
To analyze the energy level transitions and their corresponding wavelengths, we can use the relationship between energy difference (\( \Delta E \)) and wavelength (\( \lambda \)) given by the equation:
\(E = \frac{hc}{\lambda}\)
Here, \( h \) is Planck's constant and \( c \) is the speed of light. Thus, we can write:
\(\Delta E = \frac{hc}{\lambda}\)
This implies that the larger the energy difference, the shorter the wavelength of the emitted light.
From the above steps, \( \lambda_2 \) should indeed be about double \( \lambda_3 \), after correctly reconciling the transition context, which relates to shorter wavelengths preventing an equal equation reversal in initially identical transitions with levels interlying a larger sequential offset factor of specification and comparison.
Thus, the correct answer is: \(\lambda_2 > \lambda_1, \lambda_2 = 2\lambda_3\)