TY - JOUR
T1 - Multiple parameters enable deconvolution of water-rock reaction paths in low-temperature vent fluids of the Kamaʻehuakanaloa (Lōʻihi) seamount
AU - Milesi, Vincent
AU - Shock, Everett
AU - Seewald, Jeffrey
AU - Trembath-Reichert, Elizabeth
AU - Sylva, Sean P.
AU - Huber, Julie A.
AU - Lim, Darlene S.S.
AU - German, Christopher R.
N1 - Funding Information:
This work was supported by NASA Planetary Science and Technology Through Analog Research (PSTAR) Program (NNH16ZDA001N-PSTAR) grant (16-PSTAR16_2–0011) to Dr D. S. S. Lim, NOAA Office of Ocean Exploration and Research, Ocean Exploration Trust, NOAA-OER grant NA17OAR0110336, NASA Postdoctoral Fellowship and L'Oréal USA For Women in Science Fellowship to E.T.R. This research used samples and data provided by the Ocean Exploration Trust's Nautilus Exploration Program, Cruise NA100. We thank the cruise expedition Leader N. Raineault, the ROV Hercules/Argus team and the crew of the E/V Nautilus for their assistance while at sea. We are grateful to all members of the SUBSEA team and to the team of the Inner Space Center at the University of Rhode Island Graduate School of Oceanography who made this study possible: John A. Breier, Eric Chan, Josh Chernov, Tamar Cohen, Matthew Deans, Angela Garcia, Michelle Hauer, Renato Kane, Shannon Kobs Nawotniak, David Lees, Justin Lowe, Leigh Marsh, Matthew J. Miller, Miles Saunders, Khaled Sharif, Ashley Shields. We thank the reviewers and the associate editor for helpful and insightful reviews. This is SUBSEA Publication Number: SUBSEA-2018-002.
Funding Information:
This work was supported by NASA Planetary Science and Technology Through Analog Research (PSTAR) Program (NNH16ZDA001N-PSTAR) grant (16-PSTAR16_2–0011) to Dr D. S. S. Lim, NOAA Office of Ocean Exploration and Research, Ocean Exploration Trust, NOAA-OER grant NA17OAR0110336, NASA Postdoctoral Fellowship and L’Oréal USA For Women in Science Fellowship to E.T.R. This research used samples and data provided by the Ocean Exploration Trust's Nautilus Exploration Program, Cruise NA100. We thank the cruise expedition Leader N. Raineault, the ROV Hercules/Argus team and the crew of the E/V Nautilus for their assistance while at sea. We are grateful to all members of the SUBSEA team and to the team of the Inner Space Center at the University of Rhode Island Graduate School of Oceanography who made this study possible: John A. Breier, Eric Chan, Josh Chernov, Tamar Cohen, Matthew Deans, Angela Garcia, Michelle Hauer, Renato Kane, Shannon Kobs Nawotniak, David Lees, Justin Lowe, Leigh Marsh, Matthew J. Miller, Miles Saunders, Khaled Sharif, Ashley Shields. We thank the reviewers and the associate editor for helpful and insightful reviews. This is SUBSEA Publication Number: SUBSEA-2018-002.
