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Gibbs Free Energy Example

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    I have this reaction here
    where if I had a mole of
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    methane, and I react that with
    two moles of oxygen, I'll
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    produce a mole of carbon
    dioxide and
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    two moles of water.
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    And what we want to answer in
    this video is whether this
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    reaction is spontaneous.
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    And we learned in the last
    video that to answer that
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    question, we have to turn to
    Gibbs free energy, or the
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    change in Gibbs free energy.
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    And the change in Gibbs free
    energy is equal to the
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    enthalpy change for the reaction
    minus the temperature
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    at which it is occurring, times
    the change in entropy.
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    And if this is less than
    zero, then it's
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    a spontaneous reaction.
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    So I gave us a little
    bit of a head start.
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    I just calculated the change in
    enthalpy for this reaction,
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    and that's right here.
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    And we know how to do that.
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    We've done that several
    videos ago.
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    You could just look up the heats
    of formation of each of
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    these products.
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    For water you'll multiply
    it by 2, since you
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    have 2 moles of it.
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    And so you have the heats of
    formation of all the products,
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    and then you subtract
    out the heats of
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    formation of all the reactants.
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    And of course the heat of
    formation of O2 is O, so this
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    won't even show up in it, and
    you'll get minus 890.3
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    kilojoules.
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    Well, this tells us that this
    is an exothermic reaction.
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    That this side of the equation
    has less energy in it-- you
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    could kind of think of it
    that way-- is that side.
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    So some energy must have
    been released.
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    We could even put here, you
    know, plus e for energy.
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    Let me write, plus some energy
    is going to be released.
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    So that's why it's exothermic.
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    But our question is, is
    this spontaneous?
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    So to figure out if it's
    spontaneous, we also have to
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    figure out our delta s.
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    And to help figure out the
    delta s I, ahead of time,
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    looked up the standard
    molar entropies for
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    each of these molecules.
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    So for example, the standard--
    I'll write it here in a
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    different color.
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    The standard-- you put a little
    naught symbol there--
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    the standard molar entropy-- so
    when we say standard, it's
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    at 298 degrees Kelvin.
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    Actually, I shouldn't
    say degrees Kelvin.
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    It's at 298 Kelvin You don't
    use the word degrees,
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    necessarily, when you
    talk about Kelvin.
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    So it's at 298 Kelvin, which is
    25 degrees Celsius, so it's
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    at room temperature.
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    So that's why it's considered
    standard temperature.
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    So the standard entropy of
    methane at room temperature is
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    equal to this number
    right here.
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    186 joules per Kelvin mole.
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    So if I have 1 mole of methane,
    I have 186 joules per
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    Kelvin of entropy.
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    If I have 2 moles, I
    multiply that by 2.
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    If I have 3 moles, I
    multiply that by 3.
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    So the total change in entropy
    of this reaction is the total
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    standard entropies of the
    products minus the total
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    standard entropies
    of the reactants.
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    Just like what we did
    with enthalpy.
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    So that's going to be equal to
    213.6 plus-- I have 2 moles of
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    water here.
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    So it's plus 2 times-- let's
    just write 70 there.
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    69.9, almost 70.
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    Plus 2 times 70, and then I
    want to subtract out the
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    entropy of the reactants, or
    this side of the reaction.
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    So the entropy of 1 mole of CH4
    is 186 plus 2 times 205.
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    So just eyeballing it already,
    this number is close to this
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    number, but this number is much
    larger than this number.
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    Liquid water has a much
    lower-- this is
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    liquid water's entropy.
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    It has a much lower entropy
    than oxygen gas.
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    And that makes sense.
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    Because liquid formed, there's
    a lot fewer states.
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    It all falls to the bottom of
    the container, as opposed to
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    kind of taking the shape of
    the room and expanding.
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    So a gas is naturally going
    to have much higher
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    entropy than a liquid.
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    So just eyeballing it, we can
    already see that our products
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    are going to have a lower
    entropy than our reactants.
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    So this is probably going
    to be a negative number.
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    But let's confirm that.
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    So I have 200, 213.6 plus--
    well, plus 140, right?
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    2 times 70.
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    Plus 140 is equal to 353.6.
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    So this is 353.6.
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    And then from that, I'm going to
    subtract out-- so 186 plus
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    2 times 205 is equal to 596.
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    So minus 596, and what
    is that equal to?
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    So we put the minus 596, and
    then plus the 353.6, and we
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    have minus 242.4.
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    So this is equal to minus 242.4
    joules per Kelvin is our
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    delta s minus.
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    So we lose that much entropy.
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    And those units might not make
    sense to you right now, and
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    actually you know these are
    but of arbitrary units.
