This review covers the properties of a retinal protein (ESR) from the psychrotrophic bacterium Exiguobacterium sibiricum that functions as a light-driven proton pump. The presence of a lysine residue at the position corresponding to intramolecular proton donor for the Schiff base represents a unique structural feature of ESR. We have shown that Lys96 successfully facilitates delivery of protons from the cytoplasmic surface to the Schiff base, thus acting as a proton donor in ESR. Since proton uptake during the photocycle precedes Schiff base reprotonation, we conclude that this residue is initially in the uncharged state and acquires a proton for a short time after Schiff base deprotonation and M intermediate formation. Involvement of Lys as a proton donor distinguishes ESR from the related retinal proteins — bacteriorhodopsin (BR), proteorhodopsin (PR), and xanthorhodopsin (XR), in which the donor function is performed by residues with a carboxyl side chain. Like other eubacterial proton pumps (PR and XR), ESR contains a histidine residue interacting with the proton acceptor Asp85. In contrast to PR, this interaction leads to shift of the acceptor’s pK a to more acidic pH, thus providing its ability to function over a wide pH range. The presence of a strong H-bond between Asp85 and His57, the structure of the proton-conducting pathways from cytoplasmic surface to the Schiff base and to extracellular surface, and other properties of ESR were demonstrated by solving its three-dimensional structure, which revealed several differences from known structures of BR and XR. The structure of ESR, its photocycle, and proton transfer reactions are discussed in comparison with homologous retinal proteins.
One of the distinctive features of eubacterial retinal-based proton pumps, proteorhodopsins, xanthorhodopsin, and others, is hydrogen bonding of the key aspartate residue, the counterion to the retinal Schiff base, to a histidine. We describe properties of the recently found eubacterium proton pump from Exiguobacterium sibiricum (named ESR) expressed in Escherichia coli, especially features that depend on Asp-His interaction, the protonation state of the key aspartate, Asp85, and its ability to accept a proton from the Schiff base during the photocycle. Proton pumping by liposomes and E. coli cells containing ESR occurs in a broad pH range above pH 4.5. Large light-induced pH changes indicate that ESR is a potent proton pump. Replacement of His57 with methionine or asparagine strongly affects the pH-dependent properties of ESR. In the H57M mutant, a dramatic decrease in the quantum yield of chromophore fluorescence emission and a 45 nm blue shift of the absorption maximum with an increase in the pH from 5 to 8 indicate deprotonation of the counterion with a pK(a) of 6.3, which is also the pK(a) at which the M intermediate is observed in the photocycle of the protein solubilized in detergent [dodecyl maltoside (DDM)]. This is in contrast with the case for the wild-type protein, for which the same experiments show that the major fraction of Asp85 is deprotonated at pH >3 and that it protonates only at low pH, with a pK(a) of 2.3. The M intermediate in the wild-type photocycle accumulates only at high pH, with an apparent pK(a) of 9, via deprotonation of a residue interacting with Asp85, presumably His57. In liposomes reconstituted with ESR, the pK(a) values for M formation and spectral shifts are 2-3 pH units lower than in DDM. The distinctively different pH dependencies of the protonation of Asp85 and the accumulation of the M intermediate in the wild-type protein versus the H57M mutant indicate that there is strong Asp-His interaction, which substantially lowers the pK(a) of Asp85 by stabilizing its deprotonated state.
Energy transfer from light-harvesting carotenoids to chlorophyll is common in photosynthesis, but such antenna pigments have not been observed in retinal-based ion pumps and photoreceptors. Here we describe xanthorhodopsin, a proton-pumping retinal protein/carotenoid complex in the eubacterium Salinibacter ruber . The wavelength dependence of the rate of pumping and difference absorption spectra measured under a variety of conditions indicate that this protein contains two chromophores, retinal and the carotenoid salinixanthin, in a molar ratio of about 1:1. The two chromophores interact strongly, and light energy absorbed by the carotenoid is transferred to the retinal with a quantum efficiency of ∼40%. The antenna carotenoid extends the wavelength range of the collection of light for uphill transmembrane proton transport.
