SlideShare a Scribd company logo
Gases
Advanced Chemistry Chapter 5
Intro
Earth’s atmosphere is a gaseous
solution that consists mainly of
nitrogen (N2) and oxygen (O2). This
atmosphere supports life and acts as
a waste receptacle for many
industrial processes. The chemical
reactions that follow often lead to
various types of pollution, including
smog and acid rain.
Intro
The gases in the atmosphere also
shield us from harmful radiation
from the sun and keep the earth
warm by reflecting heat radiation
back toward the earth. In fact, there
is now great concern that an increase
in atmospheric carbon dioxide, a
product of the combustion of fossil
fuels , is causing a dangerous
warming of the earth.
Pressure
Pressure
Gas uniformly fills a container, is
easily compressed, and mixes
completely with any other gas.
One of the most important
properties is that it exerts pressure
on its surroundings equally.
Pressure
Incredible Tank Implosion
Pressure
Pressure
Pressure
Pressure
Barometer - A device to
measure atmospheric pressure,
was invented in 1643 by Torricelli
(a student of Galileo).
Torricelli’s barometer is
constructed by filling a glass
tube with liquid mercury and
inverting it in a dish of mercury.
Pressure
Barometer - A device to
measure atmospheric pressure,
was invented in 1643 by Torricelli
(a student of Galileo).
Notice that a large quantity of
mercury stays in the tube. In
fact, at sea level the height of
this column of mercury averages
760 mm.
Pressure
Barometer - A device to
measure atmospheric pressure,
was invented in 1643 by Torricelli
(a student of Galileo).
Atmospheric pressure results
from the mass of the air being
pulled toward the center of the
earth by gravity.
Pressure
Barometer - A device to
measure atmospheric pressure,
was invented in 1643 by Torricelli
(a student of Galileo).
Atmospheric pressure varies
with weather changes and
altitude.
Pressure
Manometer – an instrument for measuring pressure
often below that of atmospheric pressure.
Units of Pressure
Pressure = force/area
torr – in honor of Torricelli is equal
to a mm Hg.
760 mm Hg = 760 torr
1 atm = 760 torr
Pascal = N/m2
1atm = 101,325 Pa
Practice Problems
Page 225 #35, 37, 39
The Gas
Laws of
Boyle,
Charles and
Avogadro
Boyles Law
Boyle (1627-1691) –
performed the first quantitative
experiments on gases. Used a
J tube to measure pressures.
PV = k; P1V1=P2V2
k is a constant for a given
sample of air at a specific
temperature.
Boyles Law
Pressure and volume are often plotted.
P vs V – gives a hyperbola and an
inverse relationship.
Boyles law rearranged is
V=k/P=k1/P; when plotted as V vs
1/P – gives a straight line with the
intercept of zero
Boyles Law
Boyles Law
Boyles’s law holds precisely at
very low temperatures, but
varies at higher pressures. PV
will vary as pressure is varied.
An ideal gas is a gas that
strictly obeys Boyles’ law.
Boyles Law
Charles Law
Charles (1746-1823) – the first person to
fill a balloon with hydrogen gas and who
made the first solo balloon flight.
Charles found in 1787 that the volume of
a gas at constant pressure increases
linearly with the temperature of the gas.
V = bT ; V1/T1 = V2/T2
T is in Kelvin, b is a proportionality
constant
Charles Law
Temperature vs Volume plots a
straight line.
Slope will vary will type of gas.
All gas plots of T vs V will
extrapolate to zero at the same
temperature.
-273° or 0 K
Charles Law
Avogadro’s Law
Avogadro (1811) – postulated
that equal volumes of gases at
the same temperature and
pressure contain the same
number of particles (moles).
V = an; V1/n1=V2/n2
n is number of moles; a is a
proportionality constant.
Ideal Gas
Law
Ideal Gas Law
The relationships that Boyle, Charles
and Avogadro presented can be
combined to show how the volume of a
gas depends on pressure, temperature,
and number of moles of gas present.
V = R(Tn/P)
R is the universal gas constant.
A combination of proportionality
constants
Ideal Gas Law
The equation is often rearranged to
form the more common:
PV=nRT
R=.08206 Latm/Kmol
Ideal Gas Law
Limitations
A gas that obeys this equation is said
to behave ideally. The ideal gas
equation is best regarded as a limiting
law, it expresses behavior that real
gases approach at low pressures and
high temperatures.
Most gases behave ideally at pressures
below 1 atm.
Example Problem
A sample of hydrogen gas (H2) has a
volume of 8.56 L at a temperature of
0°C and a pressure of 1.5 atm.
Calculate the moles of H2 molecules
present in this gas sample.
Example Problem
V = 8.56 L at a temperature of 0°C
P =1.5 atm
Calculate the moles
PV=nRT; R = .08206 L atm/K mol
.57 mol
Example Problem 2
You have a sample of ammonia gas with
a a volume of 7.0ml at a pressure of
1.68 atm. The gas is compressed to a
volume of 2.7 ml at a constant
temperature. Use the ideal gas law to
calculate the final pressure.
Example Problem 2
V1 = 7.0 ml at a pressure of 1.68 atm
V2 =2.7 ml at a constant temperature.
Calculate the final pressure.
PV=nRT; but nRT are constant: PV=PV
4.4 atm
Example Problem 3
A sample of methane gas that has a
volume of 3.8 L at 5°C is heated to 86°C
at constant pressure. Calculate its new
volume.
Example Problem 3
V1 = 3.8 L and T15°C
T2=86°C at constant pressure.
Calculate its new volume.
PV=nRT but n, R and P are constant: V1/T1 = V2/T2
4.9 L
Example Problem 4
A sample of diborane gas (B2H6), a
substance that burst into flame when
exposed to air, has a pressure of 345 torr
at a temperature of -15°C and a volume
of 3.48 L. If conditions are changed so
that the temperature is 36°C and the
pressure is 468 torr, what will be the
volume of the sample.
Example Problem 4
P1=345 torr, T1=-15°C and V1 = 3.48L
T2=36°C and P2=468 torr,
What is the volume?
PV = nRT; nR are constant: P1V1/T1 =
P2V2/T2
3.1 L
Example Problem 5
A sample containing 0.35 mol argon gas at
a temperature of 13°C and a pressure of
568 torr is heated to 56°C and a pressure
of 897 torr. Calculate the change in
volume that occurs.
Example Problem 5
n=0.35, T1=13°C, P1=568 torr
T2=56°C, P2=897 torr
Calculate the change in volume that occurs.
-3 L
PV=nRT; R = .08206 L atm/K mol
Practice Problems
Page 226 #41, 43, 45,
47, 49, 51, 53, 57, 59,
61
Gas
Stoichiometry
Molar Volume
One mole of an ideal gas at:
 0°C (273K)
1atm
V=nRT/P = 22.42L
Gas Stoichiometry
We use STP or standard
temperature and pressure of an ideal
gas to make calculations with a gas.
1 atm
0°C (273K)
1 mole = 22.42 L becomes a
conversion factor for dimensional
analysis.
Gas Stoichiometry
Example
A sample of nitrogen gas has a volume
of 1.75 L at STP. How many moles of
N2 are present?
1.75L N2 x
1mole N2
22.42L N2
=
7.81 x 10-2
mol N2
Gas Stoichiometry
Example 2
Quicklime (CaO) is produced by the
thermal decomposition of calcium
carbonate (CaCO3). Calculate the
volume of CO2 at STP produced from
the decomposition of 152g CaCO3 by
the reaction
CaCO3(s) CaO(s) + CO2(g)
Gas Stoichiometry
Example 2
152g CaCO3
22.42 L = 1 mol of gas at STP
Calculate the volume of CO2
CaCO3(s) CaO(s) + CO2(g)
34.1 L CO2 at STP
Gas Stoichiometry
Example 3
A sample of methane gas having a
volume of 2.80 L at 25°C and 1.65
atm was mixed with a sample of
oxygen gas having a volume of 35.0 L
at 31°C and 1.25 atm. The mixture
was then ignited to form carbon
dioxide and water. Calculate the
volume of CO2 formed at a pressure of
2.50 atm and a temperature of 125°.
Gas Stoichiometry
Example 3
CH4 V=2.80 L at 25°C and 1.65 atm
Oxygen V=35.0 L at 31°C and 1.25 atm.
Calculate the volume of CO2 at 2.50 atm and
125°C.
The mixture was then ignited to form carbon
dioxide and water.
Gas Stoichiometry
Example 3
CH4 V=2.80 L at 25°C and 1.65 atm
Oxygen V=35.0 L at 31°C and 1.25 atm.
Calculate the volume of CO2 at 2.50 atm and
125°C.
CH4(g) + O2(g)  CO2(g) + H2O(g)
2.47 L
Practice Problems
Page 227 #65, 69
Molar Mass of a Gas
 One use of the ideal gas law is in the calculations of the
molar mass of a gas from its measured density.
 n =
 P
 D
 P =
grams of gas
molar mass
=
µ
µολαρµασσ
=
nRT
V
=
m / molar mass( )RT
V
=
mRT
V(molar mass)
=
m
V
dRT
molar mass
; Molar mass =
δΡΤ
Π
Gas Density/Molar
Mass Example
The density of a gas was measured
at 1.50 atm and 27°C and found to
be 1.95 g/L. Calculate the molar
mass of the gas.
32.0 g/mol
Dalton’s
Law of
Partial
Pressures
John Dalton
John Dalton formed his atomic theory from his
experiments and studies of the mixture of gases.
His observations car be summarized as follows:
For a mixture of gases in a container, the total
pressure exerted is the sum of the pressures
that each as would exert if it were alone.
John Dalton
Ptotal=P1+P2+P3+….
Subscripts refer to the individual gases
and Px refers to partial pressure that a
particular gas would exert if it were
alone in the container.
Each Partial pressure can be derived
from the ideal gas law and added
together to determine the total.
John Dalton
Ptotal=P1+P2+P3+….
Since each partial pressure can be
broken down into ; the Ptotal can be
represented by:
Ptotal=
Ptotal=
nx RT
V
(n1 + ν2 + ν3 + ...)
ΡΤ
ς




