Q.How would you account for the irregular variation of ionisation enthalpies (first and second) in the first series of the transition elements?
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Transition Elements: From Intuition to Definition
Imagine you're building a house with bricks. Most bricks are identical — you stack them in neat rows. But some bricks are special: they have extra slots on their sides where you can attach hooks, magnets, or other bricks. These special bricks can change the shape of the wall, conduct electricity, or even change colour when you heat them.
In the periodic table, transition elements are those special bricks. They are the metals that sit in the middle block — groups 3 to 12 — and they have a unique ability: they can use their inner electrons (not just the outermost ones) to form bonds, change oxidation states, and create colourful compounds.
The Intuition: Why "Transition"?
The word "transition" comes from the idea that these elements form a bridge between the highly reactive metals on the left (like sodium, magnesium) and the less reactive metals / non-metals on the right (like aluminium, silicon). Their properties are not extreme — they are in-between.
But the real reason they are special lies in their electron configuration.
The Precise Definition (IUPAC)
A transition element is an element whose atom has an incomplete d sub-shell, or which can give rise to cations with an incomplete d sub-shell.
Let's unpack that.
1. The "d" sub-shell
Electrons are arranged in shells (K, L, M, N...) and sub-shells (s, p, d, f). The d sub-shell can hold a maximum of 10 electrons. In transition elements, the d sub-shell is being filled — but not completely.
For example, consider Iron (Fe):
- Atomic number 26
- Electron configuration: 1s22s22p63s23p64s23d6
- The 3d sub-shell has 6 electrons — it is incomplete (it can hold 10).
So iron is a transition element.
2. The "or" part — cations matter
Some elements have a complete d sub-shell in their neutral atom, but when they lose electrons to form positive ions (cations), the d sub-shell becomes incomplete.
Example: Zinc (Zn)
- Neutral Zn: [Ar]3d104s2 — the 3d sub-shell is full (10 electrons).
- But Zn commonly forms Zn2+: [Ar]3d10 — still full.
- So zinc is NOT a transition element by the IUPAC definition.
Example: Copper (Cu)
- Neutral Cu: [Ar]3d104s1 — 3d is full.
- But Cu2+: [Ar]3d9 — now the 3d sub-shell is incomplete.
- So copper IS a transition element.
A common mistake: thinking that all elements in the d-block (groups 3–12) are transition elements. They are not. Zinc, cadmium, and mercury are d-block elements but NOT transition elements because their common cations have a full d sub-shell.
The "d-block" vs "Transition Elements"
| d-block elements | Transition elements |
|---|---|
| Groups 3 to 12 | Groups 3 to 11 (excluding Zn, Cd, Hg) |
| All have d electrons | Must have incomplete d sub-shell in atom or common cation |
Why this formula?
Transition Element Definition: The "Why" Behind the Definition
The Core Definition
A transition element (IUPAC definition) is an element whose atom has an incomplete d-subshell in its ground state or can form stable ions with an incomplete d-subshell.
Key exam point: This definition covers both the neutral atom and its common ions.
Why This Definition? The Reasoning
1. The d-orbital filling pattern
In the periodic table, transition elements belong to the d-block (Groups 3–12). As we move across a period, electrons fill the (n−1)d orbitals after the ns orbital.
For example, in Period 4:
- Scandium (Sc): [Ar]3d14s2 — has one d-electron → transition element
- Zinc (Zn): [Ar]3d104s2 — d-subshell is full → not a transition element
2. The "incomplete d-subshell" condition
The definition focuses on incompleteness because:
- A full d-subshell (d10) is exceptionally stable (like a noble gas configuration for d-orbitals)
- Elements with d10 configurations do not show the characteristic properties of transition metals (variable oxidation states, coloured compounds, catalytic activity, paramagnetism)
3. Why include ions?
Consider Zinc (Zn):
- Ground state: [Ar]3d104s2 — d-subshell is full → not a transition element
- Common ion: Zn2+: [Ar]3d10 — still full → still not a transition element
Now consider Copper (Cu):
- Ground state: [Ar]3d104s1 — d-subshell is full → by atom definition alone, not a transition element
- But Cu2+: [Ar]3d9 — incomplete d-subshell → is a transition element
Therefore: The definition must include ions to correctly classify elements like Cu, which form stable ions with incomplete d-subshells.
