Q.The photograph of a house occupies an area of 1.75 cm2 on a 35 mm slide. The slide is projected on to a screen, and the area of the house on the screen is 1.55 m2. What is the linear magnification of the projector-screen arrangement?
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🔒 Start your 14-day free trial to unlock the full solution →Concept understanding — Linear Magnification
Linear Magnification
Imagine looking at a tiny insect, 5 mm long, through a magnifying glass, and it appears 20 mm long. Linear magnification is simply the number that tells you how many times taller (or shorter) the image is compared with the object.
The Basic Definition
m=hohi
where hi is the image height (positive if upright, negative if inverted) and ho is the object height (always taken as positive, measured upward from the axis).
"Linear" means we compare lengths (heights), not areas. A magnification of 2 makes the image twice as tall, not twice as large in area.
Reading the Sign and the Size
| Sign of m | Meaning |
|---|---|
| Positive | Image is upright |
| Negative | Image is inverted |
| ∣m∣ | Meaning |
|---|---|
| >1 | Image is magnified |
| =1 | Image is the same size |
| <1 | Image is diminished |
Magnification from Distances — Mirrors vs Lenses
Using the New Cartesian sign convention (distances measured from the pole/optical centre; against the incident light is negative, along it is positive), magnification can also be written using object distance u and image distance v — but the formula differs for mirrors and lenses, and mixing the two up is the single most common mistake students make.
For spherical mirrors:
m=−uv
For thin lenses:
m=uv
There is no separate minus sign for lenses — the correct orientation comes out automatically once u and v are substituted with their signed values (a real object always has u negative).
Writing m=−v/u for a lens is a very common error. It happens to give the right numeric answer for a real, inverted image formed beyond 2F, but gives the wrong sign for a virtual, upright image (like a simple magnifying glass held close to an object) — always use m=v/u for lenses, with signed u and v.
Worked Example — Convex Lens
A 2 cm tall object stands 30 cm in front of a convex lens; a real image forms 60 cm on the other side. By the sign convention, u=−30 cm and v=+60 cm.
m=uv=−3060=−2
hi=m×ho=−2×2 cm=−4 cm …
Why this formula?
Linear Magnification: Why the Formula Holds
Let's build this from first principles — understanding why before what.
What is Linear Magnification?
Linear magnification (m) tells us how much larger or smaller an image is compared to the object, along the principal axis. It's defined as:
m=height of object (ho)height of image (hi)
But the real insight comes from geometry.
The Core Derivation: Why m=−uv
Step 1: Set up the geometry
Consider a concave mirror (the logic works for lenses too). Place an object of height ho at distance u from the mirror. The image forms at distance v with height hi.
Draw two rays from the top of the object:
- A ray parallel to the principal axis → reflects through the focus
- A ray through the centre of curvature → reflects back along itself
Where these rays meet is the top of the image.
Step 2: Use similar triangles
Look at the two triangles formed:
- Object triangle: base = u, height = ho (from principal axis to object top)
- Image triangle: base = v, height = hi (from principal axis to image top)
These triangles are similar because:
- Both have a right angle at the principal axis
- The ray angles are equal (law of reflection)
From similarity:
hohi=uv
Step 3: The sign convention
In optics, we use the Cartesian sign convention:
- Distances measured against incident light are negative
- Distances measured along incident light are positive
For a real image formed by a concave mirror:
- u is negative (object in front)
- v is negative (image in front)
- The image is inverted → hi is negative
So the ratio hohi is negative, while uv is positive (both negative). To match signs:
m=hohi=−uv
The negative sign tells us the image is inverted relative to the object.
Why This Matters for Exam Problems
| Condition | m value | What it means | …
The key idea is that linear magnification m is the square root of the areal magnification, because area scales as the square of the linear dimension.
- Areal magnification MA is the ratio of the image area to the object area:
MA=1.75 cm21.55 m2
Convert 1.75 cm2 to m2: 1.75×10−4 m2.
