CHAPTER II

ELEMENTARY CHEMICAL PRINCIPLES



A. Atoms

The periodic table of the elements lists atomic numbers and atomic weights for each element. The atomic numbers, the number of protons in each atom, is not commonly used in environmental analysis. However, the atomic weights are quite useful. They represent the total weight of each atom in atomic mass units (AMU) or Daltons. For many elements the tabulated atomic weights represent an average of the atomic weights of each of the naturally occurring isotopes weighted according to their abundance in the biosphere. Table 2.1 is an alphabetical list of the stable elements with their atomic numbers and weights.


B. Molecules and Chemical Bonds

1. Types of bonds

a. Ionic Bonds - transfer of an electron to complete an octet.

atoms to ions

Na + Cl --------> NaCl or Na+ + Cl- (2.1)

(2.2)

b. Covalent Bonds - sharing of one or more electron pairs

Single bond

2 H + O -----------> H-O-H (2.3)

(2.4)

Double bond

2 O --------------> O=O (2.5)

(2.6)

2. Valence.

An atom's valence is the number of chemical bonds it makes with other atoms, including ionic and covalent. Many elements have more than one valence, as noted in Table 2.1. Elements in the first column in the periodic table (i.e., the alkali metals; sodium, potassium, etc.) all have a valence of 1. They are therefore called monovalent metals. Those in the second column (i.e., the alkaline earths; magnesium, calcium, etc.) have a valence of 2, and are called divalent.

C. Oxidation State

Oxidation State is characterized by an oxidation number which is the charge one would expect for an atom if it were to dissociate from the surrounding molecule or ion. It may be either a positive or negative number, usually, an integer between -VII and +VII (Roman numerals are generally used to represent oxidation number). This concept is useful in balancing chemical equations and performing certain calculations. The rules for calculating oxidation number are as follows:

a. The oxidation number for atoms or ions simply equals the charge of the species. For example the oxidation number of sodium, Na+, or chloride, Cl-, ions is +I and -I respectively.

b. The oxidation number of atoms in an elemental molecule or homonuclear covalent molecule (e.g., oxygen, O=O) is zero.

c. The oxidation number of atoms in a covalent non-elemental molecule is determined in a stepwise fashion. Heteronuclear covalent bonds (i.e., where different atoms are joined together by a covalent bond) are generally polar, that is, the electrons are not shared evenly between the two atoms. Oxidation number is determined by imagining the charge that would exist if these polar bonds were to become completely ionic. In other words, the oxidation number is the charge on each atom after all bonding electrons have been assigned to the more electronegative of the two atoms joined by each bond. In general, the less metallic an atom is (the closer it is to the upper right hand corner of the periodic table), the more electronegative it is. However, when uncertain, one should consult Pauling's comparative electronegativities (see Table 2.1). Where the two atoms are identical, the covalent bond is non-polar and the bonding electrons are split evenly.

In most cases one can assign all hydrogens an oxidation state of +I (exception: hydrides[-I]), and oxygen an oxidation state of -II (exception: peroxides[-I]). Then, the molecule is split at the bonds between similar atoms (e.g., C-C and C=C bonds). The sum of all the valences in each fragment of the molecule must equal the overall charge of that portion of the molecule (usually zero). From this constraint, the oxidation state of the remaining atoms (usually carbon, nitrogen and sulfur) can be determined.

Table 2.1

Properties of the Stable Elements Footnote1

Element

Symbol

Atomic #

Atomic Wt.

