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GASEOUS STATE
TYPES
Basically we observe with 3 states of matter namely
 SOLIDS
 LIQUIDS &
 GASES
LET’S See …
Apart from the 3 states of matter, there are 2 more states
of matter
 Plasma
 Bohr-Einstein Condensate
Plasma is not a common state of matter on the earth ,
but a common one among stars which produces that
excessive heat & light.That means plasma matter has
high kinetic energies.
In contrast to this , Bohr-Einstein condensate(BEC) has
very low & even zero kinetic energies.
Due to this zero kinetic energies atoms loose their
molecular motions & begin to clump together and form
condensates named BEC’s.
We have to make a note that kinetic energies are directly
proportional to absolute temperatures & hence BEC’s
also would form & exist at extremely low temperatures.
GASES
 As we all know the properties of gases or the gas
mixtures ..
The formost property is DIFFUSION of GASES
 Diffusion is the movement of gases from a region of
higher concentration to a region of lower
concentration which is exactly opposite to OSMOSIS
which is a property of liquids.
 Now this diffusion of gases is measured in terms of
rates of diffusion.
Rate of Diffusion(r)
 The volume of a gas that diffuses in unit time is said to
be rate of diffusion (r) of a gas .
r=V/t
or r1/r2 = V1/V2 * t2/t1
if the two gases have equal volumes then ,
r1/r2 = t2/t1
EFFUSION
 Similar to diffusion , EFFUSION is also a property of
gases
 Effusion is defined as the movement of gases from a
region of higher concentration to that of lower
concentration through a small pore.
 The best example of effusion are like…
1) Escape of air from balloon
2) Escape of air from punctured cycle tube.
3) Gas leakages from pipes / cylinders
GAS LAWS
 A very imp. arena of this chapter is on gas laws.
 Here we shall deal with 5 gas laws….
1) Boyle ‘s law
2) Charles law
3) Avogadros law
4) Grahams law of Diffusion
5) Dalton’s law
Lets see one by one in detail……
PV = K
Boyle’s law
 The pressure of a given mass of gas is inversly
proportional to volume at constant temperature.
or
 A graph drawn for Boyles law is shown as
Pressure vs Volume
P
V
 If a graph of boyles law is drawn between P vs 1/V ,
That is represented as
P
1/V
 Similarly if a graph is drawn among PV vs P is given as
PV
P
Charles laws
 Statement 1
Charles law -1
1 states that , at constant pressure for every one degree
rise in temperature , the volume of a given mass of gas
changes by 1/273 of its volume at ‘0’ degrees
centigrade.
Vt= V0 1+ t/273
Charles law-1 graph
 A graph plotted for statement 1 of charles law is shown
as
V m
v0
0 T
Statement - 2
 It states that at constant volume , pressure of a given
mass of gas is directly proportional to temperature
or
At constant pressure, volume of a given mass of gas is
directly proportional to temperature .
V T or P T
V=KT P=KT
V1/V2=T1/T2 P1/P2=T1/T2
Graphical representation
 The graphs drawn for charles law 1 & 2 are given as
V3 P3
V2 P2
P1
V1
V P
T T
AVOGADRO’S law
 Equal volumes of all gases contain equal number of
molecules under similar conditions of temperature
and pressure.
&
or
or
V n
V=nK V/n = K
V1/n1=V2/n2
V1n2=V2n1
IDEAL GAS EQUATION
From the 3 gas laws , studied till now … ideal gas
equation can be derived as follows
PV=K ……… eq 1
P=KT ……... eq 2
V= nK ………. eq 3
From 1,2 & 3 PV=nKT
Replacing constant K, with Universal gas Constant we
get
PV=nRT
Values of ‘R’
NUMERICAL VALUE UNITS
8.314 Joules
0.08206 L.atm
1.987 Calories
62.36 L.torr
82.1 atm.cc
GRAHAMS LAW OF DIFFUSION
 Grahams law of diffusion states that the rate of
diffusion of a gas is inversly proportional to the
squareroot of density or molecular weight.
DALTONS LAW
 It states that , at constant temperature the total
pressure of a gas in a gaseous mixture is the sum of
partial pressures of the gases.
P= p1+p2+p3+……..
