Atomic Structure
Atomic structure underpins the Chemical and Physical Foundations section of the MCAT. You are expected to work with the light–energy relationships (E = hν, c = νλ), the photoelectric effect, the Bohr model and hydrogen emission spectrum, the four quantum numbers, orbital shapes, ground-state electron configurations (Aufbau, Pauli, Hund), and the periodic trends that follow directly from configuration — atomic radius, ionization energy, electron affinity and electronegativity.
Subatomic Particles & the Nuclear Atom
An atom has a tiny, dense, positively charged nucleus (protons + neutrons) surrounded by electrons in quantized orbitals. Rutherford's gold-foil experiment established this picture: most α-particles passed straight through thin gold foil, but a few were sharply deflected — showing the atom is mostly empty space with nearly all its mass concentrated in the nucleus.
- Proton — charge +1.602 × 10−19 C, mass 1.673 × 10−27 kg. The number of protons is the atomic number (Z) and fixes the element's identity.
- Neutron — electrically neutral, mass 1.675 × 10−27 kg. Nuclei of the same element with different neutron counts are isotopes.
- Electron — charge −1.602 × 10−19 C, mass 9.109 × 10−31 kg (about 1/1836 of a proton). Electrons occupy orbitals and are responsible for chemical behavior.
Mass number A = protons + neutrons. Isotopes share Z but differ in A; the atomic weight on the periodic table is the abundance-weighted average of an element's isotopes.
Quantized Light & the Photoelectric Effect
Planck (1900) proposed that energy is emitted or absorbed not continuously but in discrete packets called quanta. For light, each quantum is a photon.
Energy of one photon: E = hν, where h = Planck's constant = 6.626 × 10−34 J·s and ν is frequency in Hz.
Speed of light relation: c = νλ (c = 3.00 × 108 m/s), so E = hc/λ.
Energy of n photons: E = nhν. Shorter wavelength → higher frequency → higher energy per photon.
Light above a threshold frequency ejects electrons from a metal surface. KEmax = hν − Φ, where Φ is the work function (minimum energy to free an electron). Below the threshold frequency no electrons are emitted regardless of intensity; above it, brighter light ejects more electrons (not faster ones). This is a favorite MCAT graph — KEmax is linear in ν with slope h.
Quantization explained black-body radiation, the photoelectric effect, and the discrete line spectra of atoms.
Spectrum of Hydrogen
When a sample of hydrogen gas is excited by an electric discharge, it emits a series of discrete lines — not a continuous spectrum. Niels Bohr (1913) explained this by postulating that the electron occupies fixed circular orbits with quantized energy En = −13.6/n2 eV, and that emission/absorption occurs only when the electron jumps between these orbits.
Spectral series
- Lyman series — transitions ending at n = 1; in the UV region.
- Balmer series — transitions ending at n = 2; in the visible region (the lines Balmer himself observed).
- Paschen series — transitions ending at n = 3; in the infrared.
- Brackett series — ending at n = 4; far IR.
- Pfund series — ending at n = 5; far IR.
1/λ = RH (1/n12 − 1/n22), where RH = 1.097 × 107 m−1, n1 < n2. n1 is the lower (final) level for emission; n2 the upper (initial). Gives the wavelength of every line in the H spectrum.
Quantum Numbers
Four quantum numbers fully specify the state of every electron in an atom. Two electrons in the same atom can never have the same set of all four (Pauli's principle).
- Principal quantum number (n)
- Determines the main energy level / shell. Allowed values: 1, 2, 3, …. Larger n means higher energy and larger orbital. Maximum number of electrons in shell n = 2n2.
- Azimuthal / angular momentum quantum number (l)
- Determines the subshell shape. Allowed values: 0, 1, …, (n − 1). Subshell letters: l = 0 → s, l = 1 → p, l = 2 → d, l = 3 → f. Number of subshells in shell n = n.
- Magnetic quantum number (m or ml)
- Determines the orbital orientation in space. Allowed values: −l, −l+1, …, 0, …, +l. Number of orbitals in subshell l = (2l + 1).
