3
5
3.5
8
3.3
5
3.2
3
3.3
2
3.4
4
3.3
8
3.3
9
3.4
4
3.3
2
3.5
3
3.4
5
3.0
3
3.5
3
3.2
9
K
0.2
3
0.1
8
0.1
5
0.1
5
0.2
0
0.1
3
0.1
5
0.1
4
0.1
7
0.1
8
0.1
5
0.1
8
0.1
6
0.1
7
0.1
7
0.1
3
0.1
4
0.1
7
P
0.1
5
0.0
9
0.0
5
0.0
6
0.0
8
0.1
0
0.1
2
0.0
8
0.0
9
0.0
7
0.0
9
0.1
0
0.0
4
0.1
1
0.1
0
0.0
4
0.0
8
0.0
8
Cr
K/T
i
0.2
5
0.2
3
0.1
9
0.1
8
0.2
2
0.1
6
0.1
8
0.1
6
0.2
0
0.2
2
0.1
8
0.2
1
0.1
9
0.2
1
0.2
1
0.1
6
0.1
7
0.2
2
Cl/
K
109
Mel
t in
clu
sion
s co
nti
nu
ed
Sam
ple
P
I09
c P
I09
c P
I09
c P
I09
c P
I09
c P
I09
c P
I09
c P
I09
c P
I09
c P
I10
c P
I10
c P
I10
c P
I10
c P
I10
c P
I10
c P
I10
c P
I10
c P
I10
c
Typ
e
E
N
N
E
E
E
E
E
E
E
N
N
N
N
N
N
N
N
(wt
%)
SiO
2
49
.45
49
.05
48
.89
49
.13
49
.30
48
.92
49
.28
49
.26
49
.10
49
.34
48
.94
49
.00
48
.89
48
.94
48
.77
49
.26
49
.16
48
.85
MgO
7.4
1
7.3
7
8.4
8
8.7
4
8.3
0
8.2
1
7.1
5
8.5
5
8.4
7
8.3
7
8.6
5
8.4
3
7.5
5
7.2
5
7.3
1
6.9
9
6.4
8
8.0
5
Mn
O
0
.19
0.1
6
0.1
9
0.1
5
0.1
8
0.1
3
0.1
9
0.1
6
0.1
8
0.1
8
0.1
4
0.1
8
0.1
6
0.1
8
0.1
7
0.1
9
0.1
6
0.1
7
CaO
14
.14
14
.84
13
.18
13
.42
13
.58
13
.56
14
.31
13
.44
13
.57
13
.53
13
.55
13
.62
14
.18
14
.39
14
.25
14
.48
14
.25
14
.03
FeO
*
8.4
1
9.5
6
10
.05
9.5
1
9.0
3
10
.13
10
.02
9.4
0
9.8
7
9.7
0
9.8
8
10
.00
10
.25
10
.16
10
.28
9.8
6
9.7
3
9.8
7
Al 2
O3
16
.10
15
.53
15
.33
15
.45
15
.55
15
.04
15
.36
15
.56
15
.26
15
.59
15
.36
15
.33
15
.58
15
.53
15
.61
15
.84
16
.08
15
.42
TiO
2
1
.18
1.1
9
1.1
9
1.1
3
1.0
9
1.2
2
1.2
3
1.1
7
1.1
4
1.1
8
1.1
7
1.1
8
1.1
6
1.1
7
1.1
9
1.2
1
1.2
2
1.1
6
Na 2
O
1
.85
1.6
9
1.9
6
1.8
6
2.0
9
1.8
3
1.7
7
1.9
3
1.8
8
1.8
6
1.8
8
1.8
4
1.7
7
1.7
8
1.7
7
1.8
9
1.8
8
1.8
4
K2O
0.1
5
0.1
3
0.1
3
0.1
4
0.1
6
0.1
6
0.1
5
0.1
6
0.1
6
0.1
5
0.1
3
0.1
4
0.1
2
0.1
3
0.1
3
0.1
3
0.1
3
0.1
2
P2O
5
0.1
2
0.1
3
0.0
9
0.0
9
0.1
6
0.0
9
0.1
4
0.1
9
0.1
1
0.1
1
0.0
9
0.0
7
0.1
2
0.1
0
0.0
6
0.1
0
0.1
0
0.0
5
Cr 2
O3
To
tal
9
9.0
1
99
.64
99
.48
99
.62
99
.44
99
.29
99
.60
99
.83
99
.74
10
0.0
1
99
.79
99
.79
99
.79
99
.63
99
.54
99
.94
99
.18
99
.56
Cl
(pp
m)
S (
pp
m)
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
S
i 4
5.8
3
45
.46
45
.06
45
.26
45
.38
45
.46
45
.69
45
.26
45
.19
45
.30
45
.10
45
.09
45
.25
45
.37
45
.26
45
.47
45
.87
45
.14
Mg
10
.24
10
.18
11
.65
12
.00
11
.39
11
.37
9.8
8
11
.71
11
.62
11
.46
11
.88
11
.57
10
.42
10
.02
10
.11
9.6
2
9.0
1
11
.09
Mn
1.3
6
1.1
4
1.3
2
1.0
4
1.2
2
0.9
1
1.3
4
1.1
3
1.2
4
1.2
4
0.9
5
1.2
7
1.1
2
1.2
3
1.1
9
1.2
9
1.1
2
1.1
9
Ca
14
.04
14
.74
13
.02
13
.25
13
.39
13
.50
14
.21
13
.23
13
.38
13
.31
13
.38
13
.43
14
.06
14
.29
14
.17
14
.32
14
.25
13
.89
Fe
6.5
2
7.4
1
7.7
5
7.3
3
6.9
5
7.8
7
7.7
7
7.2
2
7.6
0
7.4
5
7.6
1
7.7
0
7.9
3
7.8
8
7.9
8
7.6
1
7.5
9
7.6
3
Al
17
.59
16
.96
16
.65
16
.78
16
.87
16
.47
16
.78
16
.85
16
.55
16
.87
16
.68
16
.63
16
.99
16
.97
17
.07
17
.23
17
.68
16
.79
Ti
0.8
2
0.8
3
0.8
3
0.7
8
0.7
5
0.8
5
0.8
6
0.8
1
0.7
9
0.8
1
0.8
1
0.8
2
0.8
1
0.8
2
0.8
3
0.8
4
0.8
6
0.8
1
Na
3.3
2
3.0
4
3.5
0
3.3
2
3.7
3
3.3
0
3.1
8
3.4
4
3.3
6
3.3
1
3.3
6
3.2
8
3.1
8
3.2
0
3.1
9
3.3
8
3.4
0
3.3
0
K
0.1
8
0.1
5
0.1
5
0.1
7
0.1
9
0.1
9
0.1
7
0.1
9
0.1
8
0.1
8
0.1
6
0.1
6
0.1
5
0.1
5
0.1
5
0.1
5
0.1
5
0.1
4
P
0.0
9
0.1
0
0.0
7
0.0
7
0.1
2
0.0
7
0.1
1
0.1
5
0.0
9
0.0
8
0.0
7
0.0
5
0.1
0
0.0
8
0.0
5
0.0
7
0.0
8
0.0
4
Cr
K/T
i
0.2
2
0.1
8
0.1
9
0.2
1
0.2
5
0.2
2
0.2
0
0.2
3
0.2
3
0.2
2
0.1
9
0.1
9
0.1
8
0.1
9
0.1
8
0.1
8
0.1
8
0.1
8
Cl/
K
110
Mel
t in
clu
sion
s co
nti
nu
ed
Sam
ple
P
I10
c P
I10
c P
I10
c P
I10
c P
I10
c P
I10
c P
I13
c P
I13
c P
I13
c P
I13
c P
I13
c P
I13
c P
I13
c P
I13
c P
I13
c P
I13
c P
I13
c P
I13
c
Typ
e
N
N
N
N
N
N
E
N
E
N
N
E
N
N
N
N
N
N
(wt
%)
SiO
2
49
.16
48
.23
48
.78
48
.91
48
.77
48
.58
49
.33
49
.11
49
.41
48
.93
48
.82
49
.34
49
.14
49
.36
48
.94
48
.84
49
.13
48
.90
MgO
5.9
8
7.3
6
7.4
2
7.6
8
8.6
6
8.0
6
6.7
5
7.3
7
7.1
6
8.1
2
7.5
6
7.3
8
6.9
2
6.2
5
7.1
7
7.9
5
6.6
4
7.7
5
Mn
O
0
.18
0.2
5
0.2
0
0.1
7
0.1
5
0.1
7
0.1
5
0.1
9
0.1
7
0.2
0
0.1
5
0.1
8
0.1
8
0.1
9
0.1
8
0.1
8
0.1
3
0.1
6
CaO
14
.52
13
.35
14
.19
14
.17
13
.44
13
.96
12
.34
13
.88
14
.39
13
.86
14
.21
14
.38
14
.38
14
.62
14
.23
13
.73
14
.43
13
.91
FeO
*
9.7
2
12
.77
10
.08
9.5
9
9.8
8
10
.07
8.6
7
10
.16
9.1
7
10
.03
10
.28
9.4
3
10
.12
10
.26
10
.33
10
.01
9.6
6
9.5
0
Al 2
O3
16
.17
14
.47
15
.77
15
.66
15
.53
15
.40
15
.72
15
.32
15
.74
15
.40
15
.26
15
.69
15
.53
