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).
The difference in energy levels of an electron at two excited levels is 13.75 eV. If it makes a transition from the higher energy level to the lower energy level then what will be the wavelength of the emitted radiation?
Given:
$ h = 6.6 \times 10^{-34} \, \text{m}^2 \, \text{kg} \, \text{s}^{-1} $, $ c = 3 \times 10^8 \, \text{ms}^{-1} $, $ 1 \, \text{eV} = 1.6 \times 10^{-19} \, \text{J} $
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:
200 ml of an aqueous solution contains 3.6 g of Glucose and 1.2 g of Urea maintained at a temperature equal to 27$^{\circ}$C. What is the Osmotic pressure of the solution in atmosphere units?
Given Data R = 0.082 L atm K$^{-1}$ mol$^{-1}$
Molecular Formula: Glucose = C$_6$H$_{12}$O$_6$, Urea = NH$_2$CONH$_2$