Abstract
Methane (CH4) is common on Earth, forms the major commercial natural gas reservoirs, and is a key component of the global carbon cycle, but its natural sources are not well-characterized. We present a geochemical dataset acquired from a red wood-ant (RWA; Formica polyctena) nest in the Neuwied Basin, a part of the East Eifel Volcanic Field (EEVF), focusing on methane (CH4), stable carbon isotope of methane (δ13C-CH4), RWA activity patterns, earthquakes, and earth tides. Nest gas and ambient air were continuously sampled in-situ and analyzed to detect microbial, thermogenic, and abiotic fault-related micro-seepage. Methane degassing was not synchronized with earth tides. Elevated CH4 concentrations in nest gas appear to result from a combination of microbial activity and fault-related emissions moving via through fault networks through the RWA nest. Two δ13C-CH4 signatures were identified in nest gas: −69‰ and −37‰. The −69‰ signature of δ13C-CH4 within the RWA nest is attributed to microbial decomposition of organic matter. This finding supports previous findings that RWA nests are hot-spots of microbial CH4. Additionally, the −37% δ13C-CH4 signature is the first evidence that RWA nests also serve as traps for fault-related emissions of CH4. The −37‰ δ13C-CH4 signature can be attributed either to thermogenic/fault-related or to abiotic/fault-related CH4 formation originating from e.g. low-temperature gas-water-rock reactions in a continental setting at shallow depths (microseepage). Sources of these micro-seeps could be Devonian schists (“Sphaerosiderith Schiefer”) with iron concretions (“Eisengallen”), sandstones, or the iron-bearing “Klerf Schichten”. We cannot exclude overlapping micro-seepage of magmatic CH4 from the Eifel plume. Given the abundance of RWA nests on the landscape, their role as sources of microbial CH4 and traps for abiotically-derived CH4 should be included in estimation of methane emissions that are contributing to climatic change.
Introduction
Methane (CH4) is common on Earth, forms the major commercial natural gas reservoirs, and is a key component of the global carbon cycle [1–2]. This second-most important greenhouse gas currently has an average atmospheric concentration of 1.82 ppm, and continues to increase [3]. Today, most natural occurrences of CH4 are associated with terrestrial and aquatic processes. In the shallow subsurface, CH4 is produced on geological time scales mainly by thermal conversion of organic matter resulting from heat and pressure deep in the Earth’s crust or by microbial activity. This biotic CH4 includes the formation of thermogenic CH4 and microbial aceticlastic methanogenesis [4–5]. In contrast, abiotic CH4 is produced in much smaller amounts on a global scale and is formed by either high-temperature magmatic processes (Sabatier-type reactions) in volcanic and geothermal areas, or via low-temperature (<100 °C) Fischer-Tropsch-Type (FTT) gas-water-rock reactions in continental settings, even at shallow depths. It is found in specific geologic environments, including volcanic and geothermal systems; fluid inclusions in igneous intrusions; crystalline rocks in Precambrian Shields; and submarine, serpentinite-hosted hydrothermal fields or land-based serpentinization fluids [2,4].
In most geologic environments, biotic and abiotic gases occur simultaneously. Both thermogenic and abiotic CH4 reach the atmosphere through marine and terrestrial geologic gas (micro-)seeps, and during the exploitation and distribution of fossil fuels. To identify whether locally elevated CH4 concentrations in the atmosphere are due transportation via fault networks, a determination of possible methane source(s) is required. At the land surface, CH4 is produced by methanogenic Archaea in anaerobic soil environments or through oxidation by methanotrophic bacteria in aerobic topsoils [6]. Isotopic measurements of δ13C-CH4 can distinguish abiotic from biotic CH4 [7–8].
