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Energy

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Title: Energy


1
Energy
  • Chapter 10

2
10.1 The Nature of Energy
  • Energy the ability to do work or produce heat
  • Potential Energy due to position or composition
  • Kinetic Energy due to motion
  • Depends on the mass of the object (m) and its
    velocity (v)
  • KE ½ mv2

3
The Law of Conservation of Energy
  • Energy can be converted from one form to another
    but can be neither created nor destroyed
  • The energy in the universe is constant

4
Work
  • Work Force x distance
  • W Fd
  • Frictional Heating 2 surfaces in contact with
    each other
  • Depends on surface and force pushing the surfaces
    together

5
State Function
  • The property of the system that changes
    independently of its pathway
  • The pathway is how you get there
  • Example
  • If you travel from Chicago to Denver what are
    state functions?
  • The route you take to get there is your pathway,
    so it is not a state function
  • Change in elevation doesnt depend on how you get
    there so it is a state function

6
10.2 Temperature and Heat
  • Temperature Measure of the random motion of the
    components of a substance

7
  • Heat The flow of energy due to a difference in
    temperature

8
10.3 Exothermic and Endothermic Processes
  • System part of universe we are looking at
  • Surroundings everything else
  • Exothermic energy flows out of a system
  • Endothermic energy flows into a system

9
  • Where does energy as heat come from in exothermic
    reactions?
  • It depends on the potential energy between the
    products and reactants

10
10.4 Thermodynamics
  • Law of Conservation of Energy (a.k.a. The First
    Law of Thermodynamics)
  • Energy can neither be created nor destroyed under
    normal conditions
  • The energy of the universe is constant

11
E internal energy
  • E is the sum of the kinetic energy and the
    potential energy
  • Can be changed by the flow of work, heat, or both
  • ? change in called delta
  • w work
  • q heat
  • ?E q w
  • Change in internal energy equals heat plus work

12
  • Thermodynamic quantities are made up of a number
    that shows magnitude and a sign that shows
    whether energy is flowing into the system
    (endothermic ) or out of the system
    (exothermic - )

13
10.5 Measuring Energy Changes
  • calorie amount of energy required to raise the
    temperature of 1 gram of water by one degree
    Celsius
  • 1000 calories (1 kilocalorie) is what we refer to
    as a Calorie with a capital C
  • 1 calorie 4.184 joules
  • 1 cal 4.184 J
  • To go from calories to joules multiply by 4.184
  • To go from joules to calories divide by 4.184

14
And now for a problem!
  • How much heat, in joules, is required to raise
    the temperature of 7.40 g water from 29.0 C to
    46.0 C?
  • We know we need 4.184 J of energy raise 1 g of
    water 1 C
  • We have 7.40 g of water so it will take 7.4 g x
    4.184 J to raise it 1 C
  • We also need to raise the temperature 17 C so
    17.0 C x 7.4 g x 4.184 J/ g x C
  • So we need 526 J of energy
  • Now try this
  • Calculate the joules of energy required to heat
    454 g of water from 5.4 C to 98.6 C?

15
  • So we know that the amount of energy we need to
    raise the temperature of a substance depends on
    the amount of substance and the change in
    temperature
  • But the substance also plays a big part
  • Specific Heat Capacity the amount of energy
    needed to raise the temperature of 1 g of a
    substance 1 C

16
Specific Heats
  • Liquid water 4.184 J
  • Aluminum 0.89 J
  • Gold 0.13 J
  • This explains why certain things heat up faster
    than others
  • The pot heats up faster than the water in it
  • The water in the pool is colder that the cement
    around it

17
Now for another equation
  • The amount of energy required the specific heat
    x mass x change in temperature
  • Q m x Cp x ?T
  • Try this sample
  • A 1.6 g sample of metal that looks like gold
    requires 5.8 J of energy to change its
    temperature from 23 C to 41 C. Is the metal
    gold? (Hint you are finding what s is and
    comparing to what you know about golds specific
    heat)
  • Answer No Golds s 0.13 J/ g C but this
    substance has an s 0.20 J / g C

18
10.6 Thermochemistry (Enthalpy)
  • Enthalpy (symbol H) is the same as the flow of
    heat
  • ?Hp heat
  • P tells us it occurred under constant pressure
  • ? means change in
  • So the enthalpy for a reaction at constant
    pressure is the same as heat

19
Calorimetry
  • Calorimeter device used to determine the heat
    associated with a chemical reaction
  • Reaction is run in calorimeter and temperature
    change is observed
  • We can use calorimeter to find ?H
  • Once we know ?H for some reactions we can use
    those to calculate ?H for other reactions

20
10.7 Hesss Law
  • The change in enthalpy for a given process is
    independent of the pathway for the process (this
    means it is a state function)
  • Hesss Law states that the change in enthalpy
    from reactants to products in a reaction is the
    same whether it takes place in one step or a
    series of steps
  • N2 2O2 ? 2NO2 ?H 68 kJ
  • or
  • N2 O2 ? 2NO ?H 180 kJ
  • 2NO O2 ? 2NO2 ?H -112 kJ
  • So 180 kJ (-112 kJ) ?H 68 kJ

21
Characteristics of Enthalpy Changes
  • If a reaction is reversed, ?H is reversed
  • Xe 2F2 ? XeF4 ?H -251 kJ
  • XeF4 ? Xe 2F2 ?H 251 kJ
  • Magnitude of ?H is proportional to quantities of
    reactants and products
  • Xe 2F2 ? XeF4 ?H -251 kJ
  • 2(Xe 2F2 ? XeF4) ?H -502 kJ

22
10.8 Quality versus Quantity of Energy
  • One of the most important characteristics is that
    it is conserved
  • Eventually all energy will take the form of heat
    and spread evenly throughout the universe and
    everything will be the same temperature
  • This means work wont be able to be done and
    universe will be dead called heat death
  • We care more about what kind of energy (quality)
    than the amount of energy (quantity)

23
10.9 Energy and Our World
  • Fossil Fuels formed by decaying products of
    plants
  • Petroleum
  • Natural Gas
  • Coal
  • Greenhouse Effect Visible light travels through
    atmosphere, converted to infrared radiation
    (heat) which is absorbed by certain molecules,
    H20 and CO2 mainly, which radiate it back to earth

24
10.10 Energy as a Driving Force
  • Energy Spread in any given process,
    concentrated energy is dispersed widely
  • Happens with every exothermic reaction
  • When gas is burned, energy stored is dispersed
    into surrounding air
  • Matter Spread molecules of a substance are
    spread out and occupy a larger volume
  • Salt dissolves in water due to matter spread
  • These 2 processes are important driving forces
    that cause events to occur

25
Entropy
  • Invented function that keeps track of disorder
  • Entropy (S) is a measure of disorder or
    randomness
  • So a cube of ice has a a lower S value than steam
  • Energy spread and Matter spread lead to greater
    entropy
  • The entropy in the universe is always increasing
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