Atomic radius

The atomic radius of a chemical element is a measure of the size of its atoms, usually the mean or typical distance from the nucleus to the boundary of the surrounding cloud of electrons. Since the boundary is not a well-defined physical entity, there are various non-equivalent definitions of atomic radius.

Depending on the definition, the term may apply only to isolated atoms, or also to atoms in condensed matter, covalently bound in molecules, or in ionized and excited states; and its value may be obtained through experimental measurements, or computed from theoretical models. Under some definitions, the value of the radius may depend on the atom's state and context.

The concept is difficult to define because the electrons do not have definite orbits, or sharply defined ranges. Rather, their positions must be described as probability distributions that taper off gradually as one moves away from the nucleus, without a sharp cutoff. Moreover, in condensed matter and molecules, the electron clouds of the atoms usually overlap to some extent, and some of the electrons may roam over a large region encompassing two or more atoms.

Despite these conceptual difficulties, under most definitions the radii of isolated neutral atoms range between 30 and 300 pm (trillionths of a meter), or between 0.3 and 3 angstroms. Therefore, the radius of an atom is more than 10,000 times the radius of its nucleus (1–10 fm), and less than 1/1000 of the wavelength of visible light (400–700 nm).

, CH₃CH₂OH. Each atom is modeled by a sphere with the element's Van der Waals radius.]] For many purposes, atoms can be modeled as spheres. This is only a crude approximation, but it can provide quantitative explanations and predictions for many phenomena, such as the density of liquids and solids, the diffusion of fluids through molecular sieves, the arrangement of atoms and ions in crystals, and the size and shape of molecules.

Atomic radii vary in a predictable and explicable manner across the periodic table. For instance, the radii generally decrease along each period (row) of the table, from the alkali metals to the noble gases; and increase down each group (column). The radius increases sharply between the noble gas at the end of each period and the alkali metal at the beginning of the next period. These trends of the atomic radii (and of various other chemical and physical properties of the elements) can be explained by the electron shell theory of the atom; they provided important evidence for the development and confirmation of quantum theory.

History

In 1920, shortly after it had become possible to determine the sizes of atoms using X-ray crystallography, it was suggested that all atoms of the same element have the same radii. However, in 1923, when more crystal data had become available, it was found that an atom does not have just one size. For example, the size of lithium atoms is different in lithium metal than in LiCl.

Definitions

Widely used definitions of atomic radius include:

Van der Waals radius: in principle, half the minimum distance between the nuclei of two atoms of the element that are not bound to the same molecule.

Ionic radius: the nominal radius of the ions of an element in a specific ionization state, deduced from the spacing of atomic nuclei in crystalline salts that include that ion. In principle, the spacing between two adjacent oppositely charged ions (the length of the ionic bond between them) should equal the sum of their ionic radii. It is only applicable to atoms and ions with a single electron, such as hydrogen, singly ionized helium, and positronium. Although the model itself is now obsolete, the Bohr radius for the hydrogen atom is still regarded as an important physical constant.

Empirically measured atomic radii

The following table shows empirically measured covalent radii for the elements, as published by J. C. Slater in 1964. The values are in picometers (pm), with an accuracy of about 5 pm. The shade of the box ranges from red to yellow as the radius increases; gray indicates lack of data.

