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- W2525282348 endingPage "121" @default.
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- W2525282348 abstract "The Moon migrated to cm over a characteristic time r/v=10 Gyr by tidal interaction with Earth’s oceans at a present velocity of v=3.8 cm yr−1. We model global dissipation to cover the entire history over the past 4.52 Gyr. We use scaling and numerical integration to model the off-resonance tidal interactions at relatively short tidal periods in the past to a near-resonance state at present. The global properties of the complex spatio-temporal dynamics and dissipation in broad spectrum ocean waves is modeled by damping ϵ=hF/(2Q0), where h is the tidal wave amplitude, F is the tidal frequency, and Q0 is the Q-factor at the present time. It satisfies Q0 ≃ 14 for consistency of migration time and age of the Moon consistent with observations for a near-resonance state today. Numerical results reveal the need for scaling with amplitude. It shows a startlingly fast eviction of the Moon from an unstable near-synchronous orbit close to the Roche limit, probably in a protolunar disk. Rapid spin down of Earth from an initial ∼ 30% of break-up by the Moon favored early formation of a clement global climate. Our theory suggests moons may be similarly advantageous to potentially habitable exoplanets." @default.
- W2525282348 created "2016-10-07" @default.
- W2525282348 creator A5088500024 @default.
- W2525282348 date "2017-07-01" @default.
- W2525282348 modified "2023-09-25" @default.
- W2525282348 title "Scaling in global tidal dissipation of the Earth-Moon system" @default.
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- W2525282348 doi "https://doi.org/10.1016/j.newast.2017.01.012" @default.
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