At const. ‘T’ ; the partial pressure of a gas is directly
proportional to its molefraction (
Kinetic gas Equation
 The kinetic gas equation is given as
PV=1/3 mnc2
Types of velocities
 Gas molecules exhibit with three different kinds of
velocities …
1) Average velocity ( C )
2) Most probable velocity ( C p )
3) Root meansquare velocity ( C rms )
Ratio of velocities
The ratio of C p , C & Crms can be given as
1:1.128 : 1.223
INTERMOLECULAR FORCES vs
THERMAL ENERGY
 Inter molecular forces are forces which mediate
interraction between molecules; be it forces of
attraction or forces of repulsion.
 These intermolecular forces of attraction are cheifly
studied as hydrogen bonding , dipole forces of
attraction.
 Thermal energy is the average kinetic energy of the
molecules of a substance.
Thermal energy is a very key factor for the liquifaction
of gases.
 Physical state of a substance always depends on the
extent of intermolecular forces & thermal energy.
REAL GAS vs IDEAL GAS
 Gases which follow ideal gas equation i.e PV=nRT
are said to be ideal gases
&
Gases which donot follow ideal gas equation are said be
real gases.
And in general , all gases are real & no gas is ideal.
The reason behind real behaviour of gases are
1) Molecules of a gas donot exhibit any forces of
attraction among them.
2) Volume of gas occupied is negligibly small wrt space
occupied by the gas.
GRAPHICAL NOTE
CO
CH4
H2 He
PV P Real gas
ideal gas
Ideal gas
P V
LIQUIFACTION OF GASES
 Ideal gases cannot be liquified.it is only a real gas that
can be liquified.
 Gases can be liquified on cooling below their boiling
points.But if the gas to be liquified is having a very low
boiling point , then it cannot be liquified by cooling
furthur.
Hence an another technique called JOULE-THOMPSON
EFFECT is to be used.
Principle behind this technique is cooling of gases by
expansion from high pressure to low pressure.
 There are 2 key points to achieve liquifaction of gases
1) Critical temperature ( Ct )
2) Critical pressure ( C p )
The highest temperature at which liquifaction of gases
occurs first is Ct & the pressure required to liquify a
gas at its critical temperature is its Cp.
THANKYOU

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How to Create a More Engaging and Human Online Learning Experience
 

States of matter - Gaseous state

  • 2. TYPES Basically we observe with 3 states of matter namely  SOLIDS  LIQUIDS &  GASES
  • 4. Apart from the 3 states of matter, there are 2 more states of matter  Plasma  Bohr-Einstein Condensate Plasma is not a common state of matter on the earth , but a common one among stars which produces that excessive heat & light.That means plasma matter has high kinetic energies.
  • 5. In contrast to this , Bohr-Einstein condensate(BEC) has very low & even zero kinetic energies. Due to this zero kinetic energies atoms loose their molecular motions & begin to clump together and form condensates named BEC’s. We have to make a note that kinetic energies are directly proportional to absolute temperatures & hence BEC’s also would form & exist at extremely low temperatures.
  • 6. GASES  As we all know the properties of gases or the gas mixtures .. The formost property is DIFFUSION of GASES  Diffusion is the movement of gases from a region of higher concentration to a region of lower concentration which is exactly opposite to OSMOSIS which is a property of liquids.  Now this diffusion of gases is measured in terms of rates of diffusion.
