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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