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Seminar Detail
Iron Isotope Constraints on the Early Redox History of the Oceans
Presenter: Olivier Rouxel ()
February 28, 2005 11:00 AM Pacific
The response of the ocean redox state to the rise of atmospheric oxygen by
ca. 2.3 Ga ago is poorly constrained although deposition of BIFs until ca.
1.8 Ga suggests at least episodical deep ocean anoxia during the
Paleoproterozoic. Since Fe, along with C and S, are coupled with and
maintain the redox state of the surface environment, Fe seawater
concentration and isotopic composition were likely affected by the change in
the redox state of the atmosphere. Here we will present a study of Fe
isotope composition of sedimentary sulfides over geological time and provide
evidence for a change in the ocean Fe cycle at the same time as atmospheric
redox state changed.
We analyzed Fe isotope compositions of ~ 150 pyrites from 20 black shale
units, specifically focusing on Late Archean to Paleoproterozoic time. δ56Fe
values of handpicked sulfides were obtained using a Neptune MC-ICPMS at WHOI
and are reported relative to IRMM-14 with an external precision of 0.1‰. The
emerged general pattern of Fe isotope record allows dividing the Earth's
history into three stages which are strikingly similar to the stages defined
by multiple S isotopes as well as other indicators of the redox state of the
atmosphere and ocean. (1) Stage 1 (>2.8 to 2.3 Ga) is characterized by
highly variable and negative δ56Fe values of pyrite (down to –3.5‰) that are
interpreted to reflect the reservoir effects during partial oxidation of
hydrothermally-derived Fe(II) and precipitation of Fe-oxides. (2) Stage 2
(2.3 to ~1.6 Ga) is characterized by δ56Fe values ranging from -0.3 to 1.2‰
that might be related to the increased effect of sulfide precipitation in a
redox-stratified ocean. (3) Stage 3, from 1.6 Ga through the Phanerozoic, is
characterized by sedimentary pyrite having a limited range of δ56Fe
variations (less than 0.5‰ around igneous value at ~0‰) reflecting the
establishment of an Fe-poor oxygenated ocean.Participation Instructions
Sites who would like to connect via Polycom must notify Diane Hawks at
dhawks@mail.arc.nasa.gov.
The slides from the seminar can be viewed real-time using WebEx at
https://naimeetings.webex.com, click on "Director's Seminar", the password
is 1KFalcon. If you've never joined a WebEx meeting before, please allow an
extra 5-10 minutes to install the plug-in. Explorer is the recommended
browser.
Sites without a Polycom system can listen to the seminar on the telephone
while viewing the slides in WebEx. The NASA Meet-me number for this is
650-604-3393.
Alternatively, participants without a Polycom system can view the webcast
at: http://vanseg-1.arc.nasa.gov/2005/AB050228-01.ram There is a 30 second
delay for the webcast, so viewers will need to advance the slides manually
in WebEx. Questions can be posted in the WebEx chat area to be
answered by Olivier at the end of his talk.December 21, 2007
The Director’s Seminar series features talks from scientists who are invited by the NAI Director to present their research results to the community. A primary goal of the seminars is to encourage interdisciplinary collaboration across NAI teams and within the astrobiology community at large.
Team Overview Seminars describe the work of the fourteen NAI teams and NAI Central. They offer an opportunity to find out more about the science, E/PO and other activities being performed by the NAI teams and the NAI Central office.
The Forum for Astrobiology Research (FAR) provides an opportunity for graduate students to present their research results and to meet as a student community for networking and mutual support.
The University of Washington seminar series is hosted by the NAI Virtual Planetary Lab (VPL) team from the UW campus in Seattle.