15
.85
15
.50
15
.36
15
.92
15
.66
TiO
2
1
.27
1.0
8
1.2
3
1.1
7
1.1
9
1.1
5
2.3
9
1.2
2
1.2
1
1.2
0
1.1
9
1.2
0
1.1
5
1.2
2
1.1
4
1.2
4
1.1
7
1.1
8
Na 2
O
1
.92
1.6
6
1.7
5
1.7
6
1.7
9
1.8
4
2.5
5
1.8
7
1.9
6
1.8
8
1.8
6
1.9
4
1.9
5
1.9
2
1.8
5
1.8
0
1.9
9
1.8
8
K2O
0.1
4
0.0
9
0.1
3
0.1
3
0.1
4
0.1
2
0.9
1
0.1
3
0.1
6
0.1
4
0.1
1
0.1
6
0.1
2
0.1
3
0.1
3
0.1
3
0.1
4
0.1
3
P2O
5
0.1
0
0.0
7
0.0
9
0.1
2
0.1
5
0.0
9
0.2
6
0.0
8
0.1
5
0.1
2
0.0
9
0.1
5
0.1
0
0.0
9
0.1
7
0.1
3
0.1
3
0.0
7
Cr 2
O3
To
tal
9
9.1
6
99
.34
99
.64
99
.37
99
.69
99
.44
99
.07
99
.34
99
.52
99
.88
99
.53
99
.85
99
.59
99
.89
99
.64
99
.37
99
.33
99
.14
Cl
(pp
m)
S (
pp
m)
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
S
i 4
5.8
9
44
.92
45
.10
45
.34
44
.98
44
.95
45
.83
45
.58
45
.72
44
.98
45
.30
45
.48
45
.56
45
.75
45
.36
45
.25
45
.79
45
.38
Mg
8.3
2
10
.22
10
.23
10
.61
11
.91
11
.12
9.3
5
10
.20
9.8
8
11
.13
10
.46
10
.14
9.5
6
8.6
4
9.9
1
10
.98
9.2
3
10
.72
Mn
1.2
9
1.7
8
1.4
1
1.2
1
1.0
1
1.2
0
1.0
3
1.3
4
1.2
0
1.4
1
1.0
8
1.2
7
1.2
5
1.3
0
1.2
6
1.2
5
0.8
8
1.1
5
Ca
14
.52
13
.32
14
.06
14
.07
13
.28
13
.84
12
.28
13
.80
14
.27
13
.65
14
.13
14
.20
14
.28
14
.52
14
.13
13
.63
14
.41
13
.83
Fe
7.5
9
9.9
5
7.7
9
7.4
3
7.6
2
7.7
9
6.7
4
7.8
9
7.1
0
7.7
1
7.9
8
7.2
7
7.8
5
7.9
5
8.0
1
7.7
6
7.5
3
7.3
7
Al
17
.79
15
.88
17
.19
17
.11
16
.88
16
.79
17
.21
16
.76
17
.17
16
.69
16
.69
17
.04
16
.97
17
.31
16
.93
16
.77
17
.49
17
.13
Ti
0.8
9
0.7
6
0.8
6
0.8
2
0.8
3
0.8
0
1.6
7
0.8
5
0.8
4
0.8
3
0.8
3
0.8
3
0.8
0
0.8
5
0.7
9
0.8
6
0.8
2
0.8
2
Na
3.4
7
3.0
0
3.1
4
3.1
6
3.2
0
3.3
0
4.5
9
3.3
7
3.5
2
3.3
5
3.3
5
3.4
7
3.5
1
3.4
5
3.3
2
3.2
3
3.6
0
3.3
8
K
0.1
6
0.1
1
0.1
5
0.1
5
0.1
6
0.1
4
1.0
8
0.1
6
0.1
9
0.1
6
0.1
3
0.1
8
0.1
4
0.1
6
0.1
6
0.1
6
0.1
6
0.1
5
P
0.0
8
0.0
6
0.0
7
0.1
0
0.1
2
0.0
7
0.2
1
0.0
6
0.1
2
0.0
9
0.0
7
0.1
2
0.0
8
0.0
7
0.1
3
0.1
0
0.1
0
0.0
6
Cr
K/T
i
0.1
8
0.1
4
0.1
8
0.1
9
0.2
0
0.1
8
0.6
4
0.1
8
0.2
3
0.2
0
0.1
6
0.2
2
0.1
8
0.1
9
0.2
0
0.1
8
0.2
0
0.1
8
Cl/
K
111
Mel
t in
clu
sion
s co
nti
nu
ed
Sam
ple
P
I14
c P
I14
c P
I14
c P
I14
c P
I14
c P
I14
c P
I14
c P
I14
c P
I14
c P
I14
c P
I14
c P
I14
c P
I14
c P
I14
c P
I14
c P
I14
c P
I14
c P
I14
c
Typ
e
N
N
N
N
N
N
N
N
N
N
N
N
N
N
N
N
N
N
(wt
%)
SiO
2
48
.79
48
.56
48
.73
49
.04
49
.52
49
.17
48
.71
48
.70
48
.90
49
.02
49
.02
48
.81
49
.89
48
.70
48
.93
48
.77
48
.54
48
.55
MgO
7.8
0
8.9
4
8.6
4
8.1
0
6.7
8
7.4
9
7.7
4
7.8
9
8.8
4
8.5
9
8.8
3
8.4
5
9.0
2
7.5
6
6.9
3
6.8
3
7.9
2
8.4
0
Mn
O
0
.18
0.1
4
0.1
8
0.1
5
0.2
0
0.1
6
0.1
8
0.1
6
0.1
5
0.1
2
0.1
5
0.1
6
0.1
7
0.2
0
0.1
8
0.1
7
0.1
5
0.1
7
CaO
14
.52
13
.86
14
.06
14
.89
14
.90
14
.77
14
.47
14
.55
13
.70
14
.17
14
.00
14
.34
14
.37
14
.80
15
.07
15
.55
14
.68
14
.33
FeO
*
9.7
6
9.2
4
9.6
1
8.8
1
8.7
5
8.7
0
9.7
9
9.6
6
9.6
0
8.6
0
9.5
0
9.6
8
7.9
0
9.6
3
9.6
6
9.2
8
9.5
9
9.5
4
Al 2
O3
15
.66
15
.69
15
.39
15
.86
16
.33
16
.12
15
.52
15
.52
15
.38
16
.03
15
.29
15
.42
15
.66
15
.78
15
.83
16
.36
15
.55
15
.51
TiO
2
1
.13
1.0
4
1.0
8
1.1
5
1.1
2
1.1
1
1.1
5
1.1
9
1.0
9
1.1
0
1.1
3
1.1
6
1.1
1
1.1
5
1.1
9
1.2
6
1.1
6
1.1
2
Na 2
O
1
.66
1.7
4
1.7
5
1.6
5
1.8
0
1.7
3
1.6
6
1.6
8
1.7
4
1.7
5
1.7
2
1.6
8
1.7
3
1.6
9
1.6
4
1.6
7
1.6
2
1.6
5
K2O
0.0
7
0.0
9
0.0
8
0.0
8
0.0
8
0.0
8
0.0
8
0.0
7
0.0
6
0.0
6
0.0
9
0.0
7
0.0
7
0.0
8
0.0
7
0.0
7
0.0
7
0.0
7
P2O
5
0.1
2
0.0
5
0.0
8
0.0
8
0.0
9
0.1
0
0.1
0
0.1
2
0.1
2
0.0
7
0.0
7
0.1
0
0.0
6
0.1
1
0.1
0
0.1
1
0.0
6
0.1
0
Cr 2
O3
To
tal
9
9.6
8
99
.34
99
.60
99
.81
99
.57
99
.42
99
.39
99
.53
99
.58
99
.51
99
.80
99
.87
99
.98
99
.70
99
.61
10
0.0
7
99
.34
99
.44
Cl
(pp
m)
S (
pp
m)
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
Si
45
.10
44
.84
44
.87
45
.20
45
.77
45
.54
45
.16
45
.10
45
.10
45
.25
45
.11
44
.95
45
.61
44
.96
45
.41
45
.04
45
.06
44
.89
Mg
10
.75
12
.31
11
.86
11
.13
9.3
4
10
.34
10
.70
10
.89
12
.15
11
.82
12
.11
11
.60
12
.29
10
.41
9.5
9
9.4
0
10
.96
11
.58
Mn
1.2
4
0.9
4
1.2
8
1.0
5
1.4
1
1.0
9
1.2
7
1.1
3
1.0
5
0.8
2
1.0
7
1.1
4
1.1
5
1.3
8
1.2
6
1.1
6
1.0
7
1.1
5
Ca
14
.38
13
.71
13
.87
14
.70
14
.76
14
.66
14
.37
14
.44
13
.54
14
.01
13
.80
14
.15
14
.08
14
.64
14
.98
15
.39
14
.60
14
.20
Fe
7.5
4
7.1
4
7.4
0
6.7
9
6.7
6
6.7
4
7.5
9
7.4
8
7.4
0
6.6
4
7.3
1
7.4
6
6.0
4
7.4
4
7.5
0
7.1
7
7.4
5
7.3
8
Al
17
.06
17
.08
16
.70
17
.23
17
.79
17
.60
16
.96
16
.94
16
.72
17
.44
16
