Summary
Nitrogen‐fixing symbiosis is globally important in ecosystem functioning and agriculture, yet the evolutionary history of nodulation remains the focus of considerable debate. Recent evidence suggesting a single origin of nodulation followed by massive parallel evolutionary losses raises questions about why a few lineages in the N2‐fixing clade retained nodulation and diversified as stable nodulators, while most did not. Within legumes, nodulation is restricted to the two most diverse subfamilies, Papilionoideae and Caesalpinioideae, which show stable retention of nodulation across their core clades.
We characterize two nodule anatomy types across 128 species in 56 of the 152 genera of the legume subfamily Caesalpinioideae: fixation thread nodules (FTs), where nitrogen‐fixing bacteroids are retained within the apoplast in modified infection threads, and symbiosomes, where rhizobia are symplastically internalized in the host cell cytoplasm within membrane‐bound symbiosomes (SYMs).
Using a robust phylogenomic tree based on 997 genes from 147 Caesalpinioideae genera, we show that losses of nodulation are more prevalent in lineages with FTs than those with SYMs.
We propose that evolution of the symbiosome allows for a more intimate and enduring symbiosis through tighter compartmentalization of their rhizobial microsymbionts, resulting in greater evolutionary stability of nodulation across this species‐rich pantropical legume clade.
Keywords: evolution, fixation threads, Leguminosae, nitrogen fixation, nodulation, phylogenomics, symbiosis, symbiosomes
Introduction
The N2‐fixing clade of angiosperms includes all plants that form specialized organs known as nodules, within which they house intracellular diazotrophic bacteria (van Velzen et al., 2018a). Within this clade, some species of Cucurbitales, Fagales and Rosales engage in nodulating symbiosis with the filamentous actinobacteria Frankia, while Parasponia (Rosales, Cannabaceae) and legumes (Fabales, Fabaceae) host phylogenetically diverse strains of α‐ and β‐proteobacteria collectively known as rhizobia (Soltis et al., 1995; Sprent et al., 2017; Griesmann et al., 2018; van Velzen et al., 2018a). Strikingly, nodulation is mostly a rare trait across these four orders, having been reported in relatively few species except in Fabales, where the majority of the c. 20 000 species in the Fabaceae appear to be nodulated (Doyle, 2011). Across the legume family, nodulation is also very unevenly distributed, with most species in Papilionoideae and the Mimosoid clade (Caesalpinioideae sensu LPWG, 2017) being nodulated, whereas nodulation is less common in nonmimosoid Caesalpinioideae and absent in the other four smaller legume subfamilies (sensu LPWG, 2017). The reasons for this uneven phylogenetic distribution of nodulation are unclear.
Despite the ecological and economic significance of N2‐fixing root nodule symbiosis in ecosystem functioning and agriculture (Peoples et al., 1995; Batterman et al., 2013; Vitousek et al., 2013; Epihov et al., 2017), there is no consensus about the evolutionary origins of this important trait. Hypotheses have shifted from a scenario of multiple origins (Doyle, 2011; Werner et al., 2014), potentially predisposed by a cryptic precursor that evolved in the ancestor of the N2‐fixing clade (Soltis et al., 1995; Werner et al., 2014), to one of a single origin and massive parallel evolutionary losses (Soltis et al., 1995; Griesmann et al., 2018; van Velzen et al., 2018a,b). This second hypothesis was generally dismissed because multiple independent origins provided a more parsimonious solution for the phylogenetic distribution of nodulating lineages, and because variation in nodule types and microsymbionts suggested that nodules are potentially nonhomologous and arose multiple times. This clustered homoplasious occurrence of nodulation, confined to just one clade of angiosperms (Marazzi et al., 2012), prompted the idea that a cryptic precursor evolved in the ancestor of the N2‐fixing clade, which conferred a propensity for nodulation that was expressed in just a subset of lineages (Soltis et al., 1995; Doyle, 2011, 2016; Werner et al., 2014). However, no evidence for such a precursor, genetic or otherwise, has been found (Doyle, 2016; Griesmann et al., 2018; van Velzen et al., 2018a). Furthermore, nodulation involves structural and biochemical innovations underpinned by many genes, multiple developmental and signalling pathways, and coordination between the host and the microsymbiont (Brewin, 2004; Oldroyd & Downie, 2008; Oldroyd, 2013; Sprent et al., 2017; Ardley & Sprent, 2021; Ledermann et al., 2021), such that evolutionary gains of nodulation are likely to be more difficult than losses (van Velzen et al., 2018a; Edwards, 2019). Recently, the alternative hypothesis of a single evolutionary origin of nodulation followed by numerous parallel evolutionary losses has gained traction, notably from comparative genomic studies documenting pseudogenization or loss of key nodulation genes in nonnodulating species, indicative of secondary losses of nodulation (Griesmann et al., 2018; van Velzen et al., 2018a; Zhao et al., 2021). Reexamination of the structural and developmental homologies and commonalities in symbiotic gene function across nodulating lineages spanning the N2‐fixing clade suggested that these also provide more compelling evidence for the single gain and multiple losses hypothesis (van Velzen et al., 2018a; Shen & Bisseling, 2020).
