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3. EARLY EARTH’S ATMOSPHERE, OCEANS, AND LIFE

3.1 Overview

 
 
Artwork courtesy of NASA.

Knowledge of Earth’s earliest life, and the environment in which it evolved, is incomplete and controversial at the present time. Here, cutting-edge, microscale, isotopic geochemistry (131Xe/136Xe, 18O, 33S, 36S) of Earth’s oldest materials (>4.0 Gyr-old zircon crystals) and Archean (3.9-2.5 Gyr-old) sulfur minerals (sulfides and sulfates) will be used to explore early atmosphere-ocean evolution and sulfur cycling. In addition, proposed theoretical and experimental studies are aimed at understanding the extraordinary gas-phase chemistry responsible for mass-independent isotope effects in oxygen and sulfur compounds. Other advanced geochemical techniques (laser Raman and optical tomography, in-situ carbon isotopic analysis) are to be used to scrutinize the microfossil evidence for Earth's earliest life. The complementary macrofossil evidence (stromatolites) will be assessed through the use of numerical simulations based on the mathematics of condensed matter physics. The pooled results from these disparate studies will provide new information about the antiquity of life on Earth and provide a firm basis for life-detection on other bodies in the Solar System.

3.2 When did Earth become suitable for habitation?
  3.2.1 The age of the atmosphere
  3.2.2 The age of the hydrosphere (and redox state of Earth’s surface)
  3.2.3 The initiation age of the geodynamo
  3.2.4 Measurements of ancient zircons- building the database
3.3 Sulfur cycling on the early Earth
  3.3.1 Ion microprobe measurements of the four stable isotopes of sulfur
  3.3.2 Laboratory experiments and theoretical analysis of the kinetics and photochemistry of mass-independent sulfur isotope effects
3.4 Geochemical context for early life
  3.4.1 Chemical feedbacks
  3.4.2 Abiotic pathways to complex organics
  3.4.3 Role of metals in early biology
  3.4.4 Equilibrium Fe isotope fractionation between Fe2+ and Fe3+ - an experimental approach
3.5 Detection and geochemical characterization of Earth’s earliest life
  3.5.1 How can biogenicity be established?
  3.5.2 Microbial morphology as evidence for early life
  3.5.3 In-situ isotopic analysis
  3.5.4 Molecular composition and geochemical alteration of organic matter
  3.5.5 Quantitative methods for evaluating the biogenicity of fossil stromatolites
3.6 Genomics, geology, and the tree of life
  3.6.1 Mapping microbial metabolisms on to the tree of life
   

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