Resonance Raman study on proton-dissociated state of bacteriorhodopsin: stabilization of L-like intermediate having the all-trans chromophore

Probing Structure and Reaction Dynamics of Proteins Using Time-Resolved Resonance Raman Spectroscopy

The mechanistic understanding of protein functions requires insight into the structural and reaction dynamics. To elucidate these processes, a variety of experimental approaches are employed. Among them, time-resolved (TR) resonance Raman (RR) is a particularly versatile tool to probe processes of proteins harboring cofactors with electronic transitions in the visible range, such as retinal or heme proteins. TR RR spectroscopy offers the advantage of simultaneously providing molecular structure and kinetic information. The various TR RR spectroscopic methods can cover a wide dynamic range down to the femtosecond time regime and have been employed in monitoring photoinduced reaction cascades, ligand binding and dissociation, electron transfer, enzymatic reactions, and protein un- and refolding. In this account, we review the achievements of TR RR spectroscopy of nearly 50 years of research in this field, which also illustrates how the role of TR RR spectroscopy in molecular life science has changed from the beginning until now. We outline the various methodological approaches and developments and point out current limitations and potential perspectives.

Two groups control light-induced Schiff base deprotonation and the proton affinity of Asp85 in the Arg82 his mutant of bacteriorhodopsin

Arg(82) is one of the four buried charged residues in the retinal binding pocket of bacteriorhodopsin (bR). Previous studies show that Arg(82) controls the pK(a)s of Asp(85) and the proton release group and is essential for fast light-induced proton release. To further investigate the role of Arg(82) in light-induced proton pumping, we replaced Arg(82) with histidine and studied the resulting pigment and its photochemical properties. The main pK(a) of the purple-to-blue transition (pK(a) of Asp(85)) 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 pK(a) 4.5 to a value approximately 40% of that in the WT. A transition with a similar pK(a) is observed in the pH dependence of the rate constant of dark adaptation, k(da). These data can be explained, assuming that some group deprotonates with pK(a) 4.5, causing an increase in the pK(a) of Asp(85) and thus affecting k(da) 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 200 micros to 75 micros with pK(a) 9. 4. The chromophore absorption band undergoes a 4-nm red shift with a similar pK(a). 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 Asp(85) and the proton release group is weakened in R82H. The pK(a) 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 tau approximately 45 ms. This transition is slowed in R82H, indicating that Arg(82) is important for the proton transfer from Asp(85) to the proton release group. A model describing the interaction of Asp(85) with two ionizable residues is proposed to describe the pH dependence of light-induced Schiff base deprotonation and proton release.

pH dependence of the absorption spectra and photochemical transformations of the archaerhodopsins

Two strains of archaebacteria have been found to contain light-driven proton pumping pigments analogous to bacteriorhodopsin (bR) in Halobacterium salinarium. These proteins are called archaerhodopsin-1 (aR-1) and archaerhodopsin-2 (aR-2). Their high degree of sequence identity with bR within the putative proton channel enables us to draw some conclusions about the roles of regions where differences in amino acids exist, and in particular the surface residues, on the structure and function of retinal-based proton pumps. We have characterized the spectral and photochemical properties of these two proteins and compared them to the corresponding properties of bR. While there are some differences in absorbance maxima and kinetics of the photocycle, most of the properties of aR-1 and aR-2 are similar to those of bR. The most striking differences of these proteins with bR are the lack of an alkaline-induced red-shifted absorption species and a dramatic (apparent) decrease in the light-induced transient proton release. In membrane sheet suspensions of aR-1 at 0.15 M KCl, the order of proton release and uptake appears opposite that of bR, in which proton release precedes uptake. The nature of this behavior appears to be due to differences in the amino acid sequence at the surfaces of the proteins. In particular, the residue corresponding to the lysine at position 129 of the extracellular loop region of bR is a histidine in aR-1 and could regulate the efficient release of protons into solution in bR.

Fourier transform Raman spectroscopy of the bacteriorhodopsin mutant Tyr-185-->Phe: formation of a stable O-like species during light adaptation and detection of its transient N-like photoproduct

Near-infrared FT-Raman spectroscopy can be used to measure the vibrations of the bacteriorhodopsin (bR) chromophore without the disadvantage of conventional visible resonance Raman spectroscopy, where the visible excitation drives the bR photoreactions. We utilized this technique to investigate the light-dark adaptation of bacteriorhodopsin and the mutant Tyr-185-->Phe (Y185F) at room temperature in solution. Compared to wild-type bR, both the FT-Raman and resonance Raman spectra of the light-adapted Y185F displayed new features characteristic of the vibrations of the O intermediate. Light adaptation of Y185F was found to involve a 13-cis, C=N syn-->all-trans isomerization of the retinal chromophore which produces a species similar to bR570 and a second O-like species. Dark adaptation, which was much slower in Y185F compared to wild-type bR, involved a parallel decay of the bR570 and O-like species and resulted in a decreased all-trans:13-cis ratio compared to wild type. Further evidence for the existence of an O-like species in Y185F comes from pump-probe Raman difference spectroscopy, where a red pump beam is found to produce a species very similar to the N intermediate in the photocycle. This species is shown by stroboscopic Raman measurements to exist transiently even at high pH. We postulate that when the Y185F chromophore has an all-trans structure the effective pKa of Asp-85 and Asp-212 is elevated in Y185F due to the disruption of the Asp-212/Tyr-185 hydrogen bond, thereby accounting for the increased protonation of these residues in the O-like species.

The use of tryptophan mutants in identifying the 296 nm transient absorbing species during the photocycle of bacteriorhodopsin

The transient absorption at 296 nm was part of the spectroscopic evidence that initiated the proposal that tyrosinate (Tyr-) is formed during, and important to, the photocycle of bacteriorhodopsin (bR). Recent evidence against such a proposal comes from the results of NMR, UV Raman as well as electron cryo-microscopic structural studies. This makes it credible to assign this absorption to a charge perturbation of the lowest energy absorption of one of the tryptophan (Trp) residues in bR. The transient absorption at 296 nm is examined for each of 8 tryptophan mutants in which Trp is substituted by phenylalanine or cysteine, which absorb at shorter wavelength. It is shown that while all go through the photocycle, all but Trp-182 mutant show this transient absorption. This strongly suggests the assignment of this absorption to a charge perturbaton of the lowest energy absorption of Trp-182 during the photocycle. The chemical identity of the perturbing charge(s) is briefly discussed.