One series of lines in the hydrogen spectrum is caused by
emission of energy accompanying the fall of an electron from outer
shells to the fourth shell. The lines can be calculated using the
Balmer-Rydberg equation:
1λ=R∞[1m2−1n2]
where m=4, R∞ = 1.097×10−2nm−1, and nis an
integer greater than 4.
Part A
Calculate the wavelengths in nanometers of the first two lines in the series.
Express your answers using four significant figures separated by a comma.
Part B
Calculate the energies in kilojoules per mole of the first two lines in the series.
Express your answers using four significant figures separated by a comma.
Part A
For the first line
For the second line
Part B
For the first line
This is for one atom. For one mole of atoms
Convert the unit from J to kJ
For the second line
This is for one atom. For one mole of atoms
Convert the unit from J to kJ
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