General Properties of Transition Elements

Slide across the fourth period of the periodic table — Sc to Zn — and the elements stop behaving like the s-block metals before them. They are harder, higher-melting, and instead of settling into one tidy oxidation state they roam across several. Their salts are often vividly coloured, their metals catalyse industrial reactions from ammonia synthesis to hydrogenation, and some of them respond to a magnet even as a compound in a bottle. All of this traces back to one structural fact: a transition element is one whose atom, or a common ion, has a partially filled d-subshell, so both the outer nsns and the inner (n−1)d(n-1)d electrons are available for bonding and for removal. This article builds the general "chemical personality" of the 3d series — metallic character, ionisation enthalpy, oxidation states, ionic radii, colour, magnetism, catalysis, and interstitial/alloy behaviour — from that single configuration fact, and quantifies the one calculation the syllabus asks you to actually do: the spin-only magnetic moment.

The core insight

Because both the nsns and (n−1)d(n-1)d electrons of a 3d atom are close in energy and available for bonding or ionisation, transition elements show variable oxidation states, coloured ions (via d–d transitions), and magnetic moments set by their unpaired d-electron count through μ=n(n+2)\mu = \sqrt{n(n+2)} BM.

The core idea

Definition and metallic character. IUPAC defines a transition element as one whose atom, or a common ion, has a partially filled d-subshell. The 3d series runs Sc([Ar]3d14s23d^14s^2) to Zn([Ar]3d104s23d^{10}4s^2). Strong metallic bonding — both nsns and (n−1)d(n-1)d electrons delocalised into the electron sea — makes every member hard, high-melting, and a good conductor.

Ionisation enthalpy. It rises gradually across the series, with irregular jumps at Cr and Cu, because increasing nuclear charge is poorly screened by d-electrons. Values sit well above those of s-block metals, so transition metals are far less reactive than alkali or alkaline-earth metals.

Oxidation states. Because nsns and (n−1)d(n-1)d electrons have comparable energies, both can be lost on oxidation, giving each element several accessible states rather than one fixed value. The lowest common state is usually +2 (loss of the two 4s4s electrons); the highest often equals the total ns + (n-1)d electron count, topping out at +7 for Mn ([Ar]3d54s23d^54s^2); the spread is widest near the middle of the series (Mn, Fe).

Ionic radii. M2+^{2+}/M3+^{3+} radii shrink gradually across the series — poor d-electron shielding against rising nuclear charge, the same mechanism (on a smaller scale) as lanthanide contraction — with a slight dip-and-rise superimposed on the trend.

Colour. A partially filled d-subshell lets an electron absorb visible light and jump to a higher d orbital — a d–d transition, treated qualitatively here and developed fully under crystal-field theory later. That is why most transition-metal ions are coloured, while d0d^0 ions (Sc3+^{3+}, Ti4+^{4+}) and d10d^{10} ions (Zn2+^{2+}, Cu+^+) are colourless — there is no d-electron to promote.

Magnetism. Unpaired d-electrons make a species paramagnetic (drawn into a field); an all-paired configuration is diamagnetic. Ignoring orbital contribution, the spin-only magnetic moment is

μ=n(n+2) BM\mu = \sqrt{n(n+2)}\ \text{BM}

where: nn is the number of unpaired electrons in the ion and BM (Bohr Magneton) is the unit of magnetic moment. μ\mu rises with nn and peaks near the middle of the series, where half-filled d5d^5 configurations maximise unpairing.

Catalysis and interstitial compounds. Variable oxidation states let transition metals offer low-activation-energy pathways through unstable intermediates (Fe in the Haber process, V2_2O5_5 in the Contact process, Ni in hydrogenation), and their surfaces adsorb and weaken reactant bonds. Because 3d atoms are similar in size they readily form substitutional alloys with each other, while small atoms (H, C, N, B) squeeze into interstitial voids of the lattice to give hard, high-melting interstitial compounds such as TiC and Fe3_3N.

