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GASES<br />

• Gases are one of the most pervasive<br />

aspects of our environment on the<br />

Earth. We continually exist with<br />

constant exposure to gases of all<br />

forms.<br />

• The steam formed in the air during a<br />

hot shower is a gas.<br />

• The Helium used to fill a birthday<br />

balloon is a gas.<br />

• The oxygen in the air is an essential<br />

gas for life. www.elearnuganda.net


GASES<br />

A windy day or a still day is a result of the difference in pressure of gases<br />

in two different locations. A fresh breeze on a mountain peak is a study in<br />

basic gas laws.<br />

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Important Characteristics of Gases<br />

1) Gases are highly compressible<br />

An external force compresses the gas sample and decreases its<br />

volume, removing the external force allows the gas volume to<br />

increase.<br />

2) Gases are thermally expandable<br />

When a gas sample is heated, its volume increases, and when it is<br />

cooled its volume decreases.<br />

3) Gases have high viscosity<br />

Gases flow much easier than liquids or solids.<br />

4) Most Gases have low densities<br />

Gas densities are on the order of grams per liter whereas liquids<br />

and solids are grams per cubic cm, 1000 times greater.<br />

5) Gases are infinitely miscible<br />

Gases mix in any proportion such as in air, a mixture of many gases.<br />

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Substances That Are Gases under<br />

Normal Conditions<br />

Substance Formula MM(g/mol)<br />

• Helium He 4.0<br />

• Neon Ne 20.2<br />

• Argon Ar 39.9<br />

• Hydrogen H 2 2.0<br />

• Nitrogen N 2 28.0<br />

• Nitrogen Monoxide NO 30.0<br />

• Oxygen O 2 32.0<br />

• Hydrogen Chloride HCl 36.5<br />

• Ozone O 3 48.0<br />

• Ammonia NH 3 17.0<br />

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• Methane CH 4 16.0


Kinetic Molecular Theory<br />

• To fully understand the world around us<br />

requires that we have a good understanding<br />

of the behavior of gases. The description of<br />

gases and their behavior can be approached<br />

from several perspectives.<br />

• The Gas Laws are a mathematical<br />

interpretation of the behavior of gases.<br />

• However, before understanding the<br />

mathematics of gases, a chemist must have<br />

an understanding of the conceptual<br />

description of gases. That is the purpose of<br />

the Kinetic Molecular Theory.<br />

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Kinetic Molecular Theory<br />

• The Kinetic Molecular Theory is a single set of<br />

descriptive characteristics of a substance known as<br />

the Ideal Gas.<br />

• All real gases require their own unique sets of<br />

descriptive characteristics. Considering the large<br />

number of known gases in the World, the task of<br />

trying to describe each one of them individually<br />

would be an awesome task.<br />

• In order to simplify this task, the scientific<br />

community has decided to create an imaginary gas<br />

that approximates the behavior of all real gases. In<br />

other words, the Ideal Gas is a substance that does<br />

not exist.<br />

• The Kinetic Molecular Theory describes that gas.<br />

While the use of the Ideal Gas in describing all real<br />

gases means that the descriptions of all real gases<br />

will be wrong, the reality is that the descriptions of<br />

real gases will be close enough to correct that any<br />

errors can be overlooked.<br />

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The Nature of Gases<br />

Three basic assumptions of the kinetic<br />

theory as it applies to gases:<br />

1. Gas is composed of particles- usually<br />

molecules or atoms<br />

–Small, hard spheres<br />

–Insignificant volume; relatively far<br />

apart from each other<br />

–No attraction or repulsion between<br />

particles<br />

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The Nature of Gases<br />

2. Particles in a gas move rapidly in<br />

constant random motion<br />

–Move in straight paths, changing<br />

direction only when colliding with one<br />

another or other objects<br />

–Average speed of O 2 in air at 20 o C is<br />

an amazing 1660 km/h!<br />

(1.6km=1mile)<br />

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The Nature of Gases<br />

3. Collisions are perfectly elasticmeaning<br />

kinetic energy is transferred<br />

without loss from one particle to<br />

another- the total kinetic energy remains<br />

constant<br />

Newtonian Cradle-<br />

Where the collisions between the balls elastic?<br />

Yes, because kinetic energy was transferred<br />

with each collision<br />

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• Why did the balls eventually stop<br />

swinging? The collisions were not<br />

perfectly elastic, some kinetic energy<br />

was lost as heat during each collision.<br />

• At constant temperatures and low to<br />

moderate pressures, collisions between<br />

gas particles are perfectly elastic<br />

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THE KINETIC THEORY OF GASES<br />

