Time-resolved step-scan Fourier transform infrared spectroscopy reveals differences between early and late M intermediates of bacteriorhodopsin.

In this report, from time-resolved step-scan Fourier transform infrared investigations from 15 ns to 160 ms, we provide evidence for the subsequent rise of three different M states that differ in their structures. The first state rises with approximately 3 microseconds to only a small percentage. Its structure as judged from amide I/II bands differs in small but well-defined aspects from the L state. The next M state, which appears in approximately 40 microseconds, has almost all of the characteristics of the "late" M state, i.e., it differs considerably from the first one. Here, the L left arrow over right arrow M equilibrium is shifted toward M, although some percentage of L still persists. In the last M state (rise time approximately 130 microseconds), the equilibrium is shifted toward full deprotonation of the Schiff base, and only small additional structural changes take place. In addition to these results obtained for unbuffered conditions or at pH 7, experiments performed at lower and higher pH are presented. These results are discussed in terms of the molecular changes postulated to occur in the M intermediate to allow the shift of the L/M equilibrium toward M and possibly to regulate the change of the accessibility of the Schiff base necessary for effective proton pumping.

Nanosecond retinal structure changes in K-590 during the room-temperature bacteriorhodopsin photocycle: picosecond time-resolved coherent anti-stokes Raman spectroscopy.

Time-resolved vibrational spectra are used to elucidate the structural changes in the retinal chromophore within the K-590 intermediate that precedes the formation of the L-550 intermediate in the room-temperature (RT) bacteriorhodopsin (BR) photocycle. Measured by picosecond time-resolved coherent anti-Stokes Raman scattering (PTR/CARS), these vibrational data are recorded within the 750 cm-1 to 1720 cm-1 spectral region and with time delays of 50-260 ns after the RT/BR photocycle is optically initiated by pulsed (< 3 ps, 1.75 nJ) excitation. Although K-590 remains structurally unchanged throughout the 50-ps to 1-ns time interval, distinct structural changes do appear over the 1-ns to 260-ns period. Specifically, comparisons of the 50-ps PTR/CARS spectra with those recorded with time delays of 1 ns to 260 ns reveal 1) three types of changes in the hydrogen-out-of-plane (HOOP) region: the appearance of a strong, new feature at 984 cm-1; intensity decreases for the bands at 957 cm-1, 952 cm-1, and 939 cm-1; and small changes intensity and/or frequency of bands at 855 cm-1 and 805 cm-1; and 2) two types of changes in the C-C stretching region: the intensity increase in the band at 1196 cm-1 and small intensity changes and/or frequency shifts for bands at 1300 cm-1 and 1362 cm-1. No changes are observed in the C = C stretching region, and no bands assignable to the Schiff base stretching mode (C = NH+) mode are found in any of the PTR/CARS spectra assignable to K-590. These PTR/CARS data are used, together with vibrational mode assignments derived from previous work, to characterize the retinal structural changes in K-590 as it evolves from its 3.5-ps formation (ps/K-590) through the nanosecond time regime (ns/K-590) that precedes the formation of L-550. The PTR/CARS data suggest that changes in the torsional modes near the C14-C15 = N bonds are directly associated with the appearance of ns/K-590, and perhaps with the KL intermediate proposed in earlier studies. These vibrational data can be primarily interpreted in terms of the degree of twisting of the C14-C15 retinal bond. Such twisting may be accompanied by changes in the adjacent protein. Other smaller, but nonetheless clear, spectral changes indicate that alterations along the retinal polyene chain also occur. The changes in the retinal structure are preliminary to the deprotonation of the Schiff base nitrogen during the formation of M-412. The time constant for the ps/ns K-590 transformation is estimated from the amplitude change of four vibrational bands in the HOOP region to be 40-70 ns.

Steric interaction between the 9-methyl group of the retinal and tryptophan 182 controls 13-cis to all-trans reisomerization and proton uptake in the bacteriorhodopsin photocycle.