This shift in thinking prompts questions about how the numerous secondary losses of nodulation are distributed across lineages and through time, why certain lineages retained nodulation to diversify as stable N2‐fixers whereas many others lost this trait, and why, through time, N2‐fixing symbiosis apparently became nonadvantageous for the large majority of N2‐fixing clade lineages.
One trait that has not been considered as a potential determinant of evolutionary stability of nodulation is the occurrence of two distinct anatomical arrangements of N2‐fixing bacteria within the nodule. In the majority of papilionoid legumes, such as pea and Medicago, an infection thread (IT), formed from invagination of a root hair cell wall, conveys rhizobia from the point of infection to the nodule primordium. Rhizobia within the IT are budded off once they reach the nodule cell and are retained within it only by the host plasmalemma‐derived symbiosome (or peribacteroid) membrane, where they differentiate into their N2‐fixing bacteroid forms (Sprent, 2001, 2009; Brewin, 2004; Sprent et al., 2017; Parniske, 2018; Ardley & Sprent, 2021; Tsyganova et al., 2021). By contrast, in all actinorhizal symbioses and in a subset of nodulating legumes the N2‐fixing bacteria are retained within modified, thin‐walled, infection threads called fixation threads (FTs), remaining enclosed within the plant cell wall and the plasmalemma. Hereafter, we refer to these as FT‐type nodules, and those in which the bacteroids are enclosed in symbiosomes as SYM‐type nodules.
FT‐type nodules were first described in actinorhizal plants (enclosing their Frankia microsymbionts), and in Parasponia, the only nonlegume known to form nodules with rhizobia (Trinick, 1980; Lancelle & Torrey, 1985; Smith et al., 1986). They were later observed in legumes, mostly in woody Caesalpinioideae (sensu LPWG, 2017) where they appeared to be relatively common (de Faria et al., 1986, 1987; Naisbitt et al., 1992; Sprent, 2001; Fonseca et al., 2012). FT‐type nodules have also been reported in a few legumes belonging to the subfamily Papilionoideae, which is sister to Caesalpinioideae (Koenen et al., 2020b; Zhao et al., 2021), including tree genera such as Andira, Dahlstedtia and Hymenolobium, and members of tribe Brongniartieae (de Faria et al., 1986, 1987; Sprent, 2001, 2009; Sprent et al., 2013, 2017). Ultrastructural and histochemical analyses of FT‐type nodules in Parasponia with rhizobia (Smith et al., 1986), actinorhizal nodules with Frankia (Pawlowski & Demchenko, 2012) and in some legumes (de Faria et al., 1986, 1987; Naisbitt et al., 1992) revealed that FTs are superficially similar to the cell wall‐bound ‘invasive’ IT, for example in harbouring some pectin (Fonseca et al., 2012). The IT is an extension of the host cell wall and comprises mainly cellulose and pectin; its role appears to be largely protective, preventing the bacteria from invading the plant in a disorganized or pathogenic manner (Brewin, 2004; Tsyganova et al., 2021). However, the composition and role of the FT remain uncertain. Moreover, the precise nature of the FT in relation to the symbiosome membrane, which in SYM‐type nodules is essential for the exchange of nutrients between the host cytoplasm and the bacteroid (White et al., 2007), remains unknown.
Within legumes, nodulation is restricted to the two largest subfamilies, Caesalpinioideae (which includes the phylogenetically nested Mimosoid clade, formerly subfamily Mimosoideae – see LPWG, 2017) and Papilionoideae (Sprent et al., 2017; Ardley & Sprent, 2021). Here we investigate the occurrence of FT‐ and SYM‐type nodulation across Caesalpinioideae, the second largest subfamily of legumes, with 152 genera and c. 4600 species distributed pantropically across all lowland tropical biomes, with minor incursions into temperate regions. We provide an updated census of nodulation occurrence, including three new records in genera of previously unknown nodulation status, plus extensive new data regarding FT‐ and SYM‐type nodules across genera. We investigate whether these two nodule types represent different degrees of ‘compartmentalization’ (i.e. physical structures that allow hosts to spatially separate symbionts; Chomicki et al., 2020), by examining the anatomy and structure of nodules in Chidlowia, Pentaclethra and Erythrophleum, genera that span an evolutionary transition from FT‐ to SYM‐type nodules that we hypothesize to have occurred within Caesalpinioideae along the branch subtending the Mimosoid clade (Fig. 1). Erythrophleum, which is placed in the sister clade of the Mimosoid clade, has FT‐type nodules, while Pentaclethra and Chidlowia, which are among the first‐branching lineages of the Mimosoid clade (Manzanilla & Bruneau, 2012; Koenen et al., 2020a), as well as all other studied taxa in the Mimosoid clade, have SYM‐type nodules.
