Open main menu

Wikipedia β

The oxidation state, sometimes referred to as oxidation number, describes degree of oxidation (loss of electrons) of an atom in a chemical compound. Conceptually, the oxidation state, which may be positive, negative or zero, is the hypothetical charge that an atom would have if all bonds to atoms of different elements were 100% ionic, with no covalent component. This is never exactly true for real bonds.

The term oxidation was first used by Antoine Lavoisier to signify reaction of a substance with oxygen. Much later, it was realized that the substance, upon being oxidized, loses electrons, and the meaning was extended to include other reactions in which electrons are lost.

Oxidation states are typically represented by integers which may be positive, zero, or negative. In some cases, the average oxidation state of an element is a fraction, such as ​83 for iron in magnetite (Fe
). The highest known oxidation state is reported to be +9 in the iridium tetroxide cation (IrO4+).[1] It is predicted that even a +10 oxidation state may be achievable by platinum in the platinum tetroxide dication (PtO42+).[2] The lowest oxidation state is −4, as for carbon in methane or for chromium[3] in [Cr(CO)4]4−.

The increase in oxidation state of an atom, through a chemical reaction, is known as an oxidation; a decrease in oxidation state is known as a reduction. Such reactions involve the formal transfer of electrons: a net gain in electrons being a reduction, and a net loss of electrons being an oxidation. For pure elements, the oxidation state is zero.

The oxidation state of an atom does not represent the "real" charge on that atom. This is particularly true of high oxidation states, where the ionization energy required to produce a multiply positive ion is far greater than the energies available in chemical reactions. The assignment of electrons between atoms in calculating an oxidation state is purely a formalism, but is a useful one for the understanding of many chemical reactions.

In inorganic nomenclature, the oxidation state is represented by a Roman numeral placed after the element name inside a parenthesis or as a superscript after the element symbol.


IUPAC definition of oxidation stateEdit

Oxidation stateEdit

A "Comprehensive definition of the term oxidation state (IUPAC Recommendations 2016)" has been published with free access.[4] It is a distillation of an IUPAC technical report "Toward a comprehensive definition of oxidation state" from 2014.[5] The current IUPAC Gold Book definition of oxidation state[6] is:

Oxidation state of an atom is the charge of this atom after ionic approximation of its heteronuclear bonds,

and the term oxidation number is nearly synonymous.[7]

The underlying principle is that the ionic signs[clarification needed] for two atoms that are bonded are deduced from the electron distribution in a LCAO-MO model. In a bond between two different elements, the bond's electrons are assigned to its main atomic contributor; in a bond between two atoms of the same element, the electrons are divided equally. In practical use, the sign of the ionic approximation follows Allen electronegativities:

Electronegativity using the Allen scale
Group → 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18
↓ Period
1 H
2 Li
3 Na
4 K
5 Rb
6 Cs
7 Fr
See also: Electronegativities of the elements (data page)

Determination of oxidation stateEdit

While introductory levels of chemistry teaching use postulated oxidation states, the IUPAC recommendation[4] and the Gold Book entry[6] list two entirely general algorithms for the calculation of the oxidation states of elements in chemical compounds.

Simple approach without bonding considerationsEdit

Introductory chemistry uses postulates: The oxidation state for an element in a chemical formula is calculated from the overall charge and postulated oxidation states for all the other atoms.

A simple example is based on two postulates,

  1. OS = +1 for H
  2. OS = −2 for O

and yields correct oxidation states in oxides and hydroxides of any single element, and in acids such as H2SO4 or H2Cr2O7. Its coverage can be extended either by a list of exceptions or by assigning priority to the postulates. The latter works for H2O2 where the priority of rule 1 leaves both oxygens with oxidation state −1.

Additional postulates and their ranking may expand the range of compounds to fit a textbook’s scope. As an example, one postulatory algorithm from many possible; in a sequence of decreasing priority:

  1. An element in a free form has OS = 0.
  2. In a compound or ion, the oxidation-state sum equals the total charge of the compound or ion.
  3. Fluorine in compounds has OS = −1; which extends to Cl and Br only when not bonded to a lighter halogen, oxygen or nitrogen.
  4. Group 1 and 2 metals in compounds have OS = +1 and +2, respectively.
  5. Hydrogen has OS = +1, but adopts −1 when bonded to metals or metalloids.
  6. Oxygen in compounds has OS = −2.