The hypothesis was tested whether in bacteriorhodopsin (BR) the reduction of the steric interaction between the 9-methyl group of the chromophore all-trans-retinal and the tryptophan at position 182 causes the same changes as observed in the photocycle of 9-demethyl-BR. For this, the photocycle of the mutant W182F was investigated by time-resolved UV-vis and pH measurements and by static and time-resolved FT-IR difference spectroscopy. We found that the second half of the photocycle was similarly distorted in the two modified systems: based on the amide-I band, the protonation state of D96, and the kinetics of proton uptake, four N intermediates could be identified, the last one having a lifetime of several seconds; no O intermediate could be detected; the proton uptake showed a pronounced biphasic time course; and the pKa of group(s) on the cytoplasmic side in N was reduced from 11 in wild type BR to around 7.5. In contrast to 9-demethyl-BR, in the W182F mutant the first part of the photocycle does not drastically deviate from that of wild type BR. The results demonstrate the importance of the steric interaction between W182 and the 9-methyl group of the retinal in providing tight coupling between chromophore isomerization and the late proton transfer steps.

Influence of the 9-methyl group of the retinal on the photocycle of bacteriorhodopsin studied by time-resolved rapid-scan and static low-temperature Fourier transform infrared difference spectroscopy.

The photocycle of bacteriorhodopsin (BR) regenerated with all-trans-9-demethylretinal was investigated by time-resolved rapid-scan Fourier transform infrared difference spectroscopy, by static low-temperature difference spectroscopy at 80, 170, and 213 K and by static steady-state difference spectroscopy at 278 K. In addition, the formation and decay of M intermediate was monitored at 412 nm with conventional flash photolysis experiments. Our data show that the removal of the 9-methyl group strongly changes the photocycle of BR. The reaction cycle is slowed down about 250-fold. The photoreaction is characterized by a slow rise of the M intermediate and by a very long-lived N intermediate. No O intermediate could be observed. The low-temperature spectra indicate that already at 80 K a KL-like photoproduct is formed. L can be obtained as in native BR at 170 K, but its decay appears to be inhibited, since it can still be observed at 213 K and high pH, in addition to the M intermediate. As in native BR, the 15-hydrogen out-of-plane modes of the L and N intermediates (observed in 2H2O) are very similar. Evidence for the existence of three N substates which differ in the protonation state of Asp96 and in the amide I bands is presented. This is explained by the extremely slowed-down reisomerization of the chromophore. The results are discussed with respect to alterations in the chromophore-protein interaction, caused by the removal of the 9-methyl group.

Aspartic acid-212 of bacteriorhodopsin is ionized in the M and N photocycle intermediates: an FTIR study on specifically 13C-labeled reconstituted purple membranes.

Purple membrane was regenerated from the denatured proteolytic (protease V8) fragments V-1 and V-2 of bacteriorhodopsin (BR), native membrane lipids, and all-trans-retinal. FTIR difference spectra of M and N intermediates of the reconstituted system are in close correspondence to those obtained from native BR. Asp-212 is the only internal aspartic acid in the V-2 fragment (helices F and G). Reconstituting a V-2 fragment from a [4-13C]Asp-labeled BR preparation with an unmodified V-1 fragment and vice versa have allowed us to assign IR bands to either Asp-212 or any of the remaining aspartic acids on V-1 (helices A-E). A carboxylate vibration at 1392 cm-1 has been identified in the M and N intermediates and assigned to Asp-212. Since no contribution of this residue to C = O stretches of protonated carboxyl groups was detected, Asp-212 must be ionized in light-adapted BR as well. The effect of [4-13C]Asp labeling of V-1 revealed a carboxylate vibration at 1385 cm-1 in light-adapted BR. Since Asp-96 and Asp-115 are protonated, this band is caused by Asp-85. All absorption changes of C = O stretches of protonated carboxyl groups are due to Asp residues on V-1. Correspondingly, the proton acceptor for Schiff base deprotonation in M is located on V-1, and must be Asp-85 (the only ionized Asp on V-1). The band assignments are compared with those reported for BR mutants, and the potential role of Asp-212 for proton translocation is discussed.