> Oceanography > Issues > Archive > Volume 23, Number 1

2010, Oceanography 23(1):174–175, http://dx.doi.org/10.5670/oceanog.2010.81

SPOTLIGHT 9 | South Chamorro Seamount

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Authors

C. Geoffrey Wheat | Global Undersea Research Unit, University of Alaska Fairbanks, based at Moss Landing, CA, USA

Patricia Fryer | School of Ocean and Earth Science and Technology (SOEST), University of Hawai`i, Honolulu, HI, USA

Ken Takai | Subground Animalcule Retrieval (SUGAR) Project, Frontier Research System for Extremophiles, Japan Agency for Marine-Earth Science and Technology, Yokosuka, Japan

Samuel Hulme | SOEST, University of Hawai`i, Honolulu, HI, USA

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First Paragraph

Sixteen large, active serpentinite mud volcanoes exist in the Mariana forearc, the region of seafloor between the Mariana Trench and the volcanic island arc (Fryer et al., 2006). Up to 50 km in diameter and rising as much as 2.4 km above the surrounding seafloor, these seamounts form as a consequence of subduction processes, which generate deep-seated faults that penetrate the crust and mantle of the overriding Mariana microplate to the depth of the underlying and subducting Pacific Plate (Figure 1). Faults that are observed up to 100 km west of the Mariana trench provide a pathway for the ascent of fluid released from dehydration reactions within the subducting Pacific Plate and for the ascent of ground-up rock fragments. As this fluid upwells, it reacts with the overlying mantle, producing serpentine, hydrogen gas, and alkaline fluids (up to pH 12.5).

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Full Article

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Citation

Wheat, C.G., P. Fryer, K. Takai, and S. Hulme. 2010. Spotlight 9: South Chamorro Seamount. Oceanography 23(1):174–175, http://dx.doi.org/10.5670/oceanog.2010.81.

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