Abstract
The great variety and abundance of chert deposits in Archean terrains constitute one of the most unusual features that mark Earth's early geological history. Proposed explanations for their origin largely relying on field observations, trace element patterns, or oxygen isotope signatures have not yielded an encompassing model. Here we document silicon isotope systematics in cherts from 3.5-3.0 Ga units in the Pilbara Craton (Western Australia) as evidence of their formation by several distinct processes in Early Archean near-surface environments. Our δ
| Original language | English |
|---|---|
| Pages (from-to) | 939-942 |
| Journal | Geology |
| Volume | 35 |
| DOIs | |
| Publication status | Published - 2007 |