2018 Volume 33 Issue 1 Pages 89-97
Light-driven ion-pumping rhodopsins are widely distributed among bacteria, archaea, and eukaryotes in the euphotic zone of the aquatic environment. H+-pumping rhodopsin (proteorhodopsin: PR), Na+-pumping rhodopsin (NaR), and Cl−-pumping rhodopsin (ClR) have been found in marine bacteria, which suggests that these genes evolved independently in the ocean. Putative microbial rhodopsin genes were identified in the genome sequences of marine Cytophagia. In the present study, one of these genes was heterologously expressed in Escherichia coli cells and the rhodopsin protein named Rubricoccus marinus halorhodopsin (RmHR) was identified as a light-driven inward Cl− pump. Spectroscopic assays showed that the estimated dissociation constant (Kd,int.) of this rhodopsin was similar to that of haloarchaeal halorhodopsin (HR), while the Cl−-transporting photoreaction mechanism of this rhodopsin was similar to that of HR, but different to that of the already-known marine bacterial ClR. This amino acid sequence similarity also suggested that this rhodopsin is similar to haloarchaeal HR and cyanobacterial HRs (e.g., SyHR and MrHR). Additionally, a phylogenetic analysis revealed that retinal biosynthesis pathway genes (blh and crtY) belong to a phylogenetic lineage of haloarchaea, indicating that these marine Cytophagia acquired rhodopsin-related genes from haloarchaea by lateral gene transfer. Based on these results, we concluded that inward Cl−-pumping rhodopsin is present in genera of the class Cytophagia and may have the same evolutionary origins as haloarchaeal HR.
Rhodopsins are seven-transmembrane proteins composed of a protein moiety (opsin) and light-absorbing chromophore (retinal). They are widely distributed among animals and prokaryotes and have been classified into two groups: type-1 (microbial origin) and type-2 (eukaryotic origin). Microbial type-1 rhodopsins were initially discovered in extremely halophilic archaea: a light-driven outward H+-pumping rhodopsin (bacteriorhodopsin [BR] ), inward Cl−-pumping rhodopsin (halorhodopsin [HR] ), and light-sensing rhodopsins (sensory rhodopsin I and II [SRI and SRII]) (31). In 2000, an H+-pumping rhodopsin was also found in a marine bacterial genomic fragment using a metagenomic approach and was named proteorhodopsin (PR) (4). Recent studies have shown that PR genes are widely present among marine bacteria and archaea inhabiting the euphotic layer of the ocean (7). Furthermore, outward Na+-pumping rhodopsin (NaR) (15) and inward Cl−-pumping rhodopsin (ClR) (43) were discovered in marine bacteria. Of note, BR and HR of haloarchaea and PR and ClR of marine bacteria belong to distinct phylogenetic lineages, suggesting that these ion-pumping rhodopsins evolved independently in their respective habitats.
The family Rhodothermaceae belongs to the class Cytophagia in the phylum Bacteroidetes. This family includes 7 genera (Longimonas , Longibacter , Rhodothermus , Rubricoccus , Rubrivirga , Salinibacter , and Salisaeta ) and has been found in diverse environments, e.g., hydrothermal vents, hypersaline environments, and oceans. The genera Longimonas, Longibacter, Salisaeta, and Salinibacter include halophilic bacteria, and members of the genus Rhodothermus are thermophiles. In contrast, members of the genera Rubricoccus and Rubrivirga have been isolated from surface or deep seawater and are not extremophiles. Salinibacter, a halophilic bacterium, dominates with halophilic archaea in hypersaline environments (5–25% according to fluorescence in situ hybridization  and 7–9% according to a metagenomic analysis ). Previous studies reported that Salinibacter ruber M31T carries multiple rhodopsin genes: xanthorhodopsin (XR), HR, and SRI (23). In addition, a genomic analysis suggested that S. ruber acquired not only the HR and SRI genes, but also many other genes that are necessary for salt adaptation from halophilic archaea by lateral gene transfer (LGT) because both of these halophilic prokaryotes inhabit and dominate the same environment (23).
Following the genome information of Rubricoccus marinus SG-29T (24), we herein report two genome sequences of Rubrivirga marina SAORIC-28T and R. profundi SAORIC-476T. A genomic analysis revealed that R. marinus SG-29T and R. marina SAORIC-28T have five rhodopsin genes belonging to two different clusters: one is included in the xenorhodopsin (XeR) cluster, and the other is a unique cluster consisting of rhodopsin containing a TSA motif (amino acid residues 85, 89, and 96 in BR numbering). A phylogenetic analysis showed that this unique rhodopsin cluster is closely related to the HR of halophilic archaea. Therefore, we named these HR-like rhodopsins RmHR (R. marinus SG-29T halorhodopsin), R28HR1, and R28HR2 (R. marina SAORIC-28T halorhodopsin 1 and 2). A functional analysis using heterologously expressed RmHR was subsequently conducted to identify its ion specificity. We further performed a spectroscopic analysis using purified RmHR to clarify its spectroscopic characteristics because even rhodopsins with the same ion transport specificity have intermediates with different ion affinities and structural changes, and the properties are important factors that define rhodopsins. In the present study, we performed genomic and phylogenetic analyses, and also characterized RmHR spectroscopically, and these properties were compared with those of known microbial rhodopsins.
