Hydrocarbons released during the Deepwater Horizon (DWH) oil spill weathered due to exposure to oxygen, light, and microbes. During weathering, the hydrocarbons’ reactivity and lability was altered, but it remained identifiable as “petrocarbon” due to its retention of the distinctive isotope signatures (14C and 13C) of petroleum. Relative to the initial estimates of the quantity of oil-residue deposited in Gulf sediments based on 2010–2011 data, the overall coverage and quantity of the fossil carbon on the seafloor has been attenuated. To analyze recovery of oil contaminated deep-sea sediments in the northern Gulf of Mexico we tracked the carbon isotopic composition (13C and 14C, radiocarbon) of bulk sedimentary organic carbon through time at 4 sites. Using ramped pyrolysis/oxidation, we determined the thermochemical stability of sediment organic matter at 5 sites, two of these in time series. There were clear differences between crude oil (which decomposed at a lower temperature during ramped oxidation), natural hydrocarbon seep sediment (decomposing at a higher temperature; Δ14C = -912‰) and our control site (decomposing at a moderate temperature; Δ14C = -189‰), in both the stability (ability to withstand ramped temperatures in oxic conditions) and carbon isotope signatures. We observed recovery toward our control site bulk Δ14C composition at sites further from the wellhead in ~4 years, whereas sites in closer proximity had longer recovery times. The thermographs also indicated temporal changes in the composition of contaminated sediment, with shifts towards higher temperature CO2 evolution over time at a site near the wellhead, and loss of higher temperature CO2 peaks at a more distant site.
Citation: Rogers KL, Bosman SH, Lardie-Gaylord M, McNichol A, Rosenheim BE, Montoya JP, et al. (2019) Petrocarbon evolution: Ramped pyrolysis/oxidation and isotopic studies of contaminated oil sediments from the Deepwater Horizon oil spill in the Gulf of Mexico. PLoS ONE 14(2): e0212433. https://doi.org/10.1371/journal.pone.0212433
Editor: Lee W. Cooper, University of Maryland Center for Environmental Science, UNITED STATES
Received: July 26, 2018; Accepted: February 2, 2019; Published: February 28, 2019
Copyright: © 2019 Rogers et al. This is an open access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.
Data Availability: Data are publicly available through the Gulf of Mexico Research Initiative Information & Data Cooperative (GRIIDC) at https://data.gulfresearchinitiative.org, 10.7266/N7KH0KWJ and 10.7266/N7Q52N7D.
Funding: This research was made possible by grants from The Gulf of Mexico Research Initiative through its consortiums: Ecosystem Impacts of Oil & Gas Inputs to the Gulf (ECOGIG), The Center for the Integrated Modeling and Analysis of the Gulf Ecosystem (C-Image), and Deep Sea to Coast Connectivity in the Eastern Gulf of Mexico (Deep-C) and the Resuspension, Redistribution and Deposition of DWH Recalcitrant Material (Re-Direct) project. This is ECOGIG Contribution # 521. Funding was also provided by the National Ocean Sciences Accelerator Mass Spectrometry Facility (NOSAMS) Graduate Student Internship Program (NSF OCE-1239667). The funders had no role in study design, data collection and analysis, decision to publish, or preparation of the manuscript.
Competing interests: The authors have declared that no competing interests exist.
The results of a number of field studies indicate unambiguously that oil residues from the Deepwater Horizon (DWH) oil spill were deposited on the seafloor [1–7]. Of the total oil released, an estimated 0.5–14.4% was deposited on the seafloor [1,3]. Passow and Ziervogel  argued that these estimates were low because they failed to consider the formation of marine oil snow over the total spread of the surface oil slicks, which could have resulted in a greater extent of seafloor deposition. The bulk of the sedimented oil-residue was limited to the surface sediment as defined by radiocarbon , hopane [1,4], and other radioisotopes .
The severity of impacts on benthic communities depends on the nature of the petroleum-derived material which was deposited on the seafloor. It has been suggested that biodegradation and dissolution of oil in the water column prior to deposition on the seafloor moderated these impacts [5,7,9]. We used ramped pyrolysis oxidation (RPO) to assess the biodegradation state of the material present on the seafloor due to the blowout. With RPO we examined 5 sites in all, 3 contaminated sites, two in time series and one as a function of depth, a control uncontaminated site and a natural seep site. Several studies have analyzed the recovery of contaminated sediments and have shown a reduction in the overall extent of contamination and have estimated degradation rates. Stout et al.  and Adhikari et al.  showed reduced coverage of elevated levels of hopane and polycyclic aromatic hydrocarbons (PAHs) in the years following the blowout. Studies by Stout and Payne  and Bagby et al.  analyzed biodegradation rates of multiple hydrocarbons in the sediment, showing that biodegradation continued on the seafloor after the deposition of the sedimented oil-residues. In contrast to focusing on specific petroleum compounds, studies by Pendergraft et al.  and Pendergraft and Rosenheim  employed ramped pyrolysis/oxidation paired with carbon isotope analysis on bulk coastal sediments. We applied their approach to the deep-sea floor.
