| Themes > Science > Astronomy > The Galaxies > The Milky Way Galaxy > Ionization and Plasmas | ||||||||||||||||||||
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Ionization of AtomsIonization is the gain or loss of electrons. The loss of electrons, which is the more common process in astrophysical environments, converts an atom into a positively charged ion, while the gain of electrons converts an atom into a negatively charged ion. In the subsequent discussion, we will use the terms ionization and ionize in the sense of losing electrons to form positive ions.There is a standard notation in astrophysics for various levels of ionization of an atom. As illustrated in the following table, this notation uses increasing Roman numerals to indicate higher levels of ionization.
We also show the standard chemist's notation for such ions, which consists of placing a right superscript on the element symbol indicating the net electrical charge on the ion (in the neutral case the superscript "0" is usually omitted). Thus, for example, we shall speak later of "H II regions", meaning volumes of space in which the radiation from nearby hot stars has completely ionized the hydrogen. PlasmasIf most of the atoms or molecules in a region are ionized, the resulting state of matter corresponds to a gas that is electrically neutral on a global scale, but composed microscopically of positively charged ions and the negatively charged electrons stripped from the atoms to form the ions. Such a state of matter is called a plasma. Most of the matter in stars is in a plasma state. Thus, although what we refer to as "normal matter" consists of atoms and molecules, the evidence is that the most abundant form of matter in the Universe is not atoms and molecules but rather the plasma state. |
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