Introduction

Hydrothermal venting in the ocean occurs along slow- to fast-spreading segments of the 60,000 km-long global system of mid-ocean ridges (MOR)1. Most spreading segments feature rocks of basaltic composition, and the chemistry of basalt-hosted vent fluids (cf2,3,4,5.) has been shown to be primarily controlled by (1) reaction-zone depth and temperature6,7, (2) the extent of water-rock interactions5, and (3) phase separation of the seawater-derived fluids8,9. Hydrothermal processes along the 17,000 km-long ultraslow-spreading MOR are generally more varied and vent fluids exhibit a wider range of compositions10. With discontinuous divergence and alternating magmatic and tectonic accretion, the interplay between tectonics and magmatism results in the exhumation of ultramafic rocks11. Accordingly, hydrothermal fluids alternately interact with both mafic and ultramafic lithologies12,13. The variable influence of serpentinization reactions in ultramafic rocks, leads to variably H2-enriched and Si- and H2S-depleted vent fluids as seen in the Lost City14,15, Rainbow16, Logatchev17 and Kairei12,13 vent fields. Similarly, MOR near continental margins are buried below terrestrial sediments, which affect hydrothermal vent fluid compositions. Syn-sedimentary volcanic activity interlayers basement rocks and sediments, causing diverse fluid compositions through alternating fluid-basement and fluid-sediment interactions18,19,20. In these settings gas composition in vent fluids is dominated by volcanic exhalation as shown in the Jade site21,22 or controlled by thermal degradation of organic matter contained in sediments as suggested for the CLAM site21,22. Additionally, microbial processes in sediments can generate CH4 and alter hydrocarbon composition to varying degrees, either when fluids heat up in the hydrothermal recharge zone or mix and cool in the discharge zone, as demonstrated in vent areas of the Okinawa Trough23,24 and the Juan de Fuca Ridge25. Nevertheless, thermal degradation of sedimentary organic matter remains the dominant control on vent fluid compositions in many sediment-associated vent fields, such as Guaymas Basin19,26, Escabana Trough27, and Loki’s Castle28, where it also produces alkalinity through sulfate reduction29. Consequently, compared to basalt-hosted systems, vent fluids affected by sediment interactions typically exhibit lower metal contents, higher pH and alkalinity, as well as elevated concentrations of CO2, CH4, H2 and other hydrocarbons. Their carbon isotope signatures and hydrocarbon ratios provide important constraints on the origin of these compounds in sediment-associated hydrothermal systems.

The 500 km-long Knipovich Ridge, as part of the Arctic Mid-Ocean Ridges30, extends from the Molloy Fracture Zone in the north to the Mohns Ridge in the south (Fig. 1a). It represents a unique geological setting, where ultraslow spreading coincides with proximity to the continental margin and terrestrial sediment deposition. Spreading initiated during the opening of the Fram Strait31,32 around 20 Ma ago and occurs in an ultraslow, asymmetric, oblique mode. Spreading rates decrease from 15.1 to 14.0 mm yr−1 northward as asymmetry increases. Here, divergence is highly oblique, with an angle of 40–53° between the ridge and the spreading direction, leading to a reduced spreading rate perpendicular to the ridge axis33. Teleseismic data and ocean bottom seismometers34,35 indicate that magmatic activity is concentrated in magmatically robust zones like the Logachev Volcanic Center (the most prominent volcanic center along the Knipovich Ridge36), which are interspersed with magmatically starved sections characterized by deeper hypocenters and aseismic behavior. While detachment faulting has not been documented along most of the Knipovich Ridge35,37, it dominates in the north, where magma supply and spreading rates are lowest37.

Fig. 1: Location and geological setting of the Jøtul hydrothermal field.
Fig. 1: Location and geological setting of the Jøtul hydrothermal field.
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a Overview of the Norwegian-Greenland Sea (Esri GEBCO basemap) with main ridge segments (red lines, dashed line: inactive) and transform faults (black lines). AR Aegir Ridge, JMFZ Jan Mayen Fracture Zone, JMR Jan Mayen Ridge, LT Lena Trough, KnR Knipovich Ridge, KoR Kolbeinsey Ridge, MhR Mohns Ridge, MR Molloy Ridge, MFZ Molloy Fracture Zone, SFZ Spitsbergen Fracture Zone. b Location of Jøtul hydrothermal field at the eastern flank of the rift valley close to the Brøgger AVR (Axial Volcanic Ridge). Ship-based multibeam bathymetry aquired during cruise MSM10946. Dashed white and black lines mark the boundaries of the rift valley floor and the Brøgger AVR, respectively. c High-resolution (AUV-derived46) bathymetry map of the fluid sampling sites in the Jøtul hydrothermal field (red stars), seafloor observations (white dots, S3a-S3d) and soapstone sample (black dot, GeoB20526-2). Maps in this figure were created using ArcGIS® software by Esri. d Conceptual schematic profile of the tectonic, lithological and hydrothermal framework below the Jøtul hydrothermal field. The sampled vents are enumerated as following: (1) Nidhogg and (2) Yggdrasil, (3) Fenris, and (4) Gyme. The black dot shows the location of soapstone GeoB25026-2 (metasomatized peridotite, c.f. c Given slopes represent averaged seafloor slopes measured from the bottom of the rift valley floor to the vent site (5°) and from the vent site to near the ridge crest in the east (13°).

