This analysis reveals how buoyancy and gravitational forces affect motion in celestial dynamics, suggesting implications for understanding local phenomena.
There are two fundamental forces in nature: (1) the Gravitational Attractive Force (GAF), as described by Newtonian mechanics, and (2) the Buoyancy Force in the Gravitational Field (BFGF), as proposed in this study. These two forces influence motion such as orbital dynamics, rotational behavior of celestial bodies, free-fall trajectories, and the evaporation of matter within a gravitational field. Local activities are affected by larger bodies through the acceleration due to gravitational attraction (g), the Newtonian gravitational attractive force (Fn), the actual gravitational attractive force (Fa), and the buoyancy force of the gravitational field (B).
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Sankar Palchoudhury (2025) studied this question.
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