CH221 CLASS 3 CHAPTER 2: POLAR COVALENT BONDS; ACIDS AND BASES Synopsis. The third class deals with ideas about polar covalent bonds, electronegativity, dipole moments, formal atomic charges and resonance. My name is Bond, Covalent Bond: shared not taken Polar Covalent Bonds and Electronegativity The two major types of chemical bonding: ionic bonding, involving complete electron transfer, and covalent bonding, involving sharing of electrons, are in reality descriptions of two extreme circumstances. The electronic nature of most chemical bonds lies somewhere between these two extremes. In particular, many bonds in organic molecules may be described as polar covalent bonds, indicating that the bond electrons are not shared equally (symmetrically), meaning that the electron distribution in the bond is not symmetrical. Bond polarity occurs when there is a difference in electronegativity between the bonded atoms. Electronegativity is the term used to describe the ability of a bonded atom to attract bond electrons: it can be can be measured on a scale (devised by L Pauling and R Mulliken) that arbitrarily sets the electronegativity of hydrogen as 2.1. All the other elements then take up values between 0.7 (Cs) and 4.0 (F), as shown on the next page. Group Period 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 1 H 2.1 2 Li Be 0.98 1.57 B C N O F Ne 2.04 2.55 3.04 3.44 3.98 0 Na Al 3 He 0 Mg 0.93 1.31 Si P S Cl Ar 1.61 1.9 2.19 2.58 3.16 0 4 K Ca 0.82 1 Sc Ti V Cr Mn Fe Co Ni Cu Zn Ga Ge As Se Br Kr 1.36 1.54 1.63 1.66 1.55 1.83 1.88 1.91 1.9 1.65 1.81 2.01 2.18 2.55 2.96 0 5 Rb Sr Y Zr Nb Mo Tc Ru Rh Pd Ag Cd In Sn Sb Te I Xe 0.82 0.95 1.22 1.33 1.6 2.16 1.9 2.2 2.28 2.2 1.93 1.69 1.78 1.96 2.05 2.1 2.66 2.6 6 Cs Ba La Hf Ta W Re Os Ir Pt Au Hg Tl Pb Bi Po 0.79 0.89 1.1 1.3 1.5 2.36 1.9 2.2 2.2 2.28 2.54 2 2.04 2.33 2.02 2 7 Fr Ra Ac Rf 0.7 0.89 1.1 Lanthanides Actinides Db Sg Bh Hs Mt At Rn 2.2 0 Uun Uuu Uub Ce Pr Nd Pm Sm Eu Gd Tb Dy Ho Er Tm Yb Lu 1.12 1.13 1.14 1.13 1.17 1.2 1.2 1.1 1.22 1.23 1.24 1.25 1.1 1.27 Th Pa U Np Pu Am Cm Bk Cf Es Fm Md No Lr 1.3 1.5 1.38 1.36 1.28 1.3 1.3 1.3 1.3 1.3 1.3 1.3 1.3 Key: Electronegativity No 0-.66 .66-1 1-1.33 1.33-1.66 1.66-2 2-2.33 2.33-2.66 2.66data Polar covalent bonds have tiny dipole moments arising from the charge separation in the bond, as illustrated below H3C F H3C Li Electronegativity of carbon is less than that of fluorine, but greater than that of lithium The ability of an atom to polarize a bond is often called the inductive (I) effect. Atoms of low electronegativity, like Li (above) and Mg are electron donors (+I), whereas atoms of high electronegativity, like N, O and F, are electron withdrawers (-I). The inductive effects in polar covalent bonds play a major part in the understanding of chemical reactivity and will be much used in future. Polar Covalent Molecules: Dipole Moments The dipole moment () of a molecule is a useful measure of the polar character of the molecule and can be measured in the laboratory, using electromagnetic or spectroscopic methods. It can be regarded as the vector sum of the individual bond dipole moments, which are discussed next. Definition of dipole moment: if two charges of equal magnitude and opposite sign (i.e. +Q and –Q) are separated by a distance R, then Dipole moment () It is symbolized as shown above = QR Units of Dipole Moment and Estimation of Bond Polarity The SI unit of is coulomb.meters, but for atomic systems, a more useful unit is the debye (D), which is equal to 3.336 x 10-30 coulomb.meters. 1D is defined as the dipole moment of two charges +e and –e that are 0.2082Å apart. (1Å = 100 pm). Therefore, if is the fraction of charge ( e) on each atom of a bond, which are R (Å) apart (i.e. Q = e), then = R 0.2082 E.g. For CH3Cl, the measured dipole moment is 1.87D and RC-Cl is known to be 178 pm (= 1.78 Å). Assume the total contribution to the measured dipole moment comes from the C-Cl bond. Then, = or = 1.87 = 1.78 0.2082 0.22 That means that the fraction of unit charge on carbon is +0.22e and on chlorine is –0.22e: the C-Cl bond is 22% ionic. The molecular dipole moment, being the vector sum of the bond dipole moments, is very much dependent upon molecular geometry, as illustrated by the examples below. Net .. H :O H = 1.85D H Net :N H H = 1.47D Cl C Cl Cl Cl Net: zero O=C=O Net: zero = 0D = 0D The two lower molecules have symmetrical structures and hence the individual bond polarities exactly cancel. Class Question Make three-dimensional drawings of the following molecules and predict which have dipole moments. Show the direction of the dipole