We test the hypothesis that the transition in nodule anatomy from FT‐ to SYM‐type nodules constituted an evolutionary innovation that led to more stable retention of nodulation, whereas lineages in which FT‐type nodules occur are more prone to evolutionary losses of nodulation. For this, we explore the number and phylogenetic distribution of evolutionary losses of nodulation using a robust phylogenomic backbone that includes 97% of Caesalpinioideae genera. We also examined the composition of the FT wall in more detail than has hitherto been achieved using immunohistochemical methods that have been used for ITs (Brewin, 2004; Tsyganova et al., 2021) in order to better elucidate its possible role in symbiosis.
Materials and Methods
Nodulation and nodule anatomy
Basic nodulation data (nodulated or nonnodulated) were obtained from Sprent (2001, 2009), from papers or reports published since 2009, and from previously unpublished records in the databases of the authors, including new reports of nodulation status (Supporting Information Tables S1 and S2). Where no data are available the nodulation status of a genus is listed as Uncertain (Un) (Table S1).
Anatomical types (FT or SYM) were determined from extensive data newly obtained here (Tables S1 and S2) alongside published data for the specific taxa that were used to construct the phylogeny, or related species in the same genus, based on substantial data that indicate that nodulation is almost always a generic trait. However, losses of nodulation have been reported within the genus Senegalia (see below), and it should be acknowledged that the relatively limited nodulation record and sampling in the Caesalpinioideae may hide additional intrageneric losses (Sprent et al., 2017). All samples were prepared for light and electron microscopy according to de Faria et al. (1986, 1987) and Fonseca et al. (2012), unless otherwise stated in Table S2; in total, samples from 95 species were newly prepared for this study. Additional samples of nodules from Chidlowia sanguinea, Entada polystachya, Erythrophleum spp., Moldenhawera spp. and Pentaclethra macroloba were prepared specifically to examine in detail the presence of FTs or symbiosomes (Table S2, Notes S1). For these samples, slices from four or more nodules per species were fixed in 2.5% glutaraldehyde and processed in two ways: (1) for light microscopy and immunogold transmission electron microscopy (TEM) with the monoclonal antibodies JIM5 and JIM7, which recognize, respectively, unesterified and esterified pectin (VandenBosch et al., 1989; Tsyganova et al., 2021), according to Fonseca et al. (2012); and (2) for identifying the symbiosome membrane by TEM using additional postfixation in osmium tetroxide followed by embedding in epoxy resin according to Rubio et al. (2009). Ultramicrotomy, staining of sections for light microscopy and for TEM, and immunogold labelling with JIM5 for TEM were as described in Fonseca et al. (2012).
For immunohistochemical analysis of the FT wall, confocal laser scanning microscopy (CLSM) was performed on slides containing semithin sections (1 μm thickness) of Erythrophleum and Pentaclethra nodules fixed and embedded as per method (1) above. The sections were incubated for 2 h in 1 : 10 dilutions of monoclonal antibodies raised against various plant cell wall components (all obtained from Plant Probes, Centre for Plant Sciences, University of Leeds, UK): Lm2, which labels β‐linked‐GlcA in arabinogalactose protein (AGP) glycan; Lm5, which labels the pectic polysaccharide rhamnogalacturonan; and Lm15, which labels the XXXG motif of the nonpectic, noncellullosic polysaccharide xyloglucan. Then, after washing twice in distilled water (dH2O) the sections were incubated for 1 h in a 1 : 500 dilution of goat antirat Alexa 488 secondary antibody (ThermoFisher, Loughborough, UK) followed by several rinses with dH2O. After mounting in coverslips and Fluoromount (ThermoFisher), the sections were examined using a Zeiss LSM 710 confocal laser scanning microscope (Carl Zeiss Microscopy Ltd, Cambourne, UK), fitted with a W Plan‐Apochromat 40× lens, using spectral imaging with excitation at 488 nm and emissions between 494 nm and 727 nm. The images were colour‐coded according to wavelength and enhanced using the Min/Max function in Zen 2010 software. Ultrathin sections (80 nm) of the same samples were then immunogold labelled for TEM using the same monoclonal antibodies as those for CLSM (Lm2, Lm5, Lm15) according to Fonseca et al. (2012).
Phylogeny and ancestral trait estimation
We used a recently constructed time‐calibrated phylogeny of Caesalpinioideae that included 147 of the 152 genera, which was based on DNA sequence data derived from targeted enrichment of 997 nuclear genes selected specifically for phylogenomics of the Mimosoid clade using the Mimobaits bait set (Koenen et al., 2020a) to generate a large phylogenomic Hybseq dataset (Ringelberg et al., 2022). Using this much larger gene set allowed us to overcome lack of resolution prevalent across the backbone of the nonmimosoid grade in previous phylogenies that were based on much smaller traditional Sanger DNA sequence datasets (Bruneau et al., 2008; Manzanilla & Bruneau, 2012; LPWG, 2017) to generate a robust and densely sampled phylogenetic hypothesis. The five unsampled genera are Hultholia, a member of the Caesalpinia clade (Gagnon et al., 2016), a group of 27 genera that are all either nonnodulating or of unknown nodulation status; Stenodrepanum, which is sister to Hoffmannseggia, and is also placed in the Caesalpinia clade (Gagnon et al., 2016); Pterogyne, which is also nonnodulating and probably forms a phylogenetically isolated monogeneric lineage in the nonmimosoid grade of Caesalpinioideae that is potentially sister to a large clade comprising all Caesalpinioideae except the Umtiza and Ceratonia clades (Zhao et al., 2021); Microlobius, which is nodulating with SYM‐type nodules and probably nested within the genus Stryphnodendron (Simon et al., 2016; Ribeiro et al., 2018); and finally the nonmimosoid Vouacapoua, which is nonnodulating, but is probably placed in the Cassia clade, which contains both nodulating and nonnodulating lineages (Bruneau et al., 2008).
