The energy required to excite a hydrogen atom between two energy levels is given by the difference in their energies.
The energy of the nth orbit of a hydrogen atom is given by: \[ E_n = -\frac{13.6}{n^2} { eV} \] For the first excited state (\(n=2\)) and the second excited state (\(n=3\)): \[ E_2 = -\frac{13.6}{2^2} = -3.4 { eV} \] \[ E_3 = -\frac{13.6}{3^2} = -1.51 { eV} \] The energy required to excite the hydrogen atom from the first excited state to the second excited state is the difference: \[ \Delta E = E_3 - E_2 = (-1.51) - (-3.4) = 1.89 { eV} \] Thus, the energy required is 1.89 eV.
Kepler's second law (law of areas) of planetary motion leads to law of conservation of
Kepler's second law (law of areas) of planetary motion leads to law of conservation of