The Jøtul hydrothermal field at the northern Knipovich Ridge was discovered in 2022 during the research expedition with R/V MARIA S. MERIAN (MSM10938) and is situated east of the Brøgger Axial Volcanic Ridge (AVR, Fig. 1b). Located ~5 km from the ridge axis, it sits amidst numerous normal faults39 on a sediment-covered neovolcanic high at the eastern boundary of the rift graben. Sediments along the Knipovich Ridge consist of a mixture of transported terrigeneous and pelagic components and contain higher amounts of organic matter. Surface sediment samples collected on the central Knipovich Ridge ~45 km south of the Jøtul hydrothermal field show concentrations of total organic carbon (TOC) of 0.2–1 wt.%40 and it was suggested that the organic matter in these sediments originated from coastal areas around Svalbard. Sediments from western Svalbard fjords (Kongsfjorden, Adventfjorden, Hornsund) have high contents of both biogenic and terrestrial components and contain 1.1–2.1 wt.% TOC41. However, due to the proximity of the Jøtul field to the limits of the Eurasian ice sheets during the last glacial period42, its location near the present maximum sea ice extent43, and the predominant south-to-north flow direction of the West Spitsbergen Current44, the mentioned fjords may not represent the exclusive source regions of the sedimentary organic matter.

Hydrothermal activity at the Jøtul hydrothermal field includes two black smokers, named Fenris and Gyme45 (Fig. 1c, Supplementary Table S1, Supplementary Fig. S2a–d), and two structures releasing clear, shimmering fluids from flanges and fissures, named Yggdrasil and Nidhogg46 (Supplementary Table S1, Supplementary Fig. S2e–h). All of them are hosted in larger sulfide mounds that crop out of the surrounding sediments (Supplementary Fig. S3a–b) and have been subject to a certain degree of mass wasting (Supplementary Fig. S3c). Sporadically exposed pillow basalts near the vent field (Supplementary Fig. S3d) suggest locally thin sediment cover or syn-sedimentary volcanic activity.

At the location of the vent field the seafloor slope is dipping westwards and changes from dipping ~5° west of the vent field, to ~13° east of the vent field (Fig. 1d). This seafloor morphology may indicate emplacement of the vent field adjacent to the emergence zone of a westward-dipping detachment fault, which bounds the rift graben in the west and a NE-SW striking ridge east of the vent field. Indeed, such a change in seafloor slope may be typical for detachment faulting and mark the transition between the hanging wall cutoff and the corrugated surface of the exposed footwall47. The western flank of the ridge in the east is interpreted to represent the uplifted footwall of this westward-dipping detachment fault (Fig. 1d). Samples of soapstone (Supplemenary Fig. S4, Supplementary Table S5) recovered only 100 m east of Yggdrasil38 support this interpretation (Fig. 1c, d). Soapstones are silica-metasomatized ultramafic rocks, and high Ni and Cr concentrations in the bulk rock analyses (Supplementary Table S5) indicate that the precursor rock was probably a mantle peridotite. Both, a low-angle seafloor slope and occurrence of (altered) ultramafic rocks have mainly been described along detachment footwalls48,49 and are supported by geodynamic numerical models that involve mixed tectonic and magmatic accretion50,51,52.

During expedition MSM109 in 2022 fluid samples were collected for the first time from hydrothermal vents in the Jøtul field46. However, the fluid samplers (KIPS; Kiel Pumping System) used were not gas-tight, so the concentrations of dissolved gases represent minimum values. Exceptionally high CH4 concentrations of up to 5 μM in the non-buoyant plume above the vent field46 suggested even higher CH4 concentrations in the vent fluids than reported previously. During expedition MSM13145 in 2024, isobaric gas-tight (IGT) fluid samplers53 were used to re-sample the hydrothermal vents at the Jøtul field. The recently aquired fluid samples have higher CH4 concentrations and are less diluted with seawater. In this publication, we report concentrations of dissolved volatiles, major fluid compositions, and stable isotope ratios from these gas-tight vent fluid samples and discuss the subsurface processes driving the formation of these particularly volatile-rich fluids.

Results and discussion

Vent fluid compositions and hydrothermal endmember

The hydrothermal fluids sampled (Supplementary Table S6, Supplementary Table S7) vented with temperatures of 214–314 °C (Fig. 2a). Low Mg and SO4 concentrations (<4.1 mM and <2.9 mM) indicate that seawater entrained during sampling was minor and that endmember hydrothermal fluids are essentially free of Mg and SO4. Vent fluid endmembers (Table 1) were calculated using a mass balance two-component mixing model, assuming a Mg-free hydrothermal endmember fluid as experimentally determined54. Since the samples were vent fluid-dominated, the measured and calculated compositions closely match. Endmember temperatures were derived using isenthalpic-isobaric mixing models (Supplementary Fig. S8) based on thermodynamic data of the H2O-NaCl system55. These temperatures slightly exceed measured temperatures, ranging from 223 °C at Nidhogg to 297–318 °C at the other three vents. The fluid compositions are typical of sediment-hosted hydrothermal systems, having elevated pH (Fig. 2b), alkalinity (3.5–4.6 mM) and NH4+ concentrations (1.7–5.3 mM) and low metal contents (Fe: <33 µM, Mn: <0.21 mM) compared to basalt-hosted systems. Noticeably, CH4 concentrations (49.7–66.3 mM) are the highest ever reported for mid-ocean ridge hydrothermal fluids (Fig. 2c) and with CO₂ concentrations of 36.0–41.6 mM both values far exceed those from the diluted, and partly degassed KIPS samples recovered in 202246.

