Q.(a) (I) Account for the following : (3 + 2)
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Start your 14-day free trial to unlock the full solution →Concept understanding — Stability of Oxidation States
Stability of Oxidation States – From Intuition to Precision
Imagine you're holding a ball on a hill. If you place it exactly at the top, it's balanced — but the slightest push sends it rolling down. That's an unstable position. If you place it in a small dip on the hillside, it stays put even if nudged — that's stable. Oxidation states work the same way: some are like the hilltop (easily changed), others like the dip (hard to change).
The Core Intuition
An oxidation state is just a number we assign to an atom to track how many electrons it has gained or lost compared to its neutral state. But atoms don't "want" to stay in arbitrary oxidation states — they want to reach a configuration that minimises their energy.
Stability here means: how reluctant is that oxidation state to change under normal conditions? A stable oxidation state resists being oxidised further or reduced further. An unstable one readily changes into something else.
The Precise Statement
Stability of an oxidation state refers to the tendency of an element to maintain that particular oxidation state under given conditions (temperature, pH, presence of other reagents). A stable oxidation state is one that does not easily undergo redox reactions — it is neither easily oxidised nor easily reduced.
This depends on three key factors:
- Electronic configuration – Half-filled and fully-filled d or f subshells confer extra stability (e.g., with is more stable than with in some contexts).
- Inert pair effect – Heavier p-block elements (like Tl, Pb, Bi) show lower oxidation states (e.g., +1 for Tl) as more stable than higher ones (+3 for Tl), because the s-electrons become reluctant to participate.
- Disproportionation tendency – Some oxidation states are unstable because they spontaneously convert into two other states (e.g., in aqueous solution gives and ).
Stability is relative — it depends on the environment. is stable in acidic solution but easily oxidised in alkaline medium. Always specify conditions when discussing stability.
Examples That Make It Concrete
Transition metals – () and () are exceptionally stable because half-filled/half-filled-like configurations have low energy. () is easily oxidised to — it's unstable.
p-block elements – is stable, is a strong oxidising agent (unstable). is a reducing agent (easily oxidised to ), so is more stable for tin.
Common pattern – For most elements, the most common oxidation state is the most stable one under standard conditions. But "most common" isn't always "most stable" — e.g., is common but is more stable in acidic solution.
Do not confuse "stability" with "occurrence". (as ) is common in the lab but is a powerful oxidising agent — it is not stable in the sense of resisting change. It readily accepts electrons.
How to Think About It in Exams …
Why this formula?
Stability of Oxidation States: Why It Works
This concept explains why certain oxidation states of an element are more stable than others — and why some states are never observed at all.
The Core Idea: Energy Minimisation
An oxidation state is stable when the total energy of the system is at a minimum. This depends on three competing factors:
- Ionisation energy (energy needed to remove electrons)
- Lattice energy (for ionic compounds) or bond energy (for covalent compounds)
- Electronic configuration (half-filled / fully-filled subshells)
There is no single formula for stability — instead, we use trends and principles that act as "formulae" for prediction.
Key Principle 1: Inert Pair Effect (for p-block elements)
Why it holds:
For heavier elements (e.g., Tl, Pb, Bi), the 6s² electrons are held very tightly due to poor shielding and relativistic effects. They resist removal.
- Result: Lower oxidation state (e.g., +1 for Tl, +2 for Pb) becomes more stable than the higher state (+3, +4).
- Example: is a strong oxidising agent — it readily gains two electrons to become .
Derivation logic:
The energy cost to remove the 6s² electrons is greater than the energy gained by forming additional bonds or lattice. So the system stays in the lower state.
Key Principle 2: Half-Filled / Fully-Filled Subshell Stability
Why it holds:
A half-filled (, ) or fully-filled (, ) subshell has extra exchange energy and symmetry — making it unusually stable.
- Example: () is more stable than (). () is more stable than ().
Derivation logic:
The exchange energy (Hund's rule) is maximum for half-filled configurations. Removing an electron from a half-filled shell costs extra energy — so the half-filled state is favoured.
Key Principle 3: Lattice Energy / Hydration Energy Compensation
For transition metals, stability of a particular oxidation state in aqueous solution depends on:
Why it holds:
- Higher oxidation states have higher ionisation energy (harder to remove electrons).
- But they also have higher hydration energy (smaller, more charged ions attract water more strongly).
- The balance determines which state is stable.
Example:
- is unstable in water because its hydration energy is too low to compensate for the loss of the second electron.
