Barber James
Department of Life Sciences, Imperial College London , Sir Ernst Chain Building, South Kensington Campus, London SW7 2AZ, U.K.
Biochemistry. 2016 Oct 25;55(42):5901-5906. doi: 10.1021/acs.biochem.6b00794. Epub 2016 Oct 14.
Photosystem II is the chlorophyll-containing enzyme in which the very first chemical energy storing reaction of photosynthesis occurs, when water is split into molecular oxygen and hydrogen equivalents at a catalytic center composed of four Mn ions and one Ca. All the oxygen in the atmosphere is derived from this reaction, and without it the biosphere, as we know it, would not exist. Indeed, the appearance of this catalytic center ∼3 billion years ago gave rise to the "big bang of evolution". Thus, understanding the structure and functioning of this metal cluster is a major topic in science, and here I discuss it in terms of research that has occurred over the past 12 years dating back to when it was first proposed to be a MnCaO cubane with the fourth Mn attached to cubane by one of its oxo bridging bonds. Since then, a number of novel properties have emerged for this metalloprotein with implications for its catalytic mechanism and evolutionary origin.
光系统II是一种含叶绿素的酶,光合作用中最初的化学能储存反应就发生于此,即水在由四个锰离子和一个钙离子组成的催化中心被分解为分子氧和氢当量。大气中的所有氧气都来源于此反应,没有它,我们所知的生物圈就不会存在。事实上,这个催化中心大约在30亿年前的出现引发了“进化大爆炸”。因此,了解这个金属簇的结构和功能是科学领域的一个主要课题,在此我将根据过去12年的研究来探讨它,这些研究可以追溯到它最初被认为是一个锰钙氧立方烷,第四个锰通过其一个氧桥键连接到立方烷上的时候。从那时起,这种金属蛋白出现了许多新特性,这对其催化机制和进化起源具有重要意义。