- So, …
Linear magnification is the ratio of image length to object length. Since area scales as the square of linear magnification, we take the square root of the area ratio. The linear magnification is approximately 94.1.
Why linear magnification from area?
When a slide is projected, every linear dimension of the image is magnified by the same factor m. That means if the original object has length L, the image has length mL. Area, being length × width, scales as m2 — because both dimensions get multiplied by m.
So if you know the area of the object on the slide and the area of the image on the screen, you can find m by taking the square root of the area ratio. This works because the shape is preserved (the house looks the same, just bigger).
A common mistake is to directly divide the screen area by the slide area and call that the linear magnification. That gives the area magnification, not the linear one. Always remember: m=AobjectAimage.
Step-by-step solution
-
Write down what’s given
Area on slide (object): Ao=1.75 cm2
Area on screen (image): Ai=1.55 m2
-
Convert units so they match
The slide area is in cm2, the screen area in m2. Linear magnification is a pure ratio, so we need both areas in the same unit.
1 m=100 cm, so 1 m2=(100)2 cm2=104 cm2.
Therefore:
Ai=1.55 m2=1.55×104 cm2
- Relate area magnification to linear magnification For a simple projection (no distortion), the area magnification MA is the square of the linear magnification m: MA=AoAi=m2 …
Method: Area-to-Linear Magnification Conversion
This method uses the fact that area magnification equals the square of linear magnification for a projector or lens system.
Steps
-
Identify the given areas
- Object area (on slide): Ao=1.75 cm2
- Image area (on screen): Ai=1.55 m2
-
Convert to consistent units
Since 1 m=100 cm,
1 m2=104 cm2
So,
Ai=1.55×104 cm2
- Relate area magnification to linear magnification Area magnification Marea=AoAi Linear magnification m satisfies:
Marea=m2
- Calculate linear magnification
m2=1.751.55×104
m2=1.7515500=8857.14 (approx) …
🧠 The Core Concept
Linear magnification (m) is the ratio of the linear dimensions (height or width) of the image to the object.
m=hohi
But here, you are given areas, not lengths.
Area magnification = m2 (since area scales as the square of linear dimensions).
So the correct approach is:
- Convert areas to the same units.
- Find area magnification.
- Take the square root to get linear magnification.
✗ Common Mistake #1: Treating area ratio as linear magnification
What students do:
They directly divide the areas:
m=1.75×10−41.55(wrong)
Why it’s wrong:
Area scales as (linear factor)2. Dividing areas gives area magnification, not linear magnification.
✓ How to avoid:
Always ask: “Am I comparing lengths or areas?”
If areas are given, remember:
Area magnification=m2
So:
m=AobjectAimage
✗ Common Mistake #2: Forgetting unit conversion
What students do:
They plug in 1.75 cm2 and 1.55 m2 without converting.
Why it’s wrong:
Magnification is a pure ratio — units must match.
1 m2=104 cm2, so 1.55 m2=1.55×104 cm2.
✓ How to avoid:
Convert both areas to the same unit (usually cm2 or m2) before forming the ratio.
✓ Correct Step-by-Step Solution
Step 1: Convert to same units
Aobject=1.75 cm2
Aimage=1.55 m2=1.55×104 cm2 …
Showing the 12 most recent of 20 on this concept.
- AP EAPCET 2026Set eng-2026-05-12-AN1 markMCQQ.A convex lens forms a real image and a virtual image of same size of an object placed separately at distances u1 and u2 respectively from the lens. Then the focal length of the lens is (A) 2u1u2 (B) (2u1+u2) (C) u1u2 (D) 2(u1+u2)
›Reveal solutionSolution
When a convex lens produces a real image and a virtual image of the same size from two different object positions u1,u2, its focal length is simply the average of the two object distances: f=(u1+u2)/2.