Increase in compressive stress, changes in the volume of the pore fluid or rock matrix, and fluid movement or buoyancy are important mechanisms driving fluid flow and keeping fractures open [9–10]. Faults and fracture networks act as preferential pathways of lateral and vertical degassing, creating linear fault-linked anomalies, irregularly-shaped diffuse or “halo” anomalies and irregularly-spaced plumes or “spot anomalies” [e.g. 11–12]. [10] showed that faults had δ13C-CH4 = −37%0 and a significantly higher CH4 flux (11.5±6.3 t CH4 km−1 yr−1) than control zones. In Europe, micro-seeps occur both onshore and offshore, with estimated CH4 flux in Europe of 0.8 Tg yr−1 and total seepage of 3 Tg yr−1 [12, 5].
Recent research has revealed close relationships between the spatial distribution of red wood-ant nests (Formica rufa-group; henceforth RWA) and tectonic fault zones [13–16]. Exploratory testing of fault-zone gases revealed that helium (He) and radon (Rn) in RWA nests exceeded atmospheric and background concentrations [13–14]. RWA mounds also have been found to be “hot spots” for CO2 emissions in European forests [17–20]. [21] showed that ant mounds (Lasius flavus, Lasius niger and Formica Candida) contributed measurable amounts to soil gas emissions from wetlands (CO2: 7.02% and N2O: 3.35%), but act as sinks with regard to the total soil CH4 budget (-4.28%). In contrast to that, higher net CH4 emission (3.5 μg m2h−1) were found in fire ant mounds situated in natural pasture soils [22]. However, continuous in-situ sampling of natural release of CH4 from RWA nests has not been done. [6] estimated CH4 flux from two nest material samples collected from the top and the rim of each of five nests on two different days (30 July and 14 October) in 2014. Finally, natural release of CH4 via fault zones [10] has been rarely considered, although there are a range of processes that could contribute to it, including micro-seepage via buoyant flux of CH4, faults increasing the flow rate of microbubbles, and gas vents responding to earth tides and earthquakes [23–24].
We used a combination of geochemical, geophysical, and biological techniques; state-of-the-art image analysis; and statistical methods to identify associations between RWA activity, continuous in-situ CH4 degassing, earth tides, and tectonic processes. We aimed to test from a geochemical/geophysical point of view three different hypothesis: a) whether a RWA nest can indicate actively in-situ degassing faults trapping migrating CH4 from the deep underground; b) whether RWA activity changes during the CH4 (micro)-seepage process; and c) whether CH4 (micro)-seepage process is affected by external agents (earth tides, earthquake events, or meteorological conditions). Specifically, we tested the null hypotheses that, in the field, in-situ concentrations of both CH4 and δ13C-CH4 and RWA activity are independent. We found a RWA nest appears to trap fault related microseepage of CH4, and that degassing pattern are independent from earth tides and meteorological conditions.
Methods
We explored associations between RWA activity, in-situ methane concentrations in an ant nest and ambient air, tectonic events, and weather processes and earth tides at the Goloring site near Koblenz, Germany during a continuous, in-situ 8-d sampling campaign that ran from 4-11 August 2016. Time and duration of the CH4 sampling was determined by the availability of the CRDS analyser owned by the Institute for Geosciences (University of Heidelberg). Our approach contrasts with prior work where different nests were statically sampled and CH4 flux was estimated from 10 nest-material samples [e.g. 6].
