This problem is solved by analyzing the given conditions alongside the equations of motion and energy.
The formulas for potential and kinetic energy are as follows:
The problem states that \(KE = 3 \times PE\).
\(\frac{1}{2}mv^2 = 3 \times mgh\)
\(v^2 = 6gh\) (Equation 1)
By the principle of conservation of energy, the total mechanical energy at the start equals the total mechanical energy at height \(h\).
Equating the initial and current energies:
\(mgS = mgh + \frac{1}{2}mv^2\)
\(mgS = mgh + 3mgh\) (since KE = 3PE)
\(mgS = 4mgh\)
\(gS = 4gh\)
\(h = \frac{S}{4}\) (Equation 2)
Substituting Equation 2 into Equation 1 yields the velocity:
\(v^2 = 6g \left(\frac{S}{4}\right)\)
\(v^2 = \frac{3gS}{2}\)
\(v = \sqrt{\frac{3gS}{2}}\)
Consequently, the particle is at a height of \(\frac{S}{4}\) from the surface, and its speed is \(\sqrt{\frac{3gS}{2}}\).
The height from Earth's surface at which acceleration due to gravity becomes \(\frac{g}{4}\) is \(\_\_\)? (Where \(g\) is the acceleration due to gravity on the surface of the Earth and \(R\) is the radius of the Earth.)