This set of postulates covers oxidation states of fluorides, chlorides, bromides, oxides, hydroxides and hydrides of any single element. It covers all oxoacids of any central atom (and all their fluoro-, chloro-, bromo- relatives), as well as salts of such acids with Group 1 and Group 2 metals. It also covers iodides, sulfides and similar simple salts of these metals.

Algorithm of assigning bondsEdit

This algorithm is performed on a Lewis structure (a formula that shows all valence electrons). Oxidation state equals the charge of an atom after its heteronuclear bonds have been assigned to the more electronegative partner (except when that partner is a reversibly bonded Lewis-acid ligand) and homonuclear bonds have been divided equally:


where "—" is an electron pair, and OS is the oxidation state as a numerical variable.

After the electrons have been assigned according to the vertical red lines on the formula, the total number of valence electrons that now "belong" to each atom are subtracted from the number N of valence electrons of the neutral atom (such as 5 for nitrogen in the periodic-table group 15, etc.) to yield that atom's oxidation state.

This example shows the importance of describing the bonding. Its summary formula, HNO3, corresponds to two structural isomers; the peroxynitrous acid in the above figure and the more stable nitric acid. With the formula HNO3, the simple approach without bonding considerations yields −2 for all three oxygens and +5 for nitrogen, which is correct for nitric acid. For the peroxynitrous acid, however, the two oxygens in the O–O bond have OS = −1 and the nitrogen has OS = +3, which requires a structure to understand.

Organic compounds are treated in a similar manner; exemplified here on functional groups occurring in between CH4 and CO2:


Analogously for transition-metal compounds; CrO(O2)2 on the left has a total of 36 valence electrons (18 pairs to be distributed), and Cr(CO)6 on the right has 66 valence electrons (33 pairs):


A key step is drawing the Lewis structure of the molecule (neutral, cationic, anionic): Atom symbols are arranged so that pairs of atoms can be joined by single two-electron bonds as in the molecule (a sort of "skeletal" structure), and the remaining valence electrons are distributed such that sp atoms obtain an octet (duet at H) with priority that increases with electronegativity. In some cases, this leads to alternative formulas that differ in bond orders (the full set of which is called the resonance formulas). Consider the sulfate anion (SO42− with 32 valence electrons; 24 from oxygens, 6 from sulfur, 2 of the anion charge obtained from the implied cation). The bond orders to terminal oxygens have no effect on the oxidation state so long as the oxygens have octets. Already the skeletal structure, top left, yields correct oxidation states, as does the Lewis structure, top right (one of the resonance formulas):


The bond-order formula at bottom is closest to the reality of four equivalent oxygens each having a total bond order of 2. That total includes the bond of order ½ to the implied cation and follows the 8−N rule[5] requiring that the main-group atom’s bond order equals 8 minus N valence electrons of the neutral atom, enforced with priority that increases with electronegativity.

This algorithm works equally for molecular cations composed of several atoms. An example is the ammonium cation of 8 valence electrons (5 from nitrogen, 4 from hydrogens, minus 1 for the cation’s positive charge due to the electron given to the implied anion):


Drawing Lewis structures with electron pairs as dashes emphasizes the essential equivalence of bond pairs and lone pairs when counting electrons and moving bonds onto atoms. Structures drawn with electron dot pairs are of course identical in every way:


The algorithm's caveatEdit

The algorithm contains a caveat, in parenthesis, which concerns rare cases of transition-metal complexes with a type of ligand that is reversibly bonded as a Lewis acid (as an acceptor of the electron-pair from the transition metal); termed a Z-type ligand in Green’s Covalent Bond Classification. The caveat originates from the simplifying use of electronegativity instead of the MO-based electron allegiance to decide the ionic sign.[4] One early example is the O2S−RhCl(CO){P(C6H5)3}2 complex[8] with SO2 as the reversibly-bonded acceptor ligand (released upon heating). The Rh−S bond is therefore extrapolated ionic against Allen electronegativities of Rh and S, yielding oxidation state +1 for rhodium:


Algorithm of summing bond ordersEdit

This algorithm works on Lewis structures and on bond graphs of extended (non-molecular) solids: Oxidation state is obtained by summing the heteronuclear-bond orders at the atom as positive if that atom is the electropositive partner in a particular bond and as negative if not, and the atom’s formal charge (if any) is added to that sum.

