LOW-PRESSURE CRYSTALLIZATION PATHS OF H2O-SATURATED BASALTIC-HAWAIITIC MELTS FROM MT ETNA - IMPLICATIONS FOR OPEN-SYSTEM DEGASSING OF BASALTIC VOLCANOS
N. Metrich et Mj. Rutherford, LOW-PRESSURE CRYSTALLIZATION PATHS OF H2O-SATURATED BASALTIC-HAWAIITIC MELTS FROM MT ETNA - IMPLICATIONS FOR OPEN-SYSTEM DEGASSING OF BASALTIC VOLCANOS, Geochimica et cosmochimica acta, 62(7), 1998, pp. 1195-1205
Melt inclusions indicate that the basaltic-hawaiitic magmas from Mt Et
na (Sicily) contained up to 2.3 wt% H2O dissolved in the melt, prior t
o eruption. The effect of H2O degassing during magma ascent has been e
xperimentally constrained between 1135 and 1009 degrees C, for P-H2O =
P-total varying from 800 to 270 bars. The starting material was a pri
mitive hawaiitic lava sample (MgO = 7.1 wt%) representative of the les
s evolved lava emitted at Mt Etna. Experiments were conducted in TZM p
ressure vessels, with Ag70Pd30 capsules in order to minimize the FeO l
oss. At temperatures of 1135-1090 degrees C, P-H2O = 800 bars, with Ni
NiO and FMQ buffers, olivine (Fo(83-80)) is the liquidus phase in equi
librium with a residual hawaiitic melt (Mg# 0.60-0.57; CaO/Al2O3 = 0.8
2). Salitic pyroxene begins to crystallize at 1075 degrees C, plagiocl
ase at 1025 degrees C and at 1009 degrees C, the magma is 33.5% crysta
llized with olivine, Ca-rich pyroxene, and plagioclase (16:60:24). At
P-H2O = 270 bars, FMQ buffer, olivine (Fo(79.3-80)) and salitic pyroxe
ne are the main liquidus phases between 1100 and 1090 degrees C. They
are in equilibrium with hawaiitic melts (Mg# 0.51; CaO/Al2O3 = 0.73).
At 1070 degrees C, the experimental charges are highly crystallized (a
pproximate to 51.5%) with olivine (Fo(70)) salite, and plagioclase (An
(78.4-76.3)) in 14:44:42 relative proportions. Increasing the water co
ntent of hawaiitic-basaltic magmas expands the stability field of the
olivine (relative to the other phases), lowers the crystallization tem
peratures of pyroxene and plagioclase, and results in the development
of a more An-rich plagioclase. When compared to the natural samples, t
hese results support a model of early and moderate crystallization of
olivine from Etnean primitive hawaiitic magmas, containing close to 2.
5 wt% H2O, with NNO oxygen buffering conditions, at low pressure (P-H2
O = P-total) We propose a model of crystallization driven by decompres
sion and water degassing during the emplacement of magma in the volcan
ic pile itself and possibly concomitant with the opening of fractures.
Copyright (C) 1998 Elsevier Science Ltd.