Institute of Crystallography, National Research Council of Italy, CNR, Rome, Italy.
PLoS One. 2013 May 14;8(5):e64352. doi: 10.1371/journal.pone.0064352. Print 2013.
Space missions have enabled testing how microorganisms, animals and plants respond to extra-terrestrial, complex and hazardous environment in space. Photosynthetic organisms are thought to be relatively more prone to microgravity, weak magnetic field and cosmic radiation because oxygenic photosynthesis is intimately associated with capture and conversion of light energy into chemical energy, a process that has adapted to relatively less complex and contained environment on Earth. To study the direct effect of the space environment on the fundamental process of photosynthesis, we sent into low Earth orbit space engineered and mutated strains of the unicellular green alga, Chlamydomonas reinhardtii, which has been widely used as a model of photosynthetic organisms. The algal mutants contained specific amino acid substitutions in the functionally important regions of the pivotal Photosystem II (PSII) reaction centre D1 protein near the QB binding pocket and in the environment surrounding Tyr-161 (YZ) electron acceptor of the oxygen-evolving complex. Using real-time measurements of PSII photochemistry, here we show that during the space flight while the control strain and two D1 mutants (A250L and V160A) were inefficient in carrying out PSII activity, two other D1 mutants, I163N and A251C, performed efficient photosynthesis, and actively re-grew upon return to Earth. Mimicking the neutron irradiation component of cosmic rays on Earth yielded similar results. Experiments with I163N and A251C D1 mutants performed on ground showed that they are better able to modulate PSII excitation pressure and have higher capacity to reoxidize the QA (-) state of the primary electron acceptor. These results highlight the contribution of D1 conformation in relation to photosynthesis and oxygen production in space.
太空任务使人们能够测试微生物、动物和植物对太空环境中极端、复杂和危险的条件的反应。光合生物被认为更容易受到微重力、弱磁场和宇宙辐射的影响,因为产氧光合作用与光能的捕获和转化为化学能密切相关,这个过程已经适应了地球上相对简单和封闭的环境。为了研究太空环境对光合作用基本过程的直接影响,我们将经过工程改造和突变的单细胞绿藻莱茵衣藻(Chlamydomonas reinhardtii)菌株送入近地轨道空间,该藻已被广泛用作光合生物的模型。藻类突变体在功能重要的区域含有特定的氨基酸取代,这些区域位于关键的光系统 II(PSII)反应中心 D1 蛋白的 QB 结合口袋附近以及周围 Tyr-161(YZ)电子受体的环境中。通过对 PSII 光化学的实时测量,我们在这里表明,在太空飞行期间,当对照菌株和两个 D1 突变体(A250L 和 V160A)无法有效地进行 PSII 活性时,另外两个 D1 突变体 I163N 和 A251C 能够有效地进行光合作用,并在返回地球后积极重新生长。在地球上模拟宇宙射线的中子辐照成分也得到了类似的结果。在地面上对 I163N 和 A251C D1 突变体进行的实验表明,它们能够更好地调节 PSII 激发压力,并具有更高的能力重新氧化初级电子受体的 QA(-)状态。这些结果突出了 D1 构象在太空光合作用和氧气产生中的作用。