Intuition What this page is
The parent note gave you three worked examples. That's not enough — optics can throw a dozen distinct situations at you, and each one tests the sign rules differently. Here we first map every case that can occur , then solve one example per case so you never meet a scenario you haven't already seen. Read the parent Sign convention for mirrors and lenses first; everything here is pure substitution into its two boxed formulas.
Before anything, let us re-earn the two tools we will use over and over, so no symbol appears unexplained.
Definition Landmarks on the axis (define before we use them)
On a curved mirror or lens, three points sit on the principal axis:
Pole / optical centre — the point on the surface where the axis meets it; all distances start here .
Focus F — the point where rays parallel to the axis are brought together. Its distance from the pole is the focal length ∣ f ∣ .
Centre of curvature C — the centre of the sphere the mirror is a slice of. For a spherical mirror it sits at twice the focal distance , i.e. ∣ C ∣ = 2∣ f ∣ . We will write "C " as shorthand for "the point at distance 2∣ f ∣ ".
So "object beyond C " simply means the object is farther than 2∣ f ∣ from the pole. This is the only place C appears; keep it as "the 2 f point."
Every problem on this topic is one cell of this table. The last column names the example that clears it. (Recall from the definition above: C = the point at distance 2∣ f ∣ , with the same sign as f .)
#
Element
Case class (the "cell")
What is being stress-tested
Example
A
Concave mirror
Object beyond C (i.e. $
u
>2
B
Concave mirror
Object between F and pole ($
u
<
C
Concave mirror
Object exactly at F (u = f )
degenerate : image at infinity
Ex 3
D
Convex mirror
Any real object
always virtual, erect, diminished; v > 0
Ex 4
E
Plane mirror
Limiting case f → ∞
v = − u , virtual, same size
Ex 5
F
Convex lens
Object beyond 2 f
real, inverted, diminished
Ex 6
G
Convex lens
Object inside f (magnifier)
virtual, erect, magnified; v < 0
Ex 7
H
Convex lens
Object exactly at F (u = f )
degenerate : image at infinity
Ex 8
I
Concave lens
Any real object
always virtual, erect, diminished
Ex 9
J
Word problem
Real-world (rear-view mirror)
translate words → signs
Ex 10
K
Exam twist
Two-lens combination + magnification
chaining v → next u
Ex 11
Cells A–K together cover every quadrant of sign, both mirror and lens degenerate/limiting inputs (C, E, H), a word problem (J) and an exam twist (K) .
Reading Figure 1. The horizontal chalk line is the principal axis (our + x , pointing right). The tall curved chalk stroke on the right is the concave mirror , with its pole P (white dot) where it meets the axis. To the left of P sit two marked points: the yellow dot is the focus F and the blue dot is the centre of curvature C (the 2 f point). The pink arrow along the top shows the incident light travelling left→right (+x) . Three upright object arrows stand left of the pole — this is why every u below is negative:
yellow arrow, beyond C = Ex 1 (Cell A),
blue arrow, between F and P = Ex 2 (Cell B),
pink arrow, planted on F = Ex 3 (Cell C), whose reflected rays leave parallel (image at infinity).
The bottom labels remind you: everything left of P is negative , everything behind P (right) is positive .
Worked example Ex 1 — Cell A: concave mirror, object beyond C
A candle is 40 cm in front of a concave mirror of focal length 15 cm. Locate the image and describe it.
Forecast: In the figure this is the yellow arrow, sitting to the left of C (the 2 f = 30 cm point). Guess: real, inverted, smaller than the object. Where does v land?
Assign signs. u = − 40 cm, f = − 15 cm.
Why this step? In the figure the yellow object arrow is left of the pole → against incident light → negative; the concave focus F is also drawn left of the pole → negative.
Substitute into the mirror formula. v 1 = f 1 − u 1 = − 15 1 − − 40 1 = − 15 1 + 40 1 .
Why this step? We use the solved-for-v mirror form v 1 = f 1 − u 1 from the summary above.
Compute. Common denominator 120: − 120 8 + 120 3 = − 120 5 = − 24 1 , so v = − 24 cm.
Why this step? Combine the two fractions into one, then invert to get v itself.
