@article{c59845379de242999135ead3ab31e9ce,
title = "Forward geochemical modeling as a guiding tool during exploration of sea cliff hydrothermal field, Gorda Ridge",
abstract = "Maximizing scientific return is critical to the success of space exploration. During the SUBSEA project, which explored the Sea Cliff vent site aboard the E/V Nautilus as an analog for hydrothermal systems on Ocean Worlds, we used forward geochemical modeling to guide decision-making during the process of exploration. Before the expedition, we performed 1670 reaction-path calculations to simulate water-rock interactions during hydrothermal circulation covering wide ranges of reaction conditions to predict the diversity of possible chemical compositions and energy available for chemosynthetic microorganisms at the Sea Cliff vents. Calculation of the information entropy of predicted concentrations of major solutes and pH allowed us to identify dissolved silica as the chemical species capable of yielding the most information about reaction conditions; as such, the measurement of this parameter was implemented aboard ship for our field program. Using telepresence, results of onboard chemical analyses of fluid samples collected during seafloor Dive n were sent to our shore-based scientific team, who processed the data and used the outcomes to inform the design of Dive n + 2. Combining data processing with forward modeling revealed, within just two dives, that all the observed fluids venting from 10 °C to 300 °C most likely resulted from simple conservative mixing between seawater and a common hydrothermal fluid end-member: the result of reaction of seawater with basalt at ≥350 °C. Identification of these reaction conditions early within the cruise allowed additional calculations to be performed to quantify the energy available from redox disequilibria as a function of vent-fluid temperatures as they exited the seafloor. These calculations can help inform and optimize real-time microbiological sampling and culture experiments onboard the ship during field expeditions. The success of our approach coupling forward modeling and onboard ship analyses allowed improved efficiency in completing process studies at the Sea Cliff vent site, providing time for further exploration and sampling of a newly discovered vent site: Apollo. This study demonstrates a novel application of forward and real-time modeling for scientific exploration that allows the time required for result-informed decision making to be reduced from years to hours – an essential breakthrough for future space exploration missions.",
keywords = "E/V nautilus, Forward geochemical modeling, Information entropy, NASA PSTAR, Ocean exploration, Ocean worlds analog, Telepresence",
author = "Vincent Milesi and Everett Shock and Tucker Ely and Megan Lubetkin and Sylva, {Sean P.} and Huber, {Julie A.} and Smith, {Amy R.} and Nawotniak, {Shannon Kobs} and Zara Mirmalek and German, {Christopher R.} and Lim, {Darlene S.S.}",
note = "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 and NOAA-OER grant NA17OAR0110336 . This research used samples and data provided by the Ocean Exploration Trust{\textquoteright}s Nautilus Exploration Program, Cruise NA108. 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, Sarah Hu, Renato Kane, David Lees, Justin Lowe, Leigh Marsh, Matthew J. Miller, Miles Saunders, Khaled Sharif, Ashley Shields. We are especially thankful to Ashley Shields and Angela Garcia who played key roles in discovering the Apollo vent-site. We thank David A. Clague who generously provided us with pre-publication maps of the Sea Cliff area. We are indebted to Jordyn Robare and James Andrew Leong from the GEOPIG group at the Arizona State University for their tremendous help in developing and implementing the Si measurements onboard ship. We thank the anonymous reviewers for helpful and insightful reviews. This is SUBSEA Publication Number: SUBSEA-2018-001. 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 and NOAA-OER grant NA17OAR0110336. This research used samples and data provided by the Ocean Exploration Trust's Nautilus Exploration Program, Cruise NA108. 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, Sarah Hu, Renato Kane, David Lees, Justin Lowe, Leigh Marsh, Matthew J. Miller, Miles Saunders, Khaled Sharif, Ashley Shields. We are especially thankful to Ashley Shields and Angela Garcia who played key roles in discovering the Apollo vent-site. We thank David A. Clague who generously provided us with pre-publication maps of the Sea Cliff area. We are indebted to Jordyn Robare and James Andrew Leong from the GEOPIG group at the Arizona State University for their tremendous help in developing and implementing the Si measurements onboard ship. We thank the anonymous reviewers for helpful and insightful reviews. This is SUBSEA Publication Number: SUBSEA-2018-001. Publisher Copyright: {\textcopyright} 2020 Elsevier Ltd",
year = "2021",
month = mar,
doi = "10.1016/j.pss.2020.105151",
language = "English (US)",
volume = "197",
journal = "Planetary and Space Science",
issn = "0032-0633",
publisher = "Elsevier Limited",
}