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首页> 外文期刊>The Journal of Experimental Biology >Eyeshine and spectral tuning of long wavelength-sensitive rhodopsins: no evidence for red-sensitive photoreceptors among five Nymphalini butterfly species
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Eyeshine and spectral tuning of long wavelength-sensitive rhodopsins: no evidence for red-sensitive photoreceptors among five Nymphalini butterfly species

机译:长波长敏感性视紫红质的眼光和光谱调谐:没有证据表明五种Nymphalini蝴蝶物种对红色敏感

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Spectral tuning of rhodopsins commonly refers to the effects of opsin amino acid substitutions on the wavelength for peak sensitivity of the rhodopsin absorption spectrum. Nymphalini butterflies provide an opportunity for identifying some of the amino acid substitutions responsible for insect rhodopsin spectral tuning because the majority of photoreceptor cells (R3-9) in the adult retina express only a single long wavelength-sensitive (LWS) opsin mRNA transcript. Therefore, the opsin genotype can be directly correlated with its phenotype. We determined the LWS opsin gene sequence from cDNA of the mourning cloak Nymphalis antiopa, and from genomic DNA of the malachite Siproeta stelenes and the peacock Inachis io. Using an epi-microspectrophotometer we examined each butterfly's eyeshine for photochemical evidence of multiple LWS rhodopsins and found only one. We then performed partial-bleaching experiments to obtain absorbance spectra for the LWS rhodopsins of all three species as well as from another nymphalid, the buckeye Junonia coenia. The isolated LWS opsin gene sequences varied in length from 1437-1612 bp and encode rhodopsins R522 (S. stelenes), R530 (I. io), R534 (N. antiopa) and, together with a previously published sequence, R510 (J. coenia). Comparative sequence analysis indicates that the S. stelenes rhodopsin is slightly blue-shifted compared to the typical 530 nm lepidopteran rhodopsin because of the presence of a S138A substitution at a homologous site that in mammalian MWS/LWS rhodopsins causes a 5 nm blue-shift. The difference in peak absorption between R522 of S. stelenes and R530 of Inachis io is therefore largely accounted for by this substitution. This suggests that spectral tuning mechanisms employing the S138A may have evolved in parallel in mammalian and butterfly MWS/LWS rhodopsins across 500 million years of evolution.
机译:视紫红质的光谱调节通常是指视紫红质氨基酸取代对视紫红质吸收光谱的峰敏感性的波长的影响。 Nymphalini蝴蝶为鉴定引起昆虫视紫红质光谱调节的某些氨基酸取代提供了机会,因为成年视网膜中的大多数感光细胞(R3-9)仅表达单个长波长敏感(LWS)视蛋白mRNA转录本。因此,视蛋白基因型可以与其表型直接相关。我们从哀悼斗篷Nymphalis antiopa的cDNA,以及孔雀石Siproeta stelenes和孔雀Inachis的基因组DNA中确定了LWS opsin基因序列。使用表观显微分光光度计,我们检查了每只蝴蝶的眼皮中是否存在多种LWS视紫红质的光化学证据,仅发现了一只。然后,我们进行了部分漂白实验,以获取所有三个物种的LWS视紫红质的吸光度光谱,以及来自另一种夜蛾类的七叶树Junonia coenia的吸收光谱。分离的LWS视蛋白基因序列的长度在1437-1612bp之间变化,并编码视紫红质R522(S.stelenes),R530(I.io),R534(N.antiopa),以及先前公开的序列R510(J.J.A。)。 coenia)。比较序列分析表明,与典型的530 nm鳞翅目视紫红质相比,链球菌视紫红质略微蓝移,因为在哺乳动物MWS / LWS视紫红质的同源位点存在S138A取代,导致蓝移5 nm。因此,这种替代很大程度上解释了链霉菌的R522和Inachis的R530之间的峰吸收差异。这表明使用S138A的光谱调谐机制可能已经在5亿年的进化过程中在哺乳动物和蝴蝶MWS / LWS视紫红质中并行进化。

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