Geology Reference
In-Depth Information
Fig. 10.1 Phase relation in
the join diopside
-
akermanite
-
leucite at 1
atmosphere (after Gupta
1972)
(Diopside)
CaMgSi
26
Di
ss
1302
0
Cb
1361
0
C
c
1281
B
Ak
ss
Lc
ss
v
KAlSi
26
(Leucite)
v
v
v
v
v
v
v
v
a
Ca MgSi
O
2 2 7
(Akermanite)
and wollastonite
ss
within melilite and below 1,240
°
C, wollastonite
ss
is absent on
the liquidus of the diopside
leucite join. As the compositions of the
crystalline phases do not lie within the join, it is not ternary and point B is therefore,
a piercing point and the lines dividing the primary phase
akermanite
-
-
fields are traces of
divergent surfaces cut by the diopside
akermanite
leucite join.
-
-
10.1.1.2 The Join Forsterite
Diopside
Leucite
-
-
Figure
10.2
shows the phase diagram (Gupta 1972) for the join forsterite
diop-
-
side
leucite. At point c (Fo
3
Di
60
Lc
37
), forsterite
ss
+ diopside
ss
+ leucite
ss
coexist in
equilibrium at 1,296
-
±
3
°
C. Again the join is not ternary and the point c is a
piercing point.
10.1.1.3 The Join Forsterite
-
Akermanite
-
Leucite
Phase diagram of the join (Gupta 1972) is presented in Fig.
10.3
, which shows that
it is pseudoternary and cuts the phase volume of monticellite
ss
. The join has two
piercing points at Fo
17
Ak
78
Lc
5
and 1,428
C(H), where the assemblage is forste-
rite
ss
+ akermanite
ss
+ monticellite
ss
+ liquid; and Fo
9
Ak
43.5
Lc
47.5
and 1,286
°
C
(G), where the assemblage is forsterite
ss
+ akermanite
ss
+ leucite
ss
. At H, montic-
ellite
ss
reacts with the liquid to form akermanite and is completely eliminated at
1,410
±
3
°
±
3
°
C. Therefore, monticellite
ss
does not coexist with leucite
ss
.
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