National Aeronautics and Space Administration
+ NASA Homepage
+ NASA en Español
+ NAI en Español
GO!
Section

This site is no longer maintained. It contains historical data.

For current information about the NASA Astrobiology Institute, please visit http://astrobiology.nasa.gov/nai/

NASA Astrobiology Institute
About NAI Teams Focus Groups Events & Seminars Education Funding Tools Directory
Home Member Portal Executive Council Website
Astrobiology Drilling Program

DTDP Drilling Plans


Drilling Coordinators: R. Buick, J. S. R. Dunlop, A. D. Anbar
Hamersley_small

Click here to enlarge image.

The Deep Time Drilling Program collaborators (DTDP) plan to drill 3 diamond drill cores in the Pilbara Craton during 2004, including two co-operative efforts with the Archean Biosphere Drilling Project. The holes will penetrate:

  • 1000 metres of the lower Hamersley – upper Fortescue Groups (~2.47-2.70 Ga) through the Archean-Proterozoic boundary, sampling banded iron formation, kerogenous shales, basinal carbonates, shallower cherts and clastics, and several meteorite impact horizons;
  • 500 metres of the Warrawoona and upper Coonterunah Groups (~3.45-3.52 Ga) through the world’s oldest unconformity, sampling pillowed basalts, tuffaceous cherts, evaporitic carbonates, quartz sandstones and kerogenous cherts; and

    Tumbiana_small

    Click here to enlarge image.

  • 300 metres into the Tumbiana Formation (~2.71 Ga), sampling lacustrine lapilli tuffs and stromatolitic carbonates.

    Drilling will be performed under clean conditions, avoiding organic lubricants and pressure-packing some samples under inert gas to avoid hydrocarbon contamination and evaporation. Samples will be released to the wider astrobiological community after a year.

    The most significant potential scientific outcomes are:
  • the confirmation of the indigenous nature of Archean hydrocarbon biomarker molecules, which have been cited as evidence for the early existence of eukaryotic organisms;
  • CoonterunahWarrawoona

    Click here to enlarge image.

    the discovery of an ancient paleosol beneath the Warrawoona-Coonterunah unconformity, possibly constraining the greenhouse-gas composition of the atmosphere at a time of weaker solar luminosity; and
  • a full biogeochemical inventory of the ocean-atmosphere system shortly before the early Paleoproterozoic glacial and oxygenation events.

    It is envisaged that these holes will start an extended program drilling critical stratigraphic intervals throughout the Precambrian around the world to resolve astrobiological questions constrained by poor sample availability.

    This project also involves the Geological Survey of Western Australia, Randolph Resources, Hamersley Iron, SIPA Resources International, and the University of Western Australia. Drilling will be funded by the NASA Astrobiology Institute as part of the Astrobiology Drilling Program.

     

  • Hamersley Drill-Core Science Motivations and Plans


    Lead Investigators: A. D. Anbar, R. Buick, A. J. Kaufman, A. H. Knoll, T. W. Lyons, R. Summons
    Hamersley_strat_small

    Click here to enlarge image.

    We plan integrated geological, paleobiological and geochemical examination of the Hamersley-Fortescue Archean sediment drill-core that will be obtained in the summer of 2004 by the Astrobiology Drilling Program. Funding for this analytical work is being sought from the National Science Foundation (Geology & Paleontology program). The general motivation of the proposed research is to characterize the nature of life and its environment in the late Archean, shortly before the rise of atmospheric oxygen. Many workers are examining the timing of this redox transition and its relationship to contemporaneous climatic oscillations that may include global ice ages. Our interest, somewhat different but complementary, is to understand how the Archean biosphere set the stage for this singular environmental transformation. Specifically, our major goal is to characterize the relative importance of different types of microbes in late Archean marine environments and, through lithofacies relationships, to study the environmental controls on their distributions. We will achieve this goal through integrated examination of hydrocarbon molecular biomarkers, redox indicators and biogeochemical cycling in kerogenous sediments. Additional goals are to characterize the status of major biogeochemical cycles in the late Archean and generate a robust baseline for future investigations by conducting sedimentological and biogeochemical reconnaissance of the entire core. Collectively, this work will test the hypothesis that oxygen-generating cyanobacteria and aerobic microorganisms were present in Archean ecosystems and that the environmental imprints of these metabolisms remained muted for hundreds of millions of years after their origins.



    Credits Feedback Related Links Sitemap
    FirstGov
    + Freedom of Information Act
    + Budgets, Strategic Plans and Accountability Reports
    + The President's Management Agenda
    + NASA Privacy Statement, Disclaimer,
    and Accessibility Certification

    + Inspector General Hotline
    + Equal Employment Opportunity Data Posted Pursuant to the No Fear Act
    + Information-Dissemination Priorities and Inventories
    National Aeronautics and Space Administration

    NASA Official: Wendy Dolci
    + Comments and Questions
    + XML Stay Updated with RSS Feeds