Applied to a Lewis structureEdit

An example of a Lewis structure with no formal charge,  , illustrates that, in this algorithm, homonuclear bonds are simply ignored (notice the bond orders in blue).

Carbon monoxide exemplifies a Lewis structure with formal charges:


To obtain the oxidation states, the formal charges are summed with the bond-order value taken positively at the carbon and negatively at the oxygen.

Applied to molecular ions, this algorithm considers the actual location of the formal (ionic) charge, as drawn in the Lewis structure. As an example, summing bond orders in the ammonium cation yields −4 at the nitrogen of formal charge 1+, with the two numbers adding to the oxidation state of −3:


Notice that the sum of oxidation states in the ion equals its charge (as it equals zero for a neutral molecule).

Also in anions, the formal (ionic) charges have to be considered when nonzero. For sulfate this is exemplified with the skeletal or Lewis structures (top), compared with the bond-order formula of all oxygens equivalent and fulfilling the octet and 8−N rules (bottom):


Applied to bond graphEdit

Bond graph in solid-state chemistry is a chemical formula of an extended structure, in which direct bonding connectivities are shown. An example is the AuORb3 perovskite, the unit-cell of which is drawn on the left and the bond graph (with added numerical values) on the right:


We see that the O atom bonds to the 6 nearest rubidium cations, each of which has 4 bonds to the auride anion. The bond graph summarizes these connectivities. The bond orders (also called bond valences) sum up to oxidation states according to the attached sign of the bond’s ionic approximation (there are no formal charges in bond graphs).

Determination of oxidation states from a bond graph can be illustrated on ilmenite, FeTiO3. We may ask whether the mineral contains Fe2+/Ti4+ or Fe3+/Ti3+. Its crystal structure has each metal atom bonded to six oxygens and each of the equivalent oxygens to two Fe and two Ti, as in the bond graph below. Experimental data show that 3 metal–oxygen bonds in the octahedron are short and 3 are long (the metals are off center). The bond orders/valences, obtained from the bond lengths by the bond valence method, sum up to 2.01 at Fe and 3.99 at Ti; rounded off to oxidation states +2 and +4, respectively:


Nominal oxidation statesEdit

A nominal oxidation state is a general term for two specific purpose-oriented values:

  • Electrochemical oxidation state; it represents a molecule or ion in the Latimer diagram or Frost diagram for its redox-active element. An example is the Latimer diagram for sulfur at pH = 0 where the electrochemical oxidation state +2 for sulfur puts HS2O3 between S and H2SO3:
  • Systematic oxidation state; it is chosen from close alternatives for pedagogical reasons of descriptive chemistry. An example is the oxidation state of phosphorus in H3PO3 (in fact the diprotic H2PHO3) taken nominally as +3, while Allen electronegativities of P and H suggest +5 by a narrow margin that makes the two alternatives almost equivalent:

Both alternative oxidation states of phosphorus make chemical sense, depending on the chemical property or reaction we wish to emphasize. In contrast, their average does not.

Balancing redoxEdit

Oxidation states can be useful for balancing chemical equations for oxidation–reduction (or redox) reactions, because the changes in the oxidized atoms have to be balanced by the changes in the reduced atoms. For example, in the reaction of acetaldehyde with the Tollens' reagent to acetic acid (shown below), the carbonyl carbon atom changes its oxidation state from +1 to +3 (by two electrons). This oxidation is balanced by reducing two Ag+ ions to Ag0 (by two electrons in total).