ntotal
RT
V




For a mixture of ideal gases, it is the total number of
moles of particles that is important, not the identity
or composition of the involved gas particle.
Dalton’s Law Example
Mixtures of helium and oxygen can be
used in scuba diving tanks to help
prevent “the bends.” For a particular
dive, 46 L He at 25° and 1.0 atm and
12 L O2 at 25° and 1.0 atm were
pumped into a tank with a volume of
5.0 L. Calculate the partial pressure of
each gas and the total pressure in the
tank at 25° C.
Mole Fraction
The ratio of the number of
moles of a given component
in a mixture to the total
number of moles in the
mixture.
 = nχ x/ntotal
 = Pχ 1/Ptotal
Dalton’s Law Example
The partial pressure of oxygen was
observed to be 156 torr in air with a
total atmospheric pressure of 743
torr. Calculate the mole fraction of O2
present.
Dalton’s Law Example
The mole fraction of nitrogen in the air
is 0.7808. Calculate the partial
pressure of N2 in air when the
atmospheric pressure is 760 torr.
Collecting Gas over
Water
A mixture of gases results whenever a
gas is collected by displacement of water.
In this situation, the gas in the bottle is a
mixture of water vapor and the oxygen
being collected.
Collecting Gas over
Water
Water vapor is present because
molecules of water escape from the
surface of the liquid and collect in the
space above the liquid.
Collecting Gas over
Water
Molecules of water also return to the
liquid. When the rate of escape equals
the rate of return, the number of water
molecules in the vapor state remain
constant.
Collecting Gas over
Water
When the number of water molecules in
the vapor state remain constant the
pressure of the water vapor remains
constant.
Collecting Gas over
Water
This pressure, which depends on
temperature, is called vapor pressure of
water.
Collecting Gas over
Water Example
A sample of solid potassium chlorate
(KClO3) was heated in a test tube and
decomposed by the reaction:
2KClO3(s) → 2ΚΧλ(σ) + 3Ο2(γ )
Collecting Gas over
Water Example
The oxygen produced was collected by
displacement of water at 22°C at a total
pressure of 754 torr. The volume of gas
collected was .650L, and the vapor
pressure of water at 22°C is 21 torr.
Calculate the partial pressure of O2 in the
gas collected and the mass of KClO3 in
the sample that was decomposed.
2KClO3(s) → 2ΚΧλ(σ) + 3Ο2(γ )
Collecting Gas over
Water Example
oxygen T=22°C and V=.650L
Total pressure = 754 torr.
vapor pressure at 22°C is 21 torr.
Calculate the partial pressure of O2 and
the mass of KClO3 in the sample
2KClO3(s) → 2ΚΧλ(σ) + 3Ο2(γ )
2.59 x 10-2
mol O2 2.12 g KClO3
The Kinetic
Molecular
Theory of
Gases
Kinetic Molecular Theory
KMT
A simple model that attempts to
explain the properties of an ideal
gas. This model is based on
speculations about the behavior of
the individual gas particles (atoms or
molecules).
Kinetic Molecular Theory
KMT
1. The particles are so small
compared with the distances
between them that the volume of
the individual particles can be
assumed to be negligible (zero).
Kinetic Molecular Theory
KMT
2. The particles are in constant
motion. The collisions of the
particles with the walls of the
container are the cause of the
pressure exerted by the gas.
Kinetic Molecular Theory
KMT
3. The particles are assumed to exert
no forces on each other; they are
assumed neither to attract nor to
repel each other.
Kinetic Molecular Theory
KMT
4. The average kinetic energy of a
collection of gas particles is
assumed to be directly
proportional to the Kelvin
temperature of the gas.
KMT and Boyle’s Law
 Because a decrease in volume, the
gas particles will hit the walls more
often, thus increasing the pressure
KMT and Charles Law
 When the gas is heated to a higher
temperature, the speeds of its molecules
increase and thus hit the walls more
often and with more force. Volume
and/or pressure will increase.
KMT and Advogadro’s Law
 An increase in the number of gas
particles at the same temperature would
cause the pressure to increase if the
volume were constant.
KMT and Advogadro’s Law
 The volume of a gas (at constant T and
P) depends only on the number of gas
particles present. The individual particles
are not a factor because the particle
volumes are so small compared with the
distances between the particles.
KMT and Dalton’s Law
 All gas particles are independent of each
other and that the volumes of the
individual particles are unimportant.
Identities of the gas particles do not
matter.
The Meaning of Temperature
Kelvin temperature indicates the
average kinetic energy of the gas
particles.
The exact relationship between
temperature and average kinetic
energy can be expressed:
(KE)avg=3/2 RT
The Meaning of Temperature
The Kelvin temperature is an index
of the random motions of the
particles of a gas, with higher
temperature meaning greater
motion.
Root Mean Square Velocity
u2
=the average of the squares of
the particle velocities.
The square root of u2
is called the
root mean square velocity and is
symbolized with urms
urms= =
M= mole of gas particles (kg)
R = ; J = kgm2
/s2
3RT
Mu2
8.3145
J
Kgmol
Root Mean Square Velocity
Example
Calculate the root mean square
velocity for the atoms in a sample
of helium gas at 25°C.
1.36 x 103
m/s
Mean Free Path
The average distance a particle travels
between collisions in a particular gas
sample.
1 x 10-7
m for O2 at STP
urms=500 m/s
Mean Free Path
A velocity distribution that show the effect
of temperature on the velocity distribution
in a gas.
Effusion
and
Diffusion
Diffusion
Diffusion describes the
mixing of gases.
The rate of mixing gases, is
the same as the rate of
diffusion
Dependent upon urms
Effusion
Effusion describes the
transfer of gas from one
chamber to another (usually
through a small hole or
porous opening).
The rate of transfer is said
to be the rate of effusion.
Effusion
The rate of effusion of a gas is
inversely proportional to the square
root of the mass of its particles.
Effusion
Rate of Effusion for gas 1
Rate of Effusion for gas 2
=
M2
M1
Temperature must be the same for
both gases.
M represents the molar masses of the
gases.
Units can be in g or kg since the
units will cancel out.
This is called Graham’s law of effusion:
Effusion Example
Calculate the effusion rates of
hydrogen gas (H2) and Uranium
hexafluoride (UF6), a gas used in the
enrichment process to produce fuel
for nuclear reactors.
13.2 : 1
Real
Gases
Real Gases
An ideal gas is a hypothetical
concept. No gas exactly
follows the ideal gas law,
although many gases come
very close at low pressures
and/or high temperatures.
Real Gases
Thus ideal gas behavior can
best be thought of as the
behavior approached by real
gases under certain
conditions.
Real Gases
Plots of PV/nRT vs. P for several gases
(200K). Ideal behavior only at low
pressures.
Real Gases
Plots of PV/nRT vs. P for N2 at three
temperatures. Ideal behavior at higher
temperatures.
KMT Modifications
Johannes van der Walls (1837-
1923), a physics professor at the
University of Amsterdam started
work in the area of ideal vs real gas
behavior. He won the nobel prize in
1910 for his work.
KMT Modifications
van der Waals modifications to the ideal
gas law accounted for the volume of
particle space. Therefore adjusting for the
volume actually available to a give gas
molecule.
V-nb
n is number of moles
b is an empirical constant
KMT Modifications
van der Waals modifications to the ideal
gas law allowed for the attractions that
occur among particle in a real gas which
is dependent upon the concentration of
the particles.
 , pressure correction
a is proportionality constant.
Pobs = Π∋
− α
ν
ϖ




2
van der Waals Equation
Insert both corrections and the equation
can be written as:
Rearranged for van der Waals:
Pobs =
νΡΤ
ς − νβ
− α
ν
ς




