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Resonances in the Early Evolution of the Earth-Moon System

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Touma, Jihad, Wisdom, Jack·1998·The Astronomical Journal

Abstract

Most scenarios for the formation of the Moon place the Moon near Earth in low-eccentricity orbit in the equatorial plane of Earth. We examine the dynamical evolution of the Earth-Moon system from such initial configurations. We find that during the early evolution of the system, strong orbital resonances are encountered. Passage through these resonances can excite large lunar orbital eccentricity and modify the inclination of the Moon to the equator. Scenarios that resolve the mutual inclination problem are presented. A period of large lunar eccentricity would result in substantial tidal heating in the early Moon, providing a heat source for the lunar magma ocean. The resonance may also play a role in the formation of the Moon.

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Metadata

Authors
Touma, J., & Wisdom, J.
Venue
The Astronomical Journal
Published
1998-04
Volume
115
Issue
4
Pages
1653-1663
ISSN
0004-6256 (ISSN-L)
OpenAlex
W2141951413
Cited by
185
References
0
FWCI
3.02
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: Resonances in the Early Evolution of the Earth-Moon System. https://app.cochat.ai/papers/10.1086/300312
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Touma, J., & Wisdom, J. (1998). Resonances in the Early Evolution of the Earth-Moon System. The Astronomical Journal. https://doi.org/10.1086/300312

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.