An inorganic example is the Bettendorf reaction using SnCl2 to prove the presence of arsenite ions in a concentrated HCl extract. When As(III) is present, a brown coloration appears forming a dark precipitate of As, according to the following simplified reaction:

2As3+ + 3Sn2+ → 2As0 + 3Sn4+

Here three tin atoms are oxidized from oxidation state +2 to +4, yielding 6 electrons that reduce two arsenic atoms from oxidation state +3 to 0. The simple one-line balancing goes as follows: The two redox couples are written down as they react; As3+ + Sn2+ ⇌ As0 + Sn4+. One Sn is oxidized from oxidation state +2 to +4, a 2-electron step, hence 2 is written in front of the two As partners. One As is reduced from +3 to 0, a 3-electron step, hence 3 goes in front of the two Sn partners. An alternative three-line procedure is to write separately the half-reactions for oxidation and for reduction, each balanced with electrons, and then to sum them up such that the electrons cross out. In general, these redox balances (the one-line balance or each half-reaction) need to be checked for the ionic- and electron-charge sums on both sides of the equation being indeed equal. If they are not equal, suitable ions are added to balance the charges and the non-redox elemental balance.

Ambiguous oxidation statesEdit

Lewis formulas are fine rule-based approximations of the chemical reality, as indeed are Allen electronegativities. Still, oxidation states may seem ambiguous when the determination is not straightforward. Rule-based oxidation states feel ambiguous when only experiment can decide. There are also truly dichotomous values to be decided by mere convenience.

Oxidation-state determination from resonance formulas is not straightforwardEdit

Seemingly ambiguous oxidation states are obtained on a set of resonance formulas of equal weights for a molecule of heteronuclear bonds where the atom connectivity does not correspond to the number of two-electron bonds dictated by the 8−N rule. An example is S2N2 where four resonance formulas featuring one S=N bond have oxidation states +2 and +4 on the two sulfur atoms, to be averaged to +3 because the two S atoms are equivalent in this square-shaped molecule.

A physical measurement is needed to decide the oxidation stateEdit

  • This happens when a non-innocent ligand is present, of hidden or unexpected redox properties that could otherwise be assigned to the central atom. An example is the nickel dithiolate complex, Ni(S2C2H2)22− (see p. 1056–7 in ref.[5] for discussion).
  • When the redox ambiguity of a central atom and ligand yields dichotomous oxidation states of close stability, thermally induced tautomerism may result, as exemplified by manganese catecholate, Mn(C6H4O2)3 (see p. 1057–8 in ref.[5] for discussion). Assignment of such oxidation states in general requires spectroscopic,[9] magnetic and/or structural data.
  • When the bond order has to be ascertained along an isolated tandem of a heteronuclear and a homonuclear bond. An example is S2O32− with two oxidation-state alternatives (note bond orders in blue and formal charges in green):
The S–S distance in thiosulfate is needed to reveal that this bond order is very close to 1, as in the formula on the left.

Truly ambiguous oxidation states occurEdit

  • When the electronegativity difference between two bonded atoms is very small (as in H3PO3 above). Two almost equivalent pairs of oxidation states, open for a choice, are obtained for these atoms.
  • When an electronegative p-block atom forms solely homonuclear bonds, the number of which differs from the number of two-electron bonds suggested by rules. Examples are homonuclear finite chains like N3 (central N connects 2 atoms while 3 two-electron bonds are required by 8−N rule) or I3 (central iodine connects 2 atoms while 1 two-electron bond fulfills the 8−N rule). A sensible approach is to distribute the ionic charge over the two outer atoms.[5] Such a placement of charges in a polysulfide Sn2− (where all inner S form 2 bonds fulfilling the 8−N rule) follows already from its Lewis structure.[5]
  • When the isolated tandem of a heteronuclear and a homonuclear bond leads to a bonding compromise in between two Lewis structures of limiting bond orders. An example here is N2O:
The typically used oxidation state of nitrogen in N2O is +1, which also obtains for both nitrogens by an MO approach.[10] It is worth noting that the formal charges on the right comply with electronegativities, and this implies an added ionic bonding contribution. Indeed, the estimated NN and NO bond orders are 2.76 and 1.9, respectively,[5] approaching the formula of integer bond orders that would include the ionic contribution explicitly as a bond (in green):
Conversely, formal charges against electronegativities in a Lewis structure decrease the bond order of the corresponding bond. An example is the CO molecule with a bond-order estimate of 2.6.[11]

