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Unit XIII · Structure of atom (lesson 24)
11 min readConcept sheetSection A objective (2 marks, two parts: match a series to its region) and MCQ (1 mark); Section B short answer (3 marks) numerical; also a NEET favourite

Hydrogen spectrum: spectral series, emission and absorption

An electron falling between levels emits hν = Eₙ − Eₘ. Falls ending on levels 1, 2 and 3 form the Lyman (UV), Balmer (visible) and Paschen (infrared) series.

Energy of a linehν = 13.6(1/m² − 1/n²) eV for a fall from level n to level m (n > m)
Wavelength form1/λ = R(1/m² − 1/n²), where R = 1.097 × 10⁷ m⁻¹ is the Rydberg constant
The five seriesLyman m = 1 (UV); Balmer m = 2 (visible); Paschen m = 3, Brackett m = 4, Pfund m = 5 (infrared)
Number of linesAtoms excited to level n can give up to n(n − 1)/2 different lines

Emission and absorption spectra

Heat a gas, or pass an electric discharge through it at low pressure, and it glows. Seen through a spectroscope, its light is a set of bright lines at fixed wavelengths. This is an emission line spectrum. Each element has its own set of lines, like a fingerprint. Now pass white light through the cool gas. Dark lines appear at the same wavelengths, because the gas takes in just those photons. This is an absorption spectrum.

How Bohr's model explains the lines

  1. 1
    Heat or an electric discharge gives energy to the atoms and lifts electrons to higher energy levels (excited states).
  2. 2
    An excited atom stays in that state only for a very short time.
  3. 3
    The electron falls to a lower level m and gives out one photon: hν = Eₙ − Eₘ.
  4. 4
    The levels are fixed, so only certain energy gaps exist. So only certain wavelengths appear: a line spectrum.
  5. 5
    In absorption, an electron takes in a photon only if its energy exactly matches a gap, which gives dark lines at the same wavelengths.

The spectral series of hydrogen

SeriesFalls toFalls fromRegion
Lymanm = 1n = 2, 3, 4, ...Ultraviolet
Balmerm = 2n = 3, 4, 5, ...Visible
Paschenm = 3n = 4, 5, 6, ...Near infrared
Brackettm = 4n = 5, 6, 7, ...Mid infrared
Pfundm = 5n = 6, 7, 8, ...Far infrared

Worked example: a blue-green line of hydrogen

Problem

In a hydrogen atom the electron falls from n = 4 to n = 2. Find the wavelength of the light given out. Is it visible, and which series is it in? (R = 1.097 × 10⁷ m⁻¹)

Working
  1. Formula: 1/λ = R(1/m² − 1/n²), with m = 2 and n = 4.
  2. 1/2² − 1/4² = 1/4 − 1/16 = 3/16.
  3. 1/λ = 1.097 × 10⁷ × 3/16 = 2.057 × 10⁶ m⁻¹.
  4. λ = 1 ÷ 2.057 × 10⁶ = 4.86 × 10⁻⁷ m = 486 nm.
  5. 486 nm lies between 400 nm and 700 nm, so it is visible (blue-green). It ends on m = 2, so it is in the Balmer series.
Answer

λ ≈ 486 nm (4860 Å): visible blue-green light in the Balmer series

Worked example: limits of the Balmer series

Problem

Find the longest and shortest wavelengths of the Balmer series of hydrogen. (R = 1.097 × 10⁷ m⁻¹)

Working
  1. Longest wavelength comes from the smallest gap: n = 3 to m = 2.
  2. 1/λ = R(1/4 − 1/9) = 5R/36, so λ = 36 ÷ (5 × 1.097 × 10⁷) = 6.56 × 10⁻⁷ m = 656 nm.
  3. Shortest wavelength comes from the largest gap: n = ∞ to m = 2.
  4. 1/λ = R(1/4 − 0) = R/4, so λ = 4 ÷ (1.097 × 10⁷) = 3.65 × 10⁻⁷ m = 365 nm.
Answer

Longest ≈ 656 nm (red); shortest ≈ 365 nm (just into the ultraviolet)

How to draw the transitions diagram

  • Draw the levels n = 1 to 5 and ∞ as horizontal lines that crowd together near the top.
  • Draw downward arrows ending on n = 1 and label the group Lyman series (ultraviolet).
  • Draw arrows ending on n = 2 and label them Balmer series (visible); mark the 3 to 2 arrow red line, 656 nm.
  • Draw arrows ending on n = 3, 4 and 5 and label them Paschen, Brackett and Pfund (infrared).
  • In each group, the longest arrow gives the shortest wavelength.
In real life

The dark Fraunhofer lines in sunlight are an absorption spectrum: cooler gases in the Sun's outer layer absorb certain wavelengths. Matching them with lines seen on Earth showed hydrogen, sodium, iron and calcium in the Sun.

Exam angle

3 marks: “An electron in a hydrogen atom falls from n = 5 to n = 2. Find the wavelength of the light emitted and name its series. (R = 1.097 × 10⁷ m⁻¹)” 1/λ = R(1/4 − 1/25) = 0.21R = 2.30 × 10⁶ m⁻¹. λ ≈ 4.34 × 10⁻⁷ m = 434 nm, violet light, in the Balmer series.

2 marks: “Distinguish between an emission spectrum and an absorption spectrum.” Emission: bright lines on a dark background, given out by an excited gas. Absorption: dark lines in a continuous spectrum when white light passes through a cool gas. For one element, both have the same wavelengths.

1 marks: “How many spectral lines can hydrogen atoms excited to n = 4 emit?” n(n − 1)/2 = 4 × 3 ÷ 2 = 6.

Remember it

Lazy Boys Prefer Bed Pillows: Lyman, Balmer, Paschen, Brackett and Pfund end on levels 1, 2, 3, 4 and 5.