Valence

Electronegativity

Aluminum

Al

13

26.98

3

1.47

Antimony

Sb

51

121.75

3,5

1.82

Argon

Ar

18

39.95

0


Arsenic

As

33

74.92

3,5

2.20

Barium

Ba

56

137.34

2

0.97

Beryllium

Be

4

9.01

2

1.47

Bismuth

Bi

83

208.98

3,5

1.67

Boron

B

5

10.81

3

2.01

Bromine

Br

35

79.91

1,3,5,7

2.74

Cadmium

Cd

48

112.40

2

1.46

Calcium

Ca

20

40.08

2

1.04

Carbon

C

6

12.01

2,4

2.50

Cerium

Ce

58

140.12

3,4

1.06

Cesium

Cs

55

132.91

1

0.86

Chlorine

Cl

17

35.45

1,3,5,7

2.83

Chromium

Cr

24

52.00

2,3,6

1.56

Cobalt

Co

27

58.93

2,3

1.70

Copper

Cu

29

63.54

1,2

1.75

Dysprosium

Cy

66

162.50

3

1.10

Erbium

Er

68

167.26

3

1.11

Europium

Eu

63

151.96

2,3

1.01

Fluorine

F

9

19.00

1

4.10

Gadolinium

Gd

64

157.25

3

1.11

Gallium

Ga

31

69.72

2,3

1.82

Germanium

Ge

32

72.59

4

2.02

Gold

Au

79

196.97

1,3

1.42

Hafnium

Hf

72

178.49

4

1.23

Helium

He

2

4.00

0


Holmiuum

Ho

67

164.93

3

1.10

Hydrogen

H

1

1.01

1

2.20

Indium

In

49

114.82

3

1.49

Iodine

I

53

126.90

1,3,5,7

2.21

Iron

Fe

26

55.85

2,3

1.64

Krypton

Kr

36

83.80

0


Lanthanium

La

57

138.91

3

1.08

Lead

Pb

82

207.19

2,4

1.55

Lithium

Li

3

6.94

1

0.97

Lutetium

Lu

71

174.97

3

1.14

Magnesium

Mg

12

24.31

2

1.23

Manganese

Mn

25

54.94

2,3,4,6,7

1.60

Table 2.1 cont.

Properties of the Stable Elements

Element

Symbol

Atomic #

Atomic Wt.

