2016
DOI: 10.1002/2016gc006305
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Asteroid bombardment and the core of Theia as possible sources for the Earth's late veneer component

Abstract: The silicate Earth contains Pt-group elements in roughly chondritic relative ratios, but with absolute concentrations <1% chondrite. This veneer implies addition of chondritelike material with 0.3-0.7% mass of the Earth's mantle or an equivalent planet-wide thickness of 5-20 km. The veneer thickness, 200-300 m, within the lunar crust and mantle is much less. One hypothesis is that the terrestrial veneer arrived after the moon-forming impact within a few large asteroids that happened to miss the smaller Moon.Al… Show more

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Cited by 23 publications
(22 citation statements)
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References 113 publications
(250 reference statements)
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“…Their concentrations, thus, do not bear on the later asteroid flux (Ryder, 2002;Zahnle and Sleep, 2006;Brasser et al, 2016;Sleep, 2016). The predicted impact flux to the Earth is relatively benign.…”
Section: Extrapolation From the Lunar Recordmentioning
confidence: 90%
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“…Their concentrations, thus, do not bear on the later asteroid flux (Ryder, 2002;Zahnle and Sleep, 2006;Brasser et al, 2016;Sleep, 2016). The predicted impact flux to the Earth is relatively benign.…”
Section: Extrapolation From the Lunar Recordmentioning
confidence: 90%
“…The average flux was 2 · 10 14 mol/ year over 600 My. The accreted mass and the flux estimates need to be reduced by a factor of *10 if most of the veneer arrived within the core of Theia rather than accreted asteroids (Sleep, 2016). Further, almost all the extraterrestrial material arrived within large bodies that likely produced a few transient episodes of global reducing conditions.…”
Section: Survival Of Life In the Hadean And Early Archean With Concenmentioning
confidence: 99%
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“…The immediate, post-impact, thermal pulse far exceeds both ultra-high-temperature metamorphism in tectonic settings (Heisinger and Head, 2006;Korhonen et al, 2014) and the liquidus temperatures of target rocks, and is therefore important for the evolution of planet and asteroid surfaces. The heat associated with impacts had a profound significance on the early Earth, and has been shown to have affected processes in Earth's core (Arkani-Hamed and Ghods, 2011;Monteux et al, 2015;Sleep, 2016), mantle (Watters et al, 2009), crust and atmosphere (Marchi et al, 2016;Marchi et al, 2014;Marchi et al, 2013;Melosh, 2008).…”
Section: Introductionmentioning
confidence: 99%