Chemistry Reference
In-Depth Information
Table 10.4 (Continued).
Massifs
Karaossky
Maysky
Bulkinsky
M-27-98
M-30-98
2150
2530
2530-1
Bl-17
Bl-4
Bl-7
Olivine
gabbro
leuco-
cratic
Gabbro-
anortho-
site
Troctolite
leucoc-
ratic
Gabbro-
norite
Element
Websterite
Wehrlite
Olivine gabbro
Pd
0,78
1,11
1,65
N.d.
0,82
24,0
1,54
1,03
Pt
13,0
5,48
4,05
5,55
3,45
10,5
8,03
23,2
Ru
6,56
3,95
2,35
1,99
2,02
0,25
2,15
1,90
Ir
0,29
0,90
0,16
0,22
0,15
0,041
0,11
0,016
Total
PGE
20,6
11,4
8,21
7,76
6,44
37,8
11,8
26,1
Pt/Ir
45
6
26
25
23
257
74
1449
Pd/Ir
2,69
1,23
10,3
N.d.
5,47
585
14,0
64,4
La
3,88
0,789
3,39
3,11
14,1
0,694
0,981
0,568
Ce
11,8
1,70
7,71
7,89
28,82
1,348
3,060
1,208
Pr
N.d.
N.d.
N.d.
N.d.
N.d.
N.d.
N.d.
N.d.
Nd
11,3
1,23
5,26
5,47
15,7
0,786
3,44
0,703
Sm
3,23
0,336
1,350
1,380
3,021
0,159
1,195
0,140
Eu
0,910
0,136
0,680
0,618
0,975
0,239
0,668
0,274
Gd
3,71
0,395
1,45
1,47
2,71
0,166
1,56
0,125
Tb
0,647
0,068
0,259
0,250
0,413
0,025
0,286
0,019
Dy
3,79
0,424
1,64
1,52
2,23
0,146
1,78
0,115
Ho
0,739
0,088
0,346
0,295
0,413
0,027
0,344
0,024
Er
2,091
0,234
1,03
0,825
1,11
0,077
0,924
0,058
Tm
0,306
0,034
0,168
0,120
0,162
0,014
0,128
0,010
Yb
1,84
0,244
1,05
0,770
0,968
0,077
0,761
0,067
Lu
0,248
0,039
0,154
0,110
0,142
0,009
0,103
0,010
(La/Yb) n
1,42
2,19
2,18
2,73
9,85
6,05
0,87
5,69
(Eu/Eu*) n
0,80
1,14
1,48
1,32
1,02
4,46
1,50
6,23
Note: The analyses were done in the Analytical Center of IGM SB RAS (analysts S. Palesskii, I. Nikolaeva,
O. Koz'menko). Detection limits of PGE (ppb): Os - 0,07; Ir - 0,002; Ru - 0,005; Pt - 0,07; Pd - 0,09. N.d. - no data.
which indicates that during the crystallization of their parent melt, no significant
fractionation of plagioclase crystals occurred (Figure 10.3, 1-3).
The REE patterns of gabbro, olivine gabbro and wehrlite of Mazhalyksky
massif, that have steep negative slopes, are complicated by positive Eu anomalies
due to fractionation of plagioclase (Figure 10.3, 4-6). In the rocks of Karaossky
massif the lowest REE contents are observed in wehrlite, slightly higher in gabbro-
norite, and much higher in websterite. The REE distribution patterns in all these
rocks have a common negative slope (Figure 10.3, 7-9). It was already mentioned,
that rocks of Maysky massif differ from samples of other massifs by a gener-
ally high REE content and especially LREE content. Similar configuration of REE
 
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