The original 420‐taxon Caesalpinioideae phylogeny of Ringelberg et al. (2022) was time‐calibrated in beast (Drummond & Rambaut, 2007), using a species tree topology estimated by astral (Zhang et al., 2018), a subset of 100 informative and clock‐like genes, and seven Caesalpinioideae fossil constraints (Ringelberg et al., 2022). We pruned this chronogram until each genus was represented by just a single taxon, with two exceptions: first, the genus Chamaecrista, for which we retained four species due to known variation in nodule type within that genus (Naisbitt et al., 1992; Santos et al., 2017); and second, the dense sampling of 420 taxa in the original phylogeny allowed us to test the monophyly of genera, and for nonmonophyletic genera we retained representative taxa for each para‐/polyphyletic lineage. Nodulation data (Table S1) were matched to the tips of this tree in as conservative a way as possible. For example, in the case of Prosopis, which is polyphyletic and is thus represented by four taxa in the tree, these were scored as follows: P. juliflora, P. cineraria and P. africana, which represent three independent lineages, are scored as SYM, as the nodule type of these taxa is known. By contrast, the taxon representing the fourth lineage, P. ferox, is scored as nodulating but with an unknown nodule type, because P. ferox and other taxa in this clade are nodulating, but their nodule types are unknown. In the case of Senegalia, which is also nonmonophyletic and where losses of nodulation have been reported (Sprent, 2001, 2009), but where the phylogenetic distribution of those losses remains unknown, we ran an additional trait reconstruction including two losses within the genus. The extensive generic nonmonophyly visible in Caesalpinioideae, especially within the mimosoid clade (Fig. 1), is the focus of current taxonomic work reported elsewhere (J. J. Ringelberg et al., unpublished).
Nodulation status was estimated across this phylogeny using a model with three character states: nonnodulating, fixation thread (FT), and symbiosome (SYM). We explicitly followed the single gain, multiple losses evolutionary model for the origins of nodulation; that is, nodulation evolved only once in angiosperms and was subsequently lost many times. To do this, we constrained the model so that the root state of the tree was set to FT and ran the reconstructions either allowing only three types of transitions: from FT to nonnodulating, from FT to SYM, and from SYM to nonnodulating, or allowing all possible transitions. We used stochastic character mapping implemented in the function make.simmap in the phytools R package (Revell, 2012) to simulate 500 independent evolutionary trajectories of nodulation across the time‐calibrated phylogeny. Results were summarized onto this tree across all simulations, with transitions inferred along branches connecting nodes that have different character states in the majority of the 500 simulations. Rates of character change (i.e., events per million years) were extracted from the transition matrix of the continuous‐time‐reversible Markov model fitted to the data by the make.simmap function. Taxa for which the nodulation status is unknown were assigned equal probabilities for all three character states.
Results
Nodulation and nodule anatomy
Data on nodule anatomy for 128 species of 56 genera of Caesalpinioideae, including more than 80 records newly reported here (Tables S1, S2), show that no species belonging to the Mimosoid clade have FT‐type nodules; that is, all known nodulating mimosoids have SYM‐type nodules (Figs 1, S1). By contrast, all nodulating species from the grade subtending the Mimosoid clade have FT‐type nodules (Figs 1, S2), except for a subset of species of Chamaecrista. In that sense Chamaecrista is exceptional among the taxa of the nonmimosoid grade, as it harbours species with either FT‐ or SYM‐type nodules (Naisbitt et al., 1992).
