Q.An object is placed at
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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) …
Using the spherical mirror equation v1+u1=f1 with f=R/2=7.5 cm (concave, so f=−7.5 cm):
Case (i), u=−10 cm: v1=−7.51−−101=−301, so v=−30 cm (real, in front of mirror). m=−uv=−3 (inverted, enlarged). …
For a concave mirror with R=15 cm (f=7.5 cm), the mirror formula and magnification formula give: (i) at u=10 cm, image is real, inverted, at v=30 cm, m=−3;
(ii) at u=5 cm, image is virtual, erect, at v=15 cm behind the mirror, m=+3.
Setting up — the spherical mirror equation
The governing relation for any spherical mirror is
v1+u1=f1,f=2R
with the New Cartesian sign convention: distances are measured from the mirror's pole, with the direction of incident light taken positive. A real object placed in front of the mirror always has u negative, and a concave mirror has its focus in front of it, so f is also negative.
Finding the focal length
f=2R=215=7.5 cm⇒f=−7.5 cm (concave)
Case (i): object at 10 cm
Here u=−10 cm.
v1=f1−u1=−7.51−−101=−7.51+101=75−10+7.5=−301
v=−30 cm
The negative sign means the image forms in front of the mirror — a real image.
Magnification:
m=−uv=−(−10)(−30)=−3
The negative sign means the image is inverted, and ∣m∣=3 means it is magnified 3 times.
This matches the expected behaviour: the object (u=10 cm) lies between F (7.5 cm) and C (15 cm), so the image is real, inverted, and enlarged, beyond C — exactly what we found.
Case (ii): object at 5 cm
Here u=−5 cm.
v1=−7.51−−51=−7.51+51=37.5−5+7.5=151
v=+15 cm
The positive sign means the image forms behind the mirror — a virtual image.
Magnification: …
Method: Mirror Formula & Sign Convention (Cartesian)
This is the standard Cartesian sign convention method used in board exams. We'll apply the mirror formula and magnification formula step-by-step.
Step 1 — Write the given data with proper signs
For a concave mirror:
- Focal length f is negative: f=−2R
- Radius of curvature R=15 cm ⇒f=−215=−7.5 cm
Object distance u is always negative (object in front of mirror):
- Case (i): u=−10 cm
- Case (ii): u=−5 cm
Step 2 — Apply the mirror formula
Mirror formula:
f1=v1+u1
Rearrange for v:
v1=f1−u1
Case (i): u=−10 cm, f=−7.5 cm
v1=−7.51−−101=−7.51+101
Take LCM = 30:
=−304+303=−301
So:
v=−30 cm
Nature: v is negative → real image (in front of mirror).
Case (ii): u=−5 cm, f=−7.5 cm
v1=−7.51−−51=−7.51+51
Take LCM = 15:
=−152+153=151
So:
v=+15 cm
Nature: v is positive → virtual image (behind the mirror).
Step 3 — Find magnification
Magnification formula:
m=−uv
Case (i): v=−30, u=−10
m=−(−10)(−30)=−1030=−3
- ∣m∣>1 → enlarged
- m negative → inverted image
Case (ii): v=+15, u=−5
m=−(−5)(+15)=+515=+3
- ∣m∣>1 → enlarged …
Common Mistakes & How to Avoid Them — Partial Mirror Obstruction
This problem is about standard mirror formula application, not partial obstruction. The "partial mirror" idea often confuses students into thinking only part of the mirror is used — but the mirror formula remains unchanged regardless of which portion of the mirror is exposed.
Here are the most frequent errors students make:
1. Confusing Radius of Curvature (R) with Focal Length (f)
Mistake: Using R=15 cm directly in the mirror formula as f.
Why it happens: Students rush and don't recall the relation.
How to avoid: Always write:
f=2R=215=7.5 cm
Key point: For a concave mirror, f is negative by sign convention:
f=−7.5 cm
2. Sign Convention Errors (Most Common)
Mistake: Using u=+10 cm or u=+5 cm.
Why it happens: Students forget that object distance is always negative in the Cartesian sign convention (object is in front of the mirror).
