Mass Spectrometry: Ionization and the Molecular Ion

An unknown white solid weighs nothing you can put on a balance. Yet it reveals its molecular weight instantly. A chemist bombards a puff of its vapor with high-energy electrons. Out comes a single sharp number. That number pins down its molecular formula to within a few candidates. This number is the mass of the molecular ion. The technique is mass spectrometry. It is arguably the fastest way to answer the very first question any structure-elucidation problem asks. How heavy is this molecule, and what is it made of? Mass spectrometry does not measure mass directly in the way a balance does. It measures the ratio of mass to charge, m/zm/z, for ions flying through a vacuum. First, an electron is torn off a neutral molecule to make it chargeable at all. That ionization step is itself a chemical event. A bond-orbital electron is ejected, leaving behind a radical cation, M+∙\mathrm{M}^{+\bullet}. Understanding why it happens the way it does is important. So is knowing which electron leaves, and how stable the resulting species is. This is exactly the kind of orbital reasoning used throughout structure determination. The peak this radical cation produces is the molecular ion peak. It is the anchor of the entire spectrum. Every other peak in the spectrum is a fragment lighter than it. Everything downstream is read relative to it. This includes degrees of unsaturation, isotope patterns, and the nitrogen rule. This article builds the physical picture of electron-impact (EI) ionization from first principles. It explains what a 70 eV electron beam actually does to a molecule in the gas phase. It explains why the process produces a radical cation rather than a simple cation. It explains why fragmentation is common but not universal. It also explains how to recognize the molecular ion peak with confidence. This holds even when the peak is small. From there we derive two of the most useful pieces of arithmetic in the whole subject. First, how m/zm/z of M+∙\mathrm{M}^{+\bullet} gives the molecular mass. This in turn constrains the molecular formula. Second, the nitrogen rule, a strikingly simple parity argument. It connects nitrogen count to whether MM is odd or even. This is The Logic of Structure Determination applied to its first and most direct instrument. What follows here sets up two natural continuations. One is reading the isotope pattern accompanying M+∙\mathrm{M}^{+\bullet}. This lets you count halogens and sulfurs (mass-spec-isotope-patterns). The other is reading the fragment peaks below MM, to reconstruct connectivity (mass-spec-fragmentation-mechanisms). Both depend entirely on first getting the molecular ion right. That is the whole business of this article.

Key takeaways
  • Electron-impact (EI) mass spectrometry ionizes gas-phase molecules by knocking an electron out with a ~70 eV electron beam, producing a radical cation M+∙\mathrm{M}^{+\bullet}.
  • The instrument measures mass-to-charge ratio m/zm/z; for a singly-charged ion, m/zm/z numerically equals the ion's mass in daltons.
  • The molecular ion peak is the highest-mass peak that is chemically reasonable (not just the highest mass in the spectrum — that role can be usurped by an isotope peak or a rare [M+1]+[M+1]^+ adduct).
  • The electron removed comes from the highest-occupied molecular orbital (lone pair > π bond > σ bond, by ionization energy ordering), which is why M+∙\mathrm{M}^{+\bullet} intensity tracks molecular stability under ionization, not molecular size.
  • The nitrogen rule: a molecule with an even number of nitrogen atoms (0, 2, 4, …) has an even nominal mass; an odd number of nitrogens gives an odd nominal mass — a direct consequence of nitrogen's odd valence with an even mass-to-valence mismatch.
  • Fragmentation competes with survival: a weak, unstable M+∙\mathrm{M}^{+\bullet} gives a small or absent molecular ion peak, forcing the chemist to hunt for it or infer MM indirectly.
  • Key idea: the molecular ion is a radical cation formed by removing one electron from a neutral molecule, and its m/zm/z is the molecular mass — every other observation in EI-MS is a deviation from, or a fragment of, this one number.

Where this lives today

EI-MS coupled to gas chromatography (GC-MS) is the backbone of forensic toxicology and environmental analysis: a molecular ion peak at a specific m/zm/z, cross-referenced against enormous spectral libraries (the NIST/EPA/NIH library holds hundreds of thousands of reference EI spectra), identifies unknown compounds in blood, urine, soil, or air in minutes. Pharmaceutical quality control leans on the same logic to confirm both the identity and the purity of a drug substance batch: an unexpected extra molecular ion peak signals a synthetic byproduct or degradation product before it ever reaches a patient. Doping-control laboratories detect anabolic steroids and their metabolites by exactly this kind of molecular-ion-plus-fragment-pattern fingerprinting, often after chemical derivatization designed to shift the molecular ion into a more diagnostic, more stable, more easily ionized mass region. Petroleum and flavor/fragrance chemistry both rely on EI-MS libraries built up over decades to instantly classify hydrocarbon mixtures and volatile natural-product components by their characteristic molecular ions and fragmentation fingerprints. In modern proteomics and metabolomics, softer ionization methods (electrospray, MALDI) have largely displaced classical EI for very large or fragile biomolecules, but the conceptual backbone — a single peak whose m/zm/z reveals mass, checked against parity and isotope logic before being trusted — remains identical; those softer methods are natural extensions once the reasoning built here for the molecular ion is secure.

Ask the tutor: How do I use the isotope pattern accompanying the molecular ion peak to figure out how many chlorine, bromine, or sulfur atoms a compound contains?

