00:01
So we can use the thin lens formula for part a.
00:05
We have 1 over do plus 1 over d .i is equal to 1 over f.
00:11
Now, interestingly, when we look at do, that's equal to 1 .5 times 10 to the power 11 meters, whereas the focal length is only 0 .1 meter.
00:26
So when we look at that do, what we can say is that 1 is almost zero so we can ignore that and therefore d .i would be equal to the focal length so d .i is equal to 0 .1 meter so the image is formed 10 centimeters or point one away from the magnifying glass.
00:50
Now the magnitude of the magnification is equal to d .i over d .o which is also equal to h .i.
00:58
Over h .o.
01:00
So, d .i.
01:01
Is 0 .1 divided by the distance from the sun, which is 1 .5 times 10 to the power 11.
01:15
That's equal to h .i.
01:17
Over each of the object, which is the diameter of the sun, 1 .39 times 10 to the power 9...