Abstract

Hydrogen gas is seeping from the sedimentary basin of São Franciso, Brazil. The seepages of H2 are accompanied by helium, whose isotopes reveal a strong crustal signature. Geophysical data indicates that this intra-cratonic basin is characterized by (i) a relatively high geothermal gradient, (ii) deep faults delineating a horst and graben structure and affecting the entire sedimentary sequence, (iii) archean to paleoproterozoïc basements enriched in radiogenic elements and displaying mafic and ultramafic units, and (iv) a possible karstic reservoir located 400 m below the surface. The high geothermal gradient could be due to a thin lithosphere enriched in radiogenic elements, which can also contribute to a massive radiolysis process of water at depth, releasing a significant amount of H2. Alternatively, ultramafic rocks that may have generated H2 during their serpentinization are also documented in the basement. The seismic profiles show that the faults seen at the surface are deeply rooted in the basement, and can drain deep fluids to shallow depths in a short time scale. The carbonate reservoirs within the Bambuí group which forms the main part of the sedimentary layers, are crossed by the fault system and represent good candidates for temporary H2 accumulation zones. The formation by chemical dissolution of sinkholes located at 400 m depth might explain the presence of sub-circular depressions seen at the surface. These sinkholes might control the migration of gas from temporary storage reservoirs in the upper layer of the Bambuí formation to the surface. The fluxes of H2 escaping out of these structures, which have been recently documented, are discussed in light of the newly developed H2 production model in the Precambrian continental crust.

Highlights

  • The natural production of molecular hydrogen has drawn increasing scientific attention due to the central role this molecule plays in fueling the deep subsurface biosphere or promoting the abiotic synthesis of organic molecules (Truche et al, 2020 [1])

  • Natural hydrogen sources have been identified for several decades in seafloor hydrothermal vents, and hyperalkaline springs in ophiolite massifs

  • Other analyses of gas sampled at the surface, from the head of the exploration wells drilled in the São Francisco basin confirmed that, besides high concentrations of H2, He (>1%) is present, in association with methane-dominated hydrocarbons and N2 (Flude et al, 2019 [17])

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Summary

Introduction

The natural production of molecular hydrogen (hereafter hydrogen or H2 ) has drawn increasing scientific attention due to the central role this molecule plays in fueling the deep subsurface biosphere or promoting the abiotic synthesis of organic molecules (Truche et al, 2020 [1]). Natural H2 sources may represent a new attractive primary carbon free energy resource (Smith, 2002 [2]; Smith et al, 2005 [3]; Truche and Bazarkina, 2019 [4]; Gaucher, 2020 [5]). This latter industrial perspective has motivated recent H2 exploration studies in ophiolite, peralkaline, Precambrian shields and intra-cratonic geological settings (see review by Zgonnik, 2020 [6]). Carolina Bay in the US (Zgonnik et al, 2015 [13]) These surface features are the only evidence used to detect these H2 seepages. We review the different layers of information that compose a supposed H2 system in this basin and lay the foundation of a H2 exploration guide

The São Francisco Basin
A Possible Deep Origin for H2
Production of H2 by Water Radiolysis
Production of H2 by Serpentinization or Hydration
Presence of Ultramafic Rocks
Magnetometric
Temperature Ranges at Depth
Possible H2 Bubbling at Depth
Accumulation
Putting It All Together: A Potential H2 System within the São Francisco Basin
Conecputal
Findings
Conclusions

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