Bacteriorhodopsin (BR), a light-driven proton pump in
Halobacterium salinarum, accommodatestwo resting forms of the retinylidene chromophore, the all-trans form (AT-BR)
and the 13-cis,15-synform (13C-BR). Both isomers are present in thermal equilibrium in the dark, but only the all-trans formhas proton-pump activity. In this study, we applied low-temperature Fourier-transform infrared (FTIR)spectroscopy to 13C-BR at 77 K
and compared the local structure around the chromophore before
andafter photoisomerization with that in AT-BR. Strong hydrogen-out-of-plane (HOOP) vibrations wereobserved at 964
and 958 cm
-1 for the K state of 13C-BR (13C-BR
K) versus a vibration at 957 cm
-1 forthe K state of AT-BR (AT-BR
K). In AT-BR
K, but not in 13C-BR
K, the HOOP modes exhibit isotopeshifts upon deuteration of the retinylidene at C15
and at the Schiff base nitrogen. Whereas the HOOPmodes of AT-BR
K were significantly affected by the mutation of Thr89, this was not the case for theHOOP modes of 13C-BR
K. These observations imply that, while the chromophore distortion is localizednear the Schiff base in AT-BR
K, it is located elsewhere in 13C-BR
K. By use of [
![](/images/gifchars/zeta.gif)
-
15N]lysine-labeled BR,we identified the N-D stretching vibrations of the 13C-BR Schiff base (in D
2O) at 2173
and 2056 cm
-1,close in frequency to those of AT-BR. These frequencies indicate strong hydrogen bonding of the Schiffbase in 13C-BR, presumably with a water molecule as in AT-BR. In contrast, the N-D stretching vibrationappears at 2332
and 2276 cm
-1 in 13C-BR
K versus values of 2495
and 2468 cm
-1 for AT-BR
K, suggestingthat the rupture of the Schiff base hydrogen bond that occurs in AT-BR
K does not occur in 13C-BR
K.Rotational motion of the Schiff base upon retinal isomerization is probably smaller in magnitude for13C-BR than for AT-BR. These differences in the primary step are possibly related to the absence oflight-driven proton pumping by 13C-BR.