Geology Reference
In-Depth Information
10.2.1.4 Paragenetic Relationship
in the System Diopside - Nepheline - Akermanite - Leucite under
Atmospheric Pressure
Of the two piercing points in the system diopside
akermanite (Onuma and
Yagi 1967), point H (Fig. 10.6 ) has a relatively lower liquidus temperature. This point
was therefore, chosen as one of the end members to which leucite was progressively
added. The join was studied to determine the temperature of the six-phase assem-
blage, forsterite ss +diopside ss +akermanite ss +leucite ss +nepheline ss +liquidinthe
system diopside
nepheline
-
-
leucite, and the phase equilibrium diagram is
presented in Fig. 10.11 . The join cuts the primary phase volumes of forsterite ss and
leucite ss . The pseudoeutectic occurs at (Di 38 Ak 3 Ne 59 ) 61 Lc 39 and 1,130
nepheline
akermanite
-
-
-
C, where
forsterite ss ,leuc te ss and liquid are in equilibrium. Figure 10.11 shows that at
1,105
±
5
°
C, forsterite ss +diopside ss + melilite + leucite ss +nepheline ss coexist with
liquid. Forsterite starts to react with liquid and is eliminated at 1,075 o
±
5
°
±
10
°
C, and
the subsolidus assemblage is Di ss +Mel+Ne ss +Lc ss .
Experimental results on the join nepheline
leucite, the pseudobinary
join (Di 38 Ak 3 Ne 59 ) 100-x Lc x and the other three bounding joins shows that the system
diopside
-
akermanite
-
-
nepheline
-
akermanite
-
leucite is pseudoquaternary.
If however,
the
'
presence of small amounts of alumina as Ca-Tschermak
s molecule in diopside and
the gehlenite molecule in melilite is ignored, the system can be treated as a quaternary
join of the
five component system, nepheline
kalsilite
CaO
MgO
SiO 2 .A
ow
-
-
-
-
sheet diagram of the system is shown in Fig. 10.12 , where only the
ve-phase
univariant lines are shown. At A (Fig. 10.7 ), forsterite ss , diopside ss , leucite ss and liquid
are in equilibrium at 1,275
±
5
°
C. Gupta and Lidiak (1973) found that with further
Fig. 10.11 Phase relation in
the join (Di 38 Ak 3 Ne 59 ) 100-x -
Lc x at 1 atmosphere (after
Gupta et al. 1973)
0 C
1200
1150
Fo
+L
ss
Fo s +Mel
+Ne ss
+L
1100
1050
1000
10
20
30
40
50
-x
(Di
+Ak +Ne
)100
38
3
59
Wt.% Lc
 
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