Entry Test Preparation 2015, Chemistry BOOK 1 Chapter # 2 Gasess , Theory and Key Concepts

Entry Test Preparation 2015, Chemistry BOOK 1
Chapter # 2
gases
States of matter:
Matter exists in four states i.e., solid, liquid, gas and plasma.
Properties of Gases:
·         Gases don’t have  definite shape and volume.
·         Their molecules move rapidly in all directions.
·         They occupy the whole space available to them in the container.
·         There are large empty spaces between molecules of a gas in normal state.
·         Gases can diffuse and effuse.
·         Gases can be compressed by applying pressure.
·         Gases expand on heating.
·         Low temperature is produced by expansion of gases. (Joule Thomson effect). For example, the escaping CNG from the cylinder makes the cylinder cool.
·         In gases molecules collide with one another and with the walls of container elastically.
·         The gases have low densities as compared to the densities of liquids and solids.
·         Gases form homogeneous mixtures.
·         The intermolecular forces in gases are very weak.
Units of pressure:
Atmospheric pressure:
The force exerted by the atmosphere of the earth per unit area is called atmospheric pressure.
The force exerted by 76 cm long column of mercury on an area of 1 cm2 at 0o C is called standard pressure or atmospheric pressure.
SI unit for measurement of pressure is Pascal (Pa). Other units are torr, mm of Hg, atmosphere and Nm-2
1 atm = 760 mm Hg
= 29.5230 in Hg
= 14.7 PSi
= 101325 Pa
= 101325 Nm-2
= 1.01325 bar
PSi used in engineering work and millibar used by meteorologists.
Scales of thermometry:
K= 0C + 273
0C=5/9(0F-32)
0F=9/5(0C) +32
Boyle’s Law:
Volume of a given mass of a gas is inversely proportional to the pressure applied at constant temperature.
V ∞  (T is kept constant)
PV = k
Charle’s Law:
The volume of a given mass of a gas is directly proportional to the absolute temperature at constant pressure.
V ∞ T    or      =  k
(Pressure is kept constant)

Ideal Gas:
A gas which obeys gas laws completely at all conditions of temperature and pressure is called ideal or perfect gas. Inert gases behave like ideal gases up to some extent.
Absolute Zero:
The hypothetical temperature at which volume of a gas becomes zero OR The temp. at which motion of molecules ceases.
                        O K = -273.15 oC
Volume of a gas at various Temperatures is
Vt = Vo (1 + ) Where
Vt = volume of gas at temperature t
Vo = volume of a gas at temperature 0oC
t = temperature on Celsius scale
Density of an Ideal Gas:
The density of an ideal gas is directly proportional to its molar mass.
Greater the pressure on the gas, greater the density.
Higher temperature make density falls.
General Gas Equation:
PV = nRT
Where
n  =  number of moles of gas with the molecular mass M, T = temperature in Kelvin, and R = gas constant.

Values R in various systems
8.314472 J . K-1  .mol-1
0.0820574587 L . atm. K-1 . mole-1
8.20574587 x 10-5 m3 . atm . K-1 . mol-1
8.314472 cm3 . MPa . K-1 . mol -1
8.314472 L . kPa . K-1 . mol-1
8.314472 m3 . Pa . K-1 . mol-1
62.3637 L . mmHg . K-1 . mol-1
6.132439833 1bf  .  ft  . K-1  .  g  .  mol-1
10.7316 ft3  .  psi  . oR-1  .  1b  .  mole-1
8.63 x 10-5 eV  .  atom-1  .  Kelvin-1
0.7302 ft3  .  atm  .  oR-1  .  1b – mole-1
62.3637 L  .  Torr  .  K-1  .  mol-1
83.14472 L  . mbar  .  K-1  .  mol-1
1.987 cal  .  K-1  .  mol-1
Avogardro’s Law:
According to this law, “Equal volumes of ideal gases at the same temperature and pressure contain equal number of molecules” 22.414 dm3 of a gas at 273.15 K and one atm. Pressure has 6.02 x 1023 molecules of the gas.
Brownian movement:
The continuous and random movement of small solid particles, suspended in a fluid medium is called the Brownian movement.
Dalton’s Law of Partial Pressures:
The total pressure exerted by the mixture of gases is equal to the sum of the partial pressures of individual gases.
Ptotal = P1 + P2  +  P3 …….
Where
P1 , P2 ,  P3 ,  …….  Are partial pressures of gases 1,2,3,…… respectively.
Important applications of Dalton’s Law of Partial Pressures
·         Some gases are collected over water in the laboratory.
·         The process of respiration depends upon the difference in the partial pressures.
·         At higher altitudes, a person feels uncomfortable breathing because the partial pressure of oxygen in the un-pressurized cabin is low, as compared to 159 g/cm3 on the earth surface.
·         Deep sea divers take oxygen mixed with an inert gas to adjust the partial pressure of oxygen according to the requirement.

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Aqueous tension:
The Partial pressure of water vapours in a gas is called aqueous tension.
Diffusion of Gases:
The spontaneous mixing of molecules of one gas with another at a given temperature and pressure is called diffusion.
The spreading of fragrance of a rose or a scent is due to diffusion.


