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Major and trace element geochemistry of ilmenite suites from the
Kimberley diamond mines, South Africa
by
Vlad-Victor Ene
A thesis submitted in conformity with the requirements
for the degree of Master of Applied Sciences
Department Of Earth Sciences
University Of Toronto
© Copyright by Vlad Victor Ene, 2014
ii
Major and trace element geochemistry of ilmenite suites from the
Kimberley diamond mines, South Africa
Vlad-Victor Ene
Master of Applied Science
Department of Earth Sciences
University of Toronto
2014
Abstract A method was developed to distinguish between ilmenites from different mantle xenoliths found
at Kimberley, South Africa: Granny Smith, dunites, orthopyroxenites, MARID and rutile-ilmenite
intergrowths. The method employs a number of oxide screens based on MgO, TiO2 and Cr2O3 and
systematically eliminating whole fields defined by mathematical equations. The classification
scheme is useful to better understand the source of the ilmenite and has been applied to ilmenite
xenocrysts from four diamond mines in the Kimberley area: Bultfontein, Kamfersdam, Otto’s
Kopje and Wesselton. A relationship between ilmenite chemistry and its paragenesis exists, but it
is not as clear as in the Cr-poor megacrysts. A more complex process is responsible for the
crystallization of ilmenite in the five different suites at Kimberley, and metasomatim by a Fe-Ti
rich magma or melt, similar in composition to the parent magma of the South African megacrysts,
plays an important role in ilmenite formation.
iii
Table of Contents
1. INTRODUCTION ..................................................................................................................................... 1
2. ANALYTICAL METHODS ................................................................................................................... 2 2.1 Microprobe analysis ................................................................................................................................... 3 2.2 Laser Ablation Inductively-Coupled Plasma Mass Spectrometry ............................................................. 3 2.3 Scanning Electron Microscope ................................................................................................................... 6
3. LOCALITY AND SAMPLES .......................................................................................................................... 7
3.1 Granny Smith .............................................................................................................................................. 8
3.2 MARID Xenoliths ....................................................................................................................................... 10
3.3 Dunites ...................................................................................................................................................... 11
3.4 Rutile-ilmenite intergrowths .................................................................................................................... 12
3.5 Orthopyroxenites ..................................................................................................................................... 14
4. RESULTS .................................................................................................................................................. 15
4.1 Ilmenite compositions .............................................................................................................................. 15 4.1.1 Major elements ..................................................................................................................................... 16 4.1.2 Trace elements ...................................................................................................................................... 24 4.2. Granny Smith clinopyroxene ............................................................................................................... 34
5. CLASSYFING THE ILMENITES ........................................................................................ 35
6. DISCUSSION ....................................................................................................................................... . 48
6.1 The classification of ilmenites .................................................................................................................. 48
6.2 Ilmenite genesis ........................................................................................................................................ 48
7. CONCLUSIONS ............................................................................................................................................... 52
References ..................................................................................................................................................... 54 Appendix ......................................................................................................................................................... 60
iv
Acknowledgements I want to thank my supervisor Dan Schulze for giving me the opportunity to carry out this research
project and showing me a part of geology that I wasn’t exposed to before. Thank you for the fruitful
discussions and encouragements and for having your full support throughout the whole project.
I also want to thank James Brenan, Mike Gorton and Mike Hamilton for their thoughtful insights,
suggestions and answers to my questions. I appreciate the technical assistance I received from
Colin Bray, Yanan Liu and George Kretschman.
Funding for the project was provided through NSERC and the KEEVIL/Miller Scholarship and
samples were provided by De Beers.
1
1. Introduction In Earth’s upper mantle diamonds are associated with peridotitic (olivine ± orthopyroxene ±
clinopyroxene ± garnet ± chrome spinel) and eclogitic (clinopyroxene + garnet) parageneses.
Diamonds are brought to Earth’s surface as accidental inclusions by alkaline magmas such as
kimberlites and lamproites which have sampled the diamond stability field in Earth’s upper mantle.
As a kimberlitic magma passes through the continental litosphere it also incorporates other upper
mantle materials as, xenoliths and xenocrysts within the kimberlite (Pearson et al., 2003). One
such important component in kimberlites is magnesian ilmenite which occurs as megacrysts
(>1cm), xenocrysts, part of the ground mass and in a variety of ultramafic xenoliths (Schulze et
al., 1995). The chemical and physical stability of ilmenite in the sedimentary environment makes
it an important an important kimberlite exploration tool. However, as ilmenite occurs in other
metamorphic and igneous rocks, a method for separating mantle and crustal ilmenites was devised
to permit the identification of ilmenite from mantle sources (Wyatt et al., 2014). Some workers
suggest that the chemistry of ilmenite can also provide information regarding the diamond content
of a kimberlite. Two methods are proposed – the Fe3+/Fe2+ ratio (Gurney et al., 1993) which may
contain information about the oxidation state of the kimberlite and the Zr/Nb ratio (Carmody et
al., 2014).
Worldwide, most ilmenite from kimberlite belongs to the Cr-poor megacryst suite
(Schulze et al., 1995). This is a co-magmatic suite of silicates and ilmenites that is the product of
fractional crystallization of a deep-seated magma, possibly the kimberlite itself (Schulze, 1987) in
which ilmenite occurs late in the fractional crystallization sequence as single crystals or intergrown
with Cr-poor suite silicates (e.g., garnet, clinopyroxene, orthopyroxene, olivine). Thus, by using
2
trace element contents, ilmenite can be used to pinpoint the start of crystallization for different co-
genetic phases. Details of geochemical trends within suites differ between localities (e.g., Schulze,
1987; Moore et al., 1992; Griffin et al., 1997). In general, early formed silicates are more
magnesian and Cr-rich than those formed later in the sequence and ilmenite, which joins the
sequence in the later stages of crystallization, behaves in a similar way. In many suites, the very
latest ilmenite reverts to higher Cr and Mg contents, possibly due to contamination of the
megacryst magma by peridotitic wallrock.
Although Cr-poor suite ilmenites appear to be the most common variety world-wide, some
kimberlites with ilmenite have no intergrowths of ilmenite and silicate members of the Cr-poor
suite. Ilmenites from these kimberlites apparently have other mantle sources. The kimberlites
from the Kimberley, South Africa area are one such case. In the present investigation I have
analyzed ilmenites from a variety of mantle xenoliths from Kimberley that do not belong to the
Cr-poor megacryst suite and compared those data with the compositions of ilmenite xenocrysts
from four Kimberley diamond mines in an effort to determine the mantle xenolith sources for the
kimberlite ilmenite xenocrysts.
2. Analytical methods Ilmenites from xenoliths were analyzed in polished or polished thin sections of rocks or in polished
sections of individual ilmenite grains plucked from hand samples. Ilmenite xenocrysts from the
four mines were analyzed in polished sections prepared from grains selected from heavy mineral
concentrates (1-3 mm). Clinopyroxene analyses were performed on polished thin-sections of
Granny Smith xenoliths.
3
2.1 Microprobe analysis
All samples were analyzed using a Cameca SX50 wavelength dispersive electron microprobe
equipped with three WDS detectors in the Department of Geology at the University of Toronto.
An accelerating voltage of 15 kV, beam current of 30/50nA for ilmenites and clinopyroxene, and
a 1 µm beam diameter was used. Two or three analyses were performed on each sample. The
standards used for calibration and counting times are provided in tables 2 and 3. Fe2O3 was
determined from stoichiometry.
2.2 Laser Ablation Inductively-Coupled Plasma Mass Spectrometry
Samples were analyzed in situ using the LA-ICP-MS in the Department of Geology at the
University of Toronto. The LA-ICP-MS set up consists of Thermo Elemental (VG) PlasmaQuad
PQ ExCell ICP-MS coupled to a Nu-Wave UP-213 Laser Ablation Microscope. The NIST 610
glass standard was used for calibration of all measured elements. For the ablation of ilmenite
a 55 µm beam size was used operating at 45% output and 10 Hz. Helium was used as a carrier
gas. Data reduction was done using Glitter version 4 and Cr was used as the internal standard
for all ilmenite analysis. For samples containing fine rutile-ilmenite intergrowths special
attention was ensured so that only ilmenite was analyzed. Standards P-MT glass and HF-12
Glass (Dalpe et al., 1995) have also been analysed to verify that our analyses are accurate and
no interference occurs. (table 1). Fig.1 a and b represents EDS vs ICP-MS graphs for Nb and
Cr.
In addition to the elements analyzed by electron microprobe 23Na, 39K, 45Sc, 51V, 59Co,
60Ni, 65Cu, 66Zn, 69Ga, 72Ge 88Sr, 89Y, 90Zr, 93Nb,118 Sn, 137Ba, 139La, 140Ce, 141Pr, 146Nd, 147Sm,
153Eu, 157Gd, 159Tb, 163Dy, 166Er, 169Tm, 172Yb, 175Lu, 178Hf, 181Ta, 182W, 208Pb, 232Th and 238U were
also measured by LA-ICP-MS.
4
P-MT Glass HF-13 Glass
Personal
analysis
Dalpe et. Al., 1995 Sol
ICP-MS
Personal
analysis
Dalpe et al, 1995
Sol ICP-MS XRF+ICP+INA
Sr88 622.175 461.7 474.6 2038.52 1532 1485 1498
Y89 13.645 12 9.73 28.695 30.46 23.89 27.4
Zr90 55.085 53.08 52.35 302.1 301.9 292.7 299.9
Nb93 17.88 13.25 16.62 100.24 103.6 114.6 90.78
Ba137 370.3 360.4 365.9 349.96 320.9 337.1 391.4
Hf178 2.585 2.14 2.35 6.305 6.05 6.54 5.99
Ta181 0.823 0.96 1.02 4.23 5.79 5.87 4.68
Pb208 2.9 3.83 4.5 0.3235 0.61 0.45 nd
Th232 0.193 0.17 0.21 6.925 9.13 9.21 9.61
U238 0.0693 0.05 0.06 2.38 2.84 2.81 2.47
La139 5.86 5.77 5.78 86.755 82.82 83.73 77.87
Ce140 18.4 17.01 18.07 152.725 159.18 167.76 139
Pr141 3.185 3.11 2.89 17.385 20.03 18.76 n.d
Nd146 16.04 14.53 15.31 79.875 73.35 76.91 67.17
Sm147 4.9 3.74 3.91 15.34 14.06 14.42 13.85
Eu153 1.6 1.29 1.36 5.245 4.48 4.49 4.08
Gd157 4.465 3.41 4.4 11.19 11.31 11.76 10.88
Tb159 0.506 0.48 0.52 1.1305 1.53 1.47 1.4
Dy163 3.04 2.53 2.62 7.02 6.97 7.04 6.71
Ho165 0.4655 0.43 0.45 0.9135 1.06 1.11 1.18
Er166 1.219 1.08 1.05 2.01 2.72 2.45 n.d
Tm169 0.1391 0.13 0.12 0.2115 0.3 0.27 0.27
Table 1 – Analysis of P-MT and HF-13 standards
5
93N
b
52C
r
18000
16000
14000
12000
10000
8000
6000
4000
Dunites
Granny Smith
MARID
Rut-ilm
Opxite
2000
0
0.000 0.500 1.000 1.500 2.000
Nb2O5
60000
50000
40000
30000
20000
10000
Dunites
Granny Smith
MARID
Rut-ilm
Opxite
0
0.000 2.000 4.000 6.000 8.000 10.000
Cr2O3
Fig. 1 –EDS vs ICP_MS graphs for Cr and Nb
6
2.3 Scanning Electron Microscope
SEM work was performed on carbon coated polished thin sections of Granny Smith
xenoliths, at the University of Toronto, Department of Earth Sciences, using a JEOL JSM-6610LV
equipped with an OXFORD INCA energy-dispersive X-ray spectrometer (EDS).
Element Standard Counting times (s)
Ti TiO2 40
Si
Ti-Al pyroxene
20
Ca
Ti-Al pyroxene
20
Al
Chromite
20
Fe
Ilmenite
20
Mg
Chromite
60
Nb
NaNbO3
40
Cr
Chromite
40
Mn
Ilmenite
30
Ni
Pentlandite
30
Table 2: Standards used for calibration, and counting times for electron microprobe analysis of ilmenite.
7
Element Standard Counting times (s)
Ti TiO2 12
Si
Cr-augite
11
Ca
Cr-augite
12
Al
Cr-augite
12
Fe
Hematite
12
Mg
Cr-augite
12
Na
Albite
12
Cr
Chromite
12
Mn
Bustamite
12
K
Sanidine
60
Table 3 : Standards used for calibration, and counting times for electron microprobe analysis of clinopyroxene.
3. Locality and samples
As a result of early mining practices at the kimberlite-hosted diamond mines in Kimberley, South
Africa,(Fig. 2) an extraordinary quantity and variety of mantle-derived ultramafic xenoliths exist in
the waste dumps of the Kimberley mines. Xenoliths were separated from the mined kimberlite by
hand and dumped in piles, now known as the Kimberley Dumps (Viljoen, 1988). The ilmenite-bearing
samples in the present study were collected from the Boshof Road, Kenilworth and Kamfersdam
Dumps. The sources of these dumps are, respectively, the Bultfontein Mine, the De Beers Mine and
the Kamfersdam Mine (Viljoen, 1988). Xenoliths were also studied from the Pulsator Dump which
consists of xenoliths and xenocrysts from the “De Beer’s Pool”, a mixture of material from the
Bultfontein, De Beers, Wesselton and Du Toit’s Pan Mines (J Robey, personal communication in
Schulze, 1995 JGR).
8
Fig. 2 – Location of kimberlite pipes in the Kimberley area, from White et al., 2012
Ilmenite xenocrysts were also studied from heavy mineral concentrates from the Wesselton and
Bultfontein mines (supplied by De Beer’s Consolidated Mining Corporation) and from the
Kamfersdam and Otto’s Kopje mines, collected on site by D.J. Schulze.
3.1. Granny Smith
Xenoliths in this suite (abbreviated GS) are dominated by apple green diopside with minor
ilmenite, phlogopite and uncommon rutile. They were named by Boyd et al. (1983) because of
their similarity in colour and general appearance to Granny Smith apples. They are also referred
to as Phlogopite Ilmenite Clinopyroxene (PIC) rocks by Gregoire et al. (2001). Modal variants are
dominated by phlogopite (Fig. 3D) with accessory ilmenite and diopside. Single undeformed
crystals range up to 10 cm in maximum dimension, though such large crystals are not common.
More commonly, the clinopyroxene is variably deformed with porphyroblastic clinopyroxene
9
surrounded by a groundmass of neoblastic clinopyroxene (Fig. 3B). Exsolution lamellae are
common in the porphyroclastic clinopyroxene and in some neoblasts. Ilmenite is anhedral, mosaic
(Fig.3A) and is present around the deformed porphyroblasts or within the neoblastic clinopyroxene
matrix as blebs or lenticles (Fig.3C). Rutile, observed by Boyd et al. (1983) and Zhao et al. (1999)
was not found in the present study. Phlogopite occurs as flakes up to several millimeters in length
and it is either deformed or undeformed. One sample also contained, orthopyroxene alongside the
clinopyroxene and ilmenite.
A B
Cpx neoblasts
0.5 mm Cpx porphyroclast
0.5 mm
C D
Clinopyroxene
Phlogopite
Ilmenite 0.5 cm 0.5 mm
Fig. 3 Textures of Granny Smith xenoliths A – mosaic ilmenite, reflected light; B – clinopyroxene neoblasts and
porprhyroclasts, tranmisted light; C – polished hand sample of Granny Smith rock with vein-like ilmenite, D –
phlogopite rich GS xenoliths with deformed phlogopite porphyroclasts and neoblasts, transmitted light
10
3.2 MARID Xenoliths
MARID suite xenoliths (Dawson et al., 1977) consist of various proportions of Mica,
Amphibole, Rutile, Ilmenite, and Diopside, hence the name. As noted by Gregoire et al. (2002),
K-richterite is the key mineral that allows distinction between MARID and a variety of other
phlogopite-bearing xenoliths and all of the MARID rocks in this study contain K-richterite. Minor
phases, such as apatite, calcite or zircon occur. Textures and grain sizes in the MARID rocks are
quite diverse, ranging from a pegmatitic K-richterite crystal 7.5 cm in length, with accessory
millimeter sized ilmenite, rutile and phlogopite to equigranular fine-grained polycrystalline rocks.
Variants dominated by phlogopite or k-richterite occur. Rutile and ilmenite are commonly
intergrown, either as patchy inclusions of rutile or ilmenite in the other, or as coarse lamellae, blebs
and veins of ilmenite inside the rutile (Fig. 4D). The amphiboles are typically euhedral to subhedral
(Fig 4A) and the pyroxenes are usually anehdral. Exsolution features are common in the
amphiboles and the pyroxenes whereas in the rutile fine ilmenite lamellae, smaller than 5 um are
present (as is typical in rutiles in kimberlite-borne xenoliths). The majority of the samples in this
study have deformed silicates and some of the phlogopite-rich rocks are layered, interpreted as a
magmatic banding (Dawson et al., 1977). Rutile and ilmenite are finely intergrown with each other
and with phlogopite. One sample contains a symplectitic intergrowth between an altered silicate,
possibly phlogopite or olivine, and rutile-ilmenite intergrowths (Fig. 4B). A similar texture occurs
in a rutile-ilmenite intergrowth sample (Fig. 6C).
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Amph A B
Ilm
Rut
Ilm
Phl 0.5 mm 0.5 mm
C D
0.5 mm
Fig. 4 MARID xenolith textures: A - amphibole, rutile-ilmenite and phlogopite, plane polarized transmitted
light, , B - rutile and ilmenite reflected light, C - symplectitic intergrowth between rutile, ilmenite and silicate, reflected
light; D – K-richtericte megacryst
3.3 Dunites (Dun) Most of these samples are fine-grained (0.05 mm - 5 mm) dominated by olivine porphyroclasts,
olivine neoblasts (Fig. 5A), phlogopite and ilmenite (Fig. 5B) with rare spinel. Calcite, most likely
of secondary origin, is also present as a minor phase. Rare iron sulphides also occur. The ratio
between olivine neoblasts and porphyroclasts differs between samples but the majority are
neoblast-rich. One sample (13-74-49) is a single, unrecrystallized olivine porphyroclast and
contains euhedral ilmenite. The size of the neoblasts ranges from 0.05 mm to 3 mm. The ilmenite
is typically anhedral, mosaic-textured and in some occurrences appears as veins rimmed by
phlogopite or serpentinite (Fig. 5D). Some very fine ilmenite is intergrown with the olivne
12
neoblasts, giving them a mottled appearance. In sample 13-69-2 ilmenite borders a Cr-rich spinel
with fine ilmenite lamellae extending into the spinel (Fig.5C)
Ol porphyroclast 0.5 mm
A B
Ol
Phl
Ol neoblasts 0.5 mm Ilm
C D
0.5 mm 0.5 mm
Fig 5 Dunite textures A – olivine neoblasts and porphyroclast with ilmenit, transmitted light crossed polars; B –
olivine neoblasts and porphyroclast with ilmenite, phlogopite and serpentine, plane polarized transmitted light; C –
ilmenite replacing chromian spinel, reflected light; D – vein-like ilmenite in mosaic olivine, reflected light
3.4 Rutile-ilmenite intergrowths (Rut-ilm) These rocks are dominated by rutile and ilmenite with minor phlogopite or altered olivine.
Macroscopically they are rounded nodules, black or reddish brown in colour. The rutile is
polygranular and has red internal reflections on the crystal margins or near cracks. The rutile and
ilmenite are finely intergrown and the ratio of ilmenite to rutile is not consistent between samples.
Several types of intergrowth textures occur, similar to those described by Tollo et al. (1987). The
most common texture is represented by vein-like ilmenite protruding into the rutiles (Fig. 6A). The
13
boundary between the two phases is sharp. Coarse grained ilmenite lamellae (1 – 3 mm in length
and ~ 10 microns in width) are also present inside the rutile. They are usually lensed shaped and
appear to occur in distinct crystallographic directions, similar to exsolution lamellae inside
titanomagnetite. Irregular mosaic blebs of ilmenite that Tollo et al. (1982) called atoll structures
(Fig. 6B) are not common and seem to be related to coarser grained lamellae. Extremely fine
ilmenite lamellae (<5 microns) appear in almost all of the rutiles in these samples, regardless of other
textures. Except for their size, they are similar to the coarser ones described above. Only two other
mineral phases are present – phlogopite in several rocks and one sample contains an altered silicate,
possibly olivine.
Ilm
A B
Ilm
Rut
Rut
0.5 mm
0.5 mm
C
0.5 mm
Fig. 6. Textures in rutile-ilmenite xenoliths A – vein-
like ilmenite inside rutile, reflected light; B – patchy
and atoll-shaped intergrowths ilmenites at rutile
boundaries, reflected light; C – symplectitic
intergrowth between rutile, ilmenite and silicate,
reflected light
14
3.5 Orthopyroxenites (Opxite)
Composed of orthopyroxene, phlogopite, ilmenite, rutile with or without diopside these
rocks range from fine to coarse grained (0.05 mm – 0.3 cm). Modally the orthopyroxenites range
from phlogopite-rich to orthopyroxene rich or ilmenite/rutile rich. Orthopyroxene is usually
anhedral and rounded (Fig. 7C) with grain sizes in the range ~ 50 um to 1-2 millimetres. Ilmenite
and rutile are anehdral, mosaic and lobate/ameoidal and some occur as veins but are typically
scattered throughout the sample (Fig. 7B, 7D). The two phases are typically finely intergrown with
each other or with the silicates. Fine ilmenite exsolution-type lamellae are common in rutiles and
the ilmenite to rutile ratio is not consistent between samples. One sample contains a mosaic
ilmenite ~0.5 cm in diameter. Phlogopite is anehdral and typically deformed with sizes in the range
<1 mm to grains a couple of centimeters in maximum dimension. Garnet does not occur in the
Kimberley samples, though it has been described elsewhere (Boyd et al., 1984; Doyle et al., 2004).
In many samples, acicular ilmenite, rutile and orthopyroxenite are finely intergrown in fasciculate
texture that is considered to be the result of quenching due to fast crystallization (Boyd et al., 1984)
(Fig 7A, 7B). In sample 13-67-54 fine grained altered phlogopite-rich orthopyroxenite is in contact
with an ilmenite bearing dunite (Fig. 7E). Altered olivine, phlogopite and extremely fine-grained
oxide phases occur at the contact of these two domains
A B
Phl
Opx
0.5 mm
0.5 mm
15
C D
Phl
Opx
Ilm+Rut
0.5 mm
0.5 mm
Ol
Opx
E 0.5 mm
Fig. 7 Textures in orthopyroxenite xenoliths A –
acicular opx in fine-grained quench-like texture
intergrown with phlogopite and rutile and ilmenite,
plane polarized transmitted light, B- acicular ilmenite
and rutile intergrown with orthopyroxene in quench-
like texture, reflected light C –acicular rutile and/or
ilmenite with orthopyroxene and phlogopite, plane
polarized transmitted light D – intergrown ilmenite and
rutile with silicates, reflected light, E – serpentinized
boundary between orthopyroxenite (right) and dunite
(left) in sample 13-67-54, plane polarized transmitted
light.