Remember the assumptions<br />

• Gas consists of large number of particles<br />

(atoms or molecules)<br />

• Particles make elastic collisions with each<br />

other and with walls of container<br />

• There exist no external forces (density<br />

constant)<br />

• Particles, on average, separated by distances<br />

large compared to their diameters<br />

• No forces between particles except when<br />

they collide<br />

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What happens to a ball when it<br />

drops?<br />

The Which potential is is converted energy into<br />

of to the the potential potential ball energy energy of<br />

in the the ball…………..<br />

…..but in reality the ball<br />

loses height and<br />

eventually stops bouncing<br />

Which Is converted is converted to kinetic to<br />

kinetic energy energy in the ball in the<br />

ball<br />

Why does this<br />

happen?<br />

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How does the bouncing ball lose<br />

energy?<br />

• Through friction with the air (air<br />

resistance)<br />

• Through sound when it hits the floor<br />

• Through deformation of the ball<br />

• Through heat energy in the bounce<br />

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IDEAL GAS MODEL<br />

• The gas consists of objects with a defined mass<br />

and zero volume.<br />

• The gas particles travel randomly in straight-line<br />

motion where their movement can be described by<br />

the fundamental laws of mechanics.<br />

• All collisions involving gas particles are elastic;<br />

the kinetic energy of the system is conserved even<br />

though the kinetic energy among the particles is<br />

redistributed.<br />

• The gas particles do not interact with each other or<br />

the with the walls of any container.<br />

• The gas phase system will have an average kinetic<br />

energy that is proportional to temperature; the<br />

kinetic energy will be distributed among the<br />

particles according to a Boltzmann type of<br />

distribution.<br />

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Boltzman Distribution. The behaviour of<br />

the gas molecules under the action of<br />

gravity.<br />

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Maxwell Distribution. Experiment with<br />

Galton board demonstrates the<br />

statistical sense of Maxwell distribution.<br />

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Ideal Gas Model<br />

Kinetic Molecular Theory (KMT) for an ideal<br />

gas states that all gas particles:<br />

• are in random, constant, straight-line motion.<br />

• are separated by great distances relative to<br />

their size; the volume of the gas particles is<br />

considered negligible.<br />

• have no attractive forces between them.<br />

• have collisions that may result in the transfer<br />

of energy between gas particles, but the total<br />

energy of the system remains constant.<br />

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Brownian motion. Chaotic motion of<br />

minute particle suspended in a gas or<br />

liquid<br />

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This animation illustrates the concept of<br />

free path length of molecules in a gas.<br />

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Ideal vs. Non-Ideal Gases<br />

x<br />

x<br />

• Kinetic Theory Assumptions<br />

– Point Mass<br />

– No Forces Between Molecules<br />

– Molecules Exert Pressure Via Elastic<br />

Collisions With Walls<br />

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(courtesy F. Remer)


Ideal vs. Non-Ideal Gases<br />

• Non-Ideal Gas<br />

– Violates Assumptions<br />

• Volume of molecules<br />

• Attractive forces of molecules<br />

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(courtesy F. Remer)


Deviations from ideal behaviour<br />

• A real gas is most like an ideal gas when the<br />

real gas is at low pressure and high<br />

temperature.<br />

• At high pressures gas particles are close<br />

therefore the volume of the gas particles is<br />

considered.<br />

• At low temperatures gas particles have low<br />

kinetic energy therefore particles have some<br />

attractive force<br />

• Example<br />

• Dry ice, liquid oxygen and nitrogen<br />

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Ideal Gases<br />

• Behave as described by the ideal gas<br />

equation; no real gas is actually ideal<br />

• Within a few %, ideal gas equation describes<br />

most real gases at room temperature and<br />

pressures of 1 atm or less<br />

• In real gases, particles attract each other<br />

reducing the pressure<br />

• Real gases behave more like ideal gases as<br />

pressure approaches www.elearnuganda.net zero.


