Ionization

Ionization is the process by which an atom or a group of atoms acquires a positive or negative charge by gaining or losing an electron. Ionization can occur as a result of high temperatures, collisions between subatomic particles, chemical reactions, electrical discharges, or radiation. Each atom requires a certain amount of energy to remove an electron from its outer shell. The amount of this energy varies according to the atom's structure, but smaller atoms with fewer electrons generally need more energy for ionization to occur.

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Background

An atom is one of the fundamental building blocks of matter. It is the smallest unit that makes up a chemical element and still maintains the characteristics of that element. Atoms are composed of three subatomic particles: protons, neutrons, and electrons. Protons carry a positive electrical charge and, together with neutrons, are found in the nucleus, or core, of an atom. Neutrons do not have an electrical charge. The number of protons in an atom determines the characteristics of that atom. For example, the simplest element, hydrogen, has one proton. Helium atoms have two protons, oxygen atoms have eight protons, and gold atoms have seventy-nine protons. The number of protons in an atom is referred to as its atomic number.

Electrons are negatively charged particles that orbit the nucleus in a cloud consisting of one or more shells. Since protons and electrons have opposite charges, stable atoms have equal numbers of both, canceling out the electrical charge. If an atom gains or loses an electron, it becomes known as an ion. Atoms that have lost an electron have a greater number of protons and develop a positive charge. These positive ions are called cations. Atoms that gain an electron display a negative charge and are called anions.

Overview

Atoms can lose electrons in a number of ways. An electron can be knocked from its orbit around a nucleus by collisions with other electrons. Because electrons are extremely small, however, this process can take a large amount of energy, as most electrons will miss their targets. Chemical ionization is more efficient; this process uses a stream of larger, positively charged ions to jolt the electrons free. Exposure to extremely high temperatures ranging upward of thousands of degrees may also be enough to ionize an atom.

Electromagnetic radiation with wavelengths shorter than the visible part of the spectrum—such as ultraviolet light, X-rays, and gamma rays—can also ionize atoms and molecules. A molecule is a group of atoms bonded together. This process is common in the upper reaches of Earth's atmosphere where ultraviolet radiation from the sun can ionize oxygen or nitrogen molecules. Ionization can occur when a molecule or an atom is subjected to an intense electrical field. An example of this can be seen when static electricity builds up on household surfaces on a dry day. The spark discharged when a person touches a piece of metal is caused by ionized electrons jumping between the person's hand and the metal surface.

The amount of energy required to remove an electron from an atom or molecule is called its ionization energy. Stable atoms exist in a ground state, or one in which they are experiencing normal energy levels. If sufficient energy is added to the atom, it reaches an excited state, and electrons can be expelled from the atom's outer shell. The ionization energy needed to remove an electron varies by chemical element. Smaller, simpler elements have electrons that orbit closer to the nucleus, which makes them harder to dislodge. As a result, elements like helium and neon require larger amounts of energy to cause ionization. More complex elements, such as cesium with fifty-five electrons or francium with eighty-seven, need less energy. Because removing an electron will result in a positively charged atom, the energy needed to remove a second electron is always higher than that needed for the first.

The structure of the atom also affects the amount of energy needed for ionization. The electrons in an atom are arranged in shells, with a maximum of two electrons in the innermost shell. Other shells for many elements can contain a maximum of eight electrons. Atoms and molecules have a tendency to attempt to reach a stable or neutral state. This means that an element with an odd number of electrons in its outer shell is more likely to ionize and bond with other elements to reach stability. The electrons in the outer shell are known as valence electrons. Hydrogen, for example, has one electron in its only shell. It is more likely to form an ionic bond in an attempt to fill out its shell and reach two electrons. Sodium, an element with eleven electrons, has two electrons in its inner shell, eight in its second, and one in its third. Chlorine has seventeen electrons, including seven valence electrons. As sodium and chlorine bond, sodium loses its lone valence electron to chlorine, giving both atoms eight electrons in their outer shells. It also forms a substance known as sodium chloride, or common table salt.

Elements such as helium, neon, argon, and krypton form part of a group of stable elements known as the noble gases. These elements have a full shell of valence electrons and require more ionization energy to remove an electron. On a periodic table—the representation of chemical elements ordered by number of protons—the noble gases take up the column on the far right. Elements in the column on the left each have one valence electron and are more reactive, requiring less ionization energy. The amount of ionization energy needed to remove an electron increases from left to right in the rows of a periodic table and decreases from top to bottom in the columns.

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