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General Chemistry

Electronegativity

Definition and meaning of Electronegativity in chemistry.

Electronegativity is a measure of an atom's ability to attract and hold onto the shared electrons in a chemical bond. Atoms with high electronegativity pull bonding electron density toward themselves more strongly than atoms with low electronegativity.

In more detail

Electronegativity is a relative, dimensionless property most commonly expressed on the Pauling scale, which runs from about 0.7 (cesium) to 3.98 (fluorine). It generally increases left to right across a period, as nuclear charge increases, and decreases down a group, as atomic radius and electron shielding increase. The electronegativity difference between two bonded atoms predicts bond character: a small difference gives a nonpolar covalent bond, a moderate difference gives a polar covalent bond, and a large difference favors an ionic bond.

Key facts

FieldGeneral Chemistry
Common scalePauling scale, ~0.7 to 3.98
Most electronegative elementFluorine (3.98)
Periodic trendIncreases across a period, decreases down a group
Example

In hydrogen fluoride (HF), fluorine (Pauling value 3.98) is far more electronegative than hydrogen (2.20), so the bonding electrons sit closer to fluorine, creating a polar covalent bond with a partial negative charge on F and a partial positive charge on H.

Frequently asked questions

How is electronegativity different from electron affinity?

Electronegativity is a relative tendency of an atom to attract shared electrons within a bond, while electron affinity is the measurable energy change when an isolated gaseous atom gains an electron to form an anion.

How does electronegativity difference predict bond type?

A difference below about 0.5 typically indicates a nonpolar covalent bond, 0.5 to 1.7 indicates a polar covalent bond, and above about 1.7 the bond is usually considered ionic, though these are approximate guidelines, not sharp cutoffs.

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