RPO is an approach to determine the thermochemical stability of organic matter . When paired with δ13C and Δ14C isotopic analysis, the source of the carbon can be inferred as a function of thermal stability. The thermochemical stability of a compound is based on the amount of energy needed to break the bonds, with higher stability requiring higher temperatures, whereas more labile bonds break at lower temperatures. The thermal stability of a compound is thus related to its lability, reactivity, and suitability as a substrate in microbially mediated reactions . Fresh crude oil is quite labile, oxidizing at relatively lower temperatures . Oil degradation leads to oxygenated and higher molecular weight compounds that oxidize at higher temperatures . Shortly after the DWH event, the oil released into the environment was oxygenated , consumed by a variety of microbes and likely converted to biomass, burned, or altered in many ways [15,17–19]. We define this altered and unaltered petroleum-based product as petrocarbon . Since portions of this material are no longer amenable to gas chromatographic separation and analysis , the best method to identify it is isotopically, specifically with radiocarbon [20–22]
Pendergraft et al.  linked PAHs, an independent oil tracer, to changes in thermographs (temperature evolution of oxidized products as measured with an infrared gas analyzer) produced from oil contaminated marsh sediments. They found that sediments with elevated PAH content produced different CO2 thermographs with C isotope signatures indicating the presence of oil. Pendergraft and Rosenheim  studied the evolution of organic carbon over time in oil contaminated marsh sediments using RPO. The thermographs shifted from lower to higher thermochemical stability and corresponding isotopic signatures indicated increasing enrichment in both δ13C and Δ14C over time, indicating a transformation of the oil as it degraded in situ. These two studies show the ability of RPO to detect oil contamination through both the thermographs and isotopic analysis of the individual CO2 fractions.
The purpose of this study is to analyze the evolution of the carbon isotopic composition of bulk organic carbon over time and the change in thermochemical composition of sediments at 5 deep-water sites in the northern Gulf of Mexico. Oil deposition following the DWH oil spill was indicated by radiocarbon depletion in the bulk organic matter in the surface layer (0-1cm) of sediment . With RPO we examined 5 sites: 3 contaminated sites, two in time series and one as a function of depth, a control site, and a natural seep site. We hypothesized that: 1) over time, the bulk isotopic composition of the surface layer in contaminated areas would return to baseline values, 2) the oil-residue deposited in the sediment following the DWH oil spill would be more thermally stable than fresh Macondo oil and 3) that over time and depth the oil residue would evolve towards greater thermochemical stability. The carbon isotope signatures of the RPO splits were used to infer the origin of the organic material.
Materials and methods
Ethics statement: No permissions were required as all sites were in unprotected areas. This field study did not involve endangered or protected species. Oil spill affected sediment was collected in time series from 4 sites (GIP07, GIP17, GIP24, GIP16, Fig 1) from 2010–2017 and analyzed for bulk radiocarbon. In 2015, we also sampled 4 sites that had contained high PAHs in 2010 as reported by Mason et al. . We revisited one of these sites, BP444, again in 2017. Sediment from 5 sites in the northern Gulf of Mexico (GOM) were analyzed using RPO, including 2 of the time series sites (GIP07 and GIP17), 1 high PAH site (BP444), 1 natural seep (GC600) and 1 non-hydrocarbon influenced control (GB480) site were analyzed using ramped pyrolysis/oxidation (Fig 1 and Table 1). Sediment samples were frozen upon collection, returned to the lab, thawed, treated in 10% HCl to remove carbonates, washed, freeze-dried and ground.
Sites of sediment collection for time series (green), high PAH (yellow), and RPO analysis (red).