Atmospheric Pressure<br />

• Weight of column of air above your head.<br />

• We can measure the density of the<br />

atmosphere by measuring the pressure it<br />

exerts.<br />

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Effect of Atmospheric Pressure on<br />

Objects at the Earth’s Surface<br />

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Atmospheric Pressure<br />

Pressure = Force per Unit Area<br />

Atmospheric Pressure is the weight of<br />

the column of air above a unit area. For<br />

example, the atmospheric pressure felt<br />

by a man is the weight of the column of<br />

air above his body divided by the area<br />

the air is resting on<br />

P = (Weight of column)/(Area of base)<br />

Standard Atmospheric Pressure:<br />

1 atmosphere (atm)<br />

14.7 lbs/in 2 (psi)<br />

760 Torr (mm Hg)<br />

1013.25 KiloPascals or Millibars (kPa =<br />

N/m 2 )<br />

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Pressure Measurement<br />

Torricelli's Barometer<br />

• Torricelli determined from this<br />

experiment that the pressure of the<br />

atmosphere is approximately 30<br />

inches or 76 centimeters (one<br />

centimeter of mercury is equal to 13.3<br />

millibars. He also noticed that height<br />

of the mercury varied with changes in<br />

outside weather conditions.<br />

For climatological and meteorological purposes, standard sea-level pressure<br />