Fig. 2: Vent fluid data from samples of the Jøtul hydrothermal field in the context of mid-ocean ridge hydrothermal fluids.
Fig. 2: Vent fluid data from samples of the Jøtul hydrothermal field in the context of mid-ocean ridge hydrothermal fluids.
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af Mg concentrations vs temperature, pH, CH4, Cl, H2 and H2S. Most chemical parameters for the Jøtul fluids plot in the typical range of sediment-hosted vent fluids (pH, CH4), while others plot in the range rather typical of ultramafic-hosted (mostly peridotite) vent fluids (H2S, H2). Compositions of Loki’s Castle and Guaymas Basin vent fluids (sediment-hosted) are highlighted in orange. Compositions of Rainbow and Logatchev vent fluids (ultramafic-hosted) are denoted in dark green. Data for comparison is from MARHYS database58,59.

Table 1 Calculated zero-Mg endmember compositions for isobaric-gas-tight fluid samples from individual orifices in the Jøtul hydrothermal field

The δ¹³C values of CH₄ (–32.3 to –31.9‰) closely match extrapolated endmembers from samples recovered in 2022, while δ¹³C-CO₂ values (–11.7 to –10.7‰) and δ2H-H₂ values (–425.2 to –372.9‰) from the Jøtul fluids are reported for the first time. These carbon isotope ratios along with molecular compositions of light hydrocarbons (C1/(C2–C3)) provide insights into carbon sources in hydrothermal fluids, distinguishing between abiotic, thermogenic, and biogenic origins24. The δ¹³C values of CO₂ and CH₄, combined with a C1/(C2–C3) value of ~108, indicate a mix of abiotic reactions and thermogenic degradation of organic matter with minor biogenic contribution that would typically be indicated by higher C1/(C2–C3) values24,25. The δ¹³C-CO2 values are lower than in basalt-hosted hydrothermal systems, which average at –5.74 ± 3.5‰, (MARHYS DB 4.0; Mg <5 mmol kg−1) and reflect a primitive mantle degassing signature. Fluids from the Middle Valley vent site have lower values between –33.9 and –20.7‰25, suggesting a substantial contribution from thermogenic processes. The δ¹³C-CO2 values at Jøtul are similar to those at Loki’s castle and we accordingly interpret dissolved CO2 to have a mixed magmatic and thermogenic origin28.

Elevated Sr (>142 µM) and radiogenic Sr isotope ratios (0.7085–0.7091)46 point to terrestrial material mobilization20,26,56. Chlorinity is 8–14% lower than seawater (Fig. 2d), and along with high water stable isotope ratios (δ2H-H2O and δ18O-H2O of +3.0–4.0‰ and +1.9–2.5‰, respectively), suggests subsurface phase separation under supercritical conditions, rather than dehydration reactions of low δ2H detrital clays57. Silica concentrations (10.6–14.0 mM) align with endmember concentrations from cruise MSM109 and are below quartz saturation for seafloor pressure and venting temperatures. Hydrogen endmember concentrations (14.8–19.1 mM) are approximately twice as high as those previously reported for sediment-hosted hydrothermal vent fluids58,59. These concentrations resemble those typical of ultramafic-hosted systems such as the Rainbow16 or Logatchev17 vent fields (Fig. 2e). Coinciding with these high H2 concentrations, are concentrations of H₂S (0.9–2.5 mM), which are lower than those reported for most sediment-hosted sites elsewhere (Fig. 2f). The high H2/H2S ratios of Jøtul vent fluids are similar to what has been reported for fluids from ultramafic-hosted vents. The Jøtul vent fluids are particularly enriched in dissolved carbon species and have higher H2 concentrations than reported in other studies of sediment-hosted vent fluids. This could point to the presence of ultramafic rocks in the reaction-zone of the hydrothermal system, which could be accountable for the observed high H2 and low H2S concentrations by magnetite-bornite-chalcocite-fluid equilibria60 or pentlandite desulfurization reactions61. The geological observation of altered ultramafic rocks and situation over an inferred detachment fault supports the notion that the fluids interact with ultramafic rocks along their flow paths.

