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Tidal Evolution of the Earth–Moon System with a High Initial Obliquity

Ćuk, Matija and Lock, Simon J. and Stewart, Sarah T. and Hamilton, Douglas P. (2021) Tidal Evolution of the Earth–Moon System with a High Initial Obliquity. Planetary Science Journal, 2 (4). Art. No. 147. ISSN 2632-3338. doi:10.3847/PSJ/ac12d1. https://resolver.caltech.edu/CaltechAUTHORS:20210813-181202854

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Abstract

A giant-impact origin for the Moon is generally accepted, but many aspects of lunar formation remain poorly understood and debated. Ćuk et al. proposed that an impact that left the Earth–Moon system with high obliquity and angular momentum could explain the Moon's orbital inclination and isotopic similarity to Earth. In this scenario, instability during the Laplace Plane transition, when the Moon's orbit transitions from the gravitational influence of Earth's figure to that of the Sun, would both lower the system's angular momentum to its present-day value and generate the Moon's orbital inclination. Recently, Tian & Wisdom discovered new dynamical constraints on the Laplace Plane transition and concluded that the Earth–Moon system could not have evolved from an initial state with high obliquity. Here we demonstrate that the Earth–Moon system with an initially high obliquity can evolve into the present state, and we identify a spin–orbit secular resonance as a key dynamical mechanism in the later stages of the Laplace Plane transition. Some of the simulations by Tian & Wisdom did not encounter this late secular resonance, as their model suppressed obliquity tides and the resulting inclination damping. Our results demonstrate that a giant impact that left Earth with high angular momentum and high obliquity (θ > 61°) is a promising scenario for explaining many properties of the Earth–Moon system, including its angular momentum and obliquity, the geochemistry of Earth and the Moon, and the lunar inclination.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.3847/psj/ac12d1DOIArticle
https://arxiv.org/abs/2107.03353arXivDiscussion Paper
ORCID:
AuthorORCID
Ćuk, Matija0000-0003-1226-7960
Lock, Simon J.0000-0001-5365-9616
Stewart, Sarah T.0000-0001-9606-1593
Hamilton, Douglas P.0000-0002-5010-0574
Additional Information:© 2021. The Author(s). Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. Received 2021 March 22; revised 2021 June 21; accepted 2021 July 7; published 2021 August 4. M.Ć. is supported by NASA's Emerging Worlds Program award 80NSSC19K0512. S.J.L. gratefully acknowledges funding from NSF through award EAR-1947614. Comments by Daniel Tamayo and two anonymous reviewers greatly improved the manuscript. The authors would like to thank Jihad Touma and the faculty and staff of the American University in Beirut for hosting a workshop on lunar formation in October 2019, which greatly advanced our understanding of early lunar evolution.
Funders:
Funding AgencyGrant Number
NASA80NSSC19K0512
NSFEAR-1947614
Subject Keywords:Earth-moon system; Inclination; Orbital resonances; Tides
Issue or Number:4
Classification Code:Unified Astronomy Thesaurus concepts: Earth-moon system (436); Inclination (78); Orbital resonances (1181); Tides (1702)
DOI:10.3847/PSJ/ac12d1
Record Number:CaltechAUTHORS:20210813-181202854
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20210813-181202854
Official Citation:Matija Ćuk et al 2021 Planet. Sci. J. 2 147
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:110253
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:16 Aug 2021 14:25
Last Modified:16 Aug 2021 14:25

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