Formation of mixed-layer sulfide-hydroxide minerals from the Tochilinite-Valleriite group during experimental serpentinization of olivine

Author:

McCollom Thomas M.1ORCID,Hoehler Tori2,Fike David A.3,Houghton Jennifer L.3,Bell Aaron4,Klein Frieder5,Moskowitz Bruce6,Solheid Peter6

Affiliation:

1. Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, Colorado 80309, U.S.A.

2. NASA Ames Research Center, Moffett Field, California 94035 U.S.A.

3. Department of Earth and Planetary Sciences, Washington University in St. Louis, St. Louis, Missouri 63130, U.S.A.

4. Department of Geological Sciences, University of Colorado, Boulder, Colorado 80309, U.S.A.

5. Department of Marine Chemistry and Geochemistry, Woods Hole Oceanographic Institution, Woods Hole, Massachusetts 02543, U.S.A.

6. Department of Earth and Environmental Sciences and Institute for Rock Magnetism, University of Minnesota, Minneapolis, Minnesota 55455, U.S.A.

Abstract

Abstract We report the formation of minerals from the tochilinite-valleriite group (TVG) during laboratory serpentinization experiments conducted at 300 and 328 °C. Minerals in the TVG are composed of a mixture of sulfide and hydroxide layers that can contain variable proportions of Fe, Mg, Cu, Ni, and other cations in both layers. Members of this group have been observed as accessory minerals in several serpentinites, and have also been observed in association with serpentine minerals in meteorites. To our knowledge, however, TVG minerals have not previously been identified as reaction products during laboratory simulation of serpentinization. The serpentinization experiments reacted olivine with artificial seawater containing 34S-labeled sulfate, with a small amount of solid FeS also added to the 300 °C experiment. In both experiments, the predominant reaction products were chrysotile serpentine, brucite, and magnetite. At 300 °C, these major products were accompanied by trace amounts of the Ni-bearing TVG member haapalaite, Ni,Fe-sulfide (likely pentlandite), and anhydrite. At 328 °C, valleriite occurs rather than haapalaite and the accompanying Ni,Fe-sulfide is proportionally more enriched in Ni. Reduction of sulfate by H2 produced during serpentinization evidently provided a source of reduced S that contributed to formation of the TVG minerals and Ni,Fe-sulfides. The results provide new constraints on the conditions that allow precipitation of tochilinite-valleriite group minerals in natural serpentinites.

Publisher

Mineralogical Society of America

Subject

Geochemistry and Petrology,Geophysics

Reference57 articles.

1. Sulfur in serpentinized oceanic peridotites: Serpentinization processes and microbial sulfate reduction;Alt;Journal of Geophysical Research,1998

2. Occurrence and composition of tochilinite and related minerals in Site 1068 serpentinites;Beard;Proceedings of the Ocean Drilling Progam, Scientific Results,2000

3. A fossil, serpentinization-related hydrothermal vent, Ocean Drilling Program, Leg 173, Site 1068 (Iberia Abyssal Plain): Some aspects of mineral and fluid chemistry;Beard;Journal of Geophysical Research,2000

4. Hydrothermal chemistry of seawater from 25 degrees to 350 degrees C;Bischoff;American Journal of Science,1978

5. Crystal-field properties of Fe in brucite Mg(OH)2;Blaauw;Physica status solidi (b),1979

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