The document discusses gases and gas laws. It provides an overview of the composition and importance of Earth's atmosphere. Key topics covered include gas pressure, how it is measured using devices like the barometer, and how pressure varies with weather and altitude. The document then explains Boyle's, Charles', and Avogadro's laws regarding the behavior of gases. It introduces the ideal gas law and provides examples of using it to solve gas problems involving changes in pressure, volume, temperature, and moles of gas. It also covers gas stoichiometry, partial pressures of gases in mixtures, and the kinetic molecular theory of gases.
The Roman Empire A Historical Colossus.pdfkaushalkr1407
The Roman Empire, a vast and enduring power, stands as one of history's most remarkable civilizations, leaving an indelible imprint on the world. It emerged from the Roman Republic, transitioning into an imperial powerhouse under the leadership of Augustus Caesar in 27 BCE. This transformation marked the beginning of an era defined by unprecedented territorial expansion, architectural marvels, and profound cultural influence.
The empire's roots lie in the city of Rome, founded, according to legend, by Romulus in 753 BCE. Over centuries, Rome evolved from a small settlement to a formidable republic, characterized by a complex political system with elected officials and checks on power. However, internal strife, class conflicts, and military ambitions paved the way for the end of the Republic. Julius Caesar’s dictatorship and subsequent assassination in 44 BCE created a power vacuum, leading to a civil war. Octavian, later Augustus, emerged victorious, heralding the Roman Empire’s birth.
Under Augustus, the empire experienced the Pax Romana, a 200-year period of relative peace and stability. Augustus reformed the military, established efficient administrative systems, and initiated grand construction projects. The empire's borders expanded, encompassing territories from Britain to Egypt and from Spain to the Euphrates. Roman legions, renowned for their discipline and engineering prowess, secured and maintained these vast territories, building roads, fortifications, and cities that facilitated control and integration.
The Roman Empire’s society was hierarchical, with a rigid class system. At the top were the patricians, wealthy elites who held significant political power. Below them were the plebeians, free citizens with limited political influence, and the vast numbers of slaves who formed the backbone of the economy. The family unit was central, governed by the paterfamilias, the male head who held absolute authority.
Culturally, the Romans were eclectic, absorbing and adapting elements from the civilizations they encountered, particularly the Greeks. Roman art, literature, and philosophy reflected this synthesis, creating a rich cultural tapestry. Latin, the Roman language, became the lingua franca of the Western world, influencing numerous modern languages.
Roman architecture and engineering achievements were monumental. They perfected the arch, vault, and dome, constructing enduring structures like the Colosseum, Pantheon, and aqueducts. These engineering marvels not only showcased Roman ingenuity but also served practical purposes, from public entertainment to water supply.
Ethnobotany and Ethnopharmacology:
Ethnobotany in herbal drug evaluation,
Impact of Ethnobotany in traditional medicine,
New development in herbals,
Bio-prospecting tools for drug discovery,
Role of Ethnopharmacology in drug evaluation,
Reverse Pharmacology.
The Indian economy is classified into different sectors to simplify the analysis and understanding of economic activities. For Class 10, it's essential to grasp the sectors of the Indian economy, understand their characteristics, and recognize their importance. This guide will provide detailed notes on the Sectors of the Indian Economy Class 10, using specific long-tail keywords to enhance comprehension.
For more information, visit-www.vavaclasses.com
We all have good and bad thoughts from time to time and situation to situation. We are bombarded daily with spiraling thoughts(both negative and positive) creating all-consuming feel , making us difficult to manage with associated suffering. Good thoughts are like our Mob Signal (Positive thought) amidst noise(negative thought) in the atmosphere. Negative thoughts like noise outweigh positive thoughts. These thoughts often create unwanted confusion, trouble, stress and frustration in our mind as well as chaos in our physical world. Negative thoughts are also known as “distorted thinking”.
The French Revolution, which began in 1789, was a period of radical social and political upheaval in France. It marked the decline of absolute monarchies, the rise of secular and democratic republics, and the eventual rise of Napoleon Bonaparte. This revolutionary period is crucial in understanding the transition from feudalism to modernity in Europe.
For more information, visit-www.vavaclasses.com
2024.06.01 Introducing a competency framework for languag learning materials ...Sandy Millin
http://sandymillin.wordpress.com/iateflwebinar2024
Published classroom materials form the basis of syllabuses, drive teacher professional development, and have a potentially huge influence on learners, teachers and education systems. All teachers also create their own materials, whether a few sentences on a blackboard, a highly-structured fully-realised online course, or anything in between. Despite this, the knowledge and skills needed to create effective language learning materials are rarely part of teacher training, and are mostly learnt by trial and error.
Knowledge and skills frameworks, generally called competency frameworks, for ELT teachers, trainers and managers have existed for a few years now. However, until I created one for my MA dissertation, there wasn’t one drawing together what we need to know and do to be able to effectively produce language learning materials.
This webinar will introduce you to my framework, highlighting the key competencies I identified from my research. It will also show how anybody involved in language teaching (any language, not just English!), teacher training, managing schools or developing language learning materials can benefit from using the framework.
How to Split Bills in the Odoo 17 POS ModuleCeline George
Bills have a main role in point of sale procedure. It will help to track sales, handling payments and giving receipts to customers. Bill splitting also has an important role in POS. For example, If some friends come together for dinner and if they want to divide the bill then it is possible by POS bill splitting. This slide will show how to split bills in odoo 17 POS.
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 Latm/Kmol
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
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.
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 = kgm2
/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.
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.
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.