L. Francalanci et al., Neogene alkaline volcanism of the Afyon-Isparta area, Turkey: petrogenesisand geodynamic implications, MINER PETR, 70(3-4), 2000, pp. 285-312
In the Kirka-Afyon and Isparta areas, potassic and ultrapotassic alkaline m
agmatism followed Upper Eocene - Middle Miocene calc-alkaline volcanism, wh
ich was related to the northward subduction of the African Plate beneath Eu
rasia. The alkaline volcanism lasted from 14.8 Ma (in the north) to 4 Ma (i
n the south) and was associated with a presently still active extensional t
ectonic regime. It is mainly located along a N-S fault, which marks the lim
it between the Aegean Are and the Cyprus Are (Isparta Angle). In the Kirka-
Afyon area the potassic to ultrapotassic rocks range from silica saturated
(trachybasalts to trachytes) to highly undersaturated (phonolitic leucitite
s). In the Isparta area ultrapotassic rocks occur together with rhyolitic l
avas. In both areas, the ultrapotassic magmatism is transitional between la
mproitic and Roman type, with a more lamproitic character for the Isparta r
ocks. The potassic suites of both the Kirka-Afyon and Isparta areas are cha
racterised by rocks with Sr isotope ratios increasing from mafic to silicic
rocks. The rocks from Kirka-Afyon area have an orogenic affinity, whereas
those from Isparta area exhibit orogenic (the potassic suite) and within-pl
ate (the ultrapotassic suite) affinities. Extreme enrichments in LIL elemen
ts characterise the Afyon phonolitic leucitites, whereas enrichments in Sr
and REE are observed in Isparta potassic rocks. A residual, probably lithos
pheric mantle metasomatised by fluids and/or melts of different origin (sub
duction-related for the Kirka-Afyon rocks; deep astenospheric origin for th
e Isparta rocks), is considered to be the source of the ultrapotassic magma
s. A more "fertile" and probably deeper mantle, enriched by subduction-rela
ted components, is believed to be the source of the potassic rocks. Lower d
egrees of partial melting, in the mantle, at higher pressure, and probably
at higher X-CO2, may account for the genesis of the phonolitic leucitite pa
rental magmas. Partial melting of the mantle took place simultaneously in b
oth sources, probably due to post-collision extensional tectonics, which wa
s also responsible for the uprise of deep astenospheric mantle.