00:01
Hi, everybody.
00:02
So we need to find the exit relative humidity.
00:07
So for that, we need to calculate the vapor pressure.
00:12
So we can find the vapor pressure of one as p30 plus p35 degrees minus p 30 degrees temperature of temperature of gas one, minus.
00:31
T30, minus t35, minus t30, okay.
00:40
And i'm going to put in the number.
00:43
So 4 .246 plus, oops, plus 5 .628, minus 4 .242 .8, minus 4 .244.
00:59
We only need one.
01:05
32 .5 minus 30 divided by 35 minus 30 equals 4 .937k pascels.
01:20
Okay.
01:21
And now we have a partial pressure of p1 v1, 5 pg1 equals 0 .85, 0 .85, and that's 85.
01:36
0 .85 times 4 .937 equals 4 .196, 45k pascels.
01:49
So we find the absolute humidity as 0 .622 times pv1 over p minus pv1 equals 0 .622, 4 .19645, 100 minus 4 .19645.
02:15
And this is going to equal to 0 .02724.
02:22
And so now we're going to do the same thing for state two with the gas.
02:29
So for this one is p15 degrees.
02:33
Plus p20 degrees minus p 15 degrees.
02:42
Tg1 minus t15 degrees over t20 degrees minus t15 degrees.
02:53
So we got 1 .705 plus 2 .339 minus 17.
03:01
Oops minus 1 .705 and it says 16 minus 15 divided by 20 minus 15 okay and this is going to equal to equal to 1 .8 318 k pascels okay and so for the volume of 2 we have 0 .8 3118 k pascels okay and so for the volume of 2 we have 0 .85 times 1 .8.
03:43
And i'll make that 8 here.
03:44
318.
03:46
Okay.
03:47
And it's going to be 1 .556 k -pascals.
03:53
And of course we can find absolute humidity here.
03:57
0 .622 times 1 .556, 100 minus 1 .556.
04:06
And we get 0 .0983.
04:13
Okay.
04:16
And we're going to keep on going because now we've got to do the continue equation.
04:24
Continuity equation.
04:26
So from that, we actually end up, we have m1 plus m2 equals m3.
04:38
And we're going to say m1.
04:40
Equals m2, which is 0 .1, and m3 equals 2.
04:46
And so from this, we have 1 plus 2, okay, and oops, it just equals 1.
05:04
There we go.
05:05
And from this, we have 0 .02724 plus 0 .093 divided by 2 .00845.
05:26
Okay.
05:28
And now we can do the energy equation.
05:32
And for that we have cp...