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PARTITION COEFFICIENTS OF URANIUM FOR SOME ROCK-FORMING MINERALS
J. DOSTAL and S. CAPEDRI*
Department of Geology, Dalhousie University, Halifax, N.S. (Canada)
(Received January 31, 1975; accepted April 7, 1975)
ABSTRACT
Dostal, J. and Capredi, S., 1975. Partition coefficients of uranium for some rock-forming minerals. Chem. Geol., 15: 285--294.
Partition coefficients of uranium between phenocrysts and their host groundmass have been determined by fission-track mapping. The minerals analyzed include plagioclase, K- feldspar, biotite, olivine, clinopyroxene and orthopyroxene. The data for all these minerals show that U is strongly partitioned into the liquid and only a small fraction of the total whole-rock U content is present in the major rock-forming minerals. In volcanic rocks, the bulk of U is usually contained in glass although in acid volcanic rocks a significant portion may also be present in the U-rich accessory minerals.
INTRODUCTION
A knowledge of the partitioning of trace elements between rock-forming minerals and silicate melts has played an important role in elucidating the genesis and evolution of igneous rocks. Although the partition coefficients for many lithophile elements are fairly well established, only limited empiri- cal data are available for uranium, the most important heat-producing element. In fact, there is relatively little information on U abundances in some common rock-forming minerals. This has led us to determine U in several minerals, main- ly from volcanic rocks.
The purpose of this paper is to report the data on the distribution of U in several igneous rocks and their const i tuent minerals, particularly on the U- partitioning between rock-forming mineral phenocrysts and the groundmass.
SAMPLE DESCRIPTIONS
The samples analyzed in this s tudy are: (1) Acid volcanic rocks from San Vincenzo, Roccastrada, Monte Amiata
and Monte Cimino, Tuscany, Italy and genetically associated plutonic rocks of Monte Capanne, Elba.
*On leave from the Insti tuto di Mineralogia e Petrologia, Universit~t di Modena, Italy.
TA
BL
E I
Ch
emic
al c
om
po
siti
on
of
min
eral
s an
d g
lass
es o
f al
kal
i bas
alts
an
d s
tru
ctu
ral
form
ula
e o
f m
iner
als a
t,0
00
W
t. %
O
liv
ine
Cli
no
py
rox
ene
sam
ple
70
b
sam
ple
73
b
sam
ple
70
b
sam
ple
73
c
core
ri
m
core
ri
m
core
ri
m
Pla
gio
clas
e
sam
ple
73
b
core
ri
m
Gla
ss
sam
ple
70
sa
mp
le 7
3
SiO
=
39
.41
3
8.8
9
40
.45
3
9.4
7
52
.11
4
6.8
4
46
.80
4
9.2
2
50
.63
T
iO=
0
.04
0
.04
0
.06
0
.06
0
.26
3
.08
2.
57
0.0
4
0.0
4
AI=
O~
0.0
5
0.0
6
0.0
5
0.07
1
.27
6
.83
5
.59
3
1.6
9
31
.09
C
r20~
0
.03
0
.04
0
.00
0.
01
0.0
0
0.1
8
0.0
7
0.0
1
0.0
1
FeO
d
16
.46
1
8.6
8
13
.93
1
8.4
5
11
.14
6
.75
7
.67
0
.28
0
.26
M
nO
0.2
1
0.31
0
.20
0
.33
0
.40
0
.10
0
.10
0
.01
0
.01
N
iO
0.1
7
0.1
7
n.d.
n.
d.
0.9
0
0.0
1
n.d.
n.
d.
n.d.