Subsurface conditions at the Jøtul field

Isotope equilibrium temperatures were calculated for δ²H (H₂O-H₂ and CH₄-H₂ exchange) and δ¹³C (CH₄-CO₂ exchange)62. While Nidhogg exhibited lower δ²H equilibrium temperatures between 277 and 281 °C (Supplementary Fig. S9a, b), temperatures across the other vents ranged from 333 to 346 °C. δ¹³C equilibrium temperatures of 350–360 °C (Supplementary Fig. S9c) are slightly higher due to slower isotope exchange kinetics despite elevated temperatures (the isotope exchange slows down upon cooling). The close agreement between δ¹³C and δ²H equilibrium temperatures (within 10–20 °C) and the overall similar vent fluid compositions support a common reaction-zone for all vent fluids. However, the lower δ²H equilibrium temperatures at Nidhogg suggest conductive cooling before venting that might be related to a subtle depletion of CO₂, NH₄, and alkalinity, as well as a subtle enrichment in CH₄ and H₂S compared to the other three Jøtul vents.

The concentrations of CH4, CO2 and H2 can be related by the Sabatier reaction:

$$2{{{\rm{H}}}}_{2}{{\rm{O}}}+{{\rm{C}}}{{{\rm{H}}}}_{4}\rightleftharpoons {{\rm{C}}}{{{\rm{O}}}}_{2}+4{{{\rm{H}}}}_{2}$$
(1)

The corresponding mass action equation can be solved for H2 concentrations from measured CH4/CO2 ratios and the temperature-dependent equilibrium constants. Concentrations of H2 and CH4/CO2 ratios can thus be used to calculate chemical equilibrium temperatures. These calculated temperatures for the Sabatier reaction equilibrium are 386 to 391 °C and higher than isotope equilibrium temperatures for all vent fluids (Supplementary Fig. S9d).

At isotopic equilibrium temperatures the reaction would yield only 5–8 mM H₂, which is notably lower than the measured concentration (15–18 mM) and indicates isotopic exchange during fluid ascent and cooling, as observed in the Middle Valley vent field, Juan de Fuca Ridge25. Chemical equilibrium, which can be reached up to 100 times faster63,64, is likely more reliable for assessing reaction-zone temperature than isotopic equilibrium. Some studies suggested that in most sediment-free hydrothermal vent fluids the Sabatier reaction is not a favorable process to explain CH4 concentrations65 and that hydrothermal conditions may prevent Sabatier equilibrium from establishing itself66,67. But other studies indicate rapid kinetics depending on reaction direction, particularly when excess CH₄ drives H₂ and CO₂ production25,68.

Chlorine concentrations and water stable isotopes (δ2H-H2O, δ18O-H2O) suggest phase separation in the subsurface. Given a water depth of 2953–3021 mbsl (meter below sealevel) and in-situ pressures of 294–301 bar, phase-separated fluids with temperatures below 320 °C have been affected by substantial conductive cooling. The seafloor pressure at the Jøtul field corresponds to the critical point of seawater at 403–406 °C69, which marks the minimum temperature for phase separation. Silica endmember concentrations (13–15 mM) are below quartz saturation at seafloor pressure and temperature of venting. However, assuming a temperature of 386–392 °C calculated for the Sabatier reaction equilibrium, the most silica-rich fluid (15.1 mM Si; Fenris) corresponds to silica saturation at 330 bar (Fig. 3). A phase-separated fluid with a chlorinity of 500 mM at this depth has an equilibrium temperature of 420 °C. The Si-Cl thermobarometer, commonly used to estimate reaction-zone depth, would suggest 480–500 °C at 495–545 bar (Fig. 3). However, high temperatures during phase separation likely prevent fluids from retaining this equilibrium signature during ascent along pressure-temperature paths that come with lower Si solubilities. We estimate that the reaction-zone occurs at pressures below 360 bar (<600 mbsf; meter below seafloor), with temperatures between the Sabatier equilibrium (386 °C) and vapor-brine equilibrium (420 °C). These conditions explain observed CH₄, CO₂, and H₂ concentrations via Reaction (1) and Si and Cl levels through solubility and phase separation constraints.

Fig. 3: Reaction-zone depth estimate for Jøtul vent fluids. Black lines denote quartz saturation as a function of pressure and temperature and show Si-isopleths of 13, 14 and 15 mM Si.
Fig. 3: Reaction-zone depth estimate for Jøtul vent fluids. Black lines denote quartz saturation as a function of pressure and temperature and show Si-isopleths of 13, 14 and 15 mM Si.
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The blue line shows the pressure-temperature relation of a phase-separated low salinity fluid (3.1 wt.% NaCl) with a conjugate brine of variable composition. Red patches mark the conditions of the hydrothermal reaction-zone inferred by a) the Sabatier equilibrium temperature, Si-solubility and phase separation constraints and (b) the Si-Cl thermobarometer.

Constraints on the shallow depth of the reaction-zone have important implications for the nature of the heat source driving hydrothermal circulation in the Jøtul field. In general, hydrothermal circulation can be driven not only by magmatic heat but also by heat released during the exhumation of hot mantle rocks along detachment faults. In many nearly amagmatic detachment faults traces of hydrothermal circulation have been detected at greater depths of up to ~15 kmbsf70,71, but chemical data from the vent fluids indicating a shallow reaction-zone suggest that this is likely not the case for the Jøtul field. We therefore assume that hydrothermal circulation at Jøtul is driven by a magmatic heat source within the detachment footwall. Such footwall intrusions are not uncommon and have been proposed in several oceanic core complexes47,72,73,74. The hydrothermal reaction-zone above a magmatically driven hydrothermal system is typically separated from the magma by a conductive boundary layer (CBL)75. The thickness of the CBL ranges from a few tens to a few hundreds of meters and depends on the current magma supply rate as well as on the permeability of the layer itself75,76. Hence the magmatic heat source can be expected to occur only slightly deeper than the estimated reaction-zone depth of ~300–2500 mbsf (corresponding to a pressure of 330–545 bar). Our interpretation is supported by the occurrence of fresh pillow lavas cropping out of the sediments near the vents, which indicates geologically recent volcanic activity. Furthermore, the mixed magmatic and thermogenic origin of CO2 suggested by δ¹³C ratios in the vent fluids supports this assumption.