4. Results
4.1 Ilmenite compositions (table 5, appendix) Based on our electron microprobe and laser ablation ICP-MS analyses a basic chemical
characterization of ilmenites from all the different suites in the present study can be devised.
16
4.1.1 Major elements
Granny Smith suite Granny Smith ilmenites have narrow ranges of values for almost all of the elements analyzed.
They have high MgO (11.0 - 14.7 wt %) (Fig. 7, 8) and moderate Cr2O3 (1.0 – 3.2 wt%) (Fig. 8,
10, 11, 12) and Fe2O3 (5.6 - 7.9 wt%).), Al2O3 ranges from 0.01 to 0.5 wt% (Fig. 8,9), TiO2 from 52.6 to 55 wt% (Fig. 10) Nb2O5 from 0.05 to 0.53 wt% (Fig. 11). The sample with the lowest
MgO content (13-74-72) also has the lowest Al2O3 and TiO2 and highest Fe2O3 and Nb2O5 content,
and resembles MARID or orthopyroxenite ilmenites.
Dunites Ilmenites in dunites have MgO values ranging from 6.1 to 14.9 wt% (Fig. 8, 9), Cr2O3 from 0.08
to 6.5 wt% (Fig. 8, 10, 11, 12), MnO from 0.2 to 0.4 wt% and Fe2O3 values ranging from 4.8 to
21.7 wt%), Al2O3 (Fig. 9, 10), TiO2 (Fig. 11) and Nb2O5 (Fig. 12) contents are between 41.6 and 55.5 wt%, 0.01 and 0.6 wt% and 0.07 and 1.7 wt%, respectively.
Rutile-ilmenite intergrowths In rutile-ilmenite intergrowths the ilmenite has MgO values similar to those of the Granny Smith
ilmenites in Fig. 7, 8 (12.2 – 14.9 wt%) with higher Cr2O3 values (1.3 – 9.1 wt%) (Fig. 8, 10, 11,
12), and Fe2O3 contents (6.0 – 11.0 wt%) ,TiO2 (Fig. 11) values are also similar to those found in Granny Smith ilmenites (50.0 – 54.8 wt%) with Al2O3 (Fig. 9, 10) and Nb2O5 (Fig. 12) values of
0.2 – 1.2 and 0.06 – 0.15 wt% respectively.
Orthopyroxenites
17
Ilmenites in orthopyroxenites are more chemically diverse than those in most of the other suites,
with MgO (Fig. 8, 9) values ranging from 6 to 14.8 wt%, Cr2O3 (Fig. 8, 10, 11, 12) values from
0.15 to 7.9 wt% and Al2O3 (Fig. 9, 10) values from 0.01 to 0.4 wt%. TiO2 (Fig. 11) and Nb2O5
(Fig. 12) also vary with values in the range 41.7 to 55.9 wt% and 0.02 to 1.4 wt%, respectively.
MARID xenoliths Ilmenites in MARID rocks have MgO values that range widely (Fig. 8, 9) (6.5 – 17.5 wt%) and
low Cr2O3 (Fig. 8, 10, 11, 12) values (0.5 – 2 wt%). Al2O3 (Fig. 9, 10) values are extremely low
(0.0 – 0.05 wt%) and Nb2O5 (Fig. 12) (0.008 – 1.2 wt%) and Fe2O3 (3.0 – 17.2 wt%) have a wide
range.
General observations Values of Al2O3 – Cr2O3 and MgO (Fig. 9 and 10) correlate positively for ilmenites in the Granny
Smith, dunite and rutile-ilmenite intergrowth suites and part of the orthopyroxenite suite. In the
rutile-ilmenite intergrowths and Granny Smith suite, TiO2 correlates negatively with Cr2O3 (Fig.
11) whereas the rest of the suites have more complex trends due to the high variance in Cr2O3 and
TiO2 values. A negative correlation also exists between Nb2O5 and MgO in ilmenites from the
Granny Smith suite. A similar trend also occurs in some of the orthopyroxenite ilmenites that
correlate well with the analysis with anomalous high Nb2O5 content, whereas the rest of the
ilmenites follow a somewhat sinusoidal trend with increasing MgO. A similar behaviour is
displayed by MARID ilmenites. Nb2O5 and Cr2O3 (Fig. 12) are negatively correlated for Granny
Smith and rutile-ilmenite intergrowth suites.
18
Cr 2
O3
wt%
M
gO w
t%
10.000
9.000
8.000
7.000
6.000
5.000
4.000
3.000
2.000
Dun Gs
MARID
Rut-ilm
Opxite
1.000
0.000
0.000 2.000 4.000 6.000 8.000 10.000 12.000 14.000 16.000 18.000
MgO wt%
Fig. 8 – MgO – Cr2O3 plot
18.000
16.000
14.000
12.000
10.000
8.000
6.000
4.000
Dun GS
MARID
Rut-ilm
Opxite
2.000
0.000
0.000 0.200 0.400 0.600 0.800 1.000 1.200 1.400
Al2O3 wt%
Fig. 9 – MgO – Al2O3 plot
22
Cr 2
O3
wt%
C
r 2O
3 w
t%
10.000
9.000
8.000
7.000
6.000
5.000
4.000
3.000
2.000
Dun GS
MARID
Rut-ilm
Opxite
1.000
0.000
0.000 0.200 0.400 0.600 0.800 1.000 1.200 1.400
Al2O3 wt%
Fig. 10 – Cr2O3 – Al2O3 plot
10.000
9.000
8.000
7.000
6.000
5.000
4.000
3.000
2.000
Dun GS
MARID
Rut-ilm
Opxite
1.000
0.000
40.000 42.000 44.000 46.000 48.000 50.000 52.000 54.000 56.000 58.000 60.000
TiO2 wt%
Fig.11 – Cr2O3 – TiO2 plot
23
Cr 2
O3
wt%
C
r 2O
3 w
t%
10
9
8
7
6
5 GS 4 Rut-ilm 3
2
1
0
0.00 0.05 0.10 0.15 0.20 0.25 0.30 0.35 0.40
Nb2O5 wt%
Fig. 12a – Cr2O3 – Nb2O5 plot for GS and Rut-ilm ilmenites
10.000
9.000
8.000
7.000
6.000
5.000
4.000
3.000
Dun
MARID
Opxite
2.000
1.000
0.000
0.000 0.200 0.400 0.600 0.800 1.000 1.200 1.400 1.600 1.800 2.000
Nb2O5 wt%
Fig. 12b – Cr2O3 – Nb2O5 plot without GS and rut-ilm ilmenites
24
4.1.2 Trace element compositions The ilmenites from the various suites analyzed in the present study are surprisingly similar in their
trace element contents, especially in their high field strength elements (table 5). Dunite, Granny
Smith, rutile-ilmenite intergrowth, orthopyroxenite and two of the MARID ilmenites have high Zr
(224 – 890 ppm) (Fig .13, 14, 18) and Nb (305 – 1316 ppm) (Fig. 15, 16) values and moderate
Hf (7 – 31 ppm) (Fig. 13, 17) and Ta (Fig. 15, 17). Ilmenites from two dunite (4354 ppm and 8975
ppm), two orthopyroxenite (5877 and 10987 ppm) and the rest of the MARID (2009 ppm – 9310
ppm) xenoliths have higher Nb (Fig. 15a, 16a) values. Except for those from the MARID
xenolithss, all the ilmenites with higher Nb contents also have anomalously high Ta (446 –
683ppm). Nb/Ta (Fig. 16) ratios are subchondritic with only four samples exceeding the 17.6
threshold defined by McDonough (1990): three MARIDs (36.8, 29.6, and 19.3) and one
orthopyroxenite (23.5). Zr/Hf (Fig. 14) values are also subchondritic (< 36) for the majority of the
ilmenites with the following exceptions: one dunite ilmenite (41.4), four of the MARID ilmenites
(39.6, 36.6, 39.5, and 39.4) and two orthopyroxenites (40.8, 49.9). All of the ilmenites have
elevated V contents (814 ppm – 2581 ppm) and a wide range for Ni values (250 – 2499 ppm).
Contents of U, Th, La, Ce, Pr, Nd, Sm, Eu, Gd, Tb, Dy, Ho, Er, Tm, Yb and Lu are small or below
detection limits. Sc (Fig. 12 – 14) is similar for all the samples (9.53 ppm – 30.85 ppm) whereas
Ga values (0.68 – 2.60 ppm) are lower in MARID ilmenites than the rest of the analyzed ilmenites
(7.37 – 15.58 ppm). Two MARID ilmenites also have anomalously low Cu values (5.22 – 7.66
ppm). The ranges for all the other chemical elements analyzed in this study are similar for all the
analyzed samples – Co (133.25 – 279.9 ppm), Zn (95.9 – 204 ppm), Sn (6.69 – 12.3 ppm with a
single MARID ilmenite having a value of 19.7 ppm).
25
A positive correlation also exists between Hf and Zr (Fig. 13) and Hf and Ta (Fig. 17) for all of
the samples. The Nb-Ta (Fig. 15) relationship is more complex and varies depending on the suites
considered. Positive correlations exist for ilmenites in the orthopyroxenite, rutile-ilmenite
intergrowths and dunite suites whereas the MARID ilmenites define a “sinusoidal” trend. In the
Granny Smith suite two trends exist both having positive correlations between the two elements
but with a different slope – the ilmenites with high Ta produce a steeper slope than ones with lower
Ta values.
Nb/Ta vs Nb (Fig. 16) slopes for ilmenites dunite, MARID, opxites and part of the Granny Smiths
are positive which is in accordance with experimental data that has shown that Ta is preferentially
fractionated by the ilmenite (Klemme et al., 2006). A negative slope is exhibited by ilmenites in
the rutile-ilmenite intergrowths whereas ilmenites from part of the Granny Smith exhibit a slope
that resembles an inverse curve. These anomalies can also be seen in a Zr/Hf vs Zr diagram (Fig.
14) for the rutile-ilmenite intergrowth ilmenites. Sc correlates well with Zn, Zr, Sn, Hf and Ta for
Granny Smith, dunite and rutile-ilmenites (Fig. 18-20), but this relationship isn’t as apparent for
the two other ilmenite suites.
Fig. 21 represents chondritic-normalized ((McDonough and Sun, 1995) spider diagrams of trace
element values of ilmenites from ilmenite-bearing samples from Kimberley. The elements have
been arranged in order to better observe the behaviour of elements with similar chemical
properties. For Nb-Ta and Zr-Hf, two pairs of elements which are enriched compared to the
chondritic value, the data is as expected from experimental work – Ta and Hf are preferentially
incorporated by the ilmenite compared to their chemical parteners. Sn is also enriched whereas V,
W, Zn and Co are only slightly enriched. Ni and Pb have subchondritic values and Ge and Cu are
at chondritic values. For comparison with samples analyzed in this study, maximum and minimum
26
values for ilmentie megacrysts from South Africa, Grib and Yakutian kimberlites have also been
analyzed
27
plotted.
Zr/H
f H
f (p
pm
)
GS
GS
40
35
30
25 Dun
20
MARID 15
Rut-ilm
10 Opxite
5
0
0 200 400 600 800 1000 1200 1400 1600
Zr (ppm)
Fig. 13 – Zr – Hf plot
60
50
40
Dun
30
MARID
20 Rut-ilm
Opxite 10
0
0 200 400 600 800 1000 1200 1400 1600
Zr (ppm)
Fig. 14– Zr – Zr/Hf plot
28
Ta (
pp
m)
Ta (
pp
m)
1400
1200
1000
800
600
400
200
Dun GS
MARID
Rut-ilm
Opxite
0
0 2000 4000 6000 8000 10000 12000 14000 16000 18000
Nb (ppm)
Fig. 15a – Nb-Ta plot
300
250
200
150
100
Dun
GS
Rut-ilm
Opxite
50
0
0 200 400 600 800 1000 1200 1400 1600 1800 2000
Nb (ppm)
Fig. 15b – Nb-Ta without MARID and ilmenites with anomalously high values
29
Nb
/Ta
Nb
/Ta GS
GS
40
35
30
25 Dun
20
MARID 15
Rut-ilm 10 Opxite
5
0
0 2000 4000 6000 8000 10000 12000 14000 16000 18000
Nb (ppm)
Fig.16a – Nb-Nb/Ta plot
20
18
16
14
Dun 12
10
8 MARID
6 Rut-ilm
4 Opxite
2
0
0 200 400 600 800 1000 1200 1400 1600 1800 2000
Nb (ppm)
Fig.16b – Nb-Nb/Ta plot wihout anomalously high values
30
Sc (
pp
m)
Hf
(pp
m)
GS
GS
40
35
30
25 Dun
20
MARID 15
Rut-ilm 10 Opxite
5
0
0 200 400 600 800 1000 1200 1400
Ta (ppm)
Fig. 17 – Hf-Ta plot
100
90
80
70
Dun 60
50
40 MARID
30 Rut-ilm
20 Opxite
10
0
0 200 400 600 800 1000 1200 1400 1600
Zr (ppm)
Fig. 18 – Sc-Zr plot
Fig. 20 – Sc-Zn plot
31
Sc (
pp
m)
Sc (
pp
m)
GS
GS
100
90
80
70
Dun 60
50
40 MARID
30 Rut-ilm
20 Opxite
10
0
0 200 400 600 800 1000 1200 1400
Ta (ppm)
Fig. 19 – Sc-Ta plot
100
90
80
70
Dun 60
50
40 MARID
30 Rut-ilm
20 Opxite
10
0
0 100 200 300 400 500 600
Zn (ppm)
32
100000
10000
1000
S Africa
100 Yakutia
Grib 10
Dunite
1
0.1
0.01
Ga Ni Zr Hf Ta Nb Cu Zn Co Sc V Cr Mn Ti Pb Y
100000
10000
1000
100 S Africa
Yakutia
Grib 10
GS
1
0.1
0.01
Ga Ni Zr Hf Ta Nb Cu Zn Co Sc V Cr Mn Ti Pb Y
100000
Dunites
10000
1000
100
10
1
S Africa min
S Africa max
Yakutia min
Yakutia max
Grib min
Grib max
0.1
0.01 Ti Zr Hf Nb Ta V Cr W Ge Sn Pb Ga Ni Cu Zn Co Mn
Fig. 21a– Trace element spider diagram for dunite ilmenites
100000
Granny Smith
10000
1000
100
10
S Africa min
S Africa max
Yakutia min
Yakutia max
Grib min
Grib max
1
0.1 Ti Zr Hf Nb Ta V Cr W Ge Sn Pb Ga Ni Cu Zn Co Mn
Fig. 21b– Trace element spider diagram for Granny Smith ilmenites
33
100000
10000
1000
100 S Africa
Yakutia
Grib 10
Rut-ilm
1
0.1
0.01
Ga Ni Zr Hf Ta Nb Cu Zn Co Sc V Cr Mn Ti Pb Y
100000
10000
1000
100 S Africa
Yakutia
Grib 10
MARID
1
0.1
0.01
Ga Ni Zr Hf Ta Nb Cu Zn Co Sc V Cr Mn Ti Pb Y
100000
Rutile-ilmenite intergrowths
10000
1000
100
10
S Africa min
S Africa max
Yakutia min
Yakutia max
Grib min
Grib max
1
0.1 Ti Zr Hf Nb Ta V Cr W Ge Sn Pb Ga Ni Cu Zn Co Mn
Fig. 21c– Trace element spider diagram for rutile-ilmenite intergrowths ilmenites
100000
MARIDs
10000
1000
100
10
S Africa min
S Africa max
Yakutia min
Yakutia max
Grib min
Grib max
1
0.1 Ti Zr Hf Nb Ta V Cr W Ge Sn Pb Ga Ni Cu Zn Co Mn
Fig. 21d– Trace element spider diagram for rutile-ilmenite intergrowths ilmenites
34
100000
10000
1000
100 S Africa
Opxite
Yakutia 10
Grib
1
0.1
0.01
Ga Ni Zr Hf Ta Nb Cu Zn Co Sc V Cr Mn Ti Pb Y
100000
Orthopyroxenite
10000
1000
100
10
1
S Africa min
S Africa max
Yakutia min
Yakutia max
Grib min
Grib max
0.1
0.01 Ti Zr Hf Nb Ta V Cr W Ge Sn Pb Ga Ni Cu Zn Co Mn
Fig. 21e– Trace element spider diagram for orthopyroxenite ilmenites
4.2 Granny Smith clinopyroxene
Fig 22. – BSE image of clinopyroxene neoblasts and
porphyroclasts
The clinopyroxene porphyroclasts analysed
are calcic [Ca/(Ca+Mg)] >0.45 and
magnesian [Mg/(Mg+Fe)] >0.89 and have
moderate TiO2 (0.2 – 0.4 wt%) and Cr2O3
(0.8 – 1.1 wt%). Small chemical differences
exist between the margins and centers of the
neoblasts and porphyroclasts (Fig. 22). The
margins are enriched in MgO, FeOt, CaO
and TiO2 and depleted in NaO, SiO2, Al2O3
and Cr2O3 (table 5 - appendix).
35
Al 2
O3
wt%
5. Classifying the ilmenites
One of the main goals of this study was to devise a basic classification scheme (Fig. 34) to
distinguish between ilmenites from the different parageneses, based on major and trace elements.
The best way found to separate them is with several oxide screens, systematically eliminating
whole fields defined by a number of mathematical equations.
1.400
1.200
1.000
0.800
0.600
0.400
Opxite
Dun
Rut-ilm
Dun lit
Opxite lit
MARID
0.200
0.000
4.000 6.000 8.000 10.000 12.000 14.000 16.000 18.000
MgO wt%
Fig. 23 – MgO – Al2O3 plot with Al2O3 boundary for MARID ilmenites MARID ilmenites are easily separated from most of the other suites by their low Al2O3 values
(Fig. 23). The boundary between MARID ilmenites and the other suite is a Al2O3 value of 0.05,
which is consistent with the MARID ilmenite core analysis of Dawson et al. (1976). Four low Mg
dunite ilmenites, one Granny Smith ilmenite and one orthopyroxenite ilmenite also have low
Al2O3.
36
2
IO T
MGO
80
70
60
50
40
30
20
10
0
0 5 1 0 1 5 2 0 2 5
Fig.24 – MgO-TiO2 plot with MARID, Dunite, Orthopyroxenites, Granny Smith ilmenite
Ilmenites can be separated by using the equation: Cr2O2 = 0.0374MgO3 - 1.429MgO2 + 18.211MgO - 24.634, with MARID ilmenites having TiO2 values above the cut off. The four
dunite ilmenites can be separated based on their MgO content, as all the low Al2O3 ilmenites have
MgO values under 10%. The Granny Smith with opx and the orthopyroxenite ilmenites can’t be
separated (Fig. 24).
The second step is separating the Granny Smith ilmenites that plot inside a very narrow field
defined by 12 – 15 wt% MgO and 1 – 3 wt% Cr2O3, with a single exception with lower MgO
content (10 wt%) that mimics the chemistry of a MARID-type ilmenite. On a MgO-Cr2O3 plot,
the boundaries of the Granny Smith field can be defined by four equations for Cr2O3 values >
0.95 wt% (Fig. 25)
37
Cr 2
O3
wt%
Cr2O3 = -0.8448MgO3 + 35.657 MgO 2 - 500.45 MgO + 2337.12, where 13.3 ≤ MgO ≤ 14.75 Cr2O3 = 0.90267 MgO 3 - 36.729 MgO 2 + 499.22 MgO - 2265.03 13.05≤ MgO ≤14.53
Cr2O3 = 23.333 MgO -342.07 for 14.75≤ MgO ≤ 14.78
Cr2O3 = -2.8929 MgO +45.556 for 14.533≤ MgO ≤ 14.78
6
5
4
3
2
1
0
12 12.5 13 13.5 14 14.5 15 15.5
MgO wt%
Fig.25 – MgO-Cr2O3 plot separating the Granny Smith ilmenite from the rest of the suites
Three dunite ilmenites also plot in the field defined by these four equations and they can’t be
separated from the the Granny Smith ilmenites.
38
A subset of the ilmenite from the rutile-ilmenite intergrowths plot close to those from the Granny
Smith suite, but don’t overlap. The following three equations are useful in separating the high and
low Cr2O3 rutile-suite ilmenites from the rest of the suites, for Cr2O3 values lower than 10 wt%:
Cr2O3 = -2.4074 MgO 2 + 68.611 MgO - 487.5, where 13. 5≤ MgO ≤15 and the rutile-ilmenite
intergrowth ilmenites plot inside the parabola
Cr2O3 = 2.1049 MgO 2 - 56.711 MgO + 385.35, where 12.36 ≤ MgO
Cr2O3 = 20.927 MgO 2 - 518.58 MgO + 3218.5, for MgO < 12.36 the rutile-ilmenite intergrowth
ilmenites plot inside the parabola defined by these two equations (Fig. 26)
Ilmenites in orthopyroxenites define a very large field of both MgO and Cr2O3 contents. Two
different groups exist based on the MgO content: 5.06 – 7.01 wt% and 10.38 – 14.84 wt% and, to
better constrain these two groups ilmenite data from orthopyroxenites at Gansfontein, South
Africa, Doyle et al. (2004) have also been used. The low magnesium group can just be separated
by taking out all the ilmenites with a MgO value lower than 7.4 wt%, whereas in order to separate
the high MgO ilmenites, the following equations are useful:
Cr2O3 = 1.663 MgO 3-58.497 MgO 2+681.8 MgO -2627
Cr2O3 = -1.1134 MgO 2 + 25.412 MgO - 141.75 (Fig. 27)
39
Cr 2
O3
wt%
C
r 2O
3 w
t%
12.000
10.000
8.000
6.000
4.000
2.000
0.000
4.000 6.000 8.000 10.000 12.000 14.000 16.000
MgO wt%
Fig.26 – MgO-Cr2O3 plot separating the rutile-ilmenite intergrowths ilmenite from the rest of the suites
12.000
10.000
8.000
6.000
4.000
2.000
0.000
4.000 6.000 8.000 10.000 12.000 14.000 16.000
MgO wt%
Fig.27 – MgO-Cr2O3 plot separating the orthopyroxenite ilmenite from the rest of the suites
40
Cr 2
O3
wt%
The dunites ilmenites define two different groups and in order to better constrain these two fields
data from Renfeldt et al. (2007) and Dawson et al.(1981) (both studies of ilmenites from Kimberley
dunites) have also been used. The first group is represented by ilmenites with lower MgO values
(6.1 – 8.7 wt%). The low magnesium samples also have low Al2O3 values and are separated by
using the method described in detail for MARID-type ilmenites. The second, high MgO group
plots close to the field defined by Granny Smith ilmenites but they can also have higher Cr2O3
values. The dunite ilmenites plot inside two parabolas defined by the following equations:
Cr2O3 = -0.2063 MgO 2 + 6.2481 MgO - 44.899, where 12.5< MgO <17.1 and
Cr2O3 = 0.2783 MgO 2 - 7.3563 MgO + 51.992
and left of the line defined by Cr2O3 = -4.5215 MgO 2 + 119.06 MgO - 780.43 (Fig. 28)
12
10
8
6
4
2
0
4 6 8 10 12 14 16
MgO wt%
Fig.28 – MgO-Cr2O3 plot separating the dunite ilmenite from the of the suites
41
Cr 2
O3
wt%
The remaining ilmenites, belonging to the rutile-ilmenite intergrowths and orthopyroxenite suites
can be distinguished using a TiO2 – Cr2O3 plot (Fig 29). The boundary between the two suites is
defined by the equation:
Cr2O3 = 1.0803 MgO 2 - 115.06 MgO + 3065.9
4
3.5
3
2.5
2
1.5
1
0.5
0
52.8 53 53.2 53.4 53.6 53.8 54 54.2 54.4 54.6 54.8
TiO2 wr%
Fig.29 TiO2-Cr2O3 plot separating the orthopyroxenite and rutile-ilmenite intergrowths ilmenites
Classification of ilmenite xenocrysts from Kimberley diamond mines The classification scheme has been applied to ilmenite xenocrysts from four diamond mines in the
Kimberley area: Bultfontein, Kamfersdam, Otto’s Kopje and Wesselton. The results are
summarized in Table 4.