Mature nodules of Erythrophleum ivorense and E. suaveolens, placed in the sister group of the Mimosoid clade (Fig. 1), are of the indeterminate type (Sprent, 2001, 2009; Sprent et al., 2017), and similar to those described in detail in the genus Dimorphandra, which is related to Erythrophleum (Fonseca et al., 2012). Accordingly, as with Dimorphandra, nodules have a meristem at the tip and a large invasion zone (IZ) (Fig. 2a), containing cells being invaded by rhizobia (Fig. 2b), and an N2‐fixing zone occupying most of the nodule volume; this contains a mix of infected and uninfected cells (Fig. 2a). Bacteria can be seen to invade the IZ cells via ITs emerging from between the cells (Fig. 2c); these ITs are intensely immunogold‐labelled with the monoclonal antibody JIM5, indicating that they contain unesterified pectin, specifically partially methylated homogalacturonan (VandenBosch et al., 1989; Tsyganova et al., 2021), and are similar in that respect to the host cell wall (Fig. 2c,d). Similar results were obtained with JIM7 (data not shown), indicating that Erythrophleum ITs also contain esterified pectin in common with papilionoid nodules (Tsyganova et al., 2021). Infected cells in the N2‐fixing zone contain numerous FTs (Fig. 2e), bound by cell walls that are thinner than those of the ITs, and either have sparser labelling with JIM5 (Fig. 2d,f) and JIM7 (not shown) or have no apparent labelling (Fig. 2f). Higher definition TEM with osmicated samples reveals that the FTs are surrounded by a cell membrane (Fig. 2g,h), which appears to be derived from the host endoplasmic reticulum (ER). This shows that the FT comprises a multilayered compartment consisting of a cell membrane, the FT cell wall, the lumen of the FT and the bacteroid (Fig. 2g). Infected cells of nodules of the neotropical legumes Moldenhawera floribunda and M. blanchetiana var. multijuga, also placed in the nonmimosoid grade of caesalpinioids (Fig. 1), are packed with bacteroids enclosed within FTs (Fig. S2a,b). As with Erythrophleum, the ITs are intensely labelled with JIM5 (Fig. S2c), but the FTs considerably less so (Fig. S2d); the FTs in Moldenhawera are also associated with membranes arising from the ER (Fig. S2e,f). Another three nonmimosoid neotropical caesalpinioid genera (Jacqueshuberia purpurea, Fig. S2g,h; Tachigali rugosa, Fig. S2i,j; and Campsiandra comosa, Fig. S2k,l) also have their bacteroids enclosed in FTs labelled to various degrees with JIM5. Together with published reports on Chamaecrista (de Faria et al., 1987; Naisbitt et al., 1992) and Dimorphandra (Fonseca et al., 2012), these observations of five additional genera demonstrate the ubiquity of FT‐type nodules across nodulating lineages in the nonmimosoid grade of Caesalpinioideae (Fig. 1).
By contrast, Pentaclethra macroloba, which is placed among the first‐branching lineages of the mimosoid clade (Fig. 1), has indeterminate nodules (Fig. 3a) with infected cells in the N2‐fixing zone surrounded by uninfected cells (Fig. 3b) containing bacteroids that are not surrounded by a cell wall (Fig. 3c) but are clearly enclosed within symbiosomes (Fig. 3d). In the same clade, Xylia xylocarpa also has SYM‐type nodules (Fig. S1g,h). Chidlowia sanguinea nodules are similar to those of P. macroloba, except that the IZ is more prominent (Fig. 3e); the bacteroids are also enclosed in symbiosomes (Fig. 3f). Chidlowia sanguinea is sister to a large clade containing the bulk of mimosoid species, wherein SYM‐type nodules are consistently present, as illustrated by Entada polystachya (Fig. S1a,b), Enterolobium cyclocarpum (Fig. S1c,d) and Lachesiodendron viridiflorum (Fig. S1e,f), showing that symbiosomes are universally found in nodulating lineages across the entire Mimosoid clade (Fig. 1; Table S1).
The FT wall in Erythrophleum nodules was investigated further using monoclonal antibodies against AGP glycan (Lm2), the pectic polysaccharide rhamnogalacturonan (Lm5) and the nonpectic, noncellullosic polysaccharide xyloglucan (Lm15). These probes were capable of clearly delineating FTs by both CLSM (Fig. 4a–d) and TEM (Fig. 4e–h), indicating that the walls of FTs contain all three of these components. By contrast, the symbiosomes in Pentaclethra nodule sections treated identically were very difficult to discern using CLSM (Fig. 4j–l), and although they could be observed under TEM they had few or no gold particles associated with them, indicating an absence of cell wall components (Fig. 4n–p). The exception was Lm2 (AGP glycan), which labelled Pentaclethra symbiosomes (Fig. 4i,m), and thus confirmed previous observations of AGP in the symbiosome membrane made with pea (Pisum sativum L.) nodules (Tsyganova et al., 2021).
Phylogeny and evolution of nodule types
Ancestral estimation of nodulation and nodule types across the caesalpinioid phylogeny reveals two independent transitions from FT‐ to SYM‐type nodules, first on the branch subtending the Mimosoid clade in the mid‐Eocene, 46–41 million years ago (Ma) (95% highest posterior density (HPD): 46.5–40.7 Ma), and later within the genus Chamaecrista (P. A. Casaes et al., unpublished) in the early to mid‐Miocene, 27–13 Ma (95% HPD: 27.6–12.4 Ma) (Fig. 1), or potentially later given our sparse sampling of species of Chamaecrista. Seventeen losses of nodulation are hypothesized across Caesalpinioideae, 12 in ancestrally FT‐type lineages and five in ancestrally SYM‐type lineages (Fig. 1; Table S3), implying rates of losses of 0.0174 per million years (ancestrally FT‐type) and 0.0028 (ancestrally SYM‐type), that is up to six times greater for FT‐type lineages than SYM‐type lineages (Fig. 1; Table S4), suggesting that nodulation based on FT‐type nodules is significantly more prone to loss than nodulation based on SYM‐type nodules. Additional analyses show that allowing all transitions between character states results in an identical reconstruction of losses (Fig. S3). Alternative scoring of character states for taxa with missing data (e.g. assigning equal weight to nodulation and nonnodulation states), or inclusion of losses within Senegalia do not significantly affect the outcome (Figs S4, S5). All this suggests that the data strongly support our model of evolution of nodule types across Caesalpinioideae and the higher rate of losses associated with FT‐type lineages (Fig. 1).
