Abstract:Compound-specific
isotope analyses of geoporphyrins, which are
derivatives of chloropigments possessed by phototrophs, provide essential
records of the biogeochemical cycle of past aquatic environments.
Here, we evaluated uncertainties in carbon and nitrogen isotopic compositions
(δ13C and δ15N) associated with
high-performance liquid chromatography (HPLC) purification and isotopic
measurements of geoporphyrins. Evaluation of total blank carbon and
nitrogen for the HPLC and our sensitivity-improved elemental a… Show more
“…This number represents the average of analytical errors (1 sigma) of various inhouse synthesized maleimide injections (also see Chikaraishi et al, 2008). The δ 15 N values of these maleimides were independently determined at JAMSTEC on an EA/IRMS (described in Isaji et al, 2020) that was calibrated with IAEA authentic standards. Methyl-isobutyl-maleimides were below the limit of reliable analysis.…”
As a key nutrient, nitrogen can limit primary productivity and carbon cycle dynamics, but also evolutionary progress. Given strong redox-dependency of its molecular speciation, environmental conditions can control nitrogen localization and bioavailability. This particularly applies to periods in Earth history with strong and frequent redox fluctuations, such as the Neoproterozoic. We here report on chlorophyll-derived porphyrins and maleimides in Ediacaran sediments from Oman. Exceptionally light δ15N values (< –10‰) in maleimides derived from anoxygenic phototrophs point towards ammonium assimilation at the chemocline, whereas the isotopic offset between kerogens and chlorophyll-derivatives indicates a variable regime of cyanobacterial and eukaryotic primary production in surface waters. Biomarker and maleimide mass balance considerations imply shallow euxinia during the terminal Ediacaran and a stronger contribution of anoxygenic phototrophs to primary productivity, possibly as a consequence of nutrient ‘lockup’ in a large anoxic ammonium reservoir. Synchronous δ13C and δ15N anomalies at the Ediacaran–Cambrian boundary may reflect one in a series of overturn events, mixing ammonium and isotopically-light DIC into oxic surface waters. By modulating access to nitrogen, environmental redox conditions may have periodically affected Ediacaran primary productivity, carbon cycle perturbations, and possibly played a role in the timing of the metazoan radiation across the terminal Ediacaran and early Cambrian.
“…This number represents the average of analytical errors (1 sigma) of various inhouse synthesized maleimide injections (also see Chikaraishi et al, 2008). The δ 15 N values of these maleimides were independently determined at JAMSTEC on an EA/IRMS (described in Isaji et al, 2020) that was calibrated with IAEA authentic standards. Methyl-isobutyl-maleimides were below the limit of reliable analysis.…”
As a key nutrient, nitrogen can limit primary productivity and carbon cycle dynamics, but also evolutionary progress. Given strong redox-dependency of its molecular speciation, environmental conditions can control nitrogen localization and bioavailability. This particularly applies to periods in Earth history with strong and frequent redox fluctuations, such as the Neoproterozoic. We here report on chlorophyll-derived porphyrins and maleimides in Ediacaran sediments from Oman. Exceptionally light δ15N values (< –10‰) in maleimides derived from anoxygenic phototrophs point towards ammonium assimilation at the chemocline, whereas the isotopic offset between kerogens and chlorophyll-derivatives indicates a variable regime of cyanobacterial and eukaryotic primary production in surface waters. Biomarker and maleimide mass balance considerations imply shallow euxinia during the terminal Ediacaran and a stronger contribution of anoxygenic phototrophs to primary productivity, possibly as a consequence of nutrient ‘lockup’ in a large anoxic ammonium reservoir. Synchronous δ13C and δ15N anomalies at the Ediacaran–Cambrian boundary may reflect one in a series of overturn events, mixing ammonium and isotopically-light DIC into oxic surface waters. By modulating access to nitrogen, environmental redox conditions may have periodically affected Ediacaran primary productivity, carbon cycle perturbations, and possibly played a role in the timing of the metazoan radiation across the terminal Ediacaran and early Cambrian.
