Concept:
The energy of an electron in the $n^{\text{th}}$ orbit of a hydrogen atom is
\[
E_n=-\frac{2.18\times10^{-18}}{n^2}\text{ J}
\]
For a Lyman series transition from $n_x$ to $n=1$, the emitted energy is
\[
\Delta E=2.18\times10^{-18}\left(1-\frac{1}{n_x^2}\right)\text{ J}
\]
Step 1: Determine the value of $n_x$
Given,
\[
1.635\times10^{-18}
=
2.18\times10^{-18}
\left(1-\frac{1}{n_x^2}\right)
\]
Dividing both sides by $2.18\times10^{-18}$,
\[
\frac{1.635}{2.18}
=
1-\frac{1}{n_x^2}
\]
\[
0.75
=
1-\frac{1}{n_x^2}
\]
\[
\frac{1}{n_x^2}
=
0.25
=
\frac{1}{4}
\]
\[
n_x=2
\]
Step 2: Calculate the excitation energy from $n=2$ to $n=3$
\[
\Delta E
=
2.18\times10^{-18}
\left(
\frac{1}{2^2}-\frac{1}{3^2}
\right)
\]
\[
=
2.18\times10^{-18}
\left(
\frac{1}{4}-\frac{1}{9}
\right)
\]
\[
=
2.18\times10^{-18}
\times\frac{5}{36}
\]
\[
\Delta E
\approx
3.03\times10^{-19}\text{ J}
\]
Therefore,
\[
\boxed{\Delta E\approx3\times10^{-19}\text{ J}}
\]