The Ramped Pyrolysis/Oxidation System (RPO) at the National Ocean Sciences Accelerator Mass Spectrometer facility (NOSAMS) was used to serially oxidize sediments in a controlled environment following the instrument protocol for pyrolysis in Rosenheim et al. . All quartz glassware used in this study was pre-combusted at 850°C for 1 hour prior to use. An aliquot of sediment, between ~80–110 mg, depending on the C content, was loaded into a pre-combusted quartz tube, between layers of pre-combusted quartz wool, and inserted into the combustion oven, sealed away from atmosphere. Macondo crude oil was added to a small quartz cup and loaded into the quartz tube. A total gas flow of 35 mL/min of helium with 8% oxygen flowed through the sample as the temperature was consistently ramped up to 800–1000°C (5°C /min). Prior to being trapped on the vacuum line, the evolved CO2 was measured with a Sable Systems CA-10a CO2 Analyzer, which was then used to plot the thermographs. The CO2 was integrated by cryogenically trapping using N2(l) over selected temperature intervals based on each sample’s unique CO2 evolution profile, by routing the flowing gases to different traps. Ultimately, the samples were expanded into a vacuum separations line, purified using alternating slurries of isopropanol cooled to liquid-solid phase transition with dry ice (CO2(s)), quantified manometrically using a capacitive diaphragm pressure gauge, and then sealed into a borosilicate glass ampoule. The samples were reduced to graphite using the hydrogen reduction method . Roughly 10% of CO2 was diverted during the graphitization process to be analyzed for δ13C. The graphite was analyzed for Δ14C on the USAMS instrument (3MV Tandetron) at NOSAMS [25–26]. Hemingway et al.  estimated the contamination blank for a typical RPO analysis on this system was 3.7 ± 0.6 μg C, with δ13C = -29.1± 0.1‰ and potentially Δ14C = -449 ± 41‰. The blank carbon correction for δ13C ranged between -0.02 to +0.15‰ and Fm ranged from -0.002 to +0.002 (Δ14C ~ 3–4 ‰) . Due to the small size of these corrections relative to the large differences in endmembers in this experiment, the data herein were not corrected. Bulk Δ14C analysis was completed at either NOSAMS or the University of Georgia Center for Applied Isotope Studies (UGA) using conventional sedimentary organic carbon 14C dating and graphitization approaches [24,28].
Results and discussion
Time series of bulk 14C values
As discerned by increasing isotopic enrichment, we observed recovery of bulk radiocarbon and stable carbon isotopes in sediments collected in time series from 4 sites (Fig 2A–2D). In general, all the spill affected sites showed recovery over the sampling time period. Δ14C signatures were as low as ~-501‰ (representative of a mixture of 38% 14C-free petrocarbon and 62% background) in 2010, and over time returned towards background values which are estimated to be Δ14C = -200±29‰ . It should be noted that oil-spill affected sites present in a fundamentally different manner from seep sites (Fig 2A). Oil spill sites contain a surface veneer of fossil carbon overlying more 14C enriched “younger” C; as also noted by Adhikari et al. , whereas seep sites have relatively uniform 14C depleted fossil carbon signature through all depths. In addition to the stratified nature of oil spill contaminated sites, evidence of Macondo hydrocarbons in the particulate phase in the deep-water hydrocarbon plume was found as far as 190 km southwest of the Macondo wellhead . In 2015, the surface sediment Δ14C signatures of the 4 high PAH sites ranged from -187.1 to -467.5‰ (Fig 2E) indicating that not all sites in the northern Gulf of Mexico had fully recovered to baseline values by 2015. Interestingly, at two of the sites, the sediment below the surface layer from 1–2 cm was just as depleted if not more so than the surface with Δ14C signatures ranging from -257.5 to -369.1‰ (Fig 2E). Below that depth, Δ14C values increased. BP444 (high PAH site) was revisited again in 2017 where we observed baseline values. We further explored the isotopic recovery at these sites by using RPO to analyze the potential evolution of the sedimented petrocarbon from the time series and the high PAH sites.
A) GIP07 and replicate cores from mega seep site GC600, B) GIP17, C) GIP16, D) GIP24, E) high PAH sites reported by Mason et al.  sampled in 2015 and Site BP444 revisited in 2017. Bulk Δ14C values of sediment in A-D exhibit recovery back to baseline values, while the high PAH sites in E indicate that not all sites had returned to baseline-like values.
