1 00:00:00,480 --> 00:00:03,910 This exercise is from 2 00:00:03,910 --> 00:00:06,880 chapter 12 of the Kotz, Treichel and Townsend 3 00:00:06,880 --> 00:00:07,950 and Chemistry and Chemical Reactivity book, 4 00:00:07,950 --> 00:00:09,020 and I'm doing it with their permission. 5 00:00:09,020 --> 00:00:13,190 So they tell us you place 2 liters of water 6 00:00:13,190 --> 00:00:15,110 in an open container in your dormitory room. 7 00:00:15,110 --> 00:00:20,590 The room has a volume of 8 00:00:20,590 --> 00:00:22,345 4.25 times 10 to the fourth liters. 9 00:00:22,345 --> 00:00:24,100 You seal the room and wait for the water to evaporate. 10 00:00:24,100 --> 00:00:26,170 Will all of the water evaporate 11 00:00:26,170 --> 00:00:28,700 at 25 degrees Celsius? 12 00:00:28,700 --> 00:00:31,580 And then they tell us at 25 degrees Celsius, 13 00:00:31,580 --> 00:00:36,050 the density of water is 0.997 grams per milliliter. 14 00:00:36,050 --> 00:00:44,180 And its vapor pressure is 23.8 millimeters of mercury. 15 00:00:44,180 --> 00:00:47,210 And this is actually the key clue 16 00:00:47,210 --> 00:00:47,720 to tell you how to solve this problem. 17 00:00:47,720 --> 00:00:49,730 And just as a bit of review, 18 00:00:49,730 --> 00:00:53,110 lets just think about what vapor pressure is. 19 00:00:53,110 --> 00:00:54,820 Let's say it's some temperature, 20 00:00:54,820 --> 00:00:57,820 and in this case we're dealing at 25 degrees Celsius. 21 00:00:57,820 --> 00:00:59,180 I have a bunch of water, 22 00:00:59,180 --> 00:01:00,530 and let me do that in a water color. 23 00:01:00,530 --> 00:01:03,140 I have a bunch of water molecules 24 00:01:03,140 --> 00:01:05,545 sitting here in a container. 25 00:01:08,290 --> 00:01:12,100 At 25 degrees Celsius, 26 00:01:12,100 --> 00:01:15,150 they're all bouncing around in every which way. 27 00:01:15,150 --> 00:01:17,790 And every now and then 28 00:01:17,790 --> 00:01:21,380 one of them is going to have enough kinetic energy 29 00:01:21,380 --> 00:01:22,530 to kind of escape the hydrogen bonds 30 00:01:22,530 --> 00:01:23,680 and all the things 31 00:01:23,680 --> 00:01:24,410 that keep liquid water in its liquid state 32 00:01:24,410 --> 00:01:25,140 and it will escape. 33 00:01:25,140 --> 00:01:26,780 It'll go off in that direction, 34 00:01:26,780 --> 00:01:27,955 and then another one will. 35 00:01:27,955 --> 00:01:29,190 And this'll just keep happening. 36 00:01:29,190 --> 00:01:32,310 The water will naturally vaporize in a room. 37 00:01:32,310 --> 00:01:38,930 But at some point, 38 00:01:38,930 --> 00:01:40,805 enough of these molecules have vaporized over here 39 00:01:40,805 --> 00:01:42,680 that they're also bumping back into the water. 40 00:01:42,680 --> 00:01:44,910 And maybe some of them can be captured back 41 00:01:44,910 --> 00:01:46,520 into the liquid state. 42 00:01:46,520 --> 00:01:50,010 Now, the pressure at which this happens 43 00:01:50,010 --> 00:01:51,380 is the vapor pressure. 44 00:01:51,380 --> 00:01:55,190 As you can imagine, 45 00:01:55,190 --> 00:01:57,025 as more and more these water molecules vaporize 46 00:01:57,025 --> 00:01:58,860 and go into the gaseous state, 47 00:01:58,860 --> 00:02:01,000 more and more will also create pressure, 48 00:02:01,000 --> 00:02:02,135 downward pressure. 49 00:02:02,135 --> 00:02:03,270 More and more will also be 50 00:02:03,270 --> 00:02:04,840 colliding with the surface of the water. 51 00:02:04,840 --> 00:02:09,020 And the pressure at which 52 00:02:09,020 --> 00:02:12,170 the liquid and the vapor states are in equilibrium 53 00:02:12,170 --> 00:02:12,780 is the vapor pressure. 