d-block Elements



General Characteristics of d-block Elements

1.    Melting and Boiling Point
Transition metals are hard having high melting point (melting point of Fe = 1535°C) and boiling point (boiling point of Fe = 2800°C). The hardness, high melting point and high boiling point are attributed to their small atomic size producing strong interatomic attraction and presence of greater number of valence electrons available for interaction. (The strength of bonding between the atoms of metals depends upon the interaction between the electrons in their outermost shell). Greater the number of valence electrons available for interaction, the stronger will be the resulting bonding and higher will be melting point and boiling point Transition metals have 3 or more electrons available for bonding. Hence the interatomic bonding is very strong. That is why their melting point and boiling point are high.

Zinc (m.p. = 419°C and b.p. = 907°C), Cd (m.p. = 320.9°C and b.p. = 765°C) and Hg (m.p. = - 38.4°C and b.p. = 357°C) are notable exceptions and have exceptionally and relatively low values of melting point and boiling points.

The reason of their low melting point and boiling point is due to their filled (n – 1) d-orbitals with no unpaired electrons [ns2 (n–1)d10]. Due to completely filled d-orbital, d-orbitals, d-electrons are not available for interatomic bonding.  Hence their melting point and boiling point are comparatively low.

There is a regular increase in melting and boiling points across each transition series along each period (except in Mn, Ni, Cu which have usually weaker IBF) due to decrease in atomic radii and increase of number of valence electrons. [In first transition series, vanadium has the highest melting point while scandium has the highest boiling point]. The melting point and boiling point increase along a each transition series and reach a maximum in the middle of the series (near group VB and VIB) and then decreases beyond VIB. In moving across a transition series, the number of unpaired d-electrons rises to maximum of five in group VIB beyond which electron pairing begins.


The melting and boiling point of d-block elements increase on descending a group due to increasing atomic mass. 
2. Interstitial Compound Formation
Transition elements form compounds of indefinite structures and properties and variable composition which are called Interstitial compounds which are non-stoichiometric compounds formed by the adsorption (penetration) of small, non-metallic atoms like H, B, C, N into the interstices of lattice of transition metals.

These compounds are non-stoichiometric as atoms are not present in simple ratios and have variable composition. So they are not true compounds because they are not in accordance with laws of chemical combination. For the same reason, they cannot be expressed by simple chemical formula. e.g. TiH1.73, VH0.56, LaH2.76, CeH2.69, CuH22.3.

This non-stoichiometry (i.e. non-stoichiometric compound formation) is due to their variable oxidation states and due to their defects in their lattices. In their solid crystal lattice, there are holes (i.e. inter-atomic spaces or interstices or void spaces) where small atoms like C, H, B, N etc are adsorbed to form their hydrides, carbides, borides and nitrides respectively giving a solid solution.

The non-stoichiometry of compounds of transition metals with O, S, Se and Te is very prominent. e.g. in ferrous oxide (FeO) ratio of Fe and O is not 1:1 but the composition varies between Fe0.94O and Fe0.84O showing non-stoichiometric nature of compound. Vanadium selenide is in another non-stoichiometric compound whose composition varies between VS0.98 and VS2.

3.    Variable Oxidation States
Transition elements exhibit a variety of oxidation states (except Zn, Cd, Sc, Y etc.) from 0 to +8 (found in ruthenium and osmium e.g RuO4, OsO4 etc) in their compounds. The lower oxidation states are generally obtained by the loss of ns electrons while higher oxidation states are achieved by sharing ns and all or some of the (n – 1 )d-electrons. In their lower oxidation states, they form ionic compounds but in their higher oxidation states they form covalent compounds. Their maximum oxidation states are largely confined to +2 to +3 but it may exceed to +3 which are only rare. (e.g. Fe shows +4, +5, +6 and Ru and Os show +8 oxidation states). The different pattern in oxidation states of Fe, Ru and Os is attributed mainly to increased size facilitating the loss of more than one 3d electrons).

The exhibition of variable oxidation states is attributed mainly due to small energy difference between ns and (n – 1)d-orbitals and partly due to partially filled (n – 1)d-orbital. Thus both ns and (n – 1)d-electrons participate in compound formation giving rise to their variable oxidation states. Along with ns electrons, one, two or more (n – 1) d-electrons may be removed or shared. For example; titanium (Z = 22) shows an oxidation state of +2 if both 4s electrons are used for bonding and show additional oxidation states of +3 and +4 when one and two 3d-electrons are also removed respectively in addition to 4s electrons. Similarly, in Vanadium (Z = 23) if only 4s electrons are removed, it will show oxidation state +2. If in addition, 1, 2 or 3, 3-d-electrons are also removed, it will show additional oxidation states of +3, +4 and +5 respectively.

Maximum oxidation state is equal to the sum of the number of ns electrons and number of unpaired (n – 1)d-electrons. For example:








The maximum oxidation state in first transition series increases from Sc (+3) to Mn (+7) then decreases from Fe (+6) to Zn (+2) as d-electrons pair up.

Maximum oxidation state is not stable. Therefore, most common oxidation states are +2 and +3. More commonly, only one electron may be removed from 3d. Thus cobalt does not show +5 oxidation state.

The stability of lower oxidation state (+2) relative to higher oxidation state (+3 or even higher) increases from left to right across the series with increasing atomic number (nuclear charge). It reflects the increasing difficulty of removing a (n – 1) d-electrons as the nuclear charge increases.