.58
16
.74
16
.87
17
.17
17
.31
17
.81
17
.01
16
.90
Ti
0.7
9
0.7
2
0.7
5
0.8
0
0.7
8
0.7
7
0.8
0
0.8
3
0.7
6
0.7
6
0.7
8
0.8
0
0.7
6
0.8
0
0.8
3
0.8
8
0.8
1
0.7
8
Na
2.9
8
3.1
2
3.1
2
2.9
5
3.2
3
3.1
1
2.9
8
3.0
2
3.1
1
3.1
3
3.0
7
3.0
0
3.0
7
3.0
3
2.9
5
2.9
9
2.9
2
2.9
6
K
0.0
8
0.1
0
0.0
9
0.1
0
0.0
9
0.0
9
0.0
9
0.0
8
0.0
7
0.0
8
0.1
0
0.0
8
0.0
8
0.0
9
0.0
9
0.0
9
0.0
8
0.0
8
P
0.0
9
0.0
4
0.0
6
0.0
6
0.0
7
0.0
7
0.0
8
0.0
9
0.0
9
0.0
5
0.0
5
0.0
8
0.0
5
0.0
9
0.0
8
0.0
9
0.0
5
0.0
8
Cr
K/T
i
0.1
0
0.1
4
0.1
2
0.1
2
0.1
2
0.1
1
0.1
1
0.0
9
0.1
0
0.1
0
0.1
3
0.1
0
0.1
1
0.1
2
0.1
0
0.1
0
0.1
0
0.1
1
Cl/
K
112
Mel
t in
clu
sion
s co
nti
nu
ed
Sam
ple
P
I15
c P
I15
c P
I15
c P
I15
c P
I15
c P
I15
c P
I17
c P
I17
c P
I17
c P
I17
c P
I17
c P
I17
c P
I17
c P
I17
c P
I17
c P
I17
c P
I17
c P
I17
c
Typ
e
N
N
N
N
N
N
E
E
E
E
E
E
E
E
E
E
E
E
(wt
%)
SiO
2
48
.94
49
.08
48
.50
48
.74
49
.16
49
.84
49
.29
49
.05
49
.27
49
.03
49
.10
49
.42
49
.12
49
.20
49
.05
49
.12
49
.31
49
.85
MgO
8.2
0
8.7
3
8.9
3
8.4
7
6.0
3
5.0
5
8.1
2
8.1
4
8.1
4
8.0
8
8.1
1
8.1
0
8.0
8
8.1
6
8.1
0
8.1
4
7.8
3
7.9
5
Mn
O
0
.20
0.2
0
0.1
7
0.1
7
0.1
7
0.1
4
0.1
8
0.1
5
0.1
9
0.1
6
0.1
8
0.1
5
0.1
4
0.1
6
0.1
9
0.1
5
0.1
5
0.1
8
CaO
14
.27
13
.83
13
.63
14
.31
15
.51
15
.60
13
.83
13
.88
13
.85
13
.63
13
.70
13
.59
13
.80
13
.82
13
.79
13
.73
13
.83
13
.77
FeO
*
9.4
9
9.5
6
9.5
2
9.6
7
9.5
6
8.8
5
9.7
5
9.9
1
9.7
2
9.7
4
9.8
4
9.9
7
9.9
1
9.8
2
9.8
3
9.7
9
9.6
5
9.7
7
Al 2
O3
15
.69
15
.20
15
.52
15
.29
16
.08
16
.56
14
.61
14
.57
14
.81
14
.54
14
.79
14
.73
14
.66
14
.69
14
.64
14
.70
14
.57
14
.45
TiO
2
1
.16
1.1
0
1.0
6
1.0
7
1.1
9
1.1
8
1.2
0
1.1
8
1.1
8
1.2
2
1.0
6
1.2
8
1.2
6
1.1
9
1.2
0
1.2
5
1.2
5
1.2
1
Na 2
O
1
.67
1.6
9
1.6
6
1.6
9
1.7
0
1.8
7
1.9
6
1.9
0
1.8
8
1.9
1
1.9
4
1.9
5
1.8
8
1.9
6
1.9
7
1.9
5
1.9
0
1.9
4
K2O
0.0
7
0.0
8
0.0
8
0.0
8
0.0
7
0.0
9
0.1
9
0.1
9
0.2
0
0.1
9
0.2
1
0.1
9
0.2
1
0.1
7
0.2
2
0.1
7
0.1
8
0.1
7
P2O
5
0.1
2
0.1
3
0.1
2
0.0
8
0.1
1
0.1
4
0.1
1
0.1
1
0.1
0
0.1
0
0.1
1
0.0
9
0.1
9
0.1
1
0.0
8
0.0
9
0.1
1
0.1
4
Cr 2
O3
To
tal
9
9.8
0
99
.60
99
.18
99
.56
99
.58
99
.32
99
.24
99
.08
99
.34
98
.60
99
.04
99
.47
99
.25
99
.28
99
.07
99
.09
98
.78
99
.43
Cl
(pp
m)
S (
pp
m)
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
S
i 4
5.0
4
45
.18
44
.84
45
.00
45
.77
46
.68
45
.64
45
.60
45
.56
45
.77
45
.54
45
.78
45
.65
45
.59
45
.46
45
.64
46
.03
46
.15
Mg
11
.25
11
.98
12
.31
11
.66
8.3
7
7.0
5
11
.21
11
.28
11
.22
11
.24
11
.21
11
.19
11
.19
11
.27
11
.19
11
.27
10
.90
10
.97
Mn
1.3
7
1.3
9
1.1
8
1.1
7
1.2
2
0.9
6
1.2
6
1.0
6
1.3
3
1.1
3
1.2
6
1.0
5
0.9
8
1.1
2
1.3
3
1.0
5
1.0
6
1.2
6
Ca
14
.07
13
.64
13
.50
14
.16
15
.47
15
.65
13
.72
13
.83
13
.72
13
.63
13
.62
13
.49
13
.74
13
.72
13
.70
13
.67
13
.83
13
.66
Fe
7.3
0
7.3
6
7.3
6
7.4
7
7.4
4
6.9
3
7.5
5
7.7
1
7.5
2
7.6
0
7.6
3
7.7
2
7.7
0
7.6
1
7.6
2
7.6
1
7.5
3
7.5
6
Al
17
.02
16
.49
16
.91
16
.64
17
.65
18
.28
15
.95
15
.96
16
.14
16
.00
16
.17
16
.08
16
.06
16
.04
15
.99
16
.10
16
.03
15
.76
Ti
0.8
0
0.7
6
0.7
4
0.7
4
0.8
3
0.8
3
0.8
4
0.8
3
0.8
2
0.8
6
0.7
4
0.8
9
0.8
8
0.8
3
0.8
4
0.8
7
0.8
8
0.8
4
Na
2.9
8
3.0
2
2.9
8
3.0
3
3.0
7
3.4
0
3.5
2
3.4
3
3.3
7
3.4
6
3.4
9
3.5
0
3.3
9
3.5
2
3.5
4
3.5
1
3.4
4
3.4
8
K
0.0
8
0.0
9
0.0
9
0.0
9
0.0
8
0.1
1
0.2
2
0.2
3
0.2
4
0.2
3
0.2
5
0.2
2
0.2
5
0.2
0
0.2
6
0.2
0
0.2
1
0.2
0
P
0.0
9
0.1
0
0.0
9
0.0
6
0.0
8
0.1
1
0.0
9
0.0
9
0.0
8
0.0
8
0.0
9
0.0
7
0.1
5
0.0
9
0.0
6
0.0
7
0.0
9
0.1
1
Cr
K/T
i
0.1
0
0.1
2
0.1
2
0.1
2
0.1
0
0.1
3
0.2
7
0.2
7
0.2
9
0.2
6
0.3
4
0.2
5
0.2
8
0.2
4
0.3
1
0.2
3
0.2
4
0.2
4
Cl/
K
113
Mel
t in
clu
sion
s co
nti
nu
ed
Sam
ple
P
I18
c P
I18
c P
I18
c P
I18
c P
I18
c P
I18
c P
I18
c P
I18
c P
I18
c P
I18
c P
I18
c P
I18
c P
I18
c P
I18
c P
I18
c P
I18
c P
I18
c P
I18
c
Typ
e
E
E
E
E
E
E
E
E
E
E
E
E
E
E
E
E
E
E
(wt
%)
SiO
2
49
.70
49
.96
49
.73
49
.67
49
.77
50
.10
49
.60
49
.51
49
.83
50
.01
49
.69
49
.74
49
.42
49
.84
49
.71
49
.58
49
.51
49
.35
MgO
8.3
5
8.2
6
8.3
5
8.2
7
8.3
1
8.2
7
7.6
9
7.8
9
7.8
1
7.1
6
8.2
8
8.0
4
7.9
5
7.8
2
7.3
0
8.0
9
8.3
6
7.9
7
Mn
O
0
.17
0.1
7
0.1
5
0.1
6
0.1
5
0.1
6
0.1
5
0.1
9
0.1
7
0.1
5
0.1
2
0.1
9
0.1
8
0.1
2
0.1
8
0.1
6
0.1
3
0.1
8
CaO
13
.37
13
.53
13
.71
13
.55
13
.45
13
.48
14
.07
13
.93
13
.85
14
.52
13
.62
13
.97
14
.09
13
.96
14
.56
13
.59
13
.50
13
.76
FeO
*
9.5
7
9.5
8
9.7
8
9.8
0
9.8
3
9.7
1