42
At Bultfontein (Fig 30), 15% of the ilmenites come from the Granny Smith xenoliths, 28% from
orthopyroxenites, 28% from dunites and 23% from MARIDs. In contrast, at Kampfersdam (Fig.
31) the majority of the ilmenite xenocrysts come from Granny Smith (38%) and dunite xenoliths
(34%) whereas ilmenites from orthopyroxenites and MARIDs make up only 15% and 11 %
respectively. Only 1% of the ilmenites belong to the rutile-ilmenite intergrowths.
The majority of the ilmenites analysed from Wesselton (Fig. 32) belong to the Granny Smith
xenoliths (45%) followed by dunites 20%, orthopyroxenites 18%, MARID 12 % and 5% belong
to the rutile-ilmenite intergrowths. At Otto’s Kopje (Fig. 33) 47% of the ilmenites belong to the
dunite suite, 23% come from MARID rocks, 21% from orthopyroxenites whereas only 6% come
from Granny Smith rocks and 1% from rutile-ilmenite intergrowhts. 63% of the ilmenites from
Otto’s Kopje belong to the low Al2O3 group (<0.05%) (Fig 33a). Granny
Smith
Dunite Orthopyroxenite MARID Rut-ilm
intergrowth
Bultfontein 15% 28% 28% 23%
Kamfersdam
38%
34%
11%
15%
1%
Wesselton
45%
20%
18%
12%
5%
Otto’s Kopje
6%
47%
21%
23%
Table 4 – Source rocks of the analysed ilmenite xenocrysts
43
Al 2
O3
wt%
C
r 2O
3 w
t%
0.8
0.7
0.6
Bultfontein
0.5
0.4
0.3
0.2
0.1
0
4 6 8 10 12 14 16 18
MgO wt%
Fig.30a – MgO-Al2O3 plot for Bultfontein xenocrysts
12.00
10.00
8.00
Bultfontein
6.00
4.00
2.00
0.00 4.00 6.00 8.00 10.00 12.00 14.00 16.00 18.00
MgO wt%
Fig.30b– MgO-Cr2O3 plot for Bultfontein xenocrysts
Fig.31b– MgO-Cr2O3 plot for Wesselton xenocrysts
44
Kampfersdam
Al 2
O3
wt%
C
r 2O
3 w
t%
0.6
0.5
0.4
0.3
0.2
0.1
0
4 6 8 10 MgO wt%
12 14 16 18
Fig.31a – MgO-Al2O3 plot for Bultfontein xenocrysts
12.00
10.00
8.00
6.00
Kamfersdam
4.00
2.00
0.00 4.00 6.00 8.00 10.00 12.00 14.00 16.00 18.00
MgO wt%
Fig.32b– MgO-Cr2O3 plot for Wesselton xenocrysts
45
Al 2
O3
wt%
C
r 2O
3 w
t%
0.7
0.6
0.5 Wesselton
0.4
0.3
0.2
0.1
0
4 6 8 10 MgO wt%
12 14 16 18
Fig.32a – MgO-Al2O3 plot for Wesselton xenocrysts
12.00
10.00
8.00
6.00
Wesselton
4.00
2.00
0.00 4.00 6.00 8.00 10.00 12.00 14.00 16.00 18.00
MgO wt%
46
Al 2
O3
wt%
C
r 2O
3 w
t%
0.7
0.6
0.5 Otto's Kopje
0.4
0.3
0.2
0.1
0
4 6 8 10 MgO wt% 12 14 16 18
Fig.33a – MgO-Al2O3 plot for Otto’s Kopje xenocrysts
12.00
10.00
8.00
6.00
Otto's Kopje
4.00
2.00
0.00 4.00 6.00 8.00 10.00 12.00 14.00 16.00 18.00
MgO wt%
Fig.33b– MgO-Cr2O3 plot for Otto’s Kopje xenocrysts
47
Fig. 34 – Ilmenite classification
scheme
48
6. Discussion
6.1 The classification of ilmenites As shown in the previous chapter, many of the distinctions and divisions are subtle and the
classification is not robust. Previous analyses of ilmenite megacrysts belonging to the Cr-poor
suite from different localities worldwide have shown a clear connection between the co-existing
phases and the major and trace element chemistry of the ilmenites. This has been interpreted as
sign of co-precipitation of ilmenite and silicate, with ilmenite being a minor phase in a fractional
crystallization process (Moore et al., 1992; Griffin et al., 1997). Thus, by analyzing trace and major
element in ilmenites from a single kimberlite, some workers have traced the onset of crystallization
of different silicates. For example, by using Zr, Ni, Ga, MgO and Cr2O3, Griffin et al. (1997)
pinpointed the start of crystallization of zircon, olivine and other silicates, for Cr-poor megacryst
suites from a variety of South African localities.
In the present study, although there are correlations between the chemistry of the ilmenites and
heir parageneses they are not as clear as those proposed for the Cr-poor megacryst suites.
Therefore, different processes are probably responsible for the crystallization of ilmenites in the
ilmenite-bearing xenoliths from Kimberley. Dunites, orthopyroxenites, Granny Smith rocks,
rutile-ilmenite intergrowths and MARID xenoliths have been previously analyzed by various
workers and in the following section their findings will be compared with the results of this study.
6.2 Ilmenite genesis Analysing the clinopyroxene and ilmenite in Granny Smiths, Boyd et al. (1984) concluded that the
ilmenite and clinopyroxene were not in equilibrium and that ilmenite was introduced during
deformation. On the other hand, according to Gregoire et al. (2001), PIC (GS) rocks are deep
49
seated segregations of alkaline melts genetically related to type 1 kimberlite magmas (the
kimberlites in Kimberley are Group I) whereas MARID rocks are related to type 2 kimberlites.
This hypothesis is in agreement with the experimental study done by Sweeney et al. (1993) which
also mentions a possible MARID formation due to metasomatism. Another process responsible
for MARID genesis described by Waters (1987) is the high-pressure crystallization of ultra-
potassic magmas, similar to lamproites. Choukroun (2004), analysed Hf isotopes in rutile and
concluded that the Ti-rich parent melt of the MARID xenoliths reacted with ancient harzburgitic
mantle rocks, but his data do not provide any information whether MARID formation is related to
crystallization of the Ti-rich melt or the metasomatism of the harzburgite. The study also suggested
a relation between MARID and PIC rocks and concluded that PIC rocks may represent more
metasomatized versions of MARIDs. An ilmenite with MARID-like chemistry was found in a
Granny Smith sample but it contained orthopyroxene, which was not found in any MARID
xenoliths.
In the single Granny Smith nodule in which clinopyroxenes were analysed with the SEM and
electron microprobe, a difference in chemical compositions was documented between the margins
and centres of the diopside neoblasts and porphyroclasts (Fig. 15). The difference in chemistry
between the margins and centers of the neoblasts and porphyroclasts could be caused by the
infiltration of a melt/fluid causing both cryptic metasomatism (changing the chemistry of the
clinopyroxene) and modal metasomatism, introducing ilmenite.
Analysing olivine porphyroclasts and neoblasts, phlogopite, ilmenite and spinel in Kimberley Fe-
rich dunite xenoliths, Rehfeldt et al. (2007) concluded that ilmenite formation was linked to
metasomatism by a Fe and Ti-rich fluid. The pre-metasomatic olivines were cumulates from large
igneous province magmatism associated with the Karoo flood basalt episode, an idea first proposed
50
by Dawson et al. (1981). Some of the ilmenites studied by Rehfeldt et al. (2007), their type 1
ilmenites, formed at the expense of Cr-rich spinel. This is in agreement with the relationship
observed in sample 13-69-2 where ilmenite was found bordering a Cr-rich spinel with fine ilmenite
lamellae extending inside the spinel (Fig. 5C). This particular ilmenite has low Cr and Mg and
high Nb, unusual for the dunite ilmenites, and may represent the incipient stage of such a
replacement. Type 1 ilmenites have higher Cr, Sc, V, and Ga and lower Cu and Zn compared to
type 2 ilmenites, but no such differentiation was observed in the samples analysed in this study.
Temporally, the metasomatic process and the deformation seem to be related.
The formation of rutile-ilmenite intergrowths similar to those documented at Kimberley has been
attributed to exsolution of ilmenite/rutile from a previous Ti-rich metasomatic phase (Tollo et al.,
1987) whereas silicate-bearing rutile nodules have been interpreted by Schulze (1990) as magmatic
crystallization products. The fact that a clear relationship between Nb-Ta and Zr-Hf in ilmenite
was not observed in the samples analysed in this study, as would be expected from the
experimental data (Green et al., 1987), does not support the formation of ilmenite as a
crystallization product. Two different possibilities exist: ilmenite formation as exsolution from a
previous and still elusive unknown Ti-rich phase (Tollo et al., 1987) or the replacement of rutile
due to contact with a Fe-rich melt or fluid. The latter mechanism could also explain the presence
of ilmenite vein structures inside the rutile.
The processes that led to the formation of the orthopyroxenites represent another debated topic
due to the presence of fine apparent quench textures. Analysing fine-grained orthopyroxenite
xenoliths from Mzongwana, South Africa, Boyd et al. (1984) concluded that they formed as rapid
crystallization products of a pyroxenitic magma. Another possible genetic process was described
by Doyle et al. (2004) in which a Fe-Ti-rich megacryst parent magma interacted with peridotitic
51
solid mantle and previously formed megacryst veins or aggregates forming orthopyroxene and
ilmenite, according to the equation:
(Mg,Fe)2SiO4 + TiO2 = (MgFe)TiO3 + (MgFe)SiO3
olivine (magma) ilmenite orthopyroxene
Sample 13-67-54, in which orthopyroxenite occurs in contact with dunite (Fig. 7E) could indicate
the boundary of such a replacement process. Regardless of the process, it must have happened
quite close in time to their entrainment by the kimberlite, otherwise the very fine quench-like
textures wouldn’t have survived.
Formation due to related metasomatic processes could explain the chemical similarity in all of the
Kimberley ilmenite samples and the lack of a clear connection between the co-existing phases and
assemblages and the chemistry of the coexisting ilmenite. Many studies of mantle xenoliths from
Kimberley have invoked metasomatism as an important agent in the development of the chemical
composition of the xenoliths: e.g., metasomatism due to oceanic crust subduction ~ 2.9 Ga ago
(Green, 2000, Griffin et al., 1999, van Achterberg, 2004), the Karoo flood basalt magmatism
(Hawkesworth et al., 1990; Griffin et al., 2003) and the formation and emplacement of kimberlites
(Dawson, 1987; Griffin et al., 2003; Rehfeldt et al., 2007). Furthermore, ilmenite formation due to
metasomatism by a Fe-Ti rich melt has been previously described in literature and is a process
known worldwide (Rehfeldt et al., 2007, Ashchepkov et al., 2013). As stated earlier, the most
common hypothesis is that a Fe-Ti rich melt is responsible for the metasomatism, but the exact
composition and nature of the metasomatic agent is still debated.
In Fig. 14, the Kimberley ilmenite trace element are shown together with the maximum and
minimum trace element values for ilmenite megacrysts from South Africa, Yakutian kimberlites
and Gribb kimberlite (Kostrovitsky et al., 2004). All the ilmenites analysed from Kimberley plot
52
inside the field defined by South African ilmenite megacrysts whereas the analysis from Gribb
have lower Zr and Hf values and the ones from Yakutia have higher minimum Nb and Ta values.
Thus, a metasomatic overprint by a proto-kimberlitic megacrystic magma, like the one proposed
by Doyle et al. (2004) is entirely possible. Interaction with a megacrystic parent magma is also
considered responsible for the formation of ilmenite-rich polymictic breccias from Kimberley
(Giuliani et al., 2013) through circulation in narrow conduits and entraining fragments of different
lithologies. Ilmenite in the breccia is found as either large microscopically observable ilmenite
laths with minor rutile and with olivine, carbonate, sulphides, phlogopite and LIMA minerals
inclusions or as microscopic ilmenite-rutile intergrowths interstitial to olivine and orthopyroxene.
7. Conclusions Ilmenite is a very important indicator mineral used in the search for kimberlites. Although most
ilmenite from kimberlite, worldwide, belongs to the magmatic suite of Cr-poor megacryst minerals
(e.g., Schulze, 1987), this is not the case in the Kimberley area of South Africa. Members of the
Cr-poor megacryst suite are rare here (Schulze, 1995), but ilmenite is known as a component of
other rock types, such as the Granny Smith suite of diopsides (Boyd et al., 1984) and the MARID
suite (e.g., Dawson et al., 1977).
In this study, I have documented the composition and paragenesis of ilmenites from five
petrographically distinct mantle xenolith suites at Kimberley (Granny Smith, MARID, Fe-rich
dunites, orthopyroxenites and rutile-ilmenite nodules. Using these data, an ilmenite classification
scheme was developed, but more data are needed in order to better constrain and verify all the
defined fields. In an effort to determine the mantle source rock type of ilmenite xenocrysts from
Kimberley, the classification scheme was applied to ilmenite xenocrysts from four mines at
Kimberley (Bultfontein, Otto’s Kopje, Kamfersdam and Wesselton), and it was found that, despite
53
their close physical proximity to one another, they sampled distinctly different portions of the
mantle, as far as represented by their ilmenite suites.
This classification scheme exploits the differences in ilmenite composition between the different
paragenesis, but the relationship between ilmenite composition and mineral
association/composition is not as clear as in the Cr-poor megacryst suites. This is an indicator that
a process more complex than relatively simple fractional crystallization is responsible for the
crystallization of ilmenite in the five different suites at Kimberley. Most likely, metasomatism
plays an important role and this has been clearly documented in the Granny Smith and the dunite
xenoliths. The exact nature of the metasomatic agent is still elusive but it might be the same or
similar to the magma responsible for the formation of South African ilmenite megacrysts as
suggested for related ilmenite suites from other kimberlite localities.
54
References
Ashchepkov I. V., Alymova N. V., Logvinova A. M., Vladykin N. V., Kuligin S. S., Mityukhin
S. I., Stegnitsky Y. B., Prokopyev S. A., Salikhov R. F., Palessky V. S., Khmelnikova O. S.
(2013) Picroilmenites in Yakutian kimberlites: variations and genetic models. Solid Earth
Discussion, vol. 5 p 1259-1334
Boyd F.R, Dawson J.B., Smith J.V. (1983). Granny Smith diopside megacrysts from the
kimberlites of the Kimberley area and Jagersfontein, South Africa. Geochimica et
Cosmochimica Acta vol. 48, p. 381-384
Boyd, F. R., Nixon, P. H. and Boctor, N. Z. (1984). Rapidly crystallized garnet pyroxenite xenoliths
possible related to discrete nodules. Contributions to Mineralogy and Petrology vol. 86, p. 119-
130.
55
Carmody L.,Bodnar, R. J, Pokhilenko L. N, Taylor L. A, Pokhilenko N. P, Thaisen K. G, Tychkov
N., Sobolev N. V. (2014). Ilmenite as a diamond indicator mineral in the Siberian Craton: a tool
to predict diamond potential. Economic Geology, vol. 109, p. 775-783
Choukroun M., O’Reilly S.Y., Griffin W.L., Pearson N.J., Dawson J.B. (2004) Hf isotopes of
MARID (mica-amphibole-rutile-ilmenite-diopside) rutile trace metasomatic processes in the
lithospheric mantle. Geology, vol. 33, p. 45
Dalpe C., Baker D.R., Sutton S.R., (1995) Synchrotron X-ray Fluorescence and laser ablation ICP-
MS microprobes: useful instruments for analysis of experimental run-products. The Canadian
Mineralogist vol 33, p. 481-498
Dawson, J.B., Smith J.V., (1977). The MARID (mica-amphibole-rutile-ilmenite-diopside) suite of
xenoliths in kimberlite. Geochimica et Cosmochimica Acta vol. 41, p. 309-323
Dawson, J. B., Hervig, R. L. & Smith, J. V. (1981). Fertile iron-rich dunite xenoliths from the
Bultfontein kimberlite, South Africa. Fortschritte der Mineralogie vol 59, p. 303 - 324.
Dawson, J. B. (1987). The MARID suite of xenoliths in Kimberlites:relationship to veined and
metasomatised peridotite xenoliths. In: Nixon, P. H. (ed.) Mantle Xenoliths. Chichester: John
Wiley, p. 465-474.
Doyle, P. M, le Roex, A.P, Bell, D. R (2004) Fine-grained pyroxenites from the Gansfontein
kimberlite, South Africa: Evidence for megacryst magma - mantle interaction. South African
Journal Of Geology. vol 107 p. 285-300
56
Giuliani A., Kamenetsky V.S., Kendrick M.A., Philips D., Wyatt B.A., Maas R. (2013) Oxide,
sulphide and carbonate minerals in a mantle polymict breccia: Metasomatism by proto-kimberlite
magmas, and relationship to the kimberlite megacrystic suite. Chemical Geology, vol 353 p. 4-18
Griffin W.L., Moore R.O., Ryan C.G., Gurney J.J., Win T.T. (1997) Geochemistry of magnesian
ilmenite megacrysts from southern african kimberlites. Russian Geology and Geophysics vol.
38, p. 421-433 Griffin,W. L., O’Reilly, S. Y., Natapov, L. M. & Ryan, C. G. (2003). The evolution of lithospheric
mantle beneath the Kalahari Craton and its margins. Lithos vol 71 p. 215-241.
Griffin, W. L., Shee, S. R., Ryan, C. G., Win, T. T. & Wyatt, B. A. (1999). Harzburgite to lherzolite
and back again: metasomatic processes in ultramafic xenoliths form the Wesselton kimberlite,
Kimberley, South Africa. Contributions to Mineralogy and Petrology, vol. 134, p.232-250.
Gregoire, M., Bell, D.R., Le Roex, A.P. (2002) Trace element geochemistry of phlogopite-rich
mafix xenoliths: Their classification and their relationship to phlogopite-bearing peridotites and
kimberlites revisited. Contributions to Mineralogy and Petrology, vol. 142, p. 603-652
Green T. and Pearson N. (1987) An experimental study of Nb and Ta partitioning between Ti-rich
minerals and silicate liquids at high pressure and temperature. Geochim. Cosmochim. Acta vol
51, p 55-62. Green D. H. (2000) Magmatism Originating in the Upper Mantle. Crust - Mantle Interactions:
Proceedings of the International School Earth and Planetary Sciences. Sienna p. 77-95
57
Gurney, J.J., Helmstaedt, H., and Moore, R.O., 1993, A review of the use and application of mantle
mineral geochemistry in diamond exploration: Pure and Applied Chemistry, vol. 65, p. 2423–
2442 Hawkesworth, C. J., Erlank, A. J., Kempton, P. D. & Waters, F. G. (1990). Mantle metasomatism:
isotope and trace-element trends in xenoliths from Kimberley, South Africa. Chemical Geology
vol 85, p 19-34.
Klemme, S., Gunther, D., Hametner, K., Prowatke, S. and Zack, T. (2006). The partitioning of
trace elements between ilmenite, ulvospinel, armalcolite and silicate melts with implications for
the early differentiation of the moon. Chemical Geology vol. 234 p. 251-263.
Kostrovitsky S.I. Malkovets V.G. Verichev E.M. Garanin V.K. Suvorova L.V. (2004)
Megacrysts from the Grib kimberlite pipe (Arkhangelsk Province, Russia), Lithos, vol. 44 p 1 –
4 McDonough, W.F. (1990). Constraints on the composition of the continental lithospheric mantle.
Earth and Planetary Science Letters, vol. 101 p. 36-909
McDonough, W.F. and Sun, S.-S. (1995). Composition of the Earth. Chemical Geology vol. 120
p.223-253.
Moore R.O., Griffin W.L., Gurney J.J., Ryan C.G., Cousens D.R., Sie S.H., Suter G.F. (1992) Trace
element geochemistry of ilmenite megacrysts from the Monastery kimberlite, South Africa.
Lithos, vol. 29 p. 1 - 18
58
Pearson, D.G., Canil, D., and Shirey, S., 2003. Mantle samples included in volcanic rocks:
Xenoliths and Diamonds. In: Holland, H.D., Turekian K.K. (Eds.), The Mantle and Core.
Treatise on Geochemistry, vol. 2, p. 171-275.
