By the end of this chapter you'll be able to…

  • 1Apply the Bohr relations to any hydrogen-like species and count the spectral lines from a given level
  • 2Count radial and angular nodes separately and check them against the total of
  • 3Identify the shapes of , and orbitals, their nodal planes, and the split into axis-directed and between-axis families
  • 4Compute effective nuclear charge using Slater's rules, including the harsher screening rule for electrons
  • 5Explain why fills before but empties first, and write ground-state configurations of transition-metal ions
  • 6Use exchange energy to justify the chromium and copper exceptions, and relate unpaired electrons to the spin-only magnetic moment
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Why this chapter matters in JEE Advanced
Every later chapter in inorganic chemistry rests on this one, and the parts it rests on are exactly the parts Main skips. Periodicity is effective nuclear charge. Coordination chemistry is the split between the two families of d orbitals. Magnetism is the unpaired-electron count. The aufbau exceptions at chromium and copper are exchange energy, not arbitrary facts to memorise. Advanced also examines the quantum picture quantitatively rather than descriptively, asking for radial and angular node counts, for the effective charge felt by a named electron, and for a configuration inferred backwards from a measured magnetic moment. The chapter is short and the ideas are few, but each of them reappears three or four times later in the syllabus, so time invested here is repaid with interest.

Before you start — revise these

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Photon energy from wavelength, and the electronvolt
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The Bohr model and the hydrogen emission series
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Electronic configuration notation and the periodic table layout
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Basic probability language: distribution, density and most probable value

Atomic Structure

The orbital fills before . So when an iron atom loses two electrons, which orbital do they come from?

Not . Both come from , and is , not .

The resolution is that "which is lower" depends on how many electrons are already there. In a bare potassium or calcium atom, lies below , so it fills first. But once begins to be occupied, the added nuclear charge pulls down sharply — it is more compact and feels the nucleus more directly — and by the time you reach scandium, is already below .

atomic number energy 4s 3d near Sc 4s lower: fills first 3d lower: 4s empties first

So the filling order and the ionisation order are governed by two different orderings of the same pair of orbitals, at two different points on the curve. Nothing is inconsistent; the energies simply moved.

This chapter is about that kind of detail. Main asks for the four quantum numbers and the order of filling. Advanced asks how many nodes an orbital has and of what kind, what the effective nuclear charge is, why chromium breaks the pattern, and what an unpaired-electron count implies for the magnetic moment.

1. Hydrogen-like species, and where Bohr stops

For any one-electron species, the Bohr results are exact:

so , and are all fair game. Transitions follow

and an atom excited to level can emit distinct lines.

Bohr fails the moment a second electron appears, because electron-electron repulsion has no place in the model. It also cannot explain the fine structure of lines, the Zeeman effect, or why orbitals have shapes at all. Its survival in the syllabus is entirely due to the one-electron case being exactly right.

Illustration 1

Find the ionisation energy of and the wavelength of the transition .

eV

eV

nm

The scaling is severe. Lithium's doubly charged ion binds its last electron nine times more strongly than hydrogen does, which is why removing it needs vacuum-ultraviolet photons.

2. Orbitals, nodes and radial distribution

An orbital is a wave function ; what has physical meaning is , the probability density. Where passes through zero there is a node, and nodes come in two kinds:

r 4 pi r sq psi sq 1s: 0 nodes 2s: 1 node 3s: 2 nodes radial nodes = n minus l minus 1; the outermost peak moves further out as n rises

A orbital therefore has radial node and nodal plane, two in all. A orbital has no radial node and two nodal planes.

The radial distribution function is what answers "where is the electron most likely to be found". For its maximum sits at exactly the Bohr radius — the one place the quantum picture and Bohr's agree.

Illustration 2

Find the number of radial nodes, angular nodes and total nodes for and .

: , . Radial ; angular ; total .

: , . Radial ; angular ; total .

The total is always , whatever the subshell, which gives a one-second check on the two separate counts.

Illustration 3

Which has more radial nodes, or ? Which has more nodal planes?

: radial ; nodal planes .

: radial ; nodal planes .

So the answers point in opposite directions. Higher trades radial nodes for angular ones, which is why orbitals are the most "layered" and orbitals the most "lobed".

