Gases

Pressure

Gas pressure is a measure of the frequency and energy of the molecules of a gas striking a surface.  An increase in either the frequency or energy of collisions results in an increased gas pressure.

The energy of collision depends on the velocity and mass of the molecule.  The collisions are continually occurring between the molecules, it is only against a surface that we measure pressure.

Pressure (P) is a measure of force (F) per unit area (A).

P = F/A

Barometer

A device used to measure atmospheric pressure

The gases of the Atmosphere also exert a pressure on all surfaces. Atmospheric pressure is the result of compression of the atmospheric gases from gravity.  The pressure of the atmosphere will vary with elevation and with the composition of the atmosphere, which changes with storm systems.

Units of Pressure

The Standard Atmospheric Pressure is defined at sea level.

Standard Atmospheric Pressure

Unit

Standard Pressure

atmosphere

1 atm (exact)

millimeters of mercury

760 mm Hg (exact)

torr (1 torr = 1 mm Hg)

760 torr (exact)

Pascal (Pa)

101,325 Pa

kilopascal

101 kPa

Bar

1.01 bar

Pressure = force/area

Pascal = Newton/m2

1 torr = 1 mm Hg

1 bar = 105 Pa

Manometer

A device for measuring pressure. (not necessarily atmospheric pressure)

mm Hg

A unit of pressure based on the height of a column of mercury in a manometer or barometer, equal to the torr.

Finding the height column of different liquids in a manometer or barometer

Density times column height = d * h = (g/cm3) (cm) = (g/cm2) = mass/ area
= (force/area)(constant) = pressure (constant)

With this line above we can see that d*h is directly proportional to pressure, so if we want the height of a second liquid based on the height (pressure) of the first liquid, the equation will be.

d1 * h1 = d2 * h2

Standard Atmosphere

A unit of pressure abbreviated atm.

1 atm = 760 mm Hg = 760 torr = 101,325 Pa = 101.3 kPa = 1.01 bar

The Gas Laws of Boyle, Charles, and Avogadro

Boyle's Law

The volume of a gas is inversely proportional to the pressure at constant temperature.

Boyles Law:

PV = k

Where k is a constant for a given gas at a specified temperature.

V = k/P = k(1/P)   gives a straight line plot of V vs (1/P), with slope = k, and intercept = 0

To use Boyle's law for changes in volume or pressure:

P1V1 = P2V2

Charle's Law

The volume of a gas is directly proportional to the absolute temperature at constant pressure.

Absolute temperature is the Kelvin scale.

Charles Law:

V = bT        where b is a constant and T is in Kelvin

or    V/T = b

To use Charles Law for changes in volume or temperature

V1/T1 = V2/T2

Absolute Zero

Extrapolation of temperature to zero volume for any gas gives the same value of
–273.15°C or 0 Kelvin

Avogadro's Law

Equal volumes of gases at the same temperature and pressure contain the same number of molecules.

Also
Volume is directly proportional to the number of moles at constant temperature and pressure

V = kn             where k is a constant and n is number of moles

V1/n1 = V2/n2

Combined Gas Law

If all the properties of a gas allowed to change except for the number of moles. The combined gas law can be used to calculate the final properties from an initial set of properties.

P1V1/T1 = P2V2/T2

If two of the new conditions are known, the third can be calculated.

 

The Ideal Gas Law

PV = nRT

Ideal gas constant = R

R = 0.08206 atm·L/mol·K

The Ideal gas law is an equation of state, it describes the state of the gas without regards of how it got to that state. Knowledge of three of the four properties is sufficient to describe the state of the gas since the fourth property can be calculated

The ideal gas law is referred to as "ideal" because it is not perfect. Real gases obey the ideal gas law to a good approximation under standard conditions and at low pressures and high temperatures. Deviations from the ideal gas law occur at high pressures and low temperatures.

If three of the properties of a gas are known, the ideal gas law can be used to determine the value of the forth property.

Standard Temperature and Pressure (STP)

0°C (273.15 K) and 1 atm

These conditions are a common reference conditions for gases and is referred to as STP

Molar Volume

One mole of an ideal gas occupies 22.41 L of volume

This is termed the molar volume and is often written 22.41 L/mol

Real gases deviate some from this value.