moment. (a) 1,1-Dichloroethene (b) trans-1,2-Dichloroethene (c) cis-1,2-Dichloroethene (d) Tetranitromethane (e) Trichloromethane (chloroform) (f) Carbon oxysulfide (OCS) (g) Sulfur dioxide (h) Ethylene Formal Charges in Polar Molecules The assignment of formal charges to specific atoms in a molecule is closely related to the previously discussed ideas of bond polarity and dipole moment. Formal charges are most important for molecules that contain atoms with an abnormal number of bonds (e.g. 3 bonds, instead of 4 bonds for carbon, 4 bonds instead of 3 bonds for nitrogen, etc). Formal charge is defined below. Some examples are given on the next page. Class Question Determine the formal charges for the non-hydrogen atoms in the following molecules. (a) CH2=N=N (diazomethane) (b) (CH3)3N-O(trimethylamine oxide) (c) CH3-NC (methyl isocyanide (d) Ph-N=N=N (phenyl azide) Examples 1. No "abnormal" valence H Chloromethane .. H :C: H .. FC = 4 - 4 - 0 = 0 :Cl: .. H:N:H .. H :C: H .. H FC = 7 - 1 - 6 = 0 FC = 5 - 3 - 2 = 0 FC = 4 - 4 - 0 = 0 Methylamine 2. "Abnormal" valence present O Nitromethane FC = 6 - 2 - 4 = 0 H O .. H:C:N .. H O Dimethyl sulfoxide FC = 5 - 4 - 0 = +1 S N FC = 6 - 6 - 1 = -1 ) O FC = 6 - 6 - 1 = -1 O CH3 (i.e. CH3 (i.e. (CH3)2S O) FC = 6 - 3 - 2 = +1 CH3 Note that expanded valence (via use of d orbitals) is allowed for period 3 elements and beyond, so that dimethyl sulfoxide can also be written (CH3)2S=O A summary of formal charges for C, N and O is given in Table 2.2, on p. 36 of the textbook. Resonance For many molecules, a single Lewis structure or line-bond structure does not fully represent the actual structures of the molecules, as determined by experiment, notably X-ray, electron and neutron diffraction methods. These molecules, which are illustrated by conjugated unsaturated groups or aromatic rings, can only be satisfactorily represented by a number of line-bond structures, each of which contributes a certain amount to the overall (real) structure. This is demonstrated for nitromethane, overleaf. O O N CH3 CH3 N O O O Overall CH3 N O Measured rNO = 122 pm, for both bonds rN=O = 116 pm rN-O = 130 pm The two conventional line-bond structures above differ only in electron distribution (position of double bond and lone pairs): they are known as resonance structures and the phenomenon is called resonance. The overall (actual) structure can be considered to be formed by the combination (in this case equal combination) of the two resonance structures and is known as a resonance hybrid. The actual structure, represented by the resonance hybrid, is more stable (of lower energy) than any of the individual resonance structures, and hence resonance leads to stabilization. Other important examples include benzene and carboxylate ions. Other, less favorable resonance structures are not shown Measured rCC = 138 pm, for all CC rC=C = 134 pm bonds rC-C = 154 pm Overall O O R C R O Overall O R C O Measured rCO= 127 pm C O rC=O = 120 pm rC-O = 135 pm for both The Rules of Resonance 1. Whenever a molecule can be represented by two or more structures that differ ONLY in the arrangement of electrons, there is said to be resonance. The individual structures are called RESONANCE STRUCTURES. The actual structure of the molecule is a RESONANCE HYBRID of those structures and cannot be satisfactorily represented by any one of them. Instead, each resonance structure contributes a certain amount to the overall structure of the molecule. 2. The actual structure of the molecule (represented by the resonance hybrid) is more stable than any of the contributing resonance structures. The energy difference is known as the RESONANCE ENERGY and the more nearly equal in stability of resonance structures, the greater the resonance energy. 3. Resonance is important when resonance structures are of about equal stability (i.e. of about the same energy) as in the case of nitromethane. The amount of contribution of each resonance structure depends on the relative stability of that structure. Generally, the greater the number of charges, the less stable is the structure. This point is illustrated in 2, above. Also structures with like charges on adjacent atoms are unstable, as are those that require redistribution of electrons in the reverse direction of electronegativity difference. An example of the latter is >C=O major >C+-Ominor >C--O+ (insignificant) 4. Stabilization can be achieved in saturated molecules by HYPERCONJUGATION or “NO-BOND RESONANCE”. E.g. the ethyl radical H H C H H . CH2 H C CH2 H . C H major all minor OR H C C CH2 H C . H H H H H . H H H CH2