Object is at 2f.
So image will also be at 2f.
(I1).
Image(I2) of I1 will be 1 m behind mirror.
Now I2 will be object for lens. u = -3 m f = + 0.5 m
=
v =
= 0.6 m So total distance from mirror = 2 + 0.6 = 2.6 m and real image.
Object is at 2f.
So image will also be at 2f.
(I1).
Image(I2) of I1 will be 1 m behind mirror.
Now I2 will be object for lens. u = -3 m f = + 0.5 m
=
v =
= 0.6 m So total distance from mirror = 2 + 0.6 = 2.6 m and real image.
Resolving power of microscope
= Numerical aperture
is the refractive index of medium.
The focal length of the lens
Shift
Now
Now the object distancce
For critical angle
For greater wavelength or lesser frequency is less.
So, critical angle would be more, So, they will not suffer reflection and come out at angles less then
By Lens maker's formula for convex lens
for,
for
The refractive index is
Therefore, the minimum of three readings are required.
A telescope magnifies by making the object appearing closer.
We know that
But
can be
That is
is less than
But
will be less than
so
The given optical situation is depicted in the following ray diagram: In this case, the image forms 55 cm behind the convex mirror and then the reflection takes place due to the mirror image that forms at a distance (v) behind the mirror.
Now, this image acts as an object for lens and the final image forms at a distance of 20 m from the lens if the focal length of convex mirror is as follows:
cm