School of Molecular Sciences and Center for Materials of the Universe, Arizona State University, Tempe, AZ 85281.
School of Molecular Sciences and Center for Materials of the Universe, Arizona State University, Tempe, AZ 85281
Proc Natl Acad Sci U S A. 2020 Nov 17;117(46):28645-28648. doi: 10.1073/pnas.2017312117. Epub 2020 Nov 2.
Iron sulfide minerals are widespread on Earth and likely in planetary bodies in and beyond our solar system. Using measured enthalpies of formation for three magnetic iron sulfide phases: bulk and nanophase FeS spinel (greigite), and its high-pressure monoclinic phase, we show that greigite is a stable phase in the Fe-S phase diagram at ambient temperature. The thermodynamic stability and low surface energy of greigite supports the common occurrence of fine-grained FeS in many anoxic terrestrial settings. The high-pressure monoclinic phase, thermodynamically metastable below about 3 GPa, shows a calculated negative P-T slope for its formation from the spinel. The stability of these three phases suggests their potential existence on Mercury and their magnetism may contribute to its present magnetic field.
硫化铁矿物在地球上广泛存在,在我们太阳系内外的行星体中也可能存在。利用三种磁性硫化铁相的实测生成焓:块状和纳米相的 FeS 尖晶石(陨硫铁)及其高压单斜相,我们表明陨硫铁在常温常压的 Fe-S 相图中是稳定相。陨硫铁的热力学稳定性和低表面能支持其在许多缺氧的地球环境中普遍存在细粒 FeS。高压单斜相在约 3 GPa 以下热力学亚稳,其从尖晶石形成的计算 P-T 斜率为负。这三种相的稳定性表明它们可能存在于水星上,并且它们的磁性可能有助于其当前的磁场。