The physical picture

A mass spectrometer never weighs a molecule directly. It takes a molecule, strips off exactly one electron in the gas phase to make a charged species, accelerates that charged species through a known electric field, and then sorts the resulting ions by their mass-to-charge ratio as they fly (or curve, or oscillate, depending on the analyzer) through vacuum. Whatever the analyzer — magnetic sector, quadrupole, time-of-flight — the fundamental quantity extracted is always

mz\frac{m}{z}

where mm is the ion's mass (in daltons, atomic mass units) and zz is the number of elementary charges it carries. In electron-impact ionization the overwhelming majority of ions are singly charged, z=1z=1, so for practical purposes in this tier,

mz≈m (in daltons).\frac{m}{z} \approx m \text{ (in daltons)}.

This is why chemists speak casually of "the peak at m/z=86m/z = 86" and mean, without further qualification, "an ion of mass 86 daltons."

How the ionization event happens. The sample is vaporized into a high-vacuum ion source (typically 10−6–10−510^{-6}\text{–}10^{-5} torr, so that molecules travel in isolation without colliding). A filament emits electrons that are accelerated through a potential of about 70 volts, giving each electron a kinetic energy of about 70 electron-volts (eV) — roughly 6700 kJ/mol6700\ \text{kJ/mol}, immensely larger than any bond dissociation energy (typical C–C or C–H bonds: 300300–420 kJ/mol420\ \text{kJ/mol}). This 70 eV beam is fired across the ionization chamber, and a molecule that happens to sit in its path is struck. The mechanism of ionization is not a bond-forming/bond-breaking curved-arrow event in the usual organic sense — it is an ejection. A single incident electron transfers enough energy to the molecule to knock one of the molecule's own electrons out of its orbital entirely, ejecting it into the vacuum as a free (low-energy) electron. This is written schematically as

M+e(70 eV)−⟶M+∙+2e(low energy)−\mathrm{M} + e^-_{(\text{70 eV})} \longrightarrow \mathrm{M}^{+\bullet} + 2e^-_{(\text{low energy})}

The molecule M\mathrm{M}, which had all electrons paired, loses one electron and becomes M+∙\mathrm{M}^{+\bullet}: a species bearing both a positive charge (one fewer electron than protons) and an unpaired electron (one electron short of a closed shell). This is a radical cation — simultaneously a radical and a cation, denoted with the dot-plus superscript. It is not the same species as a carbocation formed by heterolysis (which has no unpaired electron), nor a radical formed by homolysis (which has no charge). The molecular ion is chemically unique to this ionization method.

Which electron leaves? By an argument closely related to Koopmans' theorem, the electron most easily removed is the one in the highest-occupied molecular orbital (HOMO), because that is the electron least tightly bound (smallest ionization energy). Qualitatively, for organic molecules the ranking of "easiest to remove" is

lone pair (n)  >  π bond  >  σ bond (C–C)  >  σ bond (C–H).\text{lone pair (n)} \;>\; \pi \text{ bond} \;>\; \sigma \text{ bond (C–C)} \;>\; \sigma \text{ bond (C–H)}.

This ordering explains a huge amount of EI-MS behavior at a glance. An amine or ether ionizes preferentially by removing a nitrogen or oxygen lone-pair electron; the positive charge and radical then sit substantially localized on that heteroatom, resonance-stabilized into the adjacent framework. An alkene or arene ionizes by removing a π electron, leaving the charge/radical delocalized over the π system — which is part of why aromatic and conjugated molecules tend to give strong, long-lived molecular ions. A simple saturated alkane has only σ electrons available, and ionizing a C–C or C–H σ bond gives a much less stabilized radical cation that fragments extensively, often leaving little or no observable M+∙\mathrm{M}^{+\bullet}.

Excess energy and fragmentation. The 70 eV beam energy vastly exceeds the roughly 7–15 eV needed to ionize almost any organic molecule. The leftover energy — many electron-volts — is deposited as vibrational excitation in the newly formed M+∙\mathrm{M}^{+\bullet}. A vibrationally hot radical cation, sitting in a high vacuum with no solvent or collision partner to carry away that energy, has only one way to relax: fall apart. It does so on a timescale of roughly 10−1010^{-10} to 10−610^{-6} seconds inside the source and flight tube, breaking a bond (usually the weakest one, or the one whose cleavage gives the most stable fragment cation) to produce a smaller cation plus a neutral fragment, or occasionally two radicals plus a neutral. These lighter cations are what populate the rest of the spectrum below MM; their systematic interpretation is the subject of fragmentation mechanisms elsewhere. Here, the essential point is binary: some fraction of the M+∙\mathrm{M}^{+\bullet} population survives all the way to the detector without fragmenting, and it is that surviving population that produces the molecular ion peak.

