To determine the maximum velocity \( V \) of a solid sphere of mass \( M \) and radius \( R \) that can roll over a step of height \( \frac{R}{4} \) without losing contact with the surface, we need to analyze the forces and energy involved in this scenario. The key here is to ensure that the sphere maintains contact with the surface as it rolls over the step.
Understanding the Dynamics of the Sphere
When the sphere rolls over the step, it will pivot around the edge of the step. At the point of contact with the step, the sphere experiences a change in its center of mass height, which affects the gravitational potential energy and the kinetic energy of the sphere.
Energy Considerations
Initially, the sphere has kinetic energy due to its velocity \( V \) and gravitational potential energy due to its height. As it approaches the step, we can express the total mechanical energy as:
- Kinetic Energy: \( KE = \frac{7}{10} MV^2 \) (for a solid sphere, considering both translational and rotational motion)
- Potential Energy: \( PE = MgH \), where \( H \) is the height of the center of mass above the reference point.
When the sphere reaches the top of the step, its center of mass will rise by \( \frac{R}{4} \). Therefore, the change in potential energy as it climbs the step is:
Change in Potential Energy: \( \Delta PE = Mg \cdot \frac{R}{4} \)
Applying Conservation of Energy
Using the conservation of energy principle, the initial kinetic energy must equal the sum of the potential energy at the top of the step and the kinetic energy at that point:
\( \frac{7}{10} MV^2 = Mg \cdot \frac{R}{4} + KE_{top} \)
At the top of the step, the sphere will have some velocity \( v_{top} \). The kinetic energy at that point can be expressed as:
\( KE_{top} = \frac{7}{10} Mv_{top}^2 \)
Finding the Maximum Velocity
To ensure the sphere does not lose contact with the step, we need to analyze the forces acting on it at the top of the step. The gravitational force must provide the necessary centripetal force to keep the sphere in contact:
At the top of the step, the gravitational force acting downwards is \( Mg \), and the required centripetal force is \( \frac{Mv_{top}^2}{R} \). For the sphere to maintain contact, we need:
\( Mg \geq \frac{Mv_{top}^2}{R} \)
From this, we can derive that:
\( g \geq \frac{v_{top}^2}{R} \)
Thus, \( v_{top}^2 \leq gR \) or \( v_{top} \leq \sqrt{gR} \).
Combining the Equations
Now, substituting \( v_{top} \) back into the energy equation:
\( \frac{7}{10} MV^2 = Mg \cdot \frac{R}{4} + \frac{7}{10} M(\sqrt{gR})^2 \)
After simplifying, we get:
\( \frac{7}{10} V^2 = g \cdot \frac{R}{4} + \frac{7}{10} gR \)
Combining the terms gives:
\( \frac{7}{10} V^2 = gR \left( \frac{1}{4} + \frac{7}{10} \right) \)
Calculating the right side:
\( \frac{1}{4} + \frac{7}{10} = \frac{5}{20} + \frac{14}{20} = \frac{19}{20} \)
Thus, we have:
\( \frac{7}{10} V^2 = \frac{19}{20} gR \)
Solving for \( V^2 \):
\( V^2 = \frac{19}{20} \cdot \frac{10}{7} gR = \frac{19gR}{14} \)
Finally, taking the square root gives us the maximum velocity:
\( V = \sqrt{\frac{19gR}{14}} \)
Final Velocity After the Step
After the sphere rolls over the step, it will continue to roll with a new velocity that can be calculated using the conservation of energy principle again, considering the height change and the kinetic energy at the top of the step. However, the maximum velocity before encountering the step is crucial for ensuring it maintains contact.
In summary, the maximum velocity \( V \) of the sphere to ensure it does not lose contact while rolling over the step of height \( \frac{R}{4} \) is given by:
\( V = \sqrt{\frac{19gR}{14}} \)