M
gO
43
.27
4
1.3
1
44
.90
4
1.1
3
12
.77
1
2.7
6
13
.52
0
.06
0
.05
C
aO
0.2
3
0.3
8
0.0
9
0.2
5
21
.38
2
2.8
1
22
.43
1
5.5
8
14
.50
N
a20
0
.04
0
.03
0
.02
0
.03
0
.41
0
.53
0
.60
2
.62
3
.17
K
20
0
.02
0
.06
0
.02
0
.03
0
.03
0
.03
0
.08
0
.26
0
.33
Su
m
99
.93
9
9.9
7
99
.72
9
9.8
3
99
.77
9
9.9
2
99
.43
9
9.7
7
10
0.0
9
Si
0.9
99
0
.99
7
1.0
12
1
.00
9
1.9
68
1
.75
3
1.7
69
9
.03
8
9.2
36
IV
0
.00
1
0.0
02
0
.00
1
0.0
02
0
.03
2
0.2
47
0
.23
1
6.8
58
6
.68
4
~Al V
I 0
.02
5
0.0
54
0
.01
8
Ti
0.0
01
0
.00
1
0.0
01
0
.00
1
0.0
07
0
.08
7
0.0
73
0
.00
5
0.0
05
C
r 0
.00
1
0.0
01
0
.00
5
0.0
02
0
.00
1
0.0
01
M
g 1
.63
4
1.5
78
1
.67
4
1.5
67
0
.71
9
0.7
12
0
.76
2
0.0
16
0
.01
4
Ni
0.0
04
0
.00
4
Fe
0.3
49
0
.40
0
0.2
91
0
.39
4
0.3
52
0
.21
1
0.2
42
0
.04
3
0.0
40
M
n 0
.00
5
0.0
07
0
.00
4
0.0
07
0
.01
3
0.0
03
0
.00
3
0.0
02
0
.00
1
Ca
0.0
06
0
.01
0
0.0
02
0
.00
7
0.8
65
0
.91
5
0.9
08
3
.06
5
2.8
34
N
a 0
.00
2
0.0
02
0
.00
1
0.0
01
0
.03
0
0.0
39
0
.04
4
0.9
33
1
.12
1
K
0.0
01
0
.00
2
0.0
01
0
.00
1
0.0
01
0
.00
1
0.0
04
0
.06
1
0.0
77
X
0.9
0
0.9
6
0.9
6
4.1
3
4.0
9
Y
2.0
0
2.01
1.
97
1.9
8
1.1
2
1.0
7
1.1
0
Z
1.0
0
1.0
0
1.01
1.
01
2.0
0
2.0
0
2.0
0
15
.90
1
5.9
2
nd
. =
no
t d
eter
min
ed
56
.03
5
4.0
7
1.5
9
1.89
2
1.6
5
20
.15
0
.00
0
.00
4
.33
4
.66
0
.07
0
.07
0
.02
n.
d.
1.0
9
1.3
0
1.9
3
2.2
7
e 7.
11
e 7
.46
86
.71
9
8.9
8
a C
alcu
lati
on
on
th
e b
asis
of
4, 6
an
d 3
2 o
xy
gen
s p
er f
orm
ula
fo
r o
liv
ine,
cli
no
py
rox
ene
and
pla
gio
clas
e, r
esp
ecti
vel
y.
b P
hen
ocr
yst
. c
Gro
un
dm
ass.
d
To
tal
iro
n a
s F
eO.
e N
a=O
an
d K
20
co
uld
no
t be
mea
sure
d d
ue
to r
apid
dec
reas
e o
f X
-ray
in
ten
sity
.
287
(2) Alkali olivine basalts from Pozzomaggiore, Sardinia. The acid volcanic rocks from Tuscany are ignimbrites of late Tertiary to Quaternary age. Their composition varies from one volcanic centre to another, quartz-latites, rhyo- lites and trachytes being the dominant rock types, whereas the plutonic rocks are mainly granodiorites. The volcanic rocks contain phenocrysts of sanidine, biotite and plagioclase in a glassy groundmass. At San Vincenzo and Rocca- strada, ignimbrites also occasionally contain crystals of quartz and cordierite while hypersthene occurs in ignimbrites of Monte Amiata and Monte Cimino. Detailed geological, petrographic and chemical information on these rocks was given in a series of articles (Marinelli, 1961; Mazzuoli and Pratesi, 1963; Mittempergher and Tedesco, 1963; Barberi et al., 1967; Mazzuoli, 1967; Dupuy, 1970; Dupuy and Allegre, 1972}. In particular, the chemical composition of analyzed minerals, glasses and rocks was reported by Dupuy (1970).
The alkali basalts from Pozzomaggiore, NW Sardinia, are of Pliocene- Quaternary age (Coulon et al., 1974). These rocks consist of phenocrysts of olivine, clinopyroxene and plagioclase in a groundmass of glass, plagioclase, clinopyroxene, olivine and opaque minerals. The phenocrysts are zoned and generally euhedral in shape. The chemical composition of minerals and glasses analyzed for U is given in Table I together with their structural formulae.