9.8
8
9.6
9
9.0
8
10
.16
9.6
7
9.6
6
9.0
7
9.6
1
9.7
4
9.6
4
9.1
6
9.9
4
Al 2
O3
14
.73
14
.82
14
.77
14
.74
14
.70
14
.58
14
.75
14
.70
15
.83
14
.50
14
.67
14
.76
15
.75
15
.05
14
.68
14
.74
15
.80
15
.73
TiO
2
1
.18
1.2
0
1.1
7
1.1
4
1.2
1
1.2
1
1.2
1
1.2
1
0.9
9
1.2
2
1.2
5
1.2
5
1.1
1
1.1
8
1.2
1
1.1
4
1.1
0
1.0
0
Na 2
O
1
.90
1.9
1
1.9
5
1.8
7
1.9
2
1.9
1
1.8
4
1.7
9
1.8
1
1.7
9
1.8
7
1.8
4
1.8
2
1.8
3
1.8
0
1.8
3
1.8
5
1.8
3
K2O
0.1
9
0.2
1
0.1
7
0.1
9
0.1
9
0.1
8
0.1
7
0.1
7
0.1
7
0.1
6
0.2
0
0.1
9
0.1
6
0.1
9
0.1
6
0.2
1
0.1
3
0.1
3
P2O
5
0.1
4
0.1
2
0.1
3
0.1
3
0.0
7
0.1
0
0.1
1
0.1
2
0.1
6
0.1
4
0.1
2
0.0
7
0.1
4
0.0
7
0.0
8
0.1
3
0.1
3
0.0
8
Cr 2
O3
To
tal
9
9.3
0
99
.76
99
.91
99
.52
99
.60
99
.70
99
.47
99
.19
99
.69
99
.82
99
.49
99
.71
99
.69
99
.67
99
.42
99
.11
99
.67
99
.96
Cl
(pp
m)
S (
pp
m)
Cat
ion
s p
rop
ort
ion
s (1
00
cat
ion
s)
S
i 4
6.0
0
46
.04
45
.79
45
.93
46
.00
46
.24
46
.06
45
.95
45
.95
46
.43
46
.08
45
.89
45
.51
46
.20
46
.18
46
.06
45
.67
45
.40
Mg
11
.52
11
.35
11
.46
11
.40
11
.45
11
.38
10
.65
10
.92
10
.74
9.9
1
11
.45
11
.06
10
.92
10
.81
10
.11
11
.20
11
.50
10
.93
Mn
1.1
8
1.1
9
1.0
7
1.1
3
1.0
7
1.1
4
1.0
4
1.3
1
1.1
8
1.0
8
0.8
6
1.3
1
1.2
8
0.8
4
1.2
3
1.1
3
0.9
2
1.2
3
Ca
13
.26
13
.36
13
.53
13
.42
13
.32
13
.33
14
.00
13
.85
13
.68
14
.44
13
.53
13
.81
13
.90
13
.87
14
.49
13
.53
13
.34
13
.56
Fe
7.4
1
7.3
8
7.5
3
7.5
8
7.6
0
7.5
0
7.6
7
7.5
2
7.0
0
7.8
9
7.5
0
7.4
5
6.9
9
7.4
5
7.5
7
7.4
9
7.0
7
7.6
5
Al
16
.07
16
.10
16
.03
16
.06
16
.01
15
.86
16
.14
16
.08
17
.20
15
.87
16
.03
16
.05
17
.10
16
.44
16
.07
16
.14
17
.18
17
.06
Ti
0.8
2
0.8
3
0.8
1
0.7
9
0.8
4
0.8
4
0.8
5
0.8
4
0.6
8
0.8
5
0.8
7
0.8
7
0.7
7
0.8
2
0.8
5
0.8
0
0.7
6
0.6
9
Na
3.4
1
3.4
1
3.4
8
3.3
5
3.4
4
3.4
2
3.3
1
3.2
2
3.2
3
3.2
2
3.3
6
3.2
9
3.2
5
3.2
9
3.2
4
3.3
0
3.3
1
3.2
6
K
0.2
2
0.2
4
0.2
0
0.2
2
0.2
2
0.2
1
0.2
0
0.2
0
0.2
0
0.1
9
0.2
3
0.2
2
0.1
8
0.2
2
0.1
9
0.2
5
0.1
6
0.1
5
P
0.1
1
0.0
9
0.1
0
0.1
0
0.0
5
0.0
8
0.0
9
0.0
9
0.1
2
0.1
1
0.0
9
0.0
6
0.1
1
0.0
6
0.0
7
0.1
0
0.1
0
0.0
6
Cr
K/T
i
0.2
7
0.2
9
0.2
5
0.2
8
0.2
7
0.2
6
0.2
3
0.2
4
0.3
0
0.2
3
0.2
7
0.2
6
0.2
4
0.2
7
0.2
2
0.3
1
0.2
0
0.2
1
Cl/
K
114
Mel
t in
clu
sion
s co
nti
nu
ed
S
amp
le
PI1
9c
PI2
3c
PI2
3c
PI2
3c
PI2
3c
PI2
3c
PI2
3c
PI2
3c
PI2
3c
PI2
3c
PI2
3c
Typ
e
N
E
E
E
E
E
E
E
E
E
E
(wt
%)
S
iO2
48
.58
50
.30
49
.74
49
.57
49
.78
49
.48
49
.50
49
.12
49
.27
49
.05
48
.84
MgO
8.6
8
6.8
5
7.2
9
7.6
2
7.9
4
8.0
8
8.1
0
8.1
6
8.0
9
8.3
2
8.2
0
Mn
O
0
.17
0.1
6
0.1
4
0.1
7
0.1
7
0.1
6
0.1
4
0.1
7
0.1
7
0.1
6
0.1
5
CaO
13
.85
14
.13
14
.30
14
.23
14
.08
13
.79
14
.03
13
.88
13
.87
13
.96
13
.84
FeO
*
9.6
7
8.6
3
8.6
1
8.7
7
8.7
9
8.8
0
8.8
2
8.7
6
8.8
2
8.7
3
8.7
6
Al 2
O3
15
.25
16
.73
16
.27
16
.24
16
.16
16
.09
16
.07
15
.79
15
.64
15
.85
15
.81
TiO
2
1
.10
1.1
7
1.0
7
1.1
1
1.1
0
1.1
1
1.0
4
1.1
5
1.0
7
1.1
5
1.0
4
Na 2
O
1
.75
2.0
3
2.0
2
1.9
2
1.9
5
2.0
4
1.9
8
1.9
1
1.9
7
1.9
5
1.9
1
K2O
0.0
7
0.1
5
0.1
6
0.1
6
0.2
0
0.1
5
0.1
6
0.1
5
0.1
6
0.1
7
0.1
6
P2O
5
0.1
1
0.1
1
0.1
1
0.1
0
0.1
0
0.1
0
0.0
8
0.1
5
0.0
9
0.1
3
0.1
3
Cr 2
O3
T
ota
l
99
.23
10
0.2
6
99
.71
99
.89
10
0.2
7
99
.80
99
.92
99
.24
99
.15
99
.47
98
.84
Cl
(pp
m)
S
(pp
m)
C
atio
ns
pro
po
rtio
ns
(100
cat
ion
s)
Si
44
.94
46
.19
45
.89
45
.57
45
.53
45
.44
45
.46
45
.37
45
.54
45
.18
45
.31
Mg
11
.97
9.3
8
10
.03
10
.44
10
.83
11
.06
11
.09
11
.24
11
.15
11
.42
11
.34
Mn
1.1
9
1.1
1
0.9
8
1.1
8
1.1
8
1.1
1
0.9
7
1.1
9
1.1
9
1.1
2
1.0
5
Ca
13
.73
13
.90
14
.14
14
.02
13
.80
13
.57
13
.81
13
.74
13
.74
13
.78
13
.76
Fe
7.4
8
6.6
3
6.6
4
6.7
4
6.7
2
6.7
6
6.7
7
6.7
7
6.8
2
6.7
2
6.8
0
Al
16
.62
18
.11
17
.69
17
.59
17
.42
17
.41
17
.40
17
.19
17
.04
17
.20
17
.29
Ti
0.7
7
0.8
1
0.7
4
0.7
7
0.7
6
0.7
7
0.7
2
0.8
0
0.7
4
0.8
0
0.7
3
Na
3.1
4
3.6
1
3.6
1
3.4
2
3.4
6
3.6
3
3.5
3
3.4
2
3.5
3
3.4
8
3.4
4
K
0.0
8
0.1
8
0.1
9
0.1
9
0.2
3
0.1
8
0.1
9
0.1
8
0.1
9
0.2
0
0.1
9
P
0.0
9
0.0
9
0.0
9
0.0
8
0.0
8
0.0
8
0.0
6
0.1
2
0.0
7
0.1
0
0.1
0
Cr
K
/Ti
0
.11
0.2
2
0.2
5
0.2
4
0.3
1
0.2
3
0.2
6
0.2
2
0.2
5
0.2
5
0.2
6
Cl/
K
115
Table 4 Olivine-melt inclusion traverse for sample Db15/13. Major and minor
elements given as weight percent oxide and analyzed by electron microprobe.
Uncertainty was below 1% for major elements, checked by analyzing standards.
Mg number is defined as Mg/(Mg+Fe). All Fe as FeO*.