54 00:02:12,780 --> 00:02:13,390 And they're telling us right now. 55 00:02:13,390 --> 00:02:18,230 It is 23.8 millimeters of mercury. 56 00:02:18,230 --> 00:02:21,870 Now, what we need to do to figure out this problem is 57 00:02:21,870 --> 00:02:26,320 say, OK, if we could figure out 58 00:02:26,320 --> 00:02:28,075 how many molecules need to evaporate 59 00:02:28,075 --> 00:02:29,830 how many molecules of water need to evaporate 60 00:02:29,830 --> 00:02:33,690 to give us this vapor pressure, 61 00:02:33,690 --> 00:02:37,250 we can then use the density of water 62 00:02:37,250 --> 00:02:38,815 to figure out how many liters of water that is. 63 00:02:38,815 --> 00:02:40,380 So how do we figure out how many molecules-- 64 00:02:40,380 --> 00:02:50,035 let me write this down 65 00:02:50,035 --> 00:02:59,690 --how many molecules of water need to evaporate 66 00:02:59,690 --> 00:03:14,740 to give us the vapor pressure of 67 00:03:14,740 --> 00:03:16,740 23.8 millimeters of mercury? 68 00:03:16,740 --> 00:03:18,740 So what, I guess, law or formula-- 69 00:03:18,740 --> 00:03:21,450 and I never like to just memorize formulas, 70 00:03:21,450 --> 00:03:25,030 but we've given this formula in the past 71 00:03:25,030 --> 00:03:27,630 and it's probably one of the top most useful formulas 72 00:03:27,630 --> 00:03:30,230 in chemistry, or really all of science-- 73 00:03:30,230 --> 00:03:33,230 what formula or law deals with pressure? 74 00:03:33,230 --> 00:03:36,230 They give us the volume of the room 75 00:03:36,230 --> 00:03:37,890 because that's where the pressure will be inside of. 76 00:03:37,890 --> 00:03:41,050 So we have pressure, the equilibrium vapor pressure. 77 00:03:41,050 --> 00:03:45,620 We have a volume of a room right over here. 78 00:03:45,620 --> 00:03:49,150 We know the temperature of the room right over there. 79 00:03:49,150 --> 00:03:52,650 And we're trying to figure out the number of molecules 80 00:03:52,650 --> 00:03:57,290 that need to evaporate for us to get that pressure 81 00:03:57,290 --> 00:03:59,130 in that volume at that temperature. 82 00:03:59,130 --> 00:04:04,960 So what deals with pressure, volume, 83 00:04:06,515 --> 00:04:08,070 number of molecules, let's say in moles, 84 00:04:08,070 --> 00:04:09,385 so I'll write a lower case n 85 00:04:09,385 --> 00:04:10,700 number of molecules, and temperature? 86 00:04:10,700 --> 00:04:12,170 Well, we've seen this many, many times. 87 00:04:12,170 --> 00:04:13,920 It's the Ideal Gas Law. 88 00:04:13,920 --> 00:04:20,600 Pressure times volume is equal to 89 00:04:20,600 --> 00:04:22,515 the number of moles of our idea gas 90 00:04:22,515 --> 00:04:24,430 in this case we're going to use water as our ideal gas 91 00:04:24,430 --> 00:04:29,140 or vapor as our ideal gas 92 00:04:29,140 --> 00:04:32,950 times the universal gas constant times temperature. 93 00:04:32,950 --> 00:04:35,600 And this should never seem like some bizarre formula to 94 00:04:35,600 --> 00:04:37,990 you because it really, really makes sense. 95 00:04:37,990 --> 00:04:42,020 If your pressure goes up, then that means that either the 96 00:04:42,020 --> 00:04:44,660 number of molecules have gone up, and we're assuming the 97 00:04:44,660 --> 00:04:45,830 volume is constant. 98 00:04:45,830 --> 00:04:48,700 That means either the number of molecules have gone up, 99 00:04:48,700 --> 00:04:50,890 which makes sense-- more things bouncing onto the side 100 00:04:50,890 --> 00:04:51,740 of the container. 101 00:04:51,740 --> 00:04:53,820 Or your temperature has gone up-- the same number of 102 00:04:53,820 --> 00:04:56,480 things, but they're bumping with higher kinetic energy. 