Core GDGTs as phylogenetic markers.
A decade ago, crenarchaeol was postulated to be a specific membrane lipid for marine
Thaumarchaeota based on its ubiquity in the marine environment and its presence in the only available uniarchaeal enrichment culture at that time (
41). This hypothesis has been confirmed by the identification of crenarchaeol synthesis by
N. maritimus (
35), an AOA isolated from tropical aquarium gravel (
16) and in three marine AOA enrichment cultures, including “
Candidatus Nitrosoarchaeum limnia” (
29). Molecular ecological studies have indicated, however, that thaumarchaeota are not restricted to the marine environment and also thrive in freshwater, hot springs, and soil environments. In agreement with this, crenarchaeol has indeed been detected in such settings (
3,
26,
47) and enrichment of AOA from hot springs (
6,
9) and subsequent studies of their membrane lipids (
6,
30) confirmed the production of crenarchaeol by nonmarine AOA. On the basis of these culture studies, it has been postulated that crenarchaeol is an appropriate biomarker for AOA (
30). Various environmental microbiological studies indeed report a significant correlation between the archaeal
amoA gene abundance and expression and crenarchaeol concentration (
18,
26,
27). Furthermore, labeling studies of North Sea water using
13C-labeled bicarbonate over the annual cycle revealed incorporation of inorganic carbon into crenarchaeol at the time of maximum archaeal
amoA abundance, directly showing chemoautotrophic production of
Thaumarchaeota biomass (
28). However, recently thaumarchaeota, falling in the I.1b cluster, have been identified in a wastewater treatment plant that produced crenarchaeol, contained
amoA genes, but did not seem to perform chemoautotrophic ammonium oxidation (
21), suggesting that crenarchaeol is a biomarker for
Thaumarchaeota but not necessarily in all environments for active ammonia oxidizers.
The three (enrichment) cultures of thaumarchaeota from soil falling in both the I.1a (“
Ca. Nitrosoarchaeum koreensis”) and I.1b (
N. viennensis and “
Ca. Nitrososphaera”) phylogenetic clusters all produce crenarchaeol (
Fig. 2 and
Table 1). This is in agreement with the idea that crenarchaeol is specific for
Thaumarchaeota and confirms that crenarchaeol present in soil is derived from thaumarchaeota probably involved in ammonium oxidation. It also confirms the presence of crenarchaeol in group I.1b
Thaumarchaeota that was so far only evident from the study of the moderately thermophile “
Ca. Nitrososphaera gargensis,” isolated from a hot spring (
30). In all three soil thaumarchaeota, crenarchaeol is the most abundant GDGT (
Table 1). However, there is a marked difference in the fractional abundance of the crenarchaeol regioisomer; it is quite abundant in the two soil thaumarchaeota falling in group I.1b, whereas it is only present in small relative amounts in the group I.1a thaumarchaeote “
Ca. Nitrosoarchaeum koreensis” (
Table 1;
Fig. 2). This is fully consistent with other studies: the group I.1a
N. maritimus (
35) and marine surface sediment enrichment cultures (
29) contain no or low abundances of the crenarchaeol regioisomer (<5% of summed crenarchaeol) (
Table 3), whereas it is far more dominant in “
Ca. Nitrososphaera gargensis” (24%) (
Table 3), which belongs to the group I.1b cluster. “
Candidatus Nitrosocaldus yellowstonii,” falling into the so-called thermophilic phylogenetic cluster, does also not contain substantial amounts of the crenarchaeol regioisomer (
6), but its relative abundance was not reported. This indicates that relatively high abundances of the crenarchaeol regioisomer (>10 to 20%) (
Table 3) may be indicative for group I.1b thaumarchaeota. This is consistent with environmental GDGT data (
Table 3) since soils, which host in addition to group I.1a thaumarchaeota group I.1b thaumarchaeota, have in general higher abundances of the crenarchaeol regioisomer relative to crenarchaeol than marine and lacustrine samples, where group I.1b thaumarchaeota are far less common than group I.1a thaumarchaeota.