2
Pobs + α
ν
ς




2








ξ ς − νβ( ) = νΡΤ
van der Waals
Equation
a and b values are
determined for a given gas
by fitting experimental
behavior. That is a and b
are varied until the best fit
of the observed pressure is
obtained under all
conditions.
Characteristics of Real
Gases
A low value for a reflects
weak intermolecular forces
among gas molecules.
van der Waals
Ideal behavior at low
pressure (large volume)
makes sense because the
small amount of volume that
the particles consume are not
a factor.
van der Waals
Ideal behavior at high
temperatures also makes
sense because particles are
moving at such a high rate
that their interparticle
interactions are not very
important.
Chemistry in the
Atmosphere
Chemistry in the
Atmosphere
The most important gases to us are
those in the atmosphere that surround
the earth’s surface.
The principal components are N2 and
O2, but many other important gases,
such as H2O and CO2, are also
present.
Chemistry in the
Atmosphere
Because of gravitational effects, the
composition of the earth’s atmosphere
is not constant; heavier molecules
tend to be near the earth’s surface,
and light molecules tend to migrate to
higher altitudes, with some eventually
escaping into space.
Chemistry in the
Atmosphere
The chemistry occurring in the higher
levels of the atmosphere is mostly
determined by the effects of high-
energy radiation and particles from
the sun and other sources in space.
The upper atmosphere serves as a
shield to prevent this radiation from
reaching earth.
Chemistry in the
Atmosphere
The troposphere (closest to earth) is
strongly influenced by human
activities. Millions of tons of gases
and particulates are released into the
troposphere by our highly industrial
civilization.
Chemistry in the
Atmosphere
Severe air pollution is found around
many large cities. The two main
sources of pollution are transportation
and the production of electricity. The
combustion of petroleum in vehicles
produces CO, CO2, NO, NO2.
Chemistry in the
Atmosphere
The complex chemistry of polluted air
appears to center around the nitrogen
oxides (NOx). At high temperatures
found in the gasoline and diesel
engines of cars and trucks, N2 and O2
react to form a small quantity of NO
that is emitted into the air with the
exhaust gases. NO is immediately
oxidized in air to NO2.
Reactions in the
Atomsphere
NO2(g)
radiant
energy
→ NO(g) + O(g)
O(g) + O2(g) → O3(g)
Ozone is very reactive and can react directly with
other pollutants, or the ozone can absorb light and
break up to form an energetically excited O2 molecule
(O2*) and excited O (O*).
Reactions in the
Atomsphere
O*
+ H2O → 2OH
OH + NO2 → HNO3
The end product of this whole process is often referred
to as photochemical smog, so called because light is
required to initiate some of the reactions.
Reactions in the
Atomsphere
S(coal) + O2(g) → SO2(g)
2SO2(g ) + O2 → 2SO3(g )
SO3(g) + H2O(l) → H2SO4(aq)
Sulfuric acid is very corrosive to both living things and
building materials. Another result of this type of
pollution is called acid rain.
THE
END

More Related Content

What's hot

Gas laws
Gas lawsGas laws
Dalton's law tutorial 5.1
Dalton's law tutorial 5.1Dalton's law tutorial 5.1
Dalton's law tutorial 5.1sathiakumaran
 
Gas laws
Gas lawsGas laws
3 d presentation
3 d presentation3 d presentation
3 d presentation
Aileen Sambrano
 
New chm 151_unit_10_power_points
New chm 151_unit_10_power_pointsNew chm 151_unit_10_power_points
New chm 151_unit_10_power_pointscaneman1
 
Me 312 module 1
Me 312 module 1Me 312 module 1
Me 312 module 1
Yuri Melliza
 
Ch6 Thermochemistry (updated)
Ch6 Thermochemistry (updated)Ch6 Thermochemistry (updated)
Ch6 Thermochemistry (updated)
Sa'ib J. Khouri
 
06 dalton’s law of partial pressures
06 dalton’s law of partial pressures06 dalton’s law of partial pressures
06 dalton’s law of partial pressureszehnerm2
 
Dalton's Law of Partial Pressures
Dalton's Law of Partial PressuresDalton's Law of Partial Pressures
Dalton's Law of Partial PressuresEd Erhardt
 
Chapter 13: Gases
Chapter 13: GasesChapter 13: Gases
Chapter 13: Gases
American Nicaraguan School
 
New chm 151_unit_11_power_points_su13
New chm 151_unit_11_power_points_su13New chm 151_unit_11_power_points_su13
New chm 151_unit_11_power_points_su13caneman1
 
gaseous state
gaseous stategaseous state
gaseous state
suresh gdvm
 
state of matter gases and liquids
state of matter  gases and liquidsstate of matter  gases and liquids
state of matter gases and liquids
suresh gdvm
 
Ch5 z5e gases
Ch5 z5e gasesCh5 z5e gases
Ch5 z5e gasesblachman
 
Ch06 121227103404-phpapp01
Ch06 121227103404-phpapp01Ch06 121227103404-phpapp01
Ch06 121227103404-phpapp01
Cleophas Rwemera
 

What's hot (15)

Gas laws
Gas lawsGas laws
Gas laws
 
Dalton's law tutorial 5.1
Dalton's law tutorial 5.1Dalton's law tutorial 5.1
Dalton's law tutorial 5.1
 
Gas laws
Gas lawsGas laws
Gas laws
 
3 d presentation
3 d presentation3 d presentation
3 d presentation
 
New chm 151_unit_10_power_points
New chm 151_unit_10_power_pointsNew chm 151_unit_10_power_points
New chm 151_unit_10_power_points
 
Me 312 module 1
Me 312 module 1Me 312 module 1
Me 312 module 1
 
Ch6 Thermochemistry (updated)
Ch6 Thermochemistry (updated)Ch6 Thermochemistry (updated)
Ch6 Thermochemistry (updated)
 
06 dalton’s law of partial pressures
06 dalton’s law of partial pressures06 dalton’s law of partial pressures
06 dalton’s law of partial pressures
 
Dalton's Law of Partial Pressures
Dalton's Law of Partial PressuresDalton's Law of Partial Pressures
Dalton's Law of Partial Pressures
 
Chapter 13: Gases
Chapter 13: GasesChapter 13: Gases
Chapter 13: Gases
 
New chm 151_unit_11_power_points_su13
New chm 151_unit_11_power_points_su13New chm 151_unit_11_power_points_su13
New chm 151_unit_11_power_points_su13
 
gaseous state
gaseous stategaseous state
gaseous state
 
state of matter gases and liquids
state of matter  gases and liquidsstate of matter  gases and liquids
state of matter gases and liquids
 
Ch5 z5e gases
Ch5 z5e gasesCh5 z5e gases
Ch5 z5e gases
 
Ch06 121227103404-phpapp01
Ch06 121227103404-phpapp01Ch06 121227103404-phpapp01
Ch06 121227103404-phpapp01
 

Similar to Advchemchapt5 101015113821-phpapp01

Ch5 Gases
Ch5 GasesCh5 Gases
Ch5 Gases
Sa'ib J. Khouri
 
Combined gas law
Combined gas lawCombined gas law
Combined gas law
BernabeCeleste
 
Chapter 5 gases reduced1
Chapter 5  gases reduced1Chapter 5  gases reduced1
Chapter 5 gases reduced1
mtsaeed03
 
combined-gas-law-1.pptjsjsisujshsjsjjsjsjs
combined-gas-law-1.pptjsjsisujshsjsjjsjsjscombined-gas-law-1.pptjsjsisujshsjsjjsjsjs
combined-gas-law-1.pptjsjsisujshsjsjjsjsjs
NairdAidanMariano
 
Chapter 14 Gas Laws ppt 2017 good (1).ppt
Chapter 14 Gas Laws ppt 2017 good (1).pptChapter 14 Gas Laws ppt 2017 good (1).ppt
Chapter 14 Gas Laws ppt 2017 good (1).ppt
mikeebio1
 
States of matter
States of matterStates of matter
States of matterHoshi94
 
gaslaws-180210022037.pptx
gaslaws-180210022037.pptxgaslaws-180210022037.pptx
gaslaws-180210022037.pptx
LoryDacumosGonzalo
 
G10_Science_Q4-_Week_1-2-Constant_Temp_of_Gas[1].ppt
G10_Science_Q4-_Week_1-2-Constant_Temp_of_Gas[1].pptG10_Science_Q4-_Week_1-2-Constant_Temp_of_Gas[1].ppt
G10_Science_Q4-_Week_1-2-Constant_Temp_of_Gas[1].ppt
MelissaGanituenBauti
 
G10 Science Q4- Week 1-2-Constant Temp of Gas.ppt
G10 Science Q4- Week 1-2-Constant Temp of Gas.pptG10 Science Q4- Week 1-2-Constant Temp of Gas.ppt
G10 Science Q4- Week 1-2-Constant Temp of Gas.ppt
jinprix
 
Gases theory and basics .. general chemistry
Gases theory and basics .. general chemistryGases theory and basics .. general chemistry
Gases theory and basics .. general chemistry
fuat8
 
Ch5 Gases
Ch5 GasesCh5 Gases
Ch5 Gases
Sa'ib J. Khouri
 
Chem unit 12 presentation
Chem unit 12 presentationChem unit 12 presentation
Chem unit 12 presentation
bobcatchemistry
 
Unit 4: Behavior of Gases
Unit 4: Behavior of GasesUnit 4: Behavior of Gases
Unit 4: Behavior of Gases
Jimnaira Abanto
 
Ap physics 2_-_gas_laws
Ap physics 2_-_gas_lawsAp physics 2_-_gas_laws
Ap physics 2_-_gas_laws
kampkorten
 
