22-EPN3-110: Clumped Isotope Thermometry of Travertines in the Tauern Window (European Alps)

22-EPN3-110: Clumped Isotope Thermometry of Travertines in the Tauern Window (European Alps) – Significance for Past Seismicity and Risk Assessment of the Brenner Base Tunnel

Visit by Diethard Sanders of the University of Innsbruck (Austria), to TA2 Facility 17 – Isotoptech Stable/Clumped Isotopes Laboratory (Hungary).
Dates of visit: 06-10 November 2023.

Report summary: In the European Eastern Alps, travertines precipitated from springs with superambient temperature are very rare. Travertines show fabrics distinct from ambient-temperature
spring limestones. We had identified three fossil travertine deposits in the Navis Valley, a valley between 1005 m a.s.l. (debouch) and a watershed at ~2300–2600 m a.s.l. The travertines are located at different altitudes (1816 m, 1706 m, 1228 m), and consist of stacked laminae 1.5–4 mm thick of radial-fibrous calcite. In active travertines, such fabrics characterise crystallisation at ~15-25°C. The Navis fossil travertines post-date the Last Glacial Maximum, as shown by four U/Th ages between 10.95 ± 0.08 to 9.94 ± 0.09 ka BP 1950 AD.

Clumped isotope thermometry (Δ47-thermometry) indicates that the travertine of each location precipitated at superambient temperatures well-above the mean annual air temperature in the recharge area. The travertine-depositing waters probably rose along a steep-dipping fault system in the rock substrate, whereby the activation of these faults may have been related to seismic activity. In the subsurface of the study area, faults associated with highly mineralised warm waters were encountered also in excavation of the Brenner Base Tunnel. Our results provide the first quantitative approach with respect to formation temperature and numerical age to the rare travertine deposits of the Eastern Alps, and may alert geologists to identify this specific type of deposit as a ‘warning hint’ for potential episodes of active faulting. This is relevant to seismic hazard assessment of buildings such as the Brenner Base Tunnel.

Read the full scientific report, with kind permission from Simone Silvestro.


20-EPN2-095: Carbon Isotopic Fractionation and Quantification in Perennial Cave Ice

20-EPN2-095: Carbon Isotopic Fractionation and Quantification in Perennial Cave Ice

Visit by Artur Ionescu of the Babes-Bolyai University (Romania), to TA2 Facility 17 – Isotoptech Stable/Clumped Isotopes Laboratory (Hungary).
Dates of visit: 27 November – 08 December 2023.

Report Summary: The aim of this project is to investigate the carbon isotopic variation in perennial cave ice in different phases, for the determination of fractionation processes and estimation of the carbon source (organic or inorganic). To do so, we aim of using two types of samples, the first from
extracted ice from perennial cave glacier and ice created in laboratory conditions. We measured δ13C in gases trapped as “bubbles” in the ice mainly CO2, in dissolved carbon in the ice as HCO3 and CO3, and in the cryogenic cave carbonates.

Our hypothesis presumes that isotopic fractionation of carbon could shift an inorganic
signature towards a more organic one, thus making it difficult to assess the origin of carbon,
hence misinterpreting the origin.

In total 36 measurements have been performed on carbon-13. Our preliminary data on the
fractionation of carbon-13 show that during freezing the bubbles “concentrate” the light
isotopic ratios while the most enriched values were found in the cave carbonates. Thus
confirming our hypothesis. This is the first study that described isotopic values of carbon-13
in the different phases of the cave ice, however more laboratory experiments are needed to
better constrain the isotopic fractionation process.


22-EPN3-30: An Isotopic Inventory of Mars Analogue Environments

22-EPN3-30: An Isotopic Inventory of Mars Analogue Environments

Visit by Michael Christopher Macey of the Open University (UK), to TA2 Facility 17 – Isotoptech Stable/Clumped Isotopes Laboratory (Hungary).
Dates of visit: 06-10 November 2023.