103 00:04:56,480 --> 00:05:01,110 Or if your pressure stays the same and your volume goes up, 104 00:05:01,110 --> 00:05:04,230 then that also means that your number of molecules went up, 105 00:05:04,230 --> 00:05:05,370 or your temperature went up. 106 00:05:05,370 --> 00:05:06,760 Because you now have a bigger container. 107 00:05:06,760 --> 00:05:09,270 In order to exert the same pressure you need either more 108 00:05:09,270 --> 00:05:12,070 molecules or more kinetic energy for the molecules you 109 00:05:12,070 --> 00:05:12,215 have. 110 00:05:12,215 --> 00:05:14,200 And you could keep playing around with this, but I just 111 00:05:14,200 --> 00:05:16,750 want to make it clear this isn't some mysterious formula. 112 00:05:16,750 --> 00:05:18,810 The first time I was exposed to this I kind of did view it 113 00:05:18,810 --> 00:05:20,490 as some type of mysterious formula. 114 00:05:20,490 --> 00:05:22,230 But it's just relating pressure, volume, number of 115 00:05:22,230 --> 00:05:23,980 molecules and temperature. 116 00:05:23,980 --> 00:05:29,320 And then this is just the universal gas constant. 117 00:05:29,320 --> 00:05:32,370 So let's just get everything into the right units here. 118 00:05:32,370 --> 00:05:34,585 And then what we're trying to solve for, we want to figure 119 00:05:34,585 --> 00:05:36,290 out the number of molecules of water. 120 00:05:36,290 --> 00:05:40,780 So we want to solve for n. 121 00:05:40,780 --> 00:05:44,210 And if we know the number of moles of water, we can figure 122 00:05:44,210 --> 00:05:46,320 out the number of grams of water. 123 00:05:46,320 --> 00:05:48,580 And then given the density of water we can figure out the 124 00:05:48,580 --> 00:05:52,880 number of milliliters of water we are dealing with. 125 00:05:52,880 --> 00:05:57,120 So let's just rewrite the Ideal Gas Law by dividing both 126 00:05:57,120 --> 00:06:00,340 sides by the universal gas constant and temperature. 127 00:06:00,340 --> 00:06:07,245 So that you get n is equal to pressure times volume, over 128 00:06:07,245 --> 00:06:10,680 the universal gas constant times temperature. 129 00:06:10,680 --> 00:06:13,290 Now, the hardest thing about this is just making sure you 130 00:06:13,290 --> 00:06:15,490 have your units right and you're using the right ideal 131 00:06:15,490 --> 00:06:17,150 gas constant for the right units, and we'll 132 00:06:17,150 --> 00:06:18,310 do that right here. 133 00:06:18,310 --> 00:06:24,020 So what I want to do, because the universal gas constant 134 00:06:24,020 --> 00:06:27,960 that I have is in terms of atmospheres, we need to figure 135 00:06:27,960 --> 00:06:30,800 out this vapor pressuree- this equilibrium pressure between 136 00:06:30,800 --> 00:06:33,770 vapor and liquid-- we need to write this down in terms of 137 00:06:33,770 --> 00:06:35,040 atmospheres. 138 00:06:35,040 --> 00:06:36,450 So let me write this down. 139 00:06:36,450 --> 00:06:47,260 So the vapor pressure is equal to 23.8 140 00:06:47,260 --> 00:06:51,350 millimeters of mercury. 141 00:06:51,350 --> 00:06:55,040 And you can look it up at a table if you don't have this 142 00:06:55,040 --> 00:06:55,710 in your brain. 143 00:06:55,710 --> 00:07:06,540 One atmosphere is equivalent to 760 millimeters of mercury. 144 00:07:06,540 --> 00:07:09,110 So if we wanted to write the vapor pressure as 145 00:07:09,110 --> 00:07:12,580 atmospheres-- let me get my calculator out, get the 146 00:07:12,580 --> 00:07:15,690 calculator out, put it right over there-- so it's going to 147 00:07:15,690 --> 00:07:24,140 be 23.8 times 1 over 760, or just divided by 760. 