z-logo
open-access-imgOpen Access
EVOLUTION AND ORIGIN OF THE MARONIA PLUTON, THRACE, GREECE
Author(s) -
Lambrini Papadopoulou,
G. Christofides,
C. Koroneos,
Michael Bröcker,
Τ. Σολδάτος,
Georgios K. Eleftheriadis
Publication year - 2004
Publication title -
bulletin of the geological society of greece
Language(s) - English
Resource type - Journals
eISSN - 2529-1718
pISSN - 0438-9557
DOI - 10.12681/bgsg.16754
Subject(s) - pluton , geology , geochemistry , partial melting , fractional crystallization (geology) , mantle (geology) , gneiss , group (periodic table) , subduction , tectonics , chemistry , metamorphic rock , paleontology , organic chemistry
The Maronia pluton is the youngest of the Tertiary plutons that occurred in Thrace. Three rock groups have been distinguished: a basic, an intermediate and an acid one. Based on geochemical and isotopic characteristics, the basic group probably represents a magma that isotopically equilibrated with the intermediate group at a certain point of its evolution. The evolution of the intermediate group can be described by an assimilation-fractional crystallization process (AFC). The acid group represents crustal melts that are not genetically related to the basic and intermediate groups. The emplacement of the pluton is related to post-collisional extension resulting from the subduction of the African under the European plate. The magma source of the basic and intermediate group is considered to be a LILE- and LREE-enriched subcontinental lithospheric mantle. The acid group has probably derived by the partial melting of crustal rocks and in particular, gneiss.

The content you want is available to Zendy users.

Already have an account? Click here to sign in.
Having issues? You can contact us here
Accelerating Research

Address

John Eccles House
Robert Robinson Avenue,
Oxford Science Park, Oxford
OX4 4GP, United Kingdom