Laws from the Ideal Gas Law

If one set of conditions is known about a gas, and then two or three properties are allowed to change, with one of the new values being known, then the other property can be calculated.

Pressure-Volume

If pressure and volume vary with moles and temperature held constant, the ideal gas law can become Boyles law. Rearrange the ideal gas equation with all variables on one side and all constants on other side.

P1V1 = P2V2 = nRT = constant

Volume-Temperature

If volume and temperature are allowed to vary with moles and pressure held constant, the ideal gas law becomes equivalent to Charles Law.

V1/T1 = V2/T2 = nR/P = constant

Pressure-Volume-Temperature

If all the properties of a gas allowed to change except for the number of moles. the ideal gas equation takes the form referred to as the combined gas law.

P1V1/T1 = P2V2/T2 = nR = constant

If two of the new conditions are known, the third can be calculated.

Gas Stoichiometry

Molar Mass of a Gas/ Gas Density to Molar Mass

Molar mass of a gas can be calculated from the gas density.

P = nRT/V = mnRT/mV = (n/m)(m/V)RT = dRT/M                  where M is molar mass

PM = dRT        where M is molar mass

Where m/V = d = gas density

and molar mass = M = m/n

alternatively

n = mass/molar mass = m/molar mass

P = [mRT]/[V molar mass]

P = [dRT]/molar mass

molar mass = dRT/P

Dalton's Law of Partial Pressures

A gas in a mixture will exert the same pressure it would if it were the only gas present.  The pressure the gas exerts is not influenced by the presence of other gases.

Dalton's law of partial pressures, The total pressure of a gas mixture is the sum of the individual pressures of each gas in the mixture.

Ptotal = SPi

The pressure each gas exerts in a mixture is termed the partial pressure.

Mole Fraction & Partial Pressures

The ratio of the number of moles of one component of a mixture to the total moles of all components of the mixture.

c1 = n1/nTotal

since n = P(V/RT)

c1 = P1/PTotal

c1 = n1/nTotal = P1/PTotal

This also means that

P1 = c1 (PTotal)

The partial pressure of a component of a gas mixture is the mole fraction times the total pressure.

Gas Collection over Water

Gases can be collected over water to determine volume or quantity generated.  However, this wet gas contains the gas of interest and water vapor.  To determine the quantity of the gas of interest, the vapor pressure of water, at the collection temperature, must be subtracted off of the collection pressure, generally 1 atm.

Ptotal = Pgas + PH2O

The Kinetic Molecular Theory of Gases

This model speculates on the behavior of individual gas molecules to explain the properties of an ideal gas.

·         Gases are made up of very tiny molecule compared to the distance between thems. Gases are mostly empty space. The volume of the gas molecules is negligible. [Real gases have volume]

·         Gas molecules are in constant motion. They move in straight lines and random directions. The collisions of the molecules with the container walls is the source of the gas pressure.

·         Gas molecules exert no force on each other.  Gas molecules are not attracted to nor repel each other. 

·         Gas molecules have elastic collisions. Two molecules can exchange energy when they collide but the sum of their energies does not change from the collision. [One of the main differences between ideal and real gases]

·         The average kinetic energy of gas molecules is proportional to the Kelvin Temperature. At the same temperature, all gas molecules, regardless of type, have the same average kinetic energy.

Pressure and Volume (Boyle's Law)

As volume decreases, the number of collisions between molecules and walls will increase increasing pressure.

Volume and Temperature (Charles' Law)

As temperature increases, the molecules will travel faster and exert more force in collisions with the walls.

Volume and temperature

As temperature increases, the molecules will travel faster and exert more force in collisions with the walls, to keep pressure constant, the volume must decrease reducing the frequency of collisions.

Volume and Number of Moles (Avogadro's Law)

Increasing number of moles will increase frequency of collisions and therefore pressure unless volume is increased to decrease frequency of collisions.

Mixture of Gases (Dalton's Law)

The total pressure is equal to the sum of the individual pressures since the molecules are independent of each other and their volumes are negligible.