148 00:07:24,140 --> 00:07:27,210 And we have three significant digits, so 149 00:07:27,210 --> 00:07:31,920 it looks like 0.0313. 150 00:07:31,920 --> 00:07:40,110 So this is equal to 0.0313 atmospheres. 151 00:07:40,110 --> 00:07:41,590 That is our vapor pressure. 152 00:07:41,590 --> 00:07:43,110 So let's just deal with this right here. 153 00:07:43,110 --> 00:07:46,780 So the number of molecules of water that are going to be in 154 00:07:46,780 --> 00:07:49,900 the air in the gaseous state, in the vapor state, is going 155 00:07:49,900 --> 00:07:51,740 to be equal to our vapor pressure. 156 00:07:51,740 --> 00:07:52,990 That's our equilibrium pressure. 157 00:07:55,710 --> 00:07:59,240 If more water molecules evaporate after that point, 158 00:07:59,240 --> 00:08:01,140 then we're going to have a higher pressure, which will 159 00:08:01,140 --> 00:08:04,130 actually make them favor more of them going into the liquid 160 00:08:04,130 --> 00:08:06,570 state, so we'll go kind of past the equilibrium, which is 161 00:08:06,570 --> 00:08:07,140 not likely. 162 00:08:07,140 --> 00:08:10,060 Or another way to think about it-- more water molecules are 163 00:08:10,060 --> 00:08:12,455 not going to of evaporate at a faster rate than they are 164 00:08:12,455 --> 00:08:15,050 going to condense beyond that pressure. 165 00:08:15,050 --> 00:08:22,070 Anyway, the pressure here is 0.0313 atmospheres. 166 00:08:22,070 --> 00:08:26,420 The volume here-- they told us right over here-- so that's 167 00:08:26,420 --> 00:08:28,880 the volume-- 4.25. 168 00:08:28,880 --> 00:08:35,210 4.25 times 10 to the fourth liters. 169 00:08:35,210 --> 00:08:37,720 And then we want to divide that by-- and you want to make 170 00:08:37,720 --> 00:08:40,610 sure that your universal gas constant has the right units, 171 00:08:40,610 --> 00:08:46,370 I just looked mine up on Wikipedia-- 0.08-- see 172 00:08:46,370 --> 00:08:48,170 everything has three significant digits. 173 00:08:48,170 --> 00:08:51,250 So let me just allow that more significant digits and we'll 174 00:08:51,250 --> 00:08:52,820 just round at the end. 175 00:08:52,820 --> 00:09:07,540 0.082057, and the units here are liters atmospheres per 176 00:09:07,540 --> 00:09:12,420 mole at kelvin. 177 00:09:12,420 --> 00:09:13,310 And this makes sense. 178 00:09:13,310 --> 00:09:14,890 This liter will cancel out with that liter. 179 00:09:14,890 --> 00:09:17,330 That atmospheres cancels out with that atmospheres. 180 00:09:17,330 --> 00:09:19,940 I'm about to multiply it by temperature 181 00:09:19,940 --> 00:09:21,150 right here in kelvin. 182 00:09:21,150 --> 00:09:22,220 We'll cancel out there. 183 00:09:22,220 --> 00:09:24,920 And then we'll have a 1 over moles in the denominator. 184 00:09:24,920 --> 00:09:27,290 A 1 over moles in the denominator will just be a 185 00:09:27,290 --> 00:09:29,150 moles because you're going to invert it again. 186 00:09:29,150 --> 00:09:31,230 So that gives us our answer in moles. 187 00:09:31,230 --> 00:09:33,450 And so finally our temperature-- and you've got 188 00:09:33,450 --> 00:09:35,490 to remember you've got to do it in kelvin. 189 00:09:35,490 --> 00:09:39,800 So 25 degrees Celsius-- let me right it over here-- 25 190 00:09:39,800 --> 00:09:44,160 degrees Celsius is equal to, you just add 273 to it, so 191 00:09:44,160 --> 00:09:52,300 this is equal to 298 kelvin. 192 00:09:52,300 --> 00:09:56,360 So times 298 kelvin. 193 00:09:56,360 --> 00:09:58,490 And now we just have to calculate this. 194 00:09:58,490 --> 00:09:59,740 So let's do that. 195 00:10:02,290 --> 00:10:04,270 So let me clear this out. 196 00:10:04,270 --> 00:10:10,010 So we have-- let me use my keyboard-- so 0.0313 197 00:10:10,010 --> 00:10:21,340 atmospheres times 4.25 times 10 to the fourth. 