Interpret the sign. v < 0 ⇒ (mirror rule) image lies in − x , in front of the mirror = real — the same left side as the yellow object.
Magnification. m = − u v = − − 40 − 24 = − 0.6 ⇒ inverted, 0.6 × size.
Why this step? Apply the mirror magnification rule; its sign reveals orientation, its size the scaling.
Verify: − 24 cm lies between F (15) and C (30) as it must for an object beyond C — consistent. Plug back: − 24 1 + − 40 1 = − 120 5 − 120 3 = − 120 8 = − 15 1 = f 1 . ✔
Worked example Ex 2 — Cell B: concave mirror, object inside F
A tooth is 6 cm in front of a dentist's concave mirror of focal length 10 cm. Find the image.
Forecast: This is the blue arrow in the figure, tucked between F and the pole. Concave mirror + object inside F is the "magnifying mirror" regime → guess virtual, erect, enlarged, so v > 0 .
Signs. u = − 6 cm, f = − 10 cm.
Why this step? The blue object arrow and the focus both lie left of the pole in the figure → both negative.
Substitute. v 1 = f 1 − u 1 = − 10 1 − − 6 1 = − 10 1 + 6 1 .
Why this step? Same solved-for-v mirror form v 1 = f 1 − u 1 .
Compute. Denominator 30: − 30 3 + 30 5 = 30 2 = 15 1 , so v = + 15 cm.
Why this step? Merge to one fraction and invert; the positive result already signals a switch of side.
Interpret. v > 0 ⇒ (mirror rule) image lies in + x , behind the mirror = virtual (the positive/right zone in the figure).
Magnification. m = − u v = − − 6 15 = + 2.5 ⇒ erect, 2.5 × magnified.
Why this step? The sign of m confirms "erect", matching the dentist-mirror expectation.
Verify: Positive m > 1 and erect matches the dentist-mirror purpose. Plug back: 15 1 + − 6 1 = 30 2 − 30 5 = − 30 3 = − 10 1 = f 1 . ✔
Worked example Ex 3 — Cell C: concave mirror, object AT the focus (degenerate)
Object placed exactly at the focus of a concave mirror, f = − 12 cm, so u = − 12 cm.
Forecast: In the figure this is the pink arrow, planted right on F . It is the boundary between the "real, beyond" and "virtual, inside" regimes. Guess: image nowhere finite — rays come out parallel.
Signs. u = − 12 cm, f = − 12 cm.
Why this step? Object and focus coincide, both left of the pole → both take the same negative value.
Substitute. v 1 = f 1 − u 1 = − 12 1 − − 12 1 = 0 .
Why this step? When u = f the two identical fractions cancel exactly, driving 1/ v to zero.
Interpret. v 1 = 0 ⇒ v = ± ∞ : the reflected rays are parallel , the image forms at infinity.
Why this step? 1/ v → 0 is the mathematical face of "no crossing point" — matching the pink object's parallel outgoing rays.
Verify: This is the reverse of "parallel rays converge to F ": an object at F must produce parallel rays (reversibility of light). u 1 = f 1 ⇒ v 1 = 0 exactly. ✔ Degenerate case handled.
Worked example Ex 4 — Cell D: convex mirror (always virtual)
A convex security mirror has f = + 20 cm. A person stands 60 cm away.
Forecast: Convex mirrors always give a virtual, erect, diminished image behind the mirror → v > 0 , 0 < m < 1 .
Signs. u = − 60 cm, f = + 20 cm.
Why this step? The object is still on the left → u < 0 ; but a convex focus lies behind the mirror = downstream of light → f > 0 .
Substitute. v 1 = f 1 − u 1 = 20 1 − − 60 1 = 20 1 + 60 1 .
Why this step? Solved-for-v mirror form; subtracting a negative u turns into an addition.
Compute. Denominator 60: 60 3 + 60 1 = 60 4 = 15 1 , so v = + 15 cm.
Why this step? One fraction, then invert; positive v confirms the image is behind the mirror.
Interpret. v > 0 ⇒ (mirror rule) image in + x , behind mirror = virtual .
Magnification. m = − u v = − − 60 15 = + 0.25 ⇒ erect, quarter size.
