00:01
Alright, so there's two equations we know.
00:03
Let's start by writing those out.
00:05
One is planx equation, which states that the change in energy is equal to h times speed of light over lambda.
00:13
The other equation that we know is boresbondal equation, which states that delta e is equal to negative 2 .178 times 10 to the negative 18th times 1 over n final squared minus 1 over in initial squared.
00:46
So basically what we're going to do is just set these two equations equal to each other.
01:06
All right, and now let's go ahead and do number or letter a.
01:23
Okay.
01:24
So for a we're going from n equals 3 to n equals 2.
01:28
So what that's going to look like is final, if we're ending up at 2, 2 is going to be our final.
01:54
All right, and then we can plug in some constants for h and c.
02:01
And also, let's go ahead and rewrite this so that we make sure we're solving for a wavelength.
02:07
So we're going to have planx constant, which is h.
02:15
Struis times seconds, times the speed of light.
02:38
And that's going to equal wavelength...