Gas
GasGas
Gas
fhugob
 
Liyue.pptx
Liyue.pptxLiyue.pptx
Liyue.pptx
RoseyAckerman
 
Gases.pptx
Gases.pptxGases.pptx
Gases.pptx
FatmaMoustafa6
 

Similar to Advchemchapt5 101015113821-phpapp01 (20)

Ap Chem: Unit 5: Gases
Ap Chem: Unit 5: GasesAp Chem: Unit 5: Gases
Ap Chem: Unit 5: Gases
 
Ch5 Gases
Ch5 GasesCh5 Gases
Ch5 Gases
 
Combined gas law
Combined gas lawCombined gas law
Combined gas law
 
Chapter 5 gases reduced1
Chapter 5  gases reduced1Chapter 5  gases reduced1
Chapter 5 gases reduced1
 
combined-gas-law-1.pptjsjsisujshsjsjjsjsjs
combined-gas-law-1.pptjsjsisujshsjsjjsjsjscombined-gas-law-1.pptjsjsisujshsjsjjsjsjs
combined-gas-law-1.pptjsjsisujshsjsjjsjsjs
 
Chapter 14 Gas Laws ppt 2017 good (1).ppt
Chapter 14 Gas Laws ppt 2017 good (1).pptChapter 14 Gas Laws ppt 2017 good (1).ppt
Chapter 14 Gas Laws ppt 2017 good (1).ppt
 
States of matter
States of matterStates of matter
States of matter
 
gaslaws-180210022037.pptx
gaslaws-180210022037.pptxgaslaws-180210022037.pptx
gaslaws-180210022037.pptx
 
G10_Science_Q4-_Week_1-2-Constant_Temp_of_Gas[1].ppt
G10_Science_Q4-_Week_1-2-Constant_Temp_of_Gas[1].pptG10_Science_Q4-_Week_1-2-Constant_Temp_of_Gas[1].ppt
G10_Science_Q4-_Week_1-2-Constant_Temp_of_Gas[1].ppt
 
G10 Science Q4- Week 1-2-Constant Temp of Gas.ppt
G10 Science Q4- Week 1-2-Constant Temp of Gas.pptG10 Science Q4- Week 1-2-Constant Temp of Gas.ppt
G10 Science Q4- Week 1-2-Constant Temp of Gas.ppt
 
Gases theory and basics .. general chemistry
Gases theory and basics .. general chemistryGases theory and basics .. general chemistry
Gases theory and basics .. general chemistry
 
Ch5 Gases
Ch5 GasesCh5 Gases
Ch5 Gases
 
Chem unit 12 presentation
Chem unit 12 presentationChem unit 12 presentation
Chem unit 12 presentation
 
Unit 4: Behavior of Gases
Unit 4: Behavior of GasesUnit 4: Behavior of Gases
Unit 4: Behavior of Gases
 
Gas Laws
Gas  LawsGas  Laws
Gas Laws
 
Ap physics 2_-_gas_laws
Ap physics 2_-_gas_lawsAp physics 2_-_gas_laws
Ap physics 2_-_gas_laws
 
Gas
GasGas
Gas
 
Liyue.pptx
Liyue.pptxLiyue.pptx
Liyue.pptx
 
the gaseous state of matter
the gaseous state of matterthe gaseous state of matter
the gaseous state of matter
 
Gases.pptx
Gases.pptxGases.pptx
Gases.pptx
 

More from Cleophas Rwemera

Chapter003 150907175411-lva1-app6891
Chapter003 150907175411-lva1-app6891Chapter003 150907175411-lva1-app6891
Chapter003 150907175411-lva1-app6891
Cleophas Rwemera
 
Chapter002 150831173907-lva1-app6892
Chapter002 150831173907-lva1-app6892Chapter002 150831173907-lva1-app6892
Chapter002 150831173907-lva1-app6892
Cleophas Rwemera
 
Chapter001 150823230128-lva1-app6892
Chapter001 150823230128-lva1-app6892Chapter001 150823230128-lva1-app6892
Chapter001 150823230128-lva1-app6892
Cleophas Rwemera
 
Chapter25 cancer-140105085413-phpapp01
Chapter25 cancer-140105085413-phpapp01Chapter25 cancer-140105085413-phpapp01
Chapter25 cancer-140105085413-phpapp01
Cleophas Rwemera
 
Chapter24 immunology-140105101108-phpapp02
Chapter24 immunology-140105101108-phpapp02Chapter24 immunology-140105101108-phpapp02
Chapter24 immunology-140105101108-phpapp02
Cleophas Rwemera
 
Chapter23 nervecells-140105100942-phpapp02
Chapter23 nervecells-140105100942-phpapp02Chapter23 nervecells-140105100942-phpapp02
Chapter23 nervecells-140105100942-phpapp02
Cleophas Rwemera
 
Chapter22 themolecularcellbiologyofdevelopment-140105100412-phpapp02
Chapter22 themolecularcellbiologyofdevelopment-140105100412-phpapp02Chapter22 themolecularcellbiologyofdevelopment-140105100412-phpapp02
Chapter22 themolecularcellbiologyofdevelopment-140105100412-phpapp02
Cleophas Rwemera
 
Chapter21 cellbirthlineageanddeath-140105095914-phpapp02
Chapter21 cellbirthlineageanddeath-140105095914-phpapp02Chapter21 cellbirthlineageanddeath-140105095914-phpapp02
Chapter21 cellbirthlineageanddeath-140105095914-phpapp02
Cleophas Rwemera
 
Chapter20 regulatingtheeukaryoticcellcycle-140105095738-phpapp01
Chapter20 regulatingtheeukaryoticcellcycle-140105095738-phpapp01Chapter20 regulatingtheeukaryoticcellcycle-140105095738-phpapp01
Chapter20 regulatingtheeukaryoticcellcycle-140105095738-phpapp01
Cleophas Rwemera
 
Chapter19 integratingcellsintotissues-140105095535-phpapp02
Chapter19 integratingcellsintotissues-140105095535-phpapp02Chapter19 integratingcellsintotissues-140105095535-phpapp02
Chapter19 integratingcellsintotissues-140105095535-phpapp02
Cleophas Rwemera
 
Chapter18 cellorganizationandmovementiimicrotubulesandintermediatefilaments-1...
Chapter18 cellorganizationandmovementiimicrotubulesandintermediatefilaments-1...Chapter18 cellorganizationandmovementiimicrotubulesandintermediatefilaments-1...
Chapter18 cellorganizationandmovementiimicrotubulesandintermediatefilaments-1...
Cleophas Rwemera
 
Chapter17 cellorganizationandmovementimicrofilaments-140105094810-phpapp02
Chapter17 cellorganizationandmovementimicrofilaments-140105094810-phpapp02Chapter17 cellorganizationandmovementimicrofilaments-140105094810-phpapp02
Chapter17 cellorganizationandmovementimicrofilaments-140105094810-phpapp02
Cleophas Rwemera
 
Chapter16 cellsignalingiisignalingpathwaysthatcontrolgeneactivity-14010509451...
Chapter16 cellsignalingiisignalingpathwaysthatcontrolgeneactivity-14010509451...Chapter16 cellsignalingiisignalingpathwaysthatcontrolgeneactivity-14010509451...
Chapter16 cellsignalingiisignalingpathwaysthatcontrolgeneactivity-14010509451...
Cleophas Rwemera
 
Chapter15 cellsignalingisignaltransductionandshort-termcellularresponses-1401...
Chapter15 cellsignalingisignaltransductionandshort-termcellularresponses-1401...Chapter15 cellsignalingisignaltransductionandshort-termcellularresponses-1401...
Chapter15 cellsignalingisignaltransductionandshort-termcellularresponses-1401...
Cleophas Rwemera
 
Chapter14 vesiculartrafficsecretionandendocytosis-140105094215-phpapp01
Chapter14 vesiculartrafficsecretionandendocytosis-140105094215-phpapp01Chapter14 vesiculartrafficsecretionandendocytosis-140105094215-phpapp01
Chapter14 vesiculartrafficsecretionandendocytosis-140105094215-phpapp01
Cleophas Rwemera
 
Chapter13 movingproteinsintomembranesandorganelles-140105094005-phpapp01
Chapter13 movingproteinsintomembranesandorganelles-140105094005-phpapp01Chapter13 movingproteinsintomembranesandorganelles-140105094005-phpapp01
Chapter13 movingproteinsintomembranesandorganelles-140105094005-phpapp01
Cleophas Rwemera
 
Chapter12 cellularenergetics-140105093734-phpapp01
Chapter12 cellularenergetics-140105093734-phpapp01Chapter12 cellularenergetics-140105093734-phpapp01
Chapter12 cellularenergetics-140105093734-phpapp01
Cleophas Rwemera
 
Chapter11 transmembranetransportofionsandsmallmolecules-140105092904-phpapp02
Chapter11 transmembranetransportofionsandsmallmolecules-140105092904-phpapp02Chapter11 transmembranetransportofionsandsmallmolecules-140105092904-phpapp02
Chapter11 transmembranetransportofionsandsmallmolecules-140105092904-phpapp02
Cleophas Rwemera
 