Figure
d orbital electron filling for iron two plus showing four singly occupied boxes and one doubly occupied box giving four unpaired electrons
Fe2+ = [Ar]3d6 — Hund's rule filling of the five 3d orbitals Maximum unpairing first: four orbitals get one electron each, the fifth gets a second (paired) electron ↑ ↑ ↑ ↑ ↑ ↓ 1 unpaired 1 unpaired 1 unpaired 1 unpaired 1 pair (paired) Total unpaired electrons n = 4, so mu = sqrt(4 x 6) = 4.90 BM, paramagnetic
Derivation ASpin-only magnetic moment from an ion's configuration

The goal is to turn a bare ion formula such as Fe2+^{2+} into a numerical magnetic moment in Bohr Magnetons and a paramagnetic-or-diamagnetic verdict, using nothing beyond the atomic configuration, Hund's rule, and the spin-only formula μ=n(n+2)\mu = \sqrt{n(n+2)} — no orbital-angular-momentum correction, which the syllabus explicitly ignores at this stage.

Step 1. Write the parent atom's configuration from its atomic number, filling 4s4s before 3d3d is not needed here since we only need the total electron count; for Fe (Z = 26) it is [Ar]3d64s23d^64s^2.

Step 2. Form the ion by removing electrons in the correct order: for transition metals the 4s4s electrons are always removed before any 3d3d electron, because once occupied the 3d3d subshell drops below 4s4s in energy. Removing two electrons to form Fe2+^{2+} therefore strips both 4s4s electrons, leaving Fe2+^{2+} = [Ar]3d63d^6.

Step 3. Distribute the d-electrons among the five 3d orbitals by Hund's rule: fill all five orbitals singly first, then start pairing. For d6d^6, four orbitals hold one electron each and the fifth orbital holds the sixth (paired) electron, so the number of unpaired electrons is n=4n = 4.

Step 4. Substitute nn into the spin-only formula: μ=n(n+2)=4(4+2)=24≈4.90 BM\mu = \sqrt{n(n+2)} = \sqrt{4(4+2)} = \sqrt{24} \approx 4.90\ \text{BM}.

Step 5. Read off the magnetic classification: since n≠0n \neq 0 the ion has a nonzero moment and is paramagnetic; only an ion with n=0n = 0 (all d-electrons paired, e.g. d10d^{10} or low-spin d6d^6 in a complex, outside this scope) would be diamagnetic.

Worked example

Calculate the spin-only magnetic moment of Fe2+^{2+}, and separately rank Sc3+^{3+}, Ti3+^{3+}, Mn2+^{2+} and Zn2+^{2+} by unpaired electrons, stating which are coloured.

Step 1. Fe (Z = 26) is [Ar]3d64s23d^64s^2; removing the two 4s4s electrons gives Fe2+^{2+} = [Ar]3d63d^6. By Hund's rule, four of the five 3d orbitals hold one electron each and the fifth holds a paired second electron, so n=4n = 4.

Step 2. Apply the spin-only formula: μ=4(4+2)=24≈4.90 BM\mu = \sqrt{4(4+2)} = \sqrt{24} \approx 4.90\ \text{BM}. Since n≠0n \neq 0, Fe2+^{2+} is paramagnetic.

Step 3. Find the d-electron count of each remaining ion after removing 4s4s (then 3d, if needed) electrons: Sc3+^{3+} = [Ar]3d03d^0; Ti3+^{3+} = [Ar]3d13d^1; Mn2+^{2+} = [Ar]3d53d^5; Zn2+^{2+} = [Ar]3d103d^{10}.

Step 4. Count unpaired electrons by Hund's rule: Sc3+^{3+} (d0d^0) has 0; Ti3+^{3+} (d1d^1) has 1; Mn2+^{2+} (d5d^5, one electron in each of the five orbitals) has 5; Zn2+^{2+} (d10d^{10}, all orbitals doubly filled) has 0. Order: Sc3+^{3+} = Zn2+^{2+} (0) less than Ti3+^{3+} (1) less than Mn2+^{2+} (5).

