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Azeotropes are defined as the mixtures of liquids which boil at constant temperature like a pure liquid and possess same composition of components in liquid as well as in vapour phase. Azeotropes are also called constant boiling mixtures because whole of the azeotropes changes into vapour state at constant temperature and their components can not be separated by fractional distillation. Azeotropes are of two types as described below,   (1) Minimum boiling azeotrope : For the solutions with positive deviation there is an intermediate composition for which the vapour pressure of the solution is maximum and hence, boiling point is minimum. At this composition the solution distills at constant temperature without change in composition. This type of solutions are called minimum boiling azeotrope. e.g., \[{{H}_{2}}O+{{C}_{2}}{{H}_{5}}OH,{{H}_{2}}O+{{C}_{2}}{{H}_{5}}C{{H}_{2}}OH\] \[CHC{{l}_{3}}+{{C}_{2}}{{H}_{5}}OH\], \[{{(C{{H}_{3}})}_{2}}CO+C{{S}_{2}}\]   (2) Maximum boiling azeotrope : For the solutions with negative deviations there is an intermediate composition for which the vapour pressure of the solution is minimum and hence, boiling point is maximum. At this composition the solution distill`s at constant temperature without the change in composition. This type of solutions are called maximum boiling azeotrope. e.g., \[{{H}_{2}}O+HCl,{{H}_{2}}O+HN{{O}_{3}},{{H}_{2}}O+HCl{{O}_{4}}\]

Ideal And Non-Ideal Solutions
Ideal solutions Non-ideal solutions
Positive deviation from Raoult's law Negative deviation from Raoult's law
1.     Obey Raoult's law at every range of concentration. 1.     Do not obey Raoult's law. 1. Do not obey Raoult's law.
2.       \[\Delta {{H}_{\text{mix}}}=0;\]neither heat is evolved nor           absorbed during dissolution.  2.     \[\Delta {{H}_{\text{mix}}}>0.\]Endothermic dissolution; heat is absorbed.  2. \[\Delta {{H}_{\text{mix}}}<0.\] Exothermic dissolution; heat is evolved. 
3.     \[\Delta {{V}_{\text{mix}}}=0;\]total volume of solution is equal to sum of volumes of the components. 3.     \[\Delta {{V}_{\text{mix}}}>0.\]Volume is increased after dissolution. 3.     \[\Delta {{V}_{\text{mix}}}<0.\] Volume is decreased during dissolution.
4.        \[P={{p}_{A}}+{{p}_{B}}=p_{A}^{0}{{X}_{A}}+p_{B}^{0}{{X}_{B}}\]i.e.,         \[{{p}_{A}}=p_{A}^{0}{{X}_{A}}:{{p}_{B}}=p_{B}^{0}{{X}_{B}}\] 4.     \[{{p}_{A}}>p_{A}^{0}{{X}_{A}};\] \[{{p}_{B}}>p_{B}^{0}{{X}_{B}}\]         \[\therefore \] \[{{p}_{A}}+{{p}_{B}}>p_{A}^{0}{{X}_{A}}+p_{B}^{0}{{X}_{B}}\] 4.     \[{{p}_{A}}<p_{A}^{0}{{X}_{A}};\]\[{{p}_{B}}<p_{B}^{0}{{X}_{B}}\]         \[\therefore \] \[{{p}_{A}}+{{p}_{B}}<p_{A}^{0}{{X}_{A}}+p_{B}^{0}{{X}_{B}}\]
5.     \[A-A,\ A-B,\ B-B\] interactions should be same, i.e., 'A' and 'B' are identical in shape, size and character. 5.     \[A-B\] attractive force should be weaker than \[A-A\] and \[B-B\] attractive forces. 'A' and 'B' have different shape, size and character.   5.     \[A-B\]attractive force should be greater than \[A-A\] and \[B-B\] attractive forces. 'A' and 'B' have different shape, size and character.
6.     Escaping tendency of 'A' and 'B' should be same in pure liquids and in the solution. 6.     'A' and 'B' escape easily showing higher vapour pressure than the expected value. 6.     Escaping tendency of both components 'A' and 'B' is lowered showing lower vapour pressure than expected ideally.
Examples: Dilute solutions; benzene + toluene: n-hexane + n-heptane; chlorobenzene + bromobenzene; ethyl bromide + ethyl iodide; n-butyl chloride + n-butyl bromide   Examples: Acetone +ethanol acetone +\[C{{S}_{2}}\]: water + methanol; water + ethanol; \[CC{{l}_{4}}+\]toluene; \[CC{{l}_{4}}+CHC{{l}_{3}}\]; acetone + benzene; \[CC{{l}_{4}}+C{{H}_{3}}OH\]; cyclohexane + ethanol Examples: Acetone + aniline; acetone + chloroform; \[C{{H}_{3}}OH\ +\ C{{H}_{3}}COOH\]; \[{{H}_{2}}O\ +\ HN{{O}_{3}}\] chloroform + diethyl ether; water + HCl; acetic acid + pyridine; chloroform + benzene  
  Graphical representation of ideal and non-ideal solutions more...

