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The aim of the programme isto coordinate and encourage research on theenvironment of the early Earth and on the mannerin which life appeared and evolved. The mainresearch topics are:
(a) Composition and temperature of Archean atmosphere and oceans;
(b) The nature of Archean landmasses;(c) Interaction between Archean surface waters and
the oceanic and continental crust;(d) The nature and evolution of early life.
Activities
(a) Organization of workshops and sessions atconferences;
(b) Exchange visits of scientists and studentsbetween participating universities
(c) Promotion of a program of scientific drilling inthe 3.5 Ga Barberton belt, South Africa
Aims of the Barberton
Drilling Program
The aim of the project is to drill several shallow diamond
holes (100-500m) in the Barberton greenstone belt
• to obtain continuous drill-core through sections ofvolcanic and sedimentary rocks,
• to analyze these samples (petrology, paleontology,magnetic properties, geochemistry),
• to gain a better understanding of the conditions at thesurface of the Archean Earth, the geodynamics of theArchean crust and mantle, and the emergence andevolution of life
Why drill the volcanic rocks?
• To obtain a thick section (300-500m?) through a series ofkomatiitic and basaltic units
• To sample complete sections through individual flows andtheir contacts
• To obtain fresh samples for complete mineralogical andgeochemical analysis
• To help understand the volcanic component of early crustan essential feature of the Archean surface environment;.
• Information relevant to origin of life as well as for Archeangeodynamic processes.
hydrated upper crustgabbroolivine cumulate
6 km
0°C
1200°C
Gradient = 200°C/km
Modern oceanic crusthydratedupper crust
gabbro
olivinecumulate
30 km
0°C
1500°C
Gradient = 50°C
/km
Archean oceanic crust
Archean oceanic crust is thickand composed of low-densitycomponents; the basal parts,which might be in the garnetstability field, do not containgarnet … how did it subduct?
Modern oceanic crust is thin andcool; it converts to eclogite to dragdown subducting plates
Archeanhydrothermalsystems
• On land - mafic and felsic“continents”• In the oceans - at ridges and onmargins of volcanic plateaux
But …What was the temperature and the
compositions of ocean water andhydrothermal fluids?
What was the typical water depth?What was the geometry and scale
of hydrothermal circulation?What was the composition of
oceanic crust and how did it behavein a subduction zone?
Banded Iron Formation
Proterozoic 2.4 Ga
Archean 3.5 Ga
Magnetite (Fe304)
Hematite (Fe203) and chert
Biogeochemical goal:
Evolution of metabolism
What do we want to know?
- Nature of early microbial life
- Environments/ habitats where early microbes thrived
- Diversity of ancient microbial populations
Emergence of specific metabolisms remains unclear
e.g. oxygenic photosynthesis
stromatolite and isotope evidence are conflicting!
Limited by poor constraints on:
- Atmospheric evolution
- Early Archean ocean chemistry
- Biochemical vs inorganic controls on chemical/isotopic tracers
1. Origine (s) de la vie :
- La terre primitive
• Quelle est la chronologie de l’évolution de la t erre primitive (continents, océans,atmosphère, vie ?)
• Quelles sources endogènes de matière carbonée pour la chimie prébiotique ?• Quelles traces des sources hydothermales et d’une éventuelle synergie avec l’apport
extraterrestre de molécules organiques/matière carbonée ?• la nature de la croûte et le flux de chaleur à traverse la croûte ?• la nature et quantité de croûte « continentale » ?• les océans – pH, composition, oxydation ?• le flux de corps extraterrestres – est-ce qu’il y a eu une période de bombardement tardive
catastrophique, capable de détruire la vie si elle était déjà présente?• le flux des UV jusqu’à la surface de la Terre et l ’influence éventuelle sur une vie
« surficielle » ?
- La chimie prébiotique
• Quelle est la contribution effective des apports extraterrestres à la chimie prébiotique ?- Les molécules provenant du milieu interstellaire ont-elles été efficacement transmisesdans le système solaire primitif ?
- Quelle est la nature/quantité de molécules d’origine cométaire et/ou astéroïdale ayant atteintla terre ?
Why drill the sedimentary rocks?