Why this step? The magnification rule pins down orientation (erect) and shrinkage (0.25 × ).
Verify: 0 < v < f and 0 < m < 1 — the fingerprint of every convex mirror. Plug back: 15 1 + − 60 1 = 60 4 − 60 1 = 60 3 = 20 1 = f 1 . ✔
Worked example Ex 5 — Cell E: plane mirror as the limit
f → ∞
A plane mirror is a mirror of infinite radius, so f → ∞ and f 1 → 0 . Object at u = − 25 cm.
Forecast: Everyone knows a plane mirror gives an image "as far behind as the object is in front," same size, erect. Let the formula prove it.
Take the limit. f 1 = 0 , so the mirror formula becomes v 1 + u 1 = 0 .
Why this step? A flat mirror is the R → ∞ end of the spherical family, so its focal term vanishes.
Solve. v 1 = − u 1 ⇒ v = − u = − ( − 25 ) = + 25 cm.
Why this step? With the focal term gone, v is forced to be the exact mirror-partner of u .
Interpret. v > 0 ⇒ (mirror rule) image 25 cm behind the mirror = virtual.
Magnification. m = − u v = − − 25 25 = + 1 ⇒ erect, same size.
Why this step? m = + 1 is the algebraic statement of "identical, upright mirror image."
Verify: v = − u and m = + 1 is exactly the everyday "mirror image" rule. Limiting case confirmed. ✔
Reading Figure 2. The horizontal chalk line is again the principal axis (+x) . The double-curved chalk shape at the centre is a convex lens , with its optical centre O on the axis. The two yellow dots mark the two foci F (left) and F ′ (right). The pink top arrow is the incident light (+x) . Crucially, the page is now split into two shaded bands, drawn straight from the "meaning of v " rule above:
the blue band on the left is the v < 0 zone — for a lens that is the virtual side (same side as the object). Ex 7's answer lands here.
the yellow band on the right is the v > 0 zone — for a lens that is the real (transmitted) side. Ex 6's answer lands here.
The blue object arrow stands on the left (u < 0 ). Because light passes through the lens, the real side is the right — the mirror image of the mirror case, and exactly why the lens formula carries a minus. In Ex 8 the object is pushed onto F and the image runs off the right edge to infinity.
Worked example Ex 6 — Cell F: convex lens, object beyond 2f
A slide is 30 cm to the left of a projector lens with f = + 10 cm. Find the image.
Forecast: Object beyond 2 f (which is 20 cm) → real, inverted, diminished, image landing in the yellow right-hand zone of the figure between f and 2 f .
Signs. u = − 30 cm, f = + 10 cm.
Why this step? The blue object arrow is left of the lens → u < 0 ; a convex lens converges rays into the yellow zone on the right → focus positive.
Lens formula. v 1 = f 1 + u 1 = 10 1 + − 30 1 .
Why this step? We use the solved-for-v lens form v 1 = f 1 + u 1 from the summary (the minus in v 1 − u 1 = f 1 became a plus when we moved u 1 across).
Compute. Denominator 30: 30 3 − 30 1 = 30 2 = 15 1 , so v = + 15 cm.
Why this step? Combine to one fraction and invert; positive v places the image in the yellow (real) zone.
Interpret. v > 0 ⇒ (lens rule) image in + x on the transmitted right side = real .
Magnification. m = + u v = − 30 15 = − 0.5 ⇒ inverted, half size.
Why this step? The lens magnification rule fixes orientation (inverted) and scale (half).
Verify: 15 cm lies between f = 10 and 2 f = 20 as required for an object beyond 2 f . Plug back: 15 1 − − 30 1 = 30 2 + 30 1 = 30 3 = 10 1 = f 1 . ✔
Worked example Ex 7 — Cell G: convex lens as a magnifier (object inside f)
A stamp sits 6 cm to the left of a magnifying lens with f = + 10 cm.
Forecast: Object inside the focus of a converging lens → the "magnifying glass" mode: virtual, erect, enlarged, image on the same side as the object , i.e. back in the blue v < 0 zone of the figure.
Signs. u = − 6 cm, f = + 10 cm.
Why this step? Object on the left → u < 0 ; the lens is convex → f > 0 . The object now sits between F and the lens.