Figure
Electron-impact ionization: a 70 eV electron ejects one HOMO electron from neutral M, producing the radical cation M⁺•
Electron impact ionization M paired e⁻'s e⁻ (70 eV) M +• one unpaired e⁻ net +1 charge 2 e⁻ ejected (low KE) M + e⁻(70 eV) → M⁺• + 2e⁻ HOMO electron lost first: lone pair > π > σ(C–C) > σ(C–H)

Recognizing the molecular ion peak. In a real spectrum, the peak of highest m/zm/z is usually M+∙\mathrm{M}^{+\bullet}, but three complications require care. First, natural isotopes (13C^{13}\mathrm{C}, 2H^2\mathrm{H}, 15N^{15}\mathrm{N}, 18O^{18}\mathrm{O}, and heavier halogen isotopes) put small satellite peaks one or two mass units above the all-light-isotope peak; the true M+∙\mathrm{M}^{+\bullet} is the lowest-mass member of this isotope cluster, not necessarily the tallest peak in the cluster. Second, ion–molecule collisions in a poorly tuned or overloaded source can generate a spurious [M+1]+[\mathrm{M}+1]^+ peak by proton transfer, which must not be mistaken for the true molecular ion. Third — and most important for this tier — the molecular ion itself may be so unstable that it fragments essentially completely, leaving no detectable peak at MM at all; tertiary alcohols and highly branched alkanes are classic offenders. In such cases the chemist must use milder ionization (chemical ionization, CI) to coax a detectable [M+1]+[\mathrm{M}+1]^+ or [M−1]+[\mathrm{M}-1]^+ pseudo-molecular-ion peak, or must infer MM indirectly from a self-consistent fragmentation pattern. The chemical sanity checks for "is this peak really M+∙\mathrm{M}^{+\bullet}?" are: 1. It must be an odd-electron species. Losing a closed-shell neutral fragment (H₂O, CO, C₂H₄, HCl, CH₃•, …) from M+∙\mathrm{M}^{+\bullet} gives another odd-electron or even-electron cation consistent with radical/molecule bookkeeping; a proposed MM peak that cannot lose any chemically sensible neutral fragment to explain the very next peak down is suspect. 2. Reasonable mass losses. The gap between the candidate MM peak and the next peak down should correspond to a plausible neutral loss. Losses of 3–14 mass units (except 12, 13 CH-type oddities) are chemically implausible and usually signal that the candidate peak is not M+∙\mathrm{M}^{+\bullet} but a fragment or noise. 3. The nitrogen rule (derived below) — a parity check that either confirms or rules out a candidate MM instantly.

Figure
A schematic EI mass spectrum: fragment peaks build up below the molecular ion, whose position m/z = M is fixed by isotope-cluster logic
Schematic EI-MS: base peak, fragments, M⁺• relative intensity m/z 29 43 (base) 58 86 = M⁺• 87 (¹³C satellite, ~4.5% of 86) M⁺• is the lowest-mass peak of its isotope cluster — the tallest visible peak overall is usually a stable fragment (base peak).

The core ideas

The molecular ion's mass, read straight off the spectrum, gives the molecular mass:

M=(m/z)M+∙M = (m/z)_{\mathrm{M}^{+\bullet}}

where:

  • MM — the nominal molecular mass of the neutral molecule, in daltons (sum of the most abundant isotope masses: 12C=12^{12}\mathrm{C}=12, 1H=1^1\mathrm{H}=1, 16O=16^{16}\mathrm{O}=16, 14N=14^{14}\mathrm{N}=14, 32S=32^{32}\mathrm{S}=32, 35Cl=35^{35}\mathrm{Cl}=35, etc.)
  • (m/z)M+∙(m/z)_{\mathrm{M}^{+\bullet}} — the mass-to-charge ratio of the lowest-mass peak in the molecular-ion isotope cluster, read directly from the spectrum, with z=1z=1 assumed for EI.

Reading: because ionization only removes an electron of negligible mass (me≈0.00055 um_e \approx 0.00055\ \mathrm{u}, invisible at nominal-mass resolution), the mass of M+∙\mathrm{M}^{+\bullet} equals the mass of the neutral M\mathrm{M} to within the precision used at this level. The molecular ion peak is therefore a direct readout of molecular weight — no calibration curve, no comparison standard needed, just the position of one peak. The second core relationship is the nitrogen rule, a parity statement:

M is odd  ⟺  the number of nitrogen atoms in the molecule is odd.M \text{ is odd} \iff \text{the number of nitrogen atoms in the molecule is odd.}

Equivalently, MM even   ⟺  \iff nitrogen count even (including zero). Reading: this is not an empirical curiosity but a direct consequence of nitrogen's valence arithmetic, derived rigorously below.

Derivation 1 — why m/zm/z of the molecular ion gives molecular mass

Goal: show explicitly that the mass measured for M+∙\mathrm{M}^{+\bullet} differs from the neutral molecular mass MM by an amount too small to matter at the resolution used to read nominal masses, and quantify that difference for a real molecule.

Step 1 — mass balance on ionization. The ionization event is

M+e(fast)−⟶M+∙+2e(slow)−.\mathrm{M} + e^-_{(\text{fast})} \longrightarrow \mathrm{M}^{+\bullet} + 2e^-_{(\text{slow})}.

Conservation of mass (nonrelativistic; kinetic energies here are far too small to invoke E=mc2E=mc^2 corrections) requires

m(M)+m(e−)=m(M+∙)+2 m(e−)m(\mathrm{M}) + m(e^-) = m(\mathrm{M}^{+\bullet}) + 2\,m(e^-)

so that

m(M+∙)=m(M)−m(e−).m(\mathrm{M}^{+\bullet}) = m(\mathrm{M}) - m(e^-).

Step 2 — size of the correction. The electron mass is

m(e−)=5.486×10−4 u.m(e^-) = 5.486 \times 10^{-4}\ \mathrm{u}.

