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Question: As shown a smooth hemisphere, of mass $M = 4$ kg and radius $a = 2$ m, is placed with its plane base...

As shown a smooth hemisphere, of mass M=4M = 4 kg and radius a=2a = 2 m, is placed with its plane base on a smooth table. A rod, of mass m=2m = 2 kg is constrained to move in a vertical line with one end PP on the curved surface of the hemisphere. Find the angular speed (in rad/s) of point PP with respect to centre OO of the hemisphere when OPOP makes an angle θ=60°\theta = 60° with the vertical. Initially the rod was at the topmost point of the hemisphere. (g=10 m/s2g = 10 \ m/s^2)

Answer

2

Explanation

Solution

The problem involves a system of a hemisphere and a rod, both of which can move. Since all surfaces are smooth, there is no friction, implying that mechanical energy is conserved. The rod is constrained to move vertically by a fixed guide, and the hemisphere is on a smooth horizontal table.

1. Conservation of Mechanical Energy: The system consists of the rod (mass mm) and the hemisphere (mass MM).

  • Initial State: The rod is at the topmost point of the hemisphere. Both are at rest.
    Let the potential energy reference be the base of the hemisphere.
    Initial height of point P (on the rod) is aa.
    Initial Kinetic Energy, KEi=0KE_i = 0.
    Initial Potential Energy, PEi=mgaPE_i = mga.
    Total Initial Energy, Ei=mgaE_i = mga.

  • Final State: OP makes an angle θ=60°\theta = 60° with the vertical.
    Let vMv_M be the horizontal velocity of the hemisphere and vmv_m be the vertical velocity of the rod.
    Final Kinetic Energy, KEf=12MvM2+12mvm2KE_f = \frac{1}{2} M v_M^2 + \frac{1}{2} m v_m^2.
    Final height of point P is acosθa \cos\theta.
    Final Potential Energy, PEf=mgacosθPE_f = mg a \cos\theta.
    Total Final Energy, Ef=12MvM2+12mvm2+mgacosθE_f = \frac{1}{2} M v_M^2 + \frac{1}{2} m v_m^2 + mg a \cos\theta.

By conservation of mechanical energy (Ei=EfE_i = E_f): mga=12MvM2+12mvm2+mgacosθmga = \frac{1}{2} M v_M^2 + \frac{1}{2} m v_m^2 + mg a \cos\theta
12MvM2+12mvm2=mga(1cosθ)\frac{1}{2} M v_M^2 + \frac{1}{2} m v_m^2 = mga(1 - \cos\theta) (Equation 1)

2. Kinematic Constraint (Relation between vMv_M and vmv_m): Point P is always on the surface of the hemisphere.
Let the position of the center of the hemisphere be (X,0)(X, 0) and the rod be constrained to move along the vertical line xP=x0x_P = x_0.
The equation of the hemisphere surface for point P at (xP,yP)(x_P, y_P) is (xPX)2+yP2=a2(x_P - X)^2 + y_P^2 = a^2.
Differentiating this equation with respect to time:
2(xPX)(x˙PX˙)+2yPy˙P=02(x_P - X)(\dot{x}_P - \dot{X}) + 2y_P \dot{y}_P = 0.
We know x˙P=0\dot{x}_P = 0 (rod moves vertically).
Let X˙=vM\dot{X} = v_M (velocity of hemisphere).
Let y˙P=vm\dot{y}_P = v_m (velocity of rod).
So, (xPX)(vM)+yPvm=0(x_P - X)(-v_M) + y_P v_m = 0.

In the final state, the point P is at an angle θ\theta with the vertical. Its coordinates relative to the center O of the hemisphere are (asinθ,acosθ)(a \sin\theta, a \cos\theta) (assuming P is to the right of O).
The horizontal position of P is xP=X+asinθx_P = X + a \sin\theta.
Since xPx_P is constant, and initially xP=Xinitial+asin(0)=Xinitialx_P = X_{initial} + a \sin(0) = X_{initial}, we have xP=Xinitialx_P = X_{initial}.
So, Xinitial=X+asinθX_{initial} = X + a \sin\theta. This means XXinitial=asinθX - X_{initial} = -a \sin\theta. The hemisphere moves to the left, which is consistent with the diagram.
The term (xPX)(x_P - X) represents the horizontal distance of P from the center O. So, xPX=asinθx_P - X = a \sin\theta.
The term yPy_P represents the vertical distance of P from the base, which is acosθa \cos\theta (height of P above O).
Substituting these into the differentiated equation:
(asinθ)(vM)+(acosθ)vm=0(a \sin\theta)(-v_M) + (a \cos\theta)v_m = 0
vMsinθ+vmcosθ=0-v_M \sin\theta + v_m \cos\theta = 0
vm=vMsinθcosθ=vMtanθv_m = v_M \frac{\sin\theta}{\cos\theta} = v_M \tan\theta (Equation 2)

