Abstract
The evolution and extinction of life are tied intimately to the oxygen state of the ocean, and particularly to the presence of anoxic and H 2S-containing (euxinic) water on a global scale. Anoxia and euxinia were more common in the past, relative to today's <0.5% euxinic seafioor. We are able to constrain the distributions of these conditions through a combination of indirect numerical modeling methods and more direct geochemical proxies, with particular emphasis on Fe-S-Mo analysis of flne-grained siliciclastic rocks for the latter. Establishing the spatiotemporal pattern of oceanic redox is more difficult with very old rocks because of the limited availability of well-dated, well-preserved materials that span shallow and deep environments across time lines. Despite these difficulties, the multiple approaches synthesized in our case study point to global oxygen-deficiency in the deep ocean and perhaps euxinia during most, if not all, of the Proterozoic and likely extending into the early Paleozoic.
Original language | English (US) |
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Pages (from-to) | 507-534 |
Number of pages | 28 |
Journal | Annual Review of Earth and Planetary Sciences |
Volume | 37 |
DOIs | |
State | Published - May 2009 |
Keywords
- Anoxia
- Fe and Mo isotopes
- Fe-S-Mo paleoredox proxies
- Ocean chemistry
- Proterozoic
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Earth and Planetary Sciences (miscellaneous)
- Space and Planetary Science