Proteorhodopsin, a retinal protein of marine proteobacteria similar to bacteriorhodopsin of the archaea, is a light-driven proton pump. Absorption of a light quantum initiates a reaction cycle (turnover time of ca. 50 ms), which includes photoisomerization of the retinal from the all-trans to the 13-cis form and transient deprotonation of the retinal Schiff base, followed by recovery of the initial state. We report here that in addition to this fast cyclic conversion, illumination at high pH results in accumulation of a long-lived photoproduct absorbing at 362 nm. This photoconversion is much more efficient in the D227N mutant in which the anionic Asp227, which together with Asp97 constitutes the Schiff base counterion, is replaced with a neutral residue. Upon illumination at pH 8.5, most of the D227N pigment is converted to the 362 nm species, with a quantum efficiency of ca. 0.2. The pK(a) for this transition in the wild type is 9.6, but decreased to 7.5 after mutation of Asp227. The short wavelength of the absorption maximum of the photoproduct indicates that it has a deprotonated Schiff base. In the dark, this photoproduct is converted back to the initial pigment with a time constant of 30 min (in D227N, at pH 8.5), but it can be reconverted more rapidly by illumination with near-UV light. Experiments with "locked" retinal analogues which selectively exclude rotation around either the C9=C10, C11=C12, or C13=C14 bond show that formation of the 362 nm species involves isomerization around the C13=C14 bond. In agreement with this, retinal extraction indicates that the 362 nm photoproduct is 13-cis whereas the initial state is predominantly all-trans. A rapid shift of the pH from 8.5 to 4 greatly accelerates thermal reconversion of the 362 nm species to the initial pigment, suggesting that its recovery involving the thermal isomerization of the chromophore is controlled by ionizable residues, primarily the Schiff base and Asp97. The transformation to the long-lived 362 nm photoproduct is apparently a side reaction of the photocycle, a response to high pH, caused by alteration of the normal reprotonation and reisomerization pathway of the Schiff base.
Similarly to bacteriorhodopsin, proteorhodopsin that normally contains all-trans and 13-cis retinal is transformed at low pH to a species containing 9-cis retinal under continuous illumination at lambda > 530 nm. This species, absorbing around 430 nm, returns thermally in tens of minutes to initial pigment and can be reconverted also with blue-light illumination. The yield of the 9-cis species is negligibly small at neutral pH but increases manyfold (> 100) at acid pH with a pK(a) of 2.6. This indicates that protonation of acidic group(s) alters the photoreaction pathway that leads normally to all-trans --> 13-cis isomerization. In the D97N mutant, in which one of the two acidic groups in the vicinity of the retinal Schiff base is not ionizable, the yield of 9-cis species at low pH shows a pH dependence similar to that in the wild-type but with a somewhat increased pK(a) of 3.3. In contrast to this relatively minor effect, replacement of the other acidic group, Asp227, with Asn results in a remarkable, more than 50-fold, increase in the yield of the light-induced formation of 9-cis species in the pH range 4-6. It appears that protonation of Asp227 at low pH is what causes the dramatic increase in the yield of the 9-cis species in wild-type proteorhodopsin. We conclude that the photoisomerization pathways in proteorhodopsin to 13-cis or 9-cis photoproducts are controlled by the charge state of Asp227.
Tyrosine-83, a residue which is conserved in all halobacterial retinal proteins, is located at the extracellular side in helix C of bacteriorhodopsin. Structural studies indicate that its hydroxyl group is hydrogen bonded to Trp189 and possibly to Glu194, a residue which is part of the proton release complex (PRC) in bacteriorhodopsin. To elucidate the role of Tyr83 in proton transport, we studied the Y83F and Y83N mutants. The Y83F mutation causes an I I nm blue shift of the absorption spectrum and decreases the size of the absorption changes seen upon dark adaptation. The light-induced fast proton release, which accompanies formation of the M intermediate, is observed only at pH above 7 in Y83F. The pK(a) of the PRC in M is elevated in Y83F to about 7.3 (compared to 5.8 in WT). The rate of the recovery of the initial state (the rate of the O --> BR transition) and light-induced proton release at pH below 7 is very slow in Y83F (ca. 30 ms at pH 6). The amount of the O intermediate is decreased in Y83F despite the longer lifetime of O. The Y83N mutant shows a similar phenotype in respect to proton release. As in Y83F, the recovery of the initial state is slowed several fold in Y83N. The O intermediate is not seen in this mutant. The data indicate that the PRC is functional in Y83F and Y83N but its pK(a) in M is increased by about 1.5 pK units compared to the WT. This suggests that Tyr83 is not the main source for the proton released upon M formation in the WT; however, Tyr83 is involved in the proton release affecting the pK(a) of the PRC in M and the rate of proton transport from Asp85 to PRC during the O --> bR transition. Both the Y83F and the Y83N mutations lead to a greatly decreased functionality of the pigment at high pH because most of the pigment is converted into the inactive P480 species, with a pK(a) 8-9.
