The Payas region bauxite deposits occur as a sandwiched layer that is a few kilometers long and an average of 10 m thick between the lower and upper Cretaceous carbonates of the Arabian Platform. The bauxites occur as blanket and pocket types, are chemically and texturally homogeneous and have a thrust structure with ophiolitic mélange formations. The bauxite varies in color, from reddish-brown to grayish-green to black, and has a massive, patchy and very rare oolitic-pisolitic texture. The bauxite mainly consists of diaspore, hematite, rutile, anatase, rare kaolinite, boehmite and pyrite minerals. Prismatic and lath-shaped euhedral rutile within the bauxites indicates in situ formation of the bauxites from Ti-rich basaltic pyroclastics. The chondrite-normalized REE pattern of the bauxite is similar to the basalt pattern and has a very weak Eu anomaly (0.9). Two groups of elements have been enriched in the Payas region bauxite: the first group contains TiO 2 (9.67 wt%), Cr (752 ppm), V (617 ppm) and Ni (72 ppm), and the second group comprises Zr (993 ppm), Nb (86 ppm) and Sn (7 ppm). These two groups of element enrichment indicate that the parental material of bauxite has an alkali basalt character. The carbon and oxygen isotope stratigraphy throughout the carbonate section from the bottom to the top indicates that the climate was warm during bauxitization (mean δ 18 O VPDB :-6.15‰) and relatively cold after bauxite deposition (mean δ 18 O VPDB :-4,71‰). A marine regression during the warm climate could be related to the uplifting of the coastal zone, which is linked to vertical fault movements of normal faults. A rapid transgression after bauxite formation during the cold climate period can be explained by subsidence of the continental margin, which is associated with episodic ophiolitic nappe loading during the closure of the Neotethyan Ocean in the region.