The pressure exerted by the vapours above the liquid surface in equilibrium with the liquid at a given temperature is called vapour pressure of the liquid. The vapour pressure of a liquid depends on, (1) Nature of liquid : Liquids, which have weak intermolecular forces, are volatile and have greater vapour pressure. For example, dimethyl ether has greater vapour pressure than ethyl alcohol. (2) Temperature : Vapour pressure increases with increase in temperature. This is due to the reason that with increase in temperature more molecules of the liquid can go into vapour phase. (3) Purity of liquid : Pure liquid always has a vapour pressure greater than  its solution. Raoult’s law : When  a non-volatile substance is dissolved in a liquid, the vapour pressure of the liquid (solvent) is lowered. According to Raoult’s law (1887), at any given temperature the partial vapour pressure (pA) of any component of a solution is equal to its mole fraction (XA) multiplied by the vapour pressure of this component in the pure state \[(p_{A}^{0})\]. That is,   \[{{p}_{A}}=p_{A}^{0}\times {{X}_{A}}\] The vapour pressure of the solution \[({{P}_{total}})\] is the sum of the partial pressures of the components, i.e., for the solution of two volatile liquids with vapour pressures \[{{p}_{A}}\] and \[{{p}_{B}}\]. \[{{P}_{total}}={{p}_{A}}+{{p}_{B}}=(p_{A}^{0}\times {{X}_{A}})+(p_{B}^{0}\times {{X}_{B}})\] Alternatively, Raoult’s law may be stated as “the relative lowering of vapour pressure of a solution containing a non-volatile solute is equal to the mole fraction of the solute in the solution.” Relative lowering of vapour pressure is defined as the ratio of lowering of vapour pressure to the vapour pressure of the pure solvent. It is determined by Ostwald-Walker method. Thus according to Raoult’s law, \[\frac{{{p}^{0}}-p}{{{p}^{0}}}=\frac{n}{n+N}=\frac{\frac{w}{m}}{\frac{w}{m}+\frac{W}{M}}\] where, \[p=\] Vapour pressure of the solution \[{{p}^{0}}=\]Vapour pressure of the pure solvent \[n=\] Number of moles of the solute  \[N=\] Number of moles of the solvent \[w\] and \[m=\] weight and mol. wt. of solute \[W\] and \[M=\] weight and mol. wt. of the solvent. Limitations of Raoult’s law
  • Raoult’s law is applicable only to very dilute solutions.
  • Raoult’s law is applicable to solutions containing non-volatile solute only.
  • Raoult’s law is not applicable to solutes which dissociate or associate in the particular solution.

Certain properties of dilute solutions containing non-volatile solute do not depend upon the nature of the solute dissolved but depend only upon the concentration i.e., the number of particles of the solute present in the solution. Such properties are called colligative properties. The four well known examples of the colligative properties are, (1) Lowering of vapour pressure of the solvent. (2) Osmotic pressure of the solution. (3) Elevation in boiling point of the solvent. (4) Depression in freezing point of the solvent. Since colligative properties depend upon the number of solute particles present in the solution, the simple case will be that when the solute is a non-electrolyte. In case the solute is an electrolyte, it may split to a number of ions each of which acts as a particle and thus will affect the value of the colligative property. Each colligative property is exactly related to other, Relative lowering of vapour pressure, elevation in boiling point and depression in freezing point are directly proportional to osmotic pressure. 