Substitute. v 1 = f 1 + u 1 = 10 1 + − 6 1 = 10 1 − 6 1 .
Why this step? Same solved-for-v lens form v 1 = f 1 + u 1 ; because ∣ u ∣ < f the second term now dominates, so watch for a sign flip.
Compute. Denominator 30: 30 3 − 30 5 = − 30 2 = − 15 1 , so v = − 15 cm.
Why this step? Merge and invert; the negative result tells us the image jumped to the left (blue) zone — a virtual image.
Interpret. v < 0 ⇒ (lens rule) image in − x on the object's side (left) = virtual .
Magnification. m = + u v = − 6 − 15 = + 2.5 ⇒ erect, 2.5 × enlarged.
Why this step? The lens magnification rule confirms erect and enlarged — exactly what a magnifying glass should do.
Verify: Virtual + erect + enlarged is precisely what a magnifying glass does. Plug back: − 15 1 − − 6 1 = − 30 2 + 30 5 = 30 3 = 10 1 = f 1 . ✔
Worked example Ex 8 — Cell H: convex lens, object AT the focus (degenerate)
A collimator uses a convex lens with f = + 10 cm and an object placed exactly at its focus, so u = − 10 cm.
Forecast: This is the lens twin of Ex 3. In the figure the object arrow slides onto F itself; guess the emerging rays are parallel and the image runs off to infinity — the boundary between Ex 6 (real, right) and Ex 7 (virtual, left).
Signs. u = − 10 cm, f = + 10 cm.
Why this step? Object on the left → u < 0 ; convex lens → f > 0 ; here their magnitudes are equal because the object sits on F .
Substitute. v 1 = f 1 + u 1 = 10 1 + − 10 1 = 0 .
Why this step? Solved-for-v lens form; the two equal-and-opposite fractions cancel exactly, forcing 1/ v to zero.
Interpret. v 1 = 0 ⇒ v = ± ∞ : the transmitted rays leave parallel , the image forms at infinity (off the right edge of the figure).
Why this step? 1/ v → 0 is again the "no crossing point" signature — this is exactly how a collimator turns a point source into a parallel beam.
Verify: Reversibility: a source at F of a converging lens produces a parallel beam, the inverse of "parallel rays focus at F ′ ." u 1 = − f 1 ⇒ f 1 + u 1 = 0 exactly. ✔ Lens degenerate case handled.
Worked example Ex 9 — Cell I: concave lens (always virtual)
A concave lens has f = − 20 cm. An object is 30 cm to its left.
Forecast: Diverging lens → always virtual, erect, diminished, on the object side → v < 0 , 0 < m < 1 .
Signs. u = − 30 cm, f = − 20 cm.
Why this step? Object on the left → u < 0 ; a concave-lens focus lies upstream (left of the lens) → f < 0 .
Substitute. v 1 = f 1 + u 1 = − 20 1 + − 30 1 .
Why this step? Solved-for-v lens form; both terms are now negative, so the image is guaranteed to land on the left.
Compute. Denominator 60: − 60 3 − 60 2 = − 60 5 = − 12 1 , so v = − 12 cm.
Why this step? Combine and invert; the negative v confirms a virtual image on the object's side.
Interpret. v < 0 ⇒ (lens rule) image in − x , same side as object = virtual .
Magnification. m = + u v = − 30 − 12 = + 0.4 ⇒ erect, diminished.
Why this step? The lens rule fixes orientation (erect) and shrinkage (0.4 × ).
Verify: ∣ v ∣ < ∣ u ∣ and 0 < m < 1 — the signature of every diverging lens. Plug back: − 12 1 − − 30 1 = − 60 5 + 60 2 = − 60 3 = − 20 1 = f 1 . ✔
Worked example Ex 10 — Cell J: real-world (car rear-view mirror)
A car's convex rear-view mirror has f = + 2.0 m. A vehicle 10 m behind (i.e. 10 m in front of the mirror) is imaged. If the real vehicle is 1.5 m tall, how tall is its image and is it upright?
Forecast: Convex mirror → tiny, upright virtual image ("objects are closer than they appear").