Maximum ages of evolutionary losses of nodulation from FT‐type nodule ancestry span the late Palaeocene to the late Oligocene (59–24 Ma (95% HPD: 59.2–23.0 Ma)) and from SYM‐type nodule ancestry from the late Eocene to the late Oligocene (37–25 Ma (95% HPD: 37.2–24.6 Ma)) (Fig. 1; Table S3).
Discussion
Within legumes, nodulation is restricted to the two largest subfamilies, Caesalpinioideae (sensu LPWG, 2017) and Papilionoideae. The idea that nodulation was ‘stabilized’ in these two lineages was noted by Werner et al. (2014), who referred to core clades of Papilionoideae as ‘stable fixers’ (i.e., a clade across which losses of nodulation were almost absent) and to the Mimosoid clade (subfamily Mimosoideae in Werner et al., 2014) as having a ‘moderately stable fixing state’, where losses of nodulation were infrequent. Here we provide an explanation for this pattern: that the evolution of SYM‐type nodules, with bacteroids contained within a symbiosome, accounts for this greater stability. FT‐type nodules characterize almost all nodulating nonmimosoid Caesalpinioideae genera, while the transition to SYM‐type nodules on the stem lineage of the Mimosoid clade (Fig. 1) coincides with a shift to fewer losses of nodulation, and to a significantly lower rate of losses of nodulation per million years (i.e. a shift to greater evolutionary stability of N2‐fixation in this clade). As the FT‐type nonmimosoid Caesalpinioideae lineages are relatively more densely sampled in our phylogeny (Fig. 1) than the SYM‐type mimosoids, the difference between the rates of loss of FT and SYM is probably underestimated; the difference in rates of losses from FT‐type lineages compared to SYM‐type lineages is likely to be even greater than we report here.
In Papilionoideae, the sister group of Caesalpinioideae (LPWG, 2017; Koenen et al., 2020b), nodulating and nonnodulating genera appear to be similarly concentrated phylogenetically across the initial divergences of the subfamily, while later stabilizing as nodulating in most lineages within the large 50 kb inversion clade (Werner et al., 2014; Doyle, 2016; Epihov et al., 2017; van Velzen et al., 2018a). It remains to be tested whether there is a similar association between more frequent losses of nodulation and FT‐type nodules in Papilionoideae, where FT‐type nodules are also found sporadically, but the vast majority of nodulating lineages and all the species‐rich nodulating clades – the ‘stable fixers’ (Werner et al., 2014) – have SYM‐type nodules. Lack of phylogenetic resolution among the initial divergences in Papilionoideae (Cardoso et al., 2012, 2013; LPWG, 2017) means that this test must await a more robust phylogeny.
Assuming a single gain of nodulation followed by massive losses, the consistent occurrence of FT‐type nodules across nodulating lineages in the nonmimosoid grade of Caesalpinioideae demonstrates that FT‐type nodules are ancestral within Caesalpinioideae and persisted through early evolution of that subfamily (Fig. 1). The FT‐type nodule also characterizes actinorhizal nodules (Pawlowski & Demchenko, 2012) and rhizobial nodules in Parasponia (Lancelle & Torrey, 1985) and is thus most likely to be ancestral across the N2‐fixing clade (Shen & Bisseling, 2020) and legumes as a whole. As noted by Koenen et al. (2020b), rapid initial divergence of the six legume subfamilies implies additional losses of nodulation along the stem lineages or early in the crown group divergences of subfamilies Cercidoideae, Detarioideae, Dialioideae and Duparquetioideae, or potentially even more numerous parallel losses in more recent times, as documented within the genus Trema (Cannabaceae) (van Velzen et al., 2018a), as no extant members of these subfamilies are known to nodulate. Although we have not looked at actinorhizal symbioses here, the very low proportion of nodulated species within Cucurbitales, Fagales and Rosales (Ardley & Sprent, 2021) suggests that many lineages have suffered losses of nodulation similar to the Cercidoideae, Detarioideae, Dialioideae and Duparquetioideae, and the nonmimosoid Caesalpinioideae. However, although they might also be considered as housing their symbionts within FTs, the filamentous nature of Frankia precludes it from forming symbiosomes. Furthermore, the ability of Frankia to fix N2 ex planta and regulate gaseous and nutrient exchange via vesicles in nodules (Casuarina and Allocasuarina in the Fagales being the exceptions in that Frankia does not form vesicles in the nodules, and the host regulates gaseous exchange) means that Frankia has a fundamentally different relationship with its host compared to that between rhizobia and legumes (Pawlowski & Demchenko, 2012; Ardley & Sprent, 2021). Although losses of nodulation amongst actinorhizal lineages are the result of evolutionary drivers that are not currently well understood, it is possible that intimacy (or lack thereof) in terms of the interface between the two symbionts is not an important factor.