Elements with multiple oxidation statesEdit

Most elements have more than one possible oxidation state. For example, carbon has nine integer oxidation states:

Integer oxidation states of carbon
Oxidation state Example compound
−4 CH
−3 C
−2 C
, CH
−1 C
, C
, (CH
+4 CCl
, CO

Fractional oxidation statesEdit

Fractional oxidation states are often used to represent the average oxidation states of several atoms of the same element in a structure. For example, the formula of magnetite is Fe
, implying an average oxidation state for iron of +​83.[12] However, this average value may not be representative if the atoms are not equivalent. In an Fe
crystal below 120 K, two-thirds of the cations are Fe3+
and one-third Fe2+
, and the formula may be better represented as FeO·Fe

Likewise, propane, C
, has been described as having a carbon oxidation state of −​83.[14] Again, this is an average value since the structure of the molecule is H
, with the first and third carbon atoms each having an oxidation state of −3 and the central one −2.

An example with true fractional oxidation states for equivalent atoms is potassium superoxide, KO
. The diatomic superoxide ion has an overall charge of −1, so each of its two oxygen atoms is assigned an oxidation state of −​12. This ion can be described as a resonance hybrid of two Lewis structures, where each oxygen has oxidation state 0 in one structure and −1 in the other.

For the cyclopentadienyl anion C
, the oxidation state of C is (−1) + (−​15) = −​65. The −1 occurs because each C is bonded to one hydrogen atom (a less electronegative element), and the −​15 because the total ionic charge of −1 is divided among five equivalent C.

Examples of fractional oxidation states for carbon
Oxidation state Example species
−​65 C
−​67 C
+​32 C

Use in nomenclatureEdit

The oxidation state in compound naming is placed either as a right superscript to the element symbol in chemical formula, for example FeIII, or in parentheses after the name of the element, iron(III) in chemical names. For example, Fe
is named iron(III) sulfate and its formula can be shown as FeIII
. This is because a sulfate ion has a charge of −2, so each iron atom takes a charge of +3. Note that fractional oxidation numbers should not be used in naming.[15] Minium, Pb
, is represented as lead(II,IV) oxide, showing the actual two oxidation states of the nonequivalent lead atoms.

Oxidation state in metalsEdit

Many compounds with luster and electrical conductivity maintain a simple stoichiometric formula; such as the golden TiO, blue-black RuO2 or coppery ReO3 of obvious oxidation state. Ultimately, however, the assignment of the free metallic electrons to one of the bonded atoms has its limits and leads to unusual oxidation states. Simple examples are the LiPb and Cu3Au ordered alloys, the composition and structure of which are largely determined by size factors and packing. Should oxidation state be needed for redox balancing, it is best set to zero for all atoms of such an alloy.

History of the oxidation state conceptEdit

Early daysEdit

Oxidation itself was first studied by Antoine Lavoisier, who believed that what we now call oxidation was always the result of reactions with oxygen, thus the name. Although Lavoisier's idea has been shown to be incorrect, the name he proposed is still used, albeit more generally. Oxidation states, called oxidation grades by Friedrich Wöhler in 1835,[16] were one of the intellectual stepping stones that Mendeleev used to derive the periodic table. Jensen[17] gives an overview of the history up to 1938.

Use in nomenclatureEdit

When it was realized that some metals form two different binary compounds with the same nonmetal, the two compounds were often distinguished by using the ending -ic for the higher metal oxidation state and the ending -ous for the lower. For example, FeCl3 is ferric chloride and FeCl2 is ferrous chloride. This system is not very satisfactory (although sometimes still used) because different metals have different oxidation states which have to be learned: ferric and ferrous are +3 and +2 respectively, but cupric and cuprous are +2 and +1, and stannic and stannous are +4 and +2. Also there was no allowance for metals with more than two oxidation states, such as vanadium with oxidation states +2, +3, +4 and +5.[18]