Rehfeldt T., Jacob D.E., Carlson R.W., Foley S.F. (2007) Fe-rich Dunite Xenoliths from South
African Kimberlites: Cumulates from Karoo Flood Basalts Journal of Petrology V. 48 p 1387 –
1409 Schulze D. J. (1987) Megacrysts from alkalic volcanic rocks. In Mantle xenoliths (ed. P.
H. Nixon). John Wiley, Chichester. p. 433-451.
Schulze D.J, Anderson P.F.N., Hearn B.C., Hetman C.M., (1995) Origin and significance of
ilmenite megacrysts and macrocrysts from kimberlites. International Geology Review vol. 37,
p. 780-812
Schulze D.J. (1990) Silicate-bearing-rutile-dominated nodules from South African kimberlites:
metasomatized cumulates American Mineralogist, vol. 75, p. 97-104
Schulze D. J. (1995) Low-Ca garnet harzburgites from Kimberley, South Africa: Abundance and
bearing on the structure and evolution of the lithosphere. J. Geophys. Res. vol 100, p. 12.513-
12.526 Sweeney RJ, Thompson AB, Ulmer P (1993) Phase relations of a natural MARID composition and
implications for MARID genesis, lithospheric melting and mantle metasomatism. Contrib
Mineral Petrol vol. 115 p. 225–241
Tollo R.P., Haggerty S.E. (1987) Nb-Cr-rutile in the Orapa kimberlite, Botswana. Canadian
Mineralogist, vol. 25, p. 251-264
59
Van Achterbergh, E. (2004). Geochemical fingerprints of mantle metasomatism. PhD
thesis, Macquarie University, Sydney
Waters F.G. (1987) A suggested origin for MARID xenoliths in kimberlites by high
pressure crystallization of an ultrapotassicrock such as lamproite. Contrib Mineral
Petrol vol. 95, p. 523–
533 White J.L, Sparks R.S.J., Bailey K., Barnett W.P., Field M., Windsor L. (2012) Kimberlite
sills and dykes associated with the Wesselton Kimberlite pipe, Kimberley, South
Africa. South African Journal of Mineralogy vol. 115 p. 1-32
Wyatt, B.A., Baumgartner, M. Anckar E., Grutter H., (2004) Compositional
classification of
“kimberlitic” and “non-kimberlitic” ilmenite. Lithos, vol. 77, p. 819-840
Zhao D., Essene E.J., Zhang Y. (1999) – An oxygen barometer for rutile-ilmenite
assemblages: oxidation state of metasomatic agens in the mantle. Earth and Planetary
Science Letters, vol. 166 p. 127-137
A
PP
EN
DIX
Tab
le 5. Ilm
enite m
ajor an
d trace elem
ents an
alysis
Du
nite ilm
enites
13 - 4
1-3
3
13
-67
-52
1
3-6
7-5
4
13
-69
-1
13
-69
-2
13
-74
-49
1
3-6
7-5
4
13
-68
-4
13
-74
-47
Majo
r elem
ents w
t%
SiO2
0.0
4
0.0
1
0.0
1
0.0
1
0.0
0
0.0
0
0.0
0
0.0
1
0.0
1
TiO2
5
4.3
9
54
.06
5
4.07
5
4.3
7
41
.59
4
4.81
4
9.02
5
5.09
5
0.98
Nb
2 O5
0.0
9
0.1
0
0.1
0
0.1
1
1.7
4
1.2
0
0.0
9
0.1
3
0.0
8
Al2 O
3
0.4
1
0.1
9
0.2
7
0.3
2
0.0
1
0.0
5
0.2
2
0.2
6
0.5
9
FeO
t 2
8.0
1
30
.28
2
9.38
2
8.43
4
7.5
0
41
.31
31
.36
27
.92
30
.86
Mn
O
0.2
8
0.3
0
0.2
8
0.2
9
0.3
0
0.2
4
0.1
8
0.2
8
0.2
0
MgO
1
4.3
5
13
.36
1
3.74
1
4.2
4
6.1
5
8.7
3
11
.79
14
.68
12
.05
CaO
0.0
2
0.0
2
0.0
1
0.0
3
0.0
2
0.0
2
0.0
3
0.0
2
0.0
2
Cr
2 O3
1.8
3
1.0
7
1.8
6
1.5
0
0.0
8
1.8
6
6.5
3
1.4
5
4.7
1
TOTA
L 9
9.4
2
99
.38
9
9.73
9
9.30
9
7.3
7
98
.22
99
.21
99
.85
99
.50
Fe2 O
3
6.3
5
6.8
8
6.9
8
6.4
4
21
.71
1
8.24
1
2.77
5
.99
9
.83
FeO
2
2.3
0
24
.09
2
3.10
2
2.6
3
27
.96
2
4.90
1
9.87
2
2.53
2
2.01
Trace elemen
t pp
m
Li 2
.31
1
.64
1
.70
6
.10
2
.36
2
.86
3
.13
Na
29
7.9
9
18
5.98
2
81
.88
57
0.98
1
39
.95
65
5.92
5
38
.63
Mg
93
77
3.8
5
72
80
4.6
9
88
97
3.3
0
85
61
7.5
9
50
25
3.2
6
68
90
9.6
1
88
59
8.4
7
K
20
.66
2
3.1
1
24
.55
16
.52
25
.30
9.9
0
30
.99
Ca
72
.01
1
02
.11
77
.31
19
8.90
5
2.60
2
45
.45
10
4.59
Sc 1
5.6
8
17
.08
1
7.07
2
2.31
3
6.26
2
6.54
1
9.41
Ti 3
34
32
3.3
5
31
40
76
.97
3
38
20
1.0
0
30
39
24
.14
3
61
65
7.3
6
28
05
53
.07
3
30
52
5.2
8
V
93
2.3
0
89
2.05
1
03
7.7
3
11
06
.67
2
06
0.8
1
11
62
.25
1
15
7.6
6
Cr
12
51
8.6
1
73
19
.63
1
27
92
.25
1
02
61
.16
1
27
23
.84
4
46
68
.87
9
94
3.4
0
Mn
2
43
1.4
1
23
20
.10
2
42
4.4
6
18
86
.30
2
90
4.8
8
14
92
.12
2
30
5.9
0
Fe 1
75
62
7.8
6
15
88
41
.88
1
80
01
3.6
0
14
75
02
.01
3
54
20
1.2
1
17
59
26
.65
1
75
18
8.2
4
Co
1
72
.28
1
53
.34
16
1.46
2
02
.38
14
5.72
1
95
.48
18
6.50
60
N
i 1
18
2.0
7
60
7.84
9
70
.47
89
0.87
3
22
.32
17
36
.68
9
16
.16
Cu
2
7.3
2
23
.65
21
.10
32
.83
13
.86
44
.19
27
.86
Zn
11
0.5
9
10
5.96
1
14
.74
14
5.87
1
33
.78
13
7.38
1
36
.81
Ga
8.8
9
8.0
4
10
.08
12
.89
3.1
3
11
.46
11
.02
Ge
1
.04
1
.00
-
1.4
9
1.3
7
1.6
3
1.5
3
Sr 0
.23
0
.36
0
.18
0
.19
0
.23
1
.97
0
.24
Y 0
.07
0
.08
0
.05
0
.09
0
.10
0
.42
0
.07
Zr 2
89
.08
4
97
.02
45
6.79
4
94
.88
68
4.67
4
91
.48
53
4.26
Nb
5
66
.39
7
40
.72
69
6.34
8
24
.77
89
75
.78
5
08
.09
77
3.11
Sn
7.1
2
8.2
0
7.8
3
9.0
5
21
.60
6.3
6
9.3
1
Ba
0.3
0
0.2
8
0.3
2
0.5
5
0.4
3
1.8
0
0.4
1
La -
0.0
3
- -
0.0
2
0.3
4
0.0
2
Ce
-
0.0
5
- 0
.04
0
.04
0
.58
0
.02
Pr
- 0
.01
-
- -
0.0
6
0.0
1
Nd
-
0.0
4
- 0
.03
0
.05
0
.31
0
.04
Sm
- -
- 0
.03
0
.04
0
.14
-
Eu
0.0
1
- -
0.0
4
0.0
1
0.0
5
0.0
1
Gd
0
.07
-
- 0
.10
-
0.0
9
-
Tb
- 0
.00
-
0.0
5
0.0
0
0.0
1
0.0
0
Dy
- 0
.02
0
.03
0
.06
0
.02
0
.07
0
.02
Ho
0
.00
0
.00
-
0.0
1
0.0
0
0.0
3
0.0
0
Er -
0.0
1
- 0
.08
0
.02
0
.06
0
.02
Tm
- 0
.00
-
0.0
2
0.0
0
0.0
2
0.0
0
Yb
- 0
.02
-
0.0
2
0.0
2
0.1
1
0.0
2
Lu
0.0
0
- -
0.0
1
0.0
0
0.0
2
0.0
1
Hf
11
.96
1
5.75
1
7.01
1
6.34
1
6.52
1
6.90
1
8.44
Ta 5
5.5
1
59
.77
63
.61
11
7.91
6
83
.97
70
.65
74
.35
W
0.0
6
0.0
4
0.0
6
0.1
4
0.2
1
0.1
2
0.0
8
Pb
0
.21
0
.27
0
.31
-
0.2
2
0.5
1
6.4
8
Th
0.0
0
0.0
0
0.0
0
0.0
1
0.0
0
0.0
7
0.0
0
U
0.0
1
0.0
1
0.0
1
- 0
.06
0
.04
0
.01
61
13
-74
-75
1
3-7
4-7
4
13
-47
-12
6
13
-47
-12
5
13
-74
-77
Majo
r elem
ents w
t%
SiO2
0
.04
0.0
3
0.0
4
0.0
4
0.0
2
TiO2
4
6.92
5
4.9
6
54
.16
5
4.06
5
5.40
Nb
2 O5
0
.62
0.0
7
0.1
9
0.1
4
0.1
0
Al2 O
3
0.0
0
0.2
9
0.1
1
0.1
6
0.0
9
FeO
t 4
2.46
2
7.66
3
1.10
2
6.91
3
0.19
Mn
O
0.4
2
0.2
6
0.3
1
0.1
9
0.3
0
MgO
7
.43
1
4.9
5
13
.24
1
4.66
1
2.99
CaO
0
.01
0.0
1
0.0
0
0.0
1
0.0
6
Cr
2 O3
1
.78
2.2
6
1.0
5
4.1
0
1.1
4
TOTA
L 1
01
.23
10
1.18
1
00
.94
10
1.00
1
00
.76
Fe2 O
3
15
.62
6.8
1
7.2
9
7.0
7
4.7
7
FeO
2
8.41
2
1.5
4
24
.54
2
0.55
2
5.90
Trace elemen
t pp
m
Li
2.2
7
2.0
7
1.9
7
1.7
2
0.4
6
Na
15
2.25
1
85
.35
17
8.27
1
56
.51
21
.86
Mg
46
80
3.9
1
92
94
2.8
4
82
01
7.1
3
53
76
1.0
6
50
93
.23
K
5.7
6
8.3
6
9.3
4
- 3
8.03
Ca
50
.74
65
.01
21
1.09
9
1.80
3
1.70
Sc 3
8.09
1
7.46
2
1.58
1
2.61
0
.84
Ti 2
88
67
0.3
2
33
94
24
.50
3
40
64
3.1
9
20
12
38
.10
1
23
77
.32
V
10
72
.59
1
71
.20
10
6.64
1
11
.90
16
.40
Cr
12
14
2.3
7
15
44
4.4
1
71
97
.86
2
80
40
.33
2
45
.79
Mn
3
14
3.9
0
21
29
.87
2
24
1.6
6
99
0.40
8
5.99
Fe 2
59
88
5.4
9
16
45
37
.97
1
79
27
1.5
9
94
55
0.2
1
98
47
.73
Co
1
40
.35
17
6.23
1
68
.12
10
5.70
6
.69
Ni
34
5.43
1
36
3.3
2
82
8.71
1
32
1.4
6
42
.79
Cu
8
.00
2
8.38
3
0.54
2
0.98
2
.11
Zn
14
6.11
1
16
.19
12
1.83
6
4.11
4
.87
Ga
3.5
7
10
.19
9.2
3
7.3
7
0.1
7
Ge
1
.63
1
.18
1
.20
0
.73
0
.18
62
Sr
1.2
7
0.2
1
0.2
3
0.1
7
0.6
4
Y 0
.04
0
.06
0
.14
0
.08
0
.02
Zr 6
23
.54
43
6.05
5
97
.66
22
0.21
1
2.86
Nb
4
35
4.4
2
61
2.31
1
03
3.6
8
36
0.28
1
9.91
Sn
19
.94
7.9
8
9.8
1
4.4
4
0.1
9
Ba
1.8
9
0.3
0
0.3
2
0.1
8
1.2
3
La 0
.08
-
- 0
.02
0
.11
Ce
0
.14
0
.01
0
.03
0
.05
0
.15
Pr
0.0
2
- 0
.01
-
0.0
1
Nd
0
.05
0
.03
0
.03
0
.04
0
.05
Sm
0.0
4
- 0
.05
0
.03
0
.02
Eu
0.0
1
0.0
1
0.0
1
0.0
1
0.0
0
Gd
-
0.0
4
- 0
.01
0
.01
Tb
- 0
.00
0
.01
0
.00
0
.00
Dy
- 0
.01
0
.03
0
.01
0
.01
Ho
-
0.0
0
0.0
1
0.0
0
0.0
0
Er 0
.01
0
.01
0
.01
0
.01
0
.00
Tm
- 0
.00
0
.01
0
.00
0
.00
Yb
0.0
4
0.0
2
0.0
1
0.0
2
0.0
0
Lu
0.0
0
- 0
.00
0
.00
0
.00
Hf
17
.81
16
.18
19
.58
8.2
5
0.4
8
Ta 4
46
.58
69
.81
10
8.51
4
0.83
3
.08
W
0.1
3
0.0
9
0.0
6
0.0
6
0.0
1
Pb
1
.31
0
.92
0
.81
0
.26
0
.08
Th
0.0
0
0.0
0
0.0
0
0.0
0
0.0
2
U
0.0
4
0.0
1
0.0
1
0.0
1
0.0
0
63
Gran
ny Sm
ith ilm
enites
13
-41
-31
1
3-4
5-2
35
1
3-4
5-2
38
1
3-4
5-2
33
1
3-4
5-2
43
1
3-4
1-3
2
13
-45
-26
9
13
-74
-52
1
3-7
4-5
3
Majo
r elem
ents w
t%
SiO2
0
.02
0
.01
0
.01
0
.01
0
.00
0
.02
0
.03
0
.03
0
.02
TiO2
5
3.7
3
54
.12
54
.03
54
.04
54
.24
5
3.86
5
3.58
5
3.87
5
3.91
Nb
2 O5
0
.14
0
.11
0
.07
0
.09
0
.10
0
.09
0
.07
0
.09
0
.07
Al2 O
3
0.1
7
0.3
0
0.4
1
0.4
1
0.2
6
0.3
6
0.4
9
0.3
5
0.4
9
FeO
t 3
0.7
8
28
.97
27
.69
27
.73
29
.25
2
8.56
2
6.92
2
8.18
2
6.78
Mn
O
0.3
1
0.2
8
0.2
5
0.2
7
0.2
9
0.2
6
0.2
8
0.2
9
0.2
7
MgO
1
3.1
0
13
.94
14
.50
14
.47
13
.84
1
4.14
1
4.42
1
3.94
1
4.51
CaO
0
.02
0
.03
0
.02
0
.02
0
.03
0
.02
0
.02
0
.02
0
.03
Cr
2 O3
1
.03
1
.52
2
.19
2
.17
1
.34
2
.09
2
.71
1
.74
2
.71
TOTA
L 1
00
.01
9
9.94
9
9.86
9
9.90
1
00
.03
1
00
.13
99
.16
99
.14
99
.41
Fe2 O
3
7.1
9
6.7
1
6.8
6
6.8
0
6.6
6
7.2
1
6.5
6
6.2
1
6.2
6
FeO
2
4.3
1
22
.93
21
.52
21
.61
23
.26
2
2.08
2
1.01
2
2.59
2
1.14
Trace elemen
ts pp
m
Li 2
.59
2
.06
2
.55
2
.69
2
.32
2
.63
2
.30
4
.28
Na
26
9.0
3
29
6.12
3
10
.42
41
1.66
3
72
.99
3
70
.77
27
0.30
8
21
.70
Mg
80
40
4.1
9
87
12
7.9
0
89
63
7.3
5
92
81
8.5
7
84
29
9.0
6
88
49
5.7
5
82
65
5.2
9
83
85
4.3
8
K
28
.49
1
7.02
2
4.78
1
2.87
2
0.9
6
33
.21
18
.51
25
.36
Ca
81
.38
9
0.04
5
6.73
1
32
.93
10
7.7
9
12
3.12
9
1.54
9
1.67
Sc 1
7.8
9
15
.88
15
.52
15
.20
16
.64
1
6.20
1
6.48
1
7.52
Ti 3
30
53
5.9
1
32
69
22
.60
3
31
92
1.7
7
33
33
93
.78
3
20
12
0.4
7
33
17
26
.71
3
23
49
0.1
5
31
17
03
.58
V
10
55
.17
9
86
.85
10
22
.78
1
01
9.8
7
10
29
.95
1
05
4.5
4
99
5.77
1
16
5.6
9
Cr
70
46
.00
1
03
97
.97
1
49
81
.29
1
48
44
.48
9
16
6.6
4
14
29
7.2
2
86
87
.78
1
85
38
.49
Mn
2
66
5.0
1
23
22
.35
2
18
6.0
8
21
57
.67
2
33
7.6
2
23
54
.61
2
43
8.2
1
20
87
.18
Fe 1
77
67
3.9
1
16
13
22
.11
1
66
15
2.7
6
16
75
76
.59
1
76
45
6.4
6
17
66
36
.76
1
75
69
7.5
1
14
40
75
.04
Co
1
49
.99
1
54
.30
16
5.41
1
59
.96
16
0.9
3
16
4.84
1
56
.36
18
3.37
Ni
53
3.1
9
82
8.43
1
15
1.2
6
11
30
.58
7
33
.48
1
16
4.1
6
64
7.54
1
55
4.0
7
Cu
1
7.6
8
23
.84
24
.58
26
.31
22
.79
2
5.09
1
9.96
3
3.83
Zn
11
3.3
1
10
8.74
1
10
.17
10
5.14
1
09
.68
1
13
.92
10
9.81
1
25
.74
64
G
a 8
.61
9
.44
1
0.90
1
0.54
9
.50
1
1.18
8
.36
1
4.58
Ge
1
.12
1
.22
0
.95
1
.16
1
.03
0
.97
0
.70
1
.43
Sr 0
.22
0
.19
0
.18
0
.37
0
.23
1
.11
0
.26
0
.27
Y 0
.06
0
.07
0
.05
0
.06
0
.07
0
.07
0
.07
0
.08
Zr 5
51
.67
4
27
.23
38
5.07
3
90
.21
47
9.5
5
42
5.76
4
55
.68
49
5.63
Nb
1
05
1.2
2
86
2.13
4
90
.60
50
2.92
7
52
.26
6
02
.56
92
2.14
5
89
.95
Sn
8.9
4
7.1
1
7.0
3
6.6
9
7.5
9
7.8
6
7.6
0
10
.12
Ba
0.3
3
0.3
1
0.3
2
0.4
9
0.5
1
3.4
1
- 0
.94
La -
- -
0.0
4
- 0
.05
0
.02
-
Ce
0
.02
-
- 0
.04
-
0.0
9
0.0
3
0.0
4
Pr
- -
- 0
.01
-
- -
-
Nd
-
- -
0.0
5
- 0
.04
0
.03
-
Sm
- -
- -
- -
- 0
.04
Eu
- -
- -
- -
- 0
.02
Gd
-
- -
- -
- -
0.0
5
Tb
- -
- -
- -
- 0
.02
Dy
0.0
2
0.0
2
- 0
.02
0
.02
0
.02
0
.03
0
.06
Ho
0
.00
-
- -
- -
- 0
.02
Er 0
.01
0
.01
-
- -
- 0
.03
0
.02
Tm
0.0
0
0.0
0
- 0
.00
-
- -
0.0
1
Yb
0.0
1
- -
0.0
3
- 0
.04
0
.02
0
.02
Lu
0.0
0
0.0
0
- -
- -
- -
Hf
19
.40
1
3.67
1
4.08
1
4.23
1
7.0
3
15
.34
15
.97
17
.08
Ta 7
5.9
1
63
.86
52
.03
56
.09
67
.36
5
8.11
7
9.81
7
9.77
W
0.0
6
0.0
8
0.0
8
0.0
6
0.0
6
0.1
2
0.0
6
0.0
9
Pb
0
.09
0
.06
0
.17
0
.15
0
.32
0
.37
0
.14
0
.07
Th
0.0
0
0.0
0
- 0
.01
-
- 0
.01
-
U
0.0
1
0.0
1
- 0
.01
-
- 0
.01
0
.02
65
13
-74
-51
1
3-7
4-4
8
13
-47
-60
1
3-4
7-6
2
13
-47
-63
1
3-6
9-5
1
3-6
9-4
1
3-7
4-5
4
Majo
r elemen
ts wt%
SiO2
0
.01
0
.00
0
.01
0
.02
0
.02
0
.01
0
.02
0
.01
TiO2
5
3.5
5
54
.12
5
4.11
5
4.1
6
53
.82
54