Changes in patterns of thermal stability
Our second hypothesis was that the oil-residue deposited in the sediment following the oil spill would be more thermally stable than fresh Macondo oil. The contaminated sites that were run for RPO, GIP17, BP444 and GIP07, all exhibited thermal CO2 evolution peaks at higher temperatures than the fresh oil (Fig 3). The evolved CO2 thermographs from sediment, naturally oiled (seep) and non-oiled (control), were different from the crude oil thermograph, which exhibited two large low temperature peaks before ~200°C and tapered off at higher temperatures (Fig 3A). The thermograph for the seep, GC600, had two shoulders at lower temperatures, building to a peak at ~460°C, before rapidly falling off (Fig 3A). The petrocarbon present in GC600 sediment was clearly more thermochemically stable relative to the Macondo crude oil based on these thermographs. In contrast to the crude oil and sediment from GC600, sediment from the control site, GB480, exhibited a single prominent peak at ~370°C that tapered off with two more shoulders at higher temperatures (Fig 3A). CO2 thermographs from presumably uncontaminated sediments underlying oil-contaminated sites followed this same pattern yielding a prominent peak at ~370°C at site BP444 (3-4cm, Fig 3C), as did sediments from GIP07 in 2014 which had returned to background-like values (Fig 2). We assign this peak to typical northern Gulf sedimentary organic carbon.
A) Crude Oil, Seep site GC600 and Control site GB480, B) GIP17, crude oil and control site, C) BP444, crude oil and control site, D) GIP07, crude oil and control site. Vertical “tic” marks designate temperature boundaries of isotopic sample collections.
Our third hypothesis was that there would be a change in CO2 evolution from lower temperatures to higher temperatures in the thermographs as the petrocarbon became increasingly degraded over time. We found evidence consistent with this hypothesis in the three contaminated sites, GIP17 (Fig 3B) and GIP07 (Fig 3D), and BP444 (Fig 3C). The thermograph from GIP17 2010, the oil contaminated site closest to the well head, had a lower temperature peak straddling 300°C, and exhibited the peak at ~370°C, similar to the control site. GIP17 profiles from 2011 and 2015 also exhibited the peak at ~370°C, but the peak at 300°C shifted to higher temperatures over time to 450°C in 2011 and then 480°C in 2015 (Fig 3B). The peaks at 450°C and 480°C were similar to the peak evolving at 460°C at the seep site, GC600 (Fig 3A), indicating extremely weathered petrocarbon. The CO2 thermograph from GIP07 2010, unlike the GIP17 curve, initially exhibited three peaks at higher temperatures, with two peaks <500°C and one >500°C (Fig 3D). CO2 thermographs from subsequent years at site GIP07 (2011, 2014) are similar to the control site, exhibiting the prominent peak at 370°C, and the loss of the extra mid-high temperature peaks observed in 2010 (Fig 3D). As the weathered material evolving at around 500°C would presumably be relatively un-biodegradable, we suggest that this material may have been resuspended.
The depth profile collected in 2015 from site BP444 was similar to GIP07 and GB480, with all depths displaying a peak at ~370°C (Fig 3C). BP444 2015 0-1cm had a secondary peak at high temperature ~530°C, which decreased to a shoulder at deeper depths within the core. Considering all the data in Fig 3, we generally observed a peak at 370°C, the control site peak. Petrocarbon evolved at temperatures below 370°C, or above it, depending upon its “maturity” or evolution towards a more recalcitrant form. Changes in the magnitude and temperature of evolution of the peaks indicate changes in the thermochemical stability of the seafloor petrocarbon as it matured from evolving at 300°C, (Fig 3B, GIP17) to over 450–500°C, (BP444, GB480 and GIP07). Pendergraft and Rosenheim  observed as we did, that fresh oil evolved CO2 at temperatures well below 300°C. They observed that over time, as the oil weathered in the nearshore sediments that they studied, it shifted towards evolution at higher and higher temperatures. Consistent with this interpretation, we observed that at GIP17, over time, and with more biodegradation the evolved CO2 shifted towards higher temperatures. At GIP07, we believe our sampling effort temporally missed the less weathered, lower temperature evolving petrocarbon, and that our initial sample contained more weathered petrocarbon, similar to that found at GIP17 in 2015. Note the similarity of the samples GIP07, 0–1 in 2010, and GIP17, 0–1 in 2015 (Table 2 and Fig 4). Isotopic results (below) are consistent with this interpretation.
A paired t-test indicated no difference for Δ14C values, p = 0.259, t = 1.103, while bulk measured Δ 13C values were significantly enriched relative to the RPO weighted average (p = 0.002, t = 4.158).