198 00:10:21,340 --> 00:10:24,340 That e just means times 10 to the fourth. 199 00:10:24,340 --> 00:10:27,220 That's just the way that it works on this calculator. 200 00:10:27,220 --> 00:10:39,310 And then divided by 0.082057 divided by-- actually, just to 201 00:10:39,310 --> 00:10:41,100 make it clear, let me show you that I'm dividing by this 202 00:10:41,100 --> 00:10:47,610 whole thing, so let me insert some parentheses right here. 203 00:10:50,730 --> 00:10:53,300 So in the denominator we also are multiplying by 298. 204 00:10:53,300 --> 00:10:55,285 And let me close the parentheses. 205 00:10:58,330 --> 00:11:02,270 And then we get 54.4. 206 00:11:02,270 --> 00:11:03,710 We only have three significant digits. 207 00:11:03,710 --> 00:11:10,850 So this is equal to 54.4 moles. 208 00:11:10,850 --> 00:11:13,580 And we could see this liters cancels out with that liters. 209 00:11:13,580 --> 00:11:15,300 Kelvin cancels out with kelvin. 210 00:11:15,300 --> 00:11:16,880 Atmospheres with atmospheres. 211 00:11:16,880 --> 00:11:18,880 You have a 1 over mole in the denominator. 212 00:11:18,880 --> 00:11:24,040 So then 1 over 1 over moles is just going to be moles. 213 00:11:24,040 --> 00:11:29,730 Now, this is going to be 54.4 moles of water vapor in the 214 00:11:29,730 --> 00:11:32,580 room to have our vapor pressure. 215 00:11:32,580 --> 00:11:36,070 If more evaporates, then more will condense-- we will be 216 00:11:36,070 --> 00:11:37,800 beyond our equilibrium. 217 00:11:37,800 --> 00:11:40,610 So we won't ever have more than this amount 218 00:11:40,610 --> 00:11:41,890 evaporate in that room. 219 00:11:41,890 --> 00:11:47,440 So let's figure out how much liquid water that actually is. 220 00:11:47,440 --> 00:11:48,550 Let me do it over here. 221 00:11:48,550 --> 00:11:59,170 So 54.4 moles-- let me write it down-- moles of H2O. 222 00:11:59,170 --> 00:12:00,386 That's going to be in its vapor form and 223 00:12:00,386 --> 00:12:01,780 its going to evaporate. 224 00:12:01,780 --> 00:12:04,270 But let's figure out how many grams that is. 225 00:12:04,270 --> 00:12:08,560 So what is the molar mass of water? 226 00:12:08,560 --> 00:12:10,110 Well, it's roughly 18. 227 00:12:10,110 --> 00:12:11,910 I actually figured it out exactly. 228 00:12:11,910 --> 00:12:16,600 It's actually 18.01 if you actually use the exact numbers 229 00:12:16,600 --> 00:12:18,880 on the periodic table, at least one that I used. 230 00:12:18,880 --> 00:12:28,120 So we could say that there's 18.01 grams of H2O for every 1 231 00:12:28,120 --> 00:12:30,490 mole of H2O. 232 00:12:30,490 --> 00:12:33,580 And obviously, you can just look up the atomic weight of 233 00:12:33,580 --> 00:12:36,470 hydrogen, which is a little bit over 1, and the atomic 234 00:12:36,470 --> 00:12:38,955 weight of oxygen, which is a little bit below 16. 235 00:12:38,955 --> 00:12:40,250 So you have two of these. 236 00:12:40,250 --> 00:12:43,530 So 2 plus 16 gives you pretty close to 18. 237 00:12:43,530 --> 00:12:47,990 So this right here will tell you the grams of water that 238 00:12:47,990 --> 00:12:51,760 can evaporate to get us to that equilibrium pressure. 239 00:12:51,760 --> 00:12:53,580 So let's get the calculator out. 240 00:12:53,580 --> 00:13:05,090 So we have the 54.4 times 18.01 is equal to 970-- well, 241 00:13:05,090 --> 00:13:07,650 we only have three significant digits-- so 900, if your round 242 00:13:07,650 --> 00:13:10,380 this 0.7, it becomes 980. 