Other GDGTs produced by thaumarchaeota, apart from crenarchaeol and its regioisomer, are GDGTs with 0 to 4 cyclopentane moieties. GDGT-0 is produced in similar relative abundances to crenarchaeol, except in the case of the group 1.Ib archaeon “
Ca. Nitrososphaera gargensis” (
30), while GDGT-1 to -4 are typically produced in lower relative amounts than GDGT-0 and crenarchaeol, although their fractional abundances vary substantially between cultures (
6,
29,
30,
35). The GDGT distribution of
N. viennensis is rather different from those of most other thaumarchaeotal cultures; apart from crenarchaeol, it only contains GDGT-4 in high relative abundance (
Fig. 3) with only low (<1%) (
Table 1) fractional abundances of GDGT-1 to -3. In this respect, it is somewhat comparable to that of the moderately thermophilic “
Ca. Nitrososphaera gargensis” (
30). This may be a consequence of the relatively high temperature (37�C) at which it was cultured (discussed below). GDGT distributions of the two other soil thaumarchaeota studied here do not show the high abundance of GDGT-0 as observed in other marine thaumarchaeota (
29,
35); it only accounts for 3 to 14% of total GDGTs. The high abundance of GDGT-4 (6 to 22%) (
Table 1) in all three soil thaumarchaeota is remarkable, as it is typically not observed in such high abundances in other thaumarchaeota. However, the thaumarchaeotal enrichment culture SJ obtained from marine sediment also contained GDGT-4 with a high fractional abundance of 12% (
29). GDGT-4 is often the most abundant GDGT in (hyper)thermophilic archaea and is thought to promote dense packing of the membrane, which helps to maintain its integrity at high temperatures (
46).
Lipids with the same molecular weight as GDGT-1 to -4 but with slightly earlier elution times have been identified in environmental samples (
26) and in sedimentary thaumarchaeotal enrichments (
29). GDGT-4′, isolated from the thermophilic archaeon
Sulfolobus solfataricus, was identified by nuclear magnetic resonance (NMR) spectroscopy as the regioisomer of GDGT-4 (
41) and, by inference, GDGT-1′ to -3′ are probably the regioisomers of GDGT-1 to -3. Their presence in the soil thaumarchaeota confirms that these lipids in soil are likely also derived from thaumarchaeota. In “
Ca. N. koreensis,” GDGTs apparently produced from hydroxylated GDGTs were detected in relatively small amounts (
Fig. 2a) (GDGT-0*, -1*, and -2*). These GDGTs have been detected previously in other group I.1a AOA enriched from marine sediments (
29) but are absent in all studied group I.1b thaumarchaeota, indicating that they may be characteristic of this lineage of thaumarchaeota. This is evidently related to the absence of IPLs with a hydroxylated GDGT core in group I.1b thaumarchaeota (see below).
It is still not precisely known why the GDGT distributions of thaumarchaeotal cultures differ from each other. This may have to do with physical conditions in addition to a genetic control. The GDGT composition of archaea is substantially affected by temperature, as has been shown for both (hyper)thermophilic crenarchaeota and euryarchaeota (
46) and mesophilic thaumarchaeota (
50). Based on this observation, the TEX
86 temperature proxy has been developed (
13,
31,
36). It uses an empirical correlation between the GDGT distribution (GDGT-1 to -3 and the crenarchaeol regioisomer) and the temperature of oceans and lakes to estimate temperatures in the past based on fossil GDGT assemblages. The rationale of this proxy is that planktonic marine and lacustrine thaumarchaeota adapt their GDGT distribution according to temperature and that this signal is recorded in sediments upon fossilization of the GDGTs. The widely varying abundance of the crenarchaeol regioisomer in group I.1a and I.1b thaumarchaeota observed here is worrying in this respect because it suggests a strong genetic control on the GDGT distribution in addition to a physiological effect. However, when the GDGT distributions of the three studied soil thaumarchaeota are used to calculate temperatures using the TEX
86, it becomes apparent that for all of them the TEX
86-derived temperature is in reasonable agreement with the actual growth temperatures (25 and 37�C) (
Table 1), even for the group I.1b thaumarchaeota that are characterized by a high abundance of the crenarchaeol regioisomer relative to that of crenarcheaol.
Distribution of IPL-GDGTs in thaumarchaeota.