- Spin quantum number (s or ms)
- Spin direction of electron. Allowed values: +½ or −½. Each orbital holds at most 2 electrons with opposite spin.
Counts to memorise
| Number | Symbol | Allowed values | Tells us | Capacity rule |
|---|---|---|---|---|
| Principal | n | 1, 2, 3, … | Energy level / shell size | Max electrons in shell = 2n2 |
| Azimuthal | l | 0 … (n − 1) | Subshell shape (s/p/d/f) | Number of subshells in shell = n |
| Magnetic | ml | −l … 0 … +l | Orbital orientation in space | Orbitals per subshell = (2l + 1) |
| Spin | ms | +½ or −½ | Electron spin direction | Max 2 e− per orbital (Pauli) |
| Subshell | l | Orbitals (2l + 1) | Max electrons |
|---|---|---|---|
| s | 0 | 1 | 2 |
| p | 1 | 3 | 6 |
| d | 2 | 5 | 10 |
| f | 3 | 7 | 14 |
Total in shell n = 2n2 → 2, 8, 18, 32, …
Shapes of Orbitals
An orbital is a region of space where the probability of finding an electron is high (about 90–95 percent). Each subshell has a characteristic shape determined by l.
Spherically symmetric about the nucleus. 1s has no node; 2s has one radial node; 3s has two radial nodes. All s orbitals are non-directional.
Dumb-bell shaped, with a nodal plane through the nucleus. Three orientations along x, y, z axes — px, py, pz. Maximum electron density along the axis; zero at the nucleus.
Five orbitals, mostly four-lobed (dxy, dxz, dyz, dx2−y2) with dz2 shaped like a dumb-bell with a torus around the middle. Only encountered from the third shell upward.
Electronic Configuration
The arrangement of electrons across orbitals follows three rules.
- Aufbau principle
- Electrons fill orbitals in order of increasing energy: 1s, 2s, 2p, 3s, 3p, 4s, 3d, 4p, 5s, 4d, 5p, 6s, 4f, 5d, 6p …. The (n + l) rule predicts the order — lower (n + l) fills first; for ties, the lower n fills first.
- Pauli's exclusion principle
- No two electrons in an atom can have the same set of all four quantum numbers. Consequence: an orbital holds at most two electrons with opposite spin.
- Hund's rule of maximum multiplicity
- When electrons fill degenerate (equal-energy) orbitals (p, d, f), they occupy them singly first with parallel spins before any pairing. This minimizes electron repulsion.
Configurations of the first 30 elements
- H (1): 1s1 · He (2): 1s2.
- Li (3): [He] 2s1 · Be (4): [He] 2s2.
- B (5): [He] 2s2 2p1 · C (6): 2s2 2p2 · N (7): 2s2 2p3 · O (8): 2s2 2p4 · F (9): 2s2 2p5 · Ne (10): 2s2 2p6.
- Na (11): [Ne] 3s1 · Mg (12): 3s2 · Al (13): 3s2 3p1 · Si (14): 3p2 · P (15): 3p3 · S (16): 3p4 · Cl (17): 3p5 · Ar (18): 3p6.
- K (19): [Ar] 4s1 · Ca (20): [Ar] 4s2.
- Sc (21): [Ar] 3d1 4s2 · Ti (22): 3d2 4s2 · V (23): 3d3 4s2.
- Cr (24): [Ar] 3d5 4s1 (anomaly — half-filled d gives extra stability).
- Mn (25): 3d5 4s2 · Fe (26): 3d6 4s2 · Co (27): 3d7 4s2 · Ni (28): 3d8 4s2.
- Cu (29): [Ar] 3d10 4s1 (anomaly — full d gives extra stability).
- Zn (30): [Ar] 3d10 4s2.
Configurations of ions
To form a cation, remove electrons from the highest n first — for transition metals this means the 4s electrons leave before the 3d electrons (e.g. Fe: [Ar] 3d6 4s2 → Fe2+: [Ar] 3d6; Fe3+: [Ar] 3d5). For an anion, add electrons following Aufbau. An atom or ion with unpaired electrons is paramagnetic (attracted to a magnetic field); one with all electrons paired is diamagnetic.