Concept and Intuition
A convex lens forms a real, diminished-or-magnified, inverted image when the object is beyond the focal length, and a virtual, magnified, erect image when the object is placed between the lens and the focus. "Same size" here means the two magnifications have equal magnitude but opposite sign (one inverted, one erect). Writing the lens equation for both cases in terms of a common magnification magnitude k and eliminating k reveals a clean linear relationship between u1, u2 and f — this is a standard, elegant optics result worth remembering.
Step-by-Step Solution
- Real image case (object at distance u1, using Cartesian sign convention so u1<0): magnification m1=−k (negative, inverted), with v1=−ku1. Substituting into v11−u11=f1 and simplifying gives ∣u1∣=kf(1+k).
- Virtual image case (object at distance u2, also u2<0, but nearer the lens than f): magnification m2=+k (positive, erect, and here k>1 since a convex lens's virtual image is always magnified), with v2=ku2. Substituting similarly gives ∣u2∣=kf(k−1).
- Add the two object-distance magnitudes: ∣u1∣+∣u2∣=kf(1+k)+kf(k−1)=kf[(1+k)+(k−1)]=kf(2k)=2f. …
- AP EAPCET 2026Set eng-2026-05-14-AN1 markMCQQ.A Convex lens forms a real image 4 cm long on a screen. When the lens is shifted to a new position without disturbing the object, again a real image is formed on the screen which is 16 cm tall. The length of the object must be (A) 4 cm (B) 8 cm (C) 12 cm (D) 20 cm
›Reveal solutionSolution
Two conjugate lens positions give magnifications that are reciprocals of each other, so the object length is the geometric mean of the two image lengths — 4×16=8 cm.
Concept and Intuition
When a convex lens is displaced between object and screen (keeping the object–screen separation fixed) and a sharp real image is found at two different lens positions, those two positions are conjugate: the object distance in one case equals the image distance in the other, and vice versa. Since magnification m=v/u, the two magnifications are reciprocals: m1=v1/u1 and m2=u1/v1=1/m1, so m1m2=1.
Step-by-Step Solution
- Let the object height be h0. The two image heights are h1=m1h0=4 cm and h2=m2h0=16 cm.
- Multiply: h1h2=m1m2h02.
- Since m1m2=1 (conjugate positions): h1h2=h02.
- h0=h1h2=4×16=64=8 cm. …
- AP EAPCET 2026Set eng-2026-05-13-AN1 markMCQQ.An object is placed at 10 cm from a lens and a real image is formed with magnification of 0.5. The lens is (A) Concave with focal length of 310 cm (B) Convex with focal length of 310 cm (C) Concave with focal length of 10 cm (D) Convex with focal length of 10 cm
›Reveal solutionSolution
This tests using magnification and the lens formula together, with correct sign convention, to identify both the type of lens and its focal length from an object distance and magnification.
Concept and Intuition
Using the Cartesian sign convention for lenses (distances measured from the optical centre; distances in the direction of incident light are positive), the magnification is m=v/u. A real image formed by a lens is always inverted relative to the object, which is captured by m being negative (since a real image has v with a sign opposite to what an erect, virtual image would have relative to u). Since the object distance u is always negative for a real object, a real image requires v and u to have a specific relation making m<0 overall — concretely, real images have v>0 (for a converging/convex lens producing a real image) while u<0, so m=v/u<0 automatically.
Step-by-Step Solution
- Object distance: u=−10 cm (object on the incoming side, standard convention).
- The image is real, so m is negative; magnitude given is 0.5, so m=−0.5.
- From m=v/u: v=mu=(−0.5)×(−10)=+5 cm.
- Since v>0, the image forms on the side opposite to the object — consistent with a real image formed by a converging (convex) lens (a diverging/concave lens can only form virtual, diminished, upright images for a real object, never a real image).
