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Gases and gas laws

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Title: Gases and gas laws


1
Gases and gas laws
  • Chapter 12

2
Key concepts
  1. Understand basic characteristics of gases.
  2. Know the definition of pressure and measurement
    units commonly used with pressure
  3. Know what a barometer measures.
  4. Know the relationships described by Boyles Law,
    Charles Law, and Avogadros Law.
  5. Know the ideal gas equation and its derivation.
  6. Understand gas density and using molar masses in
    the ideal gas equation.
  7. Understand Daltons law of partial pressures and
    its applications.
  8. Know the basic principles of the kinetic theory
    of gases and how this explains gas behavior
    described by the ideal gas laws.
  9. Know the terms effusion and diffusion know
    Grahams law of effusion.
  10. Understand gas interactions that cause deviations
    from ideal gas law behavior.

3
Common characteristics of gases (uniquely
different from liquids or solids)
  • All gas mixtures are homogeneous mixtures.
  • Gases expand to fill the container they occupy
  • the volume of EACH GAS in a mixture of gases in a
    container volume of the container.
  • The actual space occupied by the gas molecules is
    small relative to the total volume.

4
Pressure
  • Force applied per unit area
  • P F/A
  • The same force may result in much different
    pressures

5
Pressure units
  • pounds per square inch (psi)
  • inches of mercury (in Hg)
  • mm Hg
  • Pascals (SI units)
  • torr (from Torricelli, inventor of the barometer)
  • 1 torr 1 mm Hg
  • standard atmospheric pressure
  • 760 torr 1 atmosphere (atm) typical pressure
    at sea level.
  • conversions
  • 1 atm 760 torr 1.01325 ? 105 Pa 14.7 psi

6
The barometer
  • Mercury barometer
  • atmospheric pressure ? force applied on Hg ?
    the change in height of mercury column.

http//www.usatoday.com/weather/wbaromtr.htm
7
Basic Gas Laws
  • Relationships between gas pressure, temperature,
    volume, and amount (moles).
  • Now, lets have some fun.

8
Boyles Law
  • Boyles law relates to changes in pressure and
    volume.
  • At constant temperature, the change in pressure
    is ________ proportional to the change in volume.

9
Charles Law
  • Charles Law relates changes in volume and
    temperature
  • At constant pressure, the change in volume is
    _______ proportional to the change in temperature

10
Avogadros Law
  • Identical volumes of a gas at the same
    temperature and pressure have the same number of
    gas particles.

11
Summary
  • P ? 1/V (constant n and T) (Boyle)
  • V ? T (constant n and P) (Charles)
  • V ? n (constant T and P) (Avogadro)
  • Combined, we get.

12
PVnRT the ideal gas equation
  • Gases that can have their temperature, volume,
    and pressure characteristics completely described
    by this equation are called ideal gases.
  • R the gas constant. Its units vary depending
    on the units of P, V, and T.
  • If
  • P is in atm,
  • V is in L,
  • T is in K,
  • STP standard temperature and pressure. Defined
    as 1 atm and 0 ?C (273.15 K).
  • What is the molar volume of a gas at STP?

13
Using ideal gas equation to represent gas laws.
  • Boyles Law.
  • PV nRT
  • P and V will change, but n, R and T are constant.

14
  • Charles Law
  • PV nRT
  • V and T will change, but n, R, and P are constant.

15
  • P, V, and T all change, but n is constant
  • PV nRT

16
More applications of the ideal gas equation.
  • Obtaining the density of a gas
  • from PV nRT
  • d PM/RT (where M is the molar mass)

17
volumes of gases in chemical reactions.
  • air bags.
  • 2 NaN3(s) ? 2 Na (s) 3 N2 (g)
  • air bag volume 36 L pressure 1.15 atm
    temperature 26.0 ?C. How much NaN3, in g, needed?

18
  • 2 KClO3 (s)? 2 KCl (s) 3 O2 (g)
  • volume of O2 produced when 1.50 g KClO3
    decomposes?

19
Gas mixtures and partial pressures
  • Daltons Law of partial pressures
  • from PV nRT.
  • Ptotal P1 P2 P3 .
  • collecting gases over waterthe gas is not alone.

20
Kinetic molecular theory of gases.
  • An explanation of what happens at the molecular
    level that causes the observations in the ideal
    gas laws.
  • Gases consist of large numbers of molecules in
    continuous random motion.
  • The volume of all the molecules of gas is
    negligible compared to the total volume (i.e.,
    each gas molecule is basically an infintessimally
    small dot).
  • Attractive and repulsive forces between molecules
    are negligible.

21
  • Energy transitions between molecules are
    perfectly elastic. The average kinetic energy of
    the molecules will not change over time as long
    as the temperature stays constant.
  • The absolute temperature is proportional to the
    average kinetic energy of the gas. At any given
    temperature all gases in the mixture have the
    same average kinetic energy.
  • KE ½ mu2. u the root mean square (rms) speed
    of the gas. (root mean square is an averaging
    technique, though it is not the same as the
    average)

22
The kinetic theory explains the gas law
  • Important observations
  • volume increases at constant temperature (Boyles
    law). Molecules must travel further to reach the
    wall of a larger container. Thus, collisions
    against the container wall are less frequent, the
    pressure therefore drops.
  • Temperature increases at constant volume
    (Charles Law). when temperature (and kinetic
    energy) increase, the speed of the molecules
    increases. Faster molecules collide with the
    container walls more often, so pressure
    increases.

23
Effusion and diffusion
  • effusion
  • diffusion
  • Lighter molecules move faster than heavier
    molecules

24
Grahams Law of effusion
  • the rate of effusion is twice as fast for r1 if
    M1 is 4 times lighter than M2.

25
Diffusion vs. effusion
  • Diffusion is complicated by the presence of other
    molecules. The mean free path is a determining
    factor.
  • Mean free path

26
Real gases
  • Assumptions in kinetic theory of gases not always
    valid.
  • Molecules are not infinitely small
  • Attractive and repulsive forces are not
    negligible.
  • Collisions are not always elastic.

27
Deviations from ideality
  • for one mole of an ideal gas (n1). PV/RT always
    1.
  • For ANY amount of ideal gas, PV/nRT 1
  • However, for real gases, PV/nRT doesnt always
    1.
  • Ideal gas equation is better in some regions than
    in others.

28
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29
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30
Deviations more likely to occur at
  • low temperature Molecules moving slower,
    intermolecular forces become a greater factor
    (especially near liquid/gas interface).
  • Higher pressure Molecule size becomes an
    greater factor interfering with travel of
    molecules.
  • Corrections to ideal gas equation are made to
    take this into account.
  • Van der Waals equation is one example
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