The percent oxidized by the temperature intervals low: <300°C, medium: 300–500°C and high: >500°C was calculated to determine shifts in the thermochemical stability of the carbon in the sediments through time . These calculations were performed using the CO2 data continuously collected during RPO prior to purification on the vacuum line. The majority of the crude oil, 82%, was oxidized below 300°C, whereas all of the sediment, both oil-contaminated and unaffected, was primarily oxidized at temperatures above 300°C, with only 10–16% oxidized at lower temperatures (Fig 4). Sediment from GIP17 was consistent with our third hypothesis, with 2010 having the most C oxidized <300°C, 29%, decreasing over time to 14% in 2015. At GIP17, the percent oxidized at >500°C increased over time from 6% in 2010 to 28% in 2015. The down core profile for BP444 (2015) had similar percentages for C oxidized <300°C, ranging from 11–14%, while at high temperatures (>500°C) there was a decrease in percent oxidized down core from 36% at 0-1cm to 28% at 1-2cm and 22% from 3-4cm. The majority of the C was oxidized in the mid-range of temperatures (300–500°C) throughout all sampling years at all sites, summarized in Table 3.
Relative to Pendergraft et al.  and Pendergraft and Rosenheim , our thermographs were shifted towards higher temperatures, even in 2010, compared to their initial oiled marsh samples, which exhibited CO2 evolution at temperatures more similar to crude oil. We suggest that degradation of the hydrocarbons en route prior to deposition on the deep seafloor would cause these differences. Almost half of the hydrocarbons released from the broken well head rose to the surface, forming a thick oil slick, before sinking, potentially during a Marine Oil Snow Sedimentation and Flocculent Accumulation (MOSFFA) event [30–34]. Smaller hydrocarbon droplets (<100 μm) suspended in the water, formed a deep-sea plume that travelled southwest of the wellhead . Both pools of hydrocarbons were exposed to extensive and rapid degradation while in the oxic water column from microbes, dissolution, temperature, and pressure changes . Through microbial processes, hydrocarbons from the surface and the deep-water plume formed aggregates or flocculants, which caused them to sink to the seafloor [1,9,33–34]. Oil degradation was faster in the water column than it was following deposition on the seafloor [5,9]. Bagby et al.  modeled the potential oil degradation rates and found that the size of the oil compound and aggregated particle affected the speed of degradation in the water column and sediment; the larger the particle and compound, the slower the degradation rate. This longer degradation period prior to settling to the seafloor for the deep-water samples accounts for the differences we observe between the crude oil and DWH contaminated sites and the marsh sediment from Pendergraft and Rosenheim .
The difference in the degradation period could account for the differences in the thermographs for GIP17 and GIP07. The oil deposited at GIP07 (~90km from the wellhead), travelled further and therefore degraded more before settling out than the oil deposited at GIP17 (~17km from the wellhead). This extended degradation period was reflected in the thermographs by the temperature differences between the initial sampling years. The thermographs from GIP17 in 2011 and 2015 and BP444 (0–1 and 1–2) from 2015 had more CO2 evolved at higher temperatures, suggesting they had similar degradation experiences.
Trends in the Δ14C composition of evolved CO2
We observed marked differences between the control (GB480) and seep site (GC600) due to the presence (GC600) and absence (GB480) of petrocarbon (Fig 5). Relative to the seep site, the control site had higher Δ14C values over all CO2 fractions, including CO2 from lower temperatures. Evolved CO2 fractions had decreasing Δ14C values as temperature increased so that the final fraction was Δ14C = -316.1‰ (Fig 5A, Tables 2 and 4). The seep site had consistently low values, indicating 14C depletion, with Δ14C ranging between -881.1 to -950.5‰ over all temperature fractions (Fig 5C). The δ13C value of the control was lowest in the first fraction, δ13C = -25.1‰, then increased at the ~370°C peak, δ13C = -21.7‰, before decreasing again in the final fraction (Fig 5B). The seep sediments followed a similar pattern, with the lowest being the first fraction, increasing at the peak and then decreasing again for the final fraction, however, the δ13C values of the CO2 evolved from the seep sediment had low δ13C values across all fractions, < -28‰ over all temperatures (Fig 5D).
Temperature interval of CO2 fractions indicated by horizontal bars. A) Control site GB480: Δ14C, B) Control site GB480 δ13C, C) Seep site GC600 Δ14C, D) Seep site GC600 δ13C.