R. marinus SG-29T was isolated from surface seawater (30° 40′ N, 138° 00′ E; depth 50 m), and additional information has been reported previously (27). R. marina SAORIC-28T was isolated from a deep seawater sample obtained from the western North Pacific Ocean (32° 00′ N, 138° 13′ E; depth 3000 m) by the R/V Tansei maru (Atmosphere and Ocean Research Institute, The University of Tokyo and Japan Agency for Marine-Earth Science and Technology [JAMSTEC]) on 3 July 2010 (KT-10-12 cruise). R. profundi SAORIC-476T was isolated from a deep seawater sample obtained from the western North Pacific Ocean (32° 00′ N, 140° 00′ E; depth 3000 m) during the research cruise (MR-11-05) of R/V Mirai (JAMSTEC) in May 2011. Details of the culture conditions and phenotypic traits of these strains have been described previously (28, 30). The genomic DNA of strains SAORIC-28T and SAORIC-476T was extracted using phenol-chloroform and ethanol precipitation (21). Library preparation was performed for strain SAORIC-28T, as previously reported for strain SG-29T (24). A KAPA HyperPlus Kit (Kapa Biosystems, Boston, MA, USA) was used for library preparation for strain SAORIC-476T. Each end of the libraries (300 bp) of SAORIC-28T and SAORIC-476T were sequenced on a MiSeq instrument with MiSeq Reagent kit version 3 (Illumina, San Diego, CA, USA).
The DNA fragments encoding RmHR, R28HR1, and R28HR2 were chemically synthesized by Eurofins Genomics (Eurofins Genomics, Tokyo, Japan) with codon optimization for Escherichia coli. These gene fragments were inserted into the NdeI and XhoI sites of the pET21a vectors (Novagen, Darmstadt, Germany); consequently, the plasmids encoded RmHR, R28HR1, and R28HR2 with hexahistidines at the C terminus. The vectors were transformed into E. coli strain C41 (DE3) (Lucigen, Middleton, WI, USA). E. coli cells with the plasmid were incubated at 37°C on an LB medium agar plate supplemented with ampicillin (final concentration, 100 μg mL−1). Cells carrying the plasmid were then grown at 37°C in 200 mL of 2×YT medium supplemented with ampicillin (final concentration, 100 μg mL−1), and protein expression was induced at an OD 660 nm (OD660) of 0.4–0.6 with 0.2 mM isopropyl β-D-1-thiogalactopyranoside (IPTG) and 10 μM all-trans-retinal (Sigma-Aldrich, St Louis, MO, USA). Rhodopsin-expressing cells were collected by centrifugation (8,000×g for 3 min), washed three times with 100 mM NaCl, and then re-suspended in the solvent for measurement. The light source was a 300 W xenon lamp (MAX-303; Asahi Spectra, Tokyo, Japan), and 6 mL of the cell suspension was initially placed in the dark and then irradiated through a 520±10 nm bandpass filter (MX0520; Asahi Spectra) for 3 min. pH was measured using a pH meter (LAQUA F-72; HORIBA, Kyoto, Japan). Measurements were repeated under the same conditions after the addition of the protonophore carbonyl cyanide m-chlorophenylhydrazone (CCCP, final concentration, 30 μM). All measurements were performed at 4°C. Different solutes (100 mM NaCl, KCl, MgCl2, NaBr, NaI, NaNO3, and Na2SO4) were used in the ion selectivity analysis of RmHR.
E. coli BL21 (DE3) cells were used for the functional expression of RmHR as a recombinant protein. The procedures for protein expression and purification were the same as those described in our previous study (35). In spectroscopic measurements, the buffer was sufficiently exchanged by centrifugation (AmiconUltra centrifuge unit; 30,000 molecular weight cut-off, Merck Millipore, Bedford, MA, USA) and the PD-10 column (GE Healthcare, Waukesha, WI, USA) with 10 mM 3-(N-morpholino)-propanesulfonic acid (MOPS) buffer (Dojindo Laboratories, Kumamoto, Japan) containing 0.1% (w/v) n-dodecyl-β-D-maltoside (DDM, Dojindo Laboratories) and NaCl at the desired concentrations (1 mM to 4 M). In order to maintain ionic strength at 4 M, Na2SO4 was added to the samples at the desired concentrations (0–1.333 M). Neither Na+ nor SO42− was a substrate ion for RmHR (see the Results and Discussion section). The optical density of DDM-solubilized RmHR was adjusted to approximately 0.5 optical density (OD) at its absorption maximum (approx. 10 μM).