{| wikitable WIDTH="80%" style="text-align:center" | Group (vertical) | 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | 13 | 14 | 15 | 16 | 17 | 18 |- align="CENTER" | Period (horizontal) | colspan=19 | |- align="CENTER" | 1 | bgcolor="#ff1900" | H25 | colspan=16 | | bgcolor="#bbbbbb" | He  |- align="CENTER" | 2 | bgcolor="#ff9100" | Li145 | bgcolor="#ff6900" | Be105 | colspan=10 | | bgcolor="#ff5500" | B85 | bgcolor="#ff4600" | C70 | bgcolor="#ff4100" | N65 | bgcolor="#ff3c00" | O60 | bgcolor="#ff3200" | F50 | bgcolor="#bbbbbb" | Ne  |- align="CENTER" | 3 | bgcolor="#ffb400" | Na180 | bgcolor="#ff9600" | Mg150 | colspan=10 | | bgcolor="#ff7d00" | Al125 | bgcolor="#ff6e00" | Si110 | bgcolor="#ff6400" | P100 | bgcolor="#ff6400" | S100 | bgcolor="#ff6400" | Cl100 | bgcolor="#bbbbbb" | Ar  |- align="CENTER" | 4 | bgcolor="#ffdc00" | K220 | bgcolor="#ffb400" | Ca180 | bgcolor="#ffa000" | Sc160 | bgcolor="#ff8c00" | Ti140 | bgcolor="#ff8700" | V135 | bgcolor="#ff8c00" | Cr140 | bgcolor="#ff8c00" | Mn140 | bgcolor="#ff8c00" | Fe140 | bgcolor="#ff8700" | Co135 | bgcolor="#ff8700" | Ni135 | bgcolor="#ff8700" | Cu135 | bgcolor="#ff8700" | Zn135 | bgcolor="#ff8700" | Ga130 | bgcolor="#ff7d00" | Ge125 | bgcolor="#ff7300" | As115 | bgcolor="#ff7300" | Se115 | bgcolor="#ff7300" | Br115 | bgcolor="#bbbbbb" | Kr  |- align="CENTER" | 5 | bgcolor="#ffeb00" | Rb235 | bgcolor="#ffc800" | Sr200 | bgcolor="#ffb400" | Y180 | bgcolor="#ff9b00" | Zr155 | bgcolor="#ff9100" | Nb145 | bgcolor="#ff9100" | Mo145 | bgcolor="#ff8700" | Tc135 | bgcolor="#ff8200" | Ru130 | bgcolor="#ff8700" | Rh135 | bgcolor="#ff8c00" | Pd140 | bgcolor="#ffa000" | Ag160 | bgcolor="#ff9b00" | Cd155 | bgcolor="#ff9b00" | In155 | bgcolor="#ff9100" | Sn145 | bgcolor="#ff9100" | Sb145 | bgcolor="#ff8c00" | Te140 | bgcolor="#ff8c00" | I140 | bgcolor="#bbbbbb" | Xe  |- align="CENTER" | 6 | bgcolor="#ffff00" | Cs260 | bgcolor="#ffd700" | Ba215 | *  | bgcolor="#ff9b00" | Hf155 | bgcolor="#ff9100" | Ta145 | bgcolor="#ff8700" | W135 | bgcolor="#ff8700" | Re135 | bgcolor="#ff8200" | Os130 | bgcolor="#ff8700" | Ir135 | bgcolor="#ff8700" | Pt135 | bgcolor="#ff8700" | Au135 | bgcolor="#ff9600" | Hg150 | bgcolor="#ffbe00" | Tl190 | bgcolor="#ffb400" | Pb180 | bgcolor="#ffa000" | Bi160 | bgcolor="#ffbe00" | Po190 | bgcolor="#bbbbbb" | At  | bgcolor="#bbbbbb" | Rn  |- align=CENTER | 7 | bgcolor="#bbbbbb" | Fr  | bgcolor="#ffd700" | Ra215 | **  | bgcolor="#bbbbbb" | Rf  | bgcolor="#bbbbbb" | Db  | bgcolor="#bbbbbb" | Sg  | bgcolor="#bbbbbb" | Bh  | bgcolor="#bbbbbb" | Hs  | bgcolor="#bbbbbb" | Mt  | bgcolor="#bbbbbb" | Ds  | bgcolor="#bbbbbb" | Rg  | bgcolor="#bbbbbb" | Cn  | bgcolor="#bbbbbb" | Uut  | bgcolor="#bbbbbb" | Uuq  | bgcolor="#bbbbbb" | Uup  | bgcolor="#bbbbbb" | Uuh  | bgcolor="#bbbbbb" | Uus  | bgcolor="#bbbbbb" | Uuo  |- align=CENTER | |- align=CENTER | Lanthanides | *  | bgcolor="#ffc300" | La195 | bgcolor="#ffb900" | Ce185 | bgcolor="#ffb900" | Pr185 | bgcolor="#ffb900" | Nd185 | bgcolor="#ffb900" | Pm185 | bgcolor="#ffb900" | Sm185 | bgcolor="#ffb900" | Eu185 | bgcolor="#ffb400" | Gd180 | bgcolor="#ffaf00" | Tb175 | bgcolor="#ffaf00" | Dy175 | bgcolor="#ffaf00" | Ho175 | bgcolor="#ffaf00" | Er175 | bgcolor="#ffaf00" | Tm175 | bgcolor="#ffaf00" | Yb175 | bgcolor="#ffaf00" | Lu175 |- align=CENTER | Actinides | **  | bgcolor="#ffc300" | Ac195 | bgcolor="#ffb400" | Th180 | bgcolor="#ffb400" | Pa180 | bgcolor="#ffaf00" | U175 | bgcolor="#ffaf00" | Np175 | bgcolor="#ffaf00" | Pu175 | bgcolor="#ffaf00" | Am175 | bgcolor="#bbbbbb" | Cm  | bgcolor="#bbbbbb" | Bk  | bgcolor="#bbbbbb" | Cf  | bgcolor="#bbbbbb" | Es  | bgcolor="#bbbbbb" | Fm  | bgcolor="#bbbbbb" | Md  | bgcolor="#bbbbbb" | No  | bgcolor="#bbbbbb" | Lr  |- align="CENTER" | colspan=20 | |}