is said to be 76.0 cm or 29.92 inches or 1013 millibars<br />

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The Nature of Gases<br />

Atmospheric pressure results from<br />

the collisions of air molecules with<br />

objects<br />

–Decreases as you climb a mountain<br />

because the air layer thins out as<br />

elevation increases<br />

Barometer is the measuring<br />

instrument for atmospheric<br />

pressure; dependent<br />

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weather


Common Units of Pressure<br />

Unit Atmospheric Pressure Scientific Field<br />

pascal (Pa); 1.01325 x 10 5 Pa SI unit; physics,<br />

kilopascal(kPa) 101.325 kPa chemistry<br />

atmosphere (atm) 1 atm* Chemistry<br />

millimeters of mercury 760 mmHg* Chemistry, medicine,<br />

( mm Hg ) biology<br />

torr 760 torr* Chemistry<br />

pounds per square inch 14.7 lb/in 2 Engineering<br />

( psi or lb/in 2 )<br />

bar 1.01325 bar<br />

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Meteorology,<br />

chemistry, physics


Converting Units of Pressure<br />

Problem: A chemist collects a sample of carbon dioxide from the<br />

decomposition of limestone (CaCO 3 ) in a closed end manometer, the<br />

height of the mercury is 341.6 mm Hg. Calculate the CO 2 pressure in<br />

torr, atmospheres, and kilopascals.<br />

Plan: The pressure is in mmHg, so we use the conversion factors from<br />

Table 5.2(p.178) to find the pressure in the other units.<br />

Solution:<br />

converting from mmHg to torr:<br />

P CO2 (torr) = 341.6 mm Hg x<br />

1 torr<br />

= 341.6 torr<br />

1 mm Hg<br />

converting from torr to atm:<br />

1 atm<br />

P CO2 ( atm) = 341.6 torr x = 0.4495 atm<br />

760 torr<br />

converting from atm to kPa:<br />

P CO2 (kPa) = 0.4495 atm x<br />

101.325 kPa<br />

1 atm<br />

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= 45.54 kPa


Change in Pressure<br />

Change in average<br />

atmospheric pressure with<br />

altitude.<br />

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The Nature of Gases<br />

Gas Pressure – defined as the<br />

force exerted by a gas per unit<br />

surface area of an object<br />

–Due to: a) force of collisions, and b)<br />

number of collisions<br />

–No particles present? Then there<br />

cannot be any collisions, and thus no<br />

pressure – called a vacuum<br />

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Manometers<br />

Manometers measure a pressure difference by balancing the<br />

weight of a fluid column between the two pressures of interest<br />

Rules of thumb:<br />

• When evaluating, start from the known<br />

pressure end and work towards the<br />

unknown end<br />

• At equal elevations, pressure is<br />

constant in the SAME fluid<br />

• When moving down a manometer,<br />

pressure increases<br />

• When moving up a manometer,<br />

pressure decreases<br />

• Only include atmospheric pressure on<br />

open ends<br />

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Manometers<br />

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Manometers<br />

Example 2<br />

Find the pressure at<br />

point A in this open u-<br />

tube manometer with an<br />

atmospheric pressure P o<br />

P D = γ H2O x h E-D + P o<br />

P c = P D<br />

P B = P C - γ Hg x h C-B<br />

P A = P B<br />

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P = γ x h + P O


The Gas Laws<br />

• What would Polly<br />

Parcel look like if she<br />

had no gas molecules<br />

inside?<br />

zero molecules = zero pressure inside<br />

zero pressure inside = zero force on the<br />

inside<br />

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Gas Law Variables<br />

• In order to describe gases, mathematically, it<br />

is essential to be familiar with the variables<br />

that are used. There are four commonly<br />

accepted gas law variables<br />

• Temperature<br />

• Pressure<br />

• Volume<br />

• Moles<br />

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Temperature<br />

• The temperature variable is always symbolized as T.<br />

• It is critical to remember that all temperature values<br />

used for describing gases must be in terms of<br />

absolute kinetic energy content for the system.<br />

• Consequently, T values must be converted to the<br />

Kelvin Scale. To do so when having temperatures<br />

given in the Celsius Scale remember the conversion<br />

factor<br />

• Kelvin = Celsius + 273<br />

• According to the Kinetic Molecular Theory, every<br />

particle in a gas phase system can have its own<br />

kinetic energy. Therefore, when measuring the<br />

temperature of the system, the average kinetic<br />

energy of all the particles in the system is used.<br />

• The temperature variable is representing the position<br />

of the average kinetic energy as expressed on the<br />

Boltzmann Distribution.<br />

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Pressure<br />

• The pressure variable is represented by the<br />

symbol P.<br />

• The pressure variable refers to the pressure<br />

that the gas phase system produces on the<br />

walls of the container that it occupies.<br />

• If the gas is not in a container, then the<br />

pressure variable refers to the pressure it<br />

could produce on the walls of a container if it<br />

were in one.<br />

• The phenomenon of pressure is really a force<br />

applied over a surface area. It can best be<br />

expressed by the equation<br />

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Pressure<br />

• Consider the Pressure equation and the impact of<br />

variables on it.<br />

• The force that is exerted is dependent upon the<br />

kinetic energy of the particles in the system. If the<br />

kinetic energy of the particles increases, for<br />

example, then the force of the collisions with a given<br />

surface area will increase. This would cause the<br />

pressure to increase. Since the kinetic energy of the<br />