For essentially any organic molecule of interest (mass tens to thousands of daltons), this is a correction of order 10−410^{-4} to 10−610^{-6} relative to MM — utterly negligible at the nominal (integer) mass resolution used throughout this tier, and still negligible at typical unit-resolution or even most high-resolution work at the level of a few parts per million unless one is doing exact-mass formula assignment (a job for high-resolution MS, not treated here).

Step 3 — conclude the working equation. To the precision relevant for reading integer m/zm/z values off a spectrum,

m(M+∙)≈m(M)=M.m(\mathrm{M}^{+\bullet}) \approx m(\mathrm{M}) = M.

Hence the m/zm/z value at which the molecular ion peak sits is the molecular weight of the compound. This is why "find MM" and "find the molecular ion peak" are, for practical purposes, the same instruction.

Step 4 — worked numeric check with an asymmetric, real molecule. Take butan-2-one (methyl ethyl ketone), CH3COCH2CH3\mathrm{CH_3COCH_2CH_3}, molecular formula C4H8O\mathrm{C_4H_8O}. Using nominal atomic masses C=12.000\mathrm{C}=12.000, H=1.008\mathrm{H}=1.008, O=15.999\mathrm{O}=15.999 (or nominal integers 12,1,1612,1,16 for the mass a low-resolution EI spectrum reports):

M=4(12)+8(1)+1(16)=48+8+16=72.M = 4(12) + 8(1) + 1(16) = 48 + 8 + 16 = 72.

An EI spectrum of butan-2-one indeed shows its molecular ion at m/z=72m/z = 72. Correcting for the ejected electron,

m(M+∙)=72.000 u−0.00055 u=71.99945 u,m(\mathrm{M}^{+\bullet}) = 72.000\ \mathrm{u} - 0.00055\ \mathrm{u} = 71.99945\ \mathrm{u},

a difference of about six parts in a hundred thousand — invisible on any unit-resolution instrument and irrelevant to the integer value 7272 that the chemist actually reads and uses.

Step 5 — limiting case. As the molecule gets arbitrarily large (M→∞M \to \infty, e.g. a small protein at M∼15,000M \sim 15{,}000), the absolute correction from the missing electron stays fixed at ∼0.00055\sim 0.00055 u while the relative error shrinks further, confirming that the neglect of electron mass is always safe at nominal-mass resolution and becomes progressively safer, not less safe, for larger molecules.

Derivation 2 — the nitrogen rule

Goal: derive, from valence and mass-parity bookkeeping alone, why the parity of the nitrogen count in a neutral organic molecule fixes the parity of its nominal molecular mass.

Step 1 — set up the counting problem. Consider a neutral, closed-shell organic molecule built from atoms of C, H, N, O, S, and halogens (X = F, Cl, Br, I) — the common elements of undergraduate organic structure work. Each atom contributes an integer nominal mass and has a fixed valence (number of bonds it forms, ignoring charge-bearing exceptions for the moment):

Elementtypical valencenominal mass
H11
C412
N314
O216
S232
F, Cl, Br, I119, 35, 79, 127

Notice the pattern that drives the whole rule: for every element except nitrogen, valence and nominal mass have the same parity — H (valence 1, mass 1: both odd), C (valence 4, mass 12: both even), O (valence 2, mass 16: both even), S (valence 2, mass 32: both even), halogens (valence 1, mass odd: both odd). Nitrogen is the exception: valence 3 (odd) but mass 14 (even) — an odd valence paired with an even mass. This single mismatch is the entire origin of the nitrogen rule.

Step 2 — total mass versus total valence, summed over the whole molecule. For a valid closed-shell neutral molecule with cc carbons, hh hydrogens, nn nitrogens, oo oxygens, ss sulfurs, and xx halogens, the nominal mass is

M=12c+h+14n+16o+32s+(halogen masses).M = 12c + h + 14n + 16o + 32s + (\text{halogen masses}).

Every coefficient except the ones multiplying hh and nn is even (12, 16, 32, and each halogen mass — 19, 35, 79, 127 — is odd, matching that halogens are odd-valence too; but each halogen appears alongside exactly one bond, so we track halogens together with hh below). Group the odd-valence atoms (H, N, and monovalent halogens X) as the ones whose parity needs tracking, since even-valence atoms (C, O, S) always contribute an even mass regardless of how many there are:

M≡h+14n+(odd atomic masses of halogens)(mod2).M \equiv h + 14n + (\text{odd atomic masses of halogens}) \pmod 2.

Since 1414 is even, 14n≡0(mod2)14n \equiv 0 \pmod 2 regardless of nn — mass-wise nitrogen looks "invisible" mod 2. But halogens are odd in mass, so each halogen contributes 1(mod2)1 \pmod 2; write xx for the total halogen count. So

M≡h+x(mod2).M \equiv h + x \pmod 2.

Step 3 — bring in the valence (degree) sum rule. In any neutral, fully-bonded organic structure (no radicals, no formal charges), the sum of all valences over all atoms must be even, because every bond is shared between two atoms and contributes 22 to the total valence count (one unit to each partner):

∑atoms(valence)=2×(number of bonds)≡0(mod2).\sum_{\text{atoms}} (\text{valence}) = 2 \times (\text{number of bonds}) \equiv 0 \pmod 2.