Report Summary: This study analysed the carbon, oxygen, sulfur, and nitrogen isotope profiles in physiochemically distinct analogue environments to establish how the viability of biologically induced isotope fractionation as a candidate biosignature. The analysis was performed on sediment samples collected from analogue environments proposed as appropriate analogues for Noachian-Hesperian waters requires environments (e.g., highly saline and sulfurous). Specifically, these environments were the Salt flats of Western Sahara, a hypersaline environment that contains sulfurous sediments below thick halite layers, the high-altitude lakes of the Argentinian Andes, which possess a chemistry like dilute, modelled martian water chemistries and are impacted by a low atmospheric pressure and large diurnal fluxes in temperature and UV, the salt pans of the Makadikadi basin, and hypersaline lakes in Spain.

The analysis identified varied isotopic signatures across locations suggestive of diverse environmental conditions in terms of their microbial community, geology and inputs to the environment. Key differences include: Positive 34S ad low 13C values in the Botswanan sediments, aligning with the detection of oxic conditions, while negative values in Argentinian and Saharan samples indicate a contribution of dissimilatory sulfur metabolisms. Variation in 15N values between environments highlight previously detected variation in the presence and abundance of nitrogen-dependent metabolisms. The 18O values also strongly support the input of glacial water into the Argentinian lakes. The synthesis of this isotopic analysis with geochemical and microbiological datasets from these Mars analogue environments stands to provide crucial insight into their role as potential biosignatures.


21-EPN-FT1-008: Detection of Isotopic Biosignatures in Antarctica Subfossils

21-EPN-FT1-008: Detection of Isotopic Biosignatures in Antarctica Subfossils – Implication for the Search of Life on Mars

Visit by Alessia Cassaro of the University of Tuscia (Italy) to TA2 Facility 16 – Carbon-14 Dating AMS Laboratory.
Dates of visit: 12-16 December 2023.

Report Summary: Victoria Land, Timber Peak (Northern Victoria Land) and Mt. Fleming (Southern Victoria Land) localities are considered as a good terrestrial analogue of the Martian surface. These localities are characterized by harsher climatic conditions and endolithic microbial communities represent a borderline lifestyle. The survival of these communities depends on a delicate balance of biological, geological and climatic factors. Any unfavourable change of this equilibrium may result in the death of the community and the alteration of the rock, potentially followed by the formation of trace fossils. This process could be similar to that experienced by hypothetical life-forms on early Mars, or reflect a decay mechanism in Mars history.

Detecting traces of extant or recently extinct life is one main goals of the upcoming NASA Mars 2020 and the near future ESA ExoMars missions. In this context, the characterisation of Antarctica subfossil rocks, may be used in support of space missions. To date, only morphological descriptions (culture-dependent method) and microanalytical techniques (SEM-EDX, confocal Raman and Infrared and EPR spectroscopies) have already been performed on these samples. In this context, the main aim of this Europlanet project will be the characterisation of carbon isotopes (13C/12C) composition on samples from Timber Peak and Mt. Fleming localities. Control samples will be compared with irradiated samples (117 kGy of gamma rays) in order to i) determine the sources of organic matter and ii) understand if cosmic-ray exposure, similar to those reported on the surface of Mars for 1.5 millions of years and 13 millions of years at 2 meters beneath the surface, may altered carbon isotopic composition.


22-EPN3-128: Northwestern Amazon regional convection and its role in the control of extreme events and the isotopic signal in Quito, Ecuador.

22-EPN3-128: Northwestern Amazon regional convection and its role in the control of extreme events and the isotopic signal in Quito, Ecuador.

Visit by Maria Sheila Fabiola Serrano Vincenti, Universidad Politécnica Salesiana (Ecuador), to TA2 Facility 17 – Isotoptech Stable/Clumped Isotopes Laboratory (Hungary).
Dates of visit: 22-26 May 2023.

Report Summary: The goal of the 2023 visit to the TA Facility was to measure rainwater δ2H and δ18O values sampled at daily and monthly resolution from October 2022 to May 2023 in three different monitoring sites at North, South and Valley sites in Quito-Ecuador. Due to the complex orography, the sites experience varying intensities of rainfall and hailstorms. These measurements are part of a project aiming to understand the dynamical processes that contribute to the observed heavy and extreme precipitation events in the Tropical Andes, specifically in Quito.

