Mechanisms and timing of carbonaceous chondrite delivery to the Earth
Francis Nimmo, Thorsten Kleine, Alessandro Morbidelli, David, Nesvorny

TL;DR
This paper investigates the timing and mechanisms of carbonaceous chondrite material delivery to Earth, revealing late accretion of CC material during Earth's formation and proposing a model involving large CC embryos impacting Earth.
Contribution
It introduces a new model suggesting Earth accreted a few large CC embryos late in its formation, contrasting with earlier dynamical models.
Findings
Majority of Earth's accreted material was non-carbonaceous.
Carbonaceous material was delivered late, enriching Earth's mantle.
Large CC embryos impacted Earth during late accretion phase.
Abstract
The nucleosynthetic isotope signatures of meteorites and the bulk silicate Earth (BSE) indicate that Earth consists of a mixture of "carbonaceous" (CC) and "non-carbonaceous" (NC) materials. We show that the fration of CC material recorded in the isotopic composition of the BSE varies for different elements, and depends on the element's tendency to partition into metal and its volatility. The observed behaviour indicates that the majority of material accreted to the Earth was NC-dominated, but that CC-dominated material enriched in moderately-volatile elements by a factor of ~10 was delivered during the last ~2-10% of Earth's acccretion. The late delivery of CC material to Earth contrasts with dynamical evidence for the early implantation of CC objects into the inner solar system during the growth and migration of the giant planets. This, together with the NC-dominated nature of both…
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Taxonomy
TopicsAstro and Planetary Science · Spacecraft and Cryogenic Technologies
