Quantifying the formation and evolution of the Archaean lithospheric mantle

Introduction

The formation of the Archean lithosphere was a key event in Earth history, resulting in the construction of the first continents, or cratons. The lithosphere formed by extensive mantle melting; however, there are conflicting models for the environment in which melting took place.

Challenges in Understanding Lithosphere Formation

Efforts to understand the formation of the cratonic lithosphere are hampered by a lack of quantitative information on:

• The depth of mantle melting
• The original thickness of the Archean lithosphere

Exsolved orthopyroxenes within peridotite xenoliths and silicate inclusions in diamond hold the key to constraining these critical parameters.

Research Approach

We will reconstruct the original compositions of an extensive collection of exsolved orthopyroxenes and use our recently published thermodynamic model to calculate their formation pressures and temperatures. This innovative approach will reveal the depth extent of Archean melting.

Constraints on Lithosphere Extent

We will provide the first constraints on the vertical extent of the lithosphere in the Archean using geothermal gradients calculated from dated diamond inclusions. To achieve this, we will perform cutting-edge laser ablation U-Pb dating of garnet inclusions. This challenging application has yielded promising results for xenolithic garnet.

Experimental Methods

Observations will be complemented by new experiments using:

1. Fertile compositions
2. Depleted compositions
3. Silica-enriched compositions

These will be coupled with thermodynamic modeling, which will lead to a better understanding of phase relations during peridotite melting.

Investigating Silica Enrichment

The origin and significance of silica enrichment is poorly understood. We will conduct melt-rock reaction experiments to test the hypothesis that silica addition occurred via interaction with ascending komatiite melt.

Fundamental Issues Addressed

We will thus address several fundamental issues:

• The depth of Archean mantle melting
• The origin of silica enrichment
• The link between cratonic peridotite and komatiite magma

Conclusion

LITHO3 will provide unprecedented insight into the formation and evolution of the cratonic lithosphere.