The stability of higher oxidation state (+3 or even higher) relative to lower oxidation state (+2) increases from top to bottom down the group with increasing atomic number (nuclear charge). It reflects the increasing readiness of removing a (n – 1) d-electrons as the nuclear charge decreases due to increasing atomic size.

4.    Catalytic Property
Catalysts are the chemical substances that accelerate or retard the rate of reaction either by forming unstable intermediate compound or by change of oxidation state. Many transition elements (V, Fe, Co, Ni, Mo, Pd, W, Pt etc) and a variety of transition metal compounds especially their oxides (V2O5, MnO2, Fe2O3, ZnO, Cr2O3, FeSO4 etc.) exhibit remarkable catalytic properties and are wonderful and effective catalysts for hydrogenation, oxidation, dehydration etc. Some industrial reactions which are catalyzed by transition metals and their compounds are:

1. Finely divided Ni or Pd are used in hydrogenation of unsaturated oils.(Sabatier-Senderen’s Reaction)
2. Finely divided Fe and Mo are used in manufacture of ammonia     (Haber’s process)
3. Pt or Pt-Rh alloy is used for oxidation of ammonia into NO        (Ostwald’s Process).
4. Pt or V2O5 is used for oxidation of SO2 into SO3 in the manufacture of H2SO4. (Contact Process)
5. ZnO-Cr2O3 (Zinc chromite) is used in the synthesis of methanol   (Petret Process)
6. Ziegler-Natta catalyst (TiCl4.AlR3)) is used in polymerization of olefins.
7. Fenten’s reagent (FeSO4 + H2O2) is used for oxidation of alcohols to aldehydes.

Their catalytic properties of transition metals are mainly due to following reasons:

1. The presence of vacant d-orbitals.
2. The tendency to exhibit variable oxidation states.
3. The ability to form high energy reaction intermediates with reactants.
4. The presence of defects (void spaces) in their crystal lattice.

[The availability of vacant orbitals, allowing reactants (which are gases) to be absorbed on their surfaces and bringing them closer for the reaction e.g. Ni is used in hydrogenation of vegetable oils into vegetable ghee. In addition they have ability to form Activated Complex of lower activation energy thereby providing low energy pathway for the reaction by either forming unstable Intermediate Compound or by change of oxidation states. e.g. V2O5 acts as catalyst in oxidation of SO2 into SO3. Here vanadium undergoes oxidation state change from +5 to +4].

V2O5
+
SO2
¾¾®
V2O4
+
SO3

2V2O4
+
O2
¾¾®
2V2O5




5. Magnetic Property of transition elements
Most of the transition elements and their compounds exhibit Paramagnetism and are paramagnetic. The substances which are weakly attracted by magnetic field are called paramagnetic substances.  Paramagnetism is due to the presence of unpaired electrons in an atom, ion or molecule, because there is a magnetic moment associates with spinning electron. The spin and revolution of an electron creates a magnetic field around it and it behaves as a small magnet, and hence is attracted by another magnets. Since transition elements have unpaired electrons in d-orbitals, they are attracted by magnetic field and so they are paramagnetic.                                                                                                                   

The magnetic moment (μs) increases with an increase in the number of unpaired electrons. Since number of unpaired electrons first increases from 1-5 (till VIIB) and then decreases gradually and finally become zero from left to right, therefore, Paramagnetism first increases in any transition elements series around the middle of the series and then decreases. Thus paramagnetic behaviour is the strongest for Fe3+ and Mn2+ both containing 5 unpaired electrons each and decreases on both sides of the first transition series. 


The substances which are weakly repelled by magnetic field are called diamagnetic substances. The diamagnetism is due to the presence of paired electrons. When the electrons are paired in an orbital, then magnetic moments of all paired electrons cancelled out and the substance becomes diamagnetic. Zinc and Cadmium are have d10 configuration containing all the paired electrons, so they are not attracted in a magnetic field and are diamagnetic.


Certain transition elements like Iron, Cobalt and Nickel and their compounds such as CrO2 which can be magnetized showing strong Paramagnetism and are strongly attracted in magnetic field are called ferromagnetic materials. They show permanent magnetism even when the magnetic field is removed. [CrO2 is ferromagnetic material used in the manufacture of audio and video tapes]. Ferromagnetism is due to a spontaneous alignment of the magnetic dipoles in the same direction. However, for each ferromagnetic material there is a critical temperature above which no ferromagnetism is observed. This temperature is called the Curie temperature. 
6. Complex Formation
Transition metals form complexes or co-ordination compounds in which metal atom or ion (central atom) is surrounded by a number of oppositely charged ions or neutral molecules called Ligands.  Ligands donate its lone pairs to central metal atom (centre of coordination) and are attached to the metal atom by co-ordinate bond, hence the name co-ordination compounds.

Transition metals form complexes due to 3 reasons:
1.    Small size of their atoms.
2.    Highly effective nuclear charge of their cations.
3.    Presence of vacant d-orbitals available for chemical bonding.     

Parts of Complex

1. Central Atom
It is an atom or ion of transition metal bounded by ligand through co-ordinate bond.

2. Ligands
Groups surrounding the central metal atom by donating its lone pair of electrons are called ligands. They are Lewis Base.  They may be negative, neutral or positive.

3. Co-ordination Number
The no. of ligands bounded or attached to the central atom are called co-ordination number.

4. Complex Ion
Group comprising of central atom and its ligands carrying +ive or –ive charge is called Complex Ion.














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XII Stereoisomerism and Its Types