particles is increased by raising the temperature,<br />

then an increase in temperature will cause an<br />

increase in pressure.<br />

• If the walls of the container were reduced in total<br />

surface area, there would be a change in the<br />

pressure of the system. By allowing a given quantity<br />

of gas to occupy a container with a smaller surface<br />

area, the pressure of the system would increase.<br />

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Pressure<br />

• As this container of gas<br />

is heated, the<br />

temperature increases.<br />

As a result, the average<br />

kinetic energy of the<br />

particles in the system<br />

increases.<br />

• With the increase in<br />

kinetic energy, the force<br />

on the available amount<br />

of surface area increases.<br />

As a result, the pressure<br />

of the system increases.<br />

• Eventually,.........................<br />

.Ka-Boom<br />

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Volume<br />

• The Volume variable is represented by the symbol V.<br />

It seems like this variable should either be very easy<br />

to work with or nonexistent.<br />

• Remember, according to the Kinetic Molecular<br />

Theory, the volume of the gas particles is set at zero.<br />

Therefore, the volume term V seems like it should be<br />

zero.<br />

• In this case, that is not true. The volume being<br />

referred to here is the volume of the container, not<br />

the volume of the gas particles.<br />

• The actual variable used to describe a gas should be<br />

the amount of volume available for the particles to<br />

move around in. In other words<br />

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Volume<br />

• Since the Kinetic Molecular Theory<br />

states that the volume of the gas<br />

particles is zero, then the equation<br />

simplifies.<br />

• As a result, the amount of available<br />

space for the gas particles to move<br />

around in is approximately equal to the<br />

size of the container.<br />

• Thus, as stated before, the variable V is<br />

the volume of the container.<br />

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Moles<br />

• The final gas law variable is the quantity of gas. This is always<br />

expressed in terms of moles. The symbol that represents the<br />

moles of gas is n. Notice that, unlike the other variables, it is in<br />

lower case.<br />

• Under most circumstances in chemistry, the quantity of a<br />

substance is usually expressed in grams or some other unit of<br />

mass. The mass units will not work in gas law mathematics.<br />

Experience has shown that the number of objects in a system<br />

is more descriptive than the mass of the objects.<br />

• Since each different gas will have its own unique mass for the<br />

gas particles, this would create major difficulties when working<br />

with gas law mathematics.<br />

• The whole concept of the Ideal Gas says that all gases can be<br />

approximated has being the same. Considering the large<br />

difference in mass of the many different gases available, using<br />

mass as a measurement of quantity would cause major errors<br />

in the Kinetic Molecular Theory.<br />

• Therefore, the mole will standardize the mathematics for all<br />

gases and minimize the chances for errors.<br />

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Conclusions<br />

There are four variables used mathematically for describing a<br />

gas phase system. While the units used for the variables may<br />

differ from problem to problem, the conceptual aspects of the<br />

variables remain unchanged.<br />

1. T, or Temperature, is a measure of the average kinetic energy of<br />

the particles in the system and MUST be expressed in the<br />

Kelvin Scale.<br />

2. P, or Pressure, is the measure of the amount of force per unit of<br />

surface area. If the gas is not in a container, then P represents<br />

the pressure it could exert if it were in a container.<br />

3. V, or Volume, is a measure of the volume of the container that<br />

the gas could occupy. It represents the amount of space<br />

available for the gas particles to move around in.<br />

4. n, or Moles, is the measure of the quantity of gas. This<br />

expresses the number of objects in the system and does not<br />

directly indicate their masses.<br />

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Gas Laws<br />

• (1) When temperature is held constant, the density of a<br />

gas is proportional to pressure, and volume is inversely<br />

proportional to pressure. Accordingly, an increase in<br />

pressure will cause an increase in density of the gas and<br />

a decrease in its volume. – Boyles’s Law<br />

• (2) If volume is kept constant, the pressure of a unit<br />

mass of gas is proportional to temperature. If<br />

temperature increase so will pressure, assuming no<br />

change in the volume of the gas.<br />

• (3) Holding pressure constant, causes the temperature of<br />

a gas to be proportional to volume, and inversely<br />

proportional to density. Thus, increasing temperature of<br />

a unit mass of gas causes its volume to expand and its<br />

density to decrease as long as there is no change in<br />

pressure. - Charles’s Law<br />

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Boyle’s Law<br />

• Hyperbolic Relation Between Pressure and<br />

Volume<br />

T 1 T 2 T 3 T 3 >T 2 >T 1<br />

(courtesy F. Remer)<br />

p<br />

isotherms<br />

V<br />

p – V Diagram<br />

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Charles’ Law<br />

• Linear Relation Between Temperature and<br />

Pressure<br />

V 1


Charles’ Law<br />

Real data must be<br />

obtained above<br />

liquefaction<br />

temperature.<br />

Experimental curves for<br />

different gasses,<br />

different masses,<br />

different pressures all<br />

extrapolate to a<br />

common zero.<br />

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Another version of Charles Law<br />