116
Oli
vin
e-m
elt
incl
usi
on
-oli
vin
e tr
aver
ses
Ph
ase
Oli
vin
e O
livin
e O
livin
e O
livin
e O
livin
e M
I M
I M
I M
I M
I M
I M
I M
I M
I M
I
Dis
tan
ce
(µm
) 0
1
0
20
30
40
50
60
70
80
90
10
0
11
0
12
0
13
0
14
0
SiO
2
40
.99
41
.01
40
.51
40
.46
49
.79
46
.33
49
.64
49
.56
49
.61
49
.52
49
.53
49
.76
49
.55
49
.58
49
.58
MgO
4
7.5
7
47
.99
47
.29
47
.14
6.4
8
13
.50
7.3
8
7.8
4
8.0
1
8.1
7
8.2
4
8.1
6
8.1
7
8.1
8
8.1
9
Mn
O
0.2
0
0.1
7
0.1
9
0.1
9
0.1
4
0.1
0
0.1
5
0.1
9
0.1
6
0.1
4
0.1
2
0.1
8
0.1
7
0.1
6
0.2
0
CaO
0
.33
0.3
3
0.3
4
0.3
8
14
.19
8.8
5
14
.37
14
.29
14
.08
14
.10
13
.99
13
.86
13
.98
13
.99
13
.95
FeO
*
11
.94
11
.87
12
.01
12
.61
9.2
2
10
.20
9.6
4
9.8
1
9.5
9
9.8
4
9.6
5
9.5
1
9.6
7
9.6
3
9.6
5
Al 2
O3
0.0
8
0.0
7
0.0
6
0.0
6
15
.86
13
.12
15
.52
15
.46
15
.44
15
.32
15
.50
15
.34
15
.36
15
.31
15
.29
TiO
2
0.0
1
0.0
0
0.0
0
0.0
1
1.1
8
1.1
0
1.1
9
1.1
5
1.1
4
1.2
2
1.1
1
1.1
3
1.2
5
1.1
2
1.1
5
Na 2
O
1.0
8
1.7
8
1.8
2
1.8
0
1.7
9
1.7
4
1.7
3
1.8
5
1.7
6
1.7
8
K2O
0.0
8
0.0
8
0.0
7
0.0
9
0.0
9
0.0
8
0.1
1
0.0
9
0.0
8
0.0
9
P2O
5
0.0
0
0.1
9
0.0
0
0.0
0
0.0
0
0.0
0
0.1
8
0.3
8
0.2
0
0.2
9
Cr 2
O3
0.0
4
0.0
6
0.0
6
0.0
7
0.0
6
0.0
6
0.0
7
0.0
5
0.0
6
0.0
9
NiO
0
.32
0.3
2
0.3
2
0.3
1
0.0
1
To
tal
10
1.4
4
10
1.7
5
10
0.7
2
10
1.1
6
96
.87
94
.40
10
0.0
0
10
0.2
6
99
.98
10
0.2
3
10
0.0
3
10
0.0
3
10
0.5
3
10
0.0
7
10
0.2
7
Cat
ion
pro
po
rtio
n (
10
0 c
atio
ns)
S
i 3
3.0
3
32
.96
32
.88
32
.77
48
.34
44
.67
45
.88
45
.48
45
.70
45
.58
45
.69
45
.78
45
.38
45
.63
45
.46
Mg
57
.13
57
.50
57
.22
56
.92
9.3
8
19
.41
10
.17
10
.73
11
.00
11
.20
11
.32
11
.19
11
.16
11
.22
11
.19
Mn
1.2
3
1.0
0
1.1
9
1.1
7
1.0
3
0.6
9
1.0
4
1.3
3
1.1
0
0.9
5
0.8
4
1.2
3
1.1
7
1.1
3
1.3
5
Ca
0.2
8
0.2
9
0.2
9
0.3
3
14
.75
9.1
5
14
.24
14
.05
13
.90
13
.90
13
.83
13
.66
13
.71
13
.79
13
.71
Fe
8.0
5
7.9
8
8.1
5
8.5
4
7.4
8
8.2
3
7.4
6
7.5
3
7.3
9
7.5
7
7.4
4
7.3
1
7.4
1
7.4
2
7.4
0
Al
0.0
7
0.0
7
0.0
6
0.0
5
18
.15
14
.91
16
.91
16
.72
16
.76
16
.62
16
.85
16
.64
16
.58
16
.61
16
.53
Ti
0.0
0
0.0
0
0.0
0
0.0
1
0.8
6
0.8
0
0.8
3
0.8
0
0.7
9
0.8
5
0.7
7
0.7
8
0.8
6
0.7
7
0.8
0
Na
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
2.0
2
3.1
9
3.2
4
3.2
1
3.1
9
3.1
2
3.0
8
3.2
9
3.1
3
3.1
6
K
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
9
0.1
0
0.0
9
0.1
0
0.1
0
0.0
9
0.1
2
0.1
1
0.0
9
0.1
1
P
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.1
4
0.0
0
0.0
0
0.0
0
0.0
0
0.1
4
0.2
9
0.1
6
0.2
3
Cr
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
3
0.0
5
0.0
4
0.0
5
0.0
4
0.0
5
0.0
5
0.0
4
0.0
4
0.0
6
Ni
0.2
1
0.2
0
0.2
1
0.2
0
0.0
1
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
Fe/
Mg
0.1
4
0.1
4
0.1
4
0.1
5
0.8
0
0.4
2
0.7
3
0.7
0
0.6
7
0.6
8
0.6
6
0.6
5
0.6
6
0.6
6
0.6
6
Mg n
um
ber
8
7.6
5
87
.82
87
.53
86
.95
55
.64
70
.23
57
.71
58
.76
59
.81
59
.68
60
.34
60
.48
60
.10
60
.21
60
.19
117
Oli
vin
e-m
elt
incl
usi
on
-oli
vin
e tr
aver
ses
con
tin
ued
Ph
ase
MI
MI
MI
MI
Oli
vin
e O
livin
e O
livin
e O
livin
e O
livin
e
Dis
tan
ce (
µm
) 1
50
16
0
17
0
18
0
19
0
20
0
21
0
22
0
23
0
SiO
2
49
.56
49
.47
49
.67
43
.20
40
.99
40
.99
40
.87
40
.86
40
.96
MgO
7
.99
7.7
6
6.8
3
36
.76
45
.05
47
.49
47
.59
47
.41
47
.76
Mn
O
0.1
8
0.1
8
0.2
1
0.1
6
0.2
0
0.2
0
0.1
9
0.2
0
0.1
8
CaO
1
4.1
2
14
.40
14
.54
3.0
6
0.4
5
0.3
4
0.3
3
0.3
5
0.3
4
FeO
*
9.6
8
10
.04
9.6
6
12
.78
12
.92
11
.95
11
.84
11
.84
11
.90
Al 2
O3
15
.26
15
.42
15
.71
4.3
8
0.3
4
0.0
5
0.0
6
0.0
5
0.0
4
TiO
2
1.0
5
1.2
0
1.1
5
0.1
8
0.0
2
0.0
1
0.0
0
0.0
0
0.0
1
Na 2
O
1.7
7
1.7
9
1.8
8
0.4
8
K
2O
0
.08
0.0
9
0.0
9
0.0
5
P
2O
5
0.0
0
0.1
4
0.0
7
0.2
2
C
r 2O
3
0.0
7
0.0
9
0.0
8
0.0
4
N
iO
0.2
8
0.3
2
0.3
2
0.3
2
0.3
3
To
tal
99
.76
10
0.5
8
99
.87
10
1.2
9
10
0.2
5
10
1.3
4
10
1.2
0
10
1.0
3
10
1.5
1
Cat
ion
pro
po
rtio
n (
10
0 c
atio
ns)
Si
45
.71
45
.36
45
.86
36
.10
33
.72
33
.07
32
.99
33
.05
33
.00
Mg
10
.99
10
.61
9.4
0
45
.79
55
.24
57
.11
57
.28
57
.17
57
.35
Mn
1.2
4
1.2
4
1.4
3
1.0
1
1.2
3
1.2
2
1.1
7
1.2
1
1.1
0
Ca
13
.96
14
.15
14
.38
2.7
4
0.4
0
0.2
9
0.2
9
0.3
1
0.2
9
Fe
7.4
7
7.7
0
7.4
6
8.9
3
8.8
9
8.0
6
7.9
9
8.0
1
8.0
1
Al
16
.59
16
.66
17
.09
4.3
2
0.3
3
0.0
5
0.0
6
0.0
4
0.0
4
Ti
0.7
3
0.8
3
0.8
0
0.1
1
0.0
1
0.0
1
0.0
0
0.0
0
0.0
0
Na
3.1
6
3.1
9
3.3
6
0.7
7
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
K
0.1
0
0.1
0
0.1
0
0.0
5
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
P
0.0
0
0.1
1
0.0
5
0.1
6
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
Cr
0.0
5
0.0
6
0.0
6
0.0
2
0.0
0
0.0
0
0.0
0
0.0
0
0.0
0
Ni
0.0
0
0.0
0
0.0
0
0.0
0
0.1
9
0.2
1
0.2
1
0.2
1
0.2
2
Fe/
Mg
0.6
8
0.7
3
0.7
9
0.1
9
0.1
6
0.1
4
0.1
4
0.1
4
0.1
4
Mg n
um
ber
5
9.5
3
57
.95
55
.77
83
.68
86
.14
87
.63
87
.76
87
.71
87
.74
118
Table 5 Pillow margin matrix glass volatile chemistry. Volatile ratios obtained
using secondary ion mass spectrometry (SIMS). Concentrations calculated using
SIMS ratio data and calibration curves and corrected for background volatiles (see
Methods). Error propagation calculated as error on calibration curve slope,
concentration and (for H2O) y-intercept.