H2 production from alteration of ultramafic rocks

The high H₂ and low H₂S concentrations in the Jøtul fluids are atypical for basalt- or sediment-fluid interactions but consistent with ultramafic-hosted vent sites. The high H₂/H₂S ratios can be explained by buffering of the fluid composition by a pentlandite-pyrrhotite-heazlewoodite mineral assemblage61 at 350 bar and 400–425 °C (Fig. 4). Supporting an ultramafic origin of these concentrations, mineral-buffered experiments reacting seawater with hematite-magnetite or pyrite-pyrrhotite-bearing sedimentary material produced only ~4 mM H₂77. Hydrothermal experiments with organic-rich diatomaceous ooze at 400 °C and 400 bar yielded <7 mM H₂ and relatively high H₂S concentrations (>3 mM)68. We employed thermodynamic reaction path models that confirm the results of these experimental investigations and the range of concentrations for vent fluid compositions associated with circulation through sediments. When seawater reacts with sulfide-bearing sediments (e.g., pyrite-pyrrhotite), H₂S concentrations are expected to be above 5 mM. Similarly, in sulfide-free sediments reduction of seawater sulfate produces high H₂S concentrations of >5 mM at temperatures around 400 °C. The observed high H2/H2S appears inconsistent with a pure sediment control of vent fluid composition and could support the idea that ultramafic rocks are present in the hydrothermal root zone below the Jøtul field.

Fig. 4: H2S vs H2 concentrations in hydrothermal vent fluids hosted in different rock types in comparison with the Jøtul fluids.
Fig. 4: H2S vs H2 concentrations in hydrothermal vent fluids hosted in different rock types in comparison with the Jøtul fluids.
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The lines show H2/H2S ratios as produced by different rock buffers at 350 bar and temperatures denoted in the legend. “po-py: pyrrhotite-pyrite buffer (Eq. 5); “pn-hz”: pentlandite-pyrrhotite-heazlewoodite buffer (Eq. 6). Compositions of Loki’s Castle and Guaymas Basin (sediment-hosted), as well as, Rainbow and Logatchev (ultramafic-hosted) vent fluids are highlighted.

H2 production through thermal degradation of organic matter

We conducted thermodynamic reaction path calculations to examine if sediment-fluid interaction may also account for high H₂/H₂S ratios under specific conditions. In our model we react sulfate-poor seawater with organic matter-bearing sediment (Fig. 5, Supplementary Table S10, Supplementary Fig. S11). Such a fluid can be expected to form in the recharge zone of hydrothermal systems due to anhydrite precipitation2,6. At intermediate temperatures (150–200 °C) seawater is depleted in SO4, as anhydrite precipitation occurs rapidly, while thermogenic SO4 reduction is negligible. Organic matter is represented in the model by S- and N-bearing amino acids (cysteine, alanine) and alkane (propane) that act as sources of C-, S- and N-species for the vent fluids. In the model we used a concentration of 0.22 wt.% of total organic matter, which represents a conservative estimate at the lower spectrum of measured TOC concentrations (0.2−1 wt.%)40 in surface sediments along the Knipovich Ridge, 45 km south of the vent field. The carbon oxidation state in the organic matter controls the CH4/CO2 ratio and Reaction (1) produces H₂ equilibrium concentrations over large ranges of water-to-rock ratios, while CH₄, CO₂, H2S, and NH3 increase with decreasing water-to-rock ratios, due to progressive fluid-sediment interaction and associated element uptake of sedimentary organic matter. Our model calculations indicate that if a SO4-poor fluid enters the high-temperature reaction-zone, thermal degradation of organic matter may result in high H₂/H₂S ratios. This model successfully explains concentrations of C-, H-, N- and S-species in the hydrothermal endmember fluids and suggests the reaction with ultramafic rocks are not required to explain the Jøtul fluid composition.

Fig. 5: Predicted concentrations of selected chemical species for a reaction-path model in which preheated and prereacted seawater reacts with organic matter-bearing sediment at 400 °C and 500 bar.
Fig. 5: Predicted concentrations of selected chemical species for a reaction-path model in which preheated and prereacted seawater reacts with organic matter-bearing sediment at 400 °C and 500 bar.
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The initial SO4-poor fluid was generated by reacting seawater with the same (but organic matter-free) sediment at 200 °C and a water-rock ratio of 10. Note that the change in slope of CH4 and CO2 at high water-rock ratios (W/R > 10) results from consumption of CH4 and production of CO2 and H2 via the Sabbatier reaction (Reaction 1). The predicted alteration mineral assemblages corresponding to this reaction path are provided in Supplementary Fig. S11.

