Abstract
The absorption maximum of blue proteorhodopsin (BPR) is the most blue-shifted of all retinal proteins found in archaea or bacteria, with the exception of sensory rhodopsin II (SRII). The absorption spectrum also exhibits a pH dependence larger than any other retinal protein. We examine the structural origins of these two properties of BPR by using optical spectroscopy, homology modeling, and molecular orbital theory. Bacteriorhodopsin (BR) and SRII are used as homology parents for comparative purposes. We find that the tertiary structure of BPR based on SRII is more realistic with respect to free energy, dynamic stability, and spectroscopic properties. Molecular orbital calculations including full single- and double-configuration interaction within the chromophore pi-electron system provide perspectives on the wavelength regulation in this protein and indicate that Arg-95, Gln-106, Glu-143, and Asp-229 play important, and in some cases pH-dependent roles. A possible model for the 0.22 eV red shift of BPR at low pH is examined, in which Glu-143 becomes protonated and releases Arg-95 to rotate up into the binding site, altering the electrostatic environment of the chromophore. At high pH, BPR has spectroscopic properties similar to SRII, but at low pH, BPR has spectroscopic properties more similar to BR. Nevertheless, SRII is a significantly better homology model for BPR and opens up the question of whether this protein serves as a proton pump, as commonly believed, or is a light sensor with structure-function properties more comparable to those of SRII. The function of BPR in the native organism is discussed with reference to the results of the homology model.
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