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    But you can just say, hey, this
    is getting more ordered.
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    And it makes sense, because
    we have a ton of gas.
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    We have 3 separate molecules,
    1 here and 2
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    molecules of oxygen.
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    And then we go to 3 molecules
    again, but the
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    water is now liquid.
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    So it makes sense to me
    that we lose entropy.
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    There's fewer states
    that the liquid,
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    especially, can take on.
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    But let's figure out whether
    this reaction is spontaneous.
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    So our delta g is equal
    to our delta h.
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    We're releasing energy,
    so it's minus 890.
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    I'll just get rid
    of the decimals.
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    We don't have to be
    that precise.
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    Minus our temperature.
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    We're assuming that we're at
    room temperature, or 298
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    degrees Kelvin.
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    That's 28-- I should just
    say, 298 Kelvin.
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    I should get in the habit
    of not saying
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    degrees when I say Kelvin.
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    Which is 25 degrees Celsius,
    times our change in entropy.
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    Now, this is going
    to be a minus.
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    Now you might say, OK, minus
    242, you might want to put
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    that there.
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    But you have to be very,
    very, very careful.
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    This right here is
    in kilojoules.
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    This right here is in joules.
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    So if we want to write
    everything in kilojoules,
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    since we already wrote that
    down, let's write this in
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    kilojoules.
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    So it's 0.242 kilojoules
    per Kelvin.
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    And so now our Gibbs free energy
    right here is going to
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    be minus 890 kilojoules minus
    290-- so the minus and the
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    minus, you get a plus.
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    And that makes sense, that the
    entropy term is going to make
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    our Gibbs free energy
    more positive.
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    Which, as we know, since we want
    to get this thing below
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    0, this is going to fight
    the spontaneity.
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    But let's see if it can
    overwhelm the actual enthalpy,
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    the exothermic nature of it.
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    And it seems like it will,
    because you multiply a
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    fraction times this,
    it's going to be a
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    smaller number than that.
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    But let's just figure it out.
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    So divided by 1, 2, 3.
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    That's our change in entropy
    times 298, that's our
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    temperature, is minus 72.
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    So this term becomes-- and then
    we put a minus there-- so
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    it's plus 72.2.
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    So this is the entropy term
    at standard temperature.
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    It turns into that.
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    And this is our enthalpy term.
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    So we can already see that the
    enthalpy is a much more
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    negative number than our
    positive term from our
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    temperature times our
    change in entropy.
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    So this term is going
    to win out.
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    Even though we lose entropy in
    this reaction, it releases so
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    much energy that's going
    to be spontaneous.
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    This is definitely less than
    0, so this is going to be a
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    spontaneous reaction.
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    As you can see, these Gibbs free
    energy problems, they're
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    really not too difficult.
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    You just really need to
    find these values.
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    And to find these values, it'll
    either be given, the
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    delta h, but we know how to
    solve for the delta h.
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    You just look up the heats
    of formations of all the
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    products, subtract out the
    reactants, and of course you
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    wait by the coefficients.
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    And then, to figure out the
    change in entropy, you do the
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    same thing.
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    You have to look up the standard
    molar entropies of
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    the products' weight by the
    coefficients, subtract out the
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    reactants, and then just
    substitute in here, and then
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    you essentially have the
    Gibbs free energy.
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    And in this case,
    it was negative.
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    Now, you could imagine a
    situation where we're at a
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    much higher temperature.
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    Like the surface of the sun or
    something, where all of a
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    sudden, instead of a 298 here,
    if you had like a 2,000 or a
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    4,000 there.
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    Then all of a sudden, things
    become interesting.
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    If you could imagine, if
    you had a 40,000 Kelvin
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    temperature here, then all of a
    sudden the entropy term, the
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    loss of entropy, is going
    to matter a lot more.
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    And so this term, this positive
    term, is going to
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    outweigh this, and maybe it
    wouldn't be spontaneous at a
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    very, very, very, very
    high temperature.
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    Another way to think about it.
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    A reaction that generates heat
    that lets out heat-- the heat
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    being released doesn't matter so
    much when there's already a
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    lot of heat or kinetic energy
    in the environment.
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    If the temperature was high
    enough, this reaction would
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    not be spontaneous, because
    maybe then the entropy term
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    would win out.
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    But anyway, I just wanted to do
    this calculation for you to
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    show you that there's nothing
    too abstract here.
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    You can look up everything on
    the web, and then figure out
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    if something is going
    to be spontaneous.
Title:
Gibbs Free Energy Example
Description:

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Video Language:
English
Team:
Khan Academy
Duration:
09:57

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