Hunt David M, Cowing Jill A, Wilkie Susan E, Parry Juliet W L, Poopalasundaram Subathra, Bowmaker James K
Institute of Ophthalmology, University College London, Bath Street, London, UK.
Photochem Photobiol Sci. 2004 Aug;3(8):713-20. doi: 10.1039/b314693f. Epub 2004 Mar 22.
Of the four classes of vertebrate cone visual pigments, the shortwave-sensitive SWS1 class shows the shortest lambda(max) values with peaks in different species in either the violet (390-435 nm) or ultraviolet (around 365 nm) regions of the spectrum. Phylogenetic evidence indicates that the ancestral pigment was probably UV-sensitive (UVS) and that the shifts between violet and UV have occurred many times during evolution. This is supported by the different mechanisms for these shifts in different species. All visual pigments possess a chromophore linked via a Schiff base to a Lys residue in opsin protein. In violet-sensitive (VS) pigments, the Schiff base is protonated whereas in UVS pigments, it is almost certainly unprotonated. The generation of VS from ancestral UVS pigments most likely involved amino acid substitutions in the opsin protein that serve to stabilise protonation. The key residues in the opsin protein for this are at sites 86 and 90 that are adjacent to the Schiff base and the counterion at Glu113. In this review, the different molecular mechanisms for the UV or violet shifts are presented and discussed in the context of the structural model of bovine rhodopsin.
在脊椎动物的四类视锥视觉色素中,短波敏感的SWS1类色素的λ(max)值最短,不同物种的峰值出现在光谱的紫光(390 - 435纳米)或紫外线(约365纳米)区域。系统发育证据表明,原始色素可能对紫外线敏感(UVS),并且在进化过程中紫光和紫外线之间的转变发生了多次。不同物种中这些转变的不同机制支持了这一点。所有视觉色素都拥有一个通过席夫碱与视蛋白中的赖氨酸残基相连的发色团。在紫光敏感(VS)色素中,席夫碱被质子化,而在UVS色素中,它几乎肯定未被质子化。从原始UVS色素产生VS色素很可能涉及视蛋白中的氨基酸取代,这些取代有助于稳定质子化。视蛋白中对此起关键作用的残基位于与席夫碱相邻的86位和90位,以及位于113位的抗衡离子谷氨酸。在这篇综述中,将结合牛视紫红质的结构模型,介绍并讨论紫外线或紫光转变的不同分子机制。