We expected the Δ14C value of the evolved CO2 at the time series sites (Fig 6) to initially exhibit lower Δ14C values due to petrocarbon contamination and to increase as petrocarbon degraded or was mobilized from the system by resuspension . However, at these sites, typically the first fraction that evolved at the lowest temperatures was the most enriched and the last fraction was the most depleted, similar to the control, in terms of Δ14C (Fig 6 and Table 4). Only two samples deviated from these trends: GIP17 2010, and GC600, where all temperature fractions were highly depleted in radiocarbon. Overall, Δ14C values of evolved CO2 fractions of sediment from GIP17 became increasingly enriched over time from 2010 to 2011, and then to 2015 (Fig 6A, 6C and 6E; Tables 2 and 4).
Temperature interval of CO2 fractions indicated by horizontal bars. A) GIP17 2010 Δ14C, B) GIP17 2010 δ13C, C) GIP17 2011 Δ14C, D) GIP17 2011 δ13C, E) GIP17 2015 Δ14C, F) GIP17 2015 δ13C.
The evolved CO2 from GIP07 also exhibited the trend of decreasing Δ14C signatures as temperature increased (Fig 7A, 7C and 7E; Table 4). At site BP444 (Fig 8), segment 0-1cm and 1-2cm had similar Δ14C values at lower temperatures, Δ14C = -215.5 and -205.8‰, but at higher temperatures, the 0-1cm segment was lower than at 1-2cm, with Δ14C = -624.5 and -464.1‰. Moving further down core at site BP444, the evolved CO2 fractions from sediment collected from 3-4cm had higher radiocarbon values than the first two segments from 0–1 and 1-2cm, with the initial and final fractions Δ14C = -96.7 and -267.0‰ (Fig 8A, 8C and 8E). Two samples, GB480 and GIP17 2015 0–1 cm (Table 4) exhibited initial CO2 evolution with high Δ14C and low δ13C values, suggesting the deposition of bomb radiocarbon that had been sequestered in the terrestrial environment, eroded, and re-deposited in the Gulf sediments.
Temperature interval of CO2 fractions indicated by horizontal bars. A) GIP07 2010 Δ14C, B) GIP07 2010 δ13C, C) GIP07 2011 Δ14C, D) GIP07 2011 δ13C, E) GIP07 2014 Δ14C, F) GIP07 2014 δ13C.
Temperature interval of CO2 fractions indicated by horizontal bars. A) 0-1cm Δ14C, B) 0-1cm δ13C, C) 1-2cm Δ14C, D) 1-2cm δ13C, E) 3-4cm Δ14C, and F) 3-4cm δ13C.
Both the level of contamination and the distance from the source played a role in the recovery rate of an oil-contaminated site [5,9]. As mentioned previously, higher contamination may slow overall degradation rates, potentially due to larger particle sizes, which sink faster from the water column . Valentine et al.  found consistently high levels of hopane (> 75ng/g) within 40 km of the wellhead. Similarly, Adhikari et al.  found elevated levels of PAHs < 35km from the well head 3 years after the blowout, whereas sediment beyond this distance returned to background levels. Because the bulk of the oil degradation occurs in the water column prior to sedimentation, the further the oil travelled, the more it degraded . This supports our interpretation of the differences between the thermographs of GIP07 and GIP17. GIP07, ~90km from the well head, has three more CO2 peaks evolved at higher temperatures in 2010 than GIP17, which is closer to the well head, ~16.9km away. This is also reflected in the depleted C isotopes of the first fractions of evolved CO2 from GIP07 and GIP17.
Trends in the δ 13C composition of evolved CO2
The trends in the δ13C values were more variable than the trends seen in the Δ14C signatures. Many of the δ13C signatures of the sediments followed the general trend of increasing from the lower δ13C value of the first fraction, and then decreasing again at higher temperatures. The peak seen at ~370°C in the control and several other samples was often the highest δ13C value of all the fractions (e.g., -21.7 to -22.5; Figs 5B, 6B, 6D, 6F, 7D, 7F, 8B, 8D and 8F), suggesting its origin as marine primary production, the dominant input term for sedimenting particles . Overall, the bulk mean calculated from all the fractions from the 2010 sediments from GIP17 and GIP07 were the most depleted in δ13C, becoming more enriched in the following years (Fig 9 and Table 2). Sediments from BP444 had the highest δ13C values, varying by ~1.1‰ throughout the core, while δ13C signatures for GC600 were lower than all the other sediment. The stable carbon and radiocarbon isotope signatures for all temperature fractions are summarized in Table 4.