1. Access to well-preserved continuous
sequences, including rocks that do
not outcrop well
2. To obtain ‘unaltered’ samples
3. Integrate approaches in
multidisciplinary program e.g. with
palaeomagnetic data that require
access to intact geomagnetic field
http://www.ipgp.jussieu.fr/pages/020204.php
Key lithological targets
Metasedimentary sequences- Silicified sandstones, siltstones, mudstones, conglomerates- Grey or black shales- Cherts- Tidal sequences- Barite/sulfide associations
Specific objectives
1. Types of microbial habitat
2. Types of metabolism and activity of
microorganisms
3. Origin of silicification
4. Sedimentology in absence of
vegetation
5. Dynamics of Earth-Moon system
6. Rate and consequences of meteorite
impacts
Methods
Micropaleontology
High resolution scanning SEM; TEM;
synchrotron techniques; microRaman;
nanoSIMS
Stable isotope geochemistry
C, N, O, S, Fe, Si, Se
Ar-Ar geochronology and noble gas studies
Paleomagnetism
Name Institute Discipline Name Institute DisciplineTraces of early life Volcanic rocks
Emmanuelle Javaux University of Liège, Belgium Biogeochemistry David Banks University of Leeds, UK Hydrothermal processesRicardo Amils Universidad Autonoma de Madrid Biogeochemistry Adam Kent Oregon State University, USA Komatiites and melt inclusionsChris Vasconcelos ETH Zurich, Switzerland Biogeochemistry and sediments Alex Sobolev Vernadsky Institute, Moscow, Russia Komatiites and melt inclusionsJudith Mckenzie ETH Zurich, Switzerland Biogeochemistry and sediments Nick Arndt Universite Grenoble, France KomatiitesPascal Philippot IPG Paris, France Geochemistry and geology Allan Wilson University Witwatersrand, South Africa KomatiitesBéatrice Luais CRPG Nancy, France Isotope geochemistry Euan Nisbet University of London, UK Komatiites and traces of lifeBernard Marty CRPG Nancy, France Isotope geochemistry Jesse Dann KomatiitesPieter Vroon Utrecht University, Netherlands Isotope geochemistry Mike Lesher Laurentian University, Canada Komatiites and ore depositsMark van Zuilen IPG Paris, France Isotope geochemistry Richard J. Walker DTM Washington, USA Komatiites -isotope geochemistryPaul Mason Utrecht University, Netherlands Isotope geochemistry and biogeochemistry Steve Shirey DTM Washington, USA Komatiites -isotope geochemistryMartin van Kranendonk Geological Survey Western Australia Isotope geochemistry and geology Wolf Maier University Western Australia KomatiitesMinik Rosing Geologisk Museum, Copenhagen Isotope geochemistry and geology Mathinus Cloete Council of Geosciences, South Africa Volcanics and tectonicsRoger Buick Washinton University, USA Isotope geochemistry and geologyManfred van Bergen Utrecht University, Netherlands Isotope geochemistry and geologyMichael Bau International University Bremen, Germany Isotope geochemistry and geologyCharles Cockell Open University, UK Traces of life - impactsFrances Westall Centre Biophysique Moléculaire, Orleans, FrancePaleontology
Sedimentary rocks Other disciplinesTanja Zegers Utrecht University, Netherlands Life and traces of life Francis Albarede ENS Lyon, France GeochemistryWlady Altermann Universitaet Munich, Germany Sedimentology Jan Kramers Universitaet Berne, Switzerland GeochemistryKen Eriksson Virginia Polytechnic Institute, USA Sedimentology Janne Blichert-Toft ENS Lyon, France GeochemistryNora Noffke Virginia Polytechnic Institute, USA Sedimentology Klaus Mezger Universitaet Munich, Germany GeochemistryBeate Orberger Université Paris sud, France Sediments - geochemistry Marian Tredoux University Free State, South Africa GeochemistryWolf Mueller University Quebec, Canada Sediments & komatiites Alfred Kroener Universitaet Mainz, Germany GeologyDon Lowe Stanford University, USA Sediments & spherules Carl Anhaeusser University Witwatersrand, South Africa GeologyGary Byerly University Louisiana, USA Sediments and komatiites Lew Ashwal University Witwatersrand, South Africa GeologyPat Eriksson University of Pretoria, South Africa Sediments and tectonics Paul Dirks University Witwatersrand, South Africa Geology, tectonicsAxel Hofmann University of Natal, South Africa Sediments geochemistry Thierry Augé BRGM, Orleans, France Ore depositsJens Gutzmer University Witwatersrand, South Africa Sediments geochemistry Chris Ballhaus Universitaet Muenster, Germany PetrologyMartin Whitehouse Swedish Museum of Natural History Sediments geochemistry Alex Kisters Stellenbosch University, South Africa TectonicsNic Beukes University Witwatersrand, South Africa Sediments geochemistry Gary Stevens Stellenbosch University, South Africa TectonicsWout Nijman Utrecht University, Netherlands Sediments geochemistry Annika Dziggel Universitaet Aarchen, Germany TectonicsBruce Simonson Oberlin College, USA Spherules and impacts Michael Meyer Universitaet Aarchen, Germany Tectonics, ore depositsUlrich Riller Humboldt-Universität, Berlin, Germany Spherules and impactsUwe Reimold Humboldt-Universität, Berlin, Germany Spherules and impacts
Budget: ca. 300 kEuros for 3000 m of drill core
Support from:
CNRS, ANR, CNES
European funding agencies - DFG, NERC, NWO, ESA …
NSF
Agouran foundation, minerals industry
The International Team involved in the Barberton Drilling Project
Meetings to Plan the Project
• October 16, 2006 - Johannesburg: Preliminarymeeting with South African participants
• December 11, 2006 - AGU San Francisco:Meeting with North American participants andNSF
• Late January, 2007 - Germany:Meeting with European participants
Please let me know if you wish to attend eithermeeting!