.01
54
.28
54
.37
Nb
2 O5
0
.07
0
.10
0
.07
0
.10
0
.08
0
.08
0
.13
0
.14
Al2 O
3
0.5
3
0.2
9
0.3
1
0.2
9
0.3
7
0.2
6
0.1
5
0.1
3
FeO
t 2
6.7
2
28
.78
2
8.36
2
8.9
1
28
.33
29
.26
29
.89
30
.10
Mn
O
0.2
5
0.2
8
0.2
9
0.3
1
0.2
7
0.3
2
0.3
2
0.3
3
MgO
1
4.4
7
13
.58
1
3.90
1
3.7
3
13
.93
13
.42
13
.32
13
.29
CaO
0
.02
0
.02
0
.03
0
.02
0
.02
0
.03
0
.06
0
.06
Cr
2 O3
3
.19
1
.47
1
.60
1
.51
1
.98
1
.43
1
.06
1
.04
TOTA
L 9
9.4
7
99
.22
9
9.29
9
9.6
7
99
.48
99
.45
99
.84
10
0.10
Fe2 O
3
6.7
3
5.7
9
6.0
9
6.2
1
6.5
4
6.1
6
6.1
7
6.2
5
FeO
2
0.6
6
23
.57
2
2.88
2
3.3
2
22
.44
23
.72
24
.34
24
.48
Trace elemen
ts pp
m
Li 3
.36
2.2
3
3.9
4
4.1
0
2.9
0
4.3
9
2.6
6
Na
89
5.1
4
6
39
.37
75
2.2
9
64
3.90
6
28
.24
68
2.37
1
40
.62
Mg
82
59
1.3
9
7
91
92
.25
7
89
59
.26
8
52
99
.44
8
82
67
.01
8
35
26
.07
9
82
44
.77
K
52
.78
36
.89
- 7
1.22
3
2.71
9
.79
6
4.51
Ca
15
7.2
2
1
18
.24
17
5.1
8
83
.11
19
3.53
2
20
.43
24
3.70
Sc 1
7.6
6
1
9.24
1
8.7
3
17
.79
18
.86
19
.55
18
.90
Ti 3
13
73
9.3
5
3
18
17
4.5
0
30
80
65
.92
3
22
95
7.0
3
30
18
02
.22
3
03
22
4.4
2
37
45
81
.93
V
12
31
.29
11
40
.93
1
16
4.7
1
11
05
.92
1
04
8.8
3
10
63
.09
8
0.52
Cr
18
53
8.4
9
1
00
55
.94
1
09
45
.24
1
03
29
.57
1
35
44
.73
9
78
2.3
0
71
14
.40
Mn
2
18
1.6
7
2
50
0.6
0
24
14
.90
2
51
4.2
9
22
09
.50
2
41
9.6
2
24
91
.77
Fe 1
45
74
8.6
9
1
60
59
4.1
8
15
12
81
.70
1
73
34
2.0
1
17
05
35
.97
1
71
64
8.0
3
20
27
87
.96
Co
1
75
.90
17
4.65
1
73
.66
1
72
.83
17
9.41
1
69
.90
16
7.97
Ni
15
94
.29
91
4.11
9
62
.07
9
90
.64
11
67
.96
9
20
.68
58
4.12
Cu
4
2.8
5
3
4.42
3
3.2
9
31
.08
32
.98
28
.88
20
.48
Zn
13
4.9
7
1
42
.93
15
4.1
4
14
8.69
1
41
.10
14
5.88
1
18
.18
Ga
15
.59
12
.88
11
.35
1
2.34
1
2.94
1
1.46
7
.71
Ge
3
.46
2.5
6
1.8
8
2.2
4
1.4
8
2.1
7
1.5
0
66
Sr
0.2
2
0.2
4
0.3
0
0.1
2
0.1
8
0.2
3
0.4
5
Y 0
.08
0
.08
0
.11
0
.04
0
.09
0
.09
0
.11
Zr 5
25
.64
58
3.96
5
67
.96
5
06
.99
41
6.41
5
09
.56
54
1.87
Nb
6
17
.74
84
5.96
6
20
.89
6
69
.14
58
8.19
5
94
.32
99
5.34
Sn
11
.18
10
.91
10
.47
8
.62
9
.12
8
.63
8
.95
Ba
1.0
9
1.6
3
0.8
0
- 0
.40
0
.17
0
.91
La 0
.04
-
0.0
3
0.0
3
0.0
1
0.0
2
0.0
3
Ce
-
0.0
2
0.0
3
- 0
.03
0
.02
0
.03
Pr
- -
0.0
3
- 0
.01
0
.03
0
.01
Nd
0
.05
-
0.0
4
0.0
9
0.1
0
- 0
.03
Sm
- -
0.1
1
0.0
6
0.0
7
- -
Eu
0.0
5
0.0
2
- 0
.03
0
.05
0
.04
-
Gd
-
0.0
8
- 0
.05
0
.07
0
.14
0
.02
Tb
0.0
1
0.0
2
0.0
0
0.0
1
- -
0.0
0
Dy
0.0
5
- -
- 0
.05
0
.02
0
.02
Ho
0
.01
-
- 0
.02
0
.00
0
.01
0
.00
Er 0
.03
0
.06
0
.04
0
.06
0
.03
-
0.0
2
Tm
0.0
1
0.0
1
0.0
0
0.0
2
0.0
1
0.0
1
0.0
0
Yb
0.0
4
0.0
4
0.0
2
0.0
2
- 0
.01
0
.02
Lu
0.0
1
- -
0.0
1
0.0
1
0.0
1
0.0
0
Hf
18
.07
19
.72
17
.73
1
8.64
1
6.23
1
8.43
2
0.20
Ta 8
7.86
1
12
.12
76
.30
9
4.24
7
4.20
8
2.58
8
3.44
W
0.1
8
0.0
9
0.0
6
0.1
5
0.0
9
0.0
4
0.0
4
Pb
0
.04
-
0.1
2
0.0
2
- 0
.02
2
.69
Th
- 0
.01
0
.01
-
0.0
1
- 0
.00
U
0.0
1
0.0
2
0.0
1
0.0
1
0.0
3
0.0
3
0.0
1
67
FR
B4
93
FR
B7
77
1
3-7
4-2
2
13
-74
-48
Majo
r elemen
ts wt%
SiO2
0.0
1
0.0
1
0.0
0
0.0
1
TiO2
54
.87
55
.06
5
2.5
8
54
.16
Nb
2 O5
0.1
1
0.1
1
0.3
4
0.0
6
Al2 O
3 0
.18
0
.35
0
.01
0
.46
FeOt
29
.36
27
.15
3
4.1
2
26
.83
Mn
O
0.3
1
0.2
7
0.3
3
0.2
4
MgO
1
3.71
1
4.7
3
11
.00
1
4.75
CaO
0
.03
0
.02
0
.05
0
.02
Cr
2 O3
1
.35
2
.15
1
.40
2
.81
TOTA
L 1
00
.51
1
00
.41
1
00
.63
1
00
.01
Fe2 O
3 5
.90
5
.63
7
.93
6
.60
FeO
24
.04
22
.08
2
6.9
8
20
.89
Trace elemen
ts pp
m
Li
3.0
0
2
.83
Na
40
5.0
7
4
43
.28
Mg
92
70
5.8
0
5
62
79
.42
K
11
9.0
3
4
7.89
Ca
50
6.1
2
5
6.26
Sc 1
6.2
8
1
3.59
Ti 3
59
35
9.5
8
2
11
56
8.4
2
V
14
7.0
7
8
14
.21
Cr
14
72
8.1
8
2
18
22
.06
Mn
2
12
6.8
3
1
02
5.0
4
Fe
17
01
80
.38
10
35
90
.06
Co
1
76
.12
14
6.40
Ni
13
21
.27
15
17
.51
Cu
3
2.7
3
2
9.71
Zn
12
0.5
4
9
6.00
Ga
11
.66
11
.85
Ge
0
.77
1.1
3
68
Sr
5.5
4
0.0
9
Y 0
.15
0
.04
Zr 3
93
.65
3
11
.75
Nb
6
12
.86
4
41
.58
Sn
7.6
5
7.3
4
Ba
6.5
0
0.6
2
La 0
.90
-
Ce
1
.63
0
.03
Pr
0.3
2
0.0
1
Nd
1
.45
-
Sm
0.2
3
-
Eu
0.0
7
-
Gd
0
.18
0
.10
Tb
0.0
1
0.0
1
Dy
0.0
5
0.0
3
Ho
0
.01
0
.00
Er 0
.03
0
.00
Tm
- 0
.00
Yb
- 0
.13
Lu
- -
Hf
14
.70
1
2.05
Ta 5
5.4
1
55
.29
W
0.0
7
0.0
6
Pb
0
.55
-
Th
0.1
7
-
U
0.0
4
0.0
1
69
MA
RID
ilmen
ites
13
-41
-22
1
3-4
5-2
68
1
3-4
0-5
4
13
-74
-40
1
3-7
4-4
0
13
-74
-19
1
3-1
20
-50
13
-74
-40
Majo
r elem
ents w
t%
SiO2
0
.01
0
.01
0
.01
0
.01
0
.03
0
.01
0
.01
0
.02
TiO2
5
2.3
5
44
.55
4
8.36
5
6.65
5
2.47
5
3.80
5
2.81
5
8.40
Nb
2 O5
0
.03
1
.23
0
.55
0
.08
0
.01
0
.32
0
.12
0
.13
Al2 O
3
0.0
2
0.0
1
0.0
1
0.0
3
0.0
5
0.0
3
0.0
3
0.0
0
FeO
t 3
8.2
0
43
.84
4
2.48
2
5.96
3
7.13
3
1.11
3
6.55
2
3.66
Mn
O
0.4
5
0.4
1
0.5
9
0.3
6
0.4
9
0.3
1
0.3
9
0.4
3
MgO
8
.08
6
.53
6
.59
1
5.21
8
.33
1
2.04
8
.88
1
7.53
CaO
0
.02
0
.01
0
.01
0
.05
0
.03
0
.02
0
.03
0
.05
Cr
2 O3
0
.47
1
.98
0
.42
0
.51
0
.40
1
.27
0
.62
0
.47
TOTA
L 1
00
.33
1
00
.30
1
00
.23
99
.14
99
.54
99
.44
10
0.04
1
01
.02
Fe2 O
3
6.8
5
17
.17
1
2.15
2
.98
6
.08
5
.28
6
.07
3
.28
FeO
3
2.0
4
28
.39
3
1.55
2
3.28
3
1.66
2
6.35
3
1.09
2
0.71
Trace elem
ents p
pm
Li 3
.10
1
.43
2
.51
Na
28
6.0
4
30
3.5
8
18
3.30
Mg
59
27
4.3
2
42
97
6.3
5
42
23
0.0
5
K
34
.56
1
7.9
5
27
.91
Ca
- 4
0.2
4
38
.97
Sc 9
.53
3
1.7
0
25
.35
Ti 3
70
69
2.7
8
27
14
64
.19
3
04
33
6.0
4
V
11
92
.45
2
23
1.7
8
11
39
.50
Cr
32
15
.16
1
35
44
.73
2
87
3.1
2
Mn
4
17
9.7
7
33
58
.10
4
95
2.7
7
Fe 2
19
15
4.6
7
27
39
78
.03
2
63
02
2.3
1
Co
1
90
.40
1
33
.26
1
36
.45
Ni
55
1.4
2
35
4.1
4
29
0.52
Cu
2
3.7
5
7.6
6
5.2
3
70
Zn
2
04
.78
1
42
.43
1
64
.33
Ga
2.1
8
1.3
2
0.6
8
Ge
1
.73
0
.96
0
.86
Sr 0
.19
0
.19
0
.18
Y 0
.12
0
.05
0
.04
Zr 2
24
.96
4
63
.75
2
83
.25
Nb
3
05
.38
9
31
0.7
4
38
85
.11
Sn
6.9
9
19
.70
9
.81
Ba
- -
-
La -
0.0
4
-
Ce
0
.12
0
.05
-
Pr
0.0
2
- -
Nd
-
- 0
.03
Sm
- -
-
Eu
- -
0.0
2
Gd
0
.20
-
-
Tb
0.0
2
- 0
.00
Dy
- 0
.02
0
.02
Ho
-
- 0
.00
Er -
0.0
2
0.0
1
Tm
- 0
.00
-
Yb
0.3
1
0.0
3
-
Lu
- 0
.01
-
Hf
7.0
4
11
.72
7
.75
Ta 2
6.6
2
57
8.3
1
10
5.54
W
2.5
4
0.1
9
0.1
5
Pb
-
0.1
3
0.1
7
Th
0.0
6
0.0
1
-
U
0.0
3
0.0
5
0.0
4
71
1
3-7
4-3
8
13
-74
-37
1
3-7
4-5
0
Majo
r elemen
ts wt%
SiO2
0
.01
0
.02
0
.02
TiO2
5
6.6
7
55
.21
5
4.51
Nb
2 O5
0
.12
0
.33
0
.18
Al2 O
3
0.0
0
0.0
3
0.0
1
FeO
t 2
9.4
4
28
.61
3
3.61
Mn
O
0.3
0
0.2
5
0.3
6
MgO
1
3.2
8
13
.96
1
0.62
CaO
0
.13
0
.03
0
.04
Cr
2 O3
0
.62
1
.62
0
.78
TOTA
L 1
00
.88
1
00
.56
1
00
.58
Fe2 O
3
3.0
7
5.0
2
4.5
4
FeO
2
6.6
8
24
.09
2
9.52
Trace elemen
ts pp
m
Li
2
.86
5
.70
Na
3
09
.53
1
84
7.6
0
Mg
9
37
73
.62
8
77
46
.68
K
1
6.1
9
63
37
.10
Ca
2
20
.67
6
49
0.9
6
Sc
17
.57
1
8.27
Ti
36
19
14
.10
3
90
54
5.3
3
V
6
39
.59
4
28
.43
Cr
1
10
75
.21
5
36
3.1
6
Mn
21
60
.54
3
25
1.2
3
Fe
1
79
68
5.1
6
21
51
33
.36
Co
22
2.0
6
31
0.94
Ni
9
52
.37
1
49
4.3
0
Cu
23
.92
3
73
.20
Zn
1
19
.16
1
86
.98
Ga
2
.61
1
.92
Ge
1.3
3
1.3
6
72
Sr
0.2
9
51
.83
Y 0
.11
0
.41
Zr 5
03
.54
4
27
.44
Nb
2
00
9.7
1
28
07
.14
Sn
8.0
2
10
.42
Ba
0.5
1
18
.55
La 0
.04
3
.60
Ce
0
.03
4
.39
Pr
0.0
2
0.4
7
Nd
0
.03
2
.04
Sm
0.0
4
0.3
1
Eu
- 0
.08
Gd
0
.03
0
.16
Tb
0.0
0
0.0
2
Dy
0.0
2
0.1
3
Ho
0
.00
0
.02
Er 0
.01
0
.05
Tm
- 0
.01
Yb
0.0
1
0.0
5
Lu
0.0
0
0.0
1
Hf
12
.79
10
.86
Ta 1
04
.23
9
4.58
W
0.0
4
0.7
9
Pb
0
.96
4
.41
Th
0.0
0
0.6
3
U
0.0
1
0.3
5
73
Ru
tile-ilmen
ite intergro
wth
s
13
-45
-25
6
13
-45
-25
4
13
-45
-25
7
13
-45
-25
3
13
-45
-25
5
13
-45
-26
7
13
-45
-26
5
13
-45
-26
6
13
-47
-52
Majo
r elem
ents w
t%
SiO2
0
.01
0
.01
0
.00
0
.01
0
.02
0
.02
0
.01
0
.00
0
.04
TiO2
5
3.4
3
54
.79
53
.79
5
4.23
5
4.05
5
3.90
5
3.5
2
52
.72
50
.68
Nb
2 O5
0
.08
0
.14
0
.10
0
.13
0
.10
0
.09
0
.12
0
.08
0
.08
Al2 O
3
0.6
1
0.4
0
0.5
4
0.2
4
0.4
0
0.5
6
0.3
6
0.5
3
1.1
9
FeO
t 2
6.4
5
28
.34
27
.73
2
8.63
2
7.74
2
6.62
2
9.9
8
28
.00
25
.72
Mn
O
0.2
5
0.2
7
0.2
4
0.2
7
0.2
9
0.2
4
0.2
5
0.2
0
0.1
6
MgO
1
4.6
8
14
.34
13
.94
1
4.20
1
4.13
1
4.88
1
2.7
8
13
.41
12
.33
CaO
0
.02
0
.05
0
.03
0
.02
0
.05
0
.02
0
.07
0
.03
0
.01
Cr
2 O3
3
.61
1
.28
3
.13
1
.26
2
.76
3
.07
2
.17
4
.58
9
.13
TOTA
L 9
9.8
5
10
0.22
1
00
.14
9
9.64
1
00
.19
10
0.08
9
9.8
9
10
0.31
1
00
.05
Fe2 O
3
7.1
7
6.0
0
6.5
0
6.5
6
6.5
0
6.9
5
6.4
9
7.5
7
7.1
9
FeO
2
0.0
0
22
.95
21
.88
2
2.72
2
1.88
2
0.36
2
4.1
3
21
.19
19
.25
Trace elemen
ts pp
m
Li 1
.99
2
.65
4
.92
2
.07
5
.63
2
.39
2
.81
-
Na
34
4.7
9
22
4.21
3
36
.82
2
73
.51
41
9.34
3
50
.29
98
0.8
3
2
07
.57
Mg
98
38
1.6
9
80
84
1.7
6
13
96
49
.07
8
74
92
.23
1
09
25
5.2
5
89
03
4.0
9
82
77
6.0
3
5
40
12
.27
K
20
.17
1
4.69
1
61
.47
1
9.62
4
0.59
1
1.64
1
1.6
6
1
27
.13
Ca
13
2.6
9
20
1.77
4
50
.17
8
3.13
3
52
.24
91
.36
32
5.6
7
2
63
.80
Sc 1
6.9
9
17
.00
29
.10
1
7.36
2
1.96
1
5.04
2
6.9
0
1
6.83
Ti 3
61
47
0.2
7
32
35
09
.75
5
05
01
8.8
6
34
32
36
.79
4
05
70
9.6
9
33
30
72
.29
3
33
31
6.5
7
2
28
98
4.5
7
V
10
68
.67
9
59
.87
16
12
.41
1
02
2.9
5
12
51
.49
1
09
1.7
0
11
50
.03
83
3.82
Cr
24
69
5.1
9
87
56
.19
2
14
11
.62
8
61
9.3
7
18
88
0.5
3
21
00
1.1
7
14
84
4.4
8
2
86
62
.84
Mn
1
35
9.3
7
21
17
.51
2
17
6.1
2
22
35
.68
2
28
4.7
0
20
03
.33
2
04
4.3
5
9
28
.63
Fe 1
70
20
8.1
4
15
24
09
.45
2
31
76
0.4
7
17
81
75
.19
1
86
06
6.0
2
14
89
49
.10
1
98
61
9.8
2
7
60
16
.02
Co
1
86
.58
1
57
.65
27
9.9
9
16
0.44
2
08
.18
16
3.51
2
05
.62
10
7.55
Ni
20
15
.24
1
32
3.9
2
24
99
.54
9
24
.78
15
75
.74
1
69
5.9
7
14
73
.43
10
17
.06
Cu
3
2.4
3
29
.41
42
.40
2
7.04
3
6.71
3
1.61
3
1.8
5
2
0.19
Zn
10
9.9
0
11
0.86
1
94
.46
1
06
.60
13
4.33
1
05
.80
16
8.2
1
5
5.45
74
G
a 1
0.5
8
8.9
2
14
.50
9
.14
1
0.45
1
1.64
1
3.5
0
6.9
5
Ge
1
.67
1
.05
-
1.2
7
1.7
9
1.4
8
1.6
8
2.1
1
Sr 0
.34
0
.31
5
.01
0
.14
0
.46
0
.23
1
.59
3
.01
Y 0
.06
0
.11
0
.12
0
.07
0
.14
0
.07
0
.20
0
.31
Zr 3
58
.59
4
56
.22
68
4.5
3
48
6.32
4
89
.07
38
6.86
8
45
.94
3
56
.05
Nb
5
34
.22
1
01
0.5
0
11
32
.86
9
45
.41
68
4.30
5
12
.25
13
16
.63
4
68
.42
Sn
7.3
7
8.2
3
12
.32
7
.85
8
.61
8
.01
1
0.1
1
4.6
4
Ba
0.4
0
- 1
8.3
4
0.4
1
0.6
0
- 3
.90
3
.85
La 0
.03
-
0.7
3
0.0
2
0.0
3
- 0
.48
0
.82
Ce
0
.04
0
.07
0
.67
-
0.1
6
0.0
2
1.3
5
1.6
1
Pr
- 0
.01
0
.10
-
0.0
6
- 0
.08
0
.12
Nd
0
.05
0
.10
0
.60
-
0.1
0
- 0
.11
0
.45
Sm
- -
- -
- -
- -
Eu
0.0
2
0.0
2
0.0
9
- 0
.07
-
0.0
7
0.0
4
Gd
-
- 0
.16
-
- -
0.1
8
0.1
0
Tb
- -
- -
0.0
0
- 0
.02
0
.01
Dy
0.0
2
0.0
3
- 0
.02
0
.06
0
.02
0
.08
0
.09
Ho
0
.00
0
.01
-
- 0
.01
0
.00
0
.02
0
.01
Er -
- 0
.05
-
- -
0.0
4
0.0
3
Tm
- -
- -
0.0
1
- -
0.0
1
Yb
0.0
2
0.0
3
- 0
.02
0
.03
0
.02
0
.03
0
.05
Lu
- -
0.0
3
- -
0.0
0
0.0
2
0.0
1
Hf
13
.73
1
3.53
2
7.2
2
16
.71
16
.47
14
.27
31
.96
1
2.09
Ta 4
2.9
3
69
.25
16
0.6
8
62
.75
68
.03
42
.70
20
0.5
1
44
.45
W
0.1
4
0.0
6
0.2
2
0.0
6
0.1
1
0.0
7
0.2
3
0.1
0
Pb
0
.09
0
.53
-
0.1
1
0.1
0
0.1
4
0.9
4
2.2
3
Th
0.0
1
0.0
0
- 0
.00
0
.01
0
.00
0
.04
0
.04
U
0.0
4
0.0
1
0.1
2
0.0
1
0.0
2
0.0
1
0.1
8
0.3
0
75
13
-47
-53
1
3-4
7-5
0
13
-47
-48
1
3-4
7-5
1
13
-47
-49
1
3-4
7-4
5
Majo
r elemen
ts wt%
SiO
2
0.0
5
0.0
6
0.0
3
0.0
2
0.0
3
0.0
2
TiO2
5
2.6
1
53
.06
51
.45
53
.38
50
.06
52
.10
Nb
2 O5
0
.07
0
.15
0
.11
0
.09
0
.06
0
.07
Al2 O
3
0.8
5
0.1
9
0.4
7
0.5
7
0.6
4
0.2
0
FeO
t 2
8.1
8
29
.51
28
.90
29
.63
30
.00
27
.00
Mn
O
0.2
0
0.1
6
0.2
2
0.2
0
0.1
0
0.1
6
MgO
1
4.0
8
12
.72
12
.73
13
.13
12
.21
14
.04
CaO
0
.03
0
.00
0
.07
0
.05
0
.03
0
.02
Cr
2 O3
4
.20
4
.60
5
.98
2
.94
6
.70
6
.36
TOTA
L 1
01
.16
1
01
.19
10
0.88
1
00
.74
10
