Significance of orthopyroxene and major element constraints on the petrogenesis of Ferrar tholeiites from southern Prince Albert Mountains, Victoria Land, Antarctica
G. Demarchi et al., Significance of orthopyroxene and major element constraints on the petrogenesis of Ferrar tholeiites from southern Prince Albert Mountains, Victoria Land, Antarctica, CONTR MIN P, 142(2), 2001, pp. 127-146
The least evolved Jurassic Ferrar tholeiites from southern Prince Albert Mo
untains (Antarctica) are characterized by the occurrence of orthopyroxene (
opx), a mineralogical feature virtually absent in the tholeiites from the l
arge igneous provinces of Karoo (South Africa) and Parand (Brazil). Petrogr
aphy suggests that opx is the early phase in the sequence of crystallizatio
n and mineral chemistry indicates that it is in equilibrium with the host r
ock. In general, MELTS modeling predicts that opx is the liquidus phase in
the Ferrar tholeiites with MgO higher than similar to7 wt% at P = 1.5-5 kba
r, H2O = 0-1 wt% and f(O2) = QFM - I log unit conditions. MELTS results als
o show that the early crystallization of opx is primarily controlled by hig
h SiO2 and high SiO2/CaO, chemical characteristics typical of the Ferrar th
oleiites, but not shown by the Karoo and Parand analogs with similar MgO co
ntent. Major element geochemistry of the least evolved Ferrar tholeiite has
been modeled through fractional crystallization and fractional crystalliza
tion coupled with crustal assimilation processes, starting from natural per
idotite-derived experimental melts. Mass balance and MELTS modeling support
the argument that theoretical magma compositions suitable to be primary to
the least evolved Ferrar tholeiites are compatible with hydrous (H2O = 0.3
-0.5 wt%) and anhydrous melts obtained at 10-15 kbar by high melting degree
s (> 25%) of fertile and depleted spinel lherzolites, respectively, and lat
er contaminated by the high-grade metamorphic rocks from the Victoria Land
crystalline basement. The genesis of primary Ferrar tholeiites does not nec
essarily reflect the generally assumed depleted source mantle being also co
mpatible with a fertile one.