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Aphelion
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Orbital Mechanics and Calculation
For an elliptical orbit under the influence of a central gravitational force, the distance $r$ from the central body (assumed to be the focus of the ellipse) varies sinusoidally around the semi-major axis $a$. Aphelion ($ra$) and perihelion ($rp$) define the extremities of this variation.
The distance at aphelion is calculated using the semi-major axis ($a$) and the eccentricity ($e$) of the o… -
Archimedes' Principle
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$g$ is the local acceleration due to gravity.
The direction of $\mathbf{F}_{\text{B}}$ is always vertically upward, opposing the net gravitational force experienced by the object.
Density and State of Buoyancy -
Ball Flight Dynamics
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Fundamental Forces Governing Trajectory
The motion of any airborne ball is primarily dictated by four interacting forces: gravitational force, initial impulse vector, aerodynamic drag, and lift(-or rotational deflection).
Gravitational Force ($F_g$) -
Ball Flight Dynamics
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Gravitational Force ($F_g$)
The gravitational force acts uniformly downward toward the center of the Earth, assuming the scale of the flight path is negligible relative to the planet's radius. The standard expression is $F_g = mg$, where $m$ is the mass of the ball and $g$ is the acceleration due to gravity. In contexts requiring high precision, such as competitive billiards played on elevated tables, the latitude-dependent variation of $g$ … -
Cavendish Experiment
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The experiment relies on the principles of Newtonian gravitation. When the large masses ($M$) are positioned near the small masses ($m$), the gravitational torque ($\tau$) causes the fiber to twist by a small angle ($\theta$).
The gravitational force ($F$) between one pair of masses is given by:
$$F = G \frac{Mm}{r^2}$$
where $r$ is the separation distance.