Concentration of solution is the amount of solute dissolved in a known amount of the solvent or solution. The concentration of solution can be expressed in various ways as discussed below, (1) Percentage : It refers to the amount of the solute per 100 parts of the solution. It can also be called as parts per hundred (pph). It can be expressed by any of following four methods, (i) Weight to weight percent % w/w \[=\frac{\text{Wt}\text{. of solute}}{\text{Wt}\text{. of solution}}\times 100\] Example : 10% \[N{{a}_{2}}C{{O}_{3}}\] solution w/w means \[10g\] of \[N{{a}_{2}}C{{O}_{3}}\] is dissolved in \[100g\] of the solution. (It means \[10g\] \[N{{a}_{2}}C{{O}_{3}}\] is dissolved in \[90g\] of \[{{H}_{2}}O\]) (ii) Weight to volume percent  % w/v \[=\frac{\text{Wt}\text{. of solute}}{\text{Volume of solution}}\times 100\] Example : 10% \[N{{a}_{2}}C{{O}_{3}}\] (w/v) means \[10g\] \[N{{a}_{2}}C{{O}_{3}}\] is dissolved in \[100\,cc\] of solution. (iii) Volume to volume percent  % v/v \[=\frac{\text{Vol}\text{. of solute}}{\text{Vol}\text{. of solution}}\times 100\] Example : 10% ethanol (v/v) means \[10\,cc\] of ethanol dissolved in \[100\,cc\] of solution. (iv) Volume to weight percent   % v/w \[=\frac{\text{Vol}\text{. of solute}}{\text{Wt}\text{. of solution}}\times 100\] Example : 10% ethanol (v/w) means \[10\,cc\]  of ethanol dissolved in \[100g\] of solution. (2) Parts per million (ppm) and parts per billion (ppb) : When a solute is present in trace quantities, it is convenient to express the concentration in parts per million and parts per billion. It is the number of parts of solute per million \[({{10}^{6}})\] or per billion \[({{10}^{9}})\] parts of the solution.  It is independent of the temperature. \[ppm=\frac{\text{mass of solute component}}{\text{Total mass of solution}}\times {{10}^{6}}\] \[ppb=\frac{\text{mass of solute component}}{\text{Total mass of solution}}\times {{10}^{9}}\] (3) Strength : The strength of solution is defined as the amount of solute in grams present in one litre (or \[d{{m}^{3}}\]) of the solution. It is expressed in g/litre or \[(g/d{{m}^{3}})\]. \[\text{Strength}=\frac{\text{Mass of solute in grams}}{\text{Volume of solution in litres}}\] (4) Normality (N) : It is defined as the number of gram equivalents (equivalent weight in grams) of a solute present per litre of the solution. Unit of normality is gram equivalents litre–1. Normality changes with temperature since it involves volume. When a solution is diluted \[x\] times, its normality also decreases by \[x\] times. Solutions in term of normality generally expressed as, \[N=\] Normal solution; \[5N=\] Penta normal, \[10N=\] Deca normal; \[N/2=\] semi normal \[N/10=\] Deci normal; \[N/5=\] Penti normal \[N/100\] or \[0.01\ N=\] centinormal, \[N/1000\] or      0.001= millinormal Mathematically normality can be calculated by following formulas, (i) \[\text{Normality (}N\text{)}=\frac{\text{Number of g}.\text{eq}\text{.}\ \text{of}\ \text{solute}}{\text{Volume}\ \text{of}\ \text{solution }(l)}\] (ii) N\[=\frac{\text{Weight of solute in }g\text{.}}{\text{g}\text{. eq}\text{. weight of solute}\times \text{Volume of solution (}l\text{)}}\] (iii)  \[N=\frac{\text{Wt}\text{. of solute per litre of solution  }}{\text{g}\ \text{eq}\text{. wt}\text{. of solute}}\] (iv) \[N=\frac{\text{Wt}\text{. of solute}}{g.\text{eq}\text{. wt}\text{. of solute}}\times \frac{1000}{\text{Vol}\text{. of solution in }ml}\] (v) \[N=\frac{\text{Percent of solute }\times \text{ 10}}{\text{g}\ \text{eq}\text{. wt}\text{. of solute}}\],     (vi) \[N=\frac{\text{Strength in }g {{l}^{-1}}\text{ of solution}}{\text{g}\ \text{eq}\text{. wt}\text{. of solute}}\] (vii) \[N=\frac{Wt%\times density\times 10}{Eq.\,\,wt.}\] (viii) If volume \[{{V}_{1}}\] and normality \[{{N}_{1}}\] is so changed that new normality and volume \[{{N}_{2}}\] and \[{{V}_{2}}\] then, \[{{N}_{1}}{{V}_{1}}={{N}_{2}}{{V}_{2}}\] (Normality more...

