A fluid flow perspective on the diagenesis of Te Aute limestones

Abstract

Pliocene cool‐water, bioclastic Te Aute limestones in East Coast Basin, New Zealand, accumulated either in shelfal shoal areas or about structurally shallow growth fold structures in the tectonically active accretionary forearc prism. Up to five stages of carbonate cementation are recognised, based on cement sequence‐stratigraphic concepts, that formed on the seafloor during exposure of the limestones before burial, during burial, uplift, and deformation. Two principal fluid types are identified—topography‐driven meteoric fluids and compaction‐driven fluids. We have developed conceptual and quantitative models that attempt to relate the physical characteristics of fluid flow to the cement paragenesis. In particular, we have simulated the effects of uplift of the axial ranges bordering East Coast Basin in terms of the degree of penetration of a meteoric wedge into the basin. The dynamics of meteoric flow changed dramatically during uplift over the last 2 m.y. such that the modelled extent of the meteoric wedge is at least 40 km across the basin, and the penetration depth 1500 m or more corresponding with measured freshwater intersections in some oil wells. Cement‐fluid relationships include: (1) true marine cements that precipitated in areas remote from shallow freshwater lenses; (2) pre‐compaction cements that formed in shallow freshwater lenses beneath limestone “islands” (3) post‐compaction cements derived from compaction‐driven flow during burial; (4) early uplift‐related fracture‐fill cements formed during deformation of the accretionary prism and uplift of the axial ranges; and (5) late uplift‐related cements associated with uplift into a shallow meteoric regime.

Keywords:

• diagenesis
• cement sequence
• meteoric wedge
• topography‐driven flow
• freshwater lens
• compaction
• modelling
• Te Aute limestones
• Pliocene‐Pleistocene
• New Zealand