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Compression and expansion of<br />

adiabatically isolated gas is accompanied<br />

by its heating and cooling.<br />

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The Gas Laws<br />

• What would Polly<br />

Parcel look like if she<br />

had a temperature of<br />

absolute zero inside?<br />

absolute zero = no molecular motion<br />

no molecular motion = zero force on<br />

the inside<br />

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Ideal Gas Law<br />

The equality for the four variables involved<br />

in Boyle’s Law, Charles’ Law, Gay-Lussac’s<br />

Law and Avogadro’s law can be written<br />

PV = nRT<br />

R = ideal gas constant<br />

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PV = nRT<br />

R is known as the universal gas constant<br />

Using STP conditions<br />

P V<br />

R = PV = (1.00 atm)(22.4 L)<br />

nT (1mol) (273K)<br />

n<br />

T<br />

= 0.0821 L-atm<br />

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Learning Check<br />

What is the value of R when the STP value<br />

for P is 760 mmHg?<br />

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Solution<br />

What is the value of R when the STP value<br />

for P is 760 mmHg?<br />

R = PV = (760 mm Hg) (22.4 L)<br />

nT (1mol) (273K)<br />

= 62.4 L-mm Hg<br />

mol-K<br />

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Learning Check<br />

Dinitrogen monoxide (N 2 O), laughing gas,<br />

is used by dentists as an anesthetic. If 2.86<br />

mol of gas occupies a 20.0 L tank at 23°C,<br />

what is the pressure (mmHg) in the tank in<br />

the dentist office?<br />

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Solution<br />

Set up data for 3 of the 4 gas variables<br />

Adjust to match the units of R<br />

V = 20.0 L<br />

T = 23°C + 273<br />

n = 2.86 mol<br />

20.0 L<br />

296 K<br />

2.86 mol<br />

P = ? ?<br />

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Rearrange ideal gas law for unknown P<br />

P = nRT<br />

V<br />

Substitute values of n, R, T and V and<br />

solve for P<br />

P = (2.86 mol)(62.4L-mmHg)(296 K)<br />

(20.0 L) (K-mol)<br />

= 2.64 x 10 3 mm Hg<br />

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Learning Check<br />

A 5.0 L cylinder contains oxygen gas<br />

at 20.0°C and 735 mm Hg. How many<br />

grams of oxygen are in the cylinder?<br />

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Solution<br />

Solve ideal gas equation for n (moles)<br />

n = PV<br />

RT<br />

= (735 mmHg)(5.0 L)(mol K)<br />

(62.4 mmHg L)(293 K)<br />

= 0. 20 mol O 2 x 32.0 g O 2 = 6.4 g O 2<br />

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1 mol O 2


Molar Mass of a gas<br />

What is the molar mass of a gas if 0.250 g of<br />

the gas occupy 215 mL at 0.813 atm and<br />

30.0°C?<br />

n = PV = (0.813 atm) (0.215 L) = 0.00703 mol<br />

RT<br />

(0.0821 L-atm/molK) (303K)<br />

Molar mass = g = 0.250 g = 35.6 g/mol<br />

mol<br />

0.00703 mol<br />

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Density of a Gas<br />

Calculate the density in g/L of O 2 gas at STP.<br />

From STP, we know the P and T.<br />

P = 1.00 atm<br />

T = 273 K<br />

Rearrange the ideal gas equation for moles/L<br />

PV = nRT PV = nRT P = n<br />

RTV RTV RT V<br />

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Substitute<br />

(1.00 atm ) mol-K = 0.0446 mol O 2 /L<br />

(0.0821 L-atm) (273 K)<br />

Change moles/L to g/L<br />

0.0446 mol O 2 x 32.0 g O 2 = 1.43 g/L<br />

1 L 1 mol O 2<br />

Therefore the density of O 2 gas at STP is<br />

1.43 grams per liter<br />

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Formulas of Gases<br />

A gas has a % composition by mass of<br />

85.7% carbon and 14.3% hydrogen. At<br />

STP the density of the gas is 2.50 g/L.<br />

What is the molecular formula of the<br />

gas?<br />

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Formulas of Gases<br />

Calculate Empirical formula<br />

85.7 g C x 1 mol C = 7.14 mol C/7.14 = 1 C<br />

12.0 g C<br />

14.3 g H x 1 mol H = 14.3 mol H/ 7.14 = 2 H<br />

1.0 g H<br />

Empirical formula = CH 2<br />

EF mass = 12.0 + 2(1.0) = 14.0 g/EF<br />

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Using STP and density ( 1 L = 2.50 g)<br />

