Paper No. 3
Presentation Time: 2:10 PM
ABRUPT RISE IN PALEOPROTEROZOIC O2 AND GLOBAL MICROBIAL SULFATE REDUCTION
The
inhibition, rise, and maintenance of atmospheric O2 each represent a
distinct mode of the evolving relationship between geological processes and
microbial activity on Earth. This
presentation will focus on sulfur isotopic evidence from Paleoproterozoic
sedimentary rocks for the rise of O2.
A
first-order similarity exists between S isotopic anomalies preserved in some
Archean rocks and those associated with short-wavelength UV photochemistry of
SO2 (Farquhar et al., 2001). The Archean environment, therefore,
likely permitted production and preservation of the isotopic signatures of
UV-driven SO2 photochemistry.
In particular, photochemical models indicate that only O2
levels below 10-5 PAL allow preservation of S isotopic anomalies
(Pavlov and Kasting, 2002). This
implies that sulfur isotopic anomalies are a low resolution but high
sensitivity proxy for O2.
In
the Transvaal Supergroup, South Africa, S isotopic anomalies are found in the
~2.46 Ga Kuruman Iron Fm. (33S anomalies from -2 to +2 per mil off
of predictions from a reference mass-dependent fractionation relationship),
while the ~2.32 Rooihoogte and Timeball Hill Fms. preserve 33S
abundances within -0.1 to 0.3 per mil of mass dependence (Bekker et al.,
2004). A significant threshold in
O2 abundance must have been crossed sometime between ~2.45 and ~2.32
Ga. In the Transvaal Basin, this
interval encompasses the Duitschland Fm., and we measured S isotopic
compositions of carbonate-associated sulfate (CAS) and acid-volatile S (AVS)
from this formation in order to more precisely define the nature of the
Paleoproterozoic rise in O2.
The
lower Duitschland Fm. preserves significant 33S isotopic anomalies
in both CAS (up to 0.8 ä) and AVS (up to 1.4 ä). In contrast, CAS from the upper Duitschland Fm. has 33S
abundances within 0.0 and 0.2 per mil of mass dependence. This shift mimics the gross S isotopic
transition that has been identified in Paleoproterozoic rocks (Farquhar et al,
2001; Bekker et al., 2004; Papineau et al., 2005) but occurs here over ~200 m
of section. Importantly, 34S
abundances in CAS jump by up to ~30 per mil when sizable 33S
anomalies disappear. This
dichotomy suggests that an abrupt re-organization of the S cycle accompanied
the rise of O2, and may imply an extreme sensitivity of the
Paleoproterozoic atmosphere to microbial and geologic forcings.