Retinal isomer compositions were analyzed using normal-phase high-performance liquid chromatography (HPLC). The procedures for the retinal oxime extraction and HPLC analysis were the same as those described in our previous study (35). Regarding measurements under dark conditions, the sample was maintained in the dark for more than 1 week. In measurements under light conditions, the sample was illuminated with 540±10 nm light for 5 min before retinal oxime extraction. The retinal oxime extracted from the purple membrane (PM) containing Halobacterium salinarum bacteriorhodopsin (HsBR) was used as a reference. The eluting retinal oxime was monitored by its absorption at 360 nm. The flow rate was 1 mL/min. All measurements were performed at 25°C.
All UV-Vis spectra were recorded at 25°C using a UV-1800 spectrophotometer (Shimadzu, Kyoto, Japan). In the Cl− titration experiment, the absorption maximum wavelength (λmax) of RmHR was plotted against the logarithm of the Cl− concentration ([Cl−]) and analyzed by fitting the data to the following Hill equation:
where a, b, Kd, and n represent the offset, the amplitude of the λmax change, the dissociation constant for Cl−, and the Hill coefficient, respectively. In the pH titration experiment, the sample was suspended in a 6-mix buffer (0.89 mM citrate, 0.89 mM MES, 1.1 mM TES, 0.78 mM TAPS, 1.1 mM CHES, 0.33 mM CAPS; MES, TES, TAPS, CHES, and CAPS are Good’s buffers and were purchased from Dojindo Laboratories) (34) containing 0.05% DDM, 0–4 M NaCl, and 0–1.333 M Na2SO4. The initial pH was approximately 3.8 and was then adjusted to the desired value by adding a very small amount of 2 M NaOH, followed by measurements of the UV-Vis absorption spectrum. The concentration change in the RmHR sample was almost negligible. The acid dissociation constant, pKa, of the protonated Schiff base of the retinal chromophore was estimated by fitting the data to the Henderson-Hasselbalch equation:
where pH and ΔA are the adjusted pH value and absorption change at 380 nm, which corresponds to the deprotonated Schiff base, respectively.
Time-dependent changes in absorbance were measured by flash-photolysis using a homemade computer-controlled apparatus equipped with a Nd:YAG laser (5 mJ pulse−1, 532 nm, 7 ns) as an actinic light source as described previously (18, 35). Due to the setting for the response time (0.5 μs) of a homemade I-V converter, a large scattering artifact from the laser flash appeared before 10 μs. Therefore, plots were started from 10 μs. Time-dependent changes in absorbance were measured from 400 to 710 nm at 10-nm intervals. Data before the laser pulse were adopted as a baseline. In order to improve the signal-to-noise ratio, the results of 30 flashes were averaged at each wavelength. No further data processing was applied. The temperature was kept at 20°C using a thermostat.
where P0 and P1–P4 represent the unphotolyzed original pigment and the 1st–4th kinetically defined states, respectively. All data on time-dependent changes in absorbance were simultaneously fit with a sum of 4 exponential decay functions. The appropriate number of exponents was selected based on reductions in the standard deviation of the residuals. The P1–P4 states were allowed to contain a few physically defined photointermediates such as L, N, and O with individual absorption maxima when a quasi-equilibrium state existed between them. The time constants τ1–τ4 and the absorbance differences Δɛ1–Δɛ4 between the P1–P4 states and the original P0 state were assessed according to the fitting results. Independently, the pure retinal spectrum of the P0 state was extracted from the UV-Vis absorption spectrum of the initial state (unphotolyzed) RmHR by spectral decomposition using the skewed Gaussian function as described previously (10). Finally, the absolute spectra of each P1–P4 state were obtained by adding the P0 spectrum to each absorbance difference Δɛ1–Δɛ4.
As described in the Results and Discussion section, the P3 state was obtained as a quasi-equilibrium mixture of N-like and O-like intermediates with relative fractions that were dependent on the Cl− concentration. P3 state spectra contained not only the main absorption bands of the N-like and O-like intermediates, but also the respective β-bands. The procedures for the spectral decomposition of the P3 state were the same as those described in previous studies (10, 29). Assuming both β-bands are identical to that of the P0 state, the spectrum of the P3 state is described as:
where f, Abs (N, λ), Abs (O, λ), and Abs (β, λ) represent the fraction of the N-like intermediate, the main absorption band of the N-like intermediate, the main absorption band of the O-like intermediate, and the β-band, respectively. We employed skewed Gaussian functions to describe these three absorption bands and then decomposed the spectrum of the P3 state to estimate f, which we assumed to be the only parameter dependent on the Cl− concentration. The fractions of the N-like and O-like intermediates were plotted against the Cl− concentration, and data were simultaneously analyzed by the Hill equation as follows:
where a, b, Kd, and n represent the offset, amplitude of the λmax change, dissociation constant for Cl−, and Hill coefficient, respectively.
