Department of Earth and Planetary Systems Science, Hiroshima University, Higashi-Hiroshima 739-8526, Japan.
Graduate School of Engineering, Osaka University, Suita 565-0871, Japan.; Photon Pioneers Center, Osaka University, Suita 565-0871, Japan.
Sci Adv. 2016 Aug 3;2(8):e1600157. doi: 10.1126/sciadv.1600157. eCollection 2016 Aug.
Forsterite (Mg2SiO4) is one of the major planetary materials, and its behavior under extreme conditions is important to understand the interior structure of large planets, such as super-Earths, and large-scale planetary impact events. Previous shock compression measurements of forsterite indicate that it may melt below 200 GPa, but these measurements did not go beyond 200 GPa. We report the shock response of forsterite above ~250 GPa, obtained using the laser shock wave technique. We simultaneously measured the Hugoniot and temperature of shocked forsterite and interpreted the results to suggest the following: (i) incongruent crystallization of MgO at 271 to 285 GPa, (ii) phase transition of MgO at 285 to 344 GPa, and (iii) remelting above ~470 to 500 GPa. These exothermic and endothermic reactions are seen to occur under extreme conditions of pressure and temperature. They indicate complex structural and chemical changes in the system MgO-SiO2 at extreme pressures and temperatures and will affect the way we understand the interior processes of large rocky planets as well as material transformation by impacts in the formation of planetary systems.
镁橄榄石(Mg2SiO4)是主要的行星物质之一,了解其在极端条件下的行为对于理解大型行星(如超级地球)的内部结构以及大规模行星撞击事件非常重要。先前对镁橄榄石的冲击压缩测量表明,它可能在 200 GPa 以下熔化,但这些测量并未超过 200 GPa。我们使用激光冲击波技术报告了约 250 GPa 以上镁橄榄石的冲击响应。我们同时测量了冲击镁橄榄石的冲击和温度,并对结果进行了解释,表明:(i)在 271 至 285 GPa 时氧化镁的不相容结晶,(ii)在 285 至 344 GPa 时氧化镁的相变,以及(iii)在约 470 至 500 GPa 以上的再熔化。这些放热和吸热反应是在压力和温度极端条件下发生的。它们表明在极端压力和温度下,MgO-SiO2 体系中的结构和化学变化复杂,这将影响我们对大型岩石行星内部过程的理解,以及行星系统形成过程中撞击引起的物质转化。