The "Formula" — A Decision Tree
The definition can be expressed as a logical condition:
Transition element⟺(Atom has d1−9)∨(Stable ion has d1−9)
Where:
- d1−9 means incomplete d-subshell (1 to 9 electrons)
- d0 or d10 means complete (empty or full) → not a transition element
Common Exam Exceptions …
The key idea is that first ionisation enthalpy rises only mildly and irregularly across the series (d-electrons shield the 4s electrons somewhat, but not perfectly), while the real, sharp irregularity shows up in the second ionisation enthalpy.
Reasoning:
- From Sc to Zn, nuclear charge increases steadily, so first ionisation enthalpy (ΔiH1) generally rises — but only slightly and with minor bumps, because the added 3d electrons shield the outer 4s electron from the growing nuclear charge almost as effectively as it shields itself, keeping the rise gentle (unlike the steep rise across a normal period of non-transition elements).
- The second ionisation enthalpy (ΔiH2) shows the real irregularity: it is unusually high for Cr and Cu, because their singly-charged ions (Cr+=3d5, Cu+=3d10) already have an extra-stable, half-filled or fully-filled d-subshell — removing a second electron means breaking into that stable subshell, which costs much more energy. …
The first ionisation enthalpy rises only slightly and irregularly across the first transition series, because the added 3d electrons imperfectly shield the 4s electrons from the growing nuclear charge. The sharper irregularity is in the second ionisation enthalpy: it is unusually high for Cr and Cu (whose M+ ions have the extra-stable 3d5/3d10 configurations, so removing a further electron breaks that stability) and comparatively low for Mn and Zn (whose M+ ions still carry one loosely-held 4s electron beyond a stable d5/d10 core).
The Real Data (Table 4.2)
| Element | ΔiH1 | M+ configuration | ΔiH2 |
|---|---|---|---|
| Sc | 631 | 3d14s1 | 1235 |
| Ti | 656 | 3d24s1 | 1309 |
| V | 650 | 3d34s1 | 1414 |
| Cr | 653 | 3d5 | 1592 |
| Mn | 717 | 3d54s1 | 1509 |
| Fe | 762 | 3d64s1 | 1561 |
| Co | 758 | 3d74s1 | 1644 |
| Ni | 736 | 3d84s1 | 1752 |
| Cu | 745 | 3d10 | 1958 |
| Zn | 906 | 3d104s1 | 1734 |
Step-by-Step Reasoning
1. First ionisation enthalpy — a gentle, only mildly irregular rise.
Across Sc→Zn, nuclear charge rises by one unit each step, so ΔiH1 generally increases (631 → 906). But the rise is much gentler than across a normal (non-transition) period, because each new electron is added to an inner 3d orbital rather than the outer shell — a 3d electron shields the 4s electrons from the nucleus almost as effectively as another 4s electron would, so the effective nuclear charge felt by the valence electron increases only slowly. This is why the chapter describes the first-ionisation-enthalpy trend as "irregular... though of little chemical significance," without pinning the irregularity to any one specific element.
2. Second ionisation enthalpy — the real, well-defined break.
ΔiH2 removes an electron from the singly-charged ion M+, and here the electronic configuration of M+ matters directly:
- Chromium: neutral Cr is 3d54s1 (the well-known half-filled-stability exception), so Cr+ is already 3d5 — a stable, half-filled d-subshell. Removing a second electron means breaking into this stable arrangement, so ΔiH2 for Cr (1592) is unusually high.
- Copper: neutral Cu is 3d104s1, so Cu+ is 3d10 — a stable, fully-filled subshell. Breaking into it likewise makes Cu's ΔiH2 (1958) the highest in the row.
- Manganese: neutral Mn is 3d54s2, so Mn+ is 3d54s1 — the stable 3d5 core is already intact, with one "spare" 4s electron still to remove. Taking that easy 4s electron gives Mn a comparatively low ΔiH2 (1509) — a dip just below Cr's spike, not a peak. …
Method: Configuration-and-Data Analysis (Table 4.2)
This method explains the irregular variation by pairing each element's electronic configurations (atom and M+ ion) with the actual printed data, instead of relying on remembered "dip" rules.
Steps
Step 1: Write the configurations that matter
ΔiH1 removes an electron from the neutral atom M; ΔiH2 removes one from the M+ ion. So write both configurations for each element (Table 4.2's M and M+ rows).
