Geology Reference
In-Depth Information
SiO 2
90
10
P .1 G a
H 2 O
80
20
Silica
70
30
60
40
Sanidine ss
50
50
m
NaAlSi 38
KAlSi 38
40
60
850
840
800
Leu cite ss
30
780
R
70
865
870
890
M750
20
80
950
10
Nepheline ss
1200 K alsilite ss
1000
1100
90
10
20
30
40
50
60
70
80
90
NaAlSiO 4
KAlSiO 4
WEIGHT PERCENT
Fig. 7.2 Phase relation in the system nepheline
kalsilite
SiO 2 under 0.1 GPa [P(H 2 O) = P(Total)]
-
-
(after Hamilton and MacKenzie 1965)
that the liquid probably got frozen, as crystallization was hindered because of
eruption.
Cundari and Mattias (1974) plotted the composition of lavas of Somma-
Vesuvius and Phlegrean Field containing very low amount of MgO and other
components in terms of nepheline, kalsilite and SiO 2 (Fig. 7.3 ), they found that the
most evolved rocks have their compositions clustering around M.
The Vesuvius rocks of more salic type were plotted by Cundari and Le Maitre
(1970, Fig. 7.3 ) and found that they plot -near the 0.1 GPa [P(H 2 O) = P(Total)]
minimum representing phonolitic composition (Qz = 27
-
34, Ne = 35
-
47,
Ks = 25
27).
The silica
-
SiO 2 was
studied under 0.2 GPa [P(H 2 O) = P(Total)] by Taylor and MacKenzie (1975,
Fig. 7.4 ) and showed that the minimum melting point occurs at Ne 51 Ks 20 Qz 29 and
710 + 7
-
undersaturated part of the system, nepheline
-
kalsilite
-
°
C. Comparison of Figs. 7.1 , 7.2 , 7.3 and 7.4 show a signi
cant reduction
of leucite
field under 0.2 GPa P(H 2 O).
Zhang and Mackenzie (1984) studied the system NaAlSiO 4 -
SiO 2 -
H 2 O under 0.5 GPa. Their results are summarized in Fig. 7.5 , which shows that in
contrast to Figs. 7.1 , 7.2 and 7.3 and 7.4 leucite
KAlSiO 4 -
cantly reduced,
because this phase produced as an incongruent melting product of sanidine, is
field has been signi
 
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