Periodic Trends
Nearly every periodic trend traces back to effective nuclear charge (Zeff = Z − S), the net positive pull the outer electrons actually feel after inner-electron shielding (S). Zeff rises across a period (protons added, same shell, poor shielding by same-shell electrons) and stays roughly constant down a group while electrons occupy higher shells farther from the nucleus.
| Property | Across a period (→) | Down a group (↓) | Driver |
|---|---|---|---|
| Atomic radius | Decreases | Increases | ↑Zeff pulls in; new shells push out |
| Ionization energy (IE) | Increases | Decreases | Tighter hold with ↑Zeff; weaker with distance |
| Electron affinity | More exothermic | Less exothermic | Nucleus attracts added e− more strongly |
| Electronegativity | Increases | Decreases | Same driver as IE; F is the maximum |
| Metallic character | Decreases | Increases | Opposite of IE/electronegativity |
- Ionization energy is the energy to remove an electron from a gaseous atom (X(g) → X+(g) + e−). Successive IEs always increase; a large jump appears once you break into a noble-gas core, revealing the number of valence electrons.
- Ionic size: cations are smaller than their parent atom (lost a shell / less repulsion); anions are larger. For an isoelectronic series (same electron count), radius decreases as Z increases (e.g. O2− > F− > Na+ > Mg2+).
- Small exceptions in IE occur at the s→p transition (B < Be) and at half-filled p (O < N), where subshell stability matters.
Worked MCQs
Five MCQs that capture the high-yield testing patterns for this chapter. Read the explanation even when you get the answer right — that's where the deeper concept lives.
Q1. Which property generally increases both across a period (left to right) and up a group?
Electronegativity (and ionization energy) rise with effective nuclear charge — across a period and up a group — peaking at fluorine. Atomic radius and metallic character show the opposite trend, decreasing across and up.
Q2. The maximum number of electrons that can be accommodated in a subshell with l = 2 is:
l = 2 corresponds to a d subshell, which has (2l + 1) = 5 orbitals. Each orbital holds 2 electrons (Pauli), giving 5 × 2 = 10.
Q3. The ground-state electronic configuration of chromium (Z = 24) is:
Chromium is one of the two famous Aufbau anomalies. A half-filled 3d5 set (one electron in each d orbital) is more stable than the predicted 3d4 4s2 — an electron promotes from 4s to 3d to give 3d5 4s1.
Q4. The principle that states "no two electrons in an atom can have the same set of all four quantum numbers" is:
Pauli's exclusion principle limits each orbital to two electrons with opposite spin. Hund deals with degenerate orbital filling; Aufbau with the order of filling; Heisenberg with the impossibility of measuring position and momentum simultaneously.
Q5. The energy of a photon of green light (λ = 500 nm) is approximately:
E = hc/λ = (6.63 × 10−34)(3 × 108) / (500 × 10−9) = 3.97 × 10−19 J. This is the order of magnitude of single-photon energies for visible light (a few eV).
Quick Recap
- Nucleus = protons + neutrons; Z (protons) = element identity; isotopes share Z, differ in A.
- Planck: E = hν = hc/λ; energy is quantized into photons.
- Photoelectric effect: KEmax = hν − Φ; needs a threshold frequency.
- H spectrum series — Lyman (UV, n → 1), Balmer (visible, n → 2), Paschen (IR, n → 3); Rydberg 1/λ = RH(1/n12 − 1/n22).
- Quantum numbers: n (shell), l (shape), ml (orientation), ms (spin); subshell capacities s = 2, p = 6, d = 10, f = 14; shell n = 2n2.
- Filling rules: Aufbau (lowest energy first), Pauli (max 2 e/orbital, opposite spin), Hund (parallel spins first); Cr and Cu are the anomalies.
- Ions: remove 4s before 3d for transition metals; unpaired e− = paramagnetic.
- Periodic trends from Zeff: radius ↓ across / ↑ down; IE and electronegativity ↑ across / ↓ down.