3. Calculate Velocities: Substitute Equation 2 into Equation 1:
12MvM2+12m(vMtanθ)2=mga(1cosθ)\frac{1}{2} M v_M^2 + \frac{1}{2} m (v_M \tan\theta)^2 = mga(1 - \cos\theta)
12vM2(M+mtan2θ)=mga(1cosθ)\frac{1}{2} v_M^2 (M + m \tan^2\theta) = mga(1 - \cos\theta)
vM2=2mga(1cosθ)M+mtan2θv_M^2 = \frac{2 mga(1 - \cos\theta)}{M + m \tan^2\theta}

Given values: M=4M = 4 kg, m=2m = 2 kg, a=2a = 2 m, θ=60°\theta = 60°, g=10 m/s2g = 10 \ m/s^2.
cos60°=1/2\cos 60° = 1/2
tan60°=3\tan 60° = \sqrt{3}, so tan260°=3\tan^2 60° = 3.
1cosθ=11/2=1/21 - \cos\theta = 1 - 1/2 = 1/2.

Substitute the values:
vM2=2×2×10×2×(1/2)4+2×3v_M^2 = \frac{2 \times 2 \times 10 \times 2 \times (1/2)}{4 + 2 \times 3}
vM2=404+6=4010=4 m2/s2v_M^2 = \frac{40}{4 + 6} = \frac{40}{10} = 4 \ m^2/s^2.
So, vM=2 m/s|v_M| = 2 \ m/s.

4. Calculate Angular Speed (ω\omega): The angular speed of point P with respect to the center O of the hemisphere, ω\omega, is related to the velocity of P relative to O.
The velocity of P relative to O is vP/O=vPvO\vec{v}_{P/O} = \vec{v}_P - \vec{v}_O.
Since the rod moves vertically, vP=vmj^\vec{v}_P = v_m \hat{j}.
The hemisphere moves horizontally, so vO=vMi^\vec{v}_O = v_M \hat{i}.
vP/O=vmj^vMi^\vec{v}_{P/O} = v_m \hat{j} - v_M \hat{i}.
The magnitude of this relative velocity is vP/O=vm2+vM2v_{P/O} = \sqrt{v_m^2 + v_M^2}.
Also, for a point moving on a circle of radius aa with angular speed ω\omega, vP/O=aωv_{P/O} = a\omega.
So, aω=vm2+vM2a\omega = \sqrt{v_m^2 + v_M^2}.
Using vm=vMtanθv_m = v_M \tan\theta:
aω=(vMtanθ)2+vM2=vM2(tan2θ+1)=vM2sec2θ=vMsecθa\omega = \sqrt{(v_M \tan\theta)^2 + v_M^2} = \sqrt{v_M^2 (\tan^2\theta + 1)} = \sqrt{v_M^2 \sec^2\theta} = |v_M \sec\theta|.
Since θ=60°\theta = 60°, secθ=sec60°=2\sec\theta = \sec 60° = 2.
aω=vMsecθa\omega = |v_M| \sec\theta.
ω=vMsecθa\omega = \frac{|v_M| \sec\theta}{a}.
Substitute vM=2 m/s|v_M| = 2 \ m/s, a=2a = 2 m, secθ=2\sec\theta = 2:
ω=2×22=2 rad/s\omega = \frac{2 \times 2}{2} = 2 \ rad/s.

The final answer is 2\boxed{2}.

Explanation: The problem is solved using the principle of conservation of mechanical energy and kinematic constraints.

  1. Conservation of Energy: Since all surfaces are smooth and the guide force does no work, the total mechanical energy of the rod-hemisphere system is conserved. The initial energy (potential energy of the rod at height 'a') is equated to the final energy (kinetic energy of both rod and hemisphere + potential energy of the rod at height 'a cosθ').
  2. Kinematic Constraint: The condition that the rod's end P remains on the hemisphere's surface and the rod moves vertically provides a crucial relationship between the velocities of the rod and the hemisphere. This relationship is derived by differentiating the equation of the hemisphere's surface with respect to time, considering the fixed horizontal position of the rod. It leads to vm=vMtanθv_m = v_M \tan\theta.
  3. Angular Speed: The angular speed of P with respect to O is the magnitude of the velocity of P relative to O, divided by the radius 'a'. The velocity of P relative to O is found by vector subtraction: vP/O=vPvO\vec{v}_{P/O} = \vec{v}_P - \vec{v}_O.

Answer: The angular speed of point P with respect to centre O of the hemisphere is 2 rad/s.