Darker shades are more contaminated, shifting towards lighter shades of the recovered time points. Dash) Overall regression (y = 92.295x + 1824.9, r = 0.9187, n = 11, p < 0.0001), time series sediments: Red) GIP17 (y = 100.06x + 2021.5, r = 0.9217, n = 3, p = 0.0783), Blue) GIP07 (y = 184.68x + 4072.6, r = .9999, n = 3, p < 0.001), Aqua) depth trend from BP444 (y = 257.42x + 5431.4, r = 0.9843, n = 3, p = 0.0157).
Several studies have explored the potential of anoxic biodegradation of oil causing enrichment in δ13C of the remaining reservoir. Wilkes et al.  incubated alkylbenzene utilizing sulfate-reducing bacteria in oil amendments and analyzed the specific oil compounds at the beginning and ending of the experiment. Wilkes et al.  found that as more of a compound was degraded, the heavier the remaining compound reservoir became. Griebler et al.  found similar results to Wilkes’ in an anoxic fresh water oil contaminated site, with specific compounds showing carbon isotope enrichment of the remaining reservoir of specific oil compounds. Sun et al.  found similar increases of the δ13C of low molecular weight n-alkanes, up to 4‰, during heavy biodegradation, but found no fractionation in high molecular weight compounds even during heavy biodegradation. This resulted in no change to the bulk δ13C signatures of the oil, no matter the level of degradation. Whereas these studies were in anaerobic, closed systems, the fractionation of δ13C during biodegradation of oil, in combination with the mixing of modern surface production carbon, could account for the increase we observe in the δ13C of the evolved CO2 of sedimented petrocarbon, the residual of the oil released from the oil spill. The petrocarbon deposited in the GOM was further degraded than the oil reservoirs Sun et al.  studied. Degradation of organic matter also causes increases in δ13C values in terrestrial soil systems. Wynn  synthesizes the results from several studies of well-drained tropical soils where primarily C-3 vegetation derived organic matter accumulated and degraded down core. The degradation down core caused δ13C signatures of the remaining organic matter to increase, up to ~ +6‰ [43–45].
Sediment source composition and variation
We calculated the weighted average for δ13C and Δ14C per sample, combining the mass-weighted results of the individual RPO CO2 fractions; which were not significantly different from the measured bulk signatures for Δ 14C (Table 2). From the RPO average we employed a two-endmember mixing model using the Δ 14C results to calculate the percent carbon from modern and fossil sources (Table 5). For modern surface sediments we used a value of Δ14C = ~-200±29‰ , and for petrocarbon we used a value of -1000‰ Eq 1 The results of a two-endmember mixing model followed the trends of the isotopes, with the proportional contribution from petrocarbon decreasing over time as the isotope signatures increased. Our seep and control sites were at opposite ends of the spectrum with the percent C from modern sources ranging from 11%, at GC600, to 101% at GB480, while petrocarbon ranged from -1%, from GB480, to 89% at GC600. GB480 is slightly more enriched than our estimated background Δ14C ~ -200±29‰, which caused it to have over 100% modern sources and below 0% petrocarbon (e.g. 101% and -1%). The time series sites GIP17 and GIP07 contain 36 and 31%, petrocarbon in 2010 and decreased to 8% and 5% by 2015 and 2014. The two-endmember mixing model data are summarized in Table 5. To test for sensitivity, we varied the radiocarbon background by ±29‰ and re-analyzed three sediments from a range of signatures including: background (BP444 2015 3-4cm), mid-range (GIP17 2010 0–1), and radiocarbon depleted (GC600). The sediment closest to background had the most potential variation between 3–4%, while the mid-range varied 2–3%, and finally there was no difference in the highly depleted sediment (Table 6).
The co-variation of the RPO averaged δ13C and Δ14C was consistent with the C isotope depletion we observed due to the addition of petrocarbon (Fig 9 and Table 2). This co-variation has also been seen for particulate organic carbon and plankton [46, 47]. We estimated recovery rates as defined as increasing isotopic enrichment over time from the linear regressions calculated from the co-variation of the averaged RPO values of δ13C and Δ14C for the 0–1 cm interval at the GIP17 and GIP07 sites. Given the low sample number at each site, there was no statistical significance for one of the regressions (GIP17, closer to the wellhead), but we used it to estimate what the recovery rates might be. Of the two time series sites, GIP07, ~90km from the well head had a faster recovery rate at Δ14C = 46‰ per year (184.68 in 4 years) than GIP17, ~23km away, with Δ14C = 18.3‰ per year (91.6 in 5 years) (Fig 9). BP444 exhibited increasing Δ14C values with depth, becoming Δ14C = 257‰ less depleted over the 4cm of sediment we analyzed. The radiocarbon profile from BP444 showed a distinct depleted layer from 0-2cm overlaying more enriched sediment from 2-4cm. These noticeable layers indicated that there was little to no mixing or bioturbation from initial deposition of petrocarbon to sample collection in 2015.