Effusion of Gases:
The movement of gas molecules through pores into a region of low pressure of the gas is called Effusion. This spreading of molecules is due to their collisions with the walls of the container.
Graham’s Law of Diffusion and Effusion:
At constant temperature and pressure, the rate of diffusion of a gas is inversely proportional to the square root of its density.
The volume of a gas diffused per unit time is called the rate of diffusion.
Rates of diffusion of two gases can be found by the following relation
Where r1 , D1, and M1 are rate of diffusion, Density, and Molar mass of the gas 1 respectively and r2, D2, and M2 are rate of diffusion, Density , and Molar mass of the gas 2 respectively.
Kinetic Molecular Theory of Gases:
Following are the fundamental postulates of the kinetic theory of gases:
·         Every gas consists of a large number of very small particles called molecules.
·         The molecules of a gas move randomly, colliding among themselves and with the walls of the container elastically and change their direction.
·         The pressure exerted by a gas is due to the collisions of its molecules with the walls of the container.
·         The collisions among the molecules are perfectly elastic.
·         The molecules of a gas have no forces of attraction for each other.
·         The actual volume of molecules of a gas is negligible as compared to the volume of the gas.
·         The effect of gravity is negligible on the gas molecules.
·         The kinetic energy of the gas molecules varies directly as the absolute temperature of the gas.
Critical Temperature and Critical Pressure:
The highest temperature, at which a substance can exist as a liquid, is called its critical temperature.
There is a corresponding pressure, which is required to bring about liquefaction at this critical temperature. This is called critical pressure.
Liquefaction of Gases
Gases can be liquefied by the following methods:
High Pressure:
At very high pressure the gas molecules come close to each other and the force of attraction between them become strong enough to make the gas liquid.
Low Temperature:
At very low temperatures the gas molecules loses kinetic energy and the slight attractive forces becomes strong enough to make the gas a liquid.
Joule Thomson Effect:
Linds method: H2 and He cannot be liquefied by this method as these have less attractive forces, small sizes and have very low critical temperatures.
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Non Ideal Behavior of Real Gases:
Real gases, such as hydrogen, oxygen etc., do not obey gas laws exactly because:
·         At low temperatures the gas molecules have less kinetic energy i.e move around less so they do attract each other.
·         At high pressure the gas molecules are forced to come close to each other so that the volume they occupy, decrease significantly.
·         Under ordinary conditions, deviations from Ideal Gas behaviour are so slight that they can be neglected.
Real gases, however, obey gas laws at low pressures and high temperature,
A real gas do not obey gas laws at high pressures and low temperatures. This is called non ideal behavior of gases.
A gas which obey gas laws at all temperatures and pressure is called an ideal gas.




Vander Waal’s Equation.

VOLUME CORRECTION: If the effective volume of the molecules per mole of a gas is represented by b, then the volume available to gas molecules is the volume of the vessel minus the volume of the gas molecules
Vfree       =          Vvessel _ Vmolecules
Vfree       =          Vvessel _ b
Where,
Vfree = volume which is available to gas molecules.
b     = excluded volume which is constant and characteristics of a gas.
            Its value depends upon the size of gas molecules.
b          =          4Vm
Where,
b     = volume of a gas which is occupied by 1 mole of a gas molecules in highly
compressed state and not in the liquid state.
PRESSURE CORRECTION:
                        Observed pressure is less than the actual pressure.
P             =          Pi _ P′
Pi            =          P + P′
P′         =          a / V2
P′         α          (n / V) x (n / V)
P′         =          n2 / V2
P′         =          an2 / V2
P′         =          a / V2                    ( where      n=1 )
Pi            =          P + (a / V2)
PV         =          RT
(P + a / V2) (V – b)                  =          RT
(P + an2 / V2) (V – nb)                        =          nRT
Units of “a”:
a          =          P′V2 / n2
a          =          (atm) x (dm3)2/ (mol)            =          atm dm6 mol-2 
In SI unit,
Nm-2 x (m3)2 /   (mol)2              =          Nm+4 (mol) -2   
Units of “a”:
dm3 mol -1  or  m3 mol -1 
The presence of intermolecular forces in gases like Cl2 and SO2 increases their 'a' factor. Value of “a” depends upon intermolecular forces and value of “b” depends upon yhe size of gas molecules. H2 has less value of “a” than SO2 or Cl2 due to greater non-polar characters.

Plasma State:
                “An electricity neutral mixture of electrons, ions, and atoms is called plasma”
            It is the fourth state of matter. Plasma was identified in 1879 by William Crook. 99% of the universe is plasma state and solid, liquid and gases are only 1%.
            Molecule         →        Atomic Gas
            Atomic Gas     →        positive ions + electrons
Natural plasma exist only at very high temperatures, or low temperatures vacuums. Natural plasma on the other hand do not breakdown or react rapidly, but are extremely hot (over 20,000oC minimum). Their energy is so high that they vaporize any material they touch.
Future Horizon:
            Scientists are working on putting plasma to effective use. Plasma would have to be low energy and should be able to survive without instantly reacting and degenerating. The application of magnetic, fields involves the use of plasma. The magnetic fields create low energy plasma which create molecules that are in what scientist call metastable state. The magnetic fields used to create the low temperature plasma give the plasma molecules electrons, which do not react until they collide with another molecule with just the right energy. This enables these metastable molecules to survive long enough to react with a designated molecule.
These metastable particles are selective in their reactivity. It makes them a potentially unique solution to problems like radioactive contamination.
Scientists are currently experimenting with mixtures of gases to work as metastable agents on plutonium and uranium, and this is just the beginning.



Best Regards :


Zohaib Hassan

Trainee Geological Engineer

GRC Private Limited

Karora Hydropower Project Besham KPK,Pakistan

Cell#+923318601240

Email:Zohaibhani@gmail.com


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