ANALYTICAL METHODS
The uranium determinations were made by the fission-track method as adapted at Dalhousie University (Aumento and Hyndman, 1971; Mitchell and Aumento, 1974). Thin pellets of the pulverized samples were used for the whole-rock determination, while the analyses of the mineral phases and glasses were done on the polished thin-sections. The precision and accuracy of these determinations can be evaluated from the data on the standard rocks BCR-1 and DTS-1 which were analyzed simultaneously with the samples studied. The values obtained are 1.79+0.12 ppm U (BCR-1) and 0.0037+-0.0005 ppm U (DTS-1). The values given by Flanagan (1973) are 1.74 and 0.004 ppm U, respectively. Each value for the reference rocks is an average of three deter- minations, while the error indicated is the standard deviation, which is less than 15%. The precision of some values for mineral phases is, however, poorer, probably up to 20%. The chemical compositions of mineral phases and glasses given in Table I were obtained by electron-microprobe at Dalhousie University.
RELIABILITY OF THE DATA
In addition to a number of problems and assumptions involved in the deter- mination of partition coefficients for trace elements (e.g., Schnetzler and Philpotts, 1968, 1970; Philpotts and Schnetzler, 1970; Albarede and Bottinga, 1972) there are two important factors when considering the reliability of our data. The first is the mode of occurrence of U in the analyzed minerals and the second is whether the assemblages studied at least approach quasi-equi-
TA
BL
E I
I
U c
on
cen
trat
ion
s (p
pm
) in
roc
ks,
mat
rice
s an
d m
iner
als
tO
0V
0V
Ro
ck
Mat
rix
B
ioti
te
K-f
eld
spar
P
lagi
ocla
se
Cli
no-
Ort
ho
- O
livi
ne
Co
rdie
rite
p
yro
xen
e p
yro
xen
e
Gra
no
dio
rite
M
. C
apan
ne
4.6
0
Ign
imb
rite
S
an V
icen
zo
7.69
10
.1
Ign
imb
rite
R
occ
astr
ada
8.22
12
.2
Ign
imb
rite
M
. A
mia
ta
7.97
11
.6
Ign
imb
rite
M
. C
imin
o
8.01
10
.6
Alk
ali
basa
lt
sam
ple
70
1.66
3.
04
Alk
ali
basa
lt
sam
ple
73
1.50
2.
72
0.2
74
0
.06
59
0
.07
54
0.2
32
0
.06
50
0
.07
56
0.27
7 0
.06
55
0
.07
87
0.2
40
0
.05
90
0
.07
77
0.2
25
0
.06
48
0.
0741
0.0
24
6
0.13
4
0.11
1
0.0
63
0
0.0
76
0
0.0
08
17
0.0
06
61
289
librium systems. With regard to the occurrence of U in major rock-forming minerals, Rogers
and Adams (1969) have pointed out that the trace amounts of U may be present in them as: (1) isomorphous substi tution in the lattice; (2) concen- tration in lattice defects; (3) adsorption along crystal imperfections and grain borders; and (4) inclusions as microcrystais o:~ uranium minerals.
Although small U-rich crystals producing a high agglomeration of tracks as well as a higher density of fission tracks along the fractures and even grain borders have been occasionally observed, particularly in the granodiorite, U was determined only in clear unfractured crystals wi thout any visible inclu- sions and with a homogeneous distribution of tracks. The petrographic obser- vations also indicate that post-crystallization alteration probably did not in- fluence the U content of mineral phases since in all samples studied even the glassy matrix is fresh without any signs of oxidation. The homogeneous distri- bution of tracks together with the regularities of determined parti t ion coeffi- cients suggest that the measured U in mineral phases is, for the most part, present in solid-solution state.
As far as the acid volcanic rocks from Tuscany are concerned the problem of equilibrium between phenocrysts and glassy matrix has been treated in some detail by Dupuy (1970) who concluded that at least quasi-equilibrium was attained for a number of major and trace elements for sanidine, plagio- clase and biotite. This probably also applies to U which in each of these min- eral phases appears to be uniformly distributed throughout a given sample. Although or thopyroxene in these rocks is of xenocrystic origin, it still might yield meaningful partition coefficients provided that equilibrium was achieved. Dupuy (1970) has indeed suggested that even this mineral phase was probably in equilibrium with liquid.