Chapter10 biomembranestructure-140105093829-phpapp02
Chapter10 biomembranestructure-140105093829-phpapp02Chapter10 biomembranestructure-140105093829-phpapp02
Chapter10 biomembranestructure-140105093829-phpapp02
Cleophas Rwemera
 
Chapter9 visualizingfractionatingandculturingcells-140105092245-phpapp01
Chapter9 visualizingfractionatingandculturingcells-140105092245-phpapp01Chapter9 visualizingfractionatingandculturingcells-140105092245-phpapp01
Chapter9 visualizingfractionatingandculturingcells-140105092245-phpapp01
Cleophas Rwemera
 

More from Cleophas Rwemera (20)

Chapter003 150907175411-lva1-app6891
Chapter003 150907175411-lva1-app6891Chapter003 150907175411-lva1-app6891
Chapter003 150907175411-lva1-app6891
 
Chapter002 150831173907-lva1-app6892
Chapter002 150831173907-lva1-app6892Chapter002 150831173907-lva1-app6892
Chapter002 150831173907-lva1-app6892
 
Chapter001 150823230128-lva1-app6892
Chapter001 150823230128-lva1-app6892Chapter001 150823230128-lva1-app6892
Chapter001 150823230128-lva1-app6892
 
Chapter25 cancer-140105085413-phpapp01
Chapter25 cancer-140105085413-phpapp01Chapter25 cancer-140105085413-phpapp01
Chapter25 cancer-140105085413-phpapp01
 
Chapter24 immunology-140105101108-phpapp02
Chapter24 immunology-140105101108-phpapp02Chapter24 immunology-140105101108-phpapp02
Chapter24 immunology-140105101108-phpapp02
 
Chapter23 nervecells-140105100942-phpapp02
Chapter23 nervecells-140105100942-phpapp02Chapter23 nervecells-140105100942-phpapp02
Chapter23 nervecells-140105100942-phpapp02
 
Chapter22 themolecularcellbiologyofdevelopment-140105100412-phpapp02
Chapter22 themolecularcellbiologyofdevelopment-140105100412-phpapp02Chapter22 themolecularcellbiologyofdevelopment-140105100412-phpapp02
Chapter22 themolecularcellbiologyofdevelopment-140105100412-phpapp02
 
Chapter21 cellbirthlineageanddeath-140105095914-phpapp02
Chapter21 cellbirthlineageanddeath-140105095914-phpapp02Chapter21 cellbirthlineageanddeath-140105095914-phpapp02
Chapter21 cellbirthlineageanddeath-140105095914-phpapp02
 
Chapter20 regulatingtheeukaryoticcellcycle-140105095738-phpapp01
Chapter20 regulatingtheeukaryoticcellcycle-140105095738-phpapp01Chapter20 regulatingtheeukaryoticcellcycle-140105095738-phpapp01
Chapter20 regulatingtheeukaryoticcellcycle-140105095738-phpapp01
 
Chapter19 integratingcellsintotissues-140105095535-phpapp02
Chapter19 integratingcellsintotissues-140105095535-phpapp02Chapter19 integratingcellsintotissues-140105095535-phpapp02
Chapter19 integratingcellsintotissues-140105095535-phpapp02
 
Chapter18 cellorganizationandmovementiimicrotubulesandintermediatefilaments-1...
Chapter18 cellorganizationandmovementiimicrotubulesandintermediatefilaments-1...Chapter18 cellorganizationandmovementiimicrotubulesandintermediatefilaments-1...
Chapter18 cellorganizationandmovementiimicrotubulesandintermediatefilaments-1...
 
Chapter17 cellorganizationandmovementimicrofilaments-140105094810-phpapp02
Chapter17 cellorganizationandmovementimicrofilaments-140105094810-phpapp02Chapter17 cellorganizationandmovementimicrofilaments-140105094810-phpapp02
Chapter17 cellorganizationandmovementimicrofilaments-140105094810-phpapp02
 
Chapter16 cellsignalingiisignalingpathwaysthatcontrolgeneactivity-14010509451...
Chapter16 cellsignalingiisignalingpathwaysthatcontrolgeneactivity-14010509451...Chapter16 cellsignalingiisignalingpathwaysthatcontrolgeneactivity-14010509451...
Chapter16 cellsignalingiisignalingpathwaysthatcontrolgeneactivity-14010509451...
 
Chapter15 cellsignalingisignaltransductionandshort-termcellularresponses-1401...
Chapter15 cellsignalingisignaltransductionandshort-termcellularresponses-1401...Chapter15 cellsignalingisignaltransductionandshort-termcellularresponses-1401...
Chapter15 cellsignalingisignaltransductionandshort-termcellularresponses-1401...
 
Chapter14 vesiculartrafficsecretionandendocytosis-140105094215-phpapp01
Chapter14 vesiculartrafficsecretionandendocytosis-140105094215-phpapp01Chapter14 vesiculartrafficsecretionandendocytosis-140105094215-phpapp01
Chapter14 vesiculartrafficsecretionandendocytosis-140105094215-phpapp01
 
Chapter13 movingproteinsintomembranesandorganelles-140105094005-phpapp01
Chapter13 movingproteinsintomembranesandorganelles-140105094005-phpapp01Chapter13 movingproteinsintomembranesandorganelles-140105094005-phpapp01
Chapter13 movingproteinsintomembranesandorganelles-140105094005-phpapp01
 
Chapter12 cellularenergetics-140105093734-phpapp01
Chapter12 cellularenergetics-140105093734-phpapp01Chapter12 cellularenergetics-140105093734-phpapp01
Chapter12 cellularenergetics-140105093734-phpapp01
 
Chapter11 transmembranetransportofionsandsmallmolecules-140105092904-phpapp02
Chapter11 transmembranetransportofionsandsmallmolecules-140105092904-phpapp02Chapter11 transmembranetransportofionsandsmallmolecules-140105092904-phpapp02
Chapter11 transmembranetransportofionsandsmallmolecules-140105092904-phpapp02
 
Chapter10 biomembranestructure-140105093829-phpapp02
Chapter10 biomembranestructure-140105093829-phpapp02Chapter10 biomembranestructure-140105093829-phpapp02
Chapter10 biomembranestructure-140105093829-phpapp02
 
Chapter9 visualizingfractionatingandculturingcells-140105092245-phpapp01
Chapter9 visualizingfractionatingandculturingcells-140105092245-phpapp01Chapter9 visualizingfractionatingandculturingcells-140105092245-phpapp01
Chapter9 visualizingfractionatingandculturingcells-140105092245-phpapp01
 

Recently uploaded

Mule 4.6 & Java 17 Upgrade | MuleSoft Mysore Meetup #46
Mule 4.6 & Java 17 Upgrade | MuleSoft Mysore Meetup #46Mule 4.6 & Java 17 Upgrade | MuleSoft Mysore Meetup #46
Mule 4.6 & Java 17 Upgrade | MuleSoft Mysore Meetup #46
MysoreMuleSoftMeetup
 
The Roman Empire A Historical Colossus.pdf
The Roman Empire A Historical Colossus.pdfThe Roman Empire A Historical Colossus.pdf
The Roman Empire A Historical Colossus.pdf
kaushalkr1407
 
Supporting (UKRI) OA monographs at Salford.pptx
Supporting (UKRI) OA monographs at Salford.pptxSupporting (UKRI) OA monographs at Salford.pptx
Supporting (UKRI) OA monographs at Salford.pptx
Jisc
 
aaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaa
aaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaa
aaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaa
siemaillard
 
The approach at University of Liverpool.pptx
The approach at University of Liverpool.pptxThe approach at University of Liverpool.pptx
The approach at University of Liverpool.pptx
Jisc
 
Ethnobotany and Ethnopharmacology ......
Ethnobotany and Ethnopharmacology ......Ethnobotany and Ethnopharmacology ......
Ethnobotany and Ethnopharmacology ......
Ashokrao Mane college of Pharmacy Peth-Vadgaon
 
Sectors of the Indian Economy - Class 10 Study Notes pdf
Sectors of the Indian Economy - Class 10 Study Notes pdfSectors of the Indian Economy - Class 10 Study Notes pdf
Sectors of the Indian Economy - Class 10 Study Notes pdf
Vivekanand Anglo Vedic Academy
 
Thesis Statement for students diagnonsed withADHD.ppt
Thesis Statement for students diagnonsed withADHD.pptThesis Statement for students diagnonsed withADHD.ppt
Thesis Statement for students diagnonsed withADHD.ppt
EverAndrsGuerraGuerr
 
How to Break the cycle of negative Thoughts
How to Break the cycle of negative ThoughtsHow to Break the cycle of negative Thoughts
How to Break the cycle of negative Thoughts
Col Mukteshwar Prasad
 
Additional Benefits for Employee Website.pdf
Additional Benefits for Employee Website.pdfAdditional Benefits for Employee Website.pdf
Additional Benefits for Employee Website.pdf
joachimlavalley1
 
ESC Beyond Borders _From EU to You_ InfoPack general.pdf
ESC Beyond Borders _From EU to You_ InfoPack general.pdfESC Beyond Borders _From EU to You_ InfoPack general.pdf
ESC Beyond Borders _From EU to You_ InfoPack general.pdf
Fundacja Rozwoju Społeczeństwa Przedsiębiorczego
 
