Campanian lacustrine organic-rich
mudstones were deposited under
a warm greenhouse climate in Egypt. In this study, integrated elemental
geochemical analyses have been applied to discriminate the paleoweathering
conditions, provenance, and tectonic setting of these mudstones. The
studied samples are relatively enriched in Al, Ca, V, Sc, and Cr compared
to Post-Archean Australian shales (PAAS). Their chondrite normalized
REE patterns show enrichment in the light REE compared to heavy REE,
with a negative Eu anomaly (Eu/Eu* = ∼0.77). The low values
of Th/Sc (0.42), Zr/Sc (5.05), and Zr/Hf (36.3) for the studied samples
indicate no input from recycled older sedimentary strata. The ratios
of the compositional variability index (ICV = 0.76), K/Al
(0.072), Al/Si (0.34), and K/Si (0.025) suppose that the mudstones
are compositionally mature source rocks and originated in quiescent
and low energy depositional environments. The average values of the
chemical index of alteration (CIA = 82), chemical proxy of alteration
(CPA = 94), and plagioclase index of alteration (PIA = 87) and ln(Al2O3/Na2O = 3.6) for the studied mudstones
imply moderate to intensive chemical weathering. Moreover, the provenance
sensitive elemental proxies (e.g., La/Sc, Th/Sc, Th/Cr, Cr/Th) and
multiple discrimination diagrams reveal that the mudstones could be
derived from intermediate igneous parent rocks. The lacustrine organic-rich
sediments were sourced from a Phanerozoic to Proterozoic arc setting
based on various tectonic discrimination diagrams.