Chemistry · Classification of Elements and Periodicity

Ionisation Enthalpy

Ionisation enthalpy is the energy needed to strip the most loosely held electron from a free gaseous atom, and it is one of the most heavily examined periodic properties in NEET. Following NCERT Class 11 Chemistry §3.7.1(c), this note develops the definition of first, second and successive ionisation enthalpies, the period-and-group trends and the factors that govern them, and the two anomalies — beryllium above boron and nitrogen above oxygen — that the examiner returns to almost every year.

What ionisation enthalpy means

A quantitative measure of an element's tendency to lose an electron is its ionisation enthalpy ($\Delta_i H$). NCERT defines it as the energy required to remove an electron from an isolated gaseous atom (X) in its ground state. The first ionisation enthalpy is the enthalpy change for the process in which the single most loosely bound electron departs:

$$\ce{X(g) -> X+(g) + e-} \qquad \Delta_i H_1$$

Because work must be done against the attraction between the negative electron and the positive nucleus, energy is always absorbed; ionisation enthalpy is therefore always positive. It is reported in $\text{kJ mol}^{-1}$. The qualifier "isolated gaseous atom" is deliberate — it ensures that the value reflects only the atom itself, free from the interactions an atom would feel in a liquid or solid. When the term ionisation enthalpy is used without qualification, it always means the first ionisation enthalpy.

Figure 1 · Energetics

The first ionisation step on an energy axis

Energy → X(g) X⁺(g) + e⁻ ΔᵢH₁ > 0
The cation-plus-electron state lies above the neutral atom, so removing the first electron is endothermic. The vertical gap is the first ionisation enthalpy, always a positive quantity.

Successive ionisation enthalpies

Once the first electron has gone, a second electron can be removed from the resulting cation. The energy needed for this is the second ionisation enthalpy, the energy required to detach the second most loosely bound electron:

$$\ce{X+(g) -> X^2+(g) + e-} \qquad \Delta_i H_2$$

NCERT states the governing rule plainly: the second ionisation enthalpy is always higher than the first, because it is more difficult to remove an electron from a positively charged ion than from a neutral atom. In the same way the third ionisation enthalpy exceeds the second, and so on. The reason is electrostatic — after one electron leaves, the nucleus still carries its full charge but now acts on fewer electrons, so each remaining electron is held more tightly. The general inequality is therefore:

$$\Delta_i H_1 < \Delta_i H_2 < \Delta_i H_3 < \dots$$

QuantityProcessComparison
First IE, $\Delta_i H_1$X(g) → X⁺(g) + e⁻Smallest of the set
Second IE, $\Delta_i H_2$X⁺(g) → X²⁺(g) + e⁻Larger than the first
Third IE, $\Delta_i H_3$X²⁺(g) → X³⁺(g) + e⁻Larger than the second

Factors that control IE

Because ionisation enthalpy measures how firmly the outermost electron is held, it is fixed by the balance between two opposing influences identified in NCERT: the attraction of the electrons towards the nucleus and the repulsion of the electrons from one another. Working through these, four operational factors emerge.

FactorEffect on IEWhy
Nuclear charge (Z)Higher Z → higher IEA larger positive charge pulls the valence electron in more strongly.
Atomic size / distanceLarger atom → lower IEThe farther the electron, the weaker the nuclear pull; IE and atomic radius are closely related properties.
Shielding (screening)More shielding → lower IEInner-core electrons screen the valence electron, so it feels a reduced effective nuclear charge.
Penetration of the orbitalBetter penetration → higher IEAn s electron penetrates closer to the nucleus than a p electron of the same shell, so it is held more tightly.

The unifying idea is effective nuclear charge. NCERT explains that the charge a valence electron actually experiences is less than the full nuclear charge because the intervening core electrons shield it. In lithium, for example, the 2s electron is screened by the inner $\ce{1s^2}$ core, so it experiences a net pull noticeably smaller than $+3$. Shielding is most effective when the inner shells are completely filled — the situation in the alkali metals, which carry a single $ns$ electron outside a noble-gas core and consequently have the lowest ionisation enthalpies in their periods.

