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Journal Articles Geophysical Research Letters Year : 2017

Geochemical Constraints on the Size of the Moon-Forming Giant Impact

Abstract

Recent models involving the Moon-forming giant impact hypothesis have managed to reproduce the striking isotopic similarity between the two bodies, albeit using two extreme models: one involves a high-energy small impactor that makes the Moon out of Earth's proto-mantle; the other supposes a gigantic collision between two half-Earths creating the Earth-Moon system from both bodies. Here we modeled the geochemical influence of the giant impact on Earth's mantle and found that impactors larger than 15% of Earth mass result in mantles always violating the present-day concentrations of four refractory moderately siderophile trace elements (Ni, Co, Cr, and V). In the aftermath of the impact, our models cannot further discriminate between a fully and a partially molten bulk silicate Earth. Then, the preservation of primordial geochemical reservoirs predating the Moon remains the sole argument against a fully molten mantle after the Moon-forming impact.
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Dates and versions

insu-02558677 , version 1 (29-04-2020)

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Hélène Piet, James Badro, Philippe Gillet. Geochemical Constraints on the Size of the Moon-Forming Giant Impact. Geophysical Research Letters, 2017, 44 (23), pp.11,770-11,777. ⟨10.1002/2017GL075225⟩. ⟨insu-02558677⟩
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