The areal velocity of a planet is defined as the rate at which the planet sweeps out area in its orbit. For a planet of mass \( M \) and distance \( r \) from the Sun, the areal velocity \( A \) is given by: \[ A = \frac{dA}{dt} = \frac{1}{2} r^2 \omega, \] where \( r \) is the radius vector and \( \omega \) is the angular velocity.
Step 1: Relationship between angular momentum and areal velocity
The angular momentum \( L \) of a planet is given by: \[ L = M r^2 \omega, \] where \( M \) is the mass of the planet and \( r^2 \omega \) is the angular momentum per unit mass.
Now, using the expression for areal velocity \( A = \frac{1}{2} r^2 \omega \), we can solve for \( r^2 \omega \): \[ r^2 \omega = 2A. \]
Step 2: Final angular momentum
Substitute \( r^2 \omega = 2A \) into the expression for angular momentum: \[ L = M \times 2A = 2MA. \] Thus, the angular momentum of the planet is \( 2MA \), which corresponds to option (C).
A solid cylinder of mass 2 kg and radius 0.2 m is rotating about its own axis without friction with angular velocity 5 rad/s. A particle of mass 1 kg moving with a velocity of 5 m/s strikes the cylinder and sticks to it as shown in figure.
The angular velocity of the system after the particle sticks to it will be: