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Atomic Structure - Electrons in atoms (HL only)

Grade 12IBChemistry

Review the key concepts, formulae, and examples before starting your quiz.

🔑Concepts

The energy of a photon is related to its frequency by the equation E=huE = h u, and to its wavelength by E=hcλE = \frac{hc}{\lambda}.

Line spectra provide evidence for discrete energy levels. In the hydrogen spectrum, the Lyman series (ultraviolet) corresponds to transitions to the n=1n=1 level, the Balmer series (visible) to n=2n=2, and the Paschen series (infrared) to n=3n=3.

The convergence limit of the lines in the Lyman series (nn \to \infty to n=1n=1) represents the point where the electron is completely removed from the atom, which allows for the calculation of the first ionization energy (IE1IE_1).

Successive ionization energies (IE1,IE2,IE_1, IE_2, \dots) provide evidence for the shell and sub-shell structures of atoms. Large jumps in IEIE indicate moving to a shell closer to the nucleus.

Orbitals are regions of space where there is a high probability of finding an electron. The sub-levels s,p,d,fs, p, d, f contain 1,3,5,71, 3, 5, 7 orbitals respectively, with each orbital holding a maximum of two electrons of opposite spin (Pauli Exclusion Principle).

Hund's Rule states that orbitals of the same energy (degenerate) are filled singly before being occupied in pairs to minimize electron-electron repulsion.

The electronic configurations of transition metals show exceptions: Chromium is [Ar]3d54s1[Ar] 3d^5 4s^1 and Copper is [Ar]3d104s1[Ar] 3d^{10} 4s^1 due to the extra stability of half-filled and fully-filled dd-subshells.

First Ionization Energy trends across a period show general increases but feature specific drops: between Group 2 and 13 (transition from ss to pp subshell) and between Group 15 and 16 (electron-electron repulsion in a pp-orbital).

📐Formulae

E=hνE = h\nu

c=νλc = \nu\lambda

E=hcλE = \frac{hc}{\lambda}

IE=LEphoton (where L is Avogadro’s constant)IE = L \cdot E_{photon} \text{ (where } L \text{ is Avogadro's constant)}

ΔE=EfinalEinitial\Delta E = E_{final} - E_{initial}

💡Examples

Problem 1:

The convergence limit of the Lyman series for hydrogen is observed at a wavelength of 91.16 nm91.16 \text{ nm}. Calculate the first ionization energy (IE1IE_1) of hydrogen in kJmol1kJ \cdot mol^{-1}. (Use h=6.63×1034 J sh = 6.63 \times 10^{-34} \text{ J s}, c=3.00×108 m s1c = 3.00 \times 10^8 \text{ m s}^{-1}, L=6.02×1023 mol1L = 6.02 \times 10^{23} \text{ mol}^{-1})

Solution:

Ephoton=hcλ=6.63×1034 J s×3.00×108 m s191.16×109 m=2.182×1018 JE_{photon} = \frac{hc}{\lambda} = \frac{6.63 \times 10^{-34} \text{ J s} \times 3.00 \times 10^8 \text{ m s}^{-1}}{91.16 \times 10^{-9} \text{ m}} = 2.182 \times 10^{-18} \text{ J} IE1=Ephoton×L=2.182×1018 J×6.02×1023 mol1=1.313×106 J mol1=1313 kJ mol1IE_1 = E_{photon} \times L = 2.182 \times 10^{-18} \text{ J} \times 6.02 \times 10^{23} \text{ mol}^{-1} = 1.313 \times 10^6 \text{ J mol}^{-1} = 1313 \text{ kJ mol}^{-1}

Explanation:

First, the energy of a single photon at the convergence limit is calculated using the wavelength. This energy corresponds to the energy required to remove one electron from one atom. Multiplying by Avogadro's constant (LL) gives the ionization energy per mole.

Problem 2:

Explain why the first ionization energy of Sulfur (SS) is lower than that of Phosphorus (PP).

Solution:

P:[Ne]3s23px13py13pz1P: [Ne] 3s^2 3p_x^1 3p_y^1 3p_z^1 S:[Ne]3s23px23py13pz1S: [Ne] 3s^2 3p_x^2 3p_y^1 3p_z^1

Explanation:

Phosphorus has a half-filled 3p3p subshell with three singly occupied orbitals. Sulfur has four electrons in the 3p3p subshell, meaning one 3p3p orbital contains a pair of electrons. The repulsion between these two electrons in the same orbital makes it easier to remove one of them, resulting in a lower IE1IE_1 for SS despite its higher nuclear charge.

Problem 3:

Write the full electron configuration for the Fe2+Fe^{2+} ion.

Solution:

Fe:[Ar]3d64s2    Fe2+:[Ar]3d6Fe: [Ar] 3d^6 4s^2 \implies Fe^{2+}: [Ar] 3d^6

Explanation:

When transition metals form ions, electrons are always removed from the 4s4s subshell before the 3d3d subshell. Therefore, FeFe (Z=26Z=26) loses its two 4s4s electrons first.

Electrons in atoms (HL only) - Revision Notes & Key Formulas | IB Grade 12 Chemistry