Cambridge International AS A Level Biology Coursebook - EBook (MaryFosbery J...
Cambridge International AS  A Level Biology Coursebook - EBook (MaryFosbery J...Cambridge International AS  A Level Biology Coursebook - EBook (MaryFosbery J...
Cambridge International AS A Level Biology Coursebook - EBook (MaryFosbery J...
AzmatAli747758
 
Overview on Edible Vaccine: Pros & Cons with Mechanism
Overview on Edible Vaccine: Pros & Cons with MechanismOverview on Edible Vaccine: Pros & Cons with Mechanism
Overview on Edible Vaccine: Pros & Cons with Mechanism
DeeptiGupta154
 
Sha'Carri Richardson Presentation 202345
Sha'Carri Richardson Presentation 202345Sha'Carri Richardson Presentation 202345
Sha'Carri Richardson Presentation 202345
beazzy04
 
The French Revolution Class 9 Study Material pdf free download
The French Revolution Class 9 Study Material pdf free downloadThe French Revolution Class 9 Study Material pdf free download
The French Revolution Class 9 Study Material pdf free download
Vivekanand Anglo Vedic Academy
 
2024.06.01 Introducing a competency framework for languag learning materials ...
2024.06.01 Introducing a competency framework for languag learning materials ...2024.06.01 Introducing a competency framework for languag learning materials ...
2024.06.01 Introducing a competency framework for languag learning materials ...
Sandy Millin
 
PART A. Introduction to Costumer Service
PART A. Introduction to Costumer ServicePART A. Introduction to Costumer Service
PART A. Introduction to Costumer Service
PedroFerreira53928
 
How to Split Bills in the Odoo 17 POS Module
How to Split Bills in the Odoo 17 POS ModuleHow to Split Bills in the Odoo 17 POS Module
How to Split Bills in the Odoo 17 POS Module
Celine George
 
TESDA TM1 REVIEWER FOR NATIONAL ASSESSMENT WRITTEN AND ORAL QUESTIONS WITH A...
TESDA TM1 REVIEWER  FOR NATIONAL ASSESSMENT WRITTEN AND ORAL QUESTIONS WITH A...TESDA TM1 REVIEWER  FOR NATIONAL ASSESSMENT WRITTEN AND ORAL QUESTIONS WITH A...
TESDA TM1 REVIEWER FOR NATIONAL ASSESSMENT WRITTEN AND ORAL QUESTIONS WITH A...
EugeneSaldivar
 
MARUTI SUZUKI- A Successful Joint Venture in India.pptx
MARUTI SUZUKI- A Successful Joint Venture in India.pptxMARUTI SUZUKI- A Successful Joint Venture in India.pptx
MARUTI SUZUKI- A Successful Joint Venture in India.pptx
bennyroshan06
 

Recently uploaded (20)

Mule 4.6 & Java 17 Upgrade | MuleSoft Mysore Meetup #46
Mule 4.6 & Java 17 Upgrade | MuleSoft Mysore Meetup #46Mule 4.6 & Java 17 Upgrade | MuleSoft Mysore Meetup #46
Mule 4.6 & Java 17 Upgrade | MuleSoft Mysore Meetup #46
 
The Roman Empire A Historical Colossus.pdf
The Roman Empire A Historical Colossus.pdfThe Roman Empire A Historical Colossus.pdf
The Roman Empire A Historical Colossus.pdf
 
Supporting (UKRI) OA monographs at Salford.pptx
Supporting (UKRI) OA monographs at Salford.pptxSupporting (UKRI) OA monographs at Salford.pptx
Supporting (UKRI) OA monographs at Salford.pptx
 
aaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaa
aaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaa
aaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaaa
 
The approach at University of Liverpool.pptx
The approach at University of Liverpool.pptxThe approach at University of Liverpool.pptx
The approach at University of Liverpool.pptx
 
Ethnobotany and Ethnopharmacology ......
Ethnobotany and Ethnopharmacology ......Ethnobotany and Ethnopharmacology ......
Ethnobotany and Ethnopharmacology ......
 
Sectors of the Indian Economy - Class 10 Study Notes pdf
Sectors of the Indian Economy - Class 10 Study Notes pdfSectors of the Indian Economy - Class 10 Study Notes pdf
Sectors of the Indian Economy - Class 10 Study Notes pdf
 
Thesis Statement for students diagnonsed withADHD.ppt
Thesis Statement for students diagnonsed withADHD.pptThesis Statement for students diagnonsed withADHD.ppt
Thesis Statement for students diagnonsed withADHD.ppt
 
How to Break the cycle of negative Thoughts
How to Break the cycle of negative ThoughtsHow to Break the cycle of negative Thoughts
How to Break the cycle of negative Thoughts
 
Additional Benefits for Employee Website.pdf
Additional Benefits for Employee Website.pdfAdditional Benefits for Employee Website.pdf
Additional Benefits for Employee Website.pdf
 
ESC Beyond Borders _From EU to You_ InfoPack general.pdf
ESC Beyond Borders _From EU to You_ InfoPack general.pdfESC Beyond Borders _From EU to You_ InfoPack general.pdf
ESC Beyond Borders _From EU to You_ InfoPack general.pdf
 
Cambridge International AS A Level Biology Coursebook - EBook (MaryFosbery J...
Cambridge International AS  A Level Biology Coursebook - EBook (MaryFosbery J...Cambridge International AS  A Level Biology Coursebook - EBook (MaryFosbery J...
Cambridge International AS A Level Biology Coursebook - EBook (MaryFosbery J...
 
Overview on Edible Vaccine: Pros & Cons with Mechanism
Overview on Edible Vaccine: Pros & Cons with MechanismOverview on Edible Vaccine: Pros & Cons with Mechanism
Overview on Edible Vaccine: Pros & Cons with Mechanism
 
Sha'Carri Richardson Presentation 202345
Sha'Carri Richardson Presentation 202345Sha'Carri Richardson Presentation 202345
Sha'Carri Richardson Presentation 202345
 
The French Revolution Class 9 Study Material pdf free download
The French Revolution Class 9 Study Material pdf free downloadThe French Revolution Class 9 Study Material pdf free download
The French Revolution Class 9 Study Material pdf free download
 
2024.06.01 Introducing a competency framework for languag learning materials ...
2024.06.01 Introducing a competency framework for languag learning materials ...2024.06.01 Introducing a competency framework for languag learning materials ...
2024.06.01 Introducing a competency framework for languag learning materials ...
 
PART A. Introduction to Costumer Service
PART A. Introduction to Costumer ServicePART A. Introduction to Costumer Service
PART A. Introduction to Costumer Service
 
How to Split Bills in the Odoo 17 POS Module
How to Split Bills in the Odoo 17 POS ModuleHow to Split Bills in the Odoo 17 POS Module
How to Split Bills in the Odoo 17 POS Module
 
TESDA TM1 REVIEWER FOR NATIONAL ASSESSMENT WRITTEN AND ORAL QUESTIONS WITH A...
TESDA TM1 REVIEWER  FOR NATIONAL ASSESSMENT WRITTEN AND ORAL QUESTIONS WITH A...TESDA TM1 REVIEWER  FOR NATIONAL ASSESSMENT WRITTEN AND ORAL QUESTIONS WITH A...
TESDA TM1 REVIEWER FOR NATIONAL ASSESSMENT WRITTEN AND ORAL QUESTIONS WITH A...
 
MARUTI SUZUKI- A Successful Joint Venture in India.pptx
MARUTI SUZUKI- A Successful Joint Venture in India.pptxMARUTI SUZUKI- A Successful Joint Venture in India.pptx
MARUTI SUZUKI- A Successful Joint Venture in India.pptx
 

