C. Villaseca et al., A re-examination of the typology of peraluminous granite types in intracontinental orogenic belts, T RS EDIN-E, 89, 1998, pp. 113-119
Citations number
51
Categorie Soggetti
Earth Sciences
Journal title
TRANSACTIONS OF THE ROYAL SOCIETY OF EDINBURGH-EARTH SCIENCES
Conventional rock classification diagrams do not distinguish the variety of
peraluminous rock series. Moreover, peraluminous granite types have not be
en clearly discriminated in recent revisions. The study of several peralumi
nous series in different intracontinental orogenic belts reveals that four
distinct groups can be defined. Using an A-B diagram, these four groups are
: (I)highly peraluminous granitoids (hP) characterised by high A values and
typified by an increase in peraluminosity toward the most mafic varieties;
(2) moderately peraluminous granitoids (mP) which occupy the intermediate
field and generally show increasing peraluminosity towards the most felsic
varieties; (3) low peraluminous granitoids (lP) which plot in the lowest pa
rt of the peraluminous field defining negative slope trends; (4) highly fel
sic peraluminous granites (fP) with poorly defined variation trends.
In intracontinental orogenic belts, the genesis of peraluminous granitic se
ries is favoured by the abundance of fertile crustal protoliths, mainly met
apelites, metaigneous rocks and metagreywackes. The difficulty of attaining
temperatures in excess of 950 degrees C at lower crustal levels during the
tectonothermal evolution of thickened crust, inhibits the partial melting
of more basic sources. Although the physical parameters of the melting proc
ess influence their chemical and mineralogical characteristics, source rock
composition ultimately determines the degree of peraluminosity of the gran
itic series.