Multiple alignments of amino acid sequences were performed using the CLUSTALW option in MEGA 6.0 software (32). Phylogenetic trees were constructed using the maximum-likelihood (ML) method (5) with 1,000 bootstrap replications (6). The nucleotide sequences of 16S rRNA and the amino acid sequences of rhodopsins, 15,15′-β-carotene dioxygenase (blh), and lycopene cyclase (crtY and crtYcd) genes were collected from the NCBI database and RAST annotated sequences for the genera Rubricoccus and Rubrivirga. In order to compare gene synteny around the Cl−-pumping rhodopsin gene and blh gene, we acquired the genomes of H. salinarum R1, S. ruber M31T, Synechocystis sp. PCC 7506, Mastigocladopsis repens PCC 10914, Salisaeta longa DSM 21114T, and Rhodothermus marinus DSM 4252T from the NCBI RefSeq database. The ortholog clustering of the CDSs of each genome was performed using eggNOG-mapper (13) and the bactNOG dataset in the eggNOG database, version 4.5 (14). We visualized the operon structure and colored each gene based on each eggNOG ortholog cluster using R software. In order to evaluate the potential LGT, a BLAST analysis was performed on the genomes of H. salinarum R1, genes with an e-value less than 1e-10 were counted, and a threshold with a sequence identity >50% was established. We used the genome family Rhodothermaceae, Cytophaga hutchinsonii ATCC 33406T, which is a type species of the class Cytophagia, Indibacter alkaliphilus LW1T, Spirosoma linguale DSM 74T, N. marinus S1-08T, and Flavobacterium aquatile LMG 4008T. Since I. alkaliphilus and S. linguale, belonging to the class Cytophagia, have a rhodopsin gene, these genome data were used for this assay. Furthermore, because N. marinus is a marine flavobacterium with the ClR gene and F. aquatile is a type species of the class Flavobacteriia, these genome data were also used.
A previous study showed that R. marinus SG-29T has a 4.43-Mbp chromosome encoding 3847 CDSs (24). The present genome sequence analysis of R. marina SAORIC-28T and R. profundi SAORIC-476T revealed that these strains have 4.98 Mbp and 4.48 Mbp chromosomes encoding 4267 and 3842 CDSs, respectively (Table S1). The G+C contents of both strains from the genus Rubrivirga were two of the highest (72.5% and 71.3%) among the available genomes of class Cytophagia in the NCBI database. The genera Rubrivirga and Rubricoccus belong to the family Rhodothermaceae, and the 16S rRNA phylogenetic tree is shown in Fig. 1. This family contains members of thermophilic (genus Rhodothermus), halophilic (genera Salinibacter, Salisaeta, Longimonas, and Longibacter), and slightly halophilic (genera Rubricoccus and Rubrivirga, isolated from ocean) strains. Growth ranges for the NaCl concentration of thermophilic strains were similar to those of the genera Rubricoccus and Rubrivirga (Fig. 1). In contrast, halophilic bacteria in the family Rhodothermaceae grew under high-salinity conditions (20–30%). In addition, the lower limit of the growth range for NaCl of the genera Longimonas, Longibacter, and Salisaeta (2–4%), was lower than that of the genus Salinibacter (12–15%). The temperature growth range for the genera Rubricoccus and Rubrivirga was approximately 4–42°C (Fig. 1). In contrast, halophilic Rhodothermaceae strains grew at 20–50°C, and this range was between the temperature growth range for thermophiles (50–85°C) and marine isolates (4–42°C). These physiological traits clearly showed that the family Rhodothermaceae contained two different types of extremophiles, indicating that the common ancestor of this family was a halophilic or thermophilic bacterium. Therefore, the genera Rubricoccus and Rubrivirga with members that inhabit the ocean may have a higher G+C content in class Cytophagia as a remnant of their ancestors.
Maximum-likelihood phylogenetic tree based on 16S rRNA gene sequences. Phylogenetic tree of 16S rRNA showing the taxonomic positions of strains SG-29T, SAORIC-28T, and SAORIC-476T among related species of the family Rhodothermaceae in the classes Cytophagia and Sphingobacteria. The habitats of each strain are indicated by different-colored squares. The red and open circles indicate strains containing the rhodopsin gene and no rhodopsin gene, respectively. The G+C content and growth range for temperature and NaCl concentrations are also shown on the right side. Black closed circles indicate G+C content of each strain. ND: No genome data.