“…The isotopic compositions and quantities of carbon were determined using a nano‐EA/IRMS system consisting of a modified elemental analyzer (Flash EA1112, ThermoFinnigan, San Jose, CA, USA), a continuous flow interface (ConFloIII, ThermoFinnigan) and an isotope ratio mass spectrometer (Delta plus XP, ThermoFinnigan), following the protocol reported by Ogawa et al 27 An aliquot of the AA was transferred into tin capsules. All the tin capsules were solvent rinsed (dichloromethane and methanol, 1:1, v/v) to remove contaminants from the surface 28 . The AA samples were transferred to the capsules and dried at 95°C on a hot plate before analysis.…”
Rationale
To achieve better precision and accuracy for δ13C analysis of individual amino acids (AAs), we have developed a new analytical method based on multi‐dimensional high‐performance liquid chromatography (HPLC) and elemental analyzer/isotope ratio mass spectrometry (EA/IRMS). Unlike conventional methods using gas chromatography, this approach omits pre‐column chemical derivatization, thus reducing systematic errors associated with the isotopic measurement.
Methods
The separation and isolation of individual AAs in a standard mixture containing 15 AAs and a biological sample, spear squid (Heterololigo bleekeri) were performed. AAs were isolated using an HPLC system equipped with a reversed‐phase column and a mixed‐mode column and collected using a fraction collector. After the chromatographic separation and further post‐HPLC purification, the δ13C values of AAs were measured by EA/IRMS.
Results
The complete isolation of all 15 AAs in the standard mixture was achieved. The δ13C values of these AAs before and after the experiment were in good agreement. Also, 15 AAs in the biological sample, H. bleekeri, were successfully measured. The δ13C values of AAs in H. bleekeri varied by as much as 30‰ with glycine being most enriched in13C.
Conclusions
The consistency between the δ13C values of reference and processed AAs demonstrates that the experimental procedure generates accurate δ13C values unaffected by fractionation effects and contamination. This method is therefore suitable for δ13C analysis of biological samples with higher precision than conventional approaches. We propose this new method as a tool to measure δ13C values of AAs in biological, ecological and biogeochemical studies.
“…For the measurements of total carbon and nitrogen contents and their isotopic compositions, we used an automated EA/IRMS system (Flash EA1112 elemental analyzer/Conflo III interface/Delta Plus XP isotoperatio mass spectrometer, Thermo Finnigan Co., Bremen) at Japan Agency for Marine-Earth Science and Technology (JAMSTEC), which was modified to improve the sensitivity for small sample analysis (>100 ngN, >500 ngC; Ogawa et al 2010;Isaji et al 2020). This analysis was conducted at the same time by the same methods as our previous measurement of the carbonaceous clast in the Zag meteorite (Kebukawa et al 2020).…”
Section: Bulk Carbon and Nitrogen Contents And Their Isotopic Compositionsmentioning
The Almahata Sitta (AhS) meteorite is a unique polymict ureilite. Recently, carbonaceous chondritic lithologies were identified in AhS. Organic matter (OM) is ubiquitously found in primitive carbonaceous chondrites. The molecular and isotopic characteristics of this OM reflect its origin and parent body processes, and are particularly sensitive to heating. The C1 lithologies AhS 671 and AhS 91A were investigated, focusing mainly on the OM. We found that the OM in these lithologies is unique and contains primitive isotopic signatures, but experienced slight heating possibly by short-term heating event(s). These characteristics support the idea that one or more carbonaceous chondritic bodies were incorporated into the ureilitic parent body. The uniqueness of the OM in the AhS samples implies that there were large variations in primitive carbonaceous chondritic materials in the solar system other than known primitive carbonaceous chondrite groups such as CI, CM, and CR chondrites.
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