Concept:
In the Bohr model, we have two primary conditions: the force provided by the field acting as centripetal force (\( \frac{mv^2}{r} = F(r) \)) and the quantization of angular momentum (\( mvr = \frac{nh}{2\pi} \)). Here, \( F(r) = \frac{K}{r} \).
Step 1: Solve the force equation for velocity \( v \).
$$ \frac{mv^2}{r} = \frac{K}{r} \implies mv^2 = K \implies v = \sqrt{\frac{K}{m}} $$
Since \( K \) and \( m \) are constants, the velocity \( v \) of the electron is constant in every orbit and is independent of the orbital radius \( r \) or the orbit number \( n \).
Step 2: Determine the Kinetic Energy (\( T_n \)).
$$ T_n = \frac{1}{2} mv^2 = \frac{1}{2} m \left( \sqrt{\frac{K}{m}} \right)^2 = \frac{K}{2} $$
Because \( T_n = K/2 \), the kinetic energy is constant and independent of the orbit number \( n \).
Step 3: Determine the orbit radius (\( r_n \)).
Apply Bohr's quantization condition \( mvr = \frac{nh}{2\pi} \):
$$ r_n = \frac{nh}{2\pi mv} $$
Since \( n \), \( h \), \( m \), and \( v \) are constants (except for \( n \)), we have \( r_n \propto n \).
$$\boxed{T_n \text{ is independent of n}, r_n \propto n}$$