Q.Suppose while sitting in a parked car, you notice a jogger approaching towards you in the side view mirror of R=2 m. If the jogger is running at a speed of 5 m s−1, how fast the image of the jogger appear to move when the jogger is
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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) …
The side mirror is convex, R=2 m⇒f=+1 m. With object distance u=−d and the jogger approaching, d decreases so u increases: dtdu=+5 m s−1.
Differentiating v1+u1=f1 gives dtdv=(u−ff)2dtdu=(d+1)25 m s−1.
- (a) d=39 m: 16005=0.003125 m s−1
- (b) d=29 m: 9005≈0.00556 m s−1 …
A car's side-view mirror is convex with f=R/2=+1 m. Differentiating the mirror equation with respect to time gives image speed =(u−ff)2vobject. For a jogger approaching at 5 m s−1, the image speeds are (a) 3201 m s−1≈3.1×10−3 m s−1,
(b) 1801 m s−1≈5.6×10−3 m s−1,
(c) 801 m s−1=1.25×10−2 m s−1,
(d) 201 m s−1=5.0×10−2 m s−1 — the image speeds up sharply as the jogger gets closer.
Setting up
A side-view mirror is convex, R=2 m, so f=R/2=+1 m (positive by the sign convention, since a convex mirror's focus lies behind it).
Using the Cartesian sign convention, an object a distance d in front of the mirror has u=−d. As the jogger approaches, d decreases, so u (which is negative) is becoming less negative — i.e. u is increasing with time:
dtdu=+5 m s−1
(The jogger's own speed is 5 m s−1 toward the mirror, which is exactly a rate of increase of u.)
Differentiating the mirror equation
Start from
v1+u1=f1
Differentiate with respect to time (with f constant):
−v21dtdv−u21dtdu=0⇒dtdv=−u2v2dtdu
Since v=u−ffu, we have uv=u−ff, so
dtdv=(u−ff)2dtdu
Evaluating at each distance
With f=1 m and u=−d, u−f=−(d+1), so (u−ff)2=(d+1)21, and the image speed is (d+1)25 m s−1.
| Distance d | v=u−ffu | Image speed |
|---|---|---|
| 39 m | 0.975 m | 16005=3201≈3.1×10−3 m s−1 |
| 29 m | 0.967 m | 9005=1801≈5.6×10−3 m s−1 |
Method: Differentiation of the Spherical Mirror Equation
We use the mirror equation and differentiate it with respect to time to relate object velocity and image velocity.
Step 1: Identify mirror type and sign conventions
- Side view mirror of a car is convex.
- Radius of curvature R=+2 m (convex mirror → R positive).
- Focal length:
f=2R=22=1 m
- Sign convention:
- Object distance u is negative (object in front of mirror).
- Image distance v is positive (virtual image behind mirror).
Step 2: Write the mirror equation
v1+u1=f1
With u negative, let u=−x where x is the positive distance of jogger from mirror.
v1−x1=f1
Step 3: Solve for v in terms of x
v1=f1+x1=fxx+f
⇒v=x+ffx
Here f=1 m, so:
v=x+1x
Step 4: Differentiate with respect to time
We need dtdv (speed of image). Given dtdx=−5 m/s (jogger approaching → x decreasing).
Using quotient rule:
dtdv=(x+1)2(x+1)(1)−x(1)⋅dtdx
dtdv=(x+1)21⋅dtdx
Substitute dtdx=−5:
dtdv=−(x+1)25 m/s
The negative sign means the image moves towards the mirror (virtual image gets smaller). …
Common Mistakes with the Spherical Mirror Equation (and How to Avoid Them)
This problem is a classic application of the mirror formula combined with differentiation (rate of change). Here are the most frequent errors students make:
1. Confusing Sign Convention for Convex Mirrors
The Mistake:
Students treat the side-view mirror as a concave mirror or forget that for a convex mirror, the focal length (f) is negative.
Why it happens:
The formula f1=u1+v1 is the same for both, but the sign of f changes. A side-view mirror is convex (diverging).
How to avoid:
- Always identify the mirror type first.
- For a convex mirror:
- R is positive in magnitude, but f=−2R (by Cartesian sign convention).
- Here, R=2 m, so f=−1 m.
- Write the sign explicitly before substituting.
2. Forgetting that Object Distance (u) is Negative
The Mistake:
Plugging u=+39 m directly into the formula.
Why it happens:
In the Cartesian sign convention, distances measured against the incident light direction are negative. The object is in front of the mirror, so u is negative.
How to avoid:
- Always set u=−d where d is the actual distance.
- For this problem: u=−39, −29, −19, −9 m.
3. Using the Wrong Formula for Image Velocity
The Mistake:
Directly differentiating v=u−fuf without considering the sign of f or using v=u−ffu incorrectly.
Why it happens:
Students often memorise v=u−fuf but forget that this form assumes f is positive (concave). For convex mirrors, the correct derived relation is:
v=u−fuf
but with f negative, the denominator becomes u−(−∣f∣)=u+∣f∣, which changes the sign of the result.
How to avoid:
- Derive from the mirror formula each time:
v1=f1−u1
Then solve for v after substituting signed values.
- Then differentiate:
dtdv=−u2v2⋅dtdu
(This formula is sign-sensitive — use it carefully.)
4. Ignoring the Sign of dtdu
The Mistake:
Taking dtdu=+5 m/s when the jogger is approaching.
Why it happens:
If the jogger is moving toward the mirror, the distance ∣u∣ decreases, but u itself (which is negative) becomes less negative — so dtdu is positive.
How to avoid:
- Define u=−x, where x is the positive distance.
- Then dtdu=−dtdx.
- If the jogger approaches, dtdx=−5 m/s (since x decreases), so dtdu=−(−5)=+5 m/s.
- Key: dtdu=+5 m/s.
5. Forgetting That Image Velocity is Also Negative
The Mistake:
Reporting the speed as a positive number without realising the image moves toward the mirror (opposite direction to the object's approach).
Why it happens:
Students compute dtdv and get a negative value, then panic or drop the sign.
How to avoid: …
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