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细菌视紫红质突变体Tyr-185→Phe的时间分辨傅里叶变换红外光谱:在O形成过程中Asp-96重新质子化;在O衰减过程中Asp-85和Asp-212去质子化。

Time-resolved Fourier transform infrared spectroscopy of the bacteriorhodopsin mutant Tyr-185-->Phe: Asp-96 reprotonates during O formation; Asp-85 and Asp-212 deprotonate during O decay.

作者信息

Bousché O, Sonar S, Krebs M P, Khorana H G, Rothschild K J

机构信息

Physics Department, Boston University, MA 02215.

出版信息

Photochem Photobiol. 1992 Dec;56(6):1085-95. doi: 10.1111/j.1751-1097.1992.tb09732.x.

Abstract

The protonation state of key aspartic acid residues in the O intermediate of bacteriorhodopsin (bR) has been investigated by time-resolved Fourier transform infrared (FTIR) difference spectroscopy and site-directed mutagenesis. In an earlier study (Bousché et al., J. Biol Chem. 266, 11063-11067, 1991) we found that Asp-96 undergoes a deprotonation during the M-->N transition, confirming its role as a proton donor in the reprotonation pathway leading from the cytoplasm to the Schiff base. In addition, both Asp-85 and Asp-212, which protonate upon formation of the M intermediate, remain protonated in the N intermediate. In this study, we have utilized the mutant Tyr-185-->Phe (Y185F), which at high pH and salt concentrations exhibits a photocycle similar to wild type bR but has a much slower decay of the O intermediate. Y185F was expressed in native Halobacterium halobium and isolated as intact purple membrane fragments. Time-resolved FTIR difference spectra and visible difference spectra of this mutant were measured from hydrated multilayer films. A normal N intermediate in the photocycle of Y185F was identified on the basis of characteristic chromophore and protein vibrational bands. As N decays, bands characteristic of the all-trans O chromophore appear in the time-resolved FTIR difference spectra in the same time range as the appearance of a red-shifted photocycle intermediate absorbing near 640 nm. Based on our previous assignment of the carboxyl stretch bands to the four membrane embedded Asp groups: Asp-85, Asp-96, Asp-115 and Asp-212, we conclude that during O formation: (i) Asp-96 undergoes reprotonation. (ii) Asp-85 may undergo a small change in environment but remains protonated. (iii) Asp-212 remains partially protonated. In addition, reisomerization of the chromophore during the N-->O transition is accompanied by a major reversal of protein conformational changes which occurred during the earlier steps in the photocycle. These results are discussed in terms of a proposed mechanism for proton transport.

摘要

通过时间分辨傅里叶变换红外(FTIR)差示光谱法和定点诱变技术,研究了细菌视紫红质(bR)的O中间体中关键天冬氨酸残基的质子化状态。在早期的一项研究中(Bousché等人,《生物化学杂志》,266,11063 - 11067,1991),我们发现天冬氨酸-96在M→N转变过程中发生去质子化,证实了其在从细胞质到席夫碱的再质子化途径中作为质子供体的作用。此外,在M中间体形成时质子化的天冬氨酸-85和天冬氨酸-212在N中间体中仍保持质子化状态。在本研究中,我们利用了突变体酪氨酸-185→苯丙氨酸(Y185F),该突变体在高pH和盐浓度下表现出与野生型bR相似的光循环,但O中间体的衰减要慢得多。Y185F在天然嗜盐菌中表达,并作为完整的紫色膜片段分离出来。从水合多层膜中测量了该突变体的时间分辨FTIR差示光谱和可见差示光谱。根据特征发色团和蛋白质振动带,鉴定出Y185F光循环中的正常N中间体。随着N的衰减,全反式O发色团的特征带在时间分辨FTIR差示光谱中出现在与吸收峰在640 nm附近的红移光循环中间体出现的相同时间范围内。基于我们之前将羧基伸缩带归属于四个膜嵌入天冬氨酸基团:天冬氨酸-85、天冬氨酸-96、天冬氨酸-115和天冬氨酸-212,我们得出结论,在O形成过程中:(i)天冬氨酸-96发生再质子化。(ii)天冬氨酸-85的环境可能发生微小变化,但仍保持质子化。(iii)天冬氨酸-212保持部分质子化。此外,在N→O转变过程中发色团的重新异构化伴随着在光循环早期步骤中发生的蛋白质构象变化的重大逆转。根据提出的质子传输机制对这些结果进行了讨论。

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