Valence

Electronegativity

Mercury

Hg

80

200.59

1,2

1.44

Molybdenum

Mo

42

95.94

3,4,6

1.30

Neodymium

Nd

60

144.24

3

1.30

Neon

Ne

10

20.18

0

1.07

Nickel

Ni

28

58.71

2,3

1.75

Niobium

Nb

41

92.91

3,5

1.23

Nitrogen

N

7

14.01

3,5

3.07

Osmium

Os

76

190.2

2,3,4,8

1.52

Oxygen

O

8

16.00

2

3.50

Palladium

Pd

46

106.4

2,4,6

1.39

Phosphorus

P

15

30.97

3,5

2.06

Platinum

Pt

78

195.09

2,4

1.44

Potassium

K

19

39.10

1

0.91

Praseodymium

Pr

59

140.91

3

1.07

Rhenium

Re

75

186.2


1.46

Rhodium

Rh

45

102.91

3

1.45

Rubidium

Rb

37

85.47

1

0.89

Ruthenium

Ru

44

101.07

3,4,6,8

1.42

Samarium

Sm

62

150.35

2,3

1.07

Scandium

Sc

21

44.96

3

1.20

Selenium

Se

34

78.96

2,4,6

2.48

Silicon

Si

14

28.09

4

1.74

Silver

Ag

47

107.87

1

1.42

Sodium

Na

11

22.99

1

1.01

Strontium

Sr

38

87.62

2

0.99

Sulfur

S

16

32.06

2,4,6

2.44

Tantalum

Ta

73

180.95

5

1.33

Tellurium

Te

52

127.60

2,4,6

2.01

Terbium

Tb

65

158.92

3

1.10

Thallium

Tl

81

204.37

1,3

1.44

Thorium

Th

90

232.04

4

1.11

Thulium

Tm

69

168.93

3

1.11

Tin

Sn

50

118.69

2,4

1.72

Titanium

Ti

22

47.90

3,4

1.32

Tungsten

W

74

183.85

6

1.40

Uranium

U

92

238.03

4,6

1.22

Vanadium

V

23

50.94

3,5

1.45

Xenon

Xe

54

131.30

0


Ytterbium

Y

39

88.91

2,3

1.06

Zinc

Zn

30

65.37

2

1.66

Zirconium

Zr

40

91.22

4

1.22

Table 2.2

Common Groups of Atoms

Name

Formula

Charge

Special Nomenclature

Ammonium

NH4

+1


Hydroxide

OH

-1


Bicarbonate

HCO3

-1

H2CO3-carbonic acid

Nitrate

NO3

-1

HNO3-nitric acid

Nitrite

NO2

-1

HNO2-nitrous acid

Permanganate

MnO4

-1


Hypochlorite

OCl

-1

HOCl-hypochlorous acid

Iodate

IO3

-1


Chlorate

ClO3

-1


Bromate

BrO3

-1


Chlorite

ClO2

-1


Chlorate

ClO3

-1


Perchlorate

ClO4

-1

HClO4-perchloric acid

Metaphosphate

PO3

-1

HPO3-metaphosphoric acid

Carbonate

CO3

-2


Sulfate

SO4

-2

H2SO4-sulfuric acid

Sulfite

SO3

-2


Dichromate

Cr2O7

-2


Phosphate (ortho-phosphate)

PO4

-3

H3PO4-phosphoric acid



Example 2.1: What is the oxidation state of the atoms in acetic acid?


First we know that hydrogen probably has an oxidation state of +I, and oxygen is -II. Then, we can break the atom at the carbon-carbon bond, and each half must have a total oxidation state of zero. Therefore, the carbon on the left-hand side must have an oxidation state of -III, and the one on the right side, +III. This is an example of the variable oxidation state of carbon, which ranges from -4 for methane, to +4 for carbon dioxide. Carbon may even be present in different oxidation states in the same molecule, as illustrated by this example.


D. Measures of Concentration

Quantitative analytical chemistry is based on the ability to measure concentration and express it in an unambiguous way. In the environmental sciences, concentrations can be expressed on a mass basis, a molar basis, or an equivalent basis.


1. Mass Basis.

This is simply an expression of the mass of analyte per volume of sample (e.g., per liter for an aqueous sample). Since most waters and wastewaters have a density nearly equal to pure water, one liter of these samples may be explicitly equated to one kilogram. Thus, for example, a 1 mg/L concentration might be expressed as 1 mg/kg. This is a dimensionless number equal to 1/1,000,000 or 1 part per million. For this reason, concentrations of mg/L and ppm are often used interchangeably. Table 2.3 lists mass/volume concentrations commonly used in the environmental field with equivalent mass/mass units for aqueous samples.

Table 2.3

Common Mass-Based Concentration Units

Mass/Volume Units

Mass/Mass Units

Typical Applications

g/L (grams/liter)

(parts per thousand)

Stock solutions

mg/L (milligrams/liter)

10-3g/L

ppm (parts per million)

Conventional pollutants

(DO, nitrate, chloride)

µg/L (micrograms/liter)

10-6g/L

ppb (parts per billion)

Trihalomethanes, Phenols.

ng/L (nanograms/liter)

10-9g/L

ppt (parts per trillion)

PCBs, Dioxins

pg/L (picograms/liter)

10-12g/L


Pheromones


For highly concentrated stock solutions, especially acids and bases, concentrations are sometimes expressed as the ratio of commercial compound to water. For example, 1 + 3 HCl is prepared by adding one volume of hydrochloric acid (conc.) to three parts distilled water. Thus, it is 25% of the concentration of commercial concentrated hydrochloric acid.

Concentration can also refer to a specific part of a molecule. For example, a solution of potassium sulfite will contain a certain concentration of K2SO3. However, one may wish to know the concentration of sulfite only, or perhaps any one of the elemental constituents: potassium, sulfur or oxygen.