This system has been largely replaced by one suggested by Alfred Stock in 1919[19] and adopted[20] by IUPAC in 1940. Thus, FeCl2 was written as iron(II) chloride rather than ferrous chloride. The roman numeral II at the central atom came to be called the Stock number (now an obsolete term), and its value was obtained as a charge at the central atom after removing its ligands along with electron pairs they shared with it.[21]

Development towards the current conceptEdit

The term oxidation state in English chemical literature was popularized by Wendell Mitchell Latimer in his 1938 book about electrochemical potentials[22] and its numerous re-editions. He used it for the value (synonymous with the German term Wertigkeit) previously termed valence or polar valence or polar number[23] in English, or oxidation stage or indeed[24][25] the state of oxidation. Since 1938, the term oxidation state has been connected with electrochemical potentials and electrons exchanged in redox couples participating in redox reactions. By 1948, IUPAC used the 1940 nomenclature rules with the term oxidation state,[26][27] instead of the original[20] valency. In 1948 Linus Pauling proposed that oxidation number could be determined by extrapolating bonds to 100% ionic in the direction of electronegativity.[28] A full acceptance of this suggestion was complicated by the fact that the Pauling electronegativities as such depend on the oxidation state/number and that they may lead to unusual values of oxidation states for some transition metals. In 1990 IUPAC resorted to a postulatory (rule-based) method to determine the oxidation state.[29] This was complemented by the synonymous term oxidation number as a descendant of the Stock number introduced in 1940 into the nomenclature. However, the terminology using ligands[21] gave the impression that oxidation number might be something specific to coordination compounds. This situation and the lack of a real single definition generated numerous debates about the meaning of oxidation state, suggestions about methods to obtain it and definitions of it. To resolve the issue, an IUPAC project (2008-040-1-200) was started in 2008 on the "Comprehensive Definition of Oxidation State", and was concluded by the two reports [5][4] and by the revised entries Oxidation State[6] and Oxidation Number[7] in the IUPAC Gold Book. The outcomes were a single definition of oxidation state and two algorithms to calculate it in molecular and extended-solid compounds, guided by Allen electronegativities that are independent of oxidation state.