Location of the installed rainfall collectors (red) and nearby meteorological REMMAQ stations (cyan). The borders of the city of Quito are marked by the white line.
Location of the installed rainfall collectors (red) and nearby meteorological REMMAQ stations (cyan). The borders of the city of Quito are marked by the white line. Credit: S Serrano-Vincenti.

Understanding these isotopic data will help the interpretation of the variations in δ2H and δ18O during intense rainfall events and subsequent fractionation due to local and upstream convection, orographic lift and moisture recycling. In addition to the measured isotopic signals, rainfall amount, pH, conductivity, and Total Dissolved Solids (TDS) data will be statistically analysed from the sites. Similarly, instrumental daily precipitation and cloud coverage information from instrumental and satellite data will be examined for convective rainfall (thunderstorms) and moisture provenance characterisation.

The Los Gatos spectrometer at the ISIL
The Los Gatos spectrometer at the ISIL Credit: S Serrano-Vincenti.

Read the full scientific report with kind permission by Sheila Serrano-Vincenti.


22-EPN3-032: Soil carbonate clumped isotope-based reconstruction of temperature evolution over the Mid-Pleistocene Transition and thenLate Pleistocene

22-EPN3-032: Soil carbonate clumped isotope-based reconstruction of temperature evolution over the Mid-Pleistocene Transition and the Late Pleistocene

Visit by Ramona Schneider, Uppsala University (Sweden), to TA2 Facility 17 – Isotoptech Stable/Clumped Isotopes Laboratory (Hungary).
Dates of visit: 20 February – 03 March 2023.

Report Summary: This study describes the use of carbonate clumped isotope thermometry as a method of reconstructing paleotemperatures from soil carbonate concretions. The method is based on the tendency of rare, heavy isotopes of carbon and oxygen to clump together in a single CO2 molecule, which is temperature-dependent. 

The analysis was performed on 12 samples that forme under a Mediterranean climate regime in Tajikistan to investigate the suitability of these samples for clumped isotope thermometry. The reconstructed temperatures of the Tajik Holocene soil carbonate nodules from three different locations show promising results, indicating that the Δ47 clumped isotope method provides reliable results for this sample type.

The obtained temperature values showed that these carbonates record temperatures that are biased towards summer temperatures. This is likely due to their formation during the summer when temperatures are highest and precipitation ceases after the maximum annual rainfall period. Even the results from older soil carbonates that formed under glacial and interglacial stages dating several glacial cycles back (MIS 11-12 and MIS 21) are well constrained, but a clear difference in formation temperature between glacial and interglacial stages could not be observed. This result can possibly be explained by formation processes of the soil carbonates, but more chronological and temperature data is required to further test this assumption and to investigate which exact period of the geological history is represented by the reconstructed temperatures. Despite these uncertainties, these initial results are very promising and highlight the potential of this method for paleotemperature reconstruction in Central Asia.

Example of a carbonate sample and the tools used for drilling.
Example of a carbonate sample and the tools used for drilling. Credit: R Schneider

21-EPN-FT1-012: Zebra dolomites revised – clumped isotope analysis as a tool to assess recrystallisation and dolomite cementation in overpressured settings

21-EPN-FT1-012: Zebra dolomites revised – clumped isotope analysis as a tool to assess recrystallisation and dolomite cementation in overpressured settings

Visit by Rudy Swennan, KU Leuven (Belgium), to TA2 Facility 17 – Isotoptech Stable/Clumped Isotopes Laboratory (Hungary).
Dates of visit: 22 – 31 August 2022.

Report Summary: Zebra dolomites are marked by an alternation of millimeter thick dark colored, as recrystallised interpreted bands and white cement bands. Disruption of the banding is manifested by displacements that gradually increases and subsequently deceases before disappearing. This disruption also occurs at intracrystalline scale with crystal rehealing features as observable under cathodoluminescence. This disruption of the zebra dolomites is explained by dolomitization in relation to overpressured fluid flow.  