Step 2: Check the first ionisation enthalpy against the data
Table 4.2 (kJ/mol): Sc 631, Ti 656, V 650, Cr 653, Mn 717, Fe 762, Co 758, Ni 736, Cu 745, Zn 906. The rise is gentle and only mildly irregular — each added 3d electron shields the 4s electrons from the growing nuclear charge, so the effective nuclear charge climbs slowly. Note there is no clean dip at Cr or Cu: Cr (653) is slightly above V (650), and Cu (745) is slightly above Ni (736).
Step 3: Explain the second ionisation enthalpy — where the sharp irregularity lives
- Cr⁺ is 3d5 (stable, half-filled) — removing another electron breaks into it, so ΔiH2 is unusually high (1592).
- Cu⁺ is 3d10 (stable, fully filled) — breaking into it makes Cu's ΔiH2 the highest in the row (1958).
- Mn⁺ is 3d54s1 — the second electron comes from the spare 4s, leaving the stable 3d5 intact, so ΔiH2 is comparatively low (1509).
- Zn⁺ is 3d104s1 — same pattern, so Zn's ΔiH2 (1734) sits below Cu's.
Step 4: Summarise (all values from Table 4.2, kJ/mol)
| Element | ΔiH1 | ΔiH2 | Reason |
|---|---|---|---|
| Cr | 653 — no dip (just above V's 650) | 1592 — unusually high | Cr⁺ is stable 3d5; a second removal breaks it |
| Mn | 717 — above Cr | 1509 — comparatively low | Mn⁺ is 3d54s1; the spare 4s electron goes easily |
Here is a breakdown of the common mistakes students make when explaining the irregular variation of ionisation enthalpies in the first transition series, along with how to avoid each.
The Core Concept (The "Why")
The irregular variation is attributed to the varying degrees of stability of the different 3d configurations (e.g., d0, d5, d10 are exceptionally stable). Two things follow from the real data (Table 4.2):
- First ionisation enthalpy (ΔiH1): rises gently and only mildly irregularly across Sc → Zn (631 → 906 kJ/mol), because each added 3d electron partially shields the 4s electrons from the growing nuclear charge. There is no clean dip at Cr or Cu.
- Second ionisation enthalpy (ΔiH2): shows the sharp, well-defined irregularity — unusually high for Cr (1592) and Cu (1958), whose M+ ions are the stable 3d5 and 3d10; comparatively low for Mn (1509) and Zn (1734), whose M+ ions still carry one spare, easily-removed 4s electron.
Common Mistake #1: Claiming the First Ionisation Enthalpy "Dips" at Cr and Cu
The Mistake: Students reason "Cr and Cu each have only one 4s electron, and removing it gives a stable d5/d10 ion — so their ΔiH1 must dip below their neighbours'."
Why it's wrong: Table 4.2's own numbers refute it: Cr's ΔiH1 (653) is slightly higher than V's (650), and Cu's (745) is slightly higher than Ni's (736). The stable-configuration effect shows up cleanly in ΔiH2, not as first-ionisation dips.
How to Avoid: Quote the data, not the remembered rule. If asked about ΔiH1, say the rise is gentle and only mildly irregular; save the d5/d10 stability argument for ΔiH2.
Common Mistake #2: Telling the Same Story for ΔiH1 and ΔiH2
The Mistake: Students say "Cr has low ΔiH1 and also low ΔiH2" (or high for both), applying one blanket rule to both quantities.
The Correct Logic: The two quantities remove electrons from different species:
- ΔiH1 (M → M⁺) depends on the neutral atom.
- ΔiH2 (M⁺ → M²⁺) depends on the M+ ion:
- Cr⁺ (3d5) → Cr²⁺ (3d4): destroys stable d5 → high ΔiH2.
- Cu⁺ (3d10) → Cu²⁺ (3d9): destroys stable d10 → high ΔiH2.
- Mn⁺ (3d54s1) → Mn²⁺ (3d5): removes the spare 4s electron, leaving stable d5 → low ΔiH2.
- Zn⁺ (3d104s1) → Zn²⁺ (3d10): same pattern → ΔiH2 below Cu's.
How to Avoid: Write the configurations of M, M⁺, and M²⁺ for each element. Ask: "Is the electron being removed a spare 4s electron (easy), or does it break a stable d5/d10 core (hard)?"
Common Mistake #3: Writing Wrong Ground-State Configurations
The Mistake: Students write Cr as 3d44s2 or Cu as 3d94s2, and then cannot explain the irregularities.
