High obliquity, high Angular Momentum Earth as Moon origin revisited by Advanced Kinematic Model of Earth-Moon System
Bijay Kumar Sharma

TL;DR
This paper revisits the high obliquity, high angular momentum Earth-Moon formation model using an advanced kinematic model to analyze the evolution of Earth's obliquity and lunar orbit, providing new insights and validation.
Contribution
It introduces an advanced kinematic model that accurately traces Earth's obliquity and lunar orbital parameters, validating and extending previous Moon formation theories.
Findings
AKM's valid application range is from 45R_E to 60.33R_E.
Evolution of lunar orbit parameters aligns with previous simulations.
AKM successfully models Earth's obliquity evolution and LOD curve.
Abstract
Matija Cuk et.al (2016) have proposed a new model for the birth and tidal evolution of our natural satellite Moon, born from impact generated terrestrial debris in the equatorial plane of high obliquity, high angular momentum Earth. This paper examines their findings critically in the light of advanced kinematic model (AKM) which includes Earth's obliquity (\phi), Moon's orbital plane inclination (\alpha) , Moon's obliquity (\beta) and lunar's orbit eccentricity (e). For the real Earth-Moon (E-M) system, the history of evolution of \phi, \alpha, \beta, e and (length of month)/(length of day) or LOM/LOD is traced from 45R_{E} to 60.33R_{E} where R_{E} is Earth Radius. It is shown that AKM's valid range of application is from 45R_{E} to 60.33R_{E} . The evolution of {\alpha}, \beta, e is in correspondence with the simulation results of Matija Cuk et.al (2016) but evolution of Earth's…
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Taxonomy
TopicsPlanetary Science and Exploration · Astro and Planetary Science · Marine and environmental studies