Adhikari et al.  also analyzed DWH affected sediments using RPO and found depleted radiocarbon signatures in the higher temperature CO2 fractions. Additionally, they found elevated levels of PAHs near the Macondo wellhead after collection in 2013. Adhikari et al.  and Bagby et al.  found that in highly contaminated areas, their respective tracers, PAHs and hopane, persisted for 3–4 years following the blowout. These estimates are similar to our recovery estimates for sites further from the wellhead, which was ~4 years. We found that sites closer to the wellhead, with potentially higher levels of initial contamination, took 5–6 years to reach background Δ14C signatures.
The slower recovery rates at BP444 could be caused by the highly variable sedimentation rates across the region during and shortly after the blowout. There was increased sedimentation in the Fall of 2010 through early 2011 corresponding to the MOSSFA event following the blowout , with sedimentation rates ranging between 0.48 to 2.40 g/cm2/year during the MOSSFA event but returning to pre-spill fluxes of 0.05 to 0.16 g/cm2/year later in 2011 . The large spatial heterogeneity of sedimentation [2,33], could have created areas of higher contamination, which would be indicated by lower radiocarbon signatures. Even though GIP17 is closer to the wellhead by ~6km, surface sediment from GIP17 in 2015 was more enriched with Δ14C = -264‰, than surface sediment from BP444 in 2015, which had Δ14C = -422‰. Higher contamination levels would have slowed degradation rates, explaining the lower Δ14C signatures and slower recovery at BP444 in 2015 [1,9,49]. The massive flux of hydrocarbon contaminated material to the seafloor also reduced the size of the benthic community as well as its diversity [49,50]. With the decline in these communities, there was a reduction in the amount of bioturbation in the surface sediment, which was reflected in 234Th results . The reduced mixing would also lead to slower Δ14C recovery times at site BP444.
An additional consequence of our study is to shed light on the origin of the sedimentary organic matter to the Gulf of Mexico. Gordon and Goñi [51–53] hypothesized that organic matter characterized as low-lignin, with high δ13C and low Δ14C values contributed to organic matter deposited in deep water of the northern GOM. They suggested old, highly degraded soil organic matter from historic C-4 prairie grasses along the Mississippi River as a potential source of this organic carbon. We find no evidence to support this hypothesis. The δ13C and Δ14C values from the CO2 thermograph of the control sediment (GB480, 0–1), closely resembles the samples from the deeper sediment at BP444, 3–4 cm, and the GIP07 2014 and we suggest that these three samples are representative of typical Gulf sediments. They all exhibited decreasing δ13C and Δ 14C values with increasing temperature, contrary to what would have been observed if recalcitrant C-4 organic matter was present. Recalcitrant C-4 organic matter would evolve CO2 with low Δ14C and high δ13C values at higher temperatures. The final temperature fraction of sediment from these samples were similar to or more depleted than marine organic matter δ13C ~ -20‰ and did not indicate mixing with a C-4 source with a δ13C ~ -14‰. The primary source of organic matter to deep water Gulf sediments appear to be marine .
Ramped Pyrolysis/Oxidation combined with isotopic analysis of the evolved CO2 fractions provides valuable insight into petroleum degradation over time. Hydrocarbons deposited on the seafloor of the deep-water Gulf of Mexico took years to dissipate. Compounds of low thermochemical stability were transformed to compounds of higher thermal stability, consistent with the shift from hydrocarbon to petrocarbon. The time frame of this evolution appears to depend upon distance from the well head and the distance the oil traveled prior to deposition.
AMS samples were run at the University of Georgia Center for Applied Isotopic Studies, and the National Ocean Sciences Accelerator Mass Spectrometry facility (NOSAMS) at Woods Hole Oceanographic. We thank Alexander Cherinsky, Kathryn Elder, and Mark Roberts. Samples were collected from the RV Endeavor, RV Pelican and the RV Weatherbird and we thank their crews and Ryan Sibert and Andy Montgomery for facilitating sample collection. We also thank the National Ocean Sciences Accelerator Mass Spectrometry Graduate Student Internship Program. We also thank an anonymous reviewer who provided very helpful comments and suggestions.
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