119
Pil
low
mar
gin
mat
rix g
lass
vo
lati
les
Sam
ple
A
k1
2/2
mtx
A
Ak1
2/2
mtx
B
Ak1
2/6
mtx
D
b1
5/2
6m
tx
PI1
7/1
8m
txA
P
I17
/18
mtx
B
Typ
e N
N
N
N
E
E
(pp
m)
CO
2
0
0
0
0
2
11
2
H2O
(w
t %
) 0
0
0
0
0
0
F
73
72
74
83
13
4
14
1
S
71
73
75
18
41
42
Cl
18
18
20
27
64
66
Pro
pag
ated
err
or6
CO
2
0
0
0
0
11
6
11
4
H2O
(w
t %
) 1
2
3
1
3
1
F
28
28
28
28
30
15
3
S
4
4
5
2
3
35
Cl
4
4
4
4
5
66
Co
rrec
ted
SIM
S r
atio
C/ S
i -2
.56
E-0
3
-3.0
4E
-03
-2.0
5E
-03
-2.8
6E
-03
1.4
0E
-04
8.0
9E
-03
OH/ S
i 5
.20
E-0
2
2.1
5E
-02
-1.6
5E
-02
-4.0
0E
-02
-1.7
0E
-02
6.6
0E
-02
F/ S
i 2
.13
E-0
1
2.1
3E
-01
2.1
8E
-01
2.4
5E
-01
3.9
4E
-01
4.1
4E
-01
S/ S
i 1
.15
E-0
1
1.1
8E
-01
1.2
0E
-01
2.8
2E
-02
6.6
0E
-02
6.7
2E
-02
Cl / S
i 2
.60
E-0
2
2.6
0E
-02
2.7
8E
-02
3.8
1E
-02
9.1
1E
-02
9.3
0E
-02
Err
or
on
SIM
S r
aw r
atio
C/ S
i
3.8
4E
-03
3.8
3E
-03
3.8
6E
-03
3.8
5E
-03
4.1
8E
-03
4.1
3E
-03
OH/ S
i
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
4.6
3E
-01
F/ S
i 3
.96
E-0
2
3.9
6E
-02
3.9
8E
-02
3.9
6E
-02
3.9
7E
-02
2.2
3E
-01
S/ S
i 1
.48
E-0
3
1.2
8E
-03
1.4
8E
-03
1.1
3E
-03
1.4
9E
-03
2.7
7E
-02
Cl / S
i 2
.93
E-0
3
2.9
3E
-03
2.9
5E
-03
2.9
5E
-03
3.1
6E
-03
4.7
0E
-02
120
Table 6 Melt inclusion volatile chemistry. Volatile ratios obtained using
secondary ion mass spectrometry (SIMS). Concentrations calculated using SIMS
ratio data and calibration curves and corrected for background volatiles (see
Methods). Error propagation calculated as error on calibration curve slope,
concentration and (for H2O) y-intercept.
121
Mel
t in
clu
sion
vo
lati
les
Sam
ple
A
k1
2/i
4
Ak1
2/i
7
Ak1
2/i
9
Ak1
2/i
11
Ak1
2/i
16
Ak1
2/i
24
Db
15
/i7
Db
15
/i10
Db
15
/i12
Db
15
/i18
Db
15
/i26
.1
Typ
e
N
N
N
N
N
N
E
N
N
N
N
(pp
m)
C
O2
24
16
17
4
16
40
11
57
0
36
23
9
41
1
45
4
16
H2O
(w
t %
) 0
.0
0.0
0
.0
0.0
0
.0
0.0
0
.0
0.0
0
.0
0.0
0
.0
F
54
11
64
55
73
77
96
76
46
79
61
S
12
0
12
1
16
1
15
1
19
9
15
0
80
1
23
0
83
11
2
71
Cl
15
5
20
13
18
20
50
30
23
30
23
Pro
pag
ated
err
or
C
O2
19
01
19
6
59
7
11
0
10
8
0
10
7
11
3
32
7
29
8
13
7
H2O
(w
t %
) 1
1
0
0
0
2
5
1
1
0
2
2
F
28
27
28
28
28
28
28
28
27
28
28
S
7
8
9
9
12
9
45
14
5
7
4
Cl
4
5
4
4
4
4
4
4
4
4
4
SIM
S r
atio
C/ S
i 1
.75
E-0
1
1.2
6E
-02
1.1
8E
-01
7.8
7E
-04
4.1
4E
-03
-7.9
2E
-04
2.6
0E
-03
1.7
2E
-02
2.9
7E
-02
3.2
8E
-02
1.1
4E
-03
OH/ S
i 2
.73
E-0
2
3.6
2E
-02
9.0
5E
-02
6.5
2E
-02
6.7
6E
-02
1.8
8E
-03
-4.4
7E
-02
-4.4
7E
-02
1.4
3E
-01
2.0
8E
-02
-3.0
6E
-02
F/ S
i 1
.60
E-0
1
3.3
1E
-02
1.8
9E
-01
1.6
2E
-01
2.1
4E
-01
2.2
7E
-01
2.8
3E
-01
2.2
3E
-01
1.3
5E
-01
2.3
2E
-01
1.7
8E
-01
S/ S
i 1
.93
E-0
1
1.9
4E
-01
2.5
8E
-01
2.4
2E
-01
3.1
9E
-01
2.4
1E
-01
1.2
9E
+00
3.6
9E
-01
1.3
3E
-01
1.8
0E
-01
1.1
3E
-01
Cl / S
i 2
.18
E-0
2
7.5
4E
-03
2.8
4E
-02
1.8
1E
-02
2.4
9E
-02
2.8
0E
-02
7.1
0E
-02
4.3
2E
-02
3.2
1E
-02
4.2
3E
-02
3.3
0E
-02
Err
or
on
SIM
S r
aw r
atio
C/ S
i 6
.87
E-0
2
7.0
7E
-03
2.1
6E
-02
3.9
8E
-03
3.8
9E
-03
3.8
3E
-03
3.8
6E
-03
4.0
6E
-03
1.1
8E
-02
1.0
8E
-02
4.9
6E
-03
OH/ S
i
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
F/ S
i
3.9
7E
-02
3.9
5E
-02
3.9
5E
-02
3.9
6E
-02
3.9
7E
-02
3.9
6E
-02
3.9
6E
-02
3.9
7E
-02
3.9
6E
-02
3.9
6E
-02
3.9
5E
-02
S/ S
i
1.5
2E
-03
2.8
5E
-03
2.0
6E
-03
1.7
1E
-03
2.2
6E
-03
2.0
7E
-03
4.0
2E
-03
3.9
9E
-03
1.7
0E
-03
1.4
8E
-03
1.2
8E
-03
Cl / S
i 2
.99
E-0
3
3.5
3E
-03
2.9
7E
-03
3.0
1E
-03
2.9
7E
-03
2.9
5E
-03
2.9
7E
-03
3.0
9E
-03
2.9
4E
-03
2.9
7E
-03
2.9
7E
-03
122
Mel
t in
clu
sion
vo
lati
les
con
tinu
ed
S
amp
le
Pd
13
/i1
2
Pd
13
/i1
5
Pd
13
/i1
8.1
P
d13
/i1
8.2
P
d19
/i3
Pd
19
/i6
.1
Pd
19
/i6
.2
Pd
19
/i1
1
PI1
7/i
1
PI1
7/i
2
PI1
7/i
5
Typ
e
N
N
N
N
N
N
N
N
E
E
E
(pp
m)
C
O2
4
0
48
24
22
56
13
64
44
7
70
12
44
78
12
76
H2O
(w
t %
) 0
.0
0.0
0
.0
0.0
0
.1
0.0
0
.0
0.0
0
.0
0.0
0
.0
F
99
79
10
2
45
10
2
6
11
0
3
81
12
2
70
S
77
10
2
38
5
10
2
11
2
9
15
1
1
26
8
14
5
85
Cl
29
21
23
12
64
15
23
1
25
54
36
Pro
pag
ated
err
or
C
O2
11
0
0
10
9
10
8
71
0
54
4
35
4
11
6
15
23
12
4
25
3
H2O
(w
t %
) 1
1
1
1
0
0
0
0
1
1
0
F
29
28
29
27
31
27
29
27
28
29
28
S
5
6
22
6
15
2
10
2
16
8
5
Cl
4
4
4
4
17
9
8
4
4
4
5
SIM
S r
atio
C/ S
i 2
.73
E-0
4
-1.5
4E
-03
3.5
0E
-03
1.7
1E
-03
1.6
3E
-01
9.8
5E
-02
3.2
3E
-02
5.0
6E
-03
8.9
9E
-02
5.6
3E
-03
9.2
2E
-02
OH/ S
i 3
.65
E-0
2
-6.8
5E
-02
-4.5
8E
-02
-6.6
1E
-02
4.5
9E
-01
1.8
9E
-01
1.2
7E
-01
1.4
1E
-01
4.5
0E
-02
-7.9
3E
-02
1.5
7E
-01
F/ S
i 2
.89
E-0
1
2.3
2E
-01
2.9
9E
-01
1.3
2E
-01
2.9
9E
-01
1.6
4E
-02
3.2
2E
-01
8.9
3E
-03
2.3
8E
-01
3.5
7E
-01
2.0
6E
-01
S/ S