The genome sequence analysis showed that the genomes of R. marinus SG-29T and R. marina SAORIC-28T encoded two different types of rhodopsin genes (RmXeR [WP_094549673] and RmHR [WP_094550238]) and three rhodopsin genes (R28XeR [WP_095509440], R28HR1 [WP_095509924], and R28HR2 [WP_095512583]), respectively. The identities of amino acid sequences among RmHR, R28HR1, and R28HR2 were 73% (RmHR-R28HR1), 62% (RmHR-R28HR2), and 57% (R28HR1-R28HR2) respectively. No rhodopsin gene was found in the genome of R. profundi SAORIC-476T. Although R28HR1 and R28HR2 were found from the deepsea isolate, it currently remains unclear whether these are deep-sea adapted rhodopsins because the habitat of the genus Rubrivirga is not yet understood. In the BLASTP search against the metagenome database (env_nr), no sequence with >50% identity with RmHR was found. This result implies that the RmHR gene is very rare in the marine environment. In the family Rhodothermaceae, four strains (S. ruber M31T, S. longa DSM 21114T, R. marinus SG-29T, and R. marina SAORIC-28T) have rhodopsin genes. In contrast, no rhodopsin gene was found in the two thermophilic strains belonging to the genus Rhodothermus (Fig. 1). A recent study showed that RmXeR of SG-29T functions as a light-driven inward proton pump (17). R28XeR also belongs to the same cluster of RmXeR, suggesting that the function of R28XeR is an inward H+ pump. RmHR, R28HR1, and R28HR2 formed a unique cluster close to HR and SyHR (Fig. 2 and S1). Although HR and SyHR were discovered from halophilic prokaryotes and a freshwater cyanobacterium, RmHR, R28HR1, and R28HR2 formed a unique marine bacterial cluster. RmHR and R28HR1 had the same TSA motif as HR, and R28HR2 has TTD motif sequences (Table 1). In contrast, cyanobacterial HRs had the TSD, TSV, or TSL motif sequence (9).
Unrooted maximum-likelihood phylogenetic tree of microbial rhodopsins. (A) Amino acid sequences of microbial rhodopsins were aligned using CLUSTALW, and evolutionary distances were estimated using the LG with Freg model. The tree was constructed using bootstrap values based on 1,000 replications; evolutionary analyses were conducted in MEGA 6.0. All rhodopsin amino acid sequence data used in this study were obtained from the public database (http://www.ncbi.nlm.nih.gov/). Dark gray indicates the clade consisting of the freshwater cyanobacterial rhodopsin clade, and light gray indicates halorhodopsin. An open circle and closed gray circle indicate the positions of strain SG-29T and SAORIC-28T, respectively. Sodium ion pump rhodopsin (NaR); chloride ion pump rhodopsin (ClR); xanthorhodopsin-like rhodopsin (XLR); proteorhodopsin (PR); xenorhodopsin (XeR); sensory rhodopsin (SR); bacteriorhodopsin (BR); halorhodopsin (HR). The motif sequence (amino acid residues 85, 89, and 96 in BR numbering) is shown under the rhodopsin name. (B) Detailed phylogenetic tree of the SR, BR, HR, cyanobacterial HR, and RmHR homologues. The habitats of each strain are indicated by squares of different colors. Bootstrap values >80% are indicated as a percentage of the replicates tested. Asterisk represents the strain that was isolated from seawater by using medium for freshwater cyanobacteria.
In order to clarify the function of this unique rhodopsin cluster, codon-optimized RmHR, R28HR1, and R28HR2 genes were chemically synthesized and each gene was heterologously overexpressed in E. coli. Light-induced pH changes were observed in suspensions of E. coli cells expressing each gene in 100 mM NaCl. However, light-induced pH changes in R28HR1 were smaller than those in RmHR, and were not observed in R28HR2. Therefore, RmHR was used in subsequent analyses. Light-induced alkalization was observed in 100 mM NaCl, and this pH change was not abolished by the addition of CCCP (Fig. 3A). Since CCCP is a protonophore, this alkalization may be explained by passive proton influx due to the negative membrane potential, which was created by outward Na+ or inward Cl− translocation. In order to elucidate the ion selectivity of RmHR, we performed similar observations in different salt solutions (Fig. 3B). The signal almost disappeared in 100 mM NaI and Na2SO4, suggesting that RmHR cannot transport Na+. In contrast, strong signals were observed in 100 mM KCl, NaBr, and MgCl2, and a slight pH change was noted in 100 mM NaNO3. These anion-dependent transport properties are very similar to those of archaeal HRs in halophilic archaea, suggesting that RmHR functions as a light-driven inward anion (Cl−, Br−, and NO3−) pump.