Explanation of the general trends

The way the atomic radius varies with increasing atomic number can be explained by the arrangement of electrons in shells of fixed capacity. The shells are generally filled in order of increasing radius, since the negatively charged electrons are attracted by the positively charged protons in the nucleus. As the atomic number increases along each row of the periodic table, the additional electrons go into the same outermost shell; whose radius gradually contracts, due to the increasing nuclear charge. In a noble gas, the outermost shell is completely filled; therefore, the additional electron of next alkali metal will go into the next outer shell, accounting for the sudden increase in the atomic radius.

The increasing nuclear charge is partly counterbalanced by the increasing number of electrons, a phenomenon that is known as shielding; which explains why the size of atoms usually increases down each column. However, there are two occasions where shielding is less effective: in these cases, the atoms are smaller than would otherwise be expected.

The following table summarizes the main phenomena that influence the atomic radius of an element:

Lanthanide contraction

The electrons in the 4f-subshell, which is progressively filled from cerium (Z = 58) to lutetium (Z = 71), are not particularly effective at shielding the increasing nuclear charge from the sub-shells further out. The elements immediately following the lanthanides have atomic radii which are smaller than would be expected and which are almost identical to the atomic radii of the elements immediately above them. Hence hafnium has virtually the same atomic radius (and chemistry) as zirconium, and tantalum has an atomic radius similar to niobium, and so forth. The effect of the lanthanide contraction is noticeable up to platinum (Z = 78), after which it is masked by a relativistic effect known as the inert pair effect.

Due to lanthanide contraction, the 5 following observations can be drawn:

# The size of Ln³⁺ ions regularly decreases with atomic number. According to Fajans' rules, decrease in size of Ln³⁺ ions increases the covalent character and decreases the basic character between Ln³⁺ and OH⁻ ions in Ln(OH)₃. Hence the order of size of Ln³⁺ is given: La³⁺ > Ce³⁺ > ... , ... > Lu³⁺. # There is a regular decrease in their ionic radii. # There is a regular decrease in their tendency to act as a reducing agent, with increase in atomic number. # The second and third rows of d-block transition elements are quite close in properties. # Consequently, these elements occur together in natural minerals and are difficult to separate.

d-Block contraction

The d-block contraction is less pronounced than the lanthanide contraction but arises from a similar cause. In this case, it is the poor shielding capacity of the 3d-electrons which affects the atomic radii and chemistries of the elements immediately following the first row of the transition metals, from gallium (Z = 31) to bromine (Z = 35). The values are in picometres (pm).