0.95
1
00
.89
Fe2 O
3
8.9
3
7.3
0
9.2
2
7.3
0
11
.05
9.1
8
FeO
2
0.1
4
22
.94
20
.60
23
.07
20
.05
18
.74
Trace elemen
ts pp
m
Li 3
.49
4.0
3
-
6.8
0
Na
33
7.1
1
1
19
.67
42
1.49
41
2.85
Mg
78
35
9.0
7
1
41
02
3.3
9
11
18
02
.00
81
82
5.4
2
K
14
0.8
7
1
07
.09
59
.43
2
18
.06
Ca
36
0.0
8
2
71
.37
60
5.69
11
80
.92
Sc 2
2.8
6
2
6.21
2
8.74
22
.00
Ti 3
14
90
0.8
0
4
95
43
8.2
8
51
49
23
.61
33
71
28
.44
V
10
89
.12
15
51
.69
1
19
7.9
2
1
39
9.1
2
Cr
36
58
4.4
5
4
09
14
.66
3
13
44
.42
43
50
7.3
2
Mn
1
28
1.9
6
2
23
6.0
5
21
61
.62
13
69
.66
Fe 1
07
99
9.8
1
1
31
62
5.9
2
15
94
03
.05
10
92
29
.01
Co
1
60
.31
23
6.88
2
62
.15
1
22
.97
Ni
16
31
.72
22
53
.18
2
12
7.7
9
1
40
8.5
1
Cu
2
6.7
7
3
2.94
5
3.24
32
.95
Zn
87
.51
14
4.78
1
52
.13
4
9.87
Ga
13
.62
15
.65
13
.59
8
.18
Ge
4
.27
3.0
3
5.4
4
2
.76
76
Sr
0.6
0
1.2
6
4.4
7
41
.17
Y 0
.22
0
.34
0
.47
0
.84
Zr 4
46
.48
5
43
.18
53
6.31
6
63
.87
Nb
6
28
.41
1
35
5.0
5
90
9.31
7
80
.21
Sn
6.9
8
14
.82
6.9
6
6.9
9
Ba
3.3
0
3.5
3
9.8
3
29
.33
La 0
.12
0
.74
1
.62
7
.80
Ce
0
.09
1
.13
1
.02
1
2.26
Pr
0.0
4
0.0
8
0.0
7
1.1
2
Nd
-
0.4
3
0.5
1
3.7
3
Sm
0.2
6
<0.2
13
0
.28
1
.00
Eu
- <0
.04
7
0.0
7
0.2
4
Gd
-
<0.1
56
0
.21
0
.39
Tb
0.0
1
<0.0
17
1
0.0
4
0.0
8
Dy
0.0
3
0.1
0
0.1
1
0.2
1
Ho
0
.01
0
.02
0
.03
0
.03
Er 0
.03
0
.08
0
.07
0
.08
Tm
- <0
.01
10
0
.01
0
.01
Yb
0.0
2
0.0
8
0.0
6
0.1
0
Lu
0.0
1
<0.0
12
3
- 0
.01
Hf
14
.81
2
1.10
2
2.80
2
5.05
Ta 5
8.8
0
11
9.79
1
52
.00
90
.05
W
0.1
1
0.4
5
0.1
3
0.2
8
Pb
1
.95
2
.32
3
.28
3
.89
Th
0.0
1
0.4
1
0.0
3
0.6
7
U
0.0
3
0.3
3
0.0
8
0.8
2
77
Orth
op
yroxen
ite ilmen
ites
13
-74
-46
1
3-7
4-5
5
13
-74
-56
1
3-6
7-5
4
13
-74
-21
1
3-7
4-4
5
13
-74
-20
1
3-4
7-1
9
13
-47
-26
Majo
r elem
ents w
t%
SiO2
0
.00
0
.01
0
.02
0
.01
0
.01
0
.02
0
.00
0
.03
0
.00
TiO2
4
9.6
4
41
.75
53
.85
49
.54
54
.58
5
5.89
5
5.25
5
4.81
5
4.50
Nb
2 O5
0
.56
1
.39
0
.08
0
.08
0
.08
0
.04
0
.08
0
.09
0
.10
Al2 O
3
0.1
2
0.0
6
0.3
8
0.1
0
0.1
9
0.0
9
0.0
5
0.0
6
0.3
1
FeO
t 3
6.1
2
49
.63
29
.15
32
.37
31
.99
3
1.16
3
2.31
3
2.05
2
8.56
Mn
O
0.2
9
0.2
9
0.2
6
0.1
9
0.2
7
0.3
0
0.3
0
0.2
8
0.2
7
MgO
1
0.8
3
6.0
6
13
.47
11
.42
12
.61
1
2.67
1
2.14
1
2.39
1
3.88
CaO
0
.04
0
.01
0
.03
0
.03
0
.03
0
.02
0
.02
0
.02
0
.03
Cr
2 O3
2
.45
0
.82
2
.14
6
.32
0
.56
0
.16
0
.54
0
.63
2
.57
TOTA
L 1
00
.05
1
00
.01
99
.38
10
0.05
1
00
.32
1
00
.35
10
0.69
1
00
.37
10
0.23
Fe2 O
3
11
.68
2
2.06
5
.94
1
1.28
5
.85
3
.81
4
.76
5
.34
5
.71
FeO
2
4.4
4
27
.57
23
.21
21
.08
26
.14
2
7.34
2
7.55
2
6.72
2
2.85
Trace elemen
ts pp
m
Li 2
.29
4
.13
2
.73
Na
35
8.6
2
87
3.42
7
73
.27
Mg
73
48
9.2
3
31
55
2.6
7
78
73
9.5
0
K
27
.41
1
8.49
4
4.82
Ca
24
0.0
2
47
.14
16
1.50
Sc 3
2.2
3
35
.12
19
.72
Ti 3
29
62
9.1
6
23
45
54
.71
3
08
52
3.0
5
V
11
33
.60
2
58
1.1
8
11
33
.79
Cr
16
75
9.8
9
56
09
.43
1
47
07
.66
Mn
2
72
2.8
6
26
27
.21
2
21
6.9
7
Fe 2
44
64
2.3
2
25
25
77
.73
1
55
47
7.5
4
Co
1
59
.71
1
12
.89
17
3.65
Ni
72
1.9
9
18
8.12
1
26
4.7
8
Cu
2
2.2
8
15
.58
32
.09
Zn
12
2.9
8
12
3.98
1
37
.76
78
G
a 5
.65
1
.68
1
3.13
Ge
1
.20
2
.20
2
.01
Sr 0
.27
0
.20
2
.56
Y 0
.48
0
.05
0
.17
Zr 5
71
.14
5
39
.32
50
2.84
Nb
5
87
7.4
8
10
98
7.4
7
61
6.39
Sn
13
.33
2
9.44
9
.81
Ba
- 0
.33
0
.99
La -
0.0
3
0.3
9
Ce
0
.06
0
.02
0
.44
Pr
0.0
1
- 0
.11
Nd
0
.06
0
.04
0
.53
Sm
0.0
8
- 0
.15
Eu
- 0
.04
0
.03
Gd
-
0.0
9
-
Tb
0.0
1
0.0
1
0.0
3
Dy
0.1
1
0.0
8
0.0
5
Ho
0
.02
-
-
Er 0
.07
-
0.0
3
Tm
0.0
1
0.0
1
0.0
2
Yb
0.0
8
0.0
4
0.0
8
Lu
0.0
1
0.0
2
-
Hf
14
.01
1
0.82
1
7.06
Ta 6
11
.08
4
68
.20
79
.73
W
0.1
1
0.5
0
0.1
1
Pb
0
.19
-
-
Th
0.0
2
0.0
0
0.0
8
U
0.1
0
0.1
4
0.0
3
79
1
3-7
4-5
8
13
-74
-57
1
3-7
4-6
1
13
-74
-59
1
3-4
7-2
3
13
-47
-53
1
3-4
7-5
4
13
-47
-58
1
3-4
7-4
1
Majo
r elemen
ts wt%
SiO2
0
.02
0
.01
0
.00
0
.02
0
.03
0
.01
0
.02
0
.02
0
.02
TiO2
5
4.15
5
3.6
4
52
.59
50
.97
54
.32
53
.27
53
.21
51
.39
54
.06
Nb
2 O5
0
.03
0
.08
0
.13
0
.47
0
.17
0
.06
0
.06
0
.02
0
.11
Al2 O
3
0.0
9
0.2
9
0.3
7
0.0
8
0.2
7
0.0
8
0.1
3
0.0
9
0.2
5
FeO
t 3
3.17
3
4.9
6
35
.75
34
.93
31
.38
32
.89
32
.87
32
.87
32
.81
Mn
O
0.2
9
0.2
9
0.3
0
0.2
5
0.2
6
0.2
8
0.2
7
0.2
4
0.2
8
MgO
1
1.48
1
0.8
6
10
.85
11
.24
12
.62
11
.78
11
.91
11
.45
12
.29
CaO
0
.02
0
.01
0
.02
0
.03
0
.05
0
.02
0
.03
0
.02
0
.05
Cr
2 O3
1
.16
0
.47
0
.38
2
.47
1
.45
1
.33
1
.24
3
.14
0
.52
TOTA
L 1
00
.41
10
0.6
0
10
0.39
1
00
.45
10
0.53
9
9.71
9
9.74
9
9.23
1
00
.38
Fe2 O
3
5.7
3
6.5
2
8.1
5
10
.04
5.8
2
6.8
4
7.0
5
8.7
6
6.5
4
FeO
2
7.43
2
8.4
4
27
.60
24
.90
25
.56
26
.05
25
.82
24
.10
26
.27
Trace elemen
ts pp
m
Li
5
.68
4
.61
6.3
3
Na
1
80
.11
17
2.07
26
8.36
Mg
7
84
60
.72
7
63
07
.88
97
13
5.9
0
K
2
1.02
3
9.50
36
.99
Ca
1
39
.42
17
1.69
29
4.54
Sc
24
.46
22
.10
3
0.85
Ti
33
25
35
.96
3
33
97
9.7
2
3
96
61
1.1
1
V
1
05
8.4
7
96
6.22
11
95
.80
Cr
9
07
7.5
8
85
01
.03
35
56
.05
Mn
12
21
.02
1
11
0.0
8
1
44
6.9
4
Fe
18
59
15
.04
1
85
56
9.7
6
2
16
00
5.9
1
Co
18
9.65
1
82
.75
2
35
.74
Ni
1
21
9.2
8
11
84
.74
87
2.13
Cu
23
.44
24
.27
2
1.77
Zn
1
36
.55
12
9.14
16
2.38
Ga
8
.45
7
.62
10
.05
Ge
1.6
7
2.0
0
2
.13
80
Sr
0.2
5
0.1
2
0.2
0
Y 0
.28
0
.33
0
.21
Zr 3
39
.32
31
9.94
8
02
.49
Nb
5
32
.07
40
0.66
8
72
.42
Sn
5.1
8
4.4
1
7.8
7
Ba
- -
-
La 0
.08
-
0.0
8
Ce
0
.25
0
.17
0
.29
Pr
0.0
2
- 0
.09
Nd
0
.11
-
0.0
8
Sm
0.1
4
0.2
0
0.6
7
Eu
0.0
6
0.0
9
-
Gd
0
.12
0
.20
-
Tb
0.0
1
0.0
5
0.0
2
Dy
0.2
7
- 0
.18
Ho
0
.01
0
.02
0
.02
Er 0
.04
0
.04
0
.12
Tm
0.0
2
0.0
1
-
Yb
- 0
.09
0
.16
Lu
0.0
1
0.0
2
-
Hf
13
.60
15
.30
27
.95
Ta 9
0.48
5
8.96
1
35
.91
W
0.0
5
0.0
9
0.2
7
Pb
-
- -
Th
0.0
3
0.0
3
0.0
4
U
0.1
1
0.1
4
0.2
6
81
13
-47
-55
13
-47
-58
1
3-4
7-20
13
-47-25
1
3-4
7-28
13
-47-27
1
3-4
7-24
13
-47
-21
Majo
r elem
ents w
t%
SiO2
0.0
1
0.0
2
0.0
1
0.0
1
0.0
4
0.0
1
0.0
2
0.0
0
TiO2
49
.72
52
.91
51
.74
54
.48
54
.63
54
.60
54
.46
52
.95
Nb
2 O5
0.0
6
0.1
5
0.3
9
0.1
1
0.1
4
0.1
4
0.0
5
0.1
2
Al2 O
3 0
.08
0
.38
0
.02
0
.30
0
.37
0
.41
0
.53
0
.36
FeO
t 3
1.36
3
2.12
3
5.93
3
0.84
2
9.42
2
8.72
2
7.20
3
0.61
Mn
O
0.1
8
0.2
5
0.3
1
0.2
5
0.2
3
0.2
6
0.2
3
0.2
6
MgO
1
0.72
1
2.33
1
0.99
1
2.62
1
3.26
1
3.00
1
4.84
1
2.57
CaO
0
.01
0
.03
0
.02
0
.03
0
.03
0
.03
0
.01
0
.04
Cr
2 O3
7
.94
2
.09
1
.17
1
.76
2
.19
3
.13
3
.16
3
.34
TOTA
L 1
00.08
1
00
.29
100
.58
100
.39
100
.32
100
.30
100
.49
10
0.25
Fe2 O
3 9
.62
7
.60
9
.44
5
.34
5
.02
4
.40
6
.34
7
.15
FeO
21
.74
24
.52
26
.48
25
.50
24
.40
24
.32
20
.86
23
.47
Trace elemen
ts pp
m
Li 3
.02
1
.91
Na
40
5.22
2
42
.84
Mg
71
72
7.3
5
80
65
3.2
0
K
56
.29
3
5.83
Ca
12
3.1
0
15
9.32
Sc 2
4.7
7
20
.71
Ti 3
00
37
2.6
1
32
68
91
.05
V
14
22
.57
8
61
.84
Cr
54
31
5.7
3
14
30
0.6
4
Mn
1
36
9.4
7
15
99
.44
Fe 1
67
46
7.6
4
19
51
83
.17
Co
1
72
.59
1
80
.97
Ni
13
51
.15
1
24
7.6
6
Cu
3
1.9
5
35
.97
Zn
12
2.3
7
15
4.30
Ga
8.7
3
11
.11
Ge
1
.68
0
.75
82
Sr
0.5
7
0.2
5
Y 0
.08
0
.10
Zr 4
33
.81
4
95
.84
Nb
3
78
.69
8
20
.81
Sn
5.0
3
5.9
4
Ba
3.1
2
0.7
2
La 0
.12
0
.03
Ce
0
.11
0
.11
Pr
0.0
4
0.0
3
Nd
-
0.1
0
Sm
0.2
7
0.1
3
Eu
0.0
6
-
Gd
-
-
Tb
- 0
.02
Dy
0.1
1
0.0
4
Ho
0
.01
0
.01
Er 0
.03
0
.05
Tm
- 0
.02
Yb
0.0
5
0.0
4
Lu
0.0
2
0.0
2
Hf
15
.37
2
0.29
Ta 7
4.5
5
10
2.56
W
0.0
9
0.1
7
Pb
-
-
Th
0.0
1
-
U
- 0
.05
83
Kam
fersdam
ilmen
ite xen
ocrysts
K-1
K
-2
K-3
K
-4
K-5
K
-6
K-7
K
-8
K-9
K
-10
K
-11
K
-12
Majo
r elemen
ts wt%
TiO2
4
6.2
40
5
4.2
40
4
6.9
80
4
5.52
0
53
.980
4
1.77
0
54
.310
5
3.07
0
49
.660
4
8.49
0
54
.185
5
4.21
0
SiO2
0
.00
8
0.0
05
0
.00
2
0.0
01
0
.01
9
0.0
17
0
.00
7
0.0
09
0
.01
1
0.0
06
0
.01
0
0.0
14
Nb
2 O5
0
.52
2
0.0
85
0
.56
4
0.8
25
0
.11
8
1.2
84
0
.10
9
0.1
77
0
.41
5
0.6
02
0
.10
9
0.0
91
Al2 O
3
0.0
22
0
.30
6
0.0
19
0
.02
5
0.2
50
0
.01
4
0.2
99
0
.10
0
0.0
28
0
.01
7
0.3
23
0
.32
5
Cr
2 O3
1
.83
0
1.5
90
1
.91
5
1.9
95
1
.32
1
1.2
12
1
.55
5
1.0
45
1
.46
9
2.2
65
1
.61
5
1.6
90
FeO
*
42
.08
5
28
.66
0
41
.28
0
42
.800
2
9.36
5
47
.645
2
8.14
5
32
.230
3
8.21
5
38
.670
2
8.59
0
28
.560
Mn
O
0.4
08
0
.27
3
0.4
19
0
.38
1
0.2
96
0
.36
0
0.3
22
0
.33
6
0.3
90
0
.42
2
0.3
03
0
.27
8
MgO
7
.13
0
13
.69
0
7.5
75
6
.84
5
13
.355
5
.36
0
13
.975
1
1.90
0
8.9
60
8
.65
5
13
.915
1
3.81
0
NiO
0
.02
7
0.1
23
0
.04
8
0.0
25
0
.11
3
0.0
14
0
.11
5
0.0
85
0
.05
5
0.0
70
0
.13
6
0.1
37
CaO
0
.01
3
0.0
17
0
.00
5
0.0
05
0
.01
5
0.0
04
0
.03
2
0.0
17
0
.01
5
0.0
07
0
.02
2
0.0
30
Total
98
.28
4
98
.99
0
98
.80
7
98
.422
9
8.83
2
97
.679
9
8.87
0
98
.969
9
9.21
7
99
.205
9
9.20
7
99
.144
K-1
3
K-1
4
K-1
5
K-1
6
K-1
7
K-1
8
K-1
9
K-2
0
K-2
1
K-2
2
K-2
3
K-2
4
Majo
r elemen
ts wt%
TiO2
5
3.7
00
4
8.7
60
5
3.2
50
5
4.19
5
54
.460
5
3.86
0
54
.400
5
4.10
5
54
.040
4
8.97
0
53
.005
4
7.09
0
SiO2
0
.00
5
0.0
00
0
.00
0
0.0
30
0
.01
0
0.0
04
0
.03
5
0.0
22
0
.00
8
0.0
02
0
.01
1
0.0
00
Nb
2 O5
0
.19
1
0.5
16
0
.14
7
0.0
84
0
.12
8
0.1
44
0
.10
0
0.0
87
0
.09
4
0.5
14
0
.17
7
0.7
05
Al2 O
3
0.1
42
0
.01
7
0.1
31
0
.32
8
0.2
45
0
.18
9
0.2
90
0
.35
5
0.2
96
0
.02
0
0.1
19
0
.01
9
Cr
2 O3
1
.03
0
1.9
35
1
.06
8
1.7
60
1
.34
5
1.0
49
1
.45
9
1.8
60
1
.58
0
1.6
70
1
.10
9
3.0
30
FeO
*
31
.59
0
38
.81
5
32
.02
0
28
.125
2
9.53
0
30
.730
2
8.93
0
28
.185
2
8.68
0
38
.350
3
2.02
5
39
.595
Mn
O
0.3
49
0
.40
6
0.3
41
0
.31
2
0.2
89
0
.32
9
0.2
61
0
.28
9
0.2
77
0
.40
2
0.3
34
0
.37
7
MgO
1
2.3
40
8
.65
5
12
.07
5
13
.970
1
3.29
0
12
.690
1
3.65
0
14
.000
1
3.66
0
8.7
40
1
2.11
0
8.0
40
NiO
0
.07
3
0.0
78
0
.07
7
0.1
11
0
.08
6
0.0
92
0
.13
3
0.1
45
0
.09
5
0.0
57
0
.07
0
0.0
70
CaO
0
.01
1
0.0
03
0
.01
3
0.0
35
0
.01
4
0.0
15
0
.01
0
0.0
22
0
.01
7
0.0
27
0
.02
3
0.0
14
Total
99
.43
2
99
.18
5
99
.12
2
98
.950
9
9.39
6
99
.102
9
9.26
7
99
.070
9
8.74
6
98
.753
9
8.98
2
98
.940
84
K-2
5
K-2
6
K-2
7
K-2
8
K-29
K
-30
K-31
K
-32
K-33
K
-34
K-35
K
-36
Majo
r elemen
ts wt%
TiO2
5
4.1
45
4
3.1
65
5
4.0
15
5
4.30
0
54
.145
4
3.16
0
53
.765
4
5.67
5
54
.225
5
4.00
5
53
.990
5
1.76
0
SiO2
0
.01
1
0.0
00
0
.01
0
0.0
36
0
.02
0
0.0
10
0
.01
4
0.0
00
0
.00
5
0.0
10
0
.01
1
0.0
06
Nb
2 O5
0
.09
8
1.2
55
0
.13
2
0.0
83
0
.13
2
1.3
69
0
.11
0
0.7
41
0
.09
6
0.1
10
0
.08
3
0.1
80
Al2 O
3
0.2
57
0
.01
5
0.2
38
0
.38
4
0.2
32
0
.02
0
0.5
26
0
.00
5
0.2
66
0
.20
9
0.3
68
0
.14
6
Cr
2 O3
1
.29
3
1.6
50
1
.30
7
1.9
10
1
.27
7
2.0
15
2
.70
5
2.4
20
1
.34
9
1.2
54
1
.95
0
0.9
95
FeO
*
29
.48
5
45
.73
0
29
.36
5
27
.735
2
9.67
5
42
.975
2
7.23
5
41
.625
2
9.27
5
29
.850
2
7.86
0
29
.900
Mn
O
0.2
97
0
.38
5
0.2
86
0
.28
5
0.3
02
0
.39
2
0.2
52
0
.37
5
0.3
16
0
.33
8
0.2
81
0
.30
9
MgO
1
3.3
95
5
.87
0
13
.32
0
14
.065
1
3.19
0
6.4
90
1
4.12
5
7.3
40
1
3.58
5
13
.165
1
4.12
0
12
.340
NiO
0
.11
7
0.0
30
0
.11
2
0.1
53
0
.09
2
0.0
40
0
.21
2
0.0
46
0
.10
5
0.0
73
0
.15
8
0.0
65
CaO
0
.01
6
0.0
12
0
.01
8
0.0
17
0
.02
1
0.0
02
0
.04
6
0.0
12
0
.01
9
0.0
18
0
.00
9
0.0
13
Total
99
.11
4
98
.11
2
98
.80
3
98
.968
9
9.08
6
96
.472
9
8.99
0
98
.239
9
9.24
2
99
.032
9
8.83
0
95
.713
K
-37
K
-38
K
-39
K
-40
K
-41
K
-42
K
-43
K
-44
K
-45
K
-46
K
-47
K
-48
Majo
r elemen
ts wt%
TiO2
4
5.4
50
5
3.7
75
5
4.1
20
5
2.41
0
46
.74
5
53
.925
5
3.91
5
40
.945
4
5.87
5
42
.920
5
4.27
5
54
.145
SiO2
0
.00
0
0.0
02
0
.03
6
0.0
20
0
.00
0
0.0
26
0
.00
0
0.0
06
0
.00
6
0.0
09
0
.01
5
0.0
11
Nb
2 O5
0
.84
8
0.0
97
0
.10
2
0.2
37
0
.92
3
0.0
98
0
.14
5
1.4
32
0
.60
5
1.4
