skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Rare earth element systematics of the chemically precipitated component in Early Precambrian iron formations and the evolution of the terrestrial atmosphere-hydrosphere-lithosphere system

Journal Article · · Geochimica et Cosmochimica Acta; (United States)
;  [1]
  1. Hahn-Meitner-Institut, Berlin (Germany)

The chemically precipitated component in Early Precambrian (> 2.3 Ga) iron formations (IFs) displays (Sm/Yb)[sub CN] < 1 and (Eu/Sm)[sub SN] > 1 which reflects the corresponding ratios of contemporaneous seawater. In conjunction with [epsilon][sub Nd-IF] > [epsilon][sub Nd-shale] this rare earth element (REE) signature reveals that the REE distribution in Early Precambrian IFs must be explained by mixing between a marine bottom and a surface water component, and that the REEs (and by analogy the Fe) cannot be derived from weathering of a continental source. Mixing calculations reveal that (Sm/Yb)[sub CN] in Early Precambrian marine surface waters was significantly lower than it is today. To explain this difference, two mechanisms are discussed on the basis of higher P[sub CO[sub 2]] and lower P[sub O[sub 2]] levels of the Precambrian atmosphere: (1) higher [CO[sub 3][sup 2[minus]]] in Precambrian river and coastal waters and (2) redox cycling of the REEs at an oceanwide chemocline which separated anoxic and oxic water masses. However, these processes are synergetic and could have operated in unison. The REE distribution in Precambrian IFs is described as a result of mixing in a multicomponent system, where high-T and low-T hydrothermal fluids contributed to the marine bottom water, and REE input from the dissolved REE pool in river waters, after some modification in estuaries, dominated the REE distribution in marine surface waters. After mixing of bottom and surface waters, their combined REE load was quantitatively scavenged onto precipitating iron oxihydroxides or iron carbonates and deposited with the chemically precipitated component. After addition of variable amounts of clastic detritus, this eventually resulted in the REE distribution observed in Precambrian IFs. 94 refs., 6 figs., 3 tabs.

OSTI ID:
6085184
Journal Information:
Geochimica et Cosmochimica Acta; (United States), Vol. 57:10; ISSN 0016-7037
Country of Publication:
United States
Language:
English