Study area
The Goloring site is located west of the Rhine River, southeast of the Laacher See volcano, and close to the Ochtendung Fault Zone in the seismically active Neuwied Basin, which is part of the Quaternary East Eifel Volcanic field (EEVF; western Germany; Fig 1A). The EEVF includes ≈100 Quaternary volcanic eruption centers; the Laacher See volcano experienced a phreato-plinian eruption ≈12,900 years ago [25]. The Paleozoic basement consists of alternating strata of Devonian, iron-bearing, quartzitic sandstones with a carbonate matrix and argillaceous shale reaching to 5-km depths. Several thin black coal seams (Upper Siegen) are embedded within these alternating strata [26]. Ecocene/Oligocene lignite seams are found at ≈75-160 m and are covered by Paleogene volcanites and Neogene clastic sediments. The study area has been affected by complex major tectonic and magmatic processes, including plume-related thermal expansion of the mantle-lithosphere [27–29], crustal thinning and associated volcanism [30], active rifting processes [31], and possibly crustal-scale folding or the reactivation of Variscan thrust faults under the present-day NW-SE-directed compressional stress field [31–32]. Those processes can be attributed to the existence of old zones of weakness that are reactivated under the current stress field [33–34,29]. Earthquakes (Fig 1A) are concentrated in areas that are related to the seismically active Ochtendunger Fault Zone [33]. These earthquakes are related to stress-field-controlled block movements, have a weak-to-moderate seismicity, and occur mostly in a shallow crustal depth (≤15 km) with local magnitudes (Richter scale) rarely exceeding 4.0. No fault zones have been reported from our Goloring study site, and focal depth of earthquakes near the site never exceeded 28 km during our sampling campaign [35].
Monitoring red wood ant activity
Within the research project “GeoBio-Interactions” (March – September, 2016), we monitored RWA activity using an “AntCam”: a high-resolution camera system (Mobotix MX-M12D-Sec-DNight-D135N135; 1,280 × 960 pixels) installed ≈5 m from a RWA nest (Fig 1B). During the 192-hr CH4 sampling campaign, which ran from 4-11 August, 2016, ant activities were recorded and time-stamped continuously (12 Hz). The network-compatible AntCam was connected to a network-attached storage (NAS) system for data storage via a power-over-Ethernet (POE) supply. A computer connected to the NAS evaluated the RWA activities on-site and in real time using C++ code to accelerate image evaluation. Image analysis extended the system of [36] and was based on the difference image technique (Fig 2). To reduce negative influences caused by, e.g., moving blades of grass, we used a mask to restrict analysis to only the visible top of the mound. To compensate for slight movements of the camera, e.g., due to wind, an image registration of the current image relative to the previous image was done based on mutual information before the determination of the absolute difference image [37]. Results of RWA activity were written to a file. Every hour, this file was sent via email (mobile data transfer, LTE router) to a mail server. Since two different sensors were used for the day and night, respectively, we computed different polynomials to map the sum of absolute differences onto manually designed activity categories in a follow-up procedure. The coefficients of the polynomials were obtained from a minimization of the sum of squared differences between the polynomial model and the manually assigned category for two selected weeks. A first-order polynomial was adapted to the daytime data and a third-order polynomial was adapted to the nighttime data. To avoid numerical difficulties, we first centered and scaled the data by subtracting the mean of the data during the target time and dividing by the standard deviation. Both values were computed for day-and nighttime, respectively.
Gas sampling and geochemical analyses
Field measurements of CH4 were taken from 4–11 August 2016. A stainless-steel probe (inner diameter 0,6 cm; Fig 1C) was inserted into the F. polyctena nest to a depth of 80 cm and remained there, unmoved, during the entire 192-hour sampling campaign. The probe was used for continuous CH4/δ13C-CH4 measurements. The probe was equipped with a flexible tip attached to a pushable rod and a sealable outlet for docking sampling equipment. The closed probe was inserted into the nest. After opening by pushing the rod, the probe was evacuated twice, using a 20-ml syringe. After this, the outlet was closed to prevent atmospheric influence. The outlet was only opened after docking the sampling unit to it.
Concentrations of CH4 and δ13C-CH4 in nest gas (NG) and ambient air (AA) were monitored using a portable CRDS analyser (G2201-i; Picarro, USA) that measured 12CH4, 13CH4 and H2O quasi-simultaneously at 1 Hz, and provided δ13C values relative to the Vienna Pee Dee Belemnite standard. The G2201-i uses built-in pressure and temperature control systems, and automatic water-vapor correction to ensure high stability of the portable analyzer. Effects of water vapor on the measurement were corrected automatically by the Picarro® software. The manufacturer guarantees concentration precision for the analysis of CH4 in the “high precision mode” of 5 ppbv ± 0.05 % (12C) and 1 ppbv ± 0.05% (13C) within a concentration range of 1.8-1000 ppm. The guaranteed precision of δ13C-CH4 is <0.8‰.
