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1.3Structure 1 — Models of the particulate nature of matter

Electronic Configurations — IB Chemistry SL Revision Notes & Topical Questions

15 min read 23 parts Lesson 6 of 6 1 quiz

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1.3 Electronic Configurations — IB SL Notes — IB CHEMISTRY SL notes: Relate frequency, wavelength and energy, use the hydrogen spectrum as evidence for energy levels, and write electron configurations up to Z = 36.Speed — all electromagnetic waves travel at c = 3.00 × 108 m s−1 i…

  • Photon energy
  • Relationship
  • Order of increasing energy
  • Visible range
  • Excitation
  • Line spectrum

Part 1 of 9Electromagnetic radiation

Electromagnetic radiation
Speed
  • Speed all electromagnetic waves travel at c = 3.00 × 108 m s−1 in a vacuum, with c = λν.
Photon energy
  • E = hν, with h = 6.63 × 10−34 J s.
Relationship
  • Relationship frequency and wavelength are inversely proportional, and photon energy increases with frequency.
Order of increasing energy
  • Order of increasing energy radio < microwave < IR < visible < UV < X-ray < gamma.
Visible range
  • Visible range from about 400 nm to 700 nm (red, lower energy).
    • (violet, higher energy)

Part 2 of 9Emission spectra

Excitation
  • Excitation heat or an electric discharge promotes electrons to higher levels.
Emission
  • Emission when electrons fall back they emit photons with energy equal to the level difference, ΔE = hν.
Line spectrum
  • Line spectrum only certain frequencies are emitted because levels have fixed energies, and the pattern is unique to each element.
Absorption comparison
  • Absorption comparison an absorption spectrum has dark lines on a continuous background at the same frequencies as the element's emission lines.

Part 3 of 9Hydrogen spectrum as evidence for energy levels

SeriesElectron falls toRegion
Lymann = 1Ultraviolet
Balmern = 2Visible
Paschenn = 3Infrared
Convergence
  • Convergence energy levels get closer together as n increases, so lines converge at high frequency.
Convergence limit
  • Convergence limit corresponds to an electron escaping the atom (n = ∞).
Conclusion
  • Conclusion the discrete lines show that electrons occupy fixed energy levels.

Part 4 of 9Energy levels, sublevels and orbitals

SublevelOrbitalsMax electronsShape
s12Spherical
p36Dumbbell (px, py, pz)
d510Mostly four-lobed
f714Complex
Level n
  • Level n contains n sublevels and holds up to 2n2 electrons (2, 8, 18, 32).
Sublevels by level
  • Sublevels by level n = 1: 1s; n = 2: 2s, 2p; n = 3: 3s, 3p, 3d; n = 4: 4s, 4p, 4d, 4f.
Orbital capacity
  • Orbital capacity each orbital holds two electrons of opposite spin.
Shapes
  • Shapes s orbitals are spherical and p orbitals are dumbbell-shaped along the x, y and z axes at 90°, and both grow larger as n increases.
Degenerate orbitals
  • Degenerate orbitals orbitals in the same sublevel, such as 2px, 2py and 2pz, have equal energy.

Part 5 of 9Filling rules

Filling rules
Aufbau principle
  • Aufbau principle electrons fill the lowest energy orbitals first, in the order 1s 2s 2p 3s 3p 4s 3d 4p 5s 4d 5p.
Pauli exclusion principle
  • Pauli exclusion principle an orbital holds a maximum of two electrons with opposite spins.
Hund's rule
  • Hund's rule electrons occupy degenerate orbitals singly with parallel spins before pairing.
4s before 3d
  • 4s is lower in energy before 3d is occupied, so it fills first.
Orbital diagrams
  • Orbital diagrams show each orbital as a box and each electron as an arrow;
    • nitrogen has 2p with three unpaired electrons.

Part 6 of 9Writing configurations

1
Find the total number of electrons from the atomic number, adjusted for any charge.
2
Fill the sublevels in Aufbau order with maximum occupancy s 2, p 6, d 10, f 14.
3
Check that the superscripts add up to the electron total.
4
Write the condensed form using the previous noble gas core.
Iron (Z
26) — 1s22s22p63s23p64s23d6, condensed [Ar]4s23d6.
After the d-block
  • Ga is [Ar]3d104s24p1 and Br is [Ar]3d104s24p5.

Part 7 of 9Exceptions and ions

Exceptions and ions
Chromium
  • [Ar]3d54s1 because a half-filled d sublevel is extra stable.
Copper
  • [Ar]3d104s1 because a full d sublevel is extra stable.
Transition metal cations
  • 4s electrons are removed before 3d, so Fe3+ is [Ar]3d5.
Main-group ions
  • Main-group ions lose or gain outer electrons, so Ca2+ is [Ar].

Part 8 of 9Blocks of the periodic table

  • Rule
    • elements are grouped by the sublevel that receives the last, highest-energy electron.
BlockGroups
s-block1–2 (plus He)
p-block13–18
d-block3–12
f-blockLanthanoids and actinoids

Part 9 of 9More from the specification

More from the specification
Quantum shell
  • Quantum shell electrons are arranged in main energy levels numbered n = 1, 2, 3 and so on.
Subshell
  • Subshell each shell is divided into s, p, d and f subshells with 1, 3, 5 and 7 orbitals.
Shorthand configuration
  • Shorthand configuration noble gas core notation such as [Ne] 3s2 3p4 shows the outer electrons concisely.
Light and spectra
  • Light and spectra electrons absorbing or releasing specific amounts of light energy move between shells, giving line spectra.
Quantum shell
  • Quantum shell electrons are arranged in main energy levels numbered n = 1, 2, 3 and so on.
Subshell
  • Subshell each shell is divided into s, p, d and f subshells with 1, 3, 5 and 7 orbitals.
Shorthand configuration
  • Shorthand configuration noble gas core notation such as [Ne] 3s2 3p4 shows the outer electrons concisely.
Light and spectra
  • Light and spectra electrons absorbing or releasing specific amounts of light energy move between shells, giving line spectra.
Valence electrons
  • Electrons in the outer shell.
Quantum
  • A packet of energy.
Subshell
  • A set of orbitals of the same type within a shell: s, p, d or f.
Shell
  • An energy level around the nucleus that holds a limited number of electrons.
Nucleus
  • Central part of an atom with protons and neutrons.

Key terms

TermMeaning
Electromagnetic spectrumThe full range of radiation ordered by wavelength or frequency, from radio waves to gamma rays.
Line spectrumA series of discrete lines produced when excited electrons fall to lower energy levels.
Energy levelA main shell of fixed energy labelled by principal quantum number n.
SublevelA subdivision of a main level (s, p, d or f) containing orbitals of equal energy.
Atomic orbitalA region around the nucleus with a high probability of finding an electron, holding at most two.
Aufbau principleElectrons fill orbitals in order of increasing energy.
Hund's ruleDegenerate orbitals fill singly with parallel spins before pairing.

Avoid these mistakes

1
Writing 4s before 3d for the electrons removed in ions — 4s electrons are lost first.
2
Placing paired electrons in a p sublevel before every orbital has one — Hund's rule requires singly occupied orbitals first.
3
Giving Cr as [Ar]3d44s2 — it is [Ar]3d54s1.
4
Using lines evenly spaced for the hydrogen spectrum — they converge at high frequency.

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