The Correct Logic: The actual ground-state configurations are the two exceptions:
- Cr: [Ar]3d54s1 (not 3d44s2)
- Cu: [Ar]3d104s1 (not 3d94s2)
How to Avoid: Memorise the two exceptions (Cr and Cu). For every other 3d element, the general 3dn4s2 rule holds.
Common Mistake #4: Blaming Only "Nuclear Charge" or "Shielding"
The Mistake: Students say "ionisation enthalpy increases because nuclear charge increases" and stop there. That explains the general rise, not the irregularities. …
- COMEDK 2026Set 2026-A1 markMCQQ.Pick out the correct option Assertion(A): Mercury is not considered as a transition element Reason (R): Mercury is a liquid (A) A is false but R is true (B) Both A and R are true but R is the correct explanation of A (C) A is true but R is false (D) Both A and R are true, R is not the correct explanation of A
›Reveal solutionSolution
The assertion is true (mercury is not a transition element) and the reason is true (mercury is a liquid at room temperature), but the reason does not explain the assertion — the correct classification depends on electron configuration, not physical state.
Concept & Intuition
Transition elements are defined by having an incomplete d-subshell in their neutral atom or common oxidation states. Mercury (Hg) has the electron configuration [Xe]4f145d106s2. Its 5d subshell is completely filled, so it does not meet the definition of a transition element. The fact that mercury is a liquid at room temperature is a physical property related to relativistic effects and weak metallic bonding — it has nothing to do with its electronic classification. The question tests whether you can separate a true statement (mercury is liquid) from its relevance to a different true statement (mercury is not a transition element).
Step-by-step reasoning
-
Check the Assertion (A):
Mercury’s ground-state electron configuration ends in 5d106s2. The d-subshell is full. In its common oxidation states (e.g., Hg²⁺, which loses the 6s electrons), the d-subshell remains 5d10 — still full. Since a transition element requires an incomplete d-subshell in the atom or a common ion, mercury does not qualify.
→ Assertion (A) is true.
-
Check the Reason (R):
Mercury is indeed a liquid at standard temperature and pressure (melting point −38.8 °C).
→ Reason (R) is true.
-
Evaluate the connection between A and R:
The reason given for why mercury is not a transition element is “mercury is a liquid.” But the actual reason is its filled d-subshell. The liquid state is irrelevant to the electronic definition. Therefore, R is not the correct explanation of A.
-
Match to the options: …
-
- COMEDK 2026Set 2026-M1 markMCQQ.The statements given below contains assertion and reason. Choose the correct option Assertion (A): Cr, Mo and W possess the highest melting point in their respective series of elements. Reason (R): Cr, Mo and W have stable half-filled electrons in the 'd' shell resulting in strong metallic bonding. (A) A is true but R is false (B) Both A and R are true, R is the correct explanation of A (C) Both A and R are true but R is not the correct explanation of A (D) A is false but R is true
›Reveal solutionSolution
[!TLDR]
The assertion (Cr, Mo, W have the highest melting points in their series) and the reason (their stable half-filled d configuration gives the strongest metallic bonding) are both true, and the reason is the correct explanation, so option (B).
Concept
From CBSE Class 12 d- and f-block chemistry: the melting point of a transition metal depends on the strength of metallic bonding, which rises with the number of unpaired (n−1)d and ns electrons taking part in bonding. This number is greatest near the middle of each series.
Solution …
- COMEDK 2024Set 2024-A1 markMCQQ.The correct order of increasing melting point is (A) Cr<Ti<V<Mn (B) Mn<Ti<V<Cr (C) Ti<V<Cr<Mn (D) V<Ti<Mn<Cr
›Reveal solutionSolution
The melting points of transition metals depend on the number of unpaired d-electrons available for metallic bonding. For Cr, Ti, V, and Mn, the order of increasing melting point is Mn < Ti < V < Cr, which corresponds to option (B).
The key concept here is metallic bonding strength in transition metals. In a transition metal, the melting point reflects how strongly the atoms are held together. The strength of metallic bonding depends on the number of electrons that can participate in bonding — specifically, the number of unpaired d-electrons. More unpaired d-electrons mean stronger bonding and a higher melting point.
