Gases for Students

download Gases for Students

of 43

Transcript of Gases for Students

  • 8/4/2019 Gases for Students

    1/43

    The Gaseous State of Matter

  • 8/4/2019 Gases for Students

    2/43

    General Properties

    The least dense and most mobile state of

    matter

    Molecules move at very high velocities;

    thus have high kinetic energy.

    Mixtures are uniformly distributed within

    the container they are confined

  • 8/4/2019 Gases for Students

    3/43

    Behavior of Gases

    Any form of matter exists under suitable

    conditions of temperature, pressure and

    volume.

    The effect of these three factors is quite

    obvious in gases.

  • 8/4/2019 Gases for Students

    4/43

    Behavior of Gases

    Under the same sets of conditions,

    behavior of gases can be explained by the

    Kinetic Molecular Theory (KMT).

  • 8/4/2019 Gases for Students

    5/43

    Kinetic Molecular Theory

    Studies begun in the 17th century by Robert

    Boyle

  • 8/4/2019 Gases for Students

    6/43

    Kinetic Molecular Theory

    All gases are made up of submicroscopic

    (tiny), particles called molecules.

    These molecules are very small in relation

    to the distances between them.

  • 8/4/2019 Gases for Students

    7/43

    Kinetic Molecular Theory

    Gas molecules have no attraction for one

    another.

    These molecules are in constant random

    motion causing them to collide with one

    another and the walls of the container.

  • 8/4/2019 Gases for Students

    8/43

    Kinetic Molecular Theory

    The collisions of molecules are perfectly

    elastic. No energy is lost by the collision of

    gas molecules with another or with the

    walls of the container.

    The average KE of molecules varies

    directly with the Kelvin temperature.

  • 8/4/2019 Gases for Students

    9/43

    Kinetic Molecular Theory

    The type of gas behaving according to the

    kinetic molecular theory (KMT) is called

    an ideal or perfect gas.

  • 8/4/2019 Gases for Students

    10/43

    Kinetic Molecular Theory

    No ideal gases exist, but under certain

    conditions of P and T, real gases approach

    ideal behavior, or at least show only small

    deviations from it.

  • 8/4/2019 Gases for Students

    11/43

    Kinetic Molecular Theory

    Under extreme conditions, such as very

    high P and low T, real gases deviate

    greatly from ideal behavior.

  • 8/4/2019 Gases for Students

    12/43

    Note

    All gases have the same KE at the same

    temperature, thus; lighter molecules have

    greater velocities than the heavier ones.

  • 8/4/2019 Gases for Students

    13/43

    Diffusion

    The ability of two or more gases to mix

    spontaneously until they form a uniform

    mixture.

    Because of the molecular motion of gases.

  • 8/4/2019 Gases for Students

    14/43

    Effusion

    The process by which gas molecules pass

    through a very small orifice from a

    container at higher pressure to one at

    lower pressure.

  • 8/4/2019 Gases for Students

    15/43

    Grahams Law of Effusion

    Thomas Graham was able to observed the

    rate of effusion was dependent on the

    density of a gas.

  • 8/4/2019 Gases for Students

    16/43

    Grahams Law of Effusion

    r

    r

    MW

    MW

    1

    2

    2

    1 1

  • 8/4/2019 Gases for Students

    17/43

    Pressure

    Pressure is defined as a force that is

    exerted per unit of area.

    This is obtained by dividing the force by

    the area on which the force acts.

  • 8/4/2019 Gases for Students

    18/43

    Pressure

    The atmosphere exerts pressure on the

    earth known as atmospheric pressure.

    The atmospheric pressure is

    approximately 1 atmosphere, but varies

    with elevation or altitude.

  • 8/4/2019 Gases for Students

    19/43

    Conversion of Pressure

    1 atm = 760 mm Hg 1 Torr = 1 mm Hg

    = 76 cm Hg 1 Pa = 1 N/m

    = 14.7 lbs/in2

    = 760 Torr

    = 101,325 Pa= 101.325 KPa

  • 8/4/2019 Gases for Students

    20/43

    Temperature

    Temperature is a measure of the degree of

    hotness or coldness of a body.

    To measure, temperature, thermometers

    are used.

    Three temperature scales are currently in

    use.

  • 8/4/2019 Gases for Students

    21/43

    Temperature

  • 8/4/2019 Gases for Students

    22/43

    Temperature

    Molecules of matter when heated move

    faster but when cooled, the particles move

    slower and slower until, theoretically all

    motion stops.

    The lowest possible hypothetical T at

    which V is zero is -273.15C (all molecules

    will stop moving.)

  • 8/4/2019 Gases for Students

    23/43

    Equations for Conversion

    K = C + 273.15

    100

    FF - 32 or

    5

    9 FF - 32

    CC

    CC

    180

    F F100

    + 32 or F 9 F

    5+ 32

    180

    CC

    CC

  • 8/4/2019 Gases for Students

    24/43

    Volume

    Volume maybe described as the space

    that a specific substance occupies.