The CRDS analyzer was deployed in a dry, wind-sheltered location near the RWA nest. Nest gases were pumped from the aforementioned probe into the CRDS analyzer for analysis of CH4 and δ13C-CH4 values. Ambient air was measured 2 m away from the nest for 15 min every four hours during the operation using a 3-way-valve, avoiding disturbance of the nest or the position of the steel probe. All gases passed through a chemical trap filled Ascarite® (sodium hydroxide coated silica; http://www.merckgroup.com) before entering the system to remove carbon dioxide (CO2) because the high concentrations of CO2 in the nest samples could interfere with the measurements of CH4 and δ13C-CH4. Gas samples were dried by a Nafion® drying tube (Nafion MD110, PermaPure LLC, USA) before measurements to ensure higher accuracy and subsequently analyzed for CH4 concentration and δ13C-CH4. To assure quality of the CH4 and δ13C-CH4 values, reference gas measurements were taken every 8 h during the operation. Fluctuations in atmospheric CH4 and δ13C-CH4 values were validated against a single, 4-h measurement of ambient air. Carbon isotope ratios are expressed using standard delta (6) notation as described by deviations from a standard: δsample‰ = ((Rsample/Rstandard-1)) × 1000, where R is the 13C/12C ratio in the sample or standard. A total of 459 704 samples for both CH4 and δ13C-CH4 in nest gas and 27 samples in ambient air were collected and analyzed.
Meteorological Parameters
A radio meteorological station (WH1080) placed 2 m above the ground at the Goloring site continuously logged meteorological conditions (temperature [°C], humidity [%], air pressure [hPa], wind speed [m/s], rainfall [mm], and dew point [°C]) at 5-min intervals. The recorded data were downloaded every two days, checked for completeness, and stored in a data base.
Earth tides
Cyclic changes in the earth’s environment are caused by the gravitational pull of both the Sun and the Moon on the earth. These result in two slight lunar and two solar tidal bulges (“earth tides”). The two bulges occur at the surface of the earth that approximately faces the Moon and at the opposite side while the Earth rotates around its axis. Earth tides were calculated using the tool developed by [38].
Earthquake events
Data on earthquake events during the sampling campaign were obtained from the seismological databases provided by the Erdbebenstation Bensberg [35, http://www.seismo.uni-koeln.de/events/index.htm] and by the Landesamt für Geologie und Bergbau, Rheinland-Pfalz [39, http://www.lgb-rlp.de/fachthemen-des-amtes/landeserdbebendienst-rheinland-pfalz/]. The probability density of the earthquake events was estimated using the kernel density estimator of [40] using Gaussian kernels.
Data analysis
All analyses were done using R version 3.3.2 (R Core Team 2016) or MATLAB R2017a.
We examined associations between the six measured meteorological variables and RWA activity and CH4 concentrations. As many of these variables were correlated with one another, we used principal components analysis (R function prcomp) on centred and scaled data to create composite “weather” variables (i.e., principal axes) that were used in subsequent analyses.
We used the “median+2MAD” method [41] to separate true peaks in CH4 concentrations from background or naturally-elevated concentrations: any observation greater than the overall median+2MAD (2.31 ppm CH4 in nest gas and 2.11 ppm CH4 in ambient air) was considered to be a peak concentration. Background and elevated CH4 concentrations were separated based on the 90% quantile of the CH4 concentration [42]. For interpreting the significance of the correlation coefficient, we followed [43]. For δ13C-CH4, we considered concentrations < −35‰ or > 0‰ to be peak concentrations. Only peaks occurring in both data sets at the same time were considered to be true peaks. The Keeling plot method [44] was applied to determine the carbon-isotope composition of the found peaks to obtain insights into the processes that govern the distinction between isotopes in the ecosystem.