Five thaumarchaeotal (enrichment) cultures have been previously profiled for their GDGT-IPL composition;
N. maritimus (
35), “
Ca. Nitrososphaera gargensis” (a group I.1b thaumarchaeote enriched from a hot spring) (
30), and three thaumarchaeotal cultures enriched from sediments (
29). The four thaumarchaeota falling in the I.1a group all have similar IPL profiles (
Table 4). The group I.1a thaumarchaeote enriched from soil, “
Ca. Nitrosoarchaeum koreensis,” analyzed here has a similar profile to the other four group I.1a thaumarchaeota (
Table 4): HPH IPLs are the most important peaks in the profile (
Fig. 3a), and the minor IPLs are similar to those encountered in the other group I.1a thaumarchaeota (
Table 4). The DH IPL with the hydroxyl-GDGT core lipids seems to be characteristic of this group since these IPLs were not detected in the group I.1b thaumarchaeota (
Table 4). The two soil thaumarchaeota from group I.1b analyzed here are both characterized by DH IPLs as the major peak in the IPL profile (
Fig. 3;
Table 4). These IPLs are present in much lower abundance in the group I.1a thaumarchaeota (
Table 4). It is also not present in large amounts in the group I.1b thaumarchaeote “
Ca. Nitrososphaera gargensis,” which has an IPL profile distinct from the other thaumarchaeotal (enrichment) cultures because of the abundance of unknown MH + 176 and DH + 176 IPLs (
30) (
Table 4). The TH IPLs were unique for
N. viennensis (
Table 4). IPLs with >2 sugar groups appear to be characteristic for (hyper)thermophilic archaea (
15), so the presence of this IPL may be the consequence of the higher cultivation temperature at which it was grown (i.e., 37�C), although they were not observed for “
Ca. Nitrososphaera” grown at the same temperature. It seems that both genetic and physiological factors play a role in the IPL composition.
Our analyses reveal that GDGTs are associated with particular head groups: in case of the group I.1b soil thaumarchaeote the HPH and MH IPLs only contain crenarchaeol but not GDGT-4 as a core GDGT (
Table 2), whereas GDGT-4 is only associated with DH, TH, and PH IPLs. In “
Ca. Nitrososphaera gargensis,” crenarchaeol is also the only core GDGT encountered in the HPH IPL (
30). For “
Ca. Nitrosoarchaeum koreensis” this is quite different since in addition to crenarchaeol, GDGT-0, -1, and, to a lesser extent, -2 (the major GDGTs) (
Fig. 2a) form the core of the HPH IPLs, while the minor GDGTs, GDGT-2 and -3, are predominantly associated with DH (
Table 2). This situation is quite comparable to those of
N. maritimus and the sedimentary thaumarchaeotal enrichment cultures (all belonging to group I.1a) (
29,
35). Hydroxylated GDGTs with 1 to 4 cyclopentane moieties only possess a DH head group, in good agreement what has been reported for marine sediments (
20), although these DH IPLs have the hydroxylated GDGT-0, and not GDGT-2, as their predominant core lipid. These findings indicate that there is a strong biological control of the head group composition of the different core GDGTs, probably to optimize the physical properties of the membrane composition of the thaumarchaeota. Future studies will have to address if this “GDGT speciation” is a function of temperature (and pH), since this has important implications for our understanding of the fate of fossil GDGT (
38). The similarities in “GDGT speciation” between thaumarchaeota of group I.1a on the one hand and group I.1b on the other hand suggest that there is also a genetic control. All thaumarchaeota examined so far produce IPL GDGTs with the HPH head group in often relatively large amounts and with crenarchaeol as one of the core GDGTs (
Table 4), indicating that HPH crenarchaeol is probably the most useful biomarker for detecting living AOA and other living, closely related thaumarchaeota (
21) in a wide variety of environments.
Recently it has been proposed that GDGT-containing archaea in deep sea sediments biosynthesize the glycerol units of GDGTs
de novo but use the isoprenoid alkyl chains from relic archaeal membranes and detritus (
43). This was evident from a labeling study with
13C-labeled glucose; the label was incorporated into the glycerol backbone of archaeal membranes, but the isoprenoid alkyl chain of the GDGT remained unlabeled. It was suggested that this was a strategy to cope with the energy-limited conditions in the deep sea environment. We previously determined incorporation of labeled bicarbonate into the core GDGTs (
11,
12). The experiments performed here also allowed us to look for isotopic heterogeneity within the IPLs produced by soil thaumarchaeota. However, the degree of
13C labeling of the IPLs produced during chemoautotrophic growth was similar to that of the core lipid (
Table 5), indicating that the polar head groups were labeled to the same extent as the GDGT core lipid.