The factors determining the pH dependence of the formation and decay of the O photointermediate of the bacteriorhodopsin (bR) photocycle were investigated in the wild-type (WT) pigment and in the mutants of Glu-194 and Glu-204, key residues of the proton release group (PRG) in bR. We have found that in the WT the rate constant of O --> bR transition decreases 30-fold upon decreasing the pH from 6 to 3 with a pKa of about 4.3. D2O slows the rise and decay of the O intermediate in the WT at pH 3.5 by a factor of 5.5. We suggest that the rate of the O --> bR transition (which reflects the rate of deprotonation of the primary proton acceptor Asp-85) at low pH is controlled by the deprotonation of the PRG. To test this hypothesis, we studied the E194D mutant. We show that the pKa of the PRG in the ground state of the E194D mutant, when Asp-85 is protonated, is increased by 1.2 pK units compared to that of the WT. We found a similar increase in the pKa of the rate constant of the O --> bR transition in E194D. This provides further evidence that the rate of the O --> bR transition is controlled by the PRG. In a further test, the E194Q mutation, which disables the PRG and slows proton release, almost completely eliminates the pH dependence of O decay at pHs below 6. A second phenomenon we investigated was that in the WT at neutral and alkaline pH the fraction of the O intermediate decreases with pKa 7.5. A similar pH dependence is observed in the mutants in which the PRG is disabled, E194Q and E204Q, suggesting that the decrease in the fraction of the O intermediate with pKa ca. 7.5 is not controlled by the PRG. We propose that the group with pKa 7.5 is Asp-96. The slowing of the reprotonation of Asp-96 at high pH is the cause of the decrease in the rate of the N --> O transition, leading to the decrease in the fraction of O.
Arg82 is one of the four buried charged residues in the retinal binding pocket of bacteriorhodopsin (bR). Previous studies show that Arg82 controls the pKas of Asp85 and the proton release group and is essential for fast light-induced proton release. To further investigate the role of Arg82 in light-induced proton pumping, we replaced Arg82 with histidine and studied the resulting pigment and its photochemical properties. The main pKa of the purple-to-blue transition (pKa of Asp85) is unusually low in R82H: 1.0 versus 2.6 in wild type (WT). At pH 3, the pigment is purple and shows light and dark adaptation, but almost no light-induced Schiff base deprotonation (formation of the M intermediate) is observed. As the pH is increased from 3 to 7 the M yield increases with pKa 4.5 to a value ∼40% of that in the WT. A transition with a similar pKa is observed in the pH dependence of the rate constant of dark adaptation, kda. These data can be explained, assuming that some group deprotonates with pKa 4.5, causing an increase in the pKa of Asp85 and thus affecting kda and the yield of M. As the pH is increased from 7 to 10.5 there is a further 2.5-fold increase in the yield of M and a decrease in its rise time from 200μs to 75μs with pKa 9.4. The chromophore absorption band undergoes a 4-nm red shift with a similar pKa. We assume that at high pH, the proton release group deprotonates in the unphotolyzed pigment, causing a transformation of the pigment into a red-shifted “alkaline” form which has a faster rate of light-induced Schiff base deprotonation. The pH dependence of proton release shows that coupling between Asp85 and the proton release group is weakened in R82H. The pKa of the proton release group in M is 7.2 (versus 5.8 in the WT). At pH<7, most of the proton release occurs during O→bR transition with τ≈45ms. This transition is slowed in R82H, indicating that Arg82 is important for the proton transfer from Asp85 to the proton release group. A model describing the interaction of Asp85 with two ionizable residues is proposed to describe the pH dependence of light-induced Schiff base deprotonation and proton release.
Substitution of glutamic acid-194, a residue on the extracellular surface of bacteriorhodopsin, with a cysteine inhibits the fast light-induced proton release that normally is coupled with the deprotonation of the Schiff base during the L to M transition. Proton release in this mutant occurs at the very end of the photocycle and coincides with deprotonation of the primary proton acceptor, Asp-85, during the O to bR transition. the E194C mutation also results in a slowing down of the photocycle by about 1 order of magnitude as compared to the wild type and produces a strong effect on the pH dependence of dark adaptation that is interpreted as a drastic reduction or elimination of the coupling between the primary proton acceptor Asp-85 and the proton release group. These data indicate that Glu-194 is a critical component of the proton release complex in bacteriorhodopsin.
