The thermal structure and thickness of continental roots

We compare heat flow data from the Precambrian shields in North America and in South Africa. We also review data available in other less well-sampled Shield regions. Variations in crustal heat production account for most of t he variability of the heat flow. Because of this variability, it is difficu lt to define a single average crustal model representative of a whole tecto nic province. The average heat flow values of different Archean provinces i n Canada, South Africa, Australia and India differ by significant amounts. This is also true for Proterozoic provinces. For example, the heat flow is significantly higher in the Proterozoic Namaqua-Natal Belt of South Africa than in the Grenville Province of the Canadian Shield (61 vs. 41 mW m(-2) o n average). These observations indicate that it is mot possible to define s ingle value of the average heat flow for all provinces of the same crustal age. Large amplitude short wavelength variations of the heat flow suggest t hat most of the difference between Proterozoic and Archean heat flow is of crustal origin. In eastern Canada, there is no good correlation between the local values of heat flow and heat production. In the Archean, Proterozoic and Paleozoic provinces of eastern Canada, heat flow values through rocks with the same heat production are not significantly different. There is the refore no evidence for variations of the mantle heat flow beneath these dif ferent provinces. After removing the local crustal heat production from the surface heat flow, the mantle (Moho) heat flow was estimated to be between 10-15 mW m(-2) in the Archean, Proterozoic and Paleozoic provinces of east ern Canada. Estimates of the mantle heat flow in the Kaapvaal craton of Sou th Africa may be slightly higher (approximate to 17 mW m(-2)). Large-scale variations of bulk crustal heat production are well-documented in Canada an d imply significant differences of deep lithospheric thermal structure. In thick lithosphere, surficial heat flow measurements record a time average o f heat production in the lithospheric mantle: and are not in equilibrium wi th the instantaneous heat production. The low mantle heat flow and current estimates of heat production in the lithospheric mantle do not support a me chanical (conductive) lithosphere thinner than 200 km and thicker than 330 km. Temperature anomalies with surrounding oceanic mantle extend to the con vective boundary layer below the conductive layer, and hence to depths grea ter than these estimates. Mechanical and thermal stability of the lithosphe re require the mantle part of the lithosphere to be chemically buoyant and depleted in radiogenic elements. Both characteristics are achieved simultan eously by partial melting and melt extraction. (C) 1999 Published by Elsevi er Science B.V. All rights reserved.