Summary and conclusions

The Jøtul hydrothermal vent fluids were sampled at higher temperatures and were more volatile-rich in 2024 than those collected in 2022 (MSM109). They are characterized by elevated pH, NH4+ and alkalinity, along with low metal concentrations. These characteristics are features typical of sediment-hosted hydrothermal vent fluids compared to those hosted in basalt. Additionally, the fluids carry high concentrations of CH4, CO2 and H2 and low H2S concentrations. High H2/H2S ratios are rather untypical for sediment-associated vent fluids and the geological setting around the vent field with probable detachment faulting and occurrence of ultramafic rocks give rise to the possibility of hybrid vent fluid compositions derived from both fluid-rock interactions with ultramafic rocks and sediments. Although water-ultramafic rock interaction cannot be entirely ruled out, concentrations of H2 and H2S are readily explained by SO4 reduction and CH4 oxidation following thermal degradation of organic matter in a shallow reaction-zone involving only sediments and temperatures around 400 °C. Despite being shallow in the subseafloor, the reaction-zone, due to the great water depth (~3000 mbsl), likely occurs at higher pressure and temperature than other sediment-associated vent sites like Minami-Ensei20,24 (~720 mbsl), Iheya North23,78 (~1000 mbsl) and CLAM Site22,29 (~1400 mbsl) in back-arc basins, or like Guaymas Basin19 (~2000 mbsl) and Loki’s Castle28 (~2400 mbsl) in mid-oceanic ridges. The higher pressure and temperature lead to the highest H2 concentration in such a sediment-associated vent site measured so far. Our results challenge the general view of high H2 concentrations as an indicator for water-rock reactions with ultramafic rocks and suggest that sediment-associated vent fluids are an underestimated source of carbon and H2 to the ocean.

Methods

Sampling and general fluid properties

Hydrothermal vent fluids were sampled using isobaric gas-tight (IGT) hydrothermal fluid samplers53 attached to the ROV MARUM-QUEST 4000 (Supplementary Fig. S2). The samplers are made of inert titanium and provide real time temperature measurements during sample intake. After recovery of hydrothermal fluids pressure in the sampler is maintained during subsampling in the laboratory, which allows for genuine analysis of dissolved gases in aliquots drawn from the sampler.

Fluid samples were processed immediately after dives, typically within few hours after the sampling procedure at the seafloor. After subsamples for gas analytics were drawn from the IGTs conductivity, Eh and pH values were determined using a Multi-parameter portable meter (WTW MultiLine® Multi 3630 IDS®) equipped with a SenTix® 940 pH electrode, a SenTix®ORP-T 900 Eh sensor and a TetraCon® 925 conductivity measurement cell.

All measurements were conducted at laboratory temperatures around 21 °C. Aliqouts for various ship- and shore-based analyses were prepared. These preparations included extraction of volatiles via headspace extraction (gas chromatography), filtration through 0.2 μm polyethylensulfon (PES) filters under a laminar flow bench (IC; Ion Chromatography), filtration and acidification to pH < 2, using suprapure HCl and storage in acid cleaned LDPE bottles (ICP-OES; Inductively Coupled Plasma Optical Emission Spectroscopy). Cold storage at 4 °C was applied to sample aliquots for IC, ICP-OES and Photometry and untreated sample aliquots were frozen at −24 °C for nutrient analysis.

ICP-OES and IC

Major anions (Cl⁻, SO₄²⁻, Br⁻) were determined on 150-fold diluted sample aliquots at Constructor University Bremen using a Metrohm 761 Compact IC system equipped with a Metrosep A Supp 5-150/4.0 column. As eluent a mixture of sodium carbonate (Na₂CO₃) and sodium bicarbonate (NaHCO₃) in deionized water, with a final concentrations of 1.0 mM Na₂CO₃ and 3.2 mM NaHCO₃ was used. Precision and accuracy were assessed by analysis of IAPSO as a standard seawater reference material, with an analytical uncertainty for the above mentioned anions of below 2%. Analysis of major elements (Na, K, Mg, Ca, Si, Sr) were carried out at the MARUM Sediment Geochemistry Lab, University of Bremen by ICP-OES on a Varian Vista Pro (equipped with an argon gas humidifier, a seaspray nebulizer and a cyclonic spray chamber). Samples were measured in 20-fold dilution. The machine was calibrated with a sample adapted mix of lab single element standards in 5 concentration levels. Data quality was assessed by measurements of IAPSO P-series (recommended values for major and minor elements and supplied by Ocean Scientific International Ltd), which is standardized real seawater with a salintiy of 34.994 psu. External precision for IAPSO was better than 5.5% and external accuracy is better than 1.5%. Internal precision was better than 3%. Due to the necessary dilution for sample measurements, detection limits for less abundant elements were as follows: Al (3.7 μM), Ba (0.3 μM), Cu (1.6 μM), Fe (0.7 μM), Li (28.8 μM), Mn (0.4 μM), and P (32.3 μM), with similar internal precision better than 3%.