2.50 g x 22.4 L = 56.0 g/mol<br />

1 L 1 mol<br />

n = EF/ mol = 56.0 g/mol = 4<br />

14.0 g/EF<br />

molecular formula<br />

CH 2 x 4 = C 4 H 8<br />

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Gases in Chemical Equations<br />

On December 1, 1783, Charles used 1.00 x 10 3<br />

lb of iron filings to make the first ascent in a<br />

balloon filled with hydrogen<br />

Fe(s) + H 2 SO 4 (aq) FeSO 4 (aq) + H 2 (g)<br />

At STP, how many liters of hydrogen<br />

gas were generated?<br />

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Solution<br />

lb Fe g Fe mol Fe mol H 2 L H 2<br />

1.00 x 10 3 lb x 453.6 g x 1 mol Fe x 1 mol H 2<br />

1 lb 55.9 g 1 mol Fe<br />

x 22.4 L H 2 = 1.82 x 10 5 L H 2<br />

1 mol H 2<br />

Charles generated 182,000 L of hydrogen to fill his<br />

air balloon.<br />

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Learning Check<br />

How many L of O 2 are need to react 28.0 g<br />

NH 3 at 24°C and 0.950 atm?<br />

4 NH 3 (g) + 5 O 2 (g) 4 NO(g) + 6 H 2 O(g)<br />

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Solution<br />

Find mole of O 2<br />

28.0 g NH 3 x 1 mol NH 3 x 5 mol O 2<br />

17.0 g NH 3 4 mol NH 3<br />

= 2.06 mol O 2<br />

V = nRT = (2.06 mol)(0.0821)(297K) = 52.9 L<br />

P<br />

0.950 atm<br />

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Mixture of gases<br />

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Reacting mixture of gases<br />

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Learning Check<br />

A.If the atmospheric pressure today is 745<br />

mm Hg, what is the partial pressure (mm<br />

Hg) of O 2 in the air?<br />

1) 35.6 2) 156 3) 760<br />

B. At an atmospheric pressure of 714, what is<br />

the partial pressure (mm Hg) N 2 in the air?<br />

1) 557 2) 9.14 3) 0.109<br />

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Solution<br />

A.If the atmospheric pressure today is 745<br />

mm Hg, what is the partial pressure (mm<br />

Hg) of O 2 in the air?<br />

2) 156<br />

B. At an atmospheric pressure of 714, what is<br />

the partial pressure (mm Hg) N 2 in the air?<br />

1) 557<br />

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Partial Pressure<br />

Partial Pressure<br />

Pressure each gas in a mixture would exert<br />

if it were the only gas in the container<br />

Dalton's Law of Partial Pressures<br />

The total pressure exerted by a gas mixture<br />

is the sum of the partial pressures of the<br />

gases in that mixture.<br />

P T = P 1 + P 2 + P 3 + .....<br />

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Partial Pressures<br />

The total pressure of a gas mixture depends<br />

on the total number of gas particles, not on<br />

the types of particles.<br />

STP<br />

P = 1.00 atm<br />

P = 1.00 atm<br />

1.0 mol He<br />

0.50 mol O 2<br />

+ 0.20 mol He<br />

+ 0.30 mol N 2<br />

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Health Note<br />

When a scuba diver is several hundred feet<br />

under water, the high pressures cause N 2 from<br />

the tank air to dissolve in the blood. If the<br />

diver rises too fast, the dissolved N 2 will form<br />

bubbles in the blood, a dangerous and painful<br />

condition called "the bends". Helium, which is<br />

inert, less dense, and does not dissolve in the<br />

blood, is mixed with O 2 in scuba tanks used for<br />

deep descents. www.elearnuganda.net


Learning Check<br />

A 5.00 L scuba tank contains 1.05 mole of<br />

O 2 and 0.418 mole He at 25°C. What is the<br />

partial pressure of each gas, and what is<br />

the total pressure in the tank?<br />

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Solution G20<br />

P = nRT P T = P O + P He<br />

V<br />

2<br />

P T = 1.47 mol x 0.0821 L-atm x 298 K<br />

= 7.19 atm<br />

5.00 L (K mol)<br />

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Micro Effusion<br />

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Macro Effusion<br />

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