Q.Use the mirror equation to deduce that:
[Note: This exercise helps you deduce algebraically properties of images that one obtains from explicit ray diagrams.]
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The Spherical Mirror Equation: From Intuition to Formula
Imagine you're standing in front of a concave mirror — the kind that makes your face look bigger when you're close, but flips everything upside down when you step far back. That change isn't magic; it's geometry. The spherical mirror equation is the single relationship that predicts exactly where an image will form, and whether it's real or virtual, for any spherical mirror.
The Core Idea
Every point on an object sends out light rays in all directions. A mirror redirects those rays. The mirror equation tells you: given the mirror's curvature and the object's distance, where will those rays meet again (or appear to meet)?
There are only three quantities you need:
- u — object distance (from the mirror's pole)
- v — image distance (from the mirror's pole)
- f — focal length (a property of the mirror's curvature)
The equation is:
v1+u1=f1
The power is in the sign convention, because every distance can point in one of two directions.
The Sign Convention (New Cartesian Sign Convention)
This is where most students slip. The equation works for all spherical mirrors — concave and convex — only if you follow the convention used throughout NCERT and CBSE:
- All distances are measured from the mirror's pole.
- The incident light is taken to travel left to right, so distances measured in that same direction (to the right) are positive, and distances measured against it (to the left) are negative.
- Heights above the principal axis are positive; heights below are negative.
Because a real object is always placed in front of the mirror (to the left, where the incident light originates), its distance u is always negative.
Under this convention, the focal length of a concave mirror is negative (its focus F sits in front of the mirror, on the same side as the object), and the focal length of a convex mirror is positive (its focus lies behind the mirror). This is one of the most frequently tested facts in CBSE board exams.
A very common mistake is writing f as positive for a concave mirror because "it converges light." Convergence tells you the type of mirror, not the sign — the sign comes purely from where the focus physically sits relative to the pole, under the convention above.
Where Does the Formula Come From?
For a concave mirror, parallel rays from a distant object converge at the focus, a point at (signed) distance f from the mirror. The derivation uses similar triangles from a ray diagram.
›Proof
Consider an object of height ho in front of a concave mirror. Draw the ray parallel to the axis: it reflects through the focus F. Draw the ray through the centre of curvature C: it strikes the mirror normally and reflects straight back on itself. These two reflected rays cross to form the image, of height hi.
From similar triangles formed by the ray through C:
hiho=R−vu−R
where R=2f is the radius of curvature (with the same sign convention as f).
From similar triangles formed by the ray through F:
hiho=fu−f
Equating the two ratios and simplifying (using R=2f) gives:
v1+u1=f1
What the Equation Tells You
Rearranging for v:
v=u−fuf
Because u is negative for a real object, and v takes the sign the geometry dictates:
- v negative → the image forms in front of the mirror → real image (can be projected on a screen).
- v positive → the image forms behind the mirror → virtual image.
For a concave mirror (f negative), using the magnitude of the object distance ∣u∣ measured from the pole:
- ∣u∣>2∣f∣ → real, inverted, diminished image between f and 2f
- ∣u∣=2∣f∣ → real, inverted, same-size image at 2f
- ∣f∣<∣u∣<2∣f∣ → real, inverted, magnified image beyond 2f
- ∣u∣=∣f∣ → image at infinity …
Why this formula?
Spherical Mirror Equation: Why the Formula Holds
The spherical mirror equation — also called the mirror formula — relates the object distance (u), image distance (v), and focal length (f) of a spherical mirror. Let's build the reasoning step by step.
1. The Key Formula
For a spherical mirror (concave or convex):
f1=u1+v1
Where:
- f = focal length (positive for concave, negative for convex)
- u = object distance from pole (always negative by sign convention)
- v = image distance from pole (sign depends on image location)
2. Why This Formula Holds — The Derivation
Step 1: Start with a ray diagram
Consider a concave mirror with:
- Pole P
- Centre of curvature C (radius R)
- Focus F (midpoint of PC, so f=R/2)
Take an object placed beyond C. Draw two rays from the object's tip:
- A ray parallel to the principal axis → reflects through F
- A ray through C → reflects back along itself
These rays meet at the image point.
Step 2: Use similar triangles
Let the object height be ho and image height be hi.
From the geometry of the ray through C:
- Triangle formed by object, C, and axis is similar to triangle formed by image, C, and axis.
This gives:
hiho=R−vu−R
(Here u and v are distances from P, with sign conventions applied later.)
Step 3: Use the parallel ray
From the ray parallel to the axis:
- Triangle formed by object, F, and axis is similar to triangle formed by image, F, and axis.