- Apply the lens formula v1−u1=f1: …
- COMEDK 2026Set 2026-A1 markMCQQ.An object placed 40 cm in front of a thin convex lens is moved to 60 cm from the lens. If the focal length of the lens is 30 cm the ratio of magnification of the image at the initial position to the final position is: (A) 3:2 (B) 2:3 (C) 1:3 (D) 3:1
›Reveal solutionSolution
Magnifications are ∣m1∣=3 at u=40 cm and ∣m2∣=1 at u=60 cm, so the ratio is 3:1 — option (D).
Lens formula v1−u1=f1 with f=+30 cm (object distances taken negative).
Initial position, u=−40 cm:
v1=301−401=1201 ⇒ v=120 cm,m1=uv=−40120=−3
Final position, u=−60 cm: …
- KCET 2025Set D-41 markMCQQ.The image formed by an objective lens of a compound microscope is (A) Real and diminished (B) Real and enlarged (C) Virtual and enlarged (D) Virtual and diminished
›Reveal solutionSolution
The object sits between fo and 2fo of the objective, which by the lens rules gives a real, inverted, enlarged image — the intermediate image that the eyepiece then acts on.
Step 1 — How a compound microscope is arranged.
It uses two converging lenses:
- The objective — short focal length fo, placed close to the specimen.
- The eyepiece — placed at the other end of the tube, used as a simple magnifier.
The object is deliberately placed just beyond the objective's focus, i.e.
fo<u<2fo
Step 2 — What such an object position gives.
Apply the standard convex-lens image table for an object between f and 2f: the image forms beyond 2f on the far side, and it is
- real (rays actually converge and cross — it can be caught on a screen),
- inverted,
- enlarged (∣m∣>1).
We can verify with the lens formula and the magnification relation. With v1−u1=fo1 and, say, fo=1 cm, u=−1.2 cm:
v1=11+(−1.2)1=1−0.833=0.167 ⇒ v=+6 cm
Positive v ⇒ real image on the far side. Magnification:
mo=uv=−1.26=−5
∣mo∣=5>1 (enlarged), and the minus sign says inverted.
Step 3 — Why it must be real. …
- TG EAPCET 2025Set eng-2025-05-02-FN1 markMCQQ.The total magnification produced by a compound microscope is 24 when the final image is formed at the least distance of distinct vision. If the focal length of the eyepiece is 5 cm, the magnification produced by the objective is (A) 4 (B) 4.8 (C) 120 (D) 6
›Reveal solutionSolution
The total magnification of a compound microscope is the product of the objective magnification and the eyepiece magnification. For the eyepiece used at the least distance of distinct vision (25 cm), its magnification is 1+feD. Given total magnification 24 and fe=5 cm, the objective magnification is 4.
Concept & Intuition
A compound microscope magnifies in two stages: the objective lens produces a real, enlarged image of the object, and the eyepiece then magnifies that image further. The total magnification M is simply the product:
M=mo×me
where mo is the linear magnification of the objective and me is the angular magnification of the eyepiece.
The eyepiece acts like a simple magnifier. When the final image is formed at the least distance of distinct vision (typically D=25 cm), the eyepiece’s magnification is given by:
me=1+feD
This formula comes from the fact that the eye sees the image at the near point, so the angular size is maximized.
We are told M=24 and fe=5 cm. So we can find me first, then solve for mo.
Step-by-step solution
- Identify the eyepiece magnification formula For a simple magnifier (or eyepiece) used with the final image at the near point D=25 cm:
me=1+feD
This is a standard result — the “1” accounts for the relaxed eye case being D/fe, and adding 1 gives the near-point case.
- Plug in the given focal length
me=1+525=1+5=6
So the eyepiece alone gives a magnification of 6.
- Use the total magnification relation M=mo×me⇒24=mo×6…
- AP EAPCET 2025Set eng-2025-05-22-AN1 markMCQQ.Images of same size are formed by a convex lens when an object is placed either at 20 cm or 10 cm distance from the lens. The focal length of the lens is (A) 12 cm (B) 40 cm (C) 18 cm (D) 15 cm
›Reveal solutionSolution
Two object distances giving equal-sized images on a convex lens means one image is real & magnified while the other is virtual & magnified by the same factor — this symmetry pins the focal length at 15 cm.
