Bayerisches Geoinstitut, Bayreuth, Germany.
Bayerisches Geoinstitut, Bayreuth, Germany. Observatoire de la Cote d'Azur, Nice, France.
Science. 2016 Sep 9;353(6304):1141-4. doi: 10.1126/science.aaf6919.
Highly siderophile elements (HSEs) are strongly depleted in the bulk silicate Earth (BSE) but are present in near-chondritic relative abundances. The conventional explanation is that the HSEs were stripped from the mantle by the segregation of metal during core formation but were added back in near-chondritic proportions by late accretion, after core formation had ceased. Here we show that metal-silicate equilibration and segregation during Earth's core formation actually increased HSE mantle concentrations because HSE partition coefficients are relatively low at the high pressures of core formation within Earth. The pervasive exsolution and segregation of iron sulfide liquid from silicate liquid (the "Hadean matte") stripped magma oceans of HSEs during cooling and crystallization, before late accretion, and resulted in slightly suprachondritic palladium/iridium and ruthenium/iridium ratios.
亲铁元素(HSEs)在地球的整体硅酸盐中被严重耗尽,但在近球粒陨石的相对丰度上存在。传统的解释是,HSEs 是在核心形成过程中通过金属的分异从地幔中剥离出来的,但在核心形成停止后,通过晚期吸积以近乎球粒陨石的比例添加回来。在这里,我们表明,地球核心形成过程中的金属-硅酸盐平衡和分异实际上增加了 HSE 地幔浓度,因为在地球核心形成的高压下,HSE 的分配系数相对较低。在晚期吸积之前,铁硫化物液体从硅酸盐液体(“冥古宙的铁镁矿”)中广泛的出溶和分异,在冷却和结晶过程中从岩浆海洋中剥离了 HSE,导致钯/铱和钌/铱的比值略高于球粒陨石。