Write out that sum using the valences from the table: each C contributes 4 (even), each O contributes 2 (even), each S contributes 2 (even) — all irrelevant mod 2 — while each H contributes 1, each halogen contributes 1, and each N contributes 3 (odd). So

0≡h+x+3n(mod2)≡h+x+n(mod2)0 \equiv h + x + 3n \pmod 2 \equiv h + x + n \pmod 2

(since 3n≡n(mod2)3n \equiv n \pmod 2). Rearranged,

h+x≡n(mod2).h + x \equiv n \pmod 2.

Step 4 — combine Steps 2 and 3. Step 2 gave M≡h+x(mod2)M \equiv h+x \pmod 2; Step 3 gave h+x≡n(mod2)h + x \equiv n \pmod 2. Chaining these,

M≡n(mod2).M \equiv n \pmod 2.

This is the nitrogen rule in its entirety: the nominal molecular mass has the same parity as the number of nitrogen atoms. If nn is even (0, 2, 4, …), MM is even; if nn is odd (1, 3, 5, …), MM is odd.

Step 5 — why this is really a "hidden hydrogen" bookkeeping trick in disguise. The clean way to see it physically: every bond you could imaginatively "cut" to isolate one atom's valence requires a partner electron/atom on the other end, and only odd-valence atoms (H, N, halogens) can appear an "un-paired" number of times without violating the closed-shell requirement — but N does so while contributing an even mass number, silently absorbing an odd count of bonding partners (H atoms, typically, since amines and amides load extra H's around N) without disturbing the mass parity the way a genuinely odd-mass odd-valence atom (H, halogen) would. This is exactly the "nitrogen anomaly:" the only common element whose valence parity and mass parity disagree.

Step 6 — worked numeric check with an asymmetric molecule containing more than one nitrogen and a halogen, to stress-test the rule. Take procaine hydrochloride's free base, procaine, C13H20N2O2\mathrm{C_{13}H_{20}N_2O_2} (a local anesthetic; two nitrogens — one aromatic amine, one tertiary amine in the side chain). Compute:

M=13(12)+20(1)+2(14)+2(16)=156+20+28+32=236.M = 13(12) + 20(1) + 2(14) + 2(16) = 156 + 20 + 28 + 32 = 236.

M=236M = 236 is even, and n=2n=2 is even — consistent with the rule. Now perturb it to a genuinely asymmetric odd-nitrogen, halogen-bearing test case: chlorpheniramine, C16H19ClN2\mathrm{C_{16}H_{19}ClN_2} — wait, that has two nitrogens (even), so instead take a single-nitrogen halogenated amine, 4-chloroaniline, C6H6ClN\mathrm{C_6H_6ClN}:

M=6(12)+6(1)+35+14=72+6+35+14=127.M = 6(12) + 6(1) + 35 + 14 = 72 + 6 + 35 + 14 = 127.

M=127M = 127 is odd, and n=1n=1 is odd — again consistent. As a genuinely different-flavored check with three nitrogens, take melamine, C3H6N6\mathrm{C_3H_6N_6}:

M=3(12)+6(1)+6(14)=36+6+84=126,M = 3(12) + 6(1) + 6(14) = 36 + 6 + 84 = 126,

even, with n=6n=6 (even) — consistent. And with one nitrogen and no halogen, pyridine, C5H5N\mathrm{C_5H_5N}:

M=5(12)+5(1)+14=60+5+14=79,M = 5(12) + 5(1) + 14 = 60 + 5 + 14 = 79,

odd, with n=1n=1 (odd) — consistent. Every one of these independent, structurally unrelated, asymmetric test molecules obeys M≡n(mod2)M \equiv n \pmod 2 exactly as Step 4 predicts.

Step 7 — limiting case. Set n=0n=0 (no nitrogen at all): the rule then says MM must be even for any ordinary CHO(S)(halogen) organic molecule with no nitrogen — check against glucose, C6H12O6\mathrm{C_6H_{12}O_6}: M=72+12+96=180M = 72+12+96=180, even, consistent, since n=0n=0 is even. This is the "trivial" limiting case built into the rule and it recovers a fact organic chemists use constantly without naming it: ordinary hydrocarbons, alcohols, ketones, ethers, esters, and sugars — anything with zero nitrogen — always have even nominal molecular weight.

Worked examples

Example 1 — Foundational: reading M and a formula candidate from a clean EI spectrum. An EI-MS of a neutral, colorless liquid shows its highest chemically sensible peak at m/z=88m/z = 88, with a very weak, chemically consistent [M+1][\mathrm{M}+1] satellite at m/z=89m/z=89 (about 4–5% the height of the 8888 peak — consistent with natural 13C^{13}\mathrm{C} abundance for a handful of carbons, not with a distinct compound). We assign

M=88.M = 88.

By the nitrogen rule, M=88M=88 is even, so this compound contains an even number of nitrogens — most simply, zero. Suppose independent evidence (IR: strong C=O stretch near 1735 cm⁻¹, no N–H or O–H stretch; a companion technique) suggests an ester. A reasonable formula with M=88M=88 and no nitrogen is C4H8O2\mathrm{C_4H_8O_2}:

M=4(12)+8(1)+2(16)=48+8+32=88✓M = 4(12) + 8(1) + 2(16) = 48+8+32 = 88 \checkmark

consistent with, e.g., ethyl acetate or methyl propanoate — both common C4H8O2C_4H_8O_2 esters, distinguished later by fragmentation patterns, not by MM alone. The key skill exercised here is entirely arithmetic-plus-parity: one peak position, one parity check, and a short list of candidate formulas collapses dramatically.

