Parameter Space Exploration of Low-to-moderate-temperature Hydrothermal Systems on Ocean Worlds Using a Monte Carlo Framework

Abstract We explore the hydrogeologic and physical conditions necessary to sustain hydrothermal activity within the shallow subseafloors of ocean worlds, exploring wide ranges of multiple parameters using a Monte Carlo framework. We apply multiple analytical calculations to represent coupled fluid-thermal flow systems, as have been observed on Earth, using idealized representations that link lateral transport below a conductive boundary layer between sites of hydrothermal inflow (recharge) and outflow (discharge). These analytical calculations replicate outcomes and trends in results generated from more complex numerical simulations once we account for excess driving pressure that is consumed by secondary (local) convection during transport within the subseafloor. We investigate low heat flux scenarios that are expected to be limiting cases for sustaining hydrothermal flows (≤10 mW m −2 ) for which there is modest heating from radiometric decay and/or tidal dissipation within the interior of an ocean world. We explore limiting conditions appropriate for Europa’s deep subseafloor, and a subset of sustainable hydrothermal siphon calculations are identified that are especially efficient for mining interior heat. We identify parameters that can sustain a hydrothermal siphon for reaction temperatures of 80°C–120°C and water/rock mass ratios of ≤100 Gy –1 . These conditions should result in discharging fluids that are altered relative to inflowing water and a silicate interior that is more likely to retain the potential for geochemical reactions over geologic time. These conditions are of particular interest because they could help create habitable conditions below or at the seafloor of an ocean world and can provide a foundation for linked reaction modeling.

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Publication Details

Journal
The Planetary Science Journal
Published
2025-09-01
DOI
https://doi.org/10.3847/psj/adf558
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
0.00

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article

Parameter Space Exploration of Low-to-moderate-temperature Hydrothermal Systems on Ocean Worlds Using a Monte Carlo Framework

Ryunosuke Akiba, Andrew T Fisher
The Planetary Science Journal
Astro and Planetary Science
article

Parameter Space Exploration of Low-to-moderate-temperature Hydrothermal Systems on Ocean Worlds Using a Monte Carlo Framework

Ryunosuke Akiba, Andrew T Fisher
article en

Abstract

Abstract We explore the hydrogeologic and physical conditions necessary to sustain hydrothermal activity within the shallow subseafloors of ocean worlds, exploring wide ranges of multiple parameters using a Monte Carlo framework. We apply multiple analytical calculations to represent coupled fluid-thermal flow systems, as have been observed on Earth, using idealized representations that link lateral transport below a conductive boundary layer between sites of hydrothermal inflow (recharge) and outflow (discharge). These analytical calculations replicate outcomes and trends in results generated from more complex numerical simulations once we account for excess driving pressure that is consumed by secondary (local) convection during transport within the subseafloor. We investigate low heat flux scenarios that are expected to be limiting cases for sustaining hydrothermal flows (≤10 mW m −2 ) for which there is modest heating from radiometric decay and/or tidal dissipation within the interior of an ocean world. We explore limiting conditions appropriate for Europa’s deep subseafloor, and a subset of sustainable hydrothermal siphon calculations are identified that are especially efficient for mining interior heat. We identify parameters that can sustain a hydrothermal siphon for reaction temperatures of 80°C–120°C and water/rock mass ratios of ≤100 Gy –1 . These conditions should result in discharging fluids that are altered relative to inflowing water and a silicate interior that is more likely to retain the potential for geochemical reactions over geologic time. These conditions are of particular interest because they could help create habitable conditions below or at the seafloor of an ocean world and can provide a foundation for linked reaction modeling.

The Planetary Science JournalVol. 6(9)
University of California, Santa Cruz (US)
National Aeronautics and Space Administration
Openalex Percentile: Top 84%
Astro and Planetary Science
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