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  • - [Instructor] We're told an athlete takes a deep breath,

  • inhaling 1.85 liters of air

  • at 21 degrees Celsius

  • and 754 millimeters of mercury.

  • How many moles of air are in the breath?

  • How many molecules?

  • So pause this video,

  • and see if you can figure this out on your own.

  • All right, now let's work through this together.

  • So let's think about what they are giving us

  • and what we need to figure out.

  • So, they are giving us a volume, right over here.

  • They are also giving us a temperature, right over here.

  • They're also giving us,

  • I'm trying to use all of my colors here,

  • they're giving us a pressure.

  • And they want us to figure out the number of moles.

  • I'm gonna use a green color here.

  • So they want to know,

  • so we often use the lowercase letter, n,

  • to represent the number of moles.

  • And so, do we know something that connects pressure,

  • temperature, volume, and the number of moles?

  • Well, you might be thinking of the Ideal Gas Law,

  • which tells us that pressure

  • times volume

  • is equal to the number of moles, n,

  • times the ideal gas constant, R,

  • times temperature, T.

  • And so we know everything here except for n,

  • so we can solve for n.

  • I know what some of you are saying,

  • "Wait, do we know R?"

  • Well, R is a constant.

  • And it's going to be dependent on which units we use,

  • and we'll figure out which version of R we use.

  • But that's why I gave you this little table here,

  • that you might see on a formula sheet,

  • if you were taking something like an AP exam.

  • So we actually do know what R is.

  • So, we just need to solve for n.

  • So, to solve for n, you just divide both sides by RT,

  • and so you are going to get

  • that n is equal to

  • pressure times the volume

  • over

  • R

  • times T,

  • R times T.

  • And so this is going to be equal to what?

  • Well, our pressure is 754 millimeters of mercury.

  • Now, over here, where they give us the ideal gas

  • or the different versions of the ideal gas constants,

  • you don't see any of them that deal

  • with millimeters of mercury.

  • But they do tell us that each millimeter

  • of mercury is equal to a Torr.

  • If you get very, very, very precise,

  • they are slightly different.

  • But for the purposes of a first-year chemistry class,

  • you can view a millimeter of mercury as being a Torr.

  • So, you can view the pressure here as 754 Torr.

  • So, let me write that down.

  • So, this is 754 Torr.

  • And then we're going to multiply that times the volume.

  • And here, they give the volume

  • in liters in several of these,

  • and we're probably going to be using this one,

  • this version of the ideal gas constant,

  • that has liters, Torr, moles, and Kelvin.

  • And so let's multiply times the volume,

  • so times 1.85 liters.

  • And then that is going to be divided by

  • the ideal gas constant.

  • I'll use this version because it's using all

  • of the units that I already have.

  • I know what you're thinking,

  • "Wait, the temperature's given in degrees Celsius."

  • But it's easy to convert from degrees Celsius to Kelvin.

  • You just have to add 273

  • to whatever you have in degrees Celsius to get to Kelvin,

  • because none of these are given in degrees Celsius.

  • And so, I will use this ideal gas constant.

  • So this is going to be 62.36 liter Torr

  • liter Torr,

  • per mole Kelvin.

  • Mole to the negative one is just one over mole,

  • so I could write it like this.

  • Kelvin to the negative one is just one over Kelvin.

  • And then, I'm gonna multiply that times the temperature.

  • So times, what is 21 degrees Celsius in terms of Kelvin?

  • Well, I add 273 to that, so that's going to be 294 Kelvin.

  • And we can validate that the units all work out.

  • This liter cancels out with this liter.

  • This Torr cancels out with that Torr.

  • This Kelvin cancels out with this Kelvin.

  • And so, we're going to be left with some calculation.

  • And, it's going to be one over one over moles,

  • or it's essentially going to simplify

  • to just being a certain number of moles.

  • And so, let's get our calculator out

  • to figure out the number of moles in that breath.

  • So n, I keep using slightly different colors,

  • so n is going to be equal to

  • 754

  • times 1.85

  • divided by 62.36

  • and then, also divided by,

  • divided by 294,

  • is equal to this thing.

  • And let's see how many significant digits we have.

  • We have three here, three here, three here, four here.

  • So, when we're multiplying and dividing,

  • we just want to use the fewest amount that I'm dealing with.

  • So I wanna go to three significant figures.

  • So 0.0, one, two, three significant figures, so 0.0761.

  • This is going to be 0.0761.

  • And I could say approximately 'cause I am rounding.

  • But that's three significant figures there.

  • So, that's the number of moles of air in the breath.

  • Now, the next question is how many molecules is that?

  • Well, we know that each mole has roughly 6.022

  • times 10 to the 23rd molecules in it,

  • so we just have to multiply this times 6.022

  • times 10 to the 23rd.

  • So, we could write it this way.

  • We could write 0.0761 moles,

  • I'll write mole, times

  • 6.022 times 10 to the 23rd molecules,

  • molecules per mole.

  • Now these are going to cancel out,

  • and I'm just going to be left with molecules.

  • And I can just take the number that I had before

  • 'cause it's nice to be able to retain precision

  • until you have to think about your significant figures.

  • And so, but once again,

  • because we did this whole calculation,

  • we're going to wanna round everything

  • to three significant figures.

  • So, let's just multiply this times 6.022.

  • EE means times 10 to the,

  • times 10 to the 23rd,

  • is equal to that.

  • And, if I round to three significant figures,

  • because my whole calculation,

  • that was my limiting significant figures,

  • I have 4.58 times 10 to the 22nd.

  • So, this is 4.58

  • times 10

  • to the 22nd molecules.

  • Squeeze that in there, and we're done.

- [Instructor] We're told an athlete takes a deep breath,

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B1 中級

理想気体の法則(PV=nRT)の適用例 (Applying ideal gas law (PV=nRT) example)

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    林宜悉 に公開 2021 年 01 月 14 日
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