With respect to alkali basalts, some petrographic features such as the ab- sence of reaction rims and corrosion and well-defined crystal boundaries with the matrix are consistent with the equilibrium conditions. On the other hand, as can also be ascertained from Table I, phenocrysts are composit ionally zoned implying that only their outermost zones may be in equilibrium with the matrix. The distribution of tracks in these phenocrysts does not, however, show any obvious zonation, at least not outside the limits of analytical pre- cision. This also appears from a comparison of data on cl inopyroxene in both analyzed samples. The U partition coefficient of the small c l inopyroxene crystals of the matrix of sample 73 is almost the same as that of large pheno- crysts of sample 70 although the major-element composi t ion of the former is rather similar to the outer zone of the latter. Thus, the partition coefficients measured for these zoned phenocrysts might indeed approximate the actual coefficients operative during the evolution of the magma.
RESULTS
U abundances of individual mineral phases and corresponding glassy ma-
290
trices are given in Table II while the simple partition coefficients calculated as (U concentrat ion in phenocrys t ) / (U concentrat ion in matrix) (D U) are presented in Table III. Regarding the distribution of U in whole-rock samples, Table IV shows that only a small fraction of U is concentrated in the main rock-forming minerals. In the case of the granodiorite, most of U occurs in accessory minerals (zircon, allanite, apatite), although an appreciable amount of U appears to be present along the fractures and grain borders of the rock- forming minerals. In volcanic rocks from Tuscany, a major port ion of U is held by glass. But once again accessory minerals contain a significant part of the total whole-rock U concentration. It is of interest that the U content of individual mineral phases is about the same in volcanic and plutonic rocks, thus agreeing with a comagmatic origin as invoked by Marinelli (1961) and Dupuy (1970). The bulk of U in alkali basalts is contained in glass; no acces- sory U-rich minerals were observed in these samples.
TABLE III
Partition coefficients of U (D U × 103 ) between minerals and liquid
A comparison of our data with previously determined U abundances of rock-forming minerals and their partit ion coefficients may be of some interest In general, the U contents of minerals of acid volcanic and plutonic rocks given in Table II are at least of an order of magnitude lower than those com- piled recently by Rogers and Adams (!969) . The concentrat ion of U in clino- pyroxene, olivine and plagioclase of alkali basalts is, however, comparable to the values reported by Nagasawa and Wakita (1968), Henderson et al. (197 i ) and Nishimura (1972) for the same mineral phases f rom basic vol- canic and plutonic rocks.
TA
BL
E I
V
Co
ntr
ibu
tio
n o
f in
divi
dual
n~
ajor
ph
ases
to
wh
ole
-ro
ck U
co
nte
nt
Bio
tite
K
-fel
dsp
ar
Pla
gioc
lase
C
M
C
M
C
M
Py
rox
ene
C
M
Oli
vine
C
M
Co
rdie
rite
C
M
Mat
rix
C
M
U
(pp
m)
Gra
no
dio
rite
' M
. C
apan
ne
Ign
imb
rite
3
San
Vic
enzo
Ign
imb
rite
3
Ro
ccas
trad
a
Ign
imb
rite
2 M
. A
mia
ta
Ign
imb
rite
2 M
. C
imin
o
Alk
ali
bas
alt
sam
ple
70
Alk
ali
bas
alt
sam
ple
73
0.2
74
x
0.1
2
0.0
66
x
0.2
3
0.0
75
x
0.4
0
0.2
32
x
0.1
0
0.0
65
x
0.0
9
0.0
76
x
0.2
0
0.27
7 x
0.0
4
0.0
66
x
0.17
0
.07
9
x 0
.10
0.2
40
x
0.0
3
0.0
59
x
0.1
4
0.0
78
x
0.1
6
0.2
25
x
0.0
9
0.0
65
x
0.11
0
.07
4 x
0
.24
0.0
25
x
0.07
0.0
63
x
0.0
5
0.1
34
X 0
.24
0.1
11
x 0
.21
0.0
08
x
0.1
8
0.0
07
x
0.1
7
0.0
76
×
0.0
2
10.1
x
0.5
4
12.2
x
0.5
3
11.6
x
0.6
2
10.6
x
0.5
0
3.0
4 x
0
.51
2.7
2 x
0
.52
0.0
78
(4
.60
).