243 00:13:10,380 --> 00:13:17,180 So this is 980 grams of H2O needs to evaporate for us to 244 00:13:17,180 --> 00:13:19,160 get to our equilibrium pressure, 245 00:13:19,160 --> 00:13:20,540 to our vapor pressure. 246 00:13:20,540 --> 00:13:24,180 So let's figure out how many milliliters of water this is. 247 00:13:24,180 --> 00:13:27,090 So they tell us the density of water right here. 248 00:13:27,090 --> 00:13:33,500 0.997-- let me do this in a darker color-- 0.997 grams per 249 00:13:33,500 --> 00:13:34,920 millileter. 250 00:13:34,920 --> 00:13:39,370 Or another way you could view this is for everyone 1 251 00:13:39,370 --> 00:13:49,780 milliliter you have 0.997 grams of water 252 00:13:49,780 --> 00:13:52,810 at 25 degrees Celsius. 253 00:13:52,810 --> 00:13:55,200 So for every milliliter-- this is grams per milliliter-- we 254 00:13:55,200 --> 00:13:58,470 want milliliters per gram because we want this and this 255 00:13:58,470 --> 00:13:59,600 to cancel out. 256 00:13:59,600 --> 00:14:04,260 So we're essentially just going to divide 980 by 0.997. 257 00:14:04,260 --> 00:14:05,185 So what is that? 258 00:14:05,185 --> 00:14:06,860 Get the calculator out. 259 00:14:06,860 --> 00:14:16,760 So we have 980-- not cover up our work-- divided by 0.997 is 260 00:14:16,760 --> 00:14:21,580 equal to 980-- we'll just round this-- 983. 261 00:14:21,580 --> 00:14:25,930 So this is equal to 983. 262 00:14:25,930 --> 00:14:29,230 This and this canceled out, or that and that canceled out. 263 00:14:29,230 --> 00:14:32,620 So 983 milliliters of H2O. 264 00:14:32,620 --> 00:14:38,140 So we've figured out, using the Ideal Gas Law, that at 25 265 00:14:38,140 --> 00:14:44,090 degrees Celsius, which was 298 kelvin, that 983 milliliters 266 00:14:44,090 --> 00:14:47,520 of H2O will evaporate to get us to our 267 00:14:47,520 --> 00:14:50,730 equilibrium vapor pressure. 268 00:14:50,730 --> 00:14:53,590 Nothing more will evaporate, because beyond that if we have 269 00:14:53,590 --> 00:14:57,540 higher pressure than that, then you'll also have more 270 00:14:57,540 --> 00:14:58,930 vapor going to the liquid state. 271 00:14:58,930 --> 00:15:01,640 Because you'll have more stuff bouncing here. 272 00:15:01,640 --> 00:15:07,950 So if this much volume of water evaporates, we'll have 273 00:15:07,950 --> 00:15:11,020 the state where just as much is evaporating as just as much 274 00:15:11,020 --> 00:15:11,700 is condensing. 275 00:15:11,700 --> 00:15:16,350 So you will never get to a higher pressure than that at 276 00:15:16,350 --> 00:15:18,190 that temperature. 277 00:15:18,190 --> 00:15:21,320 So going back to the question, we figured out that 983 278 00:15:21,320 --> 00:15:23,990 milliliters of water will evaporate. 279 00:15:23,990 --> 00:15:26,940 The question was is that we placed 2 liters of water in an 280 00:15:26,940 --> 00:15:28,360 open container. 281 00:15:28,360 --> 00:15:31,920 So we just figured out that only 983 milliliters of that-- 282 00:15:31,920 --> 00:15:34,200 so that's a little bit less than a liter. 283 00:15:34,200 --> 00:15:40,460 So this is a little bit less than 1,000 milliliters, and 284 00:15:40,460 --> 00:15:41,960 this is 1 liter. 285 00:15:41,960 --> 00:15:47,050 So a little bit less than half of this will evaporate for us 286 00:15:47,050 --> 00:15:48,430 to get to our vapor pressure. 287 00:15:48,430 --> 00:15:50,370 So to answer our question-- will all of the water 288 00:15:50,370 --> 00:15:52,390 evaporate at 25 degrees Celsius? 289 00:15:52,390 --> 00:15:55,730 No-- if we're assuming the room is sealed-- well, no, all 290 00:15:55,730 --> 00:15:56,870 of it will not. 291 00:15:56,870 --> 00:16:00,980 Only a little bit less than half of it will.