The two extremes of the periodic landscape make the same point. The alkali metals, with their single, well-shielded valence electron, sit at the minima of any plot of ionisation enthalpy; their low values correlate directly with their high chemical reactivity. The noble gases, with closed shells and very stable configurations, sit at the maxima. Every periodic trend in ionisation enthalpy is, at heart, a contest between rising nuclear charge on one side and growing size plus shielding on the other.

Two broad trends govern the first ionisation enthalpy: it generally increases across a period and decreases down a group. Each follows from the same factors, but with a different factor winning.

Moving from left to right across a period, successive electrons enter orbitals of the same principal quantum level. The shielding by the inner core barely increases, yet the nuclear charge keeps climbing. NCERT puts it crisply: across a period, increasing nuclear charge outweighs the shielding. The outermost electrons are therefore held more and more tightly and the ionisation enthalpy rises. Descending a group, the valence electron lies in a shell increasingly far from the nucleus, and shielding by the filled inner shells grows. Here the increase in shielding outweighs the rising nuclear charge, the outermost electron is held more loosely, and less energy is needed to remove it.

Figure 2 · Trend map

Direction of increasing first ionisation enthalpy

IE increases across a period → IE increases up a group ↑ low (alkali metals) high (noble gases)
First ionisation enthalpy is lowest at the bottom-left (alkali metals) and highest at the top-right (noble gases). The arrows show the dominant directions, before the period-2 anomalies are layered on.
Related concept

Ionisation enthalpy and atomic size move in opposite directions. To see why the radius shrinks across a period and grows down a group, read Atomic and Ionic Radius.

Second-period data and the saw-tooth

The general "increase across a period" rule is only the backbone of the trend. Plotting the actual first ionisation enthalpies of the second period reveals a saw-tooth, not a straight climb: the rise from lithium to neon is interrupted at boron and again at oxygen. The values from NCERT Fig. 3.6(a) make the dips explicit.

ElementValence config.$\Delta_i H_1$ / kJ mol⁻¹Note
Li2s¹520Period minimum
Be2s²899Filled 2s gives a local peak
B2s² 2p¹801Dip — below Be
C2s² 2p²1086Trend resumes
N2s² 2p³1402Half-filled 2p peak
O2s² 2p⁴1314Dip — below N
F2s² 2p⁵1681Sharp rise
Ne2s² 2p⁶2080Period maximum
Figure 3 · Saw-tooth plot

First ionisation enthalpy of Li → Ne against atomic number

ΔᵢH₁ (kJ mol⁻¹) → Atomic number Z → Li Be B C N O F Ne Be > B dip N > O dip
The overall upward march from Li to Ne carries two breaks: boron falls below beryllium and oxygen falls below nitrogen. These two dips are the anomalies tested in NEET.

The Be > B and N > O anomalies

The two dips in Figure 3 are not measurement quirks — they follow directly from the penetration factor and from electron configuration stability. Both must be reasoned, not memorised, because the examiner phrases them in many disguises.

Beryllium above boron. Boron (Z = 5) has a higher nuclear charge than beryllium (Z = 4), yet its first ionisation enthalpy is the lower of the two. The reason lies in which electron is removed. In beryllium ($\ce{2s^2}$) the electron removed is a 2s electron; in boron ($\ce{2s^2 2p^1}$) it is the 2p electron. A 2s electron penetrates closer to the nucleus than a 2p electron, so the 2p electron of boron is more shielded by the inner core and is held less tightly. It is therefore easier to remove the 2p electron of boron than the 2s electron of beryllium, and boron has the smaller first ionisation enthalpy.

Nitrogen above oxygen. Nitrogen ($\ce{2s^2 2p^3}$) carries its three 2p electrons in three separate orbitals, in line with Hund's rule. Oxygen ($\ce{2s^2 2p^4}$) must place two of its four 2p electrons in the same orbital, and the resulting electron–electron repulsion makes that paired electron easier to remove. So although oxygen has the greater nuclear charge, its fourth 2p electron is less firmly held than any of nitrogen's three unpaired electrons, and the ionisation enthalpy of nitrogen exceeds that of oxygen. The extra stability of the exactly half-filled 2p³ shell is the same idea, viewed from nitrogen's side.

