Murthy V R
Science. 1991 Jul 19;253(5017):303-6. doi: 10.1126/science.253.5017.303.
The long-standing problem of the excess abundances of siderophile elements in the mantle can be resolved by considering an equilibrium core-mantle differentiation in the earth at 3000 to 3500 kelvin. This high-temperature differentiation results in mantle siderophile element abundances that closely match the observed values. Some lithophile (light) elements could enter the core in this process as is necessary to account for its low density. The abundances of siderophile elements in the mantle are consistent with the conclusion derived from the recent physical models that the earth was molten during accretion.
通过考虑地球在3000至3500开尔文时的地核 - 地幔平衡分异,可以解决长期存在的地幔中亲铁元素丰度过高的问题。这种高温分异导致地幔亲铁元素丰度与观测值紧密匹配。在这个过程中,一些亲石(轻)元素可能进入地核,这对于解释地核的低密度是必要的。地幔中亲铁元素的丰度与最近的物理模型得出的结论一致,即地球在吸积过程中是熔融状态的。