Availability of data
Data are available from the Harvard Forest Data Archive (http://harvardforest.fas.harvard.edu/data-archive), dataset HF-XXX.
Results
Meteorological conditions
During the one-week field campaign in August 2016, air temperatures ranged from 5.7-29.1 °C (mean = 16.2 °C), with only 2.1 mm rainfall overnight between 9 and 10 August. Variation in atmospheric pressure (mean 988 ± 2.24 hPa) and wind speed (1.67 ± 1.72 km/h) were small. The first three axes derived by the principal components analysis accounted for nearly 80% of the variance in the data (Table 1). The first axis represents temperature and humidity, the second axis represents atmospheric pressure (with additional contributions of humidity and windspeed), and the third axis represents rainfall and windspeed (with a minor contribution of temperature).
Median RWA activity and the three principal axes of weather were modestly associated, and accounted for only 8% of the variance in ant activity (Table 2). The ant activity increased slightly at lower temperatures (PC-1) and slightly decreased when rainfall (PC-3) was present. PC-2 was not associated significantly with RWA activity.
Weather conditions explained 10% of the variation in CH4 (ppm) (Table 3), but explained 22% of the variation in δ13C-CH4 (‰), which decreased with all measured weather variables (Table 4).
RWA activity
Ants were most active during the late afternoon and early evening hours (Fig 3A; 4A). The video streams showed that the ants went on foraging, building and maintaining the nest as they had done since the start (on March, 18th) of our longer 7-month field campaign. Decomposition of the time-series into its additive components (Fig 3B-D) illustrated that during the one-week gas-sampling campaign, there was a trend towards increasing activity over the first four days, followed by a sharp decline towards the end of the week (Fig 3B). There were two noticeable peaks of activity, at mid-day and early afternoon, followed by sharp spikes in activity near 16:30 hours (Fig 3C).
Additional external agents that may have influenced RWA activity were also visually assessed: No nuptial flight happened during this week. Ventilation phases of the nest took place in the early morning (6:40 - 7:30 UTC) on 5 August for 50 minutes and on 7 August for 20 minutes (6:40 - 7:00 UTC) after sunrise with varying ant activities (Fig 4A). On two days (07.08. and 09.08.), at 04:30 and 05:50 (UTC), respectively, golden hammer birds (Emberiza citronella) were “anting” for ≈5 min to kill parasites on their feathers with formic acid; a mouse was observed on the nest at 22:00 (UTC) for 10 minutes on 04.08.16. These biotic effects did not appear to influence any RWA activity.
CH4 and δ13C-CH4 in nest gas
A total of 459,704 data points were collected during the 192-hr sampling for each of CH4 and δ13C-CH4. Concentrations of CH4 in the nest exceeded the global atmospheric background concentration (1.82 ppm; Saunois et al. 2016) and ranged from 1.93 to 3.07 ppm (Fig 4B, Table 5). Atmospheric CH4 concentrations were slightly variable (1.90 - 2.33 ppm). The calculated anomalous threshold concentration after [41] for atmospheric CH4 was 2.11 ppm CH4 (Fig 4B). In ambient air, only four measurements out of 27 exceeded this threshold. In nest gas, the anomalous threshold was 2.31 ppm CH4. To compare our findings to fault-related emissions [10], the 90th percentile of CH4 was estimated. In nest gas, 10% of measured CH4 was larger than the 90th percentile (Table 5). Nest gas concentrations of CH4 appear to result from fault-related emissions moving via fault networks through the RWA nest. A comparison with fugitive emissions of CH4 (ppm) from basin bounding faults in the UK [10; Table 5] showed that mean nest gas emissions are of the same order, although we had 20× more observations.