It is well established that N2‐fixation is energy‐demanding, limited by photosynthesis, and confers fitness advantages only when nitrogen is limiting and when the benefits derived from greater availability of nitrogen (e.g. in fostering higher photosynthetic rates in N2‐fixing plants) are greater than the costs of photosynthetic carbon (McKey, 1994; Hoffman et al., 2014; Taylor & Menge, 2018; van Velzen et al., 2018a). Additionally, there is experimental evidence showing that legumes increase N2‐fixation at elevated CO2 levels and that nitrogenase activity declines rapidly above 35°C and below 25°C (Trinick, 1980). Taken together, this suggests a greater advantage in being an N2‐fixer under early Cenozoic CO2 levels and temperatures (Rogers et al., 2009; Chen & Markham, 2021), and for those advantages to be preferentially retained in the tropics and subtropics, where FT‐type nodulators are largely restricted. Falling atmospheric CO2 levels and temperatures through the Cenozoic could have triggered global evolutionary losses of nodulation across the N2‐fixing clade (as suggested by van Velzen et al., 2018a) and we show that maximum ages of losses of nodulation across Caesalpinioideae are widely scattered from the late Palaeocene to the late Oligocene, 59–24 Ma (Fig. 1). However, it is important to consider that these are maximum ages rather than precise indicators of the timing of losses, and furthermore, the number of estimated losses per lineage is the minimum number of losses to explain the observed pattern at the tips, given the taxa sampled here.
It has long been recognized that evolutionary conflicts arise between hosts and symbionts over symbiont mixing, proliferation and transmission (Frank, 1996) because the presence of multiple, genetically heterogeneous symbiont strains within a host will cause symbionts to evolve traits that increase symbiont proliferation, competition and conflict, but decrease the efficiency of the symbiosis (Frank, 1996). There is clear evidence that this happens in the rhizobia–legume symbiosis (Oono et al., 2009; Sachs et al., 2018). In response to such conflicts, hosts have evolved ways to control symbiont proliferation (i.e. terminally differentiated bacteroids lose their ability to reproduce) (Mergaert et al., 2006; De La Peña et al., 2018; Ardley & Sprent, 2021), discriminate among symbionts (Yang et al., 2017; De La Peña et al., 2018; Ardley & Sprent, 2021) and penalize noncooperating symbionts (Kiers et al., 2003; Oono et al., 2009; Ardley & Sprent, 2021). All these approaches are more effective when symbionts are compartmentalized within hosts, and all occur in the rhizobia–legume symbiosis (Sachs et al., 2018), although almost all evidence is from SYM‐type papilionoids. We suggest that the anatomical differences between legume FTs and SYMs represent different degrees to which symbionts are effectively compartmentalized, as argued by Chomicki et al. (2020). The SYM‐type nodule, in which the microsymbiont is released from the wall‐bound IT into membrane‐bound symbiosomes within the host cell, allows for a more intimate and potentially more effective and enduring symbiotic partnership where the plant has invested in the establishment of an N2‐fixing ‘organelle’, which Parniske (2018) argued has only occurred in legumes and in the Gunnera–Nostoc symbiosis. In SYM‐type nodules, the plant host assumes greater control of the microsymbiont and supplies more of the components required for bacteroid metabolism and N2‐fixation (Hakoyama et al., 2009; Udvardi & Poole, 2013). This more intimate endosymbiosis reaches its pinnacle in the Inverted Repeat Lacking Clade (IRLC) of Papilionoideae, in which swollen endoreduplicated bacteroids that have lost their capacity for free‐living growth, but which are highly efficient at fixing N, are prevalent (Oono et al., 2009; Ardley & Sprent, 2021). The bacteroid in the FT, although surrounded by a membrane analogous to the SYM membrane, remains surrounded by a cell wall, albeit a thin one which contains little pectin, which means that it is extracellular (i.e. in the apoplast). Thus, while FTs represent a modest degree of compartmentalization, at least in Parasponia there is evidence to suggest that FTs are not effective in controlling growth of inefficient rhizobial strains (Op den Camp et al., 2012). These differing degrees of compartmentalization provide a compelling reason why SYM‐type nodulators, especially those in the IRLC (Westhoek et al., 2021), are less likely to be affected by cheating or infiltration by inefficient microsymbionts compared to FT‐type nodulator hosts, which remain in a ‘looser’ relationship with their symbionts.
It might be assumed that the wall of the FT would also present an additional barrier in terms of nodule O2 relationships and host–symbiont nutrient exchange. However, the FT wall is thin, consisting mainly of cellulose, hemicelluloses and AGP, but with reduced levels of homogalacturonan (HG) pectin components compared to the thicker and stiffer IT wall (this study), and hence presumably relatively permeable to C4‐dicarboxylates and ammonia (Brewin, 2004). The presence of abundant leghaemoglobin (Lb) suggests that rhizobial FT nodules are not obviously different from SYM‐type nodules in their O2 exchange. We propose that the role of the thin‐walled FT appears to be protective; that is, it prevents the undifferentiated bacteroids going ‘rogue’ and proliferating within the host cell, but in parallel, prevents the plant from identifying them as pathogens and attacking them. In all other respects, FT‐type nodules are similar to SYM‐types in still possessing a symbiosome membrane which surrounds the FT and is the real interface of nutrient exchange between the two partners. In short, the FT represents an example of a symbiosis that functions well enough to benefit both partners, but is a looser, more metabolically independent association.