All the three states of matter (gas, liquid or solid) may behave either as solvent or solute. Depending on the state of solute or solvent, mainly there may be following nine types of binary solutions.
Solvent Solute Example
Gas Gas Mixture of gases, air.
Gas Liquid Water vapours in air, mist.
Gas Solid Sublimation of a solid into a gas, smoke.
Liquid Gas CO2 gas dissolved in water (aerated drinks).
Liquid Liquid Mixture of miscible liquids, e.g., alcohol in water.
Liquid more...
"Solubility of a substance may be defined as the amount of solute dissolved in 100 gms of a solvent to form a saturated solution at a given temperature". A saturated solution is a solution which contains at a given temperature as much solute as it can hold in presence of dissolveding solvent. Any solution may contain less solute than would be necessary to saturate it. Such a solution is known as unsaturated solution. When the solution contains more solute than would be necessary to saturate it then it is termed as supersaturated solution.

In 1920, Latimer and Rodebush introduced the idea of "hydrogen bond".          For the formation of H-bonding the molecule should contain an atom of high electronegativity such as F, O or N bonded to hydrogen atom and the size of the electronegative atom should be quite small.          Types of hydrogen bonding            (1) Intermolecular hydrogen bond : Intermolecular hydrogen bond is formed between two different molecules of the same or different substances.            (i) Hydrogen bond between the molecules of hydrogen fluoride.            (ii) Hydrogen bond in alcohol and water molecules            (2) Intramolecular hydrogen bond (Chelation)          Intramolecular hydrogen bond is formed between the hydrogen atom and the highly electronegative atom (F, O or N) present in the same molecule. Intramolecular hydrogen bond results in the cyclisation of the molecules and prevents their association. Consequently, the effect of intramolecular hydrogen bond on the physical properties is negligible.            For example : Intramolecular hydrogen bonds are present in molecules such as o-nitrophenol, o-nitrobenzoic acid, etc.                                                                                                                      The extent of both intramolecular and intermolecular hydrogen bonding depends on temperature.            Effects of hydrogen bonding            Hydrogen bond helps in explaining the abnormal physical properties in several cases. Some of the properties affected by H-bond are given below,          (1) Dissociation : In aqueous solution, hydrogen fluoride dissociates and gives the difluoride ion \[(HF_{2}^{-})\] instead of fluoride ion \[({{F}^{-}})\]. This is due to H-bonding in HF. This explains the existence of\[KH{{F}_{2}}\]. H-bond formed is usually longer than the covalent bond present in the molecule (e.g. in \[{{H}_{2}}O,\,\,O-H\] bond = 0.99 Å but H-bond = 1.77 Å).          (2) Association : The molecules of carboxylic acids exist as dimers because of the hydrogen bonding. The molecular masses of such compounds are found to be double than those calculated from their simple formulae. For example, molecular mass of acetic acid is found to be 120.          (3) High melting and boiling point : The compounds having hydrogen bonding show abnormally high melting and boiling points.            The high melting points and boiling points of the compounds \[({{H}_{2}}O,\ HF\] and \[N{{H}_{3}})\] containing hydrogen bonds is due to the fact that some extra energy is needed to break these bonds.          (4) Solubility : The compound which can form hydrogen bonds with the covalent molecules are soluble in such solvents. For example, lower alcohols are soluble in water because of the hydrogen bonding which can take place between water and alcohol molecules as shown below, \[\begin{align}   & \overset{\delta +}{\mathop{H}}\,-\overset{\delta -}{\mathop{O}}\,................\overset{\delta +}{\mathop{H}}\,-\overset{\delta -}{\mathop{O}}\,...............\overset{\delta +}{\mathop{H}}\,-\overset{\delta -}{\mathop{O}}\, \\  & \,\,\,\,\,\,\overset{\,}{\mathop{\,}}\,\,{{C}_{2}}{{H}_{5}}\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,H\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,\,{{C}_{2}}{{H}_{5}} \\ \end{align}\]            The intermolecular hydrogen bonding increases solubility of the compound in water while, the intramolecular hydrogen bonding decreases. (5) As the compounds involving hydrogen bonding between different molecules (intermolecular hydrogen bonding) have higher boiling points, so they are less volatile.          more...

