Concept:
For a hydrogen-like atom,
\[
E_n=-\frac{13.6Z^2}{n^2}\,\text{eV}
\]
For Balmer series, the electron finally reaches \(n=2\).
The largest wavelength corresponds to the smallest energy transition.
Therefore,
\[
n_i=3 \rightarrow n_f=2
\]
Step 1: Determine the transition energy formula.
Photon energy emitted:
\[
E=13.6Z^2
\left(
\frac{1}{2^2}-\frac{1}{3^2}
\right)
\]
\[
E=13.6Z^2
\left(
\frac{5}{36}
\right)
\]
\[
E=\frac{68}{36}Z^2
\]
\[
E=1.8889\,Z^2
\]
Step 2: Calculate \(E_0\) for \(Z=24\).
\[
E_0=1.8889(24)^2
\]
\[
E_0=1.8889(576)
\]
\[
E_0\approx1088\,\text{eV}
\]
Step 3: Calculate \(E_1\) for \(Z=25\).
\[
E_1=1.8889(25)^2
\]
\[
E_1=1.8889(625)
\]
\[
E_1\approx1180.6\,\text{eV}
\]
Step 4: Compute the difference.
\[
|E_1-E_0|
=
1.8889(625-576)
\]
\[
=
1.8889(49)
\]
\[
\approx92.6\,\text{eV}
\]
Thus,
\[
|E_1-E_0|\approx 93\,\text{eV}
\]
Correct option:
\[
\boxed{90}
\]