Fischer Rebecca A, Zube Nicholas G, Nimmo Francis
Department of Earth and Planetary Sciences, Harvard University, Cambridge, USA.
Department of Earth and Planetary Sciences, University of California Santa Cruz, Santa Cruz, USA.
Nat Commun. 2021 Jan 4;12(1):35. doi: 10.1038/s41467-020-20266-1.
The Earth and Moon have identical or very similar isotopic compositions for many elements, including tungsten. However, canonical models of the Moon-forming impact predict that the Moon should be made mostly of material from the impactor, Theia. Here we evaluate the probability of the Moon inheriting its Earth-like tungsten isotopes from Theia in the canonical giant impact scenario, using 242 N-body models of planetary accretion and tracking tungsten isotopic evolution, and find that this probability is <1.6-4.7%. Mixing in up to 30% terrestrial materials increases this probability, but it remains <10%. Achieving similarity in stable isotopes is also a low-probability outcome, and is controlled by different mechanisms than tungsten. The Moon's stable isotopes and tungsten isotopic composition are anticorrelated due to redox effects, lowering the joint probability to significantly less than 0.08-0.4%. We therefore conclude that alternate explanations for the Moon's isotopic composition are likely more plausible.
地球和月球在包括钨在内的许多元素上具有相同或非常相似的同位素组成。然而,月球形成撞击的标准模型预测,月球应该主要由撞击体忒伊亚的物质构成。在此,我们使用242个行星吸积的N体模型并追踪钨同位素的演化,评估在标准的巨型撞击情景下月球从忒伊亚继承其类似地球的钨同位素的概率,发现这个概率小于1.6 - 4.7%。混入高达30%的地球物质会增加这个概率,但仍小于10%。实现稳定同位素的相似性也是一个低概率结果,并且由与钨不同的机制控制。由于氧化还原效应,月球的稳定同位素和钨同位素组成呈反相关,将联合概率降低到显著小于0.08 - 0.4%。因此,我们得出结论,对于月球同位素组成的其他解释可能更合理。