3. The shapes of the orbitals

Shape is fixed by alone, and the shapes matter because bonding depends on how orbitals overlap in space.

orbitals are spherical, with no directional preference at all. Higher orbitals are spheres within spheres, separated by the radial nodes counted above.

orbitals are dumbbells aligned with the three axes. Each has exactly one nodal plane, passing through the nucleus perpendicular to its own axis — so has the plane as its node, and the electron density there is exactly zero.

orbitals split into two families, and the distinction is the single most useful fact in the whole chapter:

lobes BETWEEN the axes d_xy, d_yz, d_zx lobes ALONG the axes d x squared minus y squared d z squared, with its ring this split into three plus two is exactly what a ligand field later exploits every d orbital has two angular nodes; for d z squared they are cones, not planes

Three of them — , and — have their lobes lying between the axes. The other two, and , have lobes along the axes. In a free atom all five are degenerate, but surround the atom with ligands sitting on the axes and the two families are no longer equivalent — which is the whole origin of crystal field splitting.

The wave function also carries a sign, alternating from lobe to lobe. Two orbitals overlap constructively only where their signs match, which is why bonding and antibonding combinations exist at all.

Illustration 4

Identify the nodal planes of the orbital and state where its electron density is greatest.

Its lobes lie in the plane, between the and axes.

Its two nodal planes are the and planes, since density vanishes wherever or .

Maximum density lies along the lines within the plane.

Read the subscript literally. The function is proportional to the product , so it must vanish whenever either coordinate does — which locates both nodal planes without any further work.

Illustration 5

Which orbitals point directly at ligands placed on the six coordinate axes, and what follows?

and point straight at them; , and point between them.

Electrons in the first pair are therefore repelled more strongly and rise in energy.

This produces the octahedral splitting into a lower set of three and an upper set of two, which is the foundation of everything in coordination chemistry — colour, magnetism and geometry alike.

4. Quantum numbers, and what each one controls

NumberSymbolValuesControls
Principalsize and energy
Azimuthal to shape, orbital angular momentum
Magnetic to orientation in a field
Spinintrinsic spin

Orbital angular momentum is — note that this is zero for every orbital, which Bohr's model could never accommodate, since it gave and never zero.

Capacities follow immediately: electrons per subshell and per shell.

Illustration 6

How many electrons in an atom can have and ? How many can have and ?

, is the subshell: electrons.

with requires , so or : one orbital from each, two orbitals in all, holding electrons.

The second form is the harder one, because it cuts across subshells. Enumerate which values can produce the given , count one orbital for each, and double.

5. Effective nuclear charge and Slater's rules

An outer electron does not feel the full nuclear charge; inner electrons screen it:

Slater's rules give numerically. Group the configuration as and for an electron in an or group:

Contributing electronsContribution to
Others in the same group each
Each electron in the shell
Each electron in shells below that

For a or electron the rule is harsher: within the group and a full for everything inside, because orbitals penetrate poorly.

Illustration 7

Calculate the effective nuclear charge felt by a electron in silicon ().

Configuration grouped:

Only three of the fourteen protons are effectively felt. This is why the outer electrons of a large atom behave so much more like those of a light one than the raw nuclear charge would suggest.

Illustration 8

Compare the effective nuclear charge on a and a electron in scandium ().

For : , giving .

For : everything inside counts fully, , giving .

Two electrons in the same atom feel measurably different charges. Screening, not the bare nuclear charge, is what determines chemical behaviour.

6. Aufbau, and the two orderings

Filling follows the rule: lower fills first, and where two are equal, the lower wins. That is why () precedes ().

But as the hook showed, once is occupied it drops below . Two consequences follow, and both are examined:

Electrons are removed from the highest first, so transition metals always lose before . is ; is ; is .

No transition-metal cation ever retains an electron in its ground state, which makes writing ionic configurations mechanical once the rule is remembered.

Illustration 9

Write the ground-state configurations of , and , and count the unpaired electrons in each.

: — the has unpaired.

: — still unpaired.

: unpaired, a half-filled set.

The three-plus ion is the more stable of the two, which is why iron(III) salts are so common. A half-filled subshell carries extra exchange stabilisation, as the next section explains.

7. Exceptions, exchange energy and magnetic moment

Chromium is and copper is , not the and that naive filling predicts. Two effects combine.

Exchange energy. Electrons of parallel spin in degenerate orbitals can exchange places, and every such pair lowers the energy. The number of exchange pairs for parallel electrons is , so going from to raises the count from to — a gain of four pairs, more than enough to pay for promoting an electron.

d4: 6 exchange pairs d5: 10 exchange pairs pairs = n(n minus 1) over 2, so 4 gives 6 and 5 gives 10 the gain of four pairs pays for promoting one 4s electron only PARALLEL electrons in DEGENERATE orbitals can exchange

Symmetrical distribution. Half-filled and fully filled subshells are spherically symmetric, which lowers the repulsion energy.