Advchemchapt5 101015113821-phpapp01

  • 2. Intro Earth’s atmosphere is a gaseous solution that consists mainly of nitrogen (N2) and oxygen (O2). This atmosphere supports life and acts as a waste receptacle for many industrial processes. The chemical reactions that follow often lead to various types of pollution, including smog and acid rain.
  • 3. Intro The gases in the atmosphere also shield us from harmful radiation from the sun and keep the earth warm by reflecting heat radiation back toward the earth. In fact, there is now great concern that an increase in atmospheric carbon dioxide, a product of the combustion of fossil fuels , is causing a dangerous warming of the earth.
  • 5. Pressure Gas uniformly fills a container, is easily compressed, and mixes completely with any other gas. One of the most important properties is that it exerts pressure on its surroundings equally.
  • 10. Pressure Barometer - A device to measure atmospheric pressure, was invented in 1643 by Torricelli (a student of Galileo). Torricelli’s barometer is constructed by filling a glass tube with liquid mercury and inverting it in a dish of mercury.
  • 11. Pressure Barometer - A device to measure atmospheric pressure, was invented in 1643 by Torricelli (a student of Galileo). Notice that a large quantity of mercury stays in the tube. In fact, at sea level the height of this column of mercury averages 760 mm.
  • 12. Pressure Barometer - A device to measure atmospheric pressure, was invented in 1643 by Torricelli (a student of Galileo). Atmospheric pressure results from the mass of the air being pulled toward the center of the earth by gravity.
  • 13. Pressure Barometer - A device to measure atmospheric pressure, was invented in 1643 by Torricelli (a student of Galileo). Atmospheric pressure varies with weather changes and altitude.
  • 14. Pressure Manometer – an instrument for measuring pressure often below that of atmospheric pressure.
  • 15. Units of Pressure Pressure = force/area torr – in honor of Torricelli is equal to a mm Hg. 760 mm Hg = 760 torr 1 atm = 760 torr Pascal = N/m2 1atm = 101,325 Pa
  • 18. Boyles Law Boyle (1627-1691) – performed the first quantitative experiments on gases. Used a J tube to measure pressures. PV = k; P1V1=P2V2 k is a constant for a given sample of air at a specific temperature.
  • 19. Boyles Law Pressure and volume are often plotted. P vs V – gives a hyperbola and an inverse relationship. Boyles law rearranged is V=k/P=k1/P; when plotted as V vs 1/P – gives a straight line with the intercept of zero
  • 21. Boyles Law Boyles’s law holds precisely at very low temperatures, but varies at higher pressures. PV will vary as pressure is varied. An ideal gas is a gas that strictly obeys Boyles’ law.
  • 23. Charles Law Charles (1746-1823) – the first person to fill a balloon with hydrogen gas and who made the first solo balloon flight. Charles found in 1787 that the volume of a gas at constant pressure increases linearly with the temperature of the gas. V = bT ; V1/T1 = V2/T2 T is in Kelvin, b is a proportionality constant
  • 24. Charles Law Temperature vs Volume plots a straight line. Slope will vary will type of gas. All gas plots of T vs V will extrapolate to zero at the same temperature. -273° or 0 K
  • 26. Avogadro’s Law Avogadro (1811) – postulated that equal volumes of gases at the same temperature and pressure contain the same number of particles (moles). V = an; V1/n1=V2/n2 n is number of moles; a is a proportionality constant.
  • 28. Ideal Gas Law The relationships that Boyle, Charles and Avogadro presented can be combined to show how the volume of a gas depends on pressure, temperature, and number of moles of gas present. V = R(Tn/P) R is the universal gas constant. A combination of proportionality constants
  • 29. Ideal Gas Law The equation is often rearranged to form the more common: PV=nRT R=.08206 Latm/Kmol
  • 30. Ideal Gas Law Limitations A gas that obeys this equation is said to behave ideally. The ideal gas equation is best regarded as a limiting law, it expresses behavior that real gases approach at low pressures and high temperatures. Most gases behave ideally at pressures below 1 atm.
  • 31. Example Problem A sample of hydrogen gas (H2) has a volume of 8.56 L at a temperature of 0°C and a pressure of 1.5 atm. Calculate the moles of H2 molecules present in this gas sample.
  • 32. Example Problem V = 8.56 L at a temperature of 0°C P =1.5 atm Calculate the moles PV=nRT; R = .08206 L atm/K mol .57 mol
  • 33. Example Problem 2 You have a sample of ammonia gas with a a volume of 7.0ml at a pressure of 1.68 atm. The gas is compressed to a volume of 2.7 ml at a constant temperature. Use the ideal gas law to calculate the final pressure.
  • 34. Example Problem 2 V1 = 7.0 ml at a pressure of 1.68 atm V2 =2.7 ml at a constant temperature. Calculate the final pressure. PV=nRT; but nRT are constant: PV=PV 4.4 atm
  • 35. Example Problem 3 A sample of methane gas that has a volume of 3.8 L at 5°C is heated to 86°C at constant pressure. Calculate its new volume.
  • 36. Example Problem 3 V1 = 3.8 L and T15°C T2=86°C at constant pressure. Calculate its new volume. PV=nRT but n, R and P are constant: V1/T1 = V2/T2 4.9 L
  • 37. Example Problem 4 A sample of diborane gas (B2H6), a substance that burst into flame when exposed to air, has a pressure of 345 torr at a temperature of -15°C and a volume of 3.48 L. If conditions are changed so that the temperature is 36°C and the pressure is 468 torr, what will be the volume of the sample.
  • 38. Example Problem 4 P1=345 torr, T1=-15°C and V1 = 3.48L T2=36°C and P2=468 torr, What is the volume? PV = nRT; nR are constant: P1V1/T1 = P2V2/T2 3.1 L
  • 39. Example Problem 5 A sample containing 0.35 mol argon gas at a temperature of 13°C and a pressure of 568 torr is heated to 56°C and a pressure of 897 torr. Calculate the change in volume that occurs.
  • 40. Example Problem 5 n=0.35, T1=13°C, P1=568 torr T2=56°C, P2=897 torr Calculate the change in volume that occurs. -3 L PV=nRT; R = .08206 L atm/K mol
  • 41. Practice Problems Page 226 #41, 43, 45, 47, 49, 51, 53, 57, 59, 61
  • 43. Molar Volume One mole of an ideal gas at:  0°C (273K) 1atm V=nRT/P = 22.42L
  • 44. Gas Stoichiometry We use STP or standard temperature and pressure of an ideal gas to make calculations with a gas. 1 atm 0°C (273K) 1 mole = 22.42 L becomes a conversion factor for dimensional analysis.
  • 45. Gas Stoichiometry Example A sample of nitrogen gas has a volume of 1.75 L at STP. How many moles of N2 are present? 1.75L N2 x 1mole N2 22.42L N2 = 7.81 x 10-2 mol N2
  • 46. Gas Stoichiometry Example 2 Quicklime (CaO) is produced by the thermal decomposition of calcium carbonate (CaCO3). Calculate the volume of CO2 at STP produced from the decomposition of 152g CaCO3 by the reaction CaCO3(s) CaO(s) + CO2(g)
  • 47. Gas Stoichiometry Example 2 152g CaCO3 22.42 L = 1 mol of gas at STP Calculate the volume of CO2 CaCO3(s) CaO(s) + CO2(g) 34.1 L CO2 at STP
  • 48. Gas Stoichiometry Example 3 A sample of methane gas having a volume of 2.80 L at 25°C and 1.65 atm was mixed with a sample of oxygen gas having a volume of 35.0 L at 31°C and 1.25 atm. The mixture was then ignited to form carbon dioxide and water. Calculate the volume of CO2 formed at a pressure of 2.50 atm and a temperature of 125°.
  • 49. Gas Stoichiometry Example 3 CH4 V=2.80 L at 25°C and 1.65 atm Oxygen V=35.0 L at 31°C and 1.25 atm. Calculate the volume of CO2 at 2.50 atm and 125°C. The mixture was then ignited to form carbon dioxide and water.
  • 50. Gas Stoichiometry Example 3 CH4 V=2.80 L at 25°C and 1.65 atm Oxygen V=35.0 L at 31°C and 1.25 atm. Calculate the volume of CO2 at 2.50 atm and 125°C. CH4(g) + O2(g)  CO2(g) + H2O(g) 2.47 L
  • 52. Molar Mass of a Gas  One use of the ideal gas law is in the calculations of the molar mass of a gas from its measured density.  n =  P  D  P = grams of gas molar mass = µ µολαρµασσ = nRT V = m / molar mass( )RT V = mRT V(molar mass) = m V dRT molar mass ; Molar mass = δΡΤ Π
  • 53. Gas Density/Molar Mass Example The density of a gas was measured at 1.50 atm and 27°C and found to be 1.95 g/L. Calculate the molar mass of the gas. 32.0 g/mol
  • 55. John Dalton John Dalton formed his atomic theory from his experiments and studies of the mixture of gases. His observations car be summarized as follows: For a mixture of gases in a container, the total pressure exerted is the sum of the pressures that each as would exert if it were alone.
  • 56. John Dalton Ptotal=P1+P2+P3+…. Subscripts refer to the individual gases and Px refers to partial pressure that a particular gas would exert if it were alone in the container. Each Partial pressure can be derived from the ideal gas law and added together to determine the total.
  • 57. John Dalton Ptotal=P1+P2+P3+…. Since each partial pressure can be broken down into ; the Ptotal can be represented by: Ptotal= Ptotal= nx RT V (n1 + ν2 + ν3 + ...) ΡΤ ς     ntotal RT V    
  • 58. For a mixture of ideal gases, it is the total number of moles of particles that is important, not the identity or composition of the involved gas particle.
  • 59. Dalton’s Law Example Mixtures of helium and oxygen can be used in scuba diving tanks to help prevent “the bends.” For a particular dive, 46 L He at 25° and 1.0 atm and 12 L O2 at 25° and 1.0 atm were pumped into a tank with a volume of 5.0 L. Calculate the partial pressure of each gas and the total pressure in the tank at 25° C.
  • 60. Mole Fraction The ratio of the number of moles of a given component in a mixture to the total number of moles in the mixture.  = nχ x/ntotal  = Pχ 1/Ptotal
  • 61. Dalton’s Law Example The partial pressure of oxygen was observed to be 156 torr in air with a total atmospheric pressure of 743 torr. Calculate the mole fraction of O2 present.
  • 62. Dalton’s Law Example The mole fraction of nitrogen in the air is 0.7808. Calculate the partial pressure of N2 in air when the atmospheric pressure is 760 torr.