Anion transport activity of RmHR. Light-induced pH changes in E. coli cell suspensions expressing RmHR in solutions containing (A) 100 mM NaCl without (black solid line) and with (gray broken line) 30 μM CCCP and (B) 100 mM KCl, MgCl2, NaBr, NaI, NaNO3, and Na2SO4 without CCCP. The cell suspension was illuminated with green light (520 nm). Temperature was maintained at 4°C. The word “div.” represents division.
In order to investigate the spectroscopic properties of RmHR, we prepared a detergent DDM-solubilized sample. Under this condition, the results described below were able to be precisely compared to those of all the other anion-pumping rhodopsins investigated, such as Natronomonas pharaonis halorhodopsin (NpHR), H. salinarum halorhodopsin (HsHR), Nonlabens marinus S1-08T rhodopsin 3 (NM-R3), Synechocystis sp. PCC 7509 halorhodopsin (SyHR), and Mastigocladopsis repens PCC 10914 halorhodopsin (MrHR) (11, 25, 33, 35, 42). Based on this background, we used DDM-solubilized RmHR in the subsequent spectroscopic analysis. We also focused on the photochemical properties of RmHR in the presence of NaCl because Cl− is considered to be a candidate substrate anion for RmHR in the native habitat of R. marinus SG-29T (Cl− concentration of approximately 500 mM).
We initially examined the retinal isomer composition of RmHR under dark and light conditions in the presence of 1 M NaCl. As shown in Fig. S2A, RmHR predominantly possesses all-trans retinal as a chromophore, which is responsible for the light-driven anion pump function, at 99.6 and 96.2% under dark and light conditions, respectively. This property is the same as those of the other anion-pumping rhodopsins reported to date (11, 25, 33, 35). On the other hand, another rhodopsin encoded in the R. marinus SG-29T gene (RmXeR) showed a light-dependent retinal composition change in the initial state (75 and 45% of all-trans retinal under dark and light conditions, respectively) (17). The biological significance of RmXeR currently remains unclear.
In order to evaluate this feature in RmHR, we measured the UV-Vis absorption spectra under various Cl− concentrations ranging between 1 mM and 4 M (Fig. S2B). Many anionpumping rhodopsins show a spectral blue-shift upon substrate anion binding. In the experiment, ionic strength was maintained at 4 M by adding Na2SO4 at appropriate concentrations because in many Cl−-pumping rhodopsins, Cl− binding reaches a plateau at 4 M and SO42− is not a substrate ion for RmHR, as shown in Fig. 3B. As shown in Fig. S2B, RmHR exhibited a Cl−-dependent spectral blue-shift from 550 nm in the presence of 1 mM Cl− to 542 nm in the presence of 4 M Cl−. Based on this dependency, Cl−-binding affinity in the initial state (practically the dissociation constant, Kd,int.) was estimated to be 7.6±1.7 mM by the Hill equation (Fig. S2C). The Hill coefficient was 1.2±0.23, indicating positive cooperativity for Cl− binding. The estimated Kd,int. value of RmHR was in the same order as those of NpHR, HsHR, and MrHR (2–6 mM) (10, 11, 18, 33, 42), but was approximately 100-fold lower than that of SyHR (approximately 0.1 mM) (25) and approximately 3- and 5-fold larger than those of NM-R3 (24 mM) and Fulvimarina pelagi HTCC 2506T rhodopsin (FR) (84 mM), respectively (16, 35). In addition, the acid dissociation constant, pKa, of the Schiff base was dependent on the Cl− concentration (Fig. S2D), which is similar to archaeal HsHR and NpHR (39). At low concentrations of NaCl (0 - several tens of mM), the absorption band of the deprotonated Schiff base appeared in the shorter wavelength region at approximately 380 nm (Fig. S2B). Therefore, subsequent experiments were performed in the presence of more than 100 mM NaCl.