K129 is a residue located in the extracellular loop connecting transmembrane helices D and E of bacteriorhodopsin. Replacement of K129 with a histidine alters the pKa's of two key residues in the proton transport pathway, D85, and the proton release group (probably E204); the resulting pigment has properties that differ markedly from the wild type. 1) In the unphotolyzed state of the K129H mutant, the pKa of D85 is 5.1 +/- 0.1 in 150 mM KCl (compared to approximately 2.6 in the wild-type bacteriorhodopsin), whereas the unphotolyzed-state pKa of E204 decreases to 8.1 +/- 0.1 (from approximately 9.5 in the wild-type pigment). 2) The pKa of E204 in the M state is 7.0 +/- 0.1 in K129H, compared to approximately 5.8 in the wild-type pigment. 3) As a result of the change in the pKa of E204 in M, the order of light-induced proton release and uptake exhibits a dependence on pH in K129H differing from that of the wild type: at neutral pH and moderate salt concentrations (150 mM KCl), light-induced proton uptake precedes proton release, whereas it follows proton release at higher pH. This pumping behavior is similar to that seen in a related bacterial rhodopsin, archaerhodopsin-1, which has a histidine in the position analogous to K129. 4) At alkaline pH, a substantial fraction of all-trans K129H pigment (approximately 30%) undergoes a conversion into a shorter wavelength species, P480, with pKa approximately 8.1, close to the pKa of E204. 5) Guanidine hydrochloride lowers the pKa's of D85 and E204 in the ground state and the pKa of E204 in the M intermediate, and restores the normal order of proton release before uptake at neutral pH. 6) In the K129H mutant the coupling between D85 and E204 is weaker than in wild-type bacteriorhodopsin. In the unphotolyzed pigment, the change in the pKa's of either residue when the other changes its protonation state is only 1.5 units compared to 4.9 units in wild-type bacteriorhodopsin. In the M state of photolyzed K129H pigment, the corresponding change is 1 unit, compared to 3.7 units in the wild-type pigment. We suggest that K129 may be involved in stabilizing the hydrogen bonding network that couples E204 and D85. Substitution of K129 with a histidine residue causes structural changes that alter this coupling and affect the pKa's of E204 and D85.
Titration of Asp-85, the proton acceptor and part of the counterion in bacteriorhodopsin, over a wide pH range (2-11) leads us to the following conclusions: 1) Asp-85 has a complex titration curve with two values of pKa; in addition to a main transition with pKa = 2.6 it shows a second inflection point at high pH (pKa = 9.7 in 150-mM KCl). This complex titration behavior of Asp-85 is explained by interaction of Asp-85 with an ionizable residue X'. As follows from the fit of the titration curve of Asp-85, deprotonation of X' increases the proton affinity of Asp-85 by shifting its pKa from 2.6 to 7.5. Conversely, protonation of Asp-85 decreases the pKa of X' by 4.9 units, from 9.7 to 4.8. The interaction between Asp-85 and X' has important implications for the mechanism of proton transfer. In the photocycle after the formation of M intermediate (and protonation of Asp-85) the group X' should release a proton. This deprotonated state of X' would stabilize the protonated state of Asp-85.2) Thermal isomerization of the chromophore (dark adaptation) occurs on transient protonation of Asp-85 and formation of the blue membrane. The latter conclusion is based on the observation that the rate constant of dark adaptation is directly proportional to the fraction of blue membrane (in which Asp-85 is protonated) between pH 2 and 11. The rate constant of isomerization is at least 10(4) times faster in the blue membrane than in the purple membrane. The protonated state of Asp-85 probably is important for the catalysis not only of all-trans <=> 13-cis thermal isomerization during dark adaptation but also of the reisomerization of the chromophore from 13-cis to all-trans configuration during N-->O-->bR transition in the photocycle. This would explain why Asp-85 stays protonated in the N and O intermediates.