Example 2 — Applied: catching a deceptively small molecular ion peak in a real drug fragment. An EI spectrum of a suspected metabolite shows a tall base peak at m/z=58m/z=58, a moderate peak at m/z=91m/z=91, and only a very faint peak at m/z=135m/z=135, so faint a careless reader might miss it and instead (wrongly) call 9191 the molecular ion. Applying the sanity checks: is the gap from 135135 down to 9191 chemically plausible? 135−91=44135-91 = 44, a plausible loss of CO2\mathrm{CO_2} or of C3H8O\mathrm{C_3H_8O}-type neutral, or — more diagnostically — is the gap down to the base peak plausible? 135−58=77135 - 58 = 77, not an obviously clean single neutral loss, but 91−58=3391-58=33 is unusual too, suggesting 9191 is itself already a fragment, not MM. Apply the nitrogen rule as the tie-breaker: is 135135 or 9191 the more sensible candidate for MM? If we hypothesize the molecule is an amine, expect an odd MM if it carries one nitrogen. 135135 is odd — consistent with one nitrogen. 9191 is also odd, so parity alone can't fully discriminate, but 9191 corresponds suspiciously exactly to the mass of the extremely common, extremely stable tropylium cation C7H7+\mathrm{C_7H_7^+} (7×12+7×1=84+7=917\times12 + 7\times1 = 84+7=91), a famous fragmentation product of essentially any compound with a benzylic C–C bond (arising from loss of a radical to give an aromatic, 6π-electron, fully conjugated cation — a fragmentation covered in full elsewhere but worth flagging here because its characteristic mass, 91, is one of the most notorious "fake molecular ion" traps in the whole subject). Recognizing 9191 as tropylium, not MM, forces the correct assignment

M=135,M = 135,

odd, one nitrogen, consistent with an aromatic amine bearing a benzylic substituent — for instance a molecule like NN-methyl-α\alpha-methylbenzylamine-type fragment (C9H13N\mathrm{C_9H_{13}N}: 9(12)+13(1)+14=108+13+14=135✓9(12)+13(1)+14 = 108+13+14=135\checkmark). This example is deliberately built to show why "highest visible peak" and "true M+∙\mathrm{M}^{+\bullet}" are not automatically the same peak, and why chemical reasoning about both neutral-loss plausibility and nitrogen parity must be combined, not used in isolation.

Example 3 — Exam/competition level: combining the nitrogen rule with a formula search under an isotope constraint. A compound of unknown structure shows M+∙\mathrm{M}^{+\bullet} at m/z=151m/z = 151 (confirmed as the true molecular ion by a clean, chemically sensible loss of 15 mass units — a methyl radical — down to a strong peak at m/z=136m/z=136, i.e. M−CH3\mathrm{M-CH_3}, a classic and diagnostic loss). Elemental analysis independently establishes the empirical composition contains carbon, hydrogen, one nitrogen, and one oxygen, with no halogens or sulfur. Determine the molecular formula. Step 1 — apply the nitrogen rule as a consistency check first. M=151M=151 is odd. One nitrogen (odd count) is exactly what makes MM odd, per M≡n(mod2)M \equiv n \pmod 2 with n=1n=1. This is consistent and does not by itself pin the formula, but it rules out any candidate formula with an even nitrogen count (e.g., accidentally proposing 0 or 2 N would immediately fail the parity check and can be discarded without further arithmetic). Step 2 — set up the mass equation. Let the formula be CcHhN1O1\mathrm{C_cH_hN_1O_1} (one N, one O, fixed by the elemental analysis):

151=12c+h+14+16=12c+h+30151 = 12c + h + 14 + 16 = 12c + h + 30
12c+h=121.12c + h = 121.

Step 3 — apply the degree-of-unsaturation / valence constraint to narrow (c,h)(c,h). For a molecule CcHhN1O1\mathrm{C_cH_hN_1O_1}, the maximum possible hydrogen count (fully saturated, acyclic) is given by the standard valence formula

hmax⁡=2c+2+n=2c+3h_{\max} = 2c + 2 + n = 2c+3

(the +n+n correction because a trivalent N can carry one extra H relative to a tetravalent-C skeleton count; oxygen, being divalent, doesn't change the H count). We need h≤2c+3h \le 2c+3 and h≥h\ge some small positive number, and 12c+h=12112c+h=121 with h>0h>0 forces

c≤⌊121−112⌋=10,c≥⌈121−(2c+3)1⌉ solved jointly with 12c+h=121.c \le \left\lfloor \frac{121-1}{12}\right\rfloor = 10, \qquad c \ge \left\lceil \frac{121-(2c+3)}{1}\right\rceil \text{ solved jointly with } 12c+h=121.

