Minerals and Rocks
44
Systematic Mineralogy
Pure forsterite melts at 1890°C and pure fayalite at 1205°C and there is complete solid solution between
them. A temperature - composition diagram for olivine is a "cigar-diagram" (Fig. 4.2).
Fig. 4.2: Temperature-composition diagram (at atmospheric pressure) for the
olivine system (forsterite Mg
2
[SiO
4
] - fayalite Fe
2
[SiO
4
]).
A. The diagram is divided into three fields by two curves. A “melt” field occurs above the upper (liquidus)
curve. A “solid” field occurs below the lower (solidus) curve. The two curves outline a cigar-shaped field
where solid (olivine crystals) and melt occur in equilibrium. B. The crystallization process illustrated here is
explained in the text.
Consider a melt with composition A (melt with the composition of Fo
50
) at a temperature of >1800°C. On
cooling this will intersect the liquidus at B at a temperature of 1660°C. Crystals of Mg-rich olivine with
composition C (Fo
77
) will begin to form. Crystals with composition C are in equilibrium with melt with
composition B and they are, of course, at the same temperature. With further cooling new crystals will grow
and the crystals that have already formed will gradually change composition along the solidus curve while
the melt changes composition along the liquidus curve. The crystals will always remain in equilibrium with
the cooling melt e.g. crystals at E will be in equilibrium with melt D. The amount of crystals relative to melt
will gradually increase and the final drop of melt will have composition F (melt with a composition of Fo
21
)
which is in equilibrium with crystals at G. Note that G (Fo
50
) has the same composition as the initial melt A.
Note that the composition of the melt will always be more iron-rich than that of the coexisting crystals at the
same temperature. This crystallization path assumes perfect equilibrium - the melt is always able to react
with the crystals. This is seldom achieved in nature. For example, early crystals may be removed from the
melt to form a rock composed of Mg-rich olivine (called dunite). In our diagram the final melt can therefore
reach more Fe-rich compositions than F and the final crystals can therefore be more Fe-rich than G (Fo
50
)
even though the starting melt had a composition of Fo
50
. A fraction of the crystallizing assemblage has been
removed from the system and this process, called fractional crystallization, is very important in igneous
petrology.