Sulfide & nutrients measurement

Immediately after the samples have been drawn from the IGT sampler, aliquots of 100 and 750 µL were given into 1.8 and 4.0 mL glass vials, which were pre-filled with 11.8 mM and 47.4 mM of zinc acetate solution. The zinc acetate solution was prepared on a weekly basis by sparging ultrapure water with N2 gas for 15 min to remove oxygen prior to dissolving zinc acetate. The samples were measured photometrically using the methylene blue method79. The photometric measurements were performed at the MARUM Sediment Geochemistry Lab, University of Bremen.

Nutrients (ammonium, nitrate and phosphate) and total alkalinity were measured at the Leibniz Center for Tropical Marine Research. A Tecan infinite M 200pro microplate spectrophotometer from TECAN Trading AG (Switzerland) was used. The methods presented by Benesch and Mangelsdorf80, Sarazin, et al.81. and Ringuet, et al.82. were adapted to improve the resolution at low concentrations. For all parameters despite ammonium precision and accuracy have been controlled using either reference materials RMNS, KANSO or Dickson. In both cases the accuracy was better than 2%, except of phosphate where it was better than 6.3%. The precision for all parameters was better than 1%.

Analyses of dissolved gases

Dissolved gases were measured by an improved and modified method derived from Reeves, et al.83. For this, dissolved gases were first extracted from the liquid samples via headspace extraction before they were inserted in a custom-made sample injection system and determined via gas chromatography using an Agilent 7820 A gas chromatograph operated at 70 °C. Nitrogen was used as carrier gas and the compounds were separated by a Molsieve 60/80 column (Sigma-Aldrich, St Louis, MO) before they were determined via a thermal conductivity detector (H2) and a flame ionization detector (CH4). The system was calibrated with a certified reference gas mixture (Air Liquide, Crystal) with 0.999 mol-% H2 and 1.014 mol-% CH4 in a matrix of N2. The reproduciblility during the calibration in all cases was better than 1% relative. All samples were measured in triplicates from individual fluid aliquots. The reproduciblility was 4% relative or significantly better for all samples.

Total dissolved CO2 was determined by gas chromatography in the Laboratory Petrology of the Oceancrust at the University Bremen. Samples were stored in evacuated He-filled glass vials. The aliquots were acidified with 25 wt.% phosphoric acid to convert all DIC species to CO2. The samples were measured with a Thermo Scientific Trace GC Ultra equipped with a Haysep 80/100 column (Sigma-Aldrich, St Louis, MO) using He as carrier gas at 50 °C. The CO2 concentration was detected with a TCD detector. The system was calibrated with a certified reference gas mixture of CO2 in a He matrix. The measurement was validated using a control standard solution with 25 mM CO2. Two control standards measured in triplicates resulted in an average value of 22.8 mM suggesting accuracy was better than 10%. All measurements in triplicates yielded a reproducibility of better than 3%.

Analysis of light hydrocarbons and stable hydrogen and carbon isotopes analyses

Volatiles were extracted from IGT samples by a headspace extraction and transferred into 20 mL glass vials prefilled with satured NaCl solution for storage. Molecular compositions of light hydrocarbons (C1 to C6) were analyzed onboard with a 7890B (Agilent Technologies) gas chromatograph equipped with a HP-PLOT/Q capillary column and a flame ionization detector. Calibrations and performance checks of the analytical system were conducted regularly using commercial pure gas standards and gas mixtures. The coefficient of variation determined for the analytical procedure is lower than 2%. The molecular hydrocarbon composition is expressed as C1/(C2–C3).

Stable carbon and hydrogen isotope ratios (13C/12C and 2H/1H) of CO2, CH4 and H2 were determined by gas chromatography-compound specific isotope ratio mass spectrometry in the MARUM Stable Isotope Laboratory as described in Pape, et al.84. For this, a Trace GC Ultra-GC IsoLink connected to a MAT 253 isotope ratio mass spectrometer via a ConFlo IV interface (all components Thermo Fisher Scientific Inc.) was used. Reported isotope ratios are arithmetic means (of duplicate measurements at least) in the δ-notation relative to Vienna Pee Dee Belemnite (VPDB) and Vienna Standard Mean Ocean Water (VSMOW) for carbon and hydrogen, respectively. Reproducibility was checked daily using commercial CH4 standards (Isometric Instruments, Canada; Air Liquide GmbH, Germany). Standard deviations of triplicate stable isotope measurements were <0.5‰ for δ13C-CO2 and δ13C-CH4 and <1.0‰ for δ2H-CH4 and δ2H-H2.

Stable hydrogen and oxygen isotope ratios (δ2H-H2O, δ18O-H2O) in water were measured using cavity ringdown spectroscopy (DLT-100 – Los Gatos Research, USA) in the Geochemistry and Hydrogeology group’s laboratories at the Department of Geosciences, University Bremen. Lead by 6 equilibrating injections, each sample was measured in quadruples and analysis were averaged with the standard deviation falling well within the range recommended by the IAEA (δ2H < 2‰, δ18O < 0.3‰, Aggarwal, et al.85). Analyses were calibrated with externally referenced in-house standards bracketing the sample blocks. Accuracy was monitored through repeated measurements of the VSMOW standard (n = 3) with a maximum deviation of 2.27‰ (δ2H) and 0.38‰ (δ18O).