    Several units of volume maybe used such

    as liter (L), milliliters (mL), cubic

    centimeter (cm), cubic meter (m), etc.

  • 8/4/2019 Gases for Students

    25/43

    Properties of Gases

    Gases assume the volume and shape oftheir containers.

    Gases have low densities.

    Gases are able to exert pressure.

    Gases diffuse rapidly.

    Gases expand when heated.

    Gases are the most compressible of thestates of matter.

  • 8/4/2019 Gases for Students

    26/43

    Boyles Law

    The volume of a fixed amount of gas is

    inversely proportional to its pressure when

    its temperature is kept constant.

    The Pressure of the gas Varies Inversely

    with Volume at Constant Temperature.

    Robert Boyle

  • 8/4/2019 Gases for Students

    27/43

    In Equation

    V1

    P

  • 8/4/2019 Gases for Students

    28/43

    Boyles Law

    The heart of Boyles Law is the experimental factthat the product of pressure and volume isconstant.

    This can be expressed in the following form,which is easier to use in calculations. Thesubscripts 1 and 2 rearranging,

    P1V1 = P2V2

  • 8/4/2019 Gases for Students

    29/43

    Charles Law

    The volume of a given amount of gas heldat constant pressure is directlyproportional to the absolute (Kelvin)

    temperature. The Absolute Temperature (Kelvin) of the

    gas varies proportionally with volume atconstant pressure.

    Jacques Charles

  • 8/4/2019 Gases for Students

    30/43

    In Equation

    V T

    VT = VT 1

    1

    2

    2

  • 8/4/2019 Gases for Students

    31/43

    Gay Lussacs Law

    The pressure of a fixed amount of gas is

    directly relationship proportional to the

    absolute temperature (Kelvin) only when

    its volume is held constant.

    French scientists Jacques Charles and

    Joseph Gay Lussac,

  • 8/4/2019 Gases for Students

    32/43

    In Equation

    P T

    P

    T =

    P

    T 1

    1

    2

    2

  • 8/4/2019 Gases for Students

    33/43

    STP Condition

    Under STP,

    pressure is fixed at 1 atm

    temperature at 0 0C or 273.15 K

    volume of 1 mole of a gas is constant at 22.4 L

    called the standard molar volume.

  • 8/4/2019 Gases for Students

    34/43

    Combined Gas Law

    The volume of a fixed amount of a gas is

    directly proportional to the ratio of its

    absolute temperature and its pressure.

  • 8/4/2019 Gases for Students

    35/43

    In Equation

    VT

    P

    P V

    T=

    P V

    T1 1

    1

    2 2

    2

  • 8/4/2019 Gases for Students

    36/43

    Avogadros Principle

    The volume of a gas is directly

    proportional to the number of moles of the

    gas present at constant pressure and

    temperature

    V n

  • 8/4/2019 Gases for Students

    37/43

    Summary of Gas Laws

    Boyle's Law: V 1/P (constant n & T)

    Charles' Law: V T (constant n & P)

    Avogadro's Law: V n (constant P & T)

    V nTP

  • 8/4/2019 Gases for Students

    38/43

    Ideal Gas Equation

    PV = nRT

    V = R

    nT

    P

  • 8/4/2019 Gases for Students

    39/43

    Universal Gas Constant, R

    R = 0.08205 atm-Lmol-K

    = 62.36mmHg-L

    mol-K

    = 62,358.97torr - mL

    mol-K

    82.05 atm-mLmol-K

  • 8/4/2019 Gases for Students

    40/43

    Gas Stoichiometry

    Stoichometry problems involving moles

    and masses were discussed in the previous

    chapter.

    There is also a relationship between

    volumes and amounts of reactants and

    products in a balanced chemical equation.

    The flow chart suggests the basic tools for

    solving problems involving gases.

  • 8/4/2019 Gases for Students

    41/43

    Mass-Volume Relationship

    The balanced equation for the metabolicbreakdown of glucose (C6H12O6) is similaras that for the combustion of glucose in

    air. This equation maybe written as:C6H12O6 (s) + 6O2(g) 6CO2 (g) + 6H2O(l)

    Calculate the volume of CO2 produced at40C and 760 torr when 6.50 g of glucose isused up in the reaction.

  • 8/4/2019 Gases for Students

    42/43

    Volume-Volume Relationship

    Ammonia gas, NH3, may be prepared bythe Haber Process. In this process for thesynthesis of ammonia,

    N2(g) + 3H2(g) 2NH3(g)

    how many liters of N2 are needed to reactcompletely with 50.0 L of H2, if thevolumes of both gases are measured atSTP?

  • 8/4/2019 Gases for Students

    43/43

    Air Pollution

    Global Warming

    Ozone Depletion