The correct option is B 6.91×1014 Hz, 434 nm
Since ni=5 and nf=2, this transition gives rise to a spectral line in the visible region of the Balmer series. From equation.
ΔE=2.18×10−18J[152−122]
=−4.58×10−19J
Negative sign implies that it is an emission energy.
The frequency of the photon (taking energy in terms of magnitude) is given by
v=ΔEh
=4.58×10−19J6.626×10−34Js
⇒6.91×1014 Hz
The wavelength of photon emitted (λ)=cv
=3.0×108 ms−16.91×1014Hz
=4.34×10−7m or 434 nm