Molecular orbital theory was given by Hund and Mulliken in 1932.          The main ideas of this theory are,              (1) When two atomic orbitals combine or overlap, they lose their identity and form new orbitals. The new orbitals thus formed are called molecular orbitals.              (2) Molecular orbitals are the energy states of a molecule in which the electrons of the molecule are filled just as atomic orbitals are the energy states of an atom in which the electrons of the atom are filled.            (3) In terms of probability distribution, a molecular orbital gives the electron probability distribution around a group of nuclei just as an atomic orbital gives the electron probability distribution around the single nucleus.            (4) Only those atomic orbitals can combine to form molecular orbitals which have comparable energies and proper orientation.            (5) The number of molecular orbitals formed is equal to the number of combining atomic orbitals.              (6) When two atomic orbitals combine, they form two new orbitals called bonding molecular orbital and antibonding molecular orbital.              (7) The bonding molecular orbital has lower energy and hence greater stability than the corresponding antibonding molecular orbital.            (8) The bonding molecular orbitals are represented by  etc, whereas the corresponding antibonding molecular orbitals are represented by  etc.            (9) The shapes of the molecular orbitals formed depend upon the type of combining atomic orbitals.            (10) The filling  of molecular orbitals in a molecule takes place in accordance with Aufbau principle, Pauli's exclusion principle and Hund's rule. The general order of increasing energy among the molecular orbitals formed by the elements of second period and hydrogen and their general electronic configurations are given below.              (11) Electrons are filled in the increasing energy of the MO which is in order            (a) \[\sigma 1s<{{\sigma }^{*}}1s<\sigma 2s<{{\sigma }^{*}}2s<\sigma 2{{p}_{z}}<\pi 2{{p}_{y}}\] \[=\pi 2{{p}_{x}}<{{\pi }^{*}}2{{p}_{x}}={{\pi }^{*}}2{{p}_{y}}={{\pi }^{*}}2{{p}_{z}}\] (b) \[=\frac{Increasing\text{ }energy\text{ }\left( for\text{ }electrons\text{ }>\text{ }14 \right)}{\sigma 1s<{{\sigma }^{*}}1s<\sigma 2s<{{\sigma }^{*}}2s<\pi 2{{p}_{x}}=\pi 2{{p}_{y}}<\sigma 2{{p}_{z}}<{{\pi }^{*}}2{{p}_{x}}}\] \[={{\pi }^{*}}2{{p}_{y}}<{{\sigma }^{*}}2{{p}_{z}}\]               (12) \[\frac{Increasing\text{ }energy\text{ }(for\text{ }electrons\le 14)}{Number\text{ }of\text{ }bonds\text{ }between\text{ }two\text{ }atoms\text{ }is\text{ }called}\]            bond order and is given by                       where number of electrons in bonding MO.                      number of electrons in antibonding MO.            For a stable molecule/ion,            (13) Bond order µ Stability of molecule µ Dissociation energy µ .            (14) If all the electrons in a molecule are paired then the substance is a diamagnetic on the other hand if there are unpaired electrons in the molecule, then the substance is paramagnetic. More the number of unpaired electron in the molecule greater is the paramagnetism of the substance.                 more...

The basic concept of the theory was suggested by Sidgwick and Powell (1940). It provides useful idea for predicting shapes and geometries of molecules. The concept tells that, the arrangement of bonds around the central atom depends upon the repulsions operating between electron pairs(bonded or non bonded) around the central atom. Gillespie and Nyholm developed this concept as VSEPR theory.            The main postulates of VSEPR theory are            (1) For polyatomic molecules containing 3 or more atoms, one of the atoms is called the central atom to which other atoms are linked.            (2) The geometry of a molecule depends upon the total number of valence shell electron pairs (bonded or not bonded) present around the central atom and their repulsion due to relative sizes and shapes.            (3) If the central atom is surrounded by bond pairs only. It gives the symmetrical shape to the molecule.            (4) If the central atom is surrounded by lone pairs (lp) as well as bond pairs (bp) of  then the molecule has a distorted geometry.            (5) The relative order of repulsion between electron pairs is as follows : lp - lp > lp - bp > bp - bp.            A lone pair is concentrated around the central atom while a bond pair is pulled out between two bonded atoms. As such repulsion becomes greater when a lone pair is involved.     Geometry of Molecules/Ions having bond pair as well as lone pair of electrons 
Type of mole-cule No. of bond pairs of electron No. of lone pairs of electrons Hybridi-zation Bond angle Expected geometry Actual geometry Examples
\[A{{X}_{3}}\] 2 1 \[s{{p}^{2}}\] < 120o Trigonal planar V-shape, Bent, Angular SO2, SnCl2, NO2–
\[A{{X}_{4}}\] 2 2 \[s{{p}^{3}}\] < 109o 28' Tetrahedral V-shape, Angular H2O, H2S, SCl2, OF2, NH2–, ClO2–
\[A{{X}_{4}}\] 3 1 \[s{{p}^{3}}\] < 109o 28' more...


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