Try c=9c=9: h=121−108=13h = 121-108=13; check hmax⁡=2(9)+3=21≥13h_{\max}=2(9)+3=21 \ge 13 ✓, and the degree of unsaturation

DoU=2c+2+n−h2=18+2+1−132=82=4\mathrm{DoU} = \frac{2c+2+n-h}{2} = \frac{18+2+1-13}{2} = \frac{8}{2}=4

is a whole, non-negative number — exactly right for, e.g., one aromatic ring (4 degrees: ring + 3 π bonds) which is also completely consistent with a facile loss of CH3\mathrm{CH_3} (methyl loss from an aromatic methyl ketone-oxime or a methoxy/methyl-substituted aromatic amine is common and stabilized by the resulting aromatic cation). So the formula C9H13NO\mathrm{C_9H_{13}NO} is fully consistent:

M=9(12)+13(1)+14+16=108+13+14+16=151✓M = 9(12)+13(1)+14+16 = 108+13+14+16 = 151 \checkmark

Step 4 — sanity-check alternative cc values are rejected. Try c=10c=10: h=121−120=1h=121-120=1, giving DoU=20+2+1−12=11\mathrm{DoU}=\frac{20+2+1-1}{2}=11 for only 10 carbons and 1 nitrogen — implausibly unsaturation-dense (would require more π-bonds/rings than there are heavy atoms to support sensibly) and is discarded as chemically unreasonable at this level. Try c=8c=8: h=121−96=25>hmax⁡=2(8)+3=19h=121-96=25 > h_{\max}=2(8)+3=19 — violates the valence bound outright, impossible. So c=9c=9, h=13h=13 is the unique sensible solution, giving C9H13NO\mathrm{C_9H_{13}NO}, DoU=4\mathrm{DoU}=4 — a formula matching, for instance, a methoxy-substituted phenethylamine-type structure, whose facile loss of a methyl radical (from the aromatic methoxy group, stabilizing the resulting oxocarbenium-like aromatic cation) explains the clean 151→136151\to136 transition observed experimentally.

Limiting cases, scope & common traps

SituationWhat happens to M+∙\mathrm{M}^{+\bullet}Correct handling
Aromatic, conjugated, or heteroatom-lone-pair-rich moleculeStrong, often base-peak-level M+∙\mathrm{M}^{+\bullet}Read MM directly with confidence
Highly branched alkane / tertiary alcoholM+∙\mathrm{M}^{+\bullet} very weak or absent (fast fragmentation of unstable radical cation)Use chemical ionization (CI) for [M+1]+[\mathrm{M}+1]^+; or infer MM from self-consistent fragment ladder
Overloaded/dirty ion sourceSpurious [M+1]+[\mathrm{M}+1]^+ from ion–molecule proton transferDon't mistake for true M+∙\mathrm{M}^{+\bullet}; check isotope ratios and reduce sample pressure
Natural isotopes present (13^{13}C, 37^{37}Cl, 81^{81}Br, etc.)Extra peaks 1–2, or +2, mass units above MMTrue M+∙\mathrm{M}^{+\bullet} = lowest-mass peak of the cluster, not the tallest
Even number of nitrogens (0, 2, 4, …)—MM must be even; odd candidate MM is impossible for this nitrogen count
Odd number of nitrogens (1, 3, 5, …)—MM must be odd; even candidate MM is impossible for this nitrogen count
Nitrogen rule applied to an ion, not the neutral moleculeRule fails (it is derived for closed-shell neutrals)Never apply directly to fragment cations, which are missing electrons/atoms and can break the valence-sum argument

The chemist behind it

Origins · 1 minFrancis William Aston and how this was discovered
FW
Francis William Aston
1877–1945 · Cambridge, Cavendish Laboratory, early 20th century

Aston built the first high-resolution mass spectrograph and used it to demonstrate, atom by atom, that elements are mixtures of isotopes of slightly different mass — the physical basis for everything a modern EI spectrum's isotope satellites report. His whole number rule, that isotopic masses are close to (but not exactly) integers relative to oxygen-16, was itself a precursor observation to the very "nominal mass" bookkeeping used throughout this article; understanding why masses cluster near integers, and why the small deviations matter for high-resolution formula assignment, traces directly back to his instrument-building and careful measurement.

Aston's mass spectrograph, built at the Cavendish Laboratory under J. J. Thomson's influence (Thomson had already shown that "positive rays" — early ion beams — could be deflected by electric and magnetic fields to sort by charge-to-mass ratio), used combined electric and magnetic sector fields to focus ions of the same m/zm/z regardless of their initial velocity spread — the key instrumental innovation ("velocity focusing") that gave dramatically sharper mass resolution than Thomson's parabola method. With it, Aston identified the isotopes of neon (²⁰Ne and ²²Ne, resolving a decades-old puzzle about neon's non-integer average atomic weight), then went on to characterize the isotopic composition of most of the periodic table, work recognized with the 1922 Nobel Prize in Chemistry. The organic chemist's EI-MS instrument, though built for very different molecules and questions than Aston's atomic-mass work, is a direct descendant of his sector-field, velocity-focusing design philosophy — and the entire practice of trusting an m/zm/z peak position as a faithful readout of mass rests on the resolving power his instruments first achieved.

Origins · 1 minhow this was discovered
History
- 1897 — J. J. Thomson discovers the electron and develops early charged-particle deflection methods.
- 1912–1919 — Thomson's "positive ray" parabola apparatus reveals that neon gives two distinct mass traces, hinting at isotopes.
- 1919 — Francis Aston builds the first true mass spectrograph with velocity focusing, resolving neon's isotopes ²⁰Ne and ²²Ne cleanly.
- 1920s–1930s — Aston systematically measures isotopic masses across the periodic table; formulates the whole-number rule.
- 1940s–1960s — Electron-impact ion sources adapted specifically for organic molecules; EI-MS becomes a routine structure-elucidation tool alongside IR and early NMR.
Why does electron-impact ionization use exactly around 70 eV, and would a different energy change the molecular ion?