2. Molar Concentrations.

Molar concentrations are expressed as the number of moles of a substance present in one liter volume. A mole is a gram molecular weight (GMW) or more generally, a gram formula weight (GFW) of a substance. This corresponds to the quantity of substance in grams which is equal to the atomic weight of the substance, whether it be an atom, a molecule or an ion. The utility of these units is that one mole contains the same number of atoms, molecules or ions (Avogadro's Number, 6.02x1023) regardless of the identity of the substance. A solution of 1 mole of a substance dissolved in a liter of water (i.e, 1 mole/L) is called a 1 Molar solution, and is said to have a Molarity of one.

(2.7a)

or more generally:

(2.7b)


Example 2.2: What is the concentration in grams/liter of a 1 Molar solution of ammonium sulfate, (NH4)2SO4?

2 x MW(N) = 2 x 14 = 28
8 x MW(H) = 8 x 1 = 8
1 x MW(S) = 1 x 32 = 32
4 x MW(O) = 4 x 16 = 64
GMW = 132
Answer: 132 g/L.


3. Equivalent Concentrations.

Equivalent concentration or normality is commonly used with acid/base or oxidation/reduction reactions. It is calculated such that one equivalent of a substance will react with exactly one equivalent of another substance. A 1 Normal solution contains 1 gram equivalent weight (GEW) of a substance per liter of volume.


(2.8)

A gram equivalent weight is the mass of the substance which contains one gram atom of "available" hydrogen or its equivalent.

(2.9)


where Z is some positive integer (usually 1,2, or 3) which represents the number of equivalents per mole. A solution containing one equivalent per liter is said to be 1 Normal (or 1 N). Solutions of fractional normality are often expressed as a fraction; for example, 0.25 Normal may be abbreviated as N/4.

From equations 2.7, 2.8 and 2.9, the following relationship between molarity and normality can be derived. Note that since Z is generally equal to or greater than unity, the normality of a solution will be equal to or greater than its molarity.

Normality = Molarity * Z (2.10)

For acids, Z is simply the number of protons that will be donated.

Z = 1, for monoprotic acids (e.g., hydrochloric acid or acetic acid)

HCl ---------> H+ + Cl- (2.11)

CH3COOH -----> CH3COO- + H+ (2.12)

Z = 2, for diprotic acids (e.g., sulfuric acid)

H2SO4 --------> 2H+ + SO42 (2.13)

Z = 3, for triprotic acids (e.g., phosphoric acid)

H3PO4 --------> 3H+ + PO43 (2.14)

For bases, Z is the number of hydroxide ions liberated, because one hydroxide neutralizes one proton to form water.

Z = 1, for mono-hydroxides (e.g., sodium hydroxide)

NaOH -----------> Na+ + OH- (2.15)

Z = 2, for di-hydroxides (e.g., calcium hydroxide)

Ca(OH)2 ----------> Ca+ + 2OH- (2.16)

For species undergoing oxidation or reduction (redox) reactions, Z is the number of electrons transferred per molecule.

Z = 1, for single electron transfers, such as the oxidation of ferrous iron to ferric iron.

Fe+2 -------------> Fe+3 + e- (2.17)

Z = 6, for six electron transfers, such as the reduction of potassium dichromate to trivalent chromium.

K2Cr2O7 + 7H+ + 6e- ----------> 2K+ + 2Cr+3 + 7OH- (2.18)

For other reactions such as precipitation or complexation, Z will depend on the particular stoichiometry. However, in most cases the value of Z will be equal to the value of the oxidation state of the atom (or group) that will be reacting times the number of these atoms (or groups) that are bound in the reacting molecule. For example there are two atoms of Al(+III) in one molecule of alum (Al2(SO4)3 18H2O). Therefore, the Z value for alum is equal to six.


