The linear momentum (P) of a system of particles, when considered relative to its center of mass (G), satisfies DP/DT = sum of external forces, indicating that the translation of the center of mass is dictated solely by external forces, independent of internal interactions.
Torque from External Forces about an Arbitrary Point
The total external torque about an arbitrary point P is the sum of (r_i - X) cross F_i_external, where r_i is the position of particle i and X is the position of point P. This term represents the rotational effect of external forces on the system about point P.
Angular Momentum about the Origin and Center of Mass
When the reference point P is the origin of an inertial frame or the center of mass (G), the angular momentum equation simplifies significantly. If P is the origin, L_0 dot = tau_0_ext. If P is G, L_G dot = tau_G_ext, as the term involving the velocity of G and total momentum P vanishes.
The trajectory of a particle under a central inverse square force law, when analyzed using the substitution u=1/r, results in a second-order linear differential equation whose solutions are conic sections: ellipses, parabolas, or hyperbolas, depending on the eccentricity.
Derek Moulton: Comet Deflection Dynamics
The deflection angle of a comet passing near the Sun can be calculated by analyzing its trajectory using the derived orbital equations, considering initial conditions like velocity (v) and the closest approach distance (p) if the Sun were absent, leading to a deflection angle dependent on mv^2/k.
Derek Moulton: Translating Infinity Conditions
Initial conditions at 'infinity', such as a comet approaching from a large distance with a specific velocity, can be mathematically translated into conditions on u(theta) and du/d(theta) at theta=0, simplifying the solution of the orbital equation.