70 eV is a practical compromise, not a fundamental constant. Ionization energies for organic molecules are typically 7–15 eV, so 70 eV guarantees essentially every molecule that enters the beam's path gets ionized, giving high, reproducible sensitivity. It also happens to sit on a broad plateau in the ionization efficiency curve, where small voltage fluctuations in the instrument barely change the fragmentation pattern — which is why 70 eV EI spectra are so reproducible across different instruments and laboratories, and why enormous shared spectral libraries work at all. Lower energies (10–20 eV) do produce less fragmentation and often a stronger molecular ion peak, but at the cost of lower overall ionization efficiency and less reproducible, less library-comparable spectra, so 70 eV remains the de facto standard for routine EI work.

Is the molecular ion peak always present in an EI spectrum?

No. Whether M+∙\mathrm{M}^{+\bullet} survives to the detector depends on how quickly the excited radical cation fragments relative to its transit time through the instrument. Aromatic rings, conjugated π systems, and heteroatom lone pairs stabilize the radical cation (by delocalizing both the positive charge and the unpaired electron), giving strong, often dominant molecular ion peaks. Highly branched alkanes, tertiary alcohols, and some ethers ionize into radical cations that fragment almost instantly, sometimes leaving no detectable M+∙\mathrm{M}^{+\bullet} peak at all. In those cases, chemists switch to a gentler ionization method such as chemical ionization (CI), which transfers far less excess energy and reliably gives an [M+1]+[\mathrm{M}+1]^+ or [M−1]+[\mathrm{M}-1]^+ pseudo-molecular ion instead.

How is the nitrogen rule different from — and related to — the ring-plus-double-bond (degree of unsaturation) formula?

Both come from the same underlying valence-sum bookkeeping, but they answer different questions. The nitrogen rule is a parity (mod-2) statement purely about mass, telling you whether MM is odd or even from the nitrogen count alone. The degree-of-unsaturation formula, DoU=(2c+2+n−h)/2\mathrm{DoU} = (2c+2+n-h)/2, is a full count of rings-plus-π-bonds, requiring the complete formula (all of cc, hh, nn) rather than just a parity. In practice a chemist often uses the nitrogen rule first, as an extremely fast sanity check on a proposed molecular formula, and only then works out the full degree-of-unsaturation to test whether the proposed carbon–hydrogen count is structurally sensible.

Can the nitrogen rule be fooled by an odd number of halogens?

No, and this is exactly why the derivation tracks halogens explicitly. Halogens are monovalent with odd nominal mass (F=19, Cl=35, Br=79, I=127), so they behave, mass-parity-wise, exactly like hydrogen: both valence and mass are odd, so they never disturb the M≡n(mod2)M \equiv n \pmod 2 relationship regardless of how many halogens are present. You can freely add or remove halogens (or hydrogens) from a molecule without breaking the nitrogen rule, precisely because their valence parity and mass parity always agree — it is only nitrogen's parity mismatch (odd valence, even mass) that has any effect on the overall parity relationship.

Why is m/z used instead of just "m" if almost all EI ions are singly charged?

The notation m/zm/z is kept general because not every ionization method or every ion produced is singly charged. Even within EI, doubly charged ions (z=2z=2) occasionally appear, especially for large, easily doubly-ionized aromatic systems, and they show up at half their true mass — a classic trap if you forget to consider z≠1z\neq1. More importantly, other ionization techniques used alongside EI in the broader toolkit of mass spectrometry (electrospray ionization, for instance) routinely produce multiply charged ions for large biomolecules, so the general m/zm/z axis label is the correct universal convention even though, for the specific case of EI-MS of small organic molecules covered here, z=1z=1 is overwhelmingly the practical default.

Does electron-impact ionization ever add mass to the molecule instead of removing an electron?

Not in classical EI — the defining act of EI is electron removal, producing M+∙\mathrm{M}^{+\bullet} at (essentially) the same mass as the neutral molecule. Techniques that add mass, such as protonation to form [M+H]+[\mathrm{M}+\mathrm{H}]^+, belong to a different ionization family (chemical ionization, electrospray ionization), where the ionizing species is a reagent gas or solvent adduct rather than a bare high-energy electron. It is important not to conflate the two: in EI, the molecular ion's m/zm/z equals the neutral mass to extremely high precision (differing only by one electron mass); in CI or ESI, the observed pseudo-molecular ion is systematically shifted by the mass of whatever is added or removed (commonly ±1\pm 1 for a proton), and that shift must be subtracted before quoting MM.

If I only have the molecular formula, can I predict the intensity of the molecular ion peak without running the experiment?

Only qualitatively, via the HOMO-based reasoning developed here: molecules with easily ionized, well-stabilized HOMOs (aromatic rings, extended conjugation, lone pairs on nitrogen or sulfur especially) tend to give strong, long-lived molecular ions, while molecules whose ionization necessarily removes a strained or poorly-stabilized σ electron (highly branched saturated alkanes, some ethers, tertiary alcohols prone to fast α-cleavage) tend to give weak or absent molecular ion peaks. Precise quantitative intensity prediction, however, requires either experimental measurement or detailed computational modeling of the radical cation's potential energy surface and unimolecular fragmentation rates — well beyond formula-level reasoning alone.

Before this