How to avoid:
- Object is placed in front of mirror → u is negative
- For case (i): u=−10 cm
- For case (ii): u=−5 cm
Correct formula:
v1+u1=f1
3. Thinking "Partial Mirror" Changes the Formula
Mistake: Students believe that if only half the mirror is exposed, the image position changes.
Why it happens: Misunderstanding of "partial obstruction" concept.
How to avoid:
- Partial obstruction only reduces image brightness, not its position or nature
- The mirror formula works for any portion of the mirror
- Treat it as a full mirror for calculations
4. Incorrect Magnification Sign
Mistake: Writing m=−uv but forgetting to substitute signs correctly.
How to avoid:
- Always substitute u and v with their signs
- m negative → real, inverted image
- m positive → virtual, erect image
5. Not Checking Object Position Relative to Focus
Mistake: Applying the same logic for both cases without checking.
How to avoid: …
- GUJCET 2024Set 131 markMCQQ.For plane mirror focal length is ________ m. (A) ∞ (B) −1 (C) 0 (D) 1
›Reveal solutionSolution
A plane mirror is a sphere of infinite radius, so its focal length is infinite.
Concept. For any mirror f=R/2. A plane mirror has radius of curvature R→∞, hence …
- GSEB Higher Secondary Certificate (HSC) Examination 2023Set ANNUAL1 markMCQQ.Power of plane mirror is ___.(a) +1(b) infinity(c) 0(d) -1
›Reveal solutionSolution
Power = 1/f; a plane mirror has f = infinity, so its power is zero.
Optical power is P = 1/f (in metres). A plane mirror neither converges nor diverges parallel rays, s …
- GSEB Higher Secondary Certificate (HSC) Examination 2022Set ANNUAL1 markMCQQ.The radius of curvature of a concave mirror is 20 cm. If an object is placed 15 cm in front of this mirror, the image distance will be ______ cm.(a) -30(b) -28(c) -22(d) -32
›Reveal solutionSolution
Applying the mirror formula with the correct sign convention gives an image distance of -30 cm (real image, same side as the object).
For a concave mirror, f=−R/2=−20/2=−10 cm (sign convention: distances measured against incident light direction are negative).
Object distance: u=−15 cm.
Mirror formula: v1+u1=f1
…
- GUJCET 2020Set 071 markMCQQ.What is the type of nature of image formed for an object placed an axis of concave mirror between pole & centre? (A) Real, inverted & magnified (B) Virtual, erect & diminished (C) Real, inverted & diminished (D) Virtual, erect & magnified
›Reveal solutionSolution
[!TLDR]
Object between pole and focus of a concave mirror ⇒ image is virtual, erect and magnified.
Concept
Concave-mirror image formation (NCERT/GSEB ray optics): the only position giving a virtual, erect, magnified image is when the object is between the pole (P) and the focus (F). All positions from F outward give real, inverted images.
Solution …
- GSEB Higher Secondary Certificate (HSC) Examination 2019Set ANNUAL1 markMCQQ.For plane mirror, value of magnification m = 1, then its focal length f = ___.(a) zero(b) positive(c) negative(d) infinite
›Reveal solutionSolution
A plane mirror always gives m=+1 regardless of object distance, consistent with it being the limiting case of a spherical mirror with R→∞.
…
- GSEB Higher Secondary Certificate (HSC) Examination 2019Set ANNUAL1 markMCQQ.An object is placed at a distance of 25 cm on the axis of a concave mirror having focal length 20 cm. What will be the lateral magnification of an image?(a) 4(b) 2(c) -4(d) -2
›Reveal solutionSolution
Use the mirror formula 1/v+1/u=1/f, then m=−v/u, with the sign convention that distances measured against the incident light are negative.
Given u=−25 cm, f=−20 cm (concave mirror).
…
- GUJCET 2015Set C1 markMCQQ.The power of plane mirror is _____. (A) 0 (B) ∞ (C) 2D (D) 4D
›Reveal solutionSolution
[!TLDR] For a plane mirror f=∞, so P=1/f=0.
Concept
The power of a mirror or lens is P=f1 (with f in metres). Power measures the ability to converge or diverge light; a surface that neither converges nor diverges has zero power.
Solution …
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