Translate to signs. "10 m in front" ⇒ u = − 10 m; convex ⇒ f = + 2 m; height h = + 1.5 m.
Why this step? Front of the mirror is the object/left side → negative distance; convex focus is behind → positive.
Find v . v 1 = f 1 − u 1 = 2 1 − − 10 1 = 2 1 + 10 1 = 10 5 + 10 1 = 10 6 , so v = + 6 10 ≈ 1.667 m.
Why this step? Solved-for-v mirror form; positive v = image behind the mirror (virtual).
Magnification. m = − u v = − − 10 1.667 = + 0.1667 .
Why this step? The magnification rule turns the two distances into orientation + scale.
Image height. h ′ = m h = 0.1667 × 1.5 = + 0.25 m, i.e. 25 cm, positive ⇒ upright.
Why this step? h ′ = m h converts the abstract magnification into a real measurable height.
Verify: Positive small m , upright, diminished ⇒ matches the real mirror warning label. Units: metres throughout, h ′ in metres. ✔
Worked example Ex 11 — Cell K: exam twist, two thin lenses in a row
Two thin convex lenses L 1 (f 1 = + 10 cm) and L 2 (f 2 = + 20 cm) are placed 40 cm apart. An object is 15 cm to the left of L 1 . Find the final image. (See Combination of thin lenses .)
Forecast: L 1 makes an intermediate image; that image becomes the object for L 2 . Chase the signs carefully — the u for L 2 is measured from L 2 's optical centre.
Lens 1. u 1 = − 15 , f 1 = + 10 : v 1 1 = f 1 1 + u 1 1 = 10 1 + − 15 1 = 30 3 − 30 2 = 30 1 , so v 1 = + 30 cm (real, 30 cm right of L 1 ).
Why this step? Solve L 1 alone first with the solved-for-v lens form to locate the intermediate image.
Object for lens 2. The intermediate image is 30 cm right of L 1 ; the lenses are 40 cm apart, so it is 40 − 30 = 10 cm to the left of L 2 ⇒ u 2 = − 10 cm.
Why this step? Every distance for L 2 is measured from its own centre; still on L 2 's left, it acts as a normal real object → negative.
Lens 2. f 2 = + 20 : v 2 1 = f 2 1 + u 2 1 = 20 1 + − 10 1 = 20 1 − 20 2 = − 20 1 , so v 2 = − 20 cm.
Why this step? Apply the lens formula again to get the final image position from L 2 .
Interpret. v 2 < 0 ⇒ (lens rule) final image 20 cm to the left of L 2 = virtual (for L 2 ).
Total magnification. m = m 1 m 2 = u 1 v 1 ⋅ u 2 v 2 = − 15 30 ⋅ − 10 − 20 = ( − 2 ) × ( 2 ) = − 4 ⇒ inverted, 4 × .
Why this step? Magnifications of a lens chain multiply; the product's sign gives the final orientation.
Verify: m 1 = − 2 (inverted), m 2 = + 2 , product − 4 . Each stage reproduces 1/ f : stage 1 30 1 − − 15 1 = 10 1 ; stage 2 − 20 1 − − 10 1 = 20 1 . ✔
Recall Fast self-test: which cell?
An erect, magnified, virtual image from a single curved mirror — which element and where is the object? ::: Concave mirror, object inside the focus (Cell B).
A real, diminished, inverted image from a single lens — which lens and where? ::: Convex lens, object beyond 2 f (Cell F).
v 1 = 0 came out of your algebra for a mirror — what happened physically? ::: Object sat at the focus; image at infinity, rays parallel (Cell C).
v 1 = 0 came out for a convex lens — what device is this? ::: A collimator: object at F , parallel beam out, image at infinity (Cell H).
v > 0 for a lens vs v > 0 for a mirror — same physical meaning? ::: No: v > 0 always means "image in + x ", but for a lens that is real (right, transmitted) while for a mirror it is virtual (behind).
Before trusting an answer, ask: does the SIGN of v match the geometry I expected? Mirror real → v < 0 ; lens real → v > 0 ; every convex mirror and concave lens → tiny virtual erect image; object exactly at F → 1/ v = 0 (image at infinity). If the sign disagrees with the picture, you flipped a u or an f .