In the framework of the Europlanet project zebra dolomite samples from 3 deep Belgian boreholes (Soumagne, Soiron and Bolland) were selected for clumped isotope analysis.  The aim was to sample and analyse the dark fine crystalline and white coarse dolomite cements separately to infer the original (re)crystallization temperature.  The following research questions were raised: i) is there a systematic difference in deduced temperature between the dark and white dolomite bands.  If so then this could help to better constrain the recrystallisation and cementation.  This would allow to assess the potential resetting of the original clumped isotope signature of the dark bands due to recrystallisation; ii) if the cement phases display uniform temperatures then this temperature can be compared with the minimum crystallization temperature deduced from primary fluid inclusion microthermometry [1]. The discrepancy between both temperatures, which links to the pressure correction, normally allows to quantify the overpressure of the system; iii) based on deduced crystallization temperature and δ18OPDB, the δ18OSMOW of the fluid can be assessed, allowing to constrain the origin of the dolomitizing fluids, certainly when combined with Sr isotope analysis.


21-EPN-FT1-010: Tracking the Thermal Evolution of the Miocene Ries Crater Lake as a Potential Analogue for Microbial Habitats on Early Mars

21-EPN-FT1-010: Tracking the Thermal Evolution of the Miocene Ries Crater Lake as a Potential Analogue for Microbial Habitats on Early Mars

Visit by Duncan Mifsud, University of Kent (UK), to TA2 Facility 17 – Isotoptech Stable/Clumped Isotopes Laboratory (Hungary).
Dates of visit: 21 March – 01 April 2022.

Report Summary: We have measured the clumped carbonate (13C18O16O) isotope ratios, as well as the stable isotope ratios δ18O and δ13C, of a number of bioherm, travertine, and crater fill marl samples from a drill core taken from the Nördlinger Ries Crater (NRC) in Bavaria, Germany. The aim of the project was to make use of the clumped carbonate isotope ratios so as to re-construct a palaeotemperature record of the lake environment, which could be used to assess its habitability in the time since its formation. Such information would be useful for assessing the past habitability of similar crater lake environments on Mars, which are presently of great interest.

At first glance, our results demonstrate that the analysed carbonate samples were formed at temperatures well below what would be expected in the NRC lake environment. On closer inspection, however, it was hypothesised that our carbonate samples were either collected from too high up in the stratigraphy, or they were formed under non-equilibrium conditions and thus suffered from kinetic fractionation effects. The result of the latter is a depression of the precipitation temperature as calculated by palaeothermometric scales.

Future studies are planned to investigate samples from suevite (i.e. the oldest crater infill) and to quantify the extent and causes of these kinetic fractionation effects. Future studies on other crater fill marls may thus also be worthwhile.


20-EPN-030: Identification of Metabolic Activity in Millennial Old Cave Ice

20-EPN-030: Identification of Metabolic Activity in Millennial Old Cave Ice

Visit by Aurel Persoiu of the Emil Racovita Institute of Speleology (Romania) to TA2 Facility 17 – Stable/Clumped Isotopes Laboratory (Hungary).
Dates of visit: 15-29 November 2023

Report Summary: Scarisoara Ice Cave (Apuseni Mts., Romania) hosts a more than 10,000 years old ice block. Previous studies have shown that the ice hosts a varied microbial and fungal ecosystem, with more than 50% of taxa being culturable (i.e., alive). The main question of this project was whether the oxygen gas was consumed in the ice by the metabolic activity of microbes (and/or fungi), so we aimed to determine the Ar/O2 ratio in the gas extracted from the ice.

Two duplicate ice samples were analysed. One of them was deposited during the warm Medieval Warm Period, roughly between AD 800 and 1200 (labelled MWP), while the other accumulated during the subsequent cold Little Ice Age, between AD 1200 and 1850 (labelled as LIA). The Ar/Kr and Ar/Xe ratios indicate the ice was deposited as ponding water was slowly freezing. No entrapped air bubbles were present in the ice. This data fits to modern observations, since the top of the ice are covered by liquid water during summertime, which subsequently freezes in winter. As Ar/O2 ratios show oxygen depletion cannot be detected in the ice. The δ13C of CO2 in the air equilibrated water samples compares to dissolved atmospheric CO2, while δ13C in the ice samples represents depleted CO2 from the root zone of vegetation growing above the cave. δ18O of O2 is similar to that of atmospheric oxygen. As a conclusion, we cannot confirm that oxygen depletion occurs on the ice due to microbial consumption; however, the results are not conclusive and a subsequent sampling campaign to collect more samples is scheduled for 18-25 February 2023.