The number of unpaired electrons is measurable, through the spin-only magnetic moment:

Illustration 10

Calculate the spin-only magnetic moments of , and .

is , : BM

is , : BM

is , : , diamagnetic

A measured moment identifies the ion. Going backwards from to and then to the configuration is a standard Advanced question, and BM is the unmistakable signature of a high-spin ion.

Illustration 11

An ion has a magnetic moment of BM. Find the number of unpaired electrons and suggest a ion.

Three unpaired electrons in a set means or : or .

The moment alone cannot distinguish them. Colour, coordination geometry or oxidation-state chemistry is needed to settle which, which is exactly why the question usually supplies one more clue.

8. Uncertainty, matter waves and the end of the orbit

The two together destroy the idea of an orbit. If an electron's position within an atom is known to about m, its momentum is uncertain by enough to give a velocity uncertainty of order m s — comparable with the speed itself. A trajectory is therefore not merely unknown but meaningless.

Orbit and orbital are different objects: an orbit is a definite path, an orbital is a region in which the probability of finding the electron is high.

Illustration 12

An electron is confined to a region of Å. Estimate the minimum uncertainty in its velocity.

m s

Compare the Bohr velocity of m s. The uncertainty is a quarter of the speed itself, which is precisely why the electron cannot be said to follow a path.

Illustration 13

Repeat the estimate for a cricket ball of g localised to mm.

m s

Utterly unmeasurable. The principle applies to the ball exactly as it does to the electron; it simply produces no observable consequence, which is why classical mechanics survives everywhere except inside atoms.

Summary

  • fills before but lies lower once occupied, so empties first: is .
  • Hydrogen-like: eV, Å; level emits lines.
  • Bohr fails the instant a second electron appears, since it contains no electron-electron repulsion.
  • Radial nodes ; nodal planes ; total always.
  • peaks at for — the one point where Bohr and quantum mechanics agree.
  • , , have lobes between the axes; and lie along them — the origin of crystal field splitting.
  • Orbital angular momentum is , and is zero for every orbital.
  • Capacities: per subshell, per shell.
  • by Slater: same group, for , deeper — but for everything inside a or electron.
  • Filling by the rule; ionisation always removes the highest first, so cations of transition metals keep no electrons.
  • Exchange pairs for parallel electrons; gains four pairs, which is why chromium is .
  • Half-filled and fully filled subshells are also spherically symmetric, lowering repulsion.
  • BM: BM is the signature of five unpaired electrons.
  • makes a velocity uncertainty comparable to the speed itself for a confined electron — an orbital is not an orbit.

Key formulas & results

Everything to memorise for the exam hall, in one card. Screenshot this for revision.

Hydrogen-like species
Exact for one electron only. Bohr fails the instant a second electron appears, because it contains no electron-electron repulsion term at all.
Spectral transitions and line count
The $Z^{2}$ scaling is severe: $\text{Li}^{2+}$ binds its electron nine times more strongly than hydrogen, so its lines lie far into the ultraviolet.
Node counting
The total is $n-1$ **whatever the subshell**, which is a one-second check on the two separate counts. Higher $l$ trades radial nodes for angular ones.
Radial distribution function
Answers where the electron is most likely to be found. For $1s$ it peaks at exactly $a_0$ — the single point where the Bohr and quantum pictures agree.
Orbital angular momentum
**Zero for every $s$ orbital**, which Bohr's model could not accommodate since it gave $nh/2\pi$ and never allowed zero.
Shapes and nodal planes
$p_x$ has the $yz$ plane as its node. $d_{xy}$ vanishes wherever $x=0$ or $y=0$, giving the $xz$ and $yz$ planes — read the subscript literally.
The two families of d orbitals
Degenerate in a free atom, but ligands placed on the axes repel the second family more — which is the entire origin of crystal field splitting.
Capacities
For questions specifying $n$ and $m_l$ rather than $n$ and $l$, enumerate which $l$ values can produce that $m_l$, take one orbital from each, and double.
Slater's rules for s and p electrons
Group the configuration as $\left(1s\right)\left(2s2p\right)\left(3s3p\right)\left(3d\right)\left(4s4p\right)$ before counting. Only three of silicon's fourteen protons are effectively felt.
Slater's rule for d and f electrons
Harsher because $d$ orbitals penetrate the core poorly. In scandium a $3d$ electron feels $3.00$ while a $4s$ electron feels $3.35$.
Filling and ionisation orders
$4s$ fills before $3d$ but empties first, so $\text{Fe}^{2+}$ is $3d^{6}$. **No transition-metal cation retains an $s$ electron** in its ground state.
Exchange energy
Going $d^{4}\to d^{5}$ raises the count from $6$ to $10$, and that gain of four pairs pays for promoting a $4s$ electron — which is why chromium is $3d^{5}4s^{1}$.
Spin-only magnetic moment and uncertainty
$5.92$ BM is the unmistakable signature of five unpaired electrons. An electron confined to an angstrom has a velocity uncertainty a quarter of its own speed.
⚠️

Traps JEE Advanced sets — and how to dodge them

These are the exact option-traps and misreads that cost marks under negative marking.