- is stable in water.
Key Principle 4: Disproportionation
Some oxidation states are unstable and spontaneously convert to two other states:
Why it holds: …
(a) is strongly positive (stable ); () colourless, () coloured; actinoids show many oxidation states; made by fusing with KOH/ then oxidising .
(b) Transition metals form alloys (similar radii); is a strong oxidiser (→ ); Ln & An both show +3 but An has more oxidation states; .
(I)(i) vs
A more positive reduction potential means the higher ion is reduced more easily. () is reduced to (, an exceptionally stable half-filled shell), so the reduction is very favourable ( V). (, half-filled ) is itself stable and resists reduction to (), so V.
(I)(ii) Colour of vs
Colour arises from d–d transitions, which need a partially filled d-subshell. is (no d-electron) → no transition → colourless. is ; its single electron in the split level absorbs visible light and jumps to → the ion appears violet.
(I)(iii) Wide range of oxidation states in actinoids
Actinoids: . The 5f, 6d and 7s orbitals lie very close in energy and the 5f orbitals are poorly shielded (more available for bonding than the buried 4f of lanthanoids), so electrons are removed from all these levels, giving oxidation states from +3 up to +7.
(II) Preparation of from
The green manganate is then oxidised to purple permanganate, e.g. by (a disproportionation) or electrolytically:
Concept understanding — Actinoids
Actinoids: The Heavy, Radioactive Inner Transition Metals
Imagine you are walking through the periodic table, row by row. You know the lanthanoids — the 14 elements from cerium to lutetium that sit below the main table, where the 4f subshell is being filled. Now go one row lower. The elements that follow actinium (atomic number 89) are the actinoids: thorium (90) through lawrencium (103). Here, the 5f subshell is being filled.
The name comes from actinium, the first element of the series. But the real story begins with uranium and plutonium — the elements that made nuclear energy and atomic bombs possible. These are not just academic curiosities; they are the workhorses of nuclear physics.
The Precise Statement
Actinoids are the 14 elements from thorium () to lawrencium () in which the 5f orbitals are progressively filled. They are all radioactive, exhibit a wide range of oxidation states, and show a steady decrease in ionic radii across the series — the actinoid contraction.
Why They Are Special
1. Radioactivity is the rule, not the exception. Every actinoid is radioactive. Some, like uranium-238, have half-lives comparable to the age of the Earth. Others, like lawrencium, exist for only seconds. This radioactivity is not a side effect — it is the defining property. It means their chemistry is often studied with trace amounts, using radiation detectors rather than test tubes.
2. Multiple oxidation states — more than you expect. Unlike the lanthanoids, which mostly stick to +3, the actinoids show a rich variety. Uranium, for example, exists as U, U, UO (U), and UO (U). The early actinoids (Th, Pa, U, Np, Pu) are especially versatile because the 5f, 6d, and 7s orbitals are close in energy. As you move right, the +3 state becomes more stable — curium and beyond behave more like lanthanoids.
3. The actinoid contraction. As you go from Th to Lr, the nuclear charge increases by 14 protons. The 5f electrons are poor at shielding each other, so the effective nuclear charge felt by the outer electrons rises steadily. The result: ionic radii shrink smoothly across the series. This is exactly analogous to the lanthanoid contraction, and it has the same consequence — the chemistry of later actinoids becomes very similar to their lanthanoid counterparts, making separation difficult.
The actinoid contraction is why americium and curium are so hard to separate from the lanthanoids in nuclear waste. Their ionic radii are nearly identical.
A Quick Comparison with Lanthanoids
| Property | Lanthanoids (4f) | Actinoids (5f) |
|---|---|---|
| Radioactivity | Mostly stable (except Pm) | All radioactive |
| Common oxidation state | +3 (strongly dominant) | +3, +4, +5, +6 (early ones) |
| 5f vs 4f character | 4f deeply buried, little bonding | 5f more exposed, can participate in bonding |
(a) is strongly positive (stable ); () colourless, () coloured; actinoids show many oxidation states; made by fusing with KOH/ then oxidising .
(b) Transition metals form alloys (similar radii); is a strong oxidiser (→ ); Ln & An both show +3 but An has more oxidation states; .
(I)(i) Transition metals form alloys
Their atomic and metallic radii are very similar, so atoms of one transition metal replace those of another in the crystal lattice with little distortion, forming solid solutions (alloys) such as brass and steel.
(I)(ii) is a strong oxidising agent …
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