Chromophore structure in a long-lived intermediate of heliorhodopsins : switching of a hydrogen bonding partner of protonated Schiff base

Urui Taito, Otomo Akihiro, Mizuno Misao, Kandori Hideki, Mizutani Yasuhisa
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Abstract

Heliorhodopsin (HeR) is a novel class of retinal proteins discovered in 2018 [1]. HeR contains an all-trans-retinal as a chromophore, which is covalently bound to a lysine residue through a protonated Schiff base linkage. Although amino acid sequences of HeR are largely different from those of type1 rhodopsins, a family of HeR shares the seven-transmembrane helix motif. Photoexcitation of the all-trans-retinal chromophore results in isomerization to a 13-cis form. This isomerization initiates a photocycle involving a series of intermediates, which are similar to those observed for type-1 rhodopsins. HeR has a long-lived intermediate in its photocycle, which is named the O intermediate, suggesting that the function of HeR is light sensing. In order to understand the functional role of the O intermediate, we investigated the chromophore structure in two HeRs, HeR 48C12 and T. archaeon HeR, using time-resolved resonance Raman spectroscopy. We measured resonance Raman spectra of the O intermediate of the two HeRs in H2O and D2O (Figure 1). The observed spectra of the O intermediate of the both HeRs showed that the chromophore configuration is 13-cis and 15-anti and that the polyene chain around the Schiff base is distorted. A comparison of frequencies and bandwidths of the C=N stretch bands of the O intermediate in H2O and D2O solutions indicated that the Schiff base is protonated and hydrogenbonded to a water molecule. The latter feature is in contrast to that the hydrogen bond partner is amino acid residue in the unphotolyzed state [2]. Therefore, it is likely that the protein structure around the Schiff base is much altered in the transition from the O intermediate to the unphotolyzed state. This alternation may be a reason for the long lifetime of the O intermediate, which is essential to signal transduction.
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长寿命的太阳紫质中间体中的发色团结构:质子化希夫碱的氢键伴侣的开关
Heliorhodopsin (HeR)是2018年发现的一类新的视网膜蛋白。HeR含有全反式视网膜作为发色团,通过质子化希夫碱键与赖氨酸残基共价结合。虽然HeR的氨基酸序列与1型视紫红质有很大的不同,但一个HeR家族具有7个跨膜螺旋基序。全反视网膜发色团的光激发导致异构化为13-顺式形式。这种异构化启动了一个涉及一系列中间产物的光循环,这与1型视紫红质中观察到的相似。HeR在其光循环中有一个长寿命的中间体,被命名为O中间体,这表明HeR的功能是光感应。为了了解O中间体的功能作用,我们利用时间分辨共振拉曼光谱研究了HeR 48C12和T. archaeon HeR两种HeR的发色团结构。我们测量了两种her的O中间体在H2O和D2O中的共振拉曼光谱(图1)。观察到两种her的O中间体的光谱显示,发色团的构型为13-顺式和15-反式,席夫碱周围的多烯链扭曲。比较了O中间体在H2O和D2O溶液中的C=N拉伸带的频率和带宽,表明希夫碱被质子化并与水分子形成氢键。后一特征与氢键伙伴为未光解状态[2]的氨基酸残基形成对比。因此,在从O中间体到未光解状态的转变过程中,希夫碱周围的蛋白质结构很可能发生了很大的变化。这种交替可能是O中间体长寿命的原因,这对信号转导至关重要。
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