The terrestrial late veneer from core disruption of a lunar-sized impactor
The terrestrial late veneer from core disruption of a lunar-sized impactor
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DOI:
10.1016/j.epsl.2017.09.041
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发表时间:
2017-12-05
影响因子:
5.3
通讯作者:
Mojzsis, S. J.
中科院分区:
文献类型:
--
作者:
Genda, H.;Brasser, R.;Mojzsis, S. J.
Overabundances in highly siderophile elements (HSEs) of Earth's mantle can be explained by conveyance from a singular, immense (D similar to 3000 km) "Late Veneer" impactor of chondritic composition, subsequent to lunar formation and terrestrial core-closure, Such rocky objects of approximately lunar mass (similar to 00.01 M-circle plus) ought to be differentiated, such that nearly all of their HSE payload is sequestered into iron cores. Here, we analyze the mechanical and chemical fate of the core of such a Late Veneer impactor, and trace how its HSEs are suspended - and thus pollute - the mantle. For the statistically most-likely oblique collision (similar to 45 degrees), the impactor's core elongates and thereafter disintegrates into a metallic hail of small particles (similar to 10 m). Some strike the orbiting Moon as sesquinary impactors, but most re-accrete to Earth as secondaries with further fragmentation. We show that a single oblique impactor provides an adequate amount of' HSEs to the primordial terrestrial silicate reservoirs via oxidation of (