δ13C-CH4 in the nest ranged from −58.48 to −49.54‰ (Fig 4C). Eight significant peaks (red and blue marks in Fig 5A, B) in nest gas were found for CH4 and δ13C-CH4 (Fig 5a, b). These peaks occurred between 17:39 (UTC) and 06:54 (UTC) the following day, but were otherwise not temporally predictable. Results of the Keeling plots [44] revealed two signatures for δ13C-CH4 at −37‰ (blue markers and dots in Fig 5A, B and C) and −69‰ (red markers and dots in in Fig 5A, B and C) in nest gas (Fig 5C).
Joint visualization of the time series of ant activity, methane concentrations, and weather (Fig 6A) reveal that all the time series exhibited a periodicity of approximately 24 hours. Cross-correlations showed positive and negative peaks at daily intervals (Fig 6B). The absolute value of the crosscorrelation coefficient ≤ 0.3, and the strongest cross-correlation occurred at a lag of ≈-30 minutes, less than the original filter width of the ant activity time series.
Discussion
Our results provide for the first time a continuous in-situ record of 192-hr sampling of both CH4 and δ13C-CH4 in a RWA nest. Although our results of CH4 and δ13C-CH4 in nest gas may not be representative of these values for the entire year, the measurement data provide a continuous set of observations of multiple variables matched in time, in contrast to other data reported in literature for which different nests were sampled at different times (two days) and CH4 flux was estimated in lab incubations from 10 nest material samples [e.g. 6].
CH4 and δ13C-CH4 in nest gas
Results from our short but continuous in-situ sampling confirmed our 1st hypothesis that elevated CH4 concentrations in nest gas appear to result from fault-related emission moving via fault networks through the RWA nest. In contrast to [21] our results show that also a red wood ant nest acts as a CH4 source. [22] attribute nest gas CH4 to high NH4-N concentrations in ant mounds. A comparison of our results with data on fugitive emissions of CH4 (ppm) from basin bounding faults in the UK (Boothroyd et al. 2017; Table 5) showed that mean nest gas emissions are of the same order. Elevated CH4 concentrations in nest gas appear to result from a combination of microbial activity and fault-related emissions moving via through fault networks through the RWA nest.
Comparison of δ13C-CH4 nest gas signatures with published data suggests that it can be attributed to two different sources (Fig 7). The δ13C-CH4 signature of −69‰ in nest gas indicates a microbial source, such as decomposing organic matter that is high in nutrients [8]. This result supports the findings of [22] that the aboveground parts of ant nests are hot-spots of CH4 production.
The second isotope signature, −37‰ δ13C-CH4, can be attributed either to thermogenic/fault-related [10] or to abiotic/fault-related CH4 formation [45]. This result provides the first evidence that RWA nests may serve as traps for fault-related emissions of CH4. [10] found a δ13C-CH4 signature of −37‰ for fugitive emission of CH4 via migration along fault zones in the United Kingdom. Our result of −37‰ δ13C-CH4 is of the same order (Fig 7) and can be attributed to fault-related CH4 emission moving through the RWA nest.
Continental loss of volatiles requires tectonically active parts and the formation of fluid-filled conduits through the continental crust. Suitable locations can be found in extensional regimes and their related volcanism [30], such as are present in our study area. Gas permeable faults and fractured rocks are pathways to naturally release significant amounts of "old" CH4 of crustal origin. Significant geologic CH4 emissions, comprising both biogenic and thermogenic CH4, are due to hydrocarbon production in sedimentary basins and, subordinately, to inorganic Fischer-Tropsch type reactions occurring in geothermal systems [24]. A variety of geological, chemical and biological processes have impacts on the deep carbon cycle. There are three possible sources for the fault-related CH4 we find in RWA nests.