WATCH OUT
Removing electrons before when writing a transition-metal cation
Ionisation always takes the highest principal quantum number first. is , never .
Why it happens: The filling order puts first, so it feels like the last-filled orbital should be the last emptied — but the two orderings are taken at different points on the energy curve.
WATCH OUT
Treating the total node count as the radial node count
Radial nodes are and angular nodes are . Only their sum is .
Why it happens: For orbitals the two happen to coincide, and orbitals are the case always shown first.
WATCH OUT
Assuming is somehow anomalous and should be excluded from the axis-directed set
It has lobes along and a ring in the plane, and it points at axial ligands. It belongs with in the higher-energy pair.
Why it happens: Its shape looks unlike the other four, so it is easy to treat as a special case rather than as a member of a family.
WATCH OUT
Using the screening factor for a electron's inner shells
For and electrons everything inside contributes a full . The term applies only to and electrons.
Why it happens: The two versions of Slater's rules look almost identical, and the reason for the difference — poor penetration by orbitals — is rarely stated.
WATCH OUT
Treating chromium and copper as arbitrary exceptions to memorise
Count exchange pairs. The gain from to is four pairs, and from to the fully filled set gains both symmetry and pairing relief.
Why it happens: They are usually presented as a list of two elements to remember, with the energetics left out entirely.
WATCH OUT
Using to identify a unique ion
The moment gives only the number of unpaired electrons. Three unpaired could be or , so a second clue is always needed.
Why it happens: The formula produces one number, which suggests a unique answer, whereas the same count arises from more than one configuration.

Exam-pattern practice

PYQ-style questions with full solutions. Work through them as a readiness check — mark yourself honestly and get your gap report at the end.

Readiness check

Are you exam-ready for Atomic Structure?

12 problems from this chapter. Try each one, reveal the worked solution, mark yourself honestly — get your gap report at the end.

12 questions~8 min worth ~8 marks in JEE Advanced exams

5-minute revision

The whole chapter, distilled. Read this the night before the exam.

  • fills first, is lower once occupied, so empties first: .
  • eV, Å; level emits lines.
  • Radial nodes , angular nodes , total always.
  • peaks at for ; orbital angular momentum is zero for .
  • has the nodal plane; vanishes where or — read the subscript literally.
  • lie between axes; lie along them, and are raised by axial ligands.
  • per subshell, per shell.
  • Slater (, ): same group, for , deeper. For and : for everything inside.
  • Fill by increasing ; ionise from the highest first. No transition-metal cation keeps an electron.
  • Exchange pairs ; gains four, explaining .
  • BM; BM means five unpaired, but the count alone never fixes a unique ion.
  • : a confined electron's velocity uncertainty rivals its speed, so an orbital is not an orbit.

JEE Advanced question blueprint

How this topic is asked, tier by tier — so you can prep to the pattern.

Typical weightage: ~2 questions (roughly 6-8 marks) across the two papers combined, of the ~120 marks of Chemistry

Question styleMarks eachTypical countWhat it tests
Hydrogen-like species and spectra31Bohr energies, radii and speeds for one-electron ions, spectral series, line counting and de Broglie consistency
Orbitals, nodes and quantum numbers41Radial and angular node counting, orbital shapes and nodal planes, the two d-orbital families, and quantum number combinations
Effective nuclear charge and electronic configuration31Slater's rules for s, p and d electrons, aufbau ordering, and configurations of neutral atoms and their cations
Exchange energy, magnetism and uncertainty41Exchange-pair counting and the aufbau exceptions, spin-only magnetic moments in both directions, and the uncertainty principle

Exam-hall strategy

Battle-tested tips from mentors and toppers for this topic under the sectional clock.

  1. For any question about a transition-metal ion, write the neutral atom first and then remove electrons from the highest principal shell. That one rule prevents the commonest error in the chapter.
  2. Count nodes with the two separate rules and immediately check that they sum to one less than the principal quantum number. Errors show up instantly.
  3. For Slater's rules, write out the grouped configuration before counting anything, and note whether the electron of interest is in an s, p, d or f group — the rule changes.
  4. If a magnetic moment is given, invert the formula to get the unpaired-electron count first, then list every configuration consistent with it before choosing.
  5. When a question names an orbital by its subscript, read the subscript as an algebraic expression. It tells you directly where the function vanishes and therefore where the nodal planes are.