5.4
98
(7
.69
)
6.4
98
(8
.22
)
7.2
20
~
7.9
7)
5.3
48
(8
.01
)
1.5
84
(1
.66
)
1.4
41
(1
.50
)
C =
U c
on
ten
t (p
pm
); M
= m
od
al p
rop
ort
ion
. (
) D
eter
min
atio
n o
f U
co
nte
nt
in w
ho
le-r
ock
sam
ple
. '
Zir
con,
all
anit
e, a
pat
ite,
sp
hen
e (a
cces
sory
min
eral
s p
rese
nt)
. 2
Zir
con,
all
anit
e, a
pat
ite
(acc
esso
ry m
iner
als
pre
sen
t).
3 Z
irco
n, a
pat
ite
(acc
esso
ry m
iner
als
pre
sen
t).
b~
¢D
292
There are only a few published data on partition coefficients for U. For natural clinopyroxene, Nagasawa and Wakita (1968) have given values (D U X 103 ) from volcanic rocks ranging 4--84, while Kleeman et al. (1969) obtained D U X 103 values of 4--10 from lherzolite inclusions of basanites. Seitz and Shimizu (1972) and Seitz (1973) have reported experimental data on clino- pyroxene-liquid and orthopyroxene-l iquid partitioning of U at high pressures and temperatures. Their data indicate that the partitioning of U is not ap- preciably dependent on the composi t ion of the melt or temperature or pres- sure. The D U X 103 of 8.0 for synthetic or thopyroxene given by Seitz and Shimizu (1972) is in good agreement with the hypersthene value in Table III (6.0).
The D U values for all rock-forming minerals in Table III are substantially lower than 1, resulting in a considerable enrichment of U in the residual liquid phase during differentiation. This is consistent with the nearly universal trend for U to increase towards the more differentiated rocks in a con- sanguinous igneous series. The data also indicate that the variation of U, par- ticularly in the more acid rocks might be strongly influenced by the acces- sory U-rich minerals.
PETROLOGICAL IMPLICATIONS
As an example of an application of partition coefficients of U, the ultra- mafic rocks of ophiolite suites and the olivine gabbro inclusions of alkali basalts are considered below. Ultramafic rocks of Tethyan ophiolites, which probably are slices of oceanic lithosphere tectonically emplaced on the con- tinent, correspond predominantly to harzburgites and lherzolites. The U con- tents of cl inopyroxene and olivine in a number of these rocks from the nor- t hem Appennines and Hellenides range from about 4.4 to 6.2 and from 0.3 to 1.3 ppb respectively (our unpublished data). If these minerals were in equi- librium with mafic magma, the U content of such a melt may be calculated using the D U given in Table III at about 100--150 ppb for c!inopyroxene and about 110--550 ppb for olivine. These U concentrations are similar to those found in typical oceanic tholeiites which contain 100--300 ppb (Tatsumoto et al., 1965; Aumento, 1971). Thus, the U data are consistent with models for the origin of ophiolites where ultramafic rocks are either cumulates from or residuum after extraction of the oceanic tholeiite liquid.
For magnetite-bearing olivine gabbro inclusions of alkali basalts from Iki Island, Japan, Kuno and Aoki (1970) invoked their derivation from moderate- ly differentiated alkali basalt magma, while Nishimura (1972) suggested that they represent residuum after the extraction of tholeiitic melt. The uranium content of olivine from these inclusions is about 5 ppb (Nishimura, 1972). Using D U reported here, the U concentrat ion in the hypothet ical liquid in equilibrium with the olivine would be about 1,850--2,090 ppb U. Such values are similar to those observed in some alkali basalts but differ notably from those of tholeiites, thus agreeing with the hypothesis of Kuno and Aoki (1970).
293
ACKNOWLEDGEMENT
We thank Dr. C. Dupuy for providing the samples from Tuscany and Dr. C.A.R. Albuquerque for his helpful comments.
REFERENCES
Albarede, F. and Bottinga, Y., 1972. Kinetic disequilibrium in trace element partitioning between phenocrysts and host lava. Geochim. Cosmochim. Acta, 3 6 : 141--156.
Aumento, F. and Hyndman, R.D., 1971. Uranium content of the oceanic upper mantle. Earth Planet. Sci. Lett., 12: 373--384.
Barberi, F., Innocenti, F. and Mazzuoli, F., 1967. Contributo alla conoscenzo chimico- petrografica e magmatologica delle rocce intrusive, vulcaniche e filoniane del Campigliese (Toscana). Soc. Geol. Ital., Mere. 6: 643--681.
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