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research article

H-2-rich fluids from serpentinization: Geochemical and biotic implications

Meibom, A.  
•
Fridriksson, T.
•
Coleman, R.G.
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2004
Proceedings Of The National Academy Of Sciences Of The United States Of America (PNAS)

Metamorphic hydration and oxidation of ultramafic rocks produces serpentinites, composed of serpentine group minerals and varying amounts of brucite, magnetite, and/or FeNi alloys. These minerals buffer imetamorphic fluids to extremely reducing conditions that are capable of producing hydrogen gas. Awaruite, FeNi3, forms early in this process when the serpentinite minerals are Fe-rich. Olivine with the current mantle Fe/Mg ratio was oxidized during serpentinization after the Moon-forming impact. This process formed some of the ferric iron in the Earth's mantle. For the rest of Earth's history, serpentinites covered only a small fraction of the Earth's surface but were an important prebiotic and biotic environment. Extant methanogens react H-2 with CO2 to form methane. This is a likely habitable environment on large silicate planets. The catalytic properties of FeNi3 allow complex organic compounds to form within serpentinite and, when mixed with atmospherically produced complex organic matter and waters that circulated through basalts, constitutes an attractive prebiotic substrate. Conversely, inorganic catalysis of methane by FeNi3 competes with nascent and extant life.

  • Details
  • Metrics
Type
research article
DOI
10.1073/pnas.0405289101
Web of Science ID

WOS:000223694700010

Author(s)
Meibom, A.  
Fridriksson, T.
Coleman, R.G.
Bird, D.K.
Sleep, N.H.
Date Issued

2004

Publisher

National Academy of Sciences

Published in
Proceedings Of The National Academy Of Sciences Of The United States Of America (PNAS)
Volume

101

Start page

12818

End page

12823

Subjects

Zambales Ophiolite

•

Thermodynamic Properties

•

Abiogenic Methane

•

Hydrogen Gas

•

Earths Crust

•

Philippines

•

Carbon

•

Mantle

•

Ridge

•

Atmosphere

Editorial or Peer reviewed

REVIEWED

Written at

OTHER

EPFL units
LGB  
Available on Infoscience
May 15, 2012
Use this identifier to reference this record
https://infoscience.epfl.ch/handle/20.500.14299/80377
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