90
0
.12
1
0.1
07
Al2 O
3
0.0
19
0
.33
1
0.3
63
0
.07
0
0.0
25
0
.31
3
0.2
06
0
.00
5
0.0
06
0
.01
3
0.2
79
0
.26
2
Cr
2 O3
2
.79
0
1.6
80
1
.87
0
1.1
53
2
.74
5
1.6
65
1
.19
2
0.8
60
2
.01
5
1.7
70
1
.18
0
1.5
00
FeO
*
35
.47
5
28
.12
5
28
.14
0
33
.080
3
9.4
00
2
9.02
0
29
.910
4
9.28
5
42
.305
4
5.85
0
29
.670
2
8.98
5
Mn
O
0.3
41
0
.29
4
0.2
71
0
.37
0
0.4
11
0
.29
6
0.3
13
0
.33
8
0.4
04
0
.37
7
0.2
59
0
.30
4
MgO
8
.69
5
13
.89
0
13
.99
0
11
.265
8
.01
5
13
.560
1
3.13
5
4.9
65
7
.20
0
5.7
65
1
3.31
0
13
.395
NiO
0
.08
5
0.1
36
0
.14
3
0.0
97
0
.06
0
0.1
30
0
.09
4
0.0
30
0
.03
8
0.0
37
0
.15
0
0.1
16
CaO
0
.01
5
0.0
13
0
.01
9
0.0
11
0
.01
2
0.0
12
0
.01
8
0.0
03
0
.00
9
0.0
03
0
.02
5
0.0
16
Total
93
.71
8
98
.34
3
99
.05
4
98
.712
9
8.3
36
9
9.04
5
98
.927
9
7.86
8
98
.463
9
8.23
4
99
.285
9
8.84
0
85
FeO
*
Mn
O
MgO
NiO
CaO
Total
34
.79
0
0.4
25
10
.05
0
0.1
01
0.0
06
98
.32
2
29
.010
0.2
29
13
.320
0.2
19
0.0
33
98
.658
26
.42
0
0.2
36
14
.05
0
0.2
25
0.0
30
97
.88
1
41
.150
0.4
05
7.2
90
0.0
56
0.0
19
98
.197
43
.610
0.3
37
6.3
90
0.0
00
0.0
03
97
.377
41
.410
0.3
92
7.2
10
0.0
30
0.0
04
98
.079
38
.46
0
0.4
34
8.5
40
0.0
36
0.0
01
98
.70
6
48
.800
0.3
86
4.8
90
0.0
26
0.0
09
97
.238
39
.090
0.1
84
10
.400
0.1
43
0.0
14
97
.822
32
.900
0.2
26
10
.940
0.1
47
0.0
48
98
.228
29
.370
0.2
63
13
.180
0.1
59
0.0
19
98
.842
31
.820
0.3
09
12
.300
0.0
98
0.0
12
99
.114
K-4
9
K-5
0
K-5
1
K-5
2
K-5
3
Majo
r elemen
ts wt%
TiO2
5
1.2
00
4
7.1
20
5
4.4
60
5
4.07
5
53
.90
5
SiO2
0
.01
5
0.0
00
0
.01
3
0.0
04
0
.03
0
Nb
2 O5
0
.10
2
0.8
74
0
.12
0
0.1
02
0
.08
9
Al2 O
3
0.3
33
0
.02
2
0.3
02
0
.28
7
0.3
07
Cr
2 O3
1
.60
0
2.7
70
1
.30
7
1.4
41
1
.58
0
FeO
*
26
.24
5
39
.29
5
28
.51
0
28
.925
2
8.4
50
Mn
O
0.2
73
0
.42
4
0.2
79
0
.29
8
0.2
95
MgO
1
3.6
50
8
.13
0
13
.70
0
13
.590
1
3.8
80
NiO
0
.12
2
0.0
69
0
.11
0
0.1
33
0
.12
8
CaO
0
.01
3
0.0
11
0
.02
1
0.0
18
0
.01
6
Total
93
.55
3
98
.71
5
98
.82
2
98
.873
9
8.6
81
Otto
’s Ko
pje ilm
enite xe
no
crysts
OK
-1 O
K-2
O
K-3
OK
-4
OK
-5 O
K-6
OK
-7 O
K-8
OK
-9 O
K-10
OK
-11 O
K-12
Majo
r elemen
ts wt%
TiO2
4
9.9
70
5
3.3
70
5
2.6
00
4
6.62
0
43
.470
4
6.04
0
49
.460
4
0.98
0
44
.660
5
0.09
0
53
.470
5
3.15
0
SiO2
0
.02
2
0.0
54
0
.00
1
0.0
13
0
.01
3
0.0
35
0
.01
0
0.0
18
0
.01
2
0.0
37
0
.02
0
0.0
30
Nb
2 O5
0
.54
4
0.0
98
0
.06
3
0.7
83
1
.30
4
0.6
99
0
.42
3
1.4
50
1
.31
7
0.6
11
0
.10
0
0.1
98
Al2 O
3
0.0
24
0
.51
5
0.6
06
0
.01
1
0.0
21
0
.02
0
0.0
23
0
.00
5
0.2
72
0
.34
0
0.3
63
0
.12
8
Cr
2 O3
2
.39
0
1.8
10
3
.65
0
1.8
50
2
.23
0
2.2
40
1
.32
0
0.6
74
1
.73
0
2.8
90
1
.90
0
1.0
69
86
FeO
*
Mn
O
MgO
NiO
CaO
Total
30
.04
0
0.2
54
12
.24
0
0.1
55
0.0
30
98
.21
4
28
.310
0.2
71
13
.900
0.1
34
0.0
09
98
.543
31
.15
0
0.3
13
12
.20
0
0.0
71
0.0
18
97
.83
6
47
.110
0.3
61
5.4
90
0.0
22
0.0
07
97
.723
42
.040
0.6
09
5.7
80
0.0
47
0.0
16
98
.670
37
.870
0.3
79
8.7
60
0.0
70
0.0
10
98
.311
30
.11
0
0.2
41
12
.57
0
0.1
92
0.0
25
98
.13
0
43
.240
0.3
81
6.6
20
0.0
32
0.0
12
97
.746
45
.350
0.4
09
5.7
90
0.0
39
0.0
05
97
.783
36
.680
0.3
65
9.8
40
0.0
45
0.0
59
98
.331
27
.620
0.2
40
13
.870
0.1
54
0.0
43
98
.160
38
.270
0.3
93
8.2
30
0.0
33
0.0
05
97
.160
OK
-13
OK
-14
OK
-15
O
K-1
6
OK
-17
O
K-1
8
OK
-19
O
K-2
0
OK
-21
OK
-22
OK
-23
OK
-24
Majo
r elemen
ts wt%
TiO2
4
7.8
50
4
7.0
10
4
3.1
80
4
9.06
0
52
.740
4
5.54
0
49
.590
4
6.67
0
46
.870
4
7.92
0
46
.410
4
0.91
0
SiO2
0
.00
5
0.0
02
0
.00
4
0.0
12
0
.02
8
0.0
12
0
.01
2
0.0
00
0
.00
8
0.0
00
0
.00
3
0.0
00
Nb
2 O5
0
.46
6
0.6
72
1
.52
0
0.4
13
0
.05
4
0.7
93
0
.54
7
0.9
04
0
.95
8
0.7
17
1
.04
0
1.4
70
Al2 O
3
0.0
28
0
.02
6
0.0
20
0
.02
6
0.0
00
0
.01
7
0.0
27
0
.02
0
0.0
20
0
.02
4
0.0
20
0
.01
8
Cr
2 O3
1
.68
0
2.5
30
1
.89
0
1.5
40
1
.30
0
2.3
10
1
.29
1
2.5
30
2
.75
0
2.4
00
2
.68
0
0.7
56
FeO
*
38
.84
0
39
.52
0
43
.92
0
38
.220
3
3.41
0
42
.050
3
7.30
0
39
.590
3
9.18
0
38
.520
3
9.59
0
49
.000
Mn
O
0.3
80
0
.38
6
0.3
83
0
.36
5
0.4
30
0
.42
8
0.3
14
0
.36
4
0.4
16
0
.39
8
0.4
04
0
.34
8
MgO
8
.74
0
8.0
80
6
.53
0
8.6
30
1
0.40
0
6.9
10
9
.31
0
7.9
50
8
.16
0
8.5
40
7
.93
0
4.8
80
NiO
0
.06
3
0.0
58
0
.04
5
0.0
65
0
.11
9
0.0
46
0
.06
6
0.0
62
0
.06
4
0.0
83
0
.06
5
0.0
38
CaO
0
.01
5
0.0
13
0
.02
0
0.0
08
0
.03
0
0.0
02
0
.02
0
0.0
05
0
.01
8
0.0
00
0
.00
5
0.0
13
Total
98
.06
8
98
.29
8
97
.51
1
98
.338
9
8.51
0
98
.108
9
8.47
6
98
.095
9
8.44
4
98
.602
9
8.14
6
97
.433
OK
-25
OK
-26
OK
-27
O
K-2
8
OK
-29
O
K-3
0
OK
-31
O
K-3
2
OK
-33
OK
-34
OK
-35
OK
-36
Majo
r elemen
ts wt%
TiO2
5
3.2
00
5
3.8
10
5
2.7
40
4
1.97
0
48
.130
4
8.81
0
52
.170
4
3.85
0
42
.890
4
7.33
0
53
.670
4
6.97
0
SiO2
0
.00
8
0.0
03
0
.03
5
0.0
00
0
.00
0
0.0
00
0
.01
6
0.0
00
0
.01
9
0.0
27
0
.00
5
0.0
07
Nb
2 O5
0
.13
6
0.1
08
0
.14
1
1.4
18
0
.58
0
0.6
05
0
.13
6
1.3
40
1
.49
0
0.9
66
0
.07
6
0.7
43
Al2 O
3
0.3
81
0
.32
7
0.1
47
0
.01
2
0.0
11
0
.01
7
0.4
60
0
.01
2
0.0
01
0
.16
0
0.4
21
0
.01
9
Cr
2 O3
1
.77
0
1.6
70
1
.02
1
1.3
33
1
.45
7
1.7
90
2
.21
0
2.2
60
1
.79
0
2.8
60
2
.06
0
2.4
90
87
FeO
*
Mn
O
MgO
NiO
CaO
Total
38
.59
0
0.4
18
8.5
10
0.0
71
0.0
03
98
.78
0
30
.080
0.2
88
12
.990
0.0
80
0.0
25
98
.607
46
.44
0
0.3
98
5.6
40
0.0
59
0.0
14
97
.88
4
32
.400
0.3
64
11
.750
0.0
75
0.0
11
98
.791
37
.050
0.3
69
9.0
20
0.0
75
0.0
15
98
.474
44
.670
0.3
73
6.1
70
0.0
40
0.0
00
97
.816
41
.37
0
0.4
21
7.3
00
0.0
51
0.0
19
98
.58
0
39
.840
0.3
95
7.9
70
0.0
53
0.0
02
98
.318
41
.280
0.3
87
7.6
00
0.0
31
0.0
01
98
.139
38
.650
0.3
49
8.5
30
0.0
80
0.0
09
98
.433
26
.760
0.2
50
13
.860
0.1
85
0.0
63
95
.833
33
.640
0.3
31
10
.880
0.0
74
0.0
54
98
.771
OK
-37
OK
-38
OK
-39
O
K-4
0
OK
-41
O
K-4
2
OK
-43
O
K-4
4
OK
-45
OK
-46
OK
-47
OK
-48
Majo
r elemen
ts wt%
TiO2
4
9.9
40
5
3.6
70
3
9.2
90
5
3.86
0
43
.290
4
6.29
0
45
.860
4
8.99
0
46
.750
4
5.56
0
46
.740
4
8.31
0
SiO2
0
.00
1
0.0
15
0
.02
0
0.0
00
0
.01
7
0.0
08
0
.00
0
0.0
32
0
.00
2
0.0
13
0
.00
4
0.0
05
Nb
2 O5
0
.40
4
0.1
61
1
.59
0
0.0
82
1
.33
1
0.6
54
0
.87
8
0.6
05
0
.56
5
0.7
01
0
.54
8
0.4
44
Al2 O
3
0.0
15
0
.42
3
0.0
12
0
.39
5
0.0
18
0
.01
1
0.0
18
0
.02
7
0.0
16
0
.02
1
0.0
16
0
.02
0
Cr
2 O3
1
.28
1
2.0
80
0
.29
9
1.8
20
2
.03
0
1.9
60
2
.57
0
2.0
50
1
.68
0
1.8
80
1
.70
0
1.7
90
FeO
*
38
.56
0
28
.99
0
50
.69
0
28
.320
4
4.79
0
41
.250
4
0.94
0
37
.140
4
1.73
0
42
.450
4
0.46
0
38
.950
Mn
O
0.4
37
0
.23
1
0.3
18
0
.27
1
0.3
92
0
.42
8
0.3
70
0
.33
4
0.3
90
0
.42
6
0.3
04
0
.39
4
MgO
8
.69
0
13
.17
0
4.4
80
1
3.73
0
6.3
50
7
.18
0
7.4
90
9
.51
0
7.2
20
7
.10
0
8.3
00
8
.51
0
NiO
0
.05
0
0.1
93
0
.01
9
0.1
97
0
.01
3
0.0
33
0
.05
2
0.0
70
0
.03
7
0.0
32
0
.03
5
0.0
82
CaO
0
.02
0
0.0
64
0
.01
2
0.0
54
0
.00
5
0.0
04
0
.00
2
0.0
17
0
.02
5
0.0
00
0
.01
5
0.0
22
Total
99
.39
8
98
.99
6
96
.72
9
98
.729
9
8.23
5
97
.818
9
8.17
9
98
.774
9
8.41
4
98
.183
9
8.12
3
98
.526
OK
-49
O
K-50
O
K-51
O
K-5
2
OK
-53
O
K-5
4
OK
-55
O
K-5
6
OK
-57
OK
-58
OK
-59
OK
-60
Majo
r elemen
ts wt%
TiO2
4
7.8
40
5
3.7
00
4
2.5
70
5
2.86
0
49
.240
4
3.59
0
46
.470
4
6.61
0
46
.360
4
8.83
0
52
.870
5
1.81
0
SiO2
0
.04
4
0.0
00
0
.00
0
0.0
01
0
.00
0
0.0
00
0
.00
0
0.0
26
0
.00
0
0.0
27
0
.02
7
0.0
30
Nb
2 O5
0
.80
3
0.1
53
1
.40
5
0.1
70
0
.50
1
0.9
16
0
.67
0
0.7
54
0
.66
5
0.4
35
0
.10
9
0.3
28
Al2 O
3
0.0
23
0
.19
1
0.0
17
0
.09
0
0.0
25
0
.00
7
0.0
28
0
.02
9
0.0
16
0
.02
4
0.3
72
0
.09
5
Cr
2 O3
2
.48
0
1.1
00
1
.34
2
1.0
71
2
.18
0
2.0
50
2
.25
0
2.6
40
1
.80
0
1.5
00
1
.33
8
1.5
30
88
O
K-61
O
K-6
2
OK
-63
O
K-6
4
OK
-65
O
K-6
6
OK
-67
O
K-68
O
K-69
O
K-70
M
ajor e
leme
nts
wt%
TiO2
5
4.1
00
5
2.6
20
5
0.09
0
49
.190
4
8.34
0
53
.460
5
1.11
0
53
.770
5
3.99
0
53
.170
SiO2
0
.00
7
0.0
31
0
.01
7
0.0
29
0
.01
2
0.0
09
0
.02
8
0.0
04
0
.01
2
0.0
00
Nb
2 O5
0
.10
1
0.2
09
0
.32
5
0.3
68
0
.56
5
0.1
23
0
.43
3
0.1
01
0
.11
9
0.1
64
Al2 O
3
0.3
26
0
.07
2
0.0
24
0
.02
1
0.0
14
0
.44
7
0.2
85
0
.21
2
0.2
59
0
.12
7
Cr
2 O3
1
.66
0
1.1
61
1
.33
7
1.3
43
2
.07
0
2.2
10
2
.00
0
1.4
51
1
.44
9
1.0
67
FeO
*
28
.34
0
33
.26
0
37
.580
3
8.52
0
38
.630
2
9.45
0
33
.730
3
0.38
0
29
.020
3
1.83
0
Mn
O
0.2
41
0
.35
9
0.4
03
0
.41
5
0.3
72
0
.24
2
0.2
32
0
.29
5
0.3
28
0
.34
5
MgO
1
3.8
10
1
1.4
10
9
.09
0
8.6
70
8
.51
0
12
.690
1
1.03
0
12
.830
1
3.42
0
12
.170
NiO
0
.13
0
0.0
61
0
.07
6
0.0
68
0
.08
8
0.2
06
0
.07
9
0.1
11
0
.11
4
0.0
67
CaO
0
.03
7
0.0
18
0
.00
5
0.0
22
0
.00
0
0.0
63
0
.05
7
0.0
66
0
.02
1
0.0
07
Total
98
.75
3
99
.20
0
98
.946
9
8.64
5
98
.600
9
8.89
9
98
.983
9
9.22
1
98
.732
9
8.94
6
Wesselto
n ilm
enite
xen
ocrysts
M
ajor el
W-1
emen
ts wt%
W-2
W
-3
W-4
W
-5
W-6
W
-7
W-8
W
-9
W-1
0
W-1
1
W-1
2
TiO2
5
5.1
10
5
2.9
60
5
5.63
0
54
.66
0
54
.500
5
5.49
0
49
.270
5
4.99
0
54
.920
5
4.7
20
5
4.92
0
55
.060
SiO2
0
.03
9
0.0
01
0
.02
2
0.0
00
0
.03
3
0.0
03
0
.00
0
0.0
07
0
.01
7
0.0
11
0
.04
9
0.0
14
Nb
2 O5
0
.08
8
0.1
62
0
.10
6
0.0
60
0
.08
4
0.1
41
0
.61
5
0.1
17
0
.14
0
0.0
92
0
.11
7
0.0
77
Al2 O
3
0.2
51
0
.10
8
0.2
41
0
.41
3
0.4
27
0
.28
9
0.0
18
0
.23
6
0.1
74
0
.25
1
0.2
65
0
.36
9
Cr
2 O3
1
.34
3
3.2
00
1
.36
2
2.2
20
2
.29
0
1.1
65
2
.07
0
1.2
94
1
.12
7
1.4
16
1
.45
5
1.8
10
FeO
t 2
8.7
10
2
9.2
40
2
8.65
0
26
.34
0
26
.500
2
7.99
0
37
.530
2
8.50
0
29
.870
2
8.8
90
2
8.29
0
27
.330
Mn
O
0.2
90
0
.23
9
0.2
99
0
.28
7
0.2
65
0
.34
8
0.4
46
0
.27
8
0.3
11
0
.27
4
0.2
89
0
.23
9
MgO
1
3.6
10
1
2.9
70
1
3.53
0
14
.33
0
14
.420
1
4.15
0
8.6
10
1
3.54
0
12
.960
1
3.3
90
1
3.63
0
14
.320
CaO
0
.02
3
0.0
14
0
.01
0
0.0
25
0
.03
6
0.0
53
0
.00
0
0.0
26
0
.01
9
0.0
16
0
.00
6
0.0
22
Total
99
.46
3
98
.89
3
99
.850
9
8.3
35
9
8.55
5
99
.630
9
8.55
8
98
.987
9
9.53
8
99
.06
1
99
.020
9
9.24
2
89
M
ajor el
W-1
3
emen
ts wt%
W-1
4
W-1
5
W-1
6
W-1
7
W-1
8
W-1
9
W-2
0
W-2
1
W-2
2
W-2
3
W-2
4
TiO2
4
7.6
90
5
4.2
60
5
0.30
0
54
.87
0
54
.010
5
4.4
90
5
4.13
0
54
.650
5
3.86
0
54
.88
0
52
.080
5
4.80
0
SiO2
0
.00
9
0.0
10
0
.03
2
0.0
02
0
.01
8
0.0
46
0
.02
7
0.0
16
0
.00
0
0.0
17
0
.00
7
0.0
16
Nb
2 O5
0
.80
7
0.1
66
0
.40
4
0.1
43
0
.18
3
0.1
53
0
.15
9
0.0
94
0
.17
2
0.0
97
0
.32
8
0.0
85
Al2 O
3
0.0
12
0
.14
3
0.0
11
0
.21
4
0.1
32
0
.14
1
0.1
32
0
.46
1
0.1
03
0
.26
3
0.0
34
0
.21
2
Cr
2 O3
2
.42
0
1.0
70
1
.76
0
1.2
67
1
.14
0
1.0
57
1
.08
8
2.0
90
1
.17
4
1.4
10
1
.50
0
1.2
37
FeO
t 3
9.3
50
3
0.6
90
3
6.96
0
29
.27
0
31
.190
3
0.8
90
3
0.87
0
27
.380
3
1.77
0
28
.41
0
36
.930
2
9.32
0
Mn
O
0.3
84
0
.32
1
0.4
02
0
.28
9
0.3
05
0
.34
7
0.3
20
0
.28
8
0.3
06
0
.29
2
0.4
79
0
.31
7
MgO
7
.98
0
12
.50
0
9.1
20
1
3.4
00
1
2.11
0
12
.47
0
12
.240
1
4.34
0
11
.900
1
3.7
70
7
.97
0
13
.370
CaO
0
.01
3
0.0
12
0
.00
9
0.0
26
0
.03
3
0.0
18
0
.01
3
0.0
33
0
.01
3
0.0
18
0
.00
3
0.0
13
Total
98
.66
4
99
.17
1
98
.998
9
9.4
81
9
9.12
0
99
.61
1
98
.979
9
9.35
1
99
.298
9
9.1
57
9
9.33
0
99
.370
Majo
r el
W-2
5
emen
ts wt%
W-2
6
W-2
7
W-2
8
W-2
9
W-3
0
W-3
1
W-3
2
W-3
3
W-3
4
W-3
5
W-3
6
TiO2
5
4.2
70
5
5.0
60
5
4.88
0
55
.01
0
54
.940
5
4.6
00
5
5.19
0
50
.370
5
0.20
0
47
.14
0
54
.390
5
5.04
0
SiO2
0
.01
6
0.0
00
0
.00
8
0.0
39
0
.00
8
0.0
10
0
.01
0
0.0
04
0
.00
0
0.0
06
0
.00
0
0.0
00
Nb
2 O5
0
.16
8
0.1
09
0
.13
8
0.0
81
0
.13
9
0.1
47
0
.14
6
0.3
09
0
.98
7
0.5
28
0
.09
9
0.1
04
Al2 O
3
0.0
94
0
.31
0
0.2
93
0
.45
5
