Consider a point charge +Q of mass m suspended by a massless, inextensible string of length l in free space (permittivity \( \epsilon_0 \)) as shown in the figure. It is placed at a height \( d \) (\( d > l \)) over an infinitely large, grounded conducting plane. The gravitational potential energy is assumed to be zero at the position of the conducting plane and is positive above the plane. 
Consider a spherical galaxy of total mass \( M \) and radius \( R \), having a uniform matter distribution. In this idealized situation, the orbital speed \( v \) of a star of mass \( m \ll M \) as a function of the distance \( r \) from the galactic centre is best described by \[ (G \text{ is the universal gravitational constant}) \] 
A uniform block of mass \(M\) slides on a smooth horizontal bar. Another mass \(m\) is connected to it by an inextensible string of length \(l\) of negligible mass, and is constrained to oscillate in the X-Y plane only. Neglect the sizes of the masses. The number of degrees of freedom of the system is two and the generalized coordinates are chosen as \(x\) and \(\theta\), as shown in the figure.

If \(p_x\) and \(p_\theta\) are the generalized momenta corresponding to \(x\) and \(\theta\), respectively, then the correct option(s) is(are)