Step 5. Colour needs a partially filled d-subshell so a d–d transition is possible. Sc3+^{3+} (d0d^0) and Zn2+^{2+} (d10d^{10}) are colourless; Ti3+^{3+} (d1d^1) and Mn2+^{2+} (d5d^5) are coloured in principle, though Mn2+^{2+}'s colour is unusually faint because its particular d–d transitions are spin-forbidden. Answer: Fe2+^{2+} has μ≈4.90\mu \approx 4.90 BM (paramagnetic); unpaired-electron order is Sc3+^{3+} = Zn2+^{2+} (0) less than Ti3+^{3+} (1) less than Mn2+^{2+} (5), with only Ti3+^{3+} and Mn2+^{2+} coloured.

Competitive stretch

Quick check: what is the spin-only moment of Cr3+^{3+}? Cr (Z = 24) is the exception [Ar]3d54s13d^54s^1; removing three electrons (the one 4s4s, then two 3d3d) gives Cr3+^{3+} = [Ar]3d33d^3, with all three electrons unpaired by Hund's rule (n=3n = 3). So μ=3(3+2)=15≈3.87 BM\mu = \sqrt{3(3+2)} = \sqrt{15} \approx 3.87\ \text{BM} — a reminder that Cr's own atomic configuration (one 4s electron, not two) does not change the removal order once ionised.

Common traps

  • Removing d-electrons before s-electrons when forming a cation — always strip the nsns electrons first, then (n−1)d(n-1)d if more are needed (Cr3+^{3+} above needs one 4s4s and two 3d3d removed, in that order).
  • Assuming more unpaired electrons always means a more intense colour — colour intensity depends on whether the d–d transition is spin- and symmetry-allowed, not simply on the unpaired-electron count (Mn2+^{2+}'s 5 unpaired electrons give only a very faint colour).
  • Forgetting that d0d^0 (Sc3+^{3+}) and d10d^{10} (Zn2+^{2+}) ions are colourless — a common assumption is that all transition-metal ions are coloured.
  • Treating the ionisation-enthalpy trend as perfectly smooth — Cr and Cu (and neighbours) show irregular values from the extra stability of half-filled and fully-filled configurations.

Ask the tutor: Want to work through the spin-only moment for a few more ions, like Cr2+^{2+} or Co2+^{2+}, to get faster at the removal-order and Hund's-rule steps?

Why does the highest oxidation state of Mn go all the way to plus 7 but Zn stops at plus 2?

The highest oxidation state a 3d metal can reach is governed by how many ns and (n-1)d electrons it can plausibly lose. Mn is [Ar]3d54s23d^54s^2, with seven electrons in that combined shell, all removable under strong enough oxidising conditions, giving +7 (as in KMnO4_4). Zn is [Ar]3d104s23d^{10}4s^2: its 3d103d^{10} shell is complete and exceptionally stable, so only the two 4s4s electrons are ever lost, capping Zn at +2. A full or half-full d-subshell resists further ionisation, which is also why Zn is sometimes excluded from the "typical" transition-metal properties like variable oxidation states.

If colour comes from d to d transitions, why is Mn2+ barely coloured despite having 5 unpaired electrons?

Having unpaired electrons only tells you a transition metal ion is not automatically colourless; it does not guarantee an intense colour. Mn2+^{2+} (d5d^5, high-spin) has every d-orbital singly occupied, so any transition would have to flip an electron's spin as well as change its orbital — a spin-forbidden transition. Spin-forbidden transitions are allowed only very weakly by relativistic effects, so Mn2+^{2+} solutions look almost colourless (a very pale pink) even though, by unpaired-electron count alone, you might expect vivid colour. Colour intensity ultimately depends on selection rules, not just on how many electrons are unpaired.

Do I need to remember exact ionisation enthalpy or ionic radius values for CBSE Class 12?

No — the syllabus asks for the trend and its reasoning, not memorised numbers. You should be able to state that ionisation enthalpy rises gradually across the 3d series with irregularities at Cr and Cu, and that M2+^{2+}/M3+^{3+} ionic radii shrink gradually (with a small dip-and-rise) due to poor d-electron shielding against increasing nuclear charge. Board questions typically ask you to explain why these trends occur, using the ns/(n-1)d energy picture, rather than to recall a specific enthalpy or radius figure.

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