{| wikitable WIDTH="80%" style="text-align:center" | Group (vertical) | 1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | 13 | 14 | 15 | 16 | 17 | 18 |- align="CENTER" | Period (horizontal) | colspan=19 | |- align="CENTER" | 1 | bgcolor="#ff3500" | H53 | colspan=16 | | bgcolor="#ff1f00" | He31 |- align="CENTER" | 2 | bgcolor="#ffa700" | Li167 | bgcolor="#ff7000" | Be112 | colspan=10 | | bgcolor="#ff5700" | B87 | bgcolor="#ff4300" | C67 | bgcolor="#ff3800" | N56 | bgcolor="#ff3000" | O48 | bgcolor="#ff2a00" | F42 | bgcolor="#ff2600" | Ne38 |- align="CENTER" | 3 | bgcolor="#ffbe00" | Na190 | bgcolor="#ff9100" | Mg145 | colspan=10 | | bgcolor="#ff7600" | Al118 | bgcolor="#ff6f00" | Si111 | bgcolor="#ff6200" | P98 | bgcolor="#ff5800" | S88 | bgcolor="#ff4f00" | Cl79 | bgcolor="#ff4700" | Ar71 |- align="CENTER" | 4 | bgcolor="#fff300" | K243 | bgcolor="#ffc200" | Ca194 | bgcolor="#ffb800" | Sc184 | bgcolor="#ffb000" | Ti176 | bgcolor="#ffab00" | V171 | bgcolor="#ffa600" | Cr166 | bgcolor="#ffa100" | Mn161 | bgcolor="#ff9c00" | Fe156 | bgcolor="#ff9800" | Co152 | bgcolor="#ff9500" | Ni149 | bgcolor="#ff9100" | Cu145 | bgcolor="#ff8e00" | Zn142 | bgcolor="#ff8800" | Ga136 | bgcolor="#ff7d00" | Ge125 | bgcolor="#ff7200" | As114 | bgcolor="#ff6700" | Se103 | bgcolor="#ff5e00" | Br94 | bgcolor="#ff5800" | Kr88 |- align="CENTER" | 5 | bgcolor="#ffff0a" | Rb265 | bgcolor="#ffdb00" | Sr219 | bgcolor="#ffd400" | Y212 | bgcolor="#ffce00" | Zr206 | bgcolor="#ffc600" | Nb198 | bgcolor="#ffbe00" | Mo190 | bgcolor="#ffb700" | Tc183 | bgcolor="#ffb600" | Ru178 | bgcolor="#ffac00" | Rh173 | bgcolor="#ffa900" | Pd169 | bgcolor="#ffa500" | Ag165 | bgcolor="#ffa100" | Cd161 | bgcolor="#ff9c00" | In156 | bgcolor="#ff9100" | Sn145 | bgcolor="#ff8500" | Sb133 | bgcolor="#ff7b00" | Te123 | bgcolor="#ff7300" | I115 | bgcolor="#ff6c00" | Xe108 |- align="CENTER" | 6 | bgcolor="#ffff2b" | Cs298 | bgcolor="#fffd00" | Ba253 | *  | bgcolor="#ffd000" | Hf208 | bgcolor="#ffc800" | Ta200 | bgcolor="#ffc100" | W193 | bgcolor="#ffbc00" | Re188 | bgcolor="#ffb900" | Os185 | bgcolor="#ffb400" | Ir180 | bgcolor="#ffb100" | Pt177 | bgcolor="#ffae00" | Au174 | bgcolor="#ffab00" | Hg171 | bgcolor="#ff9c00" | Tl156 | bgcolor="#ff9a00" | Pb154 | bgcolor="#ff8f00" | Bi143 | bgcolor="#ff8700" | Po135 | bgcolor="#bbbbbb" | At  | bgcolor="#ff7800" | Rn120 |- align=CENTER | 7 | bgcolor="#bbbbbb" | Fr  | bgcolor="#bbbbbb" | Ra  | **  | bgcolor="#bbbbbb" | Rf  | bgcolor="#bbbbbb" | Db  | bgcolor="#bbbbbb" | Sg  | bgcolor="#bbbbbb" | Bh  | bgcolor="#bbbbbb" | Hs  | bgcolor="#bbbbbb" | Mt  | bgcolor="#bbbbbb" | Ds  | bgcolor="#bbbbbb" | Rg  | bgcolor="#bbbbbb" | Cn  | bgcolor="#bbbbbb" | Uut  | bgcolor="#bbbbbb" | Uuq  | bgcolor="#bbbbbb" | Uup  | bgcolor="#bbbbbb" | Uuh  | bgcolor="#bbbbbb" | Uus  | bgcolor="#bbbbbb" | Uuo  |- align=CENTER | |- align=CENTER | Lanthanides | *  | bgcolor="#bbbbbb" | La  | bgcolor="#bbbbbb" | Ce  | bgcolor="#fff700" | Pr247 | bgcolor="#ffce00" | Nd206 | bgcolor="#ffcd00" | Pm205 | bgcolor="#ffee00" | Sm238 | bgcolor="#ffe700" | Eu231 | bgcolor="#ffe900" | Gd233 | bgcolor="#ffe100" | Tb225 | bgcolor="#ffe400" | Dy228 | bgcolor="#bbbbbb" | Ho  | bgcolor="#ffe200" | Er226 | bgcolor="#ffde00" | Tm222 | bgcolor="#ffde00" | Yb222 | bgcolor="#ffd900" | Lu217 |- align=CENTER | Actinides | **  | bgcolor="#bbbbbb" | Ac  | bgcolor="#bbbbbb" | Th  | bgcolor="#bbbbbb" | Pa  | bgcolor="#bbbbbb" | U  | bgcolor="#bbbbbb" | Np  | bgcolor="#bbbbbb" | Pu  | bgcolor="#bbbbbb" | Am  | bgcolor="#bbbbbb" | Cm  | bgcolor="#bbbbbb" | Bk  | bgcolor="#bbbbbb" | Cf  | bgcolor="#bbbbbb" | Es  | bgcolor="#bbbbbb" | Fm  | bgcolor="#bbbbbb" | Md  | bgcolor="#bbbbbb" | No  | bgcolor="#bbbbbb" | Lr  |- align="CENTER" | colspan=20 | |}

See also

Atomic radii of the elements (data page)

Chemical bond

Covalent radius

Bond length

Steric hindrance

References

Category:Atoms Category:Properties of chemical elements