Example 2.3: Consider a solution of Ammonium Sulfate prepared by dissolving 66 g of the anhydrous compound in water and diluting to 1 liter. What is the concentration of this solution in:

a) g/L?

b) moles/L?

c) equivalents/L?

d) g/L as sulfate?

e) g/L as N?

Answer:

a) 66 g/L

b) In example 2.1, the gram molecular weight of ammonium sulfate was determined to be 132 g/mole. So, using equation 2.7, on gets:

Molarity = 132 g/mole = 0.5 moles/L or 0.5 M.

c) Without any specific information regarding the use of this solution, one might simply presume that either the sulfate group or the ammonium group will be the reacting species. In either case, Z should be equal to two (product of the oxidation state times the number of groups). Using equation 2.10, one calculates:

Normality = 0.5 moles/L * 2 equivalents/mole

= 1 equivalent/L or 1.0 N or N/1.

d) The GFW for sulfate is:

GFW = 32 + 4*16 = 96.

The molarity of sulfate is:

Molarity = 0.5 moles-(NH4)2SO4/L * 1 mole-SO4/mole-(NH4)2SO4

= 0.5 moles-SO4/L

Then, rearranging equation 2.7b, one gets:

mass/L = Molarity * GFW = 0.5 moles-SO4/L * 96 g-SO4/mole-SO4

= 48 g-SO4/L

e) The GFW for nitrogen is simply 14:

The molarity of nitrogen is:

Molarity = 0.5 moles-(NH4)2SO4/L * 2 moles-N/mole-(NH4)2SO4

= 1 mole-N/L

Again, rearranging equation 2.7b, one gets:

mass/L = Molarity * GFW = 1 mole-N/L * 14 g-N/mole-N

= 14 g-N/L or 14 g NH3-N/L


E. pC

pC is defined as the negative of the logarithm of the molar concentration of any chemical species, "C" (equation 2.19). This notation is most commonly used in conjunction with the hydrogen ion concentration (i.e, pH). Since hydrogen ions react with so many species found in water, their concentration is critical to understanding the kinetics and thermodynamics of aquatic chemical processes. It is often easiest to base chemical models of such systems on pH, and as a result pH has been referred to as the "master variable" (see Stumm & Morgan, 1981, Chapt.3)

pC = -log[C] (2.19)

F. Balancing Chemical Equations

Balanced chemical equations conform to the laws of conservation of mass and conservation of charge. The law of conservation of mass dictates that the total number of atoms of each type on one side of the equation must equal the number on the other. Conservation of charge requires that the net charge of all reactants equal the net charge of all the products. In order to obtain a balanced equation one must start with accurate knowledge of the identity of all reactants and all products. Then the laws of conservation of mass and charge may be satisfied by adjusting the coefficients associated with any of the reactants or products. Frequently, this is not enough. One might also have to add a variable number of water molecules (H2O) or its constituents (H+ or OH-) to either side. This is an acceptable practice, because it is very difficult to determine if these species are produced or consumed by a reaction carried out in dilute aqueous solution. However, it is well established that they are common participants in aqueous-phase reactions.



PROBLEMS

2.1 Calculate the gram molecular weight of: (a) NaNO3, (b) Mg(OH)2, (c) Al2(SO4)3, (d) KMnO4.

2.2 How much potassium dichromate must be added to a liter of water to make a 0.05 molar solution?

2.3 What is the gram equivalent weight of: (a) HClO4, (b) BaSO4?

2.4 Balance the following equations:

a) CaCl2 + Na2CO3 ----------> CaCO3 + NaCl

b) MnO2 + NaCl + H2SO4 ---------> MnSO4 + H2O + Cl2 + Na2SO4

c) C6H4(COOH)2 + O2 ----------> CO2



Footnote1

from; The Chemists Companion: A Handbook of Practical Data, Techniques and References. A.J. Gordon & R.A. Ford, J. Wiley & Sons Publ., New York, 1972.