Palings I, van den Berg E M, Lugtenburg J, Mathies R A
Department of Chemistry, University of California, Berkeley 94720.
Biochemistry. 1989 Feb 21;28(4):1498-507. doi: 10.1021/bi00430a012.
Resonance Raman vibrational spectra of the retinal chromophore in bathorhodopsin have been obtained after regenerating bovine visual pigments with an extensive series of 13C- and deuterium-labeled retinals. A low-temperature spinning cell technique was used to produce high-quality bathorhodopsin spectra exhibiting resolved hydrogen out-of-plane wagging vibrations at 838, 850, 858, 875, and 921 cm-1. The isotopic shifts and a normal coordinate analysis permit the assignment of these lines to the HC7 = C8H Bg, C14H, C12H, C10H, and C11H hydrogen out-of-plane wagging modes, respectively. The coupling constant between the C11H and C12H wags as well as the C12H wag force constant are unusually low compared to those of retinal model compounds. This quantitatively confirms the lack of coupling between the C11H and C12H wags and the low C12H wag vibrational frequency noted earlier by Eyring et al. [(1982) Biochemistry 21, 384]. The force constants for the C10H and C14H wags are also significantly below the values observed in model compounds. We suggest that the perturbed hydrogen out-of-plane wagging and C-C stretching force constants for the C10-C11 = C12-C13 region of the chromophore in bathorhodopsin result from electrostatic interactions with a charged protein residue. This interaction may also contribute to the 33 kcal/mol energy storage in bathorhodopsin.
在用一系列广泛的13C和氘标记的视黄醛再生牛视觉色素后,获得了视紫红质中视黄醛发色团的共振拉曼振动光谱。采用低温旋转池技术产生高质量的视紫红质光谱,该光谱在838、850、858、875和921 cm-1处呈现出分辨的氢面外摇摆振动。同位素位移和正常坐标分析允许将这些谱线分别归属于HC7 = C8H Bg、C14H、C12H、C10H和C11H氢面外摇摆模式。与视黄醛模型化合物相比,C11H和C12H摇摆之间的耦合常数以及C12H摇摆力常数异常低。这定量地证实了C11H和C12H摇摆之间缺乏耦合以及Eyring等人(1982年,《生物化学》21卷,384页)早先指出的C12H摇摆振动频率较低。C10H和C14H摇摆的力常数也明显低于模型化合物中观察到的值。我们认为,视紫红质中发色团C10 - C11 = C12 - C13区域的氢面外摇摆和C - C伸缩力常数受到扰动,是由于与带电荷的蛋白质残基发生静电相互作用所致。这种相互作用也可能对视紫红质中33 kcal/mol的能量储存有贡献。