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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Start your 14-day free trial to unlock the full solution →The first ionisation enthalpy rises only slightly and irregularly across the first transition series, because the added electrons imperfectly shield the electrons from the growing nuclear charge. The sharper irregularity is in the second ionisation enthalpy: it is unusually high for Cr and Cu (whose ions have the extra-stable / configurations, so removing a further electron breaks that stability) and comparatively low for Mn and Zn (whose ions still carry one loosely-held electron beyond a stable / core).
The Real Data (Table 4.2)
| Element | configuration | ||
|---|---|---|---|
| Sc | 631 | 1235 | |
| Ti | 656 | 1309 | |
| V | 650 | 1414 | |
| Cr | 653 | 1592 | |
| Mn | 717 | 1509 | |
| Fe | 762 | 1561 | |
| Co | 758 | 1644 | |
| Ni | 736 | 1752 | |
| Cu | 745 | 1958 | |
| Zn | 906 | 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 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 orbital rather than the outer shell — a electron shields the electrons from the nucleus almost as effectively as another 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.
removes an electron from the singly-charged ion , and here the electronic configuration of matters directly:
- Chromium: neutral Cr is (the well-known half-filled-stability exception), so is already — a stable, half-filled -subshell. Removing a second electron means breaking into this stable arrangement, so for Cr (1592) is unusually high.
- Copper: neutral Cu is , so is — a stable, fully-filled subshell. Breaking into it likewise makes Cu's (1958) the highest in the row.
- Manganese: neutral Mn is , so is — the stable core is already intact, with one "spare" electron still to remove. Taking that easy electron gives Mn a comparatively low (1509) — a dip just below Cr's spike, not a peak. …
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