X-ray fluorenscence analysis of bulk rock samples

Whole rock X-Ray Fluorescence (XRF) analyses of major- and trace elements were conducted at the University of Oldenburg on a Panalytical AXIOSmax wavelength dispersive X-Ray Fluorescence Spectrometer. Representative rock fragments were ground to powder and fused to glass tablets. International standard materials (SDO-1 and BE-N, Govindaraju86) were measured to monitor analytical accuracy, which is <3% for major elements and <5% for selected trace elements for BE-N. Accuracy for SDO-1 is worse but generally below 8% except for MnO (14.1%), P2O5 (9.1%) and Ni (11.6%).

Computational methods

Isotope equilibrium temperatures for δ¹³C were calculated using isotope fractionation factors after Horita62 (Eq. 2). δ2H isotope equilibrium temperatures for the systems H2-H2O (Eq 3) and H2-CH4 (Eq. 4) were calculated using isotope fractionation factors after Horibe and Craig87.

$${10}^{3}{\mathrm{ln}}{{\rm{\alpha }}}({{{\rm{CO}}}}_{2}-{{{\rm{CH}}}}_{4}) = \, 26.70{{\rm{\hbox{--}}}}49.137* ({10}^{3}/{{\rm{T}}})\\ +40.828* ({10}^{6}/{{\rm{T}}}){{\rm{\hbox{--}}}}7.512({10}^{9}/{{\rm{T}}})$$
(2)
$${{\rm{\alpha }}}({{{\rm{H}}}}_{2}{{\rm{O}}}-{{{\rm{H}}}}_{2})=1.0473+201036/{{{\rm{T}}}}^{2}+2.060* {10}^{9}/{{{\rm{T}}}}^{4}+0.180* {10}^{15}/{{{\rm{T}}}}^{6}$$
(3)
$${{\rm{\alpha }}}({{{\rm{CH}}}}_{4}-{{{\rm{H}}}}_{2})=0.8994+183.54/{{{\rm{T}}}}^{2}$$
(4)

Quartz solubility was calculated for the chemical system H2O-CO2-CH4-NaCl-KCl using the software package LonerAP (developed by R.J. Bakker 2008, Fluid Inclusion Laboratory Leoben), which uses the approaches of Akinfiev and Diamond88 and Manning89. Saturation was calculated for different temperatures and pressures for a fluid with concentrations of 460 mM NaCl, 20 mM KCl, 60 mM CH4 and 40 mM CO2 that closely resemble the vent fluid composition.

Vapor brine equilibria were calculated for the chemical system H2O-NaCl according to empirical solution of Driesner and Heinrich90. The software SOWAT (sowatflinc_plotdata, version 0.1/2007) was used to calculate isobaric sections of the V + L plane. From these isobaric sections the intersection of a 3.1 wt.% NaCl equivalent fluid was interpolated to provide p-T conditions for a phase separating fluid in vapor-brine equilibrium.

Thermodynamic equilibrium calculations were performed with the SUPCRT92 software package91. The database used for this study combines all upgrades from the “slop98.dat” and the “speq02.dat” databases by Wolery and Jove-Colon92 and data for heazlewoodite and pentlandite from Klein and Bach61. Temperature dependend Log K values were calculated for the Sabbatier reaction (Eq. 1), the pyrrhotite-pyrite buffer (Eq. 5) and the pentlandite-pyrrhotite-heazlewoodite buffer (Eq. 6) at 350 bar.

$${{\rm{FeS}}}+{{{\rm{H}}}}_{2}{{\rm{S}}}\rightleftharpoons {{{\rm{FeS}}}}_{2}+{{{\rm{H}}}}_{2}$$
(5)
$$2{{{\rm{Fe}}}}_{4.5}{{{\rm{Ni}}}}_{4.5}{{{\rm{S}}}}_{8}+{{{\rm{H}}}}_{2}\rightleftharpoons 9{{\rm{FeS}}}+3{{\rm{Ni}}}_{3}{{{\rm{S}}}}_{2}+{{{\rm{H}}}}_{2}{{\rm{S}}}$$
(6)

Reaction path models were conducted using the software Geochemist Workbench93. The Debye-Huckel activity model and a Taylor-made (SUPCRT92) thermodynamic database for 500 bar was used. In a first step seawater was heated to 200 °C and reacted with Corg-free sediment at a water to rock ratio of 10. Mineral precipitation was allowed for this pre-react procedure that simulates reaction of the hydrothermal fluid during the fluid recharge before reaching the high-temperature reaction-zone. The seawater was then heated to 400 °C with all minerals suppressed to simulate rapid heating in the vicinity of the reaction-zone. The 400 °C hot fluid was subsequently reacted with the same sediment including 0.22 wt.% of organic matter till a water-rock ratio of one was reached. The components used during the reaction path model and the resulting reaction-zone fluid are tabulated in Supplementary Table S10 the equilibrium mineral assemblages are shown in Supplementary Fig. S11.

Reporting summary

Further information on research design is available in the Nature Portfolio Reporting Summary linked to this article.