A ROLE FOR LOWER CONTINENTAL-CRUST IN FLOOD-BASALT GENESIS - ISOTOPICAND INCOMPATIBLE ELEMENT STUDY OF THE LOWER 6 FORMATIONS OF THE WESTERN DECCAN TRAPS
Zx. Peng et al., A ROLE FOR LOWER CONTINENTAL-CRUST IN FLOOD-BASALT GENESIS - ISOTOPICAND INCOMPATIBLE ELEMENT STUDY OF THE LOWER 6 FORMATIONS OF THE WESTERN DECCAN TRAPS, Geochimica et cosmochimica acta, 58(1), 1994, pp. 267-288
Flows of the lower six formations of the western Deccan Traps (Jawhar
through Khandala) cover a range epsilon(Nd)(T) from 0 to -20, (Sr-87/S
r-86)T from 0.7062 to 0.7128, and Pb-206/Pb-204 from 16.72 to 22.43. O
xygen isotopic data for fresh clinopyroxene and plagioclase separates
indicate magmatic deltaO-18 values between +6.6 and +7.4 parts per tho
usand. Previous isotopic studies of the upper four formations (Bushe t
hrough Mahabaleshwar) have revealed two major trends that, to a first
approximation, correspond to variable contamination of epsilon(Nd)(T)
greater-than-or-equal-to +7 source magmas by two very different negati
ve epsilon(Nd) lithospheric endmembers. Isotopic data for the lower si
x formations describe completely different arrays from those of the up
per formations, and the fields for the individual lower formations are
also distinct from one another. Significantly, the lower formation ar
rays overlap at or converge toward a common range of isotopic signatur
es, with epsilon(Nd)(T) almost-equal-to 0.0 to -5.5, (Sr-87/Sr-86)T al
most-equal-to 0.7067 to 0.7085, and Pb-206/Pb-204 almost-equal-to 19.2
to 20.9. These values are unlike those of oceanic mantle, and interme
diate between the extremes defined by the little-contaminated Ambenali
and highly crustally contaminated Bushe formations in the upper part
of the stratigraphic sequence. One explanation for this common signatu
re is that it represents a mantle source located in the continental li
thosphere, and quite distinct from the Ambenali-like source dominating
the upper formations. However, the incompatible element patterns of t
he common-signature (and other lower formation) samples do not resembl
e those of typical Proterozoic or Phanerozoic continental mantle xenol
iths and, unlike the Ambenali basalts, all of the lower formation samp
les analyzed to date have significantly higher delta O-18 values than
oceanic lavas or the great majority of continental lithospheric mantle
xenoliths. An alternative possibility is that the common signature ma
gmas could be the products of a large-scale, open-system, lower crusta
l contamination process similar to that postulated for the thick mafic
complex in the Ivrea Zone of northern Italy. If so, then the isotopic
arrays emanating from the common signature would represent secondary
contamination episodes involving at least three different crustal endm
embers. In the upper formations, a two-stage mixing process also appea
rs necessary to account for the Pb-Nd and Pb-Sr isotopic relationships
displayed by data for the Bushe and Poladpur formations. Model calcul
ations indicate that incompatible element patterns and isotopic ratios
similar to those of the common-signature samples can be produced, whi
le still maintaining a basaltic major and compatible trace element com
position, by mixing a large-degree partial melt (approximately 40%) of
Indian Archean basic amphibolite into Ambenali-type or Reunion-type p
rimitive magma. With the particular amphibolite composition used, the
proportion of contamination required is large: roughly 10-30%, compara
ble to the amounts proposed for the mafic complex in the Ivrea Zone. M
ore siliceous contaminants permit smaller amounts of contamination but
generally yield poorer trace element fits.