The Cl−-transporting photoreaction, called a photocycle, of RmHR was analyzed using a time-resolved flash-photolysis technique. Fig. S3A shows the flash-induced light-minusdark difference absorption spectra in the 10-μs to 388-ms time domain. After flash excitation, photointermediates with absorption bands at approximately 460 nm and 610 nm, respectively, were generated with the concomitant disappearance of the initial state absorption band at approximately 550 nm. Time-dependent absorption changes in these three absorption bands are shown in Fig. S3B. Data were simultaneously fit to the exponential decay function with 4 exponents, which was the same number as NpHR (10, 18), indicating that RmHR passed through 4 kinetically intermediate states, P1–P4, in its photocycle. The time constants between each transition, τ1–τ4, were 0.105, 0.483, 2.14, and 23.5 ms, respectively. According to the sequential model (10, 18), we calculated the absolute spectra of the P1–P4 states of RmHR in the presence of 1,000 mM NaCl, as shown in Fig. S3C. The spectrum of P0 corresponded to the initial state pure absorption spectrum of RmHR, which was extracted from the experimentally measured absorption spectrum (see the Materials and Methods section). The P1 and P2 states each contained a blue-shifted photointermediate with a similar absorption maximum at 510 nm. Analogous to NpHR, we tentatively assigned these intermediates as L1- and L2-like, respectively. The following P3 state contained at least two photointermediates with absorption maxima at 520 and 590 nm, which we tentatively assigned as N- and O-like intermediates, respectively, by referring to the P3 state of NpHR. In the case of NpHR, the molar ratio of N and O changed in a Cl− concentration-dependent manner (10, 18). In order to evaluate this phenomenon, we performed flash photolysis measurements on RmHR with varying Cl− concentrations. It is important to note that the Cl− concentration-dependent absorption change was significant in the P3 state (Fig. S4). Fig. S3D shows the Cl−-dependent change in the molar ratio of N-like and O-like intermediates between 100 mM and 4 M NaCl. The fraction of the N-like intermediate increased with elevations in the Cl− concentration, indicating that this intermediate is the Cl−-binding form. In contrast, the fraction of the O-like intermediate decreased with the increase in the Cl− concentration, indicating that the O-like intermediate is the Cl−-releasing form. Data were simultaneously fit by the skewed Gaussian function in order to identify the fractions of the N-like and O-like intermediates. As shown in Fig. S3E, we plotted these fractions against NaCl concentrations and then estimated the dissociation constant for Cl− release, Kd,rel, as 308±45.6 mM using the Hill equation. The value was approximately 40-fold larger than that of the initial state (Kd,int.=7.6 [mM]), the behavior of which was the same as NpHR, whereas the magnitude of the change was different (Kd,int.=2 [mM] and Kd,rel=1.2 [M]) (33). In the P4 state (Fig. S3C), a photointermediate with the same absorption maximum at 540 nm as the initial state (P0) was identified, and we named it the RmHR′-intermediate by referring to other anion-pumping rhodopsins, including NpHR (18, 35). Analogous to NpHR, in the O-like-to-RmHR’ transition, Cl− was entered into the initial binding site on the extracellular side of RmHR, which was supported by the blue-shifted absorption from O-like to RmHR’ and the same absorption maximum of RmHR’ as that of the initial state. We summarized the Cl− transporting photocycle model of RmHR in Fig. S3F. The initially captured Cl− on the extracellular side of RmHR was transferred to the intracellular side in the L2-like-to-N-like transition and was then released into the intracellular bulk space in the N-like-to-O-like transition. The next Cl− was entered into the initial binding site through the intracellular side of the molecule in the O-like to RmHR’ and RmHR’ to initial state transitions. The mechanism was similar to that of NpHR (18), but significantly different from that of the bacterial anion pumps, NM-R3 and FR, which are evolutionally distant from RmHR (Table 2) (Fig. 2) (16, 35).
N.D. indicates “Not determined”.
Functional and spectroscopic analyses revealed that RmHR is a light-driven inward Cl−-pumping rhodopsin similar to the HR of halophilic archaea rather than to ClR (e.g., NM-R3 and FR) of marine flavobacteria. In order to further examine the evolutionary history of RmHR, we performed phylogenetic analyses on retinal biosynthesis pathway genes, such as crtY (lycopene cyclase) and blh (15,15′-β-carotene dioxygenase). The enzymes encoded by the crtY and blh genes catalyze the terminal cyclization reaction from all-trans-lycopene to all trans-β-carotene and cleave β-carotene to produce two molecules of all-trans-retinal as a chromophore of rhodopsin. ML phylogenetic trees based on the blh and crtY genes are shown in Fig. 4 and S5. Regarding SAORIC-476T, since this strain lacks rhodopsin and blh genes, only the crtY gene was used in this analysis. In the phylogenetic tree of the blh gene, although each cluster was mainly formed according to the taxonomic group, the blh genes of SG-29T and SAORIC-28T in the class Cytophagia belonged to the lineage containing halophilic archaea and bacteria (Fig. 4). The phylogenetic tree based on crtY showed that three clusters: Bacteroidetes crtY and Proteobacteria crtY and crtYcd, had formed, and the genes of strains SG-29T, SAORIC-28T, and SAORIC-476T were included in the crtYcd cluster (Fig. S5). Carotenoid cyclases such as crtY are considered to be diversified by LGT or gene duplication, and some Actinobacteria (20), archaea (12), and Bacteroidetes (19) contain crtYcd. Although the similarity between the crtYcd and crtY genes is not high, the crtYcd gene is in a carotenoid biosynthesis gene cluster and has been shown to encode an enzyme that functions as a lycopene cyclase-like crtY gene. Halophilic archaea, the genera Natronomonas, Halobacterium, and Haloarcula, and halophilic bacteria, S. ruber M31T and S. longa DSM 21114T, possess the crtYcd, but not crtY gene. Similar to the phylogenetic tree of the blh gene, the crtYcd genes of Rubricoccus and Rubrivirga were not close to the genes of the Bacteroidetes crtY clade, whereas these crtYcd genes were closely related to the halophilic archaeal ones. Although the family Rhodothermaceae belongs to the class Cytophagia in the phylum Bacteroidetes, blh and lycopene cyclase genes formed a phylogenetic lineage that is distinct from these genes in Bacteroidetes.
