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细菌视紫红质突变体的振动光谱。天冬氨酸212与酪氨酸185相互作用的证据及其在质子泵机制中的可能作用。

Vibrational spectroscopy of bacteriorhodopsin mutants. Evidence for the interaction of aspartic acid 212 with tyrosine 185 and possible role in the proton pump mechanism.

作者信息

Rothschild K J, Braiman M S, He Y W, Marti T, Khorana H G

机构信息

Department of Physics, Boston University, Massachusetts 02215.

出版信息

J Biol Chem. 1990 Oct 5;265(28):16985-91.

PMID:2211604
Abstract

The role of Asp-212 in the proton pumping mechanism of bacteriorhodopsin (bR) has been studied by a combination of site-directed mutagenesis and Fourier transform infrared difference spectroscopy. Difference spectra were recorded at low temperature for the bR----K and bR----M photoreactions of the mutants Asp-212----Glu, Asp-212----Asn, and Asp-212----Ala. Despite an increased proportion of the 13-cis form of bR (normally associated with dark adaptation), all of the mutants exhibited a light-adapted form containing as a principal component the normal all-trans retinal chromophore. The absence of a shift in the retinal C = C stretching frequency in these mutants indicates that Asp-212 is not a major determinant of the visible absorption wavelength maximum in light-adapted bR. It is unlikely that Asp-212 is the acceptor group for the Schiff base proton since both the Asp-212----Glu and Asp-212----Ala mutants formed an M intermediate. All of the Asp-212 mutants were missing a Fourier transform infrared difference band that had been assigned previously to protonation changes of Tyr-185. These results are discussed in terms of a model in which Tyr-185 and Asp-212 form a polarizable hydrogen bond and are positioned near the C13-Schiff base portion of the chromophore. These 2 residues may be involved in stabilizing the relative orientation of the F and G helices and isomerizing the retinal in a regioselective manner about the C13 = C14 double bond.

摘要

通过定点诱变和傅里叶变换红外差示光谱相结合的方法,对天冬氨酸-212在细菌视紫红质(bR)质子泵机制中的作用进行了研究。在低温下记录了突变体天冬氨酸-212→谷氨酸、天冬氨酸-212→天冬酰胺和天冬氨酸-212→丙氨酸的bR→K和bR→M光反应的差示光谱。尽管bR的13-顺式形式(通常与暗适应相关)比例增加,但所有突变体均表现出一种光适应形式,其主要成分是正常的全反式视黄醛发色团。这些突变体中视黄醛C = C伸缩频率没有发生位移,这表明天冬氨酸-212不是光适应bR中可见吸收波长最大值的主要决定因素。天冬氨酸-212不太可能是席夫碱质子的受体基团,因为天冬氨酸-212→谷氨酸和天冬氨酸-212→丙氨酸突变体均形成了M中间体。所有天冬氨酸-212突变体均缺失一条先前已指定为酪氨酸-185质子化变化的傅里叶变换红外差示带。根据一个模型对这些结果进行了讨论,在该模型中,酪氨酸-185和天冬氨酸-212形成一个可极化氢键,并位于发色团的C13-席夫碱部分附近。这两个残基可能参与稳定F和G螺旋的相对取向,并以区域选择性方式使视黄醛围绕C13 = C14双键异构化。

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