First, carboniferous coals are sources of thermogenic coalbed methane (CBM) in numerous basins, including the Ruhr and Donets Basins. Their δ13C are values between −20‰ and −75‰ [46–48; Fig 9). Both basins have coal thicknesses of ≈100 m [48–49]. In our study area, much older Devonian coal seams with very small thicknesses [26] are reported at depths up to 9000 m. Though the study area is situated in a suitable tectonic compression/extensional regime, any thermogenic CH4 would likely be small because of the very low thickness of the seams and might not even lead to measurable coal-bed CH4 concentrations in nest gas. On the other hand, lignite and coal formations are often associated with aerobic methylotrophs at depths of over 1 km and are usually considered to be anaerobic [50–52]. In the study area, several small lignite seams (Middle to Upper Eocene) with a thickness of up to 5 m are found in depths of approx. 75 to 160 m. The low thickness and the shallow depth of the lignite may not lead to thermogenic CH4 seepage.
Second, δ13C-CH4 in land-based serpentinized ultramafic rocks can be as light as −37‰, and methane from Precambrian shields may exhibit even lower values (−45‰) [2,4,45]. Laboratory experiments have produced abiotic methane with a wide range of δ13C-CH4 signatures, including isotopically “light” values once thought to be indicative of biological activity (e.g. −19 to −53.6‰ by [53]; −41 to −142‰ by [54]). Abiotic CH4 can be mistaken for biotic CH4 of microbial or thermogenic origin because minor amounts of abiotic gas in biotic gas may prevent its recognition based on C and H isotope analysis [55, 45]. Sources of abiotic CH4 formation in the study area can be attributed to magmatic CH4 formation due to late magmatic (<600°C) re-distribution of C-O-H fluids during magma cooling or gas-water-rock-interactions even at low temperatures and pressures [2]. In the study area, the magmatic source for magmatic CH4 formation could be the so called “Eifel plume”, a region of about 100-120 km in diameter between 50-60 km depth and at least 410 km depth beneath the study area. The buoyant Eifel plume is characterized by excess temperature of 100-150 K, has approx. 1% of partial melt and is the main source of regional Quaternary volcanism [56].
Third, gas-water-rock-interactions, including dissolution of C- and Fe-bearing minerals in water at ~300 °C and carbonate methanation between 250 and 800 °C, do not depend on magma or magma-derived fluids [2,5]. The “Klerf Schichten” (Lower Ems) are alternating layers of reddish Fe-bearing sandstones and C-bearing shales and schists ≤ 2200-m thick and may be suitable formations for decomposition of C- and Fe-bearing minerals. Paleozoic bedrock sediments, especially the “Sphaerosiderith Schiefer” (Upper Ems; ≤ 150-m thick) schists with iron concretions (“Eisengallen”), are suitable formations for carbonate methanation: the decomposition of carbonate minerals (calcite, magnesite, siderite) at lower temperatures in H2-rich environments without mediation of gaseous CO2 (as it is usually the case for catalytic hydrogenation or FTT reaction) [2]. Within the habitable zone in the upper crust, at temperatures >150 °C and in the presence of CO2, CO, and H2, CH4 may be produced in aqueous solution even in the absence of a heterogeneous catalyst or gas phase by a series of redox reactions leading to the formation of formic acid, formaldehyde and methanol. Finally, abiotic CH4 also can form in situ through low temperature processes including the Sabatier and Fischer-Tropsch type (FTT) synthesis reactions with metals like Fe or Ni or clay minerals as catalysts [2,5].
Because the largest quantities of abiotic gases found on Earth’s surface are produced by low-temperature gas-water-rock reactions [54] we attribute the −37‰ δ13C-CH4 signature in RWA nests to fault-related emissions of abiotically formed CH4 by gas-water-rock reactions occurring at low-temperatures in a continental setting at shallow depths (micro-seepage). Probable sources might be Devonian schists (“Sphaerosiderith Schiefer”) with iron concretions (“Eisengallen”) sandstones and/or the iron-bearing “Klerf Schichten”. However, we cannot exclude the possibility of overlap by magmatic CH4 micro-seepage from the Eifel plume.
In summary, we suggest that RWA nests can indicate actively degassing faults trapping migrating CH4 from the deep underground, but that future work should seek to determine if the −37‰ signature can be attributed to a purely abiotic source, or a combination of abiotic/thermogenic source. Such a study should use additional measurements of δ13H and run long enough to determine the influence of irregularly timed earthquake events on patterns of methane degassing.