(KE)avg = (3/2)RT

Root Mean Square Velocity

The root-mean-square (rms) speed, u, of molecules is the speed of a molecule possessing the average kinetic energy, e, of the gas.

e = (1/2)mu2

The rms speed is different from the most probable speed or the average speed.

This is related to temperature by:

(KE)avg = (3/2)RT

Difference between average speed and rms speed: If we have 4 objects with speeds of 4.0, 6.0, 10.0 and 12.0 m/s, the average speed is (4.0 + 6.0 + 10.0 + 12.0)/4 = 8.0 m/s. The rms speed is Ö(4.02 + 6.02 + 10.02 + 12.02)/4) = 8.6 m/s.

Effusion and Diffusion

The rms speed can be derived from the kinetic molecular theory.

urms = Ö3RT/M)

The rms velocity is inversely proportional to molar mass, M, at constant temperature. Light molecules travel faster than larger molecules.

Using the gas constant in the form of R = 8.3145 J/mol K mol will give urms in terms of m/s, since the joule is defined as J = kg m2/s2, so the units of R are kg m2/(mol K s2). M is the molar mass with units of kg/mole.

The kinetic energy and rms velocity are both averages. The gas molecules are in constant collisions within a short travel distance. This transfers energy with each collisions having molecules constantly increasing and decreasing their energies.

Effusion

Effusion is the process of a gas passing through a hole into a vacuum.

The rate of effusion measures the speed at which the gas is transferred into the evacuated chamber.

The rate of effusion is inversely proportional to the square root of the mass of its particles (or molar mass)

Rate of effusion a 1/ÖM)

Graham's law of Effusion

The ratio of rates of effusion of two gases is equal to the inverse ratio of the square roots of the masses of the gas particles

Rate of effusion(1) = ÖM2)
Rate of effusion(2)   
ÖM1)

Low mass molecules effuse faster than high mass molecules.

Diffusion

Diffusion is the mixing or spread of one gas in another.

This is the mixing of gases by molecular motion.

Gases at room temperature have a velocity close to half a kilometer per second. But they also have collisions on the order of 1010 times per second. The average distance between collisions is called the mean free path of the molecule. The mean free path of air at sea level is about 60 nm.

Real Gases

The ideal gas equation only approximates the behavior of real gases.

Real gases deviate from the ideal gas equation. This deviation increases at high pressures and at low temperatures.

The main differences between real gases and the ideal gas equation and the kinetic molecular theory is that
Real gases occupy volume, and
Real gases have attractive forces between them

The volume of gases requires an adjustment to the volume term of the gas equation

The attractive forces between molecules reduces the pressure the gas exerts, so an adjustment is required to the presser term in the gas equation.

Van der Waals Equation

[P + a(n/V)2][V – nb] = nRT

another way it can be written is:

P = (nRT/[V – nb]) - a(n/V)2

The values of a and b are determined experimentally for each gas. Table 10.3 p. 429.

The two correction factors have opposing effects on the pressure. The volume correction factor increases pressure, while the pressure correction factor (based on attractions between molecules) reduces pressure. At a low pressure, the pressure correction factor dominates, reducing the observed pressure below that predicted by the ideal gas law. At high pressures, the volume term dominated creating a higher pressure than predicted by the ideal gas law.  Low temperature magnifies the effect of both terms.

Gas Equations

Boyles Law

P1V1 = P2V2

Charles Law

V1/T1 = V2/T2

Avogadro's Law

V1/n1 = V2/n2

Combined Gas Law

P1V1/T1 = P2V2/T2

Ideal Gas Law

PV = nRT

Dalton's Law of Partial Pressure

Ptotal = SPi

P1 = c1 (PTotal)

Mole Freaction

c1 = n1/nTotal

Gas law arranged with density and molar mass

PM = dRT        where M is molar mass

Energy/Temperature of a gas

(KE)avg = (3/2)RT

Root mean Square velocity

e = (1/2)mu2

urms = Ö3RT/M)

Grahams Law of Effusion

Rate of effusion(1) = ÖM2)
Rate of effusion(2)    ÖM1)

Van der Waals Equation

[P + a(n/V)2][V – nb] = nRT

or

P = (nRT/[V – nb]) - a(n/V)2

Constants

Ideal Gas Constant

R = 0.08206 atm·L/mol·K