0.1
81
0
.16
5
0.2
47
0
.01
6
0.2
79
0
.02
3
0.2
16
0
.20
9
Cr
2 O3
1
.10
8
0.9
99
1
.12
3
1.8
90
1
.05
3
1.0
09
1
.03
5
1.4
55
2
.64
0
1.8
60
1
.21
7
1.2
22
FeO
t 3
0.9
80
2
9.2
90
2
8.28
0
26
.89
0
30
.280
3
0.2
00
2
9.22
0
37
.640
3
2.80
0
41
.30
0
29
.730
2
8.85
0
Mn
O
0.2
88
0
.29
1
0.2
70
0
.25
6
0.3
11
0
.30
1
0.3
06
0
.38
9
0.3
59
0
.36
3
0.2
94
0
.29
7
MgO
1
2.6
00
1
3.4
50
1
4.04
0
14
.12
0
12
.870
1
2.7
90
1
3.56
0
8.6
80
1
1.62
0
7.0
10
1
3.22
0
13
.350
CaO
0
.01
9
0.0
08
0
.03
1
0.0
23
0
.02
4
0.0
31
0
.03
3
0.0
11
0
.08
7
0.0
08
0
.01
9
0.0
10
Total
99
.54
4
99
.51
6
99
.062
9
8.7
63
9
9.80
6
99
.25
3
99
.747
9
8.87
4
98
.972
9
8.2
38
9
9.18
5
99
.083
90
M
ajor el
W-3
7
emen
ts wt%
W-3
8
W-3
9
W-4
0
W-4
1
W-4
2
W-4
3
W-4
4
W-4
5
W-4
6
W-4
7
W-4
8
TiO2
5
4.2
80
5
5.22
0
54
.79
0
53
.620
5
5.01
0
54
.100
5
5.23
0
54
.900
5
4.75
0
53
.560
5
3.46
0
54
.870
SiO2
0
.00
0
0.0
09
0
.00
5
0.0
21
0
.00
0
0.0
02
0
.02
1
0.0
35
0
.02
0
0.0
00
0
.02
6
0.0
20
Nb
2 O5
0
.14
0
0.0
90
0
.07
2
0.1
92
0
.10
8
0.1
17
0
.08
0
0.0
91
0
.12
1
0.1
33
0
.19
6
0.1
16
Al2 O
3
0.1
67
0
.33
2
0.5
81
0
.12
5
0.2
48
0
.24
4
0.4
06
0
.36
9
0.2
05
0
.13
0
0.1
26
0
.23
0
Cr
2 O3
1
.05
5
1.4
70
3
.04
0
1.1
70
1
.36
0
1.8
50
1
.96
0
1.9
80
1
.14
7
1.0
44
1
.23
6
1.2
80
FeO
t 3
0.4
20
2
7.86
0
25
.75
0
31
.500
2
8.69
0
28
.990
2
7.18
0
27
.310
2
9.12
0
30
.870
3
1.14
0
28
.540
Mn
O
0.3
45
0
.33
0
0.2
36
0
.34
6
0.2
74
0
.29
5
0.2
76
0
.28
6
0.3
55
0
.35
3
0.3
25
0
.30
5
MgO
1
2.9
10
1
4.05
0
14
.81
0
12
.150
1
3.65
0
13
.490
1
4.31
0
14
.230
1
3.28
0
12
.210
1
2.09
0
13
.440
CaO
0
.02
3
0.0
15
0
.02
1
0.0
21
0
.00
6
0.0
20
0
.01
8
0.0
24
0
.02
3
0.0
10
0
.02
2
0.0
16
Total
99
.33
9
99
.376
9
9.3
05
9
9.14
5
99
.345
9
9.10
8
99
.481
9
9.22
4
99
.022
9
8.31
0
98
.621
9
8.81
8
M
ajor e
lemen
ts wt%
W-4
9
W-5
0
W-5
1
W-5
2
W-5
3
W-5
4
W-5
5
W-5
6
W-5
7
W-5
8
W-5
9
TiO2
4
6.3
70
4
9.8
50
4
3.63
0
54
.860
5
4.80
0
54
.910
5
4.8
40
5
5.16
0
48
.58
0
54
.560
5
4.83
0
SiO2
0
.00
0
0.0
07
0
.00
0
0.0
17
0
.01
4
0.0
17
0
.03
1
0.0
09
0
.01
0
0.0
03
0
.00
9
Nb
2 O5
0
.69
2
0.4
63
1
.24
2
0.1
13
0
.07
0
0.1
15
0
.10
6
0.1
21
0
.44
0
0.1
26
0
.12
4
Al2 O
3
0.0
29
0
.02
3
0.0
33
0
.30
1
0.5
01
0
.23
4
0.2
96
0
.29
2
0.0
09
0
.16
7
0.2
57
Cr
2 O3
1
.10
5
1.3
35
2
.10
0
1.5
90
2
.76
0
1.2
67
1
.66
0
1.1
72
1
.84
0
1.0
08
1
.36
6
FeO
t 4
3.2
70
3
8.0
90
4
4.00
0
28
.510
2
5.92
0
28
.850
2
8.3
10
2
6.91
0
39
.39
0
30
.370
2
8.25
0
Mn
O
0.3
80
0
.44
3
0.3
57
0
.29
2
0.2
73
0
.30
9
0.2
54
0
.32
3
0.4
01
0
.32
5
0.2
59
MgO
6
.49
0
8.3
00
6
.39
0
13
.710
1
4.72
0
13
.500
1
3.8
70
1
4.45
0
7.8
70
1
2.71
0
13
.980
CaO
0
.01
2
0.0
00
0
.00
4
0.0
18
0
.03
9
0.0
24
0
.01
6
0.0
38
0
.00
8
0.0
35
0
.01
9
Total
98
.34
8
98
.51
0
97
.756
9
9.41
0
99
.098
9
9.22
6
99
.38
4
98
.474
9
8.5
49
9
9.30
5
99
.094
91
Bu
ltfon
tein ilm
enite xe
no
crysts
Bu
l-1
Bu
l-2
Bu
l-3
Bu
l-4
Bu
l-5
Bu
l-6
Bu
l-7
Bu
l-8
Bu
l-9
Bu
l-10
Bu
l-11
Bu
l-12
Majo
r elemen
ts wt%
TiO2
5
2.5
95
4
2.82
5
54
.40
5
47
.22
5
53
.400
5
2.31
5
53
.970
5
4.25
0
52
.460
5
0.29
5
54
.050
5
3.39
0
SiO2
0
.00
9
0.0
00
0
.01
9
0.0
20
0
.01
3
0.0
10
0
.00
1
0.0
04
0
.00
7
0.0
14
0
.00
8
0.0
00
Nb
2 O5
0
.17
2
1.5
75
0
.06
0
0.9
06
0
.15
3
0.3
18
0
.15
6
0.1
01
0
.18
8
0.3
16
0
.10
3
0.1
65
Al2 O
3
0.0
17
0
.00
7
0.4
10
0
.02
6
0.1
42
0
.03
3
0.3
43
0
.24
9
0.0
27
0
.33
5
0.2
12
0
.14
7
Cr
2 O3
0
.82
3
0.9
02
2
.17
5
2.6
10
1
.08
2
0.8
77
1
.77
0
1.3
52
0
.39
8
0.6
46
1
.22
9
1.0
58
FeO
t 3
5.1
20
4
7.05
5
27
.55
0
39
.40
0
31
.605
3
6.55
0
30
.670
2
9.70
0
37
.560
3
7.12
5
30
.325
3
1.62
5
Mn
O
0.4
27
0
.39
2
0.2
74
0
.39
3
0.3
17
0
.38
9
0.2
36
0
.30
4
0.4
74
0
.32
5
0.3
06
0
.34
0
MgO
1
0.1
90
5
.51
0
14
.39
0
8.2
55
1
2.33
0
9.5
95
1
2.40
0
13
.410
8
.56
5
9.9
75
1
3.12
5
12
.425
NiO
0
.13
3
0.0
21
0
.15
0
0.0
70
0
.09
3
0.0
99
0
.14
6
0.0
97
0
.09
1
0.1
11
0
.07
0
0.0
68
CaO
0
.00
7
0.0
03
0
.01
1
0.0
11
0
.07
6
0.0
06
0
.02
4
0.0
18
0
.01
5
0.0
10
0
.02
6
0.0
14
Total
99
.49
4
98
.289
9
9.4
44
9
8.9
15
9
9.21
0
10
0.1
91
9
9.71
6
99
.485
9
9.78
4
99
.153
9
9.45
5
99
.232
Bu
l-13
B
ul-1
4
Bu
l-15
B
ul-1
6
Bu
l-17
B
ul-1
8
Bu
l-19
B
ul-2
0
Bu
l-21
B
ul-2
2
Bu
l-23
B
ul-2
4
Majo
r elemen
ts wt%
TiO2
5
3.3
15
5
4.34
5
54
.075
5
3.6
85
5
3.57
5
54
.020
4
8.75
5
52
.520
4
5.83
0
52
.550
4
5.28
0
47
.950
SiO2
0
.00
7
0.0
21
0
.03
0
0.0
00
0
.00
2
0.0
08
0
.00
0
0.0
16
0
.01
0
0.0
10
0
.01
1
0.0
12
Nb
2 O5
0
.17
3
0.1
18
0
.08
9
0.1
53
0
.15
1
0.0
96
0
.46
6
0.2
29
0
.68
6
0.0
96
0
.58
3
0.7
75
Al2 O
3
0.1
28
0
.28
6
0.4
16
0
.16
0
0.1
24
0
.33
9
0.0
26
0
.08
0
0.0
11
0
.03
3
0.0
20
0
.01
9
Cr
2 O3
1
.06
7
1.4
35
2
.23
0
1.0
39
1
.08
8
1.8
65
2
.36
5
1.2
72
1
.90
0
4.0
00
1
.78
5
2.6
25
FeO
t 3
1.9
85
2
8.94
0
27
.565
3
1.1
20
3
1.65
0
28
.715
3
8.65
0
32
.885
4
2.80
5
30
.070
4
4.02
5
38
.865
Mn
O
0.3
33
0
.30
3
0.2
78
0
.35
7
0.3
34
0
.28
9
0.4
46
0
.33
5
0.4
11
0
.31
6
0.3
94
0
.39
6
MgO
1
2.0
00
1
3.88
0
14
.220
1
2.5
65
1
2.27
5
13
.745
8
.69
5
11
.620
6
.99
5
12
.670
6
.60
5
8.5
45
NiO
0
.08
3
0.1
25
0
.17
2
0.0
85
0
.06
4
0.1
24
0
.11
1
0.0
63
0
.04
4
0.2
42
0
.04
1
0.0
71
CaO
0
.01
0
0.0
31
0
.01
3
0.0
10
0
.01
7
0.0
18
0
.00
7
0.0
11
0
.00
0
0.0
15
0
.00
6
0.0
03
Total
99
.10
1
99
.484
9
9.08
7
99
.17
4
99
.279
9
9.21
9
99
.521
9
9.03
1
98
.693
1
00
.00
1
98
.749
9
9.26
2
92
Bu
l-25
Bu
l-26
B
ul-2
7
Bu
l-28
B
ul-2
9
Bu
l-30
B
ul-3
1
Bu
l-32
B
ul-3
3
Bu
l-34
B
ul-3
5
Bu
l-36
Majo
r elemen
ts wt%
TiO2
5
0.0
20
5
4.22
5
53
.70
0
47
.36
5
42
.645
4
2.42
0
54
.285
4
6.91
5
46
.215
4
8.35
0
47
.160
5
0.91
0
SiO2
0
.00
0
0.0
16
0
.00
2
0.0
03
0
.00
0
0.0
17
0
.01
0
0.0
00
0
.00
0
0.0
00
0
.00
0
0.0
19
Nb
2 O5
0
.58
1
0.0
72
0
.15
1
0.8
48
1
.44
1
1.4
75
0
.12
2
0.5
59
0
.59
7
0.7
48
0
.80
3
0.0
71
Al2 O
3
0.0
22
0
.37
7
0.1
36
0
.02
0
0.0
12
0
.01
5
0.2
30
0
.01
8
0.0
18
0
.02
3
0.0
26
0
.70
5
Cr
2 O3
2
.35
5
1.9
50
1
.08
2
2.7
30
1
.43
3
1.4
08
1
.28
9
1.9
10
1
.91
0
2.3
35
2
.82
5
4.1
60
FeO
t 3
6.6
95
2
9.42
5
31
.76
5
39
.06
5
46
.565
4
7.21
0
29
.815
4
2.28
5
42
.915
3
8.93
5
40
.035
3
0.83
0
Mn
O
0.4
07
0
.27
6
0.3
28
0
.38
0
0.3
58
0
.38
1
0.2
76
0
.42
2
0.3
90
0
.42
0
0.4
08
0
.20
6
MgO
9
.47
0
13
.210
1
2.4
10
8
.38
5
5.7
90
5
.46
5
13
.360
7
.16
5
6.9
10
8
.52
0
8.0
90
1
2.30
5
NiO
0
.12
4
0.2
16
0
.08
7
0.0
78
0
.04
2
0.0
20
0
.10
3
0.0
61
0
.05
3
0.0
78
0
.04
8
0.2
35
CaO
0
.00
6
0.0
38
0
.02
1
0.0
15
0
.00
5
0.0
05
0
.01
6
0.0
05
0
.00
9
0.0
02
0
.00
1
0.0
08
Total
99
.68
0
99
.805
9
9.6
83
9
8.8
88
9
8.29
2
98
.416
9
9.50
6
99
.341
9
9.01
7
99
.411
9
9.39
6
99
.449
Bu
l-37
B
ul-3
8
Bu
l-39
Bu
l-40
Bu
l-41
Bu
l-42
Bu
l-43
Bu
l-44
Bu
l-45
Bu
l-46
Bu
l-47
Majo
r elemen
ts wt%
TiO2
5
4.72
5
53
.080
5
3.32
0
48
.55
5
53
.995
5
1.6
55
4
8.98
0
51
.565
4
7.45
0
42
.695
5
4.30
5
SiO2
0
.01
4
0.0
04
0
.00
0
0.0
28
0
.01
6
0.0
15
0
.00
6
0.0
00
0
.00
5
0.0
09
0
.02
2
Nb
2 O5
0
.11
4
0.1
62
0
.18
9
0.7
02
0
.08
4
0.2
83
0
.52
3
0.2
53
0
.86
6
1.4
31
0
.10
3
Al2 O
3
0.3
41
0
.12
8
0.1
11
0
.02
4
0.3
04
0
.03
0
0.1
35
0
.02
7
0.0
26
0
.02
4
0.2
75
Cr
2 O3
1
.45
2
1.0
59
1
.13
0
1.6
30
1
.50
5
1.4
37
1
.65
0
1.3
24
2
.63
0
1.9
65
1
.48
2
FeO
t 2
8.62
5
32
.250
3
2.25
5
38
.75
5
28
.845
3
3.1
45
3
6.64
0
35
.535
3
9.11
5
45
.765
2
9.06
0
Mn
O
0.2
60
0
.34
3
0.3
49
0
.41
2
0.2
83
0
.42
3
0.2
46
0
.40
2
0.3
69
0
.36
2
0.3
11
MgO
1
3.67
0
12
.160
1
1.88
5
8.4
15
1
3.67
5
11
.71
5
10
.695
1
0.08
5
8.5
90
6
.02
0
13
.640
NiO
0
.14
2
0.0
88
0
.07
5
0.0
65
0
.11
5
0.0
95
0
.09
5
0.1
08
0
.05
8
0.0
37
0
.13
1
CaO
0
.04
4
0.0
10
0
.01
8
0.0
07
0
.01
8
0.0
22
0
.01
6
0.0
08
0
.01
0
0.0
00
0
.04
2
Total
99
.387
9
9.28
3
99
.331
9
8.5
93
9
8.84
0
98
.82
1
98
.986
9
9.30
7
99
.120
9
8.30
8
99
.372
93
Tab
le 5. G
rann
y S
mith
Clin
op
yro
xen
e majo
r elemen
t analy
sis
13
-45
-22
1
Po
rph
yroclast
Margin
C
en
ter
W
t.%
At om
un
its
Wt.%
A
t om u
nits
SiO2
5
4.97
97
4
1.9
54
Si
SiO2
5
5.14
49
7
1.9
59
Si
TiO2
0
.33
60
96
0
.00
9
Ti TiO
2
0.3
50
11
2
0.0
09
Ti
Al2 O
3
1.8
22
56
5
0.0
76
A
l A
l2 O3
1
.99
18
41
0
.08
3
Al
Fe2 O
3
0.0
00
0
.09
3
Fe+3
Fe
2 O3
0
.00
0
0.0
99
Fe+
3
Cr
2 O3
1
.01
01
5
0.0
28
C
r+3
Cr
2 O3
1
.08
19
41
0
.03
0
Cr+3
Fe
O
3.1
27
34
1
0.0
00
Fe+
2
FeO
3
.32
09
94
0
.00
0
Fe+2
M
nO
0
.09
30
81
0
.00
3
Mn
M
nO
0
.09
36
41
0
.00
3
Mn
M
gO
16
.981
61
0
.90
0
Mg
MgO
1
6.69
13
4
0.8
84
M
g C
aO
20
.718
14
0
.78
9
Ca
CaO
2
0.22
25
0
.77
0
Ca
Na
2 O
2.1
24
72
8
0.1
46
N
a N
a2 O
2
.34
26
95
0
.16
1
Na
K2 O
0
.01
68
37
0
.00
1
K
K2 O
0
.00
69
92
0
.00
0
K
H2 O
0.0
00
H
H
2 O
0
.00
0
H
Ca/(C
a+M
g) 0
.46
71
98
C
a/(Ca+
Mg)
0.4
65
46
3
Mg/(M
g+Fe) 0
.90
63
61
M
g/(Mg+Fe)
0.8
99
59
94
Ne
ob
last
M
argin
C
en
ter
SiO
2
Wt.%
5
4.83
69
7
At
1.9
63
o
m U
nits Si
SiO
2
Wt.%
5
5.28
36
A
t 1
.97
0
om
Un
its Si
TiO2
0
.37
81
21
0
.01
0
Ti TiO
2
0.2
91
48
5
0.0
08
Ti
Al2 O
3
1.3
45
93
0
.05
7
Al
Al2 O
3
1.3
61
41
6
0.0
57
A
l Fe
2 O3
0
.00
0
0.0
88
Fe+
3
Fe2 O
3
0.0
00
0
.09
3
Fe+3
C
r2 O
3
0.7
97
92
5
0.0
23
C
r+3
Cr
2 O3
0
.80
79
85
0
.02
3
Cr+3
Fe
O
3.2
53
98
9
0.0
09
Fe+
2
FeO
3
.32
59
23
0
.00
7
Fe+2
M
nO
0
.07
01
24
0
.00
2
Mn
M
nO
0
.06
77
18
0
.00
2
Mn
M
gO
17
.133
94
0
.91
4
Mg
MgO
1
6.97
35
9
0.9
02
M
g C
aO
21
.336
67
0
.81
8
Ca
CaO
2
1.26
08
9
0.8
12
C
a N
a2 O
1
.64
67
71
0
.11
4
Na
Na
2 O
1.8
45
94
6
0.1
28
N
a K
2 O
0.0
08
28
5
0.0
00
K
K
2 O
0.0
08
28
5
0.0
00
K
H
2 O
0
.00
0
H
H2 O
0.0
00
H
C
a/(Ca+
Mg)
0.4
72
30
1
Ca/(C
a+M
g) 0
.47
37
58
M
g/(Mg+Fe)
0.9
03
71
7
Mg/(M
g+Fe) 0
.90
09
62
95
13
-45
-22
3
Po
rph
yroclast
M
argin
C
en
ter
Wt.%
At o
m U
nits
Wt.%
At o
m U
nits
SiO2
5
5.1
50
52
1
.96
7
Si SiO
2
54
.974
95
1
.96
5
Si TiO
2
0.3
06
76
6
0.0
08
Ti
TiO2
0
.29
38
44
0
.00
8
Ti A
l2 O3
1
.34
57
15
0
.05
7
Al
Al2 O
3
1.3
80
39
1
0.0
58
A
l Fe
2 O3
0
.00
0
0.0
98
Fe+
3
Fe2 O
3
0.0
00
0
.10
0
Fe+3
C
r2 O
3
0.8
33
99
2
0.0
24
C
r+3
Cr
2 O3
0
.89
07
51
0
.02
5
Cr+3
Fe
O
3.3
73
92
1
0.0
02
Fe+
2
FeO
3
.36
05
83
0
.00
0
Fe+2
M
nO
0
.11
72
65
0
.00
4
Mn
M
nO
0
.11
36
67
0
.00
3
Mn
M
gO
17
.01
91
7
0.9
05
M
g M
gO
16
.969
73
0
.90
4
Mg
CaO
2
1.0
75
43
0
.80
6
Ca
CaO
2
0.98
10
6
0.8
04
C
a N
a2 O
1
.86
50
93
0
.12
9
Na
Na
2 O
1.8
95
32
9
0.1
31
N
a K
2 O
0.0
11
84
2
0.0
01
K
K
2 O
0.0
11
84
2
0.0
01
K
H
2 O
0
0.0
00
H
H
2 O
0
.00
0
H
Ca/(C
a+M
g) 0
.47
09
06
C
a/(Ca+
Mg)
0.4
70
51
3
Mg/(M
g+Fe) 0
.89
99
18
M
g/(Mg+Fe)
0.9
00
01
2
96
Neo
blast
M
argin
C
en
ter
SiO
2
wt%
5
4.7
31
93
A
t 1
.96
7
om
un
its Si
SiO
2
wt%
5
5.24
45
6
At
1.9
71
o
m u
nits Si
TiO2
0
.37
27
65
0
.01
0
Ti TiO
2
0.2
46
24
2
0.0
07
Ti
Al2 O
3
1.2
09
37
0
.05
1
Al
Al2 O
3
1.3
18
78
9
0.0
55
A
l Fe
2 O3
0
.00
0
0.0
83
Fe+
3
Fe2 O
3
0.0
00
0
.09
0
Fe+3
C
r2 O
3
0.8
10
94
8
0.0
23
C
r+3
Cr
2 O3
0
.73
62
79
0
.02
1
Cr+3
Fe
O
3.1
28
67
3
0.0
11
Fe+
2
FeO
3
.08
29
36
0
.00
2
Fe+2
M
nO
0
.10
28
15
0
.00
3
Mn
M
nO
0
.09
68
34
0
.00
3
Mn
M
gO
16
.87
97
2
0.9
04
M
g M
gO
16
.976
12
0
.90
3
Mg
CaO
2
1.6
61
94
0
.83
4
Ca
CaO
2
1.59
49
8
0.8
26
C
a N
a2 O
1
.61
31
23
0
.11
2
Na
Na
2 O
1.7
54
55
4
0.1
21
N
a K
2 O
0
0.0
00
K
K
2 O
0.0
16
97
2
0.0
01
K
H
2 O
0
.00
0
H
H2 O
0.0
00
H
C
a/(Ca+
Mg)
0.4
79
80
3
Ca/(C
a+M
g) 0
.47
76
1
Mg/(M
g+Fe) 0
.90
58
13
M
g/(Mg+Fe)
0.9
07
54
1
97