i 1
.24
E-0
1
1.6
5E
-01
6.1
8E
-01
1.6
4E
-01
1.8
0E
-01
1.4
6E
-02
2.4
3E
-01
8.3
2E
-04
4.3
0E
-01
2.3
3E
-01
1.3
7E
-01
Cl / S
i 4
.10
E-0
2
3.0
3E
-02
3.2
5E
-02
1.6
5E
-02
9.0
3E
-02
2.1
6E
-02
3.2
3E
-02
1.2
0E
-03
3.5
8E
-02
7.6
8E
-02
5.0
7E
-02
Err
or
on
SIM
S r
aw r
atio
C/ S
i 3
.97
E-0
3
3.8
5E
-03
3.9
4E
-03
3.8
9E
-03
2.5
6E
-02
1.9
6E
-02
1.2
8E
-02
4.1
8E
-03
5.5
0E
-02
4.4
7E
-03
9.1
5E
-03
OH/ S
i
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
3.2
2E
-01
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
F/ S
i
4.0
0E
-02
3.9
7E
-02
3.9
7E
-02
3.9
7E
-02
4.2
7E
-02
3.9
9E
-02
4.0
3E
-02
3.9
9E
-02
3.9
5E
-02
3.9
6E
-02
4.0
5E
-02
S/ S
i
2.5
0E
-03
1.9
9E
-03
3.0
9E
-03
1.4
9E
-03
1.0
5E
-02
1.8
9E
-03
3.7
4E
-03
1.3
6E
-03
4.3
6E
-03
1.4
5E
-03
1.7
1E
-03
Cl / S
i 2
.99
E-0
3
2.9
7E
-03
2.9
5E
-03
2.9
4E
-03
1.1
7E
-02
6.4
2E
-03
5.6
0E
-03
2.9
9E
-03
2.9
5E
-03
2.9
4E
-03
3.1
6E
-03
123
Mel
t in
clu
sion
vo
lati
les
con
tinu
ed
S
amp
le
PI1
7/i
9.1
P
I17
/i9
.2
PI1
7/i
13
.1
PI1
7/i
13
.2
PI1
7/i
14
PI1
7/i
18
PI1
7/i
19
PI1
7/i
20
.1
PI1
7/i
20
.2
Typ
e
E
N
E
E
E
E
E
E
E
(pp
m)
C
O2
85
8
45
8
12
9
10
46
74
12
89
19
71
76
0
H2O
(w
t %
) 0
.0
0.0
0
.0
0.0
0
.0
0.0
0
.0
0.0
0
.0
F
10
5
91
18
3
14
2
11
8
12
5
11
4
13
0
13
1
S
41
2
43
7
24
0
56
51
5
38
8
19
0
16
0
16
3
Cl
28
16
15
9
79
27
51
82
60
64
Pro
pag
ated
err
or
C
O2
73
5
24
1
13
5
58
7
11
4
16
1
15
0
10
8
0
H2O
(w
t %
) 1
1
3
2
1
3
2
6
1
F
29
28
32
30
29
29
29
30
30
S
24
25
14
4
29
22
11
9
9
Cl
5
4
7
12
4
5
5
4
4
SIM
S r
atio
C/ S
i 6
.20
E-0
2
3.3
1E
-02
9.3
3E
-03
7.5
6E
-02
5.3
1E
-03
9.3
2E
-02
1.4
2E
-01
5.4
7E
-03
-1.2
0E
-03
OH/ S
i 3
.60
E-0
2
5.3
0E
-02
1.5
8E
-02
-2.7
0E
-02
-1.2
3E
-01
1.4
8E
-02
2.1
0E
-02
-8.5
6E
-03
-6.2
2E
-02
F/ S
i 3
.08
E-0
1
2.6
8E
-01
5.3
6E
-01
4.1
6E
-01
3.4
8E
-01
3.6
8E
-01
3.3
4E
-01
3.8
3E
-01
3.8
6E
-01
S/ S
i 6
.61
E-0
1
7.0
2E
-01
3.8
6E
-01
9.0
2E
-02
8.2
7E
-01
6.2
4E
-01
3.0
5E
-01
2.5
7E
-01
2.6
3E
-01
Cl / S
i 3
.93
E-0
2
2.3
2E
-02
2.2
6E
-01
1.1
2E
-01
3.7
7E
-02
7.2
8E
-02
1.1
7E
-01
8.5
8E
-02
9.1
0E
-02
Err
or
on
SIM
S r
aw r
atio
C/ S
i 2
.66
E-0
2
8.7
1E
-03
4.8
9E
-03
2.1
2E
-02
4.1
3E
-03
5.8
3E
-03
5.4
0E
-03
3.8
9E
-03
3.8
7E
-03
OH/ S
i
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
3.2
1E
-01
F/ S
i
4.0
0E
-02
3.9
6E
-02
3.9
8E
-02
3.9
7E
-02
3.9
6E
-02
3.9
7E
-02
3.9
6E
-02
3.9
6E
-02
3.9
7E
-02
S/ S
i
3.5
8E
-03
4.2
3E
-03
2.6
3E
-03
2.2
5E
-03
3.1
8E
-03
2.7
6E
-03
2.1
1E
-03
1.7
9E
-03
1.4
3E
-03
Cl / S
i 3
.70
E-0
3
2.9
4E
-03
4.8
0E
-03
8.6
4E
-03
2.9
7E
-03
3.5
3E
-03
3.1
2E
-03
2.9
7E
-03
2.9
9E
-03
124
Table 7 Geochemical models. See Appendix 1.1 for methods and details.
125
Geo
chem
ical
model
ing
Sta
rtin
g
Com
posi
tion
Ass
imil
ant
1
Ass
imil
ant
2
Ass
imil
ant
3
Pd19
(Bulk
rock
)
*B
affi
n I
slan
d
gra
nit
e
**A
lter
ed b
asal
t
(1 w
t% H
2O
added
)
**
Alt
ered
bas
alt
(5 w
t% H
2O
add
ed)
Fra
ctio
nat
ion
(wt
%)
SiO
2
44.9
3
68.0
0
59.2
8
57
.01
MgO
22.0
4
0.6
7
2.6
3
2.5
3
Mn
O
0.1
8
0.0
4
0.1
9
0.1
8
CaO
9.0
3
2.7
2
1.3
9
1.3
4
FeO
*
10.4
2
3.4
2
3.2
9
Fe 2
O3
2.2
0
0.4
1
0.3
9
FeO
3.0
1
2.8
9
Al 2
O3
10.4
5
15.8
0
19.4
3
18
.69
TiO
2
0.7
9
0.3
9
2.6
5
2.5
5
Na 2
O
0.9
1
3.8
0
2.3
2
2.2
4
K2O
0.0
2
4.4
3
7.2
5
6.9
7
P2O
5
0.0
6
0.1
1
0.4
4
0.4
3
H2O
1.8
4
0.9
9
4.7
8
Cl
(pp
m)
2000.0
2
00
0.0
K/T
i
Cl/
K
*
Sam
ple
95T
-511 f
rom
Ther
iault
et
al 2
003
* *
Sam
ple
d 8
01B
-37R
-1 f
rom
Kel
ley e
t al
. 2003 w
ith S
ite
801 C
l co
nte
nts
fro
m B
arn
es e
t
al. 2
012
126
Geo
chem
ical
model
ing
conti
nu
ed
Ass
imil
ant
1
Ass
imil
ant
2
Ass
imil
ant
3
1 %
Co
nta
min
atio
n
1 %
Conta
min
atio
n
10 %
Conta
min
atio
n
10 %
Conta
min
atio
n
20 %
Conta
min
atio
n
10
%
Co
nta
min
atio
n
50
%
Co
nta
min
atio
n
Fra
ctio
nat
ion
35
.1 %
80.6
%
5.3
%
4.4
%
4.4
%
4.4
%
4.4
%
(wt
%)
S
iO2
40
.75
52.3
1
40.8
2
40.7
4
40.7
8
40
.72
40
.80
MgO
6.9
1
1.7
1
18.1
2
18.4
5
18.0
1
18
.44
16
.47
MnO
0.1
7
0.3
3
0.1
7
0.1
7
0.1
7
0.1
7
0.1
7
CaO
11
.71
20.1
8
8.5
9
8.5
1
8.5
2
8.5
1
8.4
5
FeO
*
9.5
0
19.9
2
9.5
3
9.5
3
9.4
9
9.5
2
9.2
6
Fe 2
O3
F
eO
A
l 2O
3
27
.32
0.5
1
20.0
5
19.8
9
20.1
5
19
.88
20
.99
TiO
2
1.0
5
4.1
1
0.7
5
0.7
6
0.7
8
0.7
6
0.8
4
Na 2
O
2
.39
0.1
0
1.7
7
1.7
4
1.7
7
1.7
4
1.8
8
K2O
0.0
5
0.2
1
0.0
9
0.1
0
0.2
0
0.1
0
0.6
0
P2O
5
0.1
6
0.6
2
0.1
2
0.1
2
0.1
2
0.1
2
0.1
5
H2O
C
l (p
pm
)
40
41
40
41
K/T
i 0
.08
6
0.0
86
0.2
0.2
3
0.4
3
0.2
3
1.2
Cl/
K
0.0
3
0.0
003
2
0.0
36
0.0
06
127
Appendix 1. Supplementary methods information regarding modeling and SIMS
sample preparation.
