0:00
Hi there.
00:01
So for this problem, we have a laser beam with a wavelength of 600 nanometers.
00:12
And it is directed, well, it also gives us the, um, its diameter and its diameter is equal to, what are you going to call that? d and that diameter is equal to 12 centimeters that we know in meters is 0 .12 meters.
00:30
And this is directed to the moon.
00:35
And that is a distance that is also given, distance that we're going to call capital art, and that is 3 .82 times 10 to the 8 meters.
00:51
Now, the bean spreads only because of the disruption.
00:57
Now, the angular location for the central deprivation disk is given by the following equation.
01:05
We know that the sign of data is equal to 1 .22 the wavelength over the diameter d.
01:15
Now, where d obviously represents the being aperture.
01:21
Now, what we need to obtain is the diameter of the central disruption disk on the moon surface.
01:27
So we need to find what we are going to call the diameter d on capital d on the surface of the moon.
01:42
Now we are given the information about the distance to the moon that is capital art from the earth.
01:51
Now we note that the cone of light that this will produce in the moon has an apex angle that is 2 times theta...