This gives:
hiho=fu−f
Step 4: Equate the two ratios
Since both ratios equal ho/hi:
R−vu−R=fu−f
Step 5: Substitute R=2f
For a spherical mirror, the focal length is half the radius of curvature:
R=2f
Substitute:
2f−vu−2f=fu−f
Step 6: Cross-multiply and simplify
Cross-multiply:
f(u−2f)=(u−f)(2f−v)
Expand:
fu−2f2=2fu−uv−2f2+fv
Cancel −2f2 on both sides:
fu=2fu−uv+fv
Bring all terms to one side:
0=fu−uv+fv
Rearrange:
uv=fu+fv
Step 7: Divide by uvf
Divide both sides by uvf:
f1=v1+u1
This is the mirror formula.
3. Why the Sign Convention Matters
The derivation above used distances as positive magnitudes. In actual problem-solving, we use the Cartesian sign convention:
- Distances measured against incident light are negative
- Distances measured along incident light are positive
For a concave mirror:
- u is negative (object in front)
- f is negative (focus in front)
- v is negative for real images (in front) …
Mirror equation v1+u1=f1; magnification m=−uv. Convention: concave f<0, convex f>0, real object u<0; v<0 is a real image (in front), v>0 a virtual image (behind).
(a) Concave, object between f and 2f (2f<u<f, all <0): v1=f1−u1. Reciprocating 2f<u<f gives f1<u1<2f1, so 2f1<v1<0: thus v<0 (real) and ∣v∣>2∣f∣ — real image beyond 2f.
(b) Convex (f>0, u<0): v1=f1+∣u∣1>0, so v>0 always — image always virtual.
(c) Convex: v=f+∣u∣f∣u∣<f, so 0<v<f (between pole and focus). m=∣u∣v=f+∣u∣f<1 — diminished. …
Applying the mirror equation v1+u1=f1 with the Cartesian sign convention reproduces all four image properties algebraically — no ray diagram needed.
Convention used: distances measured from the pole; real object u<0; concave mirror f<0, convex mirror f>0; a real image has v<0 (formed in front of the mirror), a virtual image has v>0 (behind). Magnification m=−uv; ∣m∣>1 enlarged, ∣m∣<1 diminished.
(a) Concave mirror, object between f and 2f
Here f<0 and the object lies between f and 2f: 2f<u<f (all negative). From the mirror equation,
v1=f1−u1.
Taking reciprocals of 2f<u<f (order reverses for negatives): f1<u1<2f1. Subtracting from f1,
2f1<v1<0.
So v1<0⇒v<0: the image is real. And v1>2f1 with both negative means ∣v∣>2∣f∣: the image lies beyond 2f.
(b) Convex mirror — always virtual
Now f>0 and u<0, so
v1=f1−u1=f1+∣u∣1>0⇒v>0
for every object position. A positive v means the image is behind the mirror — virtual, independent of where the object is.
(c) Convex mirror — diminished, between pole and focus …
Method: Algebraic Deduction Using the Mirror Equation
Method Name: Sign Convention–Based Algebraic Analysis
Steps:
- Write the mirror equation:
f1=u1+v1
- Apply the Cartesian sign convention:
- For concave mirror: f is negative (f<0)
- For convex mirror: f is positive (f>0)
- Object distance u is always negative (u<0)
- Image distance v: positive means real image, negative means virtual image
- Solve for v in terms of u and f:
v1=f1−u1
- Use the sign of v to determine real/virtual and magnification m=−uv to determine size and orientation.
(a) Concave mirror: object between f and 2f → real image beyond 2f
- Given: f<0, u is negative, and ∣f∣<∣u∣<2∣f∣
- From mirror equation:
v1=f1−u1
Since ∣u∣>∣f∣, ∣u∣1<∣f∣1, so v1 is negative → v is negative → real image
- Magnitude: ∣v∣>2∣f∣ because ∣v∣1=∣f∣1−∣u∣1 and ∣u∣<2∣f∣ gives ∣v∣1<2∣f∣1 → ∣v∣>2∣f∣
Result: Real image beyond 2f.
(b) Convex mirror always produces a virtual image
- Given: f>0, u<0
- Mirror equation:
v1=f1−u1=f1+∣u∣1>0
So v>0 → virtual image (since v positive means behind the mirror)
Result: Virtual image for any object position.