128
1.1 Modeling crystal fractionation and crustal contamination
Both MELTS (Asimow & Ghiorso 1998) and XSTALN, a thermodynamic
modeling program by Don Francis, were used in this study to model crystal
fractionation and contamination in order to determine if these processes can
reproduce the K/Ti ratios in the Baffin suite. To see the effects of crystal
fractionation on the K/Ti ratio, sample Db14/3 was used as a representative N-
type starting composition in MELTS and the temperature was decreased from the
liquidus, ~1220 °C, in 20 ° C steps to ~1050 °C (i.e., approximate eruption
temperature calculated using the Nielsen and Dungan [1983] two-lattice mixing
model). In MELTS, olivine and plagioclase were crystallized (where the timing of
crystallization is determined by the program itself) and in XSTALN, olivine was
made to crystallize first, followed by olivine and plagioclase in the proportion
70:30 (olivine:plagioclase), an approximation of their cotectic proportions at that
temperature. The results obtained from these two modeling programs are shown
in Table 7.
To model the effects of contamination of granitic crust on the variation of
K/Ti and Cl/K, our starting composition was whole rock sample Pd-19 (22 wt %
MgO) and we used Baffin sample 95T-511 from Thériault et al. (2003) as the
contaminant composition (Table 7). In both MELTS and XSTALN, we increased
the percent of added contaminant until a K/Ti ratio of 0.2 was achieved (i.e., the
lowest E-type K/Ti ratio). To model the effects of contamination of
hydrothermally altered oceanic crust on the variation of K/Ti and Cl/K using Pd-
19 again, we used the major element composition from Kelley et al.’s (2003)
sample 801B-37R-1 with an average Cl content (0.02 wt %) for the same
129
sampling site (Site 801) from Barnes et al. (2012). As the major element
composition did not include water, 1 wt % and 5 wt % H2O were each added by
diluting the other oxides accordingly. Using both modeling programs, we
modeled the addition of each of these contaminants with concurrent fractionation
of olivine and plagioclase until a K/Ti ratio of 0.2 and a Cl/K of 0.08 (i.e., the
highest mantle value) was achieved. In XSTALN, olivine was crystalized first
followed by olivine + plagioclase in their cotectic proportions.
1.2 SIMS sample preparation
The five samples chosen for SIMS analysis were pulverized to ~500
micron fragments (approximately the size of an average olivine phenocryst). The
crushed margins were then sieved and 400-500 μm and 500-600 μm sized crystals
were used to make grain mounts. The sieved crystals were immersed in water-
soluble glycerine on blank slides under the microscope, and olivines hosting the
largest melt inclusions with the smallest shrinkage bubbles were extracted with
tweezers for SIMS analysis. Unlike microprobe analysis, melt inclusions less than
60 µm were also selected as these had no visible shrinkage bubbles. These olivine
crystals were then mounted using Stuers EpoFix epoxy in a one-inch external
diameter aluminum ring and ground until the first desired melt inclusion was
exposed. A second epoxy mount was created by removing olivine crystals as their
melt inclusions were exposed by further grinding with 600 grit paper. Olivines
were removed by hand using a soldering iron, with care was paid to avoid
fracturing the crystals. The melt inclusions were examined using transmitted and
reflected light to avoid shrinkage bubbles and/or cracks. In the case of the larger
130
melt inclusions (>60 μm diameter), however, shrinkage bubbles were almost
always present. This second mount was polished with 800- and then 1200-grit
abrasive paper, and finally with 1 micron alumina paste, rinsing in a sonic bath
between grinding steps. The crystals were then individually removed by hand
from the epoxy with a soldering iron and placed in an indium mount. Special
attention was paid to ensure that the olivine crystals were placed such that the
exposed and polished melt inclusions were flat. Once all the crystals were placed
in the indium mount, the mount was placed in a metal press for 15 minutes at a
time to ensure the grains were secured in the indium and that all inclusions were
indeed flat. The indium mount was cleaned with 0.3 μm diamond paste and rinsed
with Milli-Q water and compressed air several times to remove any paste that may
have remained between the crystals and indium. The indium mount was dried in a
vacuum oven at 110°C and 10-3
torr for at least 12 hours, gold-coated, then stored
in a 10-7
torr vacuum for 24 hours before the commencement of SIMS analysis.
1.3 Modeling crystallization depth estimation using the SolEx program
Since the water contents of the melt inclusions and pillow margin glasses
are below the background volatile levels, the SolEx CO2-H2O model for
crystallization depth/ depth of melt inclusion formation cannot be directly applied
with the observed water concentrations. This program is relatively insensitive to
changes in water content, however (i.e., the slope on a CO2 vs. H2O graph is
almost zero at low water contents), and so the SolEx program was used to
calculate CO2 solubility at the minimum water content (0.0001 wt % H2O [100
ppm]) the program would run. Melt inclusion Db15/i18 was used as a starting
131
composition to calculate the SolEx isobars, as it has a K/Ti ratio of 0.18 (and so is
not strongly E- nor strongly N-type) and has been analyzed for volatiles. The
SolEx program was run at an oxygen fugacity of NNO +0.5, and at a temperature
of ~1200°C.
132
Appendix 2. Olivine volatile ratios obtained using secondary ion mass
spectrometry (SIMS). Concentrations calculated using SIMS ratio data and
calibration curves. Error propagation calculated as error on calibration curve
slope, concentration and (for H2O) y-intercept. Cl concentrations are low in
olivine, therefore the standard deviation is large, causing unrealistic errors.
133
Olivine volatile blanks
Sample PI17/18 Pd19/8 Ak12/6a Pd13/15a
(ppm)
CO2 64 107 154 153
H2O (wt %) 0.13 0.26 0.21 0.27
F 22 35 29 34
S 1 1 1 2
Cl 1 1 1 1
Propagated error8
CO2 105 454 74 193
H2O (wt %) 0 0 0 0
F 2 3 3 3
S 1 1 1 1
Cl9 1417889 918218 1393882 1091427
SIMS raw ratio
C/Si 4.64E-03 7.76E-03 1.11E-02 1.10E-02 OH/Si 5.48E-01 8.85E-01 7.51E-01 9.04E-01
F/Si 6.50E-02 1.03E-01 8.56E-02 1.00E-01
S/Si 1.54E-03 2.32E-03 2.33E-03 2.83E-03
Cl/Si 9.75E-04 1.47E-03 1.42E-03 2.13E-03
Standard deviations on SIMS raw ratio
C/Si 1 sigma 3.81E-03 1.64E-02 2.67E-03 6.96E-03
OH/Si 1 sigma 3.46E-03 7.38E-03 3.89E-03 9.39E-03
F/Si 1 sigma 5.45E-04 1.00E-03 6.01E-04 1.20E-03
S/Si 1 sigma 4.47E-04 5.02E-04 5.37E-04 1.05E-03
Cl/Si 1 sigma 1.01E+03 6.51E+02 9.89E+02 7.74E+02
134
Appendix 3. P1326-2 glass standard composition, used to monitor SIMS
reproducibility. Major elements and trace elements analyzed by electron
microprobe. All Fe as FeO*. Concentrations calculated using SIMS ratio data and
calibration curves and corrected for background volatiles (see Methodology).
Error propagation calculated as error on calibration curve slope, concentration and
(for H2O) y-intercept.
135
P1326-2 Standard
Sample P1326-2 Propagated error
(wt %)
SiO2 49.17
MgO 7.55
MnO 0.19
CaO 12.32
FeO* 10.76
Al2O3 14.70
TiO2 1.56
Na2O 2.80
K2O 0.20
Cr2O3 0.01
Total 99.65
CO2 (ppm) 291 3.8
H2O (wt %) 0.068 0.0002
F (ppm) 150 0.45
S (ppm) 1448 2
Cl (ppm) 190 0.35
Cations proportions (100 cations)
Si 45.41
Mg 10.40
Mn 1.33
Ca 12.19
Fe 8.31
Al 16.00
Ti 1.08
Na 5.01
K 0.24
Cr 0.01
Total: 100.00
136
Appendix 4 Electron microprobe detection limits for major and minor elements.
137
Detection limits
Electron Microprobe
Glass Olivine
ppm ppm
Si 376 429
Mg 384 281
Mn 756 331
Ca 421 130
Fe 855 221
Al 340 333
Ti 1483 251
Ni n/a 133
Na 466 n/a
K 321 n/a
P 401* n/a
Cr 447 432
S 233 n/a
Cl 52 n/a
*D.L. is 2165 ppm for samples Ak2, Ak12, Ak11a, PI12 and
Db15
138
Appendix 5 Electron microprobe reproducibility data for major and minor
elements.
139
Microprobe glass data reproducibility using standard VG-2
K2O TiO2 K/Ti
Average 1s Average 1s Average 1s
Apr-11 0.22 0.013 1.81 0.072 0.20 0.017
Jul-11 0.21 0.014 1.91 0.10 0.19 0.006
Aug-11 0.21 0.010 1.86 0.070 0.20 0.014
Dec-11 0.21 0.0074 1.82 0.097 0.20 0.012
All 0.21 0.010 1.85 0.090 0.20 0.013
Microprobe olivine data reproducibility using an olivine standard
MgO FeO
Date Average Percent
difference Average
Percent
difference
Jul-11 51.02 0.57 7.70 0.34
Aug-11 51.07 0.06 7.78 0.40