For the first-row transition metals from Ti to Mn, the d-orbital filling is:
- Ti: [Ar] 3d² 4s² → 2 unpaired d-electrons
- V: [Ar] 3d³ 4s² → 3 unpaired d-electrons
- Cr: [Ar] 3d⁵ 4s¹ → 6 unpaired electrons (because of the half-filled stability, one 4s electron moves to the 3d)
- Mn: [Ar] 3d⁵ 4s² → 5 unpaired d-electrons
Watch outA common mistake is to think that Mn, with 5 unpaired d-electrons, should have a very high melting point. But Mn has an unusually low melting point because its half-filled d-subshell is stable and symmetrical, leading to weaker metallic bonding — the atoms don't "stick" as strongly.
Now, let's work through the reasoning step by step.
-
Understand the trend in metallic bonding strength.
Melting point in transition metals generally increases with the number of unpaired d-electrons, because these electrons form a "sea" that binds the positive metal ions together. However, when the d-subshell is exactly half-filled (d⁵) or fully filled (d¹⁰), the extra stability reduces the tendency to share electrons, lowering the melting point.
-
List the elements and their unpaired d-electron counts:
- Ti: 2 unpaired
- V: 3 unpaired
- Cr: 6 unpaired (due to 4s¹ 3d⁵ configuration)
- Mn: 5 unpaired
-
Predict the order based on unpaired electrons (ignoring the half-filled anomaly): …
- COMEDK 2023Set 2023-E1 markMCQQ.Match the following characteristics of transition metals given in Column I with the examples listed in Column II .tg {border-collapse:collapse;border-spacing:0;} .tg td{border-color:black;border-style:solid;border-width:1px;font-family:Arial, sans-serif;font-size:14px; overflow:hidden;padding:10px 5px;word-break:normal;} .tg th{border-color:black;border-style:solid;border-width:1px;font-family:Arial, sans-serif;font-size:14px; font-weight:normal;overflow:hidden;padding:10px 5px;word-break:normal;} .tg .tg-c3ow{border-color:inherit;text-align:center;vertical-align:top} .tg .tg-7btt{border-color:inherit;font-weight:bold;text-align:center;vertical-align:top} .tg .tg-0pky{border-color:inherit;text-align:left;vertical-align:top} S. No. Characteristic properties S. No. Examples W Chemically inert, non-stoichiometric compound A WO3 X Higher oxidation states are more stable B TiCl4 Y Due to inert pair effect, lower oxidation state is more stable C Mn4N Z. Colourless compound of transition metal D SnCl2 (A) W=BX=CY=DZ=A (B) W=CX=DY=AZ=B (C) W=CX=AY=DZ=B (D) W=AX=DY=CZ=B
›Reveal solutionSolution
[!TLDR]
Using standard d-block trends, W=Mn4N (C), X=WO3 (A), Y=SnCl2 (D), Z=TiCl4 (B), which is option (C).
Concept
This is the CBSE/NCERT Class 12 "d- and f-block" chapter: transition metals form hard, chemically inert interstitial (non-stoichiometric) compounds; heavier elements show stable high oxidation states; the inert-pair effect stabilises lower oxidation states for post-transition heavy elements; and d0/d10 ions are colourless.
Solution
W — chemically inert, non-stoichiometric compound: interstitial nitrides/carbides such as Mn4N have small atoms trapped in the metal lattice, are hard, inert and non-stoichiometric. So W=C.
X — higher oxidation states more stable: among 5d metals the highest oxidation state is very stable; tungsten is stable as W(VI) in WO3. So X=A. …
- COMEDK 2021Set 20211 markMCQQ.In 3d-transmission series, which one has the least melting point? (A) V (B) Zn (C) Mn (D) Cu
›Reveal solutionSolution
Compare: V ~ 2175 K, Mn ~ 1519 K, Cu ~ 1358 K.
Concept: Melting points across the 3d series depend on the number of unpaired d electrons available for metallic bonding.
Zn has the configuration 3d10 4s2 - a completely filled d subshell. Its d electrons are not available for metallic bonding, so only the two 4s electrons participate; metallic bonding is weakest. Zn melts …
- COMEDK 2021Set 2021-B1 markMCQQ.Which of the following statements is NOT correct with respect to interstitial compounds of transition metals? (A) They have comparatively low melting points than those of the pure metals. (B) They are chemically inert. (C) They retain metallic conductivity (D) They are very hard and rigid
›Reveal solutionSolution
Interstitial compounds are known for high (not low) melting points, so statement (A) is the incorrect one.
Properties of interstitial compounds:
- High melting points, often exceeding those of the parent metal — so (A) is wrong.
- (B) They are chemically fairly inert — correct.
- (C) They retain metallic conductivity — correct. …
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