Oxygen isotopes in sedimentary rocks have long been used to reconstruct paleo-surface temperatures. Chert, a microcrystalline form of SiO2, has also been explored as a paleotemperature proxy, but the factors controlling its isotopic composition remained uncertain. A recent numerical model of silica diagenesis has now linked chert oxygen-isotope ratios directly to paleo-heat flow, opening new opportunities for its application [1].
Diagenetic chert forms when amorphous silica (opal-A) dissolves and reprecipitates, passing through an opal-CT intermediate before becoming microcrystalline quartz. The oxygen-isotope ratios (δ18O, Δ′17O) in the resulting chert capture the temperature and fluid composition at the depth of the opal-CT to quartz transition. By simulating that diagenetic transition, the new model relates δ18Ochert and Δ′17Ochert to burial temperatures, pore fluid alteration and heat flow.
We use the model to reconstruct paleo-heat flow during prograde silica phase transformation and derive burial rates and pore fluid alteration across the Rhenohercynian basin. Our data reveal paleo-heat flow in the order of 50 to 70 mW m-2, agreeing with a previous model [2] and high burial rates in the east of up to 80 m Myr-1, agreeing with the thickness of overlying turbidites. Burial rates and clay mineral content coincide with 18O-depleted compositions of cherts, i.e compositions in three isotope space that deviate from the expected temperature-equilibrium. This dataset lays the foundation for a new tool to study the thermal- and burial histories of sedimentary basins.
[1] Tatzel, et al. (2022) PNAS 119
[2] Littke et al. (2000) Geol. Soc. Spec. Publ. 179