To explore the role of Arg82 in the catalysis of proton transfer in bacteriorhodopsin, we replaced Arg82 with Lys, which is also positively charged at neutral pH but has an intrinsic pKa of about 1.7 pH units lower than that of Arg. In the R82K mutant expressed in Halobacterium salinarium, we found the following: (1) The pKa of the purple-to-blue transition at low pH (which reflects the pKa of Asp85) is 3.6 +/- 0.1. At high pH a second inflection in the blue-to-purple transition with pKa = 8.0 is found. The complex titration behavior of Asp85 indicates that the pKa of Asp85 depends on the protonation state of another amino acid residue, X', which has a pKa = 8.0 in R82K. The fit of the experimental data to a model of two interacting residues shows that deprotonation of X' at high pH causes a shift in the pKa of Asp85 from 3.7 to 6.0. In turn, protonation of Asp85 decreases the pKa of X' by 2.3 pH units. This suggests that X' can release a proton upon formation of the M intermediate and the concomitant protonation of Asp85 in the photocycle. (2) The rate constant of dark adaptation, kda, is proportional to the fraction of blue membrane between pH 2 and 10, indicating that thermal isomerization proceeds through the transient protonation of Asp85. The pH dependence of kda shows that two groups with pKal = 3.9 and pKa2 = 8.0 control the rate of dark adaptation in R82K. The 1.7 pH unit shift in pKa2 in R82K compared to the wild type (WT) (pKa2 = 9.7) supports the hypothesis that X' is Arg82 in WT and Lys82 in R82K (or at least that these groups are the principal part of a cluster of residues that constitute X'). (3) Under steady state illumination, the efficiency of proton transport in R82K incorporated in phosphatidylcholine vesicles is at least 40% of that in the WT. A flash-induced transient signal of the pH-sensitive dye pyranine is similar to that in the WT (proton release precedes uptake), but the amplitude is small in R82K (about 15% of that found in the WT), indicating that only a small fraction of protons is released fast in R82K. This supports the suggestions that Arg82 is associated with the proton release pathway (acts as a proton release group or part of a proton release complex) and that Lys cannot efficiently substitute for Arg in this process.(ABSTRACT TRUNCATED AT 400 WORDS)
The maximum photosteady state fraction of K, x(K)max, and the ratio of the quantum yields of the forward and back light reactions, trans-bacteriorhodopsin (bR) double-line arrow pointing left and right K, phi(bR)/phi(K), were obtained by measuring the absorption changes produced by illumination of frozen water-glycerol (1:2) suspensions of light-adapted purple membrane at different wavelengths at -165-degrees-C. An independent method based on the second derivative of the absorption spectrum in the region of the beta-bands was also used. it was found that x(K)max = 0.56 +/- 0.02 (under 510 nm illumination) and phi(bR/phi(K) = 0.7 +/- 0.02 (at 510 and 567 nm) The quantum-yield ratio (0.66 +/- 0.06) was found to be independent of excitation wavelength within experimental error in the range 510-610 nm. The calculated absorption spectrum of K has its maximum at 603-606 nm and an extinction 0.85 +/- 0.03 that of bR. At shorter wavelengths there are beta-bands at 410, 354 and 336 nm. Using the data of Hurley et al. (Nature 270, 540-542, 1977) on relative rates of rhodopsin bleaching and K formation, the quantum yield of K formation was determined to be 0.66 +/- 0.04 at low temperature. The quantum efficiency of the back reaction was estimated to be 0.93 +/- 0.07. These values of quantum efficiencies of the forward and back light reactions of bR at -165-degrees-C coincide with those recently obtained at room temperature. This indicates that the quantum efficiencies of both forward and back light reactions of bacteriorhodopsin are temperature independent down to -165-degrees-C.
In aqueous suspensions of purple membranes (pH 10.2, 0.4 M KCl) an intermediate having an absorption maximum at 570-575 nm (at -196 degrees C) was produced by first heating the M intermediate up to -30 degrees C and then stabilizing it by subsequent cooling to -60 degrees C. We suggest that this species is the intermediate N (or P or R) found and characterized earlier near room temperature. Upon illumination at -196 degrees C N is transformed into a bathochromically absorbing species KN which has an absorption maximum near 605 nm and an extinction 1.35 times that of N. This light reaction is photoreversible. The quantum yield ratio for the forward and back reaction is 0.18 +/- 0.02. The maximum photo steady state concentration of KN is about 0.24. The N intermediate was also trapped in water suspensions of purple membranes at neutral pH and low salt concentration by illumination at lambda greater than 620 nm during cooling. In addition to N another intermediate absorbing in the red (maximum at 610-620 nm) was accumulated in smaller amounts. It is not photoactive at -196 degrees C and apparently is the O intermediate or a photoproduct of N.