NEET Trap

The two dips that overturn the "left-to-right increase" rule

Candidates write the period-2 order as a clean increase Li < Be < B < C < N < O < F. That is wrong on two counts. Boron drops below beryllium (a 2p electron is removed, not a 2s), and oxygen drops below nitrogen (the half-filled 2p³ of N is extra stable). The correct increasing order is Li < B < Be < C < O < N < F < Ne.

The same two effects repeat in period 3: Mg > Al (3s versus 3p removal, the basis of NCERT's Problem 3.6) and P > S (half-filled 3p³ stability). Watch the wording — a question phrased as "decreasing order" or "incorrect arrangement" hides the same anomaly.

Reason from configuration, not from atomic number. A higher Z does not guarantee a higher ionisation enthalpy when the comparison straddles an s-to-p or a half-filled-shell boundary.

Working out IE orders

Most NEET items reduce to one task: arrange a handful of elements in order of first ionisation enthalpy. The method is to apply the general period and group trend first, then check whether any pair crosses an s-to-p boundary or a half-filled-shell boundary, and finally insert the anomaly. Two worked cases show the routine.

Worked Example

Q. Arrange Li, Be, B, C, N in increasing order of first ionisation enthalpy.

All five lie in period 2, so the baseline trend is an increase from Li to N. Now check the anomaly: Be ($\ce{2s^2}$) versus B ($\ce{2s^2 2p^1}$) crosses the 2s-to-2p boundary, so B falls below Be. No half-filled-shell pair appears here (the N versus O dip is not in this set). Inserting the single anomaly gives Li < B < Be < C < N.

Worked Example

Q. Predict whether the first $\Delta_i H$ of Al is closer to 575 or 760 kJ mol⁻¹, given Na = 496, Mg = 737, Si = 786 kJ mol⁻¹. (NCERT Problem 3.6)

Aluminium ($\ce{3s^2 3p^1}$) loses a 3p electron, whereas magnesium ($\ce{3s^2}$) loses a 3s electron. The 3p electron is shielded by the 3s electrons, so Al's value should fall below Mg's 737, not rise toward Si. The answer is therefore closer to 575 kJ mol⁻¹ — the Mg > Al anomaly in action.

Quick Recap

Ionisation enthalpy at a glance

  • $\Delta_i H$ is the energy to remove the most loosely held electron from a gaseous atom, $\ce{X(g) -> X+(g) + e-}$; it is always positive and measured in kJ mol⁻¹.
  • Successive values rise: $\Delta_i H_1 < \Delta_i H_2 < \Delta_i H_3$, because removing an electron from a cation is harder than from a neutral atom.
  • Four factors: nuclear charge (↑ IE), atomic size (↓ IE), shielding (↓ IE), orbital penetration (s > p ⇒ ↑ IE).
  • IE increases across a period (Z outweighs shielding) and decreases down a group (shielding outweighs Z).
  • Anomalies: Be > B and N > O in period 2; Mg > Al and P > S in period 3.
  • Period-2 increasing order: Li < B < Be < C < O < N < F < Ne.

NEET PYQ Snapshot — Ionisation Enthalpy

Ionisation-enthalpy ordering is a NEET classic; the Be > B and N > O anomalies recur across years.

NEET 2024 · Q.59

Arrange the following elements in increasing order of first ionisation enthalpy: Li, Be, B, C, N.

  • (1) Li < Be < B < C < N
  • (2) Li < B < Be < C < N
  • (3) Li < Be < C < B < N
  • (4) Li < Be < N < B < C
Answer: (2)

The trend rises Li → N, but boron drops below beryllium because a shielded 2p electron is removed from B versus a 2s electron from Be. Hence Li < B < Be < C < N.