Beyond the exam

Where this skill shows up in the job you're competing for — and in life.

Magnetic susceptibility measurement is a routine laborato…

Magnetic susceptibility measurement is a routine laboratory method for determining the oxidation state and spin state of a transition-metal complex, working backwards from the moment to the unpaired-electron count.

Electron microscopy depends on the de Broglie relation

Electron microscopy depends on the de Broglie relation, since accelerating electrons through a modest voltage produces wavelengths far shorter than visible light.

X-ray photoelectron spectroscopy measures effective nucle…

X-ray photoelectron spectroscopy measures effective nuclear charge directly through core-electron binding energies, which shift measurably with the chemical environment of an atom.

Where else this topic is tested

Prepare once, score in every exam that asks it.

JEE Advanced
JEE Main
BITSAT
NEET UG
State engineering entrance tests

Questions aspirants ask

Pulled from the Q&A community and mentor sessions.

Because the relative energies change as the subshell is populated. In potassium and calcium, where no d electrons are present, the 4s orbital genuinely lies lower and fills first. Once electrons begin entering the 3d set, the increased nuclear charge pulls those compact orbitals down sharply, and from scandium onward 3d lies below 4s. Ionisation happens from the highest principal quantum number, which is now 4s. So the filling order and the ionisation order are both correct, taken at different points on the energy curve, and no contradiction exists.

A radial node is a spherical surface at a fixed distance from the nucleus where the wave function passes through zero. An angular node is a plane or cone through the nucleus where it does the same. Their numbers are given by different rules — radial nodes number one less than the principal quantum number minus the azimuthal quantum number, while angular nodes simply equal the azimuthal quantum number. Their sum is always one less than the principal quantum number, which is a useful check. Higher azimuthal values trade radial nodes for angular ones.

Because d orbitals penetrate the inner shells poorly. An s electron has appreciable probability density right at the nucleus, so it spends part of its time inside the shielding electrons and experiences more of the nuclear charge than a simple count would suggest. A d orbital has zero density at the nucleus and its density is pushed outward, so the inner electrons screen it almost completely. Slater's rules encode this by giving inner electrons a full unit of screening against a d electron rather than the reduced value used for s and p.

Two effects combine. The first is exchange energy: electrons with parallel spins in degenerate orbitals can exchange positions, and each such possible exchange lowers the energy. A half-filled set maximises the number of parallel electrons and therefore the number of exchanges. The second is symmetry: a half-filled or completely filled subshell has a spherically symmetric electron distribution, which minimises electron-electron repulsion. Together these outweigh the small cost of promoting an electron from the s orbital, which is why chromium and copper both end up with a single s electron.

Because the spin-only formula depends only on how many unpaired electrons there are, not on how many electrons are present in total. A high-spin d-four configuration and a high-spin d-six configuration both have four unpaired electrons and therefore the same predicted moment. So do d-three and d-seven. Distinguishing them needs another observable, such as the colour of the complex, its geometry, or the known oxidation-state chemistry of the metal. That is why examination questions of this type always supply one further clue.
Sources and How This Chapter Was CheckedSyllabus scope, what was derived rather than quoted, and how every answer here was checked.

Scope follows the JEE Advanced syllabus for 2026 (Chemistry, Atomic structure): the Bohr model and the spectrum of the hydrogen atom, the wave-particle duality of matter, the de Broglie relation and the uncertainty principle.

It also covers the qualitative quantum mechanical picture of the hydrogen atom, the shapes of , and orbitals, the four quantum numbers, the aufbau principle, the Pauli exclusion principle and Hund's rule, together with the electronic configurations of the elements.

The treatment concentrates on what Advanced adds to Main: node counting of both kinds, the radial distribution function, Slater's rules for effective nuclear charge, the reason the filling and ionisation orders of and differ, exchange energy as the explanation for the aufbau exceptions, and the spin-only magnetic moment.

Results were derived rather than quoted. The effective nuclear charges were computed group by group from Slater's rules; the exchange-pair counts from the combinatorial formula; the unpaired-electron count from inverting the magnetic moment expression; and the velocity uncertainties directly from the uncertainty relation.

Every illustration was checked against a second route or a limiting case. Node counts were verified against the requirement that the total equals ; the magnetic moment of a ion was checked against its known value near six Bohr magnetons; and the uncertainty estimate for an electron was compared with the Bohr orbital speed to confirm it is of the same order.

The illustrations are teaching problems written for this chapter, not previous-year questions, and are not labelled as such.

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