00:01
So in this problem, we have a tube that looks like this, where we have different types of liquid, mercury, filled up like this, and water.
00:19
That's filled up in some ways that looks like this.
00:25
So this is water, and the dark parts in the bottom is mercury.
00:30
And the problem labeled these heights right here as h2, and then right here as h1.
00:48
Just for the sake of the problem, let's name this height h as well.
00:55
So we know that if it's at the same level, it should have the same pressure.
01:02
So let's define the pressures at this point p1 and then at this point p2.
01:14
Mercury filling up here, p2.
01:18
So let's look at what p1 is.
01:22
Well, p1 should just equal to the atmospheric pressure plus the pressure exerted by this amount of water, which should be the density of water times the gravitational acceleration, times the depth.
01:40
So in this case, the depth is h1 plus h plus h2, right, because it's the entire height of this water column.
01:52
And then what's p2? oh, same thing.
01:55
We have atmospheric pressure, plus in this case we have the density of water times the gravitational exploration times h plus the density of mercury times h2 here.
02:21
All right...