Sridharan Deepa M, Chappell Lori J, Whalen Mary K, Cucinotta Francis A, Pluth Janice M
a Lawrence Berkeley National Laboratory, Life Sciences Division, Berkeley, California 94710;
b NASA, Lyndon B. Johnson Space Center, Houston, Texas 77058; and.
Radiat Res. 2015 Jul;184(1):105-19. doi: 10.1667/RR13684.1. Epub 2015 Jun 26.
During space travel, astronauts are exposed to a wide array of high-linear energy transfer (LET) particles, with differing energies and resulting biological effects. Risk assessment of these exposures carries a large uncertainty predominantly due to the unique track structure of the particle's energy deposition. The complex damage elicited by high charge and energy (HZE) particles results from both lesions along the track core and from energetic electrons, δ rays, generated as a consequence of particle traversal. To better define how cells respond to this complex radiation exposure, a normal hTERT immortalized skin fibroblast cell line was exposed to a defined panel of particles carefully chosen to tease out track structure effects. Phosphorylation kinetics for several key double-strand break (DSB) response proteins (γ-H2AX, pATF2 and pSMC1) were defined after exposure to ten different high-LET radiation qualities and one low-LET radiation (X ray), at two doses (0.5-2 Gy) and time points (2 and 24 h). The results reveal that the lower energy particles (Fe 300, Si 93 and Ti 300 MeV/u), with a narrower track width and higher number and intensity of δ rays, cause the highest degree of persistent damage response. The persistent γ-H2AX signal at lower energies suggests that damage from these exposures are more difficult to resolve, likely due to the greater complexity of the associated DNA lesions. However, different kinetics were observed for the solely ATM-mediated phosphorylations (pATF2 and pSMC1), revealing a shallow induction at early times and a higher level of residual phosphorylation compared to γ-H2AX. The differing phospho-protein profiles exhibited, compared to γ-H2AX, suggests additional functions for these proteins within the cell. The strong correspondence between the predicted curves for energy deposition per nucleosome for each ion/energy combination and the persistent levels of γ-H2AX indicates that the nature of energy distribution defines residual levels of γ-H2AX, an indicator of unrepaired DSBs. Our results suggest that decreasing the energy of a particle results in more complex damage that may increase genomic instability and increase the risk of carcinogenesis.
在太空旅行期间,宇航员会受到各种各样的高传能线密度(LET)粒子的辐射,这些粒子具有不同的能量并产生不同的生物效应。对这些辐射暴露进行风险评估存在很大的不确定性,主要原因是粒子能量沉积的独特径迹结构。高电荷和能量(HZE)粒子引发的复杂损伤既源于径迹核心处的损伤,也源于粒子穿过时产生的高能电子(δ射线)。为了更好地确定细胞如何应对这种复杂的辐射暴露,我们将一种正常的hTERT永生化皮肤成纤维细胞系暴露于一组精心挑选的粒子中,以梳理出径迹结构效应。在暴露于十种不同的高LET辐射性质以及一种低LET辐射(X射线)后,在两个剂量(0.5 - 2 Gy)和时间点(2小时和24小时)测定了几种关键双链断裂(DSB)反应蛋白(γ-H2AX、pATF2和pSMC1) 的磷酸化动力学。结果表明,能量较低的粒子(铁离子300 MeV/u、硅离子93 MeV/u和钛离子300 MeV/u),其径迹宽度较窄,δ射线数量和强度较高,会导致最高程度的持续性损伤反应。较低能量下持续的γ-H2AX信号表明,这些辐射暴露造成的损伤更难修复,这可能是由于相关DNA损伤的复杂性更高。然而,对于仅由ATM介导的磷酸化(pATF2和pSMC1),观察到了不同的动力学,与γ-H2AX相比,其在早期诱导较浅,残留磷酸化水平较高。与γ-H2AX相比,所呈现的不同磷酸化蛋白谱表明这些蛋白在细胞内具有额外的功能。每种离子/能量组合的每个核小体能量沉积预测曲线与γ-H2AX的持续水平之间的强烈对应关系表明,能量分布的性质决定了γ-H2AX的残留水平,γ-H2AX是未修复DSB的一个指标。我们的结果表明,降低粒子能量会导致更复杂的损伤,这可能会增加基因组不稳定性并增加致癌风险。