  • 63. Collecting Gas over Water A mixture of gases results whenever a gas is collected by displacement of water. In this situation, the gas in the bottle is a mixture of water vapor and the oxygen being collected.
  • 64. Collecting Gas over Water Water vapor is present because molecules of water escape from the surface of the liquid and collect in the space above the liquid.
  • 65. Collecting Gas over Water Molecules of water also return to the liquid. When the rate of escape equals the rate of return, the number of water molecules in the vapor state remain constant.
  • 66. Collecting Gas over Water When the number of water molecules in the vapor state remain constant the pressure of the water vapor remains constant.
  • 67. Collecting Gas over Water This pressure, which depends on temperature, is called vapor pressure of water.
  • 68. Collecting Gas over Water Example A sample of solid potassium chlorate (KClO3) was heated in a test tube and decomposed by the reaction: 2KClO3(s) → 2ΚΧλ(σ) + 3Ο2(γ )
  • 69. Collecting Gas over Water Example The oxygen produced was collected by displacement of water at 22°C at a total pressure of 754 torr. The volume of gas collected was .650L, and the vapor pressure of water at 22°C is 21 torr. Calculate the partial pressure of O2 in the gas collected and the mass of KClO3 in the sample that was decomposed. 2KClO3(s) → 2ΚΧλ(σ) + 3Ο2(γ )
  • 70. Collecting Gas over Water Example oxygen T=22°C and V=.650L Total pressure = 754 torr. vapor pressure at 22°C is 21 torr. Calculate the partial pressure of O2 and the mass of KClO3 in the sample 2KClO3(s) → 2ΚΧλ(σ) + 3Ο2(γ ) 2.59 x 10-2 mol O2 2.12 g KClO3
  • 72. Kinetic Molecular Theory KMT A simple model that attempts to explain the properties of an ideal gas. This model is based on speculations about the behavior of the individual gas particles (atoms or molecules).
  • 73. Kinetic Molecular Theory KMT 1. The particles are so small compared with the distances between them that the volume of the individual particles can be assumed to be negligible (zero).
  • 74. Kinetic Molecular Theory KMT 2. The particles are in constant motion. The collisions of the particles with the walls of the container are the cause of the pressure exerted by the gas.
  • 75. Kinetic Molecular Theory KMT 3. The particles are assumed to exert no forces on each other; they are assumed neither to attract nor to repel each other.
  • 76. Kinetic Molecular Theory KMT 4. The average kinetic energy of a collection of gas particles is assumed to be directly proportional to the Kelvin temperature of the gas.
  • 77. KMT and Boyle’s Law  Because a decrease in volume, the gas particles will hit the walls more often, thus increasing the pressure
  • 78. KMT and Charles Law  When the gas is heated to a higher temperature, the speeds of its molecules increase and thus hit the walls more often and with more force. Volume and/or pressure will increase.
  • 79. KMT and Advogadro’s Law  An increase in the number of gas particles at the same temperature would cause the pressure to increase if the volume were constant.
  • 80. KMT and Advogadro’s Law  The volume of a gas (at constant T and P) depends only on the number of gas particles present. The individual particles are not a factor because the particle volumes are so small compared with the distances between the particles.
  • 81. KMT and Dalton’s Law  All gas particles are independent of each other and that the volumes of the individual particles are unimportant. Identities of the gas particles do not matter.
  • 82. The Meaning of Temperature Kelvin temperature indicates the average kinetic energy of the gas particles. The exact relationship between temperature and average kinetic energy can be expressed: (KE)avg=3/2 RT
  • 83. The Meaning of Temperature The Kelvin temperature is an index of the random motions of the particles of a gas, with higher temperature meaning greater motion.
  • 84. Root Mean Square Velocity u2 =the average of the squares of the particle velocities. The square root of u2 is called the root mean square velocity and is symbolized with urms urms= = M= mole of gas particles (kg) R = ; J = kgm2 /s2 3RT Mu2 8.3145 J Kgmol
  • 85. Root Mean Square Velocity Example Calculate the root mean square velocity for the atoms in a sample of helium gas at 25°C. 1.36 x 103 m/s
  • 86. Mean Free Path The average distance a particle travels between collisions in a particular gas sample. 1 x 10-7 m for O2 at STP urms=500 m/s
  • 87. Mean Free Path A velocity distribution that show the effect of temperature on the velocity distribution in a gas.
  • 89. Diffusion Diffusion describes the mixing of gases. The rate of mixing gases, is the same as the rate of diffusion Dependent upon urms
  • 90. Effusion Effusion describes the transfer of gas from one chamber to another (usually through a small hole or porous opening). The rate of transfer is said to be the rate of effusion.
  • 91. Effusion The rate of effusion of a gas is inversely proportional to the square root of the mass of its particles.
  • 92. Effusion Rate of Effusion for gas 1 Rate of Effusion for gas 2 = M2 M1 Temperature must be the same for both gases. M represents the molar masses of the gases. Units can be in g or kg since the units will cancel out. This is called Graham’s law of effusion:
  • 93. Effusion Example Calculate the effusion rates of hydrogen gas (H2) and Uranium hexafluoride (UF6), a gas used in the enrichment process to produce fuel for nuclear reactors. 13.2 : 1
  • 95. Real Gases An ideal gas is a hypothetical concept. No gas exactly follows the ideal gas law, although many gases come very close at low pressures and/or high temperatures.
  • 96. Real Gases Thus ideal gas behavior can best be thought of as the behavior approached by real gases under certain conditions.
  • 97. Real Gases Plots of PV/nRT vs. P for several gases (200K). Ideal behavior only at low pressures.
  • 98. Real Gases Plots of PV/nRT vs. P for N2 at three temperatures. Ideal behavior at higher temperatures.
  • 99. KMT Modifications Johannes van der Walls (1837- 1923), a physics professor at the University of Amsterdam started work in the area of ideal vs real gas behavior. He won the nobel prize in 1910 for his work.
  • 100. KMT Modifications van der Waals modifications to the ideal gas law accounted for the volume of particle space. Therefore adjusting for the volume actually available to a give gas molecule. V-nb n is number of moles b is an empirical constant
  • 101. KMT Modifications van der Waals modifications to the ideal gas law allowed for the attractions that occur among particle in a real gas which is dependent upon the concentration of the particles.  , pressure correction a is proportionality constant. Pobs = Π∋ − α ν ϖ     2
  • 102. van der Waals Equation Insert both corrections and the equation can be written as: Rearranged for van der Waals: Pobs = νΡΤ ς − νβ − α ν ς     2 Pobs + α ν ς     2         ξ ς − νβ( ) = νΡΤ
  • 103. van der Waals Equation a and b values are determined for a given gas by fitting experimental behavior. That is a and b are varied until the best fit of the observed pressure is obtained under all conditions.
  • 104. Characteristics of Real Gases A low value for a reflects weak intermolecular forces among gas molecules.
  • 105. van der Waals Ideal behavior at low pressure (large volume) makes sense because the small amount of volume that the particles consume are not a factor.
  • 106. van der Waals Ideal behavior at high temperatures also makes sense because particles are moving at such a high rate that their interparticle interactions are not very important.
  • 108. Chemistry in the Atmosphere The most important gases to us are those in the atmosphere that surround the earth’s surface. The principal components are N2 and O2, but many other important gases, such as H2O and CO2, are also present.
  • 109.
  • 110. Chemistry in the Atmosphere Because of gravitational effects, the composition of the earth’s atmosphere is not constant; heavier molecules tend to be near the earth’s surface, and light molecules tend to migrate to higher altitudes, with some eventually escaping into space.
  • 111. Chemistry in the Atmosphere The chemistry occurring in the higher levels of the atmosphere is mostly determined by the effects of high- energy radiation and particles from the sun and other sources in space. The upper atmosphere serves as a shield to prevent this radiation from reaching earth.
  • 112. Chemistry in the Atmosphere The troposphere (closest to earth) is strongly influenced by human activities. Millions of tons of gases and particulates are released into the troposphere by our highly industrial civilization.
  • 113. Chemistry in the Atmosphere Severe air pollution is found around many large cities. The two main sources of pollution are transportation and the production of electricity. The combustion of petroleum in vehicles produces CO, CO2, NO, NO2.
  • 114. Chemistry in the Atmosphere The complex chemistry of polluted air appears to center around the nitrogen oxides (NOx). At high temperatures found in the gasoline and diesel engines of cars and trucks, N2 and O2 react to form a small quantity of NO that is emitted into the air with the exhaust gases. NO is immediately oxidized in air to NO2.
  • 115. Reactions in the Atomsphere NO2(g) radiant energy → NO(g) + O(g) O(g) + O2(g) → O3(g) Ozone is very reactive and can react directly with other pollutants, or the ozone can absorb light and break up to form an energetically excited O2 molecule (O2*) and excited O (O*).
  • 116. Reactions in the Atomsphere O* + H2O → 2OH OH + NO2 → HNO3 The end product of this whole process is often referred to as photochemical smog, so called because light is required to initiate some of the reactions.
  • 117. Reactions in the Atomsphere S(coal) + O2(g) → SO2(g) 2SO2(g ) + O2 → 2SO3(g ) SO3(g) + H2O(l) → H2SO4(aq) Sulfuric acid is very corrosive to both living things and building materials. Another result of this type of pollution is called acid rain.