SYM‐type nodules may accommodate a larger diversity of symbionts and facilitate adaptation to temperate climates. This is in line with the greater diversity of α‐ and β‐rhizobial types in SYM‐type nodules and the wider geographical distribution and environmental span of SYM‐type nodulating legumes (Sprent et al., 2017; Ardley & Sprent, 2021), compared to FT‐type nodules whose microsymbionts appear to be largely limited to Bradyrhizobium (Fonseca et al., 2012; Parker, 2015; Ardley & Sprent, 2021) and which are mostly confined to the tropics and subtropics where bradyrhizobia are dominant and widespread (Parker, 2015; Meng et al., 2019).
Despite the significantly lower rates of loss of nodulation in mimosoids with SYM‐type nodules compared to FTs in the remaining Caesalpinioideae, SYM‐type nodulation is not impervious to evolutionary loss. Our reconstruction documents five losses of nodulation within the Mimosoid clade: on the branches subtending the Amblyogonocarpus + Adenanthera clade, and the genera Parkia, Cylicodiscus, Newtonia and Zapoteca (Fig. 1; Table S3). These losses in ancestrally SYM‐type lineages suggest that even the advantages conferred by stricter SYM‐type compartmentalization can be insufficient to prevent losses of nodulation. Within the genus Senegalia, a small subset of species have apparently lost the ability to nodulate (Sprent, 2001, 2009). Current phylogenies imply that nodulation has been lost in species of each of the two main subclades within Senegalia, offering a useful system for understanding environmental or other factors associated with loss of nodulation.
Conclusions
The evolution of the symbiosome in species‐rich nodulating legume lineages offers a compelling explanation for the well‐known but poorly understood highly uneven distribution of nodulating species richness across the N2‐fixing clade. While nodulation has been suggested as a possible key innovation underpinning the evolutionary success of legumes, our results suggest that it was adoption of SYM‐type nodules and the innovation of the symbiosome that underpinned the stabilization of N2‐fixation and potentially contributed to massive diversification of species within Caesalpinioideae and Papilionoideae, the two most diverse and geographically widespread subfamilies of legumes. Furthermore, the greater propensity of the FT‐type nodule to be secondarily lost and for SYM‐type lineages to persist and diversify provides a potent example of the long‐term evolutionary benefits and outcomes of stricter compartmentalization in symbiotic cooperation, as suggested by Chomicki et al. (2020).
We show that the grade of Caesalpinioideae lineages subtending the Mimosoid clade is a hotspot of evolutionary transitions between phylogenetically intermingled nodulating and nonnodulating lineages (Fig. 1), including two independent transitions from FT‐ to SYM‐type nodules as well as numerous losses of nodulation. The phylogeny and detailed evolutionary trajectories of nodulation and nodule anatomies presented here provide a robust framework for comparative genomic analyses of FT and SYM nodulating and nonnodulating lineages across Caesalpinioideae. This includes Chamaecrista, the most species‐rich genus in the nonmimosoid grade of Caesalpinioideae, and the only nodulating genus in the subfamily which contains species with both SYM‐and FT‐type nodules (Naisbitt et al., 1992), thus representing a second possible transition from FT to SYM.
Author contributions
EJMK, JJR, CEH and EKJ designed the study and interpreted the results, JJR carried out the phylogenetic analysis, SMF, EKJ, EG, KMW and YP performed anatomical analyses, SMF, EKJ, EG, DC, GKDA, J Akomatey, NT, HSG, YP, MM, NT, PS, HCL and CEZ sampled nodules in the field, and SMF, EJMK, JJR, EKJ, J Ardley, DC, EG, YP, JIS and CEH wrote the paper.
Supporting information
Acknowledgements
We thank Gwilym Lewis for help with identification of plants, the Millennium Seedbank for supplying seeds and colleagues who have helped sample material used in this study. Jordan Price is thanked for his expert advice on actinorhizal symbioses. This work was supported by the research project Engineering Nitrogen Symbiosis for Africa (ENSA), which is funded by a grant to the University of Cambridge by the Bill & Melinda Gates Foundation and the Foreign, Commonwealth & Development Office (FCDO), the Swiss National Science Foundation (grants 310003A_156140 and 31003A_182453/1 to CEH), CNPq grant 312125/2020‐8 to SMF, and Fundação de Amparo à Pesquisa do Estado da Bahia (FAPESB, grant APP0037/2016 to DC).
Contributor Information
Colin E. Hughes, Email: colin.hughes@systbot.uzh.ch.
Euan K. James, Email: euan.james@hutton.ac.uk.
Data availability
The data that support the findings of this study are available in the Supporting Information of this article.
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Data Availability Statement
The data that support the findings of this study are available in the Supporting Information of this article.