In this work, we present the preliminary age data of the radiolarian cherts deposited on the top of basalts belonging
to the Eastern Ankara Mélange (part of the Izmir-Ankara Mélange). Petrological studies on basalts were carried out in
order to constrain the tectonic setting of formation of the studied basalt-chert sequences. Nine sections were sampled to
the East of Ankara and twenty seven samples were collected for biostratigraphic and geochemical analyses.
The oldest radiolarian cherts dated in the present paper are referrable to Late Triassic (Section 6: late Norian) and
are associated with basaltic rocks with OIB character. OIB type volcanic rocks are also found in other sections and are
associated with cherts of Late Jurassic (Section 3: middle-late Oxfordian to late Kimmeridgian-early Tithonian) and
Early Cretaceous (Section 1: late Valanginian to latest Valanginian-earliest Hauterivian) ages.
E-MORB type rocks are associated with radiolarian cherts of Cretaceous age (Section 4: late Barremian and Section
7: Valanginian to middle Aptian-early Albian), whereas the oldest N-MORBs were found in a section of Late Jurassic
age (Section 5: early-early late Tithonian). Other N-MORBs are associated with radiolarian cherts of Early Cretaceous
age (Section 8: late Valanginian-early Barremian). P-MORBs type rocks were found only in a section of Middle
Jurassic age (Section 2: early-middle Bajocian to late Bathonian-early Callovian age).
In this work, we document the occurrence of OIB-type rocks of Late Triassic and of rocks showing different
geochemical affinities (N-, E-, P-MORBs and OIB) generated in the same time span (Middle-Late Jurassic - Early
Cretaceous). N-MORBs are compatible with composition of melts generated by partial melting of a depleted MORB
mantle source. In contrast, OIBs are compatible with partial melting of enriched-type mantle source. E-MORBs may
have derived from mantle source slightly enriched with respect to DMM source, whereas P-MORBs are compatible
with melts generated from a mantle source significantly enriched, compared to DMM.
The chemical differences shown by the distinct rock-types can be related either to differences in source composition
or different tectonic settings of formation, which may have existed during the Late Jurassic - Early Cretaceous time
span
