(A) The electron in the atom revolves in specific orbits without radiating energy.
(B) The electron can only occupy discrete energy levels or orbits. The energy of the electron in the n-th orbit is given by:
\[ E_n = - \frac{k e^2}{2r_n} \]
where k is Coulomb's constant, e is the electron charge, and r_n is the radius of the n-th orbit.
(C) The transition of the electron between orbits results in the emission or absorption of energy corresponding to the difference in energy levels.
For transition between n = 1 and n = 4, the emission and absorption spectra can be derived using the following formulas:
When the electron transitions from a higher to a lower energy state, the frequency of the emitted radiation is:
\[ f = \frac{E_{\text{higher}} - E_{\text{lower}}}{h} \]
The electron absorbs energy when it moves to a higher energy state.
The number of lines in the emission spectrum is given by the number of possible transitions from n=4 to n=1, including intermediate states. The transitions are as follows:
\[ 4 \to 3, \quad 4 \to 2, \quad 4 \to 1, \quad 3 \to 2, \quad 3 \to 1, \quad 2 \to 1. \]
There are a total of 6 emission lines.
Similarly, for absorption, the number of lines will be the same, as absorption also happens when the electron moves from a lower to a higher energy state. The number of lines is 6.
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