Earth tides and earthquakes
Earth tides were basically semi-diurnal. Methane activity (Fig 8A, B) showed a low negative correlation with earth tides of ≈-0.4 at a lag of 6-8 hours. The cross-correlation between the earth tides and δ13C-CH4 was ≤ |0.15| (Fig 8C). Only one earthquake occurred nearby (local magnitude: 0.8; depth: km; distance: 20 km; Fig 4). This micro-earthquake neither influenced degassing nor RWA activity.
RWA activities and external parameters
Neither our second or third hypotheses were supported by the data. During the investigation period, ant activity was higher than we had observed in 2009-2012, although an “M-shaped” pattern in daily activity was still identifiable [36]. Relatively high RWA activities during the late afternoon and early evening hours could be attributable to direct sun hitting the nest during that time or with activities associated with rebuilding damage to the nest that had occurred on 18 March. We did not find any evidence that ant activity changed during the CH4 (micro)-seepage process, or that there were strong effects of weather (see also 36]), or methane seepage. Additional external agents, including mice and “anting” birds, or micro-earthquakes did not influence ant activities during the sampling week. We conclude that during our 8-day sampling period, RWA activity was independent from external agents.
Nest gas CH4 and δ13C-CH4 and external parameters
We also did not find strong support for a relationship between CH4 in the nest and external variables during our 8-day sampling period. Atmospheric CH4 concentrations were always lower than CH4 in the RWA nest and there seemed to be little influence of atmospheric CH4 on CH4 in the nest. Less than 25% of the variance in CH4 and δ13C-CH4 were accounted for by weather conditions (cf. [57]). Earth tides also were not correlated with methane degassing in the nest. The −37‰ δ13C-CH4 signature in nest gas was detected only once. The micro-earthquake on August 9 did not influence CH4 degassing because of its far distance (20 km). On August 13, there was another earthquake (ML: 0.7; D = 13 km) only 2.3 km away from the nest. It might be, that the −37‰ δ13C-CH4 signature in nest gas was a precursor to the August 13 earthquake, promoting degassing due to an increase in compressive stress [9,10]. But this remains unanswered as the CH4 measurement campaign was terminated at August 11.
Conclusions
For the first time, both CH4 and δ13C-CH4 in a RWA nest was continuously recorded in situ. Methane degassing nor RWA activity was synchronized with earth tides, micro-earthquakes, or weather conditions. Elevated CH4 concentrations in nest gas appear to result from a combination of microbial activity and fault-related emissions moving via through fault networks through the RWA nest. Two δ13C-CH4 signatures were identified in nest gas: −69‰ and −37‰. The −69‰ signature of δ13C-CH4 within the RWA nest is best attributed to microbial decomposition of organic matter. This finding supports previous findings that RWA nests are hot-spots of microbial CH4. Additionally, the −37‰ δ13C-CH4 signature is the first evidence that RWA nests also may serve as traps for fault-related emissions of CH4. The −37‰ δ13C-CH4 signature can be attributed either to thermogenic/fault-related or to abiotic/fault-related CH4 formation originating from, e.g., low-temperature gas-water-rock reactions in a continental setting at shallow depths (micro-seepage). Future work on the −37‰ signature should use additional measurements of δ13H and run long enough to determine the influence of irregularly timed earthquake events on patterns of methane degassing.
Acknowledgements
We thank Daniela Polag and Jan Hartmann (University of Heidelberg) for doing the nest-gas sampling. RWA activity recording was done using equipment from the Department of Geology at University of Duisburg-Essen. We also thank Dr. Peter Henrich (Leiter der Direktion Landesarchäologie - Außenstelle Koblenz) for his permission to conduct the survey on the Goloring site, and Hans-Toni Dickers, Paul Görgen and Bernd Klug from Kuratorium für Heimatforschung und -pflege, Kobern-Gondorf für their support during the field campaign.