See alsoEdit


  1. ^ G. Wang, M. Zhou, G.T. Goettel, G.J. Schrobilgen, J. Su, J. Li, T. Schlöder, S. Riedel, Identification of an iridium-containing compound with a formal oxidation state of IX, Nature 514(2014)475–477. doi:10.1038/nature13795
  2. ^ H.S. Yu, D.G. Truhlar, Oxidation state 10 exists, Angew. Chem. Int. Ed., 55(2016)9004–9006. doi:10.1002/anie.201604670
  3. ^ J.T. Lin, G.P. Hagen, J.E. Ellis, Highly reduced organometallics. 9. Synthesis and characterization of the tetrasodium tetracarbonylmetalates(4−) of chromium, molybdenum, and tungsten, Na4M(CO)4: their reactions with weak acids to generate H2M2(CO)82− (M = Cr, Mo, and W), J.Am.Chem.Soc. 105(1983)2296–2303. doi:10.1021/ja00346a032
  4. ^ a b c d P. Karen, P. McArdle, J. Takats, Comprehensive definition of oxidation state (IUPAC Recommendations 2016), Pure Appl. Chem. 88(2016)831–839. doi:10.1515/pac-2015-1204
  5. ^ a b c d e f g h P. Karen, P. McArdle, J. Takats, Toward a comprehensive definition of oxidation state (IUPAC Technical Report), Pure Appl. Chem. 86(2014)1017–1081. doi:10.1515/pac-2013-0505
  6. ^ a b c IUPAC, Compendium of Chemical Terminology, 2nd ed. (the "Gold Book") (1997). Online corrected version:  (2006–) "Oxidation state".
  7. ^ a b IUPAC, Compendium of Chemical Terminology, 2nd ed. (the "Gold Book") (1997). Online corrected version:  (2006–) "Oxidation number".
  8. ^ K.W. Muir, J.A. Ibers, The structure of chlorocarbonyl(sulfur dioxide)bis(triphenylphosphine)rhodium, RhCl(CO)(SO2)(P(C6H5)3)2, Inorg. Chem. 8(1969)1921–1928. doi:10.1021/ic50079a024
  9. ^ C.K. Jørgensen, Electric Polarizability, Innocent Ligands and Spectroscopic Oxidation States, in: Structure and Bonding, Vol. 1, pp. 234–248, Springer-Verlag, Berlin (1966).
  10. ^ P. Karen, Oxidation state, a long-standing issue!, Angew. Chem. Int. Ed. 54(2015)4716–4726. doi:10.1002/anie.201407561
  11. ^ R.J. Martinie, J.J. Bultema, M.N.V. Wal, B.J. Burkhart, D.A.V. Griend, R.L. DeCock, Bond order and chemical properties of BF, CO, and N2, J. Chem. Educ. 88(2011)1094–1097. doi:10.1021/ed100758t
  12. ^ R.H. Petrucci, W.S. Harwood, F.G. Herring, General Chemistry, (8th ed., Prentice-Hall 2002) pp. 81–82.
  13. ^ M.S. Senn, J.P. Wright, J.P. Attfield, Charge order and three-site distortions in the Verwey structure of magnetite, Nature 481(2012)173–176. doi:10.1038/nature10704
  14. ^ K.W. Whitten, K.D. Galley, R.E. Davis, General Chemistry, (4th ed., Saunders 1992) p. 147.
  15. ^ N.G. Connelly, T. Damhus, R.M. Hartshorn, A.T. Hutton, Nomenclature of Inorganic Chemistry (IUPAC Recommendations 2005), RSC Publishing, p. 66.
  16. ^ F. Wöhler, Grundriss der Chemie, Unorganische Chemie, (Duncker und Humblot, Berlin, 1835) p. 4.
  17. ^ W.B. Jensen, The origin of the oxidation-state concept, J. Chem. Educ. 84(2007)1418–9. doi:10.1021/ed084p1418
  18. ^ R.H. Petrucci, W.S. Harwood, F.G. Herring, General Chemistry, (8th ed., Prentice Hall 2002) p. 84 ISBN 0-13-014329-4
  19. ^ A. Stock, Einige Nomenklaturfragen der anorganischen Chemie, Angew. Chem. 32(1919)373–374. doi:10.1002/ange.19190329802
  20. ^ a b W.P. Jorissen, H. Bassett, A. Damiens, F. Fichter, H. Rémy, Rules for naming inorganic compounds, J. Am. Chem. Soc. 63(1941)889–897. doi:10.1021/ja01849a001
  21. ^ a b N.G. Connelly, T. Damhus, R.M. Hartshorn, A.T. Hutton, Nomenclature of Inorganic Chemistry (IUPAC Recommendations 2005), RSC Publishing, p. 147.
  22. ^ W.M. Latimer, The Oxidation States of the Elements and their Potentials in Aqueous Solutions, (Prentice Hall 1938).
  23. ^ W.C. Bray, G.E.K. Branch, Valence and tautomerism, J. Am. Chem. Soc. 35(1913)1440–1447. doi:10.1021/ja02199a003
  24. ^ A.A. Noyes, K.S. Pitzer, C.L. Dunn, Argentic salts in acid solution, I. The oxidation and reduction reactions, J. Am. Chem. Soc. 57(1935)1221–1229. doi:10.1021/ja01310a018
  25. ^ A.A. Noyes, K.S. Pitzer, C.L. Dunn, Argentic salts in acid solution, II. The oxidation state of argentic salts, J. Am. Chem. Soc. 57(1935)1229–1237. doi:10.1021/ja01310a019
  26. ^ W.C. Fernelius, Some problems of inorganic nomenclature, C&EN 26(1948)161–163. doi:10.1021/cen-v026n003.p161
  27. ^ W.C. Fernelius, E.M. Larsen, L.E. Marchi, C.L. Rollinson, Nomenclature of coördination compounds, C&EN 26(1948)520–523. doi:10.1021/cen-v026n008.p520
  28. ^ L. Pauling, The modern theory of valency, J.Chem.Soc. (1948)1461–1467. doi:10.1039/JR9480001461
  29. ^ J.G. Calvert, IUPAC Recommendation 1990, Pure Appl. Chem. 62 (1990) p. 2204. doi:10.1351/pac199062112167