Skip to content

Chemistry · Ch 3 — Periodic Classification of Elements

Atomic radius

3.5.1

Atomic radius

Definition. The atomic radius of an atom is the distance from the centre of its nucleus to the outermost shell that contains a valence electron (Figure 3.1a).

Why it can't be measured directly. An isolated, non-bonded atom's electron cloud has no sharp boundary, so its radius cannot be measured directly. In practice, except for the noble gases (which use a van der Waals radius instead, since they do not form ordinary bonds), atomic radius is reported as either a covalent radius or a metallic radius, depending on the type of bonding the atom actually engages in.

Covalent radius. This is one-half of the internuclear distance between two identical atoms joined by a single covalent bond (Figure 3.1b), a distance that can be measured experimentally by X-ray diffraction. Worked example: the internuclear distance in Cl2 is 1.98 Angstrom (Figure 3.1c), so dCl−Cl=rCl+rCl=2 rCld_{Cl-Cl} = r_{Cl} + r_{Cl} = 2\,r_{Cl}, giving rCl=1.98/2=0.99r_{Cl} = 1.98 / 2 = 0.99 Angstrom. Because forming a covalent bond involves the overlap of atomic orbitals, it pulls the two nuclei slightly closer together than their "true" atomic radii would suggest -- so the covalent radius is always a little shorter than the actual atomic radius.

For a hetero-nuclear diatomic molecule A-B, the individual covalent radii can still be extracted from the measured internuclear distance dA−Bd_{A-B} using the Schomaker-Stevenson relation:

dA−B=rA+rB−0.09 (χA−χB)d_{A-B} = r_A + r_B - 0.09\,(\chi_A - \chi_B)

where χA\chi_A and χB\chi_B are the Pauling electronegativities of A and B (with χA>χB\chi_A > \chi_B by convention), and radii are in Angstrom. Worked example: for H-Cl, dH−Cl=1.28d_{H-Cl} = 1.28 Angstrom, rCl=0.99r_{Cl} = 0.99 Angstrom, χCl=3\chi_{Cl} = 3, χH=2.1\chi_H = 2.1:

1.28=rH+0.99−0.09(3−2.1)=rH+0.99−0.081=rH+0.9091.28 = r_H + 0.99 - 0.09(3 - 2.1) = r_H + 0.99 - 0.081 = r_H + 0.909

∴rH=1.28−0.909=0.371 Angstrom\therefore r_H = 1.28 - 0.909 = 0.371 \text{ Angstrom}

Metallic radius. This is one-half of the distance between two adjacent metal atoms in a closely packed metallic crystal lattice. Worked example: in solid copper the distance between adjacent Cu atoms is 2.56 Angstrom, so the metallic radius of copper is 2.56/2=1.282.56/2 = 1.28 Angstrom. (Metallic radius can also be worked out from a crystal's unit-cell length -- the detailed procedure is covered in the Class XII solid state unit.)

Trend across a period: atomic radius decreases. Moving left to right, each successive element adds its new valence electron to the same shell while simultaneously adding a proton to the nucleus. The growing nuclear charge pulls the (same-shell) valence electrons in more tightly, so atomic radius shrinks steadily across a period.

Effective nuclear charge and Slater's rules. Electrons in inner shells repel the valence electrons even as the nucleus attracts them, partly cancelling the nucleus's pull -- this partial cancellation is the shielding (screening) effect, and the net attractive charge actually felt by a valence electron is the effective nuclear charge, Zeff=Z−SZ_{eff} = Z - S, where SS is the screening constant. Slater's rules estimate SS in four steps:

  1. Write the atom's electron configuration and regroup it as (1s)(2s,2p)(3s,3p)(3d)(4s,4p)(4d)(4f)(5s,5p)…(1s)(2s,2p)(3s,3p)(3d)(4s,4p)(4d)(4f)(5s,5p)\ldots
  2. Locate the group containing the electron of interest. Any electron in a group to the right of this (higher in the list) contributes nothing to shielding it. Every other electron within the same group contributes 0.35 to SS (0.30 if the electron of interest is a 1s electron).
  3. For an electron of interest that is an s or p electron: each electron one group inward, (n−1)(n-1), contributes 0.85; each electron two or more groups inward, (n−2)(n-2) and beyond, contributes the full 1.00. For an electron of interest that is a d or f electron: every electron in any group to its left contributes the full 1.00 (Table 3.12).
  4. Sum all these contributions to get SS.

Worked example (scandium, Z = 21, configuration 1s2 2s2 2p6 3s2 3p6 4s2 3d11s^2\,2s^2\,2p^6\,3s^2\,3p^6\,4s^2\,3d^1, regrouped as (1s)2(2s,2p)8(3s,3p)8(3d)1(4s)2(1s)^2(2s,2p)^8(3s,3p)^8(3d)^1(4s)^2):

Effective nuclear charge on the 4s electron: the (4s) group itself contributes 1×0.35=0.351 \times 0.35 = 0.35 (one other 4s electron); the (n−1)(n-1) group (3s,3p,3d)(3s,3p,3d) has 9 electrons contributing 9×0.85=7.659 \times 0.85 = 7.65; the (n−2)(n-2) and lower groups (1s,2s,2p)(1s,2s,2p) have 10 electrons contributing 10×1.00=10.0010 \times 1.00 = 10.00. S=0.35+7.65+10.00=18.00S = 0.35 + 7.65 + 10.00 = 18.00, so Zeff=21−18=3Z_{eff} = 21 - 18 = 3. …

Figure 3.1Atomic radius, and atomic vs covalent radius

What this figure shows. Three small companion diagrams. (a) A single atom drawn as a circle with its radius r marked from the nucleus at the centre out to the edge of the electron cloud. (b) Two identical bonded atoms shown touching, with the internuclear distance d marked as the sum of the two atomic/covalent radii r + r. (c) The specific case of the Cl2 molecule: two chlorine atoms with the measured internuclear (covalent) distance of 1.98 Angstrom marked between their nuclei, illustrating how halving this experimental bond length gives the …

Table 3.12Shielding effect from inner shell electrons (Slater's rules)
Electron group (relative to electron of interest)If electron of interest is s or pIf electron of interest is d or f
Same group (n)0.35 (0.30 for a 1s electron)0.35
One group inward (n-1)0.851.00
Table 3.13Atomic (covalent) radius of second period elements
ElementEffective nuclear charge (Zeff)Covalent radius (pm)
3Li1.30152
4Be1.95111
5B2.6089
6C3.2577
7N3.9074
8O4.5566
9F5.2064
Table 3.14Variation of covalent radius of group 1 elements
ElementOutermost shell (n)Covalent radius (Angstrom)
LiL (n=2)1.34
NaM (n=3)1.54
KN (n=4)1.96