Analyzing the Setup
Imagine you are standing in an optics lab, holding a concave lens. You place an object exactly at its principal focus. The question asks us to find two things: the exact distance where the image will form, and how much it will be magnified.
A concave lens is a diverging lens. It takes parallel rays of light and spreads them out. Because of this, it has a reputation for always forming virtual, erect, and diminished images for any real object. But let's prove this mathematically.
The Master Equation
To unlock the secrets of this optical system, we need our master tool: the
Lens Formula. It beautifully connects the object distance
u, the image distance
v, and the focal length
f through the relation:
v1−u1=f1
We also need the formula for linear magnification
m, which tells us how large the image is compared to the object. For lenses, it is simply the ratio of the image distance to the object distance:
m=uv
Applying Sign Conventions
Before we plug in the numbers, we must strictly follow the Cartesian sign convention. This is where many students make a silly mistake!
For a concave lens, the principal focus lies on the left side (the side from which light originates). Therefore, its focal length is taken as negative, so we use −f.
The object is also placed on the left side, exactly at the focus. This means the object distance u is also negative, giving us u=−f.
The Final Calculation
Now, let's substitute these values into our lens formula.
v1−−f1=−f1
Moving the terms around, we get:
v1=−f1−f1
v1=−f2
Flipping this over, we find the image distance:
v=−2f
The negative sign tells us that the image forms on the left side of the lens, exactly halfway between the optical centre and the focus. Since distance is a positive quantity, the distance is 2f.
Finally, let's calculate the magnification:
m=uv=−f−f/2=21
The magnification is +21. The positive sign confirms the image is erect and virtual, and the value 21 tells us it is exactly half the size of the original object. The physics perfectly matches the math!