NEET 2016 · Q.23

Identify the arrangement that does not agree with the indicated property: "B < C < N < O (increasing first ionisation enthalpy)".

  • (1) B < C < N < O (increasing first ionisation enthalpy)
  • (3) Li < Na < K < Rb (increasing metallic radius)
  • (4) Al³⁺ < Mg²⁺ < Na⁺ < F⁻ (increasing ionic size)
Answer: (1) is the incorrect order

Nitrogen's half-filled 2p³ shell makes its IE greater than oxygen's, so the correct order is B < C < O < N. Option (1) wrongly places O above N.

NEET 2025 · Q.69 (statement D)

Statement D: "The correct order of the first ionisation enthalpies of Na, Mg, Al and Si is Si > Al > Mg > Na." Is statement D true?

Answer: D is false

The correct order is Si > Mg > Al > Na. Magnesium exceeds aluminium because the 3s electron penetrates the nucleus more than the 3p electron removed from Al (the Mg > Al anomaly).

Concept · Successive IE

Why is the second ionisation enthalpy of an element always greater than its first?

Reasoning

After the first electron leaves, the species is a cation; the full nuclear charge now acts on fewer electrons, holding each more tightly. Removing an electron from a positive ion needs more energy, so $\Delta_i H_2 > \Delta_i H_1$.

FAQs — Ionisation Enthalpy

Common doubts on the definition, the successive-IE rule and the period-2 anomalies.

What is ionisation enthalpy?

Ionisation enthalpy is the enthalpy change for removing the most loosely bound electron from an isolated gaseous atom in its ground state, as in X(g) → X+(g) + e–. It is always positive because energy must be supplied against the electron–nucleus attraction, and it is expressed in kJ mol⁻¹. The first ionisation enthalpy removes the first electron; unless otherwise stated, the term ionisation enthalpy refers to the first ionisation enthalpy.

Why is the second ionisation enthalpy always greater than the first?

After the first electron is removed, the species carries a positive charge, so the remaining electrons are pulled in more tightly by the unchanged nuclear charge acting on fewer electrons. Removing an electron from a cation is harder than from a neutral atom, so the second ionisation enthalpy exceeds the first, the third exceeds the second, and so on. Each successive ionisation enthalpy is therefore larger than the one before it.

Why is the first ionisation enthalpy of boron less than that of beryllium?

In beryllium the electron removed is a 2s electron, whereas in boron it is a 2p electron. A 2s electron penetrates closer to the nucleus than a 2p electron, so the 2p electron of boron is more shielded by the inner core and is held less tightly. Even though boron has a higher nuclear charge, it is easier to remove its 2p electron, making the first ionisation enthalpy of boron slightly smaller than that of beryllium.

Why does nitrogen have a higher ionisation enthalpy than oxygen?

Nitrogen has the half-filled configuration 2p³ in which the three 2p electrons occupy separate orbitals, an arrangement of extra stability with minimal electron–electron repulsion. Oxygen is 2p⁴, so two electrons must pair in one 2p orbital, creating electron–electron repulsion. The fourth 2p electron of oxygen is therefore easier to remove than one of nitrogen's three unpaired electrons, so the ionisation enthalpy of nitrogen exceeds that of oxygen.

Why does ionisation enthalpy increase across a period and decrease down a group?

Across a period, successive electrons enter the same principal shell, so shielding by the inner core barely changes while nuclear charge keeps rising. The increasing nuclear charge outweighs the shielding, the outermost electron is held more tightly, and ionisation enthalpy increases. Down a group, the valence electron is farther from the nucleus and shielding by inner shells increases enough to outweigh the rising nuclear charge, so ionisation enthalpy decreases.

What is the correct order of first ionisation enthalpy for Li, Be, B, C, N?

The increasing order is Li < B < Be < C < N. The general trend predicts a rise from lithium to nitrogen, but the Be > B anomaly drops boron below beryllium because a 2p electron is removed from boron versus a 2s electron from beryllium. Beyond boron the trend resumes through carbon up to nitrogen, whose half-filled 2p³ shell gives it the highest value in the set.