1. Hydrogen Balmer-Alpha (Hα) Line Calculation
Astrophysics StudentBackground
Studying emission nebulae where the visible red Hα line dominates optical spectra.
Problem
Determine the exact wavelength and photon energy of the H 3 → 2 transition accounting for proton mass.
How to use
Set Nuclear charge Z to 1, choose 'Hydrogen-1 (proton)', set Lower level n₁ to 2, and Upper level n₂ to 3.
Z = 1, Nucleus = H1, n₁ = 2, n₂ = 3Outcome
Yields a wavelength of 656.470 nm (red visible light), a photon energy of 1.889 eV, and a frequency of 4.567×10¹⁴ Hz.