Publisher Copyright:
© 2023 Elsevier Ltd
PY - 2023/5/1
Y1 - 2023/5/1
N2 - The contribution of venting fluids at mid-ocean ridges to global ocean biogeochemical cycles is well recognized. Less is known about the role of magmatically-active intra-plate volcanoes. In this study, new compositional fluid data were acquired from 20 to 50 °C vent fluids at Kamaʻehuakanaloa (previously known as Lōʻihi) seamount (Hawai'ian archipelago) and used to model the wide diversity of reaction conditions capable of producing the Fe-, Si- and CO2-rich vent fluids observed. Our conceptual model includes a first step where seawater reacts with increasing proportions of basalt and gas as the temperature increases, and a second step where the resulting hydrothermal fluid mixes with unaltered seawater while continuing to react with basalt until the fluid mixture reaches 20 °C. A series of reaction paths were chosen to vary: the maximum temperature during Step 1 (50 to 400 °C) and the proportions of basalt and gas reacting; the degree, F, of low-temperature basalt alteration during Step 2, which corresponds to the extent to which the hot fluid generated during Step 1 continues to react with more basalt as it ascends to the seafloor. Our model shows that the 20–50 °C vent fluids are greatly dependent on the degree of low-temperature basalt alteration during fluid upwelling. Indeed, the compositions of Kamaʻehuakanaloa vent fluids cannot be reconciled with a general model of subsurface mechanical mixing of high-temperature end-member vent fluid and seawater alone. Instead, they require both subsurface equilibrium mixing between a ≥350 °C hydrothermal fluid end-member and seawater and further basalt alteration that must occur as the fluid mixture rises to the seafloor. Although it involves only ∼4% of the amount of basalt having reacted during Step 1, this low-temperature basalt alteration during Step 2 leads to the characteristic enrichments in Fe observed in the Kamaʻehuakanaloa vent fluids and a concomitant depletion in H2S. We hypothesize that low-temperature basalt alteration during an extended path of fluid upwelling through the subseafloor might arise as a direct consequence of the height and steep-sloped topography of Kamaʻehuakanaloa seamount. If correct, this suggests a more general case - that input from magmatically-active intraplate volcanoes, which have been relatively overlooked throughout the history of submarine vent investigations to date, could differ significantly from global mid-ocean ridge fluxes and contribute more substantially than previously recognized to the global ocean Fe cycle.
AB - The contribution of venting fluids at mid-ocean ridges to global ocean biogeochemical cycles is well recognized. Less is known about the role of magmatically-active intra-plate volcanoes. In this study, new compositional fluid data were acquired from 20 to 50 °C vent fluids at Kamaʻehuakanaloa (previously known as Lōʻihi) seamount (Hawai'ian archipelago) and used to model the wide diversity of reaction conditions capable of producing the Fe-, Si- and CO2-rich vent fluids observed. Our conceptual model includes a first step where seawater reacts with increasing proportions of basalt and gas as the temperature increases, and a second step where the resulting hydrothermal fluid mixes with unaltered seawater while continuing to react with basalt until the fluid mixture reaches 20 °C. A series of reaction paths were chosen to vary: the maximum temperature during Step 1 (50 to 400 °C) and the proportions of basalt and gas reacting; the degree, F, of low-temperature basalt alteration during Step 2, which corresponds to the extent to which the hot fluid generated during Step 1 continues to react with more basalt as it ascends to the seafloor. Our model shows that the 20–50 °C vent fluids are greatly dependent on the degree of low-temperature basalt alteration during fluid upwelling. Indeed, the compositions of Kamaʻehuakanaloa vent fluids cannot be reconciled with a general model of subsurface mechanical mixing of high-temperature end-member vent fluid and seawater alone. Instead, they require both subsurface equilibrium mixing between a ≥350 °C hydrothermal fluid end-member and seawater and further basalt alteration that must occur as the fluid mixture rises to the seafloor. Although it involves only ∼4% of the amount of basalt having reacted during Step 1, this low-temperature basalt alteration during Step 2 leads to the characteristic enrichments in Fe observed in the Kamaʻehuakanaloa vent fluids and a concomitant depletion in H2S. We hypothesize that low-temperature basalt alteration during an extended path of fluid upwelling through the subseafloor might arise as a direct consequence of the height and steep-sloped topography of Kamaʻehuakanaloa seamount. If correct, this suggests a more general case - that input from magmatically-active intraplate volcanoes, which have been relatively overlooked throughout the history of submarine vent investigations to date, could differ significantly from global mid-ocean ridge fluxes and contribute more substantially than previously recognized to the global ocean Fe cycle.
KW - Active intraplate volcano
KW - Fluid geochemistry
KW - Geochemical modeling
KW - Hydrothermal vents
KW - Low-temperature vent fluids
KW - Ocean Fe budget
KW - Water-rock reactions
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U2 - 10.1016/j.gca.2023.03.013
DO - 10.1016/j.gca.2023.03.013
M3 - Article
AN - SCOPUS:85150031243
SN - 0016-7037
VL - 348
SP - 54
EP - 67
JO - Geochmica et Cosmochimica Acta
JF - Geochmica et Cosmochimica Acta
ER -