Unrooted maximum-likelihood phylogenetic tree of the blh gene. Amino acid sequences were aligned using CLUSTALW, and evolutionary distances were estimated using the LG with Freg model. The tree was constructed using bootstrap values based on 1,000 replications; evolutionary analyses were conducted in MEGA 6.0. (A) Open and closed gray circles indicate the positions of strains SG-29T and SAORIC-28T, respectively. (B) Detailed phylogenetic relationship of the blh gene among Flavobacteriia, Cytophagia, halophiles, strain SG-29T, and strain SAORIC-28T. Bootstrap values >80% are indicated as a percentage of the replicates tested.
Previous genomic and phylogenetic analyses showed that S. ruber M31T acquired several genes from halophilic archaea via LGT (23). Gene transfer beyond a domain may have occurred because Salinibacter and halophilic archaea dominate in the same niche, such as a hypersaline environment. The best example of this gene transfer is the HR gene shared by Salinibacter and halophilic archaea. In addition, not only this case, but also other genes (e.g., blh, crtYcd, the cytochrome c oxidase gene, and nitrous oxide reductase gene) were shared among halophilic bacteria and archaea. Our results based on the phylogenetic analysis suggest that the rhodopsin gene and its related genes were shared not only between Salinibacter and halophilic archaea, but also among those halophiles and marine bacteria (R. marinus SG-29T and R. marina SAORIC-28T). Furthermore, these results indicate that the common ancestor of the genera Rubricoccus and Rubrivirga acquired rhodopsin and its related genes from halophilic archaea via LGT in a hypersaline environment, as reported previously (23).
The results showing that several genes were shared among the halophiles, Rubricoccus and Rubrivirga, indicated that a common ancestor of strains SG-29T, SAORIC-28T, and SAORIC-476T inhabited the same environment, such as salt lakes, as halophiles. In order to clarify whether other genes were acquired together with the rhodopsin and blh genes, we compared the genomic flanking regions of these genes among the genera Rubricoccus and Rubrivirga and the strains possessing genes closely related to this rhodopsin or the blh gene (Fig. S6). The results of the analysis showed that there was low similarity around rhodopsin genes (Fig. S6A). This dissimilarity may suggest that only Cl−-pumping rhodopsin genes were acquired by LGT or that a gene transfer event has not recently occurred. The same analysis based on the blh gene also showed no remarkable similarity to the flanking regions of the rhodopsin gene. The flanking regions of R. profundi SAORIC-476T lacking the rhodopsin and blh genes showed the presence of multiple conserved genes between SAORIC-28T and SAORIC-476T (Fig. S6B). This result suggested that only the blh gene was deleted in SAORIC-476T or acquired in SAORIC-28T. The results of a BLAST analysis revealed that although the numbers of potential LGT of strains SG-29T, SAORIC-28T, and SAORIC-476T were lower than that of S. ruber M31T, these numbers were approximately 2- to 4-fold higher than other phylum Bacteroidetes strains (Fig. S7). This result suggests that genes in strains SG-29T, SAORIC-28T, and SAORIC-476T may be shared with H. salinarum, similar to S. ruber.
In conclusion, we herein report a novel light-driven inward Cl−-pumping rhodopsin (RmHR), similar to the HR of halophilic archaea, in marine isolates of the family Rhodothermaceae in the phylum Bacteroidetes. Spectroscopic assays also showed that the properties of RmHR resembled those of HR from the aspect of the intermediate states and mechanisms of Cl− uptake and release. Phylogenetic analyses revealed that strains of the genera Rubricoccus and Rubrivirga may have acquired some genes by LGT, including the rhodopsin and blh genes from halophilic archaea. These results suggest that these genera and halophilic archaea had once lived in the same environment. Collectively, the present results provide insights into gene sharing between marine bacteria and halophilic archaea and facilitate our understanding of the evolutionary processes occurring in the ecologically diverse environments of this family.
We are grateful to the captains and crews of R/V Mirai (JAMSTEC) and R/V Tansei Maru (Atmosphere and Ocean Research Institute, The University of Tokyo and JAMSTEC) for their assistance and support with sample collection. This work was supported by the Japan Society for the Promotion of Science (JSPS) to TT (15K18519) and SY (15H02800) and the Interdisciplinary Collaborative Research Program of the Atmosphere and Ocean Research Institute, the University of Tokyo. This work was also supported by JSTCREST and AMED to YS.