Biophysics of Photosynthesis, Department of Physics and Astronomy, Faculty of Sciences, VU University Amsterdam, Amsterdam, the Netherlands; Department of Physics, Jagannath University, Dhaka, Bangladesh.
Department of Physics, Jagannath University, Dhaka, Bangladesh.
Biophys J. 2021 May 4;120(9):1680-1691. doi: 10.1016/j.bpj.2021.02.037. Epub 2021 Mar 4.
Reported herein is a Stark fluorescence spectroscopy study performed on photosystem II core antenna complexes CP43 and CP47 in their native and aggregated states. The systematic mathematical modeling of the Stark fluorescence spectra with the aid of conventional Liptay formalism revealed that induction of aggregation in both the core antenna complexes via detergent removal results in a single quenched species characterized by a remarkably broad and inhomogenously broadened emission lineshape peaking around 700 nm. The quenched species possesses a fairly large magnitude of charge-transfer character. From the analogy with the results from aggregated peripheral antenna complexes, the quenched species is thought to originate from the enhanced chlorophyll-chlorophyll interaction due to aggregation. However, in contrast, aggregation of both core antenna complexes did not produce a far-red emission band at ∼730 nm, which was identified in most of the aggregated peripheral antenna complexes. The 730-nm emission band of the aggregated peripheral antenna complexes was attributed to the enhanced chlorophyll-carotenoid (lutein1) interaction in the terminal emitter locus. Therefore, it is very likely that the no occurrence of the far-red band in the aggregated core antenna complexes is directly related to the absence of lutein1 in their structures. The absence of the far-red band also suggests the possibility that aggregation-induced conformational change of the core antenna complexes does not yield a chlorophyll-carotenoid interaction associated energy dissipation channel.
本文报道了在天然态和聚集态下对光系统 II 核心天线复合物 CP43 和 CP47 进行斯塔克荧光光谱研究的结果。借助传统的利普泰形式主义对斯塔克荧光光谱进行系统的数学建模表明,通过去污剂去除诱导两种核心天线复合物聚集,会导致出现一种单一的猝灭物种,其发射谱线具有显著的宽化和非均匀展宽,峰值在 700nm 左右。猝灭物种具有相当大的电荷转移特征。从与聚集的外周天线复合物的结果类比来看,猝灭物种被认为是由于聚集导致叶绿素-叶绿素相互作用增强而产生的。然而,与大多数聚集的外周天线复合物不同的是,两种核心天线复合物的聚集并没有产生约 730nm 的远红发射带。聚集的外周天线复合物的 730nm 发射带归因于末端发射体位置中叶绿素-类胡萝卜素(叶黄素 1)相互作用的增强。因此,核心天线复合物中没有远红带的出现极有可能与它们的结构中缺少叶黄素 1 直接相关。远红带的缺失也表明,聚集诱导的核心天线复合物构象变化可能不会产生与叶绿素-类胡萝卜素相互作用相关的能量耗散通道。