The Role of Ammonia in the Distribution of Volatiles in the Primordial Hydrosphere of Europa

The presence of a hydrosphere on Europa raises questions about its habitability, and studies of its volatile inventory can provide insight into its formation process. Different scenarios suggest that Europa's volatiles could be derived from cometary ices or devolatilized building blocks. The st...

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Main Authors: Alizée Amsler Moulanier, Olivier Mousis, Alexis Bouquet, Christopher R. Glein
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Planetary Science Journal
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Online Access:https://doi.org/10.3847/PSJ/ad9925
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author Alizée Amsler Moulanier
Olivier Mousis
Alexis Bouquet
Christopher R. Glein
author_facet Alizée Amsler Moulanier
Olivier Mousis
Alexis Bouquet
Christopher R. Glein
author_sort Alizée Amsler Moulanier
collection DOAJ
description The presence of a hydrosphere on Europa raises questions about its habitability, and studies of its volatile inventory can provide insight into its formation process. Different scenarios suggest that Europa's volatiles could be derived from cometary ices or devolatilized building blocks. The study of post-accretion processes—in particular, the “open-ocean” phase that likely occurred before the formation of the icy crust—is crucial to distinguishing these origins, as this phase is likely to have influenced the volatile inventory. The abundance of ammonia in Europa's building blocks is also crucial for understanding the composition of its ocean and primordial atmosphere. We aim to investigate the ocean–atmosphere equilibrium during the post-accretion period by varying the ammonia fraction in the atmosphere. Our model evaluates the vapor–liquid equilibrium of water and volatiles, as well as the chemical equilibrium within the ocean, to study Europa's early hydrosphere. We explore two initial conditions: one in which Europa's hydrosphere originates from comet-like building blocks, and another in which it forms in equilibrium with a thick-and-CO _2 -rich atmosphere. In both scenarios, the initial ratio of accreted CO _2 to NH _3 determines the magnitude of their partial pressures in Europa's early atmosphere. If this ratio exceeds a certain threshold (set to 10 ^−4 in this study), the atmosphere will be CO _2 -rich; otherwise, it will be CO _2 -depleted, by multiple orders of magnitude. Overall, our work provides an initial assessment of the distribution of primordial volatiles in Europa's primitive hydrosphere and provides a baseline for interpreting data from the upcoming Europa Clipper mission.
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spelling doaj-art-b502ca42eb8e4e2e8475d206488644c52025-01-02T08:40:26ZengIOP PublishingThe Planetary Science Journal2632-33382025-01-0161110.3847/PSJ/ad9925The Role of Ammonia in the Distribution of Volatiles in the Primordial Hydrosphere of EuropaAlizée Amsler Moulanier0https://orcid.org/0009-0000-7492-1476Olivier Mousis1https://orcid.org/0000-0001-5323-6453Alexis Bouquet2https://orcid.org/0000-0001-8262-9678Christopher R. Glein3Aix-Marseille Université , CNRS, CNES, Institut Origines, LAM, Marseille, FranceAix-Marseille Université , CNRS, CNES, Institut Origines, LAM, Marseille, France; Institut Universitaire de France (IUF) , FranceAix-Marseille Université , CNRS, CNES, Institut Origines, LAM, Marseille, France; Aix-Marseille Université , CNRS, Institut Origines, PIIM, Marseille, FranceSpace Science Division, Space Sector, Southwest Research Institute , 6220 Culebra Road, San Antonio, TX 78238-5166, USAThe presence of a hydrosphere on Europa raises questions about its habitability, and studies of its volatile inventory can provide insight into its formation process. Different scenarios suggest that Europa's volatiles could be derived from cometary ices or devolatilized building blocks. The study of post-accretion processes—in particular, the “open-ocean” phase that likely occurred before the formation of the icy crust—is crucial to distinguishing these origins, as this phase is likely to have influenced the volatile inventory. The abundance of ammonia in Europa's building blocks is also crucial for understanding the composition of its ocean and primordial atmosphere. We aim to investigate the ocean–atmosphere equilibrium during the post-accretion period by varying the ammonia fraction in the atmosphere. Our model evaluates the vapor–liquid equilibrium of water and volatiles, as well as the chemical equilibrium within the ocean, to study Europa's early hydrosphere. We explore two initial conditions: one in which Europa's hydrosphere originates from comet-like building blocks, and another in which it forms in equilibrium with a thick-and-CO _2 -rich atmosphere. In both scenarios, the initial ratio of accreted CO _2 to NH _3 determines the magnitude of their partial pressures in Europa's early atmosphere. If this ratio exceeds a certain threshold (set to 10 ^−4 in this study), the atmosphere will be CO _2 -rich; otherwise, it will be CO _2 -depleted, by multiple orders of magnitude. Overall, our work provides an initial assessment of the distribution of primordial volatiles in Europa's primitive hydrosphere and provides a baseline for interpreting data from the upcoming Europa Clipper mission.https://doi.org/10.3847/PSJ/ad9925Planetary scienceGalilean satellitesOcean-atmosphere interactionsNatural satellite formationEuropa
spellingShingle Alizée Amsler Moulanier
Olivier Mousis
Alexis Bouquet
Christopher R. Glein
The Role of Ammonia in the Distribution of Volatiles in the Primordial Hydrosphere of Europa
The Planetary Science Journal
Planetary science
Galilean satellites
Ocean-atmosphere interactions
Natural satellite formation
Europa
title The Role of Ammonia in the Distribution of Volatiles in the Primordial Hydrosphere of Europa
title_full The Role of Ammonia in the Distribution of Volatiles in the Primordial Hydrosphere of Europa
title_fullStr The Role of Ammonia in the Distribution of Volatiles in the Primordial Hydrosphere of Europa
title_full_unstemmed The Role of Ammonia in the Distribution of Volatiles in the Primordial Hydrosphere of Europa
title_short The Role of Ammonia in the Distribution of Volatiles in the Primordial Hydrosphere of Europa
title_sort role of ammonia in the distribution of volatiles in the primordial hydrosphere of europa
topic Planetary science
Galilean satellites
Ocean-atmosphere interactions
Natural satellite formation
Europa
url https://doi.org/10.3847/PSJ/ad9925
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