(c) Convex mirror: image diminished, between pole and focus
- From (b), v>0 and v1=f1+∣u∣1
- Since v1>f1, we get v<f → image lies between pole and focus
- Magnification: …
Common Mistakes with the Spherical Mirror Equation
Students often struggle with algebraic deductions from the mirror formula. Here are the most frequent errors and how to avoid them.
Mistake 1: Forgetting the Sign Convention
The Error:
Using u (object distance) as positive for concave mirrors or treating f as positive for convex mirrors.
Why It Happens:
Students memorise the formula f1=u1+v1 but ignore the Cartesian sign convention:
- Concave mirror: f is negative (f=−∣f∣)
- Convex mirror: f is positive (f=+∣f∣)
- Object distance u is always negative (object in front of mirror)
How to Avoid:
Always write the sign explicitly before substituting. For a concave mirror:
f=−∣f∣,u=−∣u∣
Mistake 2: Confusing the Range of u for Concave Mirrors
The Error:
For part (a), students substitute u=−f or u=−2f directly instead of using inequalities.
Why It Happens:
The problem asks to deduce that an object between f and 2f produces an image beyond 2f. Plugging exact values gives only boundary cases.
How to Avoid:
Use the inequality:
−2f<u<−f(since f is negative)
Then solve for v using:
v1=f1−u1
and show that ∣v∣>2∣f∣ and v is negative (real image).
Mistake 3: Assuming v is Always Negative for Concave Mirrors
The Error:
Thinking all images from concave mirrors are real (v negative).
Why It Happens:
Ray diagrams for concave mirrors show real images for objects beyond focus, but virtual images occur when the object is between pole and focus.
How to Avoid:
Check the sign of v from the formula:
- If v is negative → real image (in front of mirror)
- If v is positive → virtual image (behind mirror)
For part (d): object between pole and focus means ∣u∣<∣f∣. Substituting gives v>0 → virtual and enlarged.
Mistake 4: Misinterpreting "Diminished" for Convex Mirrors
The Error:
Stating that the image is diminished only for certain object positions.
Why It Happens:
Students recall that convex mirrors always give diminished images but fail to prove it algebraically.
How to Avoid:
Use magnification:
m=−uv
For convex mirrors, f>0, u<0, and v>0 (always virtual). Show that:
∣m∣=∣u∣v<1
because v<∣u∣ always holds for convex mirrors.
--- …
- KEAM 2026Set eng-2026-04194 marksMCQQ.A real object is placed at distance of f in front of a convex mirror of focal length f. The image will be formed at a distance (A) 2f (B) 8f (C) f (D) 4f (E) 2f
›Reveal solutionSolution
An object at distance f before a convex mirror of focal length f forms its image at f/2 behind the mirror.
Mirror equation: v1+u1=f1.
For a convex mirror f=+f; the real object is at u=−f.
v1=f1−u1=f1−−f1=f1+f1=f2. …
- KEAM 2026Set eng-2026-04214 marksMCQQ.An object placed at 10 cm in front of a concave mirror of focal length of 8 cm gives image of magnification of (A) 4 (B) 6 (C) 8 (D) 2 (E) 10
›Reveal solutionSolution
Mirror formula gives v=−40cm, magnification magnitude 4.
Using the mirror sign convention, u=−10cm, f=−8cm: …
- KEAM 2025Set eng-2025-04254 marksMCQQ.The distance of an object placed in front of a concave mirror of radius of curvature 24 cm that gives its magnification as 3 is (A) 8 cm (B) 16 cm (C) 12 cm (D) 24 cm (E) 32 cm
›Reveal solutionSolution
Radius 24 cm ⇒f=12 cm. A stated (positive) magnification of 3 means an erect, virtual, enlarged image, which occurs with the object inside the focus; solving the mirror relation gives the object 8 cm from the mirror.
Focal length f=2R=12 cm; with the mirror sign convention f=−12 cm.
Using m=f−uf and u=fmm−1. Taking the magnification as +3 (an erect, virtual, magnified image, as a concave mirror gives when the object lies between the pole and focus): …
- KEAM 2021Set eng-2021-P1-A14 marksMCQQ.An object is placed at 10 cm in front of a concave mirror. If the image is at 20 cm from the mirror on the same side of the object, then the magnification produced by the mirror is (A) 3 (B) −0.5 (C) −2 (D) 0.33 (E) −1
›Reveal solutionSolution
The magnification is −2.
Concept and Intuition
For mirrors, m=−uv. A real image formed on the same side as the object (in front of a concave mirror) is inverted and, being farther out, enlarged.
Step-by-Step Solution
- Sign convention: u=−10cm, v=−20cm (both in front).
- m=−uv=−−10−20=−2. …
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