  • 7. Rate of Diffusion(r)  The volume of a gas that diffuses in unit time is said to be rate of diffusion (r) of a gas . r=V/t or r1/r2 = V1/V2 * t2/t1 if the two gases have equal volumes then , r1/r2 = t2/t1
  • 8. EFFUSION  Similar to diffusion , EFFUSION is also a property of gases  Effusion is defined as the movement of gases from a region of higher concentration to that of lower concentration through a small pore.  The best example of effusion are like… 1) Escape of air from balloon 2) Escape of air from punctured cycle tube. 3) Gas leakages from pipes / cylinders
  • 9. GAS LAWS  A very imp. arena of this chapter is on gas laws.  Here we shall deal with 5 gas laws…. 1) Boyle ‘s law 2) Charles law 3) Avogadros law 4) Grahams law of Diffusion 5) Dalton’s law Lets see one by one in detail……
  • 10. PV = K Boyle’s law  The pressure of a given mass of gas is inversly proportional to volume at constant temperature. or
  • 11.  A graph drawn for Boyles law is shown as Pressure vs Volume P V
  • 12.  If a graph of boyles law is drawn between P vs 1/V , That is represented as P 1/V
  • 13.  Similarly if a graph is drawn among PV vs P is given as PV P
  • 14. Charles laws  Statement 1 Charles law -1 1 states that , at constant pressure for every one degree rise in temperature , the volume of a given mass of gas changes by 1/273 of its volume at ‘0’ degrees centigrade. Vt= V0 1+ t/273
  • 15. Charles law-1 graph  A graph plotted for statement 1 of charles law is shown as V m v0 0 T
  • 16. Statement - 2  It states that at constant volume , pressure of a given mass of gas is directly proportional to temperature or At constant pressure, volume of a given mass of gas is directly proportional to temperature . V T or P T V=KT P=KT V1/V2=T1/T2 P1/P2=T1/T2
  • 17. Graphical representation  The graphs drawn for charles law 1 & 2 are given as V3 P3 V2 P2 P1 V1 V P T T
  • 18. AVOGADRO’S law  Equal volumes of all gases contain equal number of molecules under similar conditions of temperature and pressure. & or or V n V=nK V/n = K V1/n1=V2/n2 V1n2=V2n1
  • 19. IDEAL GAS EQUATION From the 3 gas laws , studied till now … ideal gas equation can be derived as follows PV=K ……… eq 1 P=KT ……... eq 2 V= nK ………. eq 3 From 1,2 & 3 PV=nKT Replacing constant K, with Universal gas Constant we get PV=nRT
  • 20. Values of ‘R’ NUMERICAL VALUE UNITS 8.314 Joules 0.08206 L.atm 1.987 Calories 62.36 L.torr 82.1 atm.cc
  • 21. GRAHAMS LAW OF DIFFUSION  Grahams law of diffusion states that the rate of diffusion of a gas is inversly proportional to the squareroot of density or molecular weight.
  • 22. DALTONS LAW  It states that , at constant temperature the total pressure of a gas in a gaseous mixture is the sum of partial pressures of the gases. P= p1+p2+p3+…….. At const. ‘T’ ; the partial pressure of a gas is directly proportional to its molefraction (
  • 23. Kinetic gas Equation  The kinetic gas equation is given as PV=1/3 mnc2
  • 24. Types of velocities  Gas molecules exhibit with three different kinds of velocities … 1) Average velocity ( C ) 2) Most probable velocity ( C p ) 3) Root meansquare velocity ( C rms )
  • 25. Ratio of velocities The ratio of C p , C & Crms can be given as 1:1.128 : 1.223
  • 26. INTERMOLECULAR FORCES vs THERMAL ENERGY  Inter molecular forces are forces which mediate interraction between molecules; be it forces of attraction or forces of repulsion.  These intermolecular forces of attraction are cheifly studied as hydrogen bonding , dipole forces of attraction.  Thermal energy is the average kinetic energy of the molecules of a substance. Thermal energy is a very key factor for the liquifaction of gases.
  • 27.  Physical state of a substance always depends on the extent of intermolecular forces & thermal energy.
  • 28. REAL GAS vs IDEAL GAS  Gases which follow ideal gas equation i.e PV=nRT are said to be ideal gases & Gases which donot follow ideal gas equation are said be real gases. And in general , all gases are real & no gas is ideal. The reason behind real behaviour of gases are 1) Molecules of a gas donot exhibit any forces of attraction among them. 2) Volume of gas occupied is negligibly small wrt space occupied by the gas.
  • 29. GRAPHICAL NOTE CO CH4 H2 He PV P Real gas ideal gas Ideal gas P V
  • 30. LIQUIFACTION OF GASES  Ideal gases cannot be liquified.it is only a real gas that can be liquified.  Gases can be liquified on cooling below their boiling points.But if the gas to be liquified is having a very low boiling point , then it cannot be liquified by cooling furthur. Hence an another technique called JOULE-THOMPSON EFFECT is to be used. Principle behind this technique is cooling of gases by expansion from high pressure to low pressure.
  • 31.  There are 2 key points to achieve liquifaction of gases 1) Critical temperature ( Ct ) 2) Critical pressure ( C p ) The highest temperature at which liquifaction of gases occurs first is Ct & the pressure required to liquify a gas at its critical temperature is its Cp.