Basic Mechanics of Planet-Satellite Interaction with special reference to Earth-Moon System
Bijay Kumar Sharma

TL;DR
This paper revisits Darwin's analysis of the Earth-Moon system, using modern data to model the Moon's recession and Earth's rotational changes, and proposes a novel application of day-length variations as an earthquake precursor.
Contribution
It provides a refined theoretical model of Earth-Moon interactions incorporating evolving Earth's moment of inertia and extends the mechanics to simulate other planet-satellite systems.
Findings
Theoretical graph of day-lengthening matches observational data in the post-Cambrian era.
Deviations in ancient data suggest Earth's moment of inertia has evolved.
Proposes using day-length variations as indicators for seismic activity.
Abstract
In1879 George Howard Darwin theoretically analyzed the outward spiraling orbit of Moon and the subsequent lengthening of the Mean Solar Day. The author redid the same analysis based on the fact that Moon was receding at the rate of 3.8 cm per annum. Basic Mechanics of Earth-Moon is worked out and various system parameters are optimized to fit the given boundary condition obtained by Apollo Mission and other modern means of observations. Based on this theoretical formulation the theoretical graph of the lengthening of the Mean Solar Day with respect to time is drawn and is compared with the observational graph of the same based on pale ontological data, paleo tidal data and iron-banded formation. The observational data on Mean Solar Day is found to follow the theoretical smooth curve in post-Cambrian Era but is found to deviate in the remote past. This deviation is corrected by taking…
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Taxonomy
TopicsAstro and Planetary Science · Planetary Science and Exploration · Space Science and Extraterrestrial Life
