Collisionless Encounters and the Origin of the Lunar Inclination

Abstract

The Moon is generally thought to have formed from the debris ejected by the impact of a planet-sized object with the proto-Earth towards the end of planetary accretion. Modeling of the impact process predicts that the lunar material was disaggregated into a circumplanetary disk and that lunar accretion subsequently placed the Moon in a near equatorial orbit. Forward integration of the lunar orbit from this initial state predicts a modern inclination at least an order of magnitude smaller than the lunar value, a long-standing discrepancy known as the lunar inclination problem. Here we show that the modern lunar orbit provides a sensitive record of gravitational interactions with Earth-crossing planetesimals not yet accreted at the time of the Moon-forming event. The excited lunar orbit can naturally be reproduced via interaction with a small quantity of mass (corresponding to 0.0075-0.015 ME eventually accreted to the Earth) carried by a few bodies, consistent with constraints and models of late accretion. While the process has a stochastic element, the observed value of the lunar inclination is among the most likely outcomes for a wide range of parameters. The excitation of the lunar orbit is most readily reproduced via collisionless encounters with strong tidal dissipation on the early Earth. This mechanism obviates the necessity of previously proposed (but idealized) excitation mechanisms and can constrain the planet formation context of the Moon-forming event and the pristineness of the dynamical state of the Earth-Moon system.

arXiv comment24 pages, 6 figures; updated figures

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Cited by in corpus (17)

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• Late veneer and late accretion to the terrestrial planets
• Hydrogen isotopic evidence for early oxidation of silicate Earth
• Tidal Evolution of the Evection Resonance/Quasi-Resonance and the Angular Momentum of the Earth-Moon System
• Immediate origin of the Moon as a post-impact satellite
• Primordial Earth mantle heterogeneity caused by the Moon-forming giant impact
• Speciation and Dissolution of Hydrogen in the Proto-Lunar Disk
• A past lunar dynamo thermally driven by the precession of its inner core
• Rapid solidification of Earth's magma ocean limits early lunar recession
• The thermal-orbital evolution of the Earth-Moon system with a subsurface magma ocean and fossil figure
• Moonfalls: Collisions between the Earth and its past moons
• Formation of embryos of the Earth and the Moon from the common rarefied condensation and their subsequent growth
• Secular Resonance Between Iapetus and the Giant Planets
• Growth of the Moon due to bodies ejected from the Earth
• Early Dynamics of the Lunar Core