Sa. Gibson et al., LATE CRETACEOUS RIFT-RELATED UPWELLING AND MELTING OF THE TRINDADE STARTING MANTLE PLUME HEAD BENEATH WESTERN BRAZIL, Contributions to Mineralogy and Petrology, 126(3), 1997, pp. 303-314
High mantle potential temperatures and local extension, associated wit
h the Late-Cretaceous impact of the Trindade mantle plume, produced su
bstantial widespread and voluminous magmatism around the northern half
of the Parana sedimentary basin. Our previous studies have shown that
, above the central and eastern portions of the postulated impact zone
where lithosphere extension is minimal, heat conducted by the plume c
aused large-scale melting of the more fusible parts of the subcontinen
tal lithospheric mantle beneath the margin of the Sao Francisco craton
and the surrounding Brasilia mobile belt. Here we combine geochemical
data and field evidence from the Poxoreu Igneous Province, western Br
azil to show how more intense lithospheric extension above the western
margin of the postulated impact zone permitted greater upwelling and
melting of the Trindade plume than further east. Laser Ar-40/Ar-39 age
determinations indicate that rift-related basaltic magmas of the Poxo
reu Igneous Province were emplaced at similar to 84 Ma. Our detailed g
eochemical study of the mafic magmas shows that the parental melts und
erwent polybaric crystal fractionation within the crust prior to final
emplacement. Furthermore, some magmas (quartz-normative) appear to ha
ve assimilated upper crust whereas others (nepheline- and hypersthene-
normative) appear to have been unaffected by open-system crustal magma
chamber processes. Incompatible trace element ratios (e.g. chondrite-
normalised La/Nb = 1) and isotopic ratios (Sr-87/Sr-86 = 0.704 and Nd-
143/Nd-144 = 0.51274) of the Hy-normative basalts resemble those of oc
eanic islands (GIB). We therefore propose that these ''OIB-like'' magm
as were predominantly derived from convecting-mantle-source melts (i.e
. Trindade mantle plume). Inverse modelling of rare-earth element (REE
) abundances suggests that the initial melts were predominantly genera
ted within the depth range of similar to 80-100 km, in mantle with a p
otential temperature of similar to 1500 degrees C.