Concept and Intuition
A convex lens can form images of different character depending on where the object sits relative to f and 2f: beyond 2f the image is real, inverted, and diminished; between f and 2f it's real, inverted, and magnified; inside f it's virtual, erect, and magnified. Here, two DIFFERENT object distances (20 cm and 10 cm) give images of the SAME SIZE. Since these are close to the lens, it's plausible one produces a magnified real image and the other a magnified virtual image, of equal size but opposite orientation. Algebraically, requiring ∣m1∣=∣m2∣ with m=f/(u+f) forces the denominators to be equal in magnitude but opposite in sign, which directly gives f in terms of u1,u2.
Step-by-Step Solution
- Use the Cartesian sign convention: real object distances are negative. So u1=−20 cm, u2=−10 cm.
- Lens formula: v1−u1=f1⇒v=u+fuf.
- Magnification: m=uv=u+ff.
- Equal image sizes means ∣m1∣=∣m2∣: u1+ff=u2+ff⇒∣u1+f∣=∣u2+f∣.
- Since u1=u2, the only solution (other than the trivial equal case) is u1+f=−(u2+f)⇒u1+u2+2f=0. …
- TG EAPCET 2024Set eng-2024-05-10-FN1 markMCQQ.When an object of height 12 cm is placed at a distance from a convex lens, an image of height 18 cm is formed on a screen. Without changing the positions of the object and the screen, if the lens is moved towards the screen, another clear image is formed on the screen. The height of this image is (A) 4 cm (B) 6 cm (C) 8 cm (D) 10 cm
›Reveal solutionSolution
This is the classic “lens displacement” problem: for fixed object and screen distances, two lens positions produce a sharp image, and the product of the two image heights equals the square of the object height. The second image height is 8 cm.
The key idea is that when the object and screen are fixed, there are two positions of a convex lens that form a real image on the screen (provided the distance between object and screen is greater than 4 times the focal length). This is known as the displacement method for finding focal length. The two images are conjugate: one is magnified, the other diminished, and their heights multiply to give the square of the object height.
Why this works:
For a thin lens, the lens equation is f1=u1+v1, where u is object distance and v is image distance. If the total distance D=u+v is fixed, then u and v are the two roots of a quadratic. Swapping u and v gives the second lens position. Magnification m=v/u=hi/ho. So if the first image height is h1 and the second is h2, then h1h2=ho2.
-
Set up the given data.
Object height ho=12 cm.
First image height h1=18 cm (magnified, so m1>1).
The second image is formed when the lens is moved toward the screen — this swaps object and image distances, giving a diminished image.
-
Relate magnifications.
For the first position: m1=u1v1=hoh1=1218=1.5. …
-
- AP EAPCET 2024Set ap-2024-05-16-FN1 markMCQQ.If m1 and m2 (m1>m2) are the magnification for two position of the lens between the object and the screen, and 'd' is the distance between the two positions of the lens, the focal length of the lens is (A) dm1−m2 (B) dm1m2 (C) (m1−m2)d (D) (m1−m2)d
›Reveal solutionSolution
This tests the displacement method for measuring focal length: two lens positions between a fixed object and screen give reciprocal magnifications, and the focal length can be expressed purely via the magnifications and the displacement d between positions.
Concept and Intuition
In the displacement method, the object and screen (a fixed distance D apart) stay put while the lens is moved to two different positions, both giving a sharp image on the screen. By the principle of reversibility of light paths, the object and image distances simply swap between the two positions — so if the magnification is m1 at the first position, it becomes m2=1/m1 at the second. Combining this reciprocal relation with the thin lens equation lets us eliminate the object/image distances entirely and express f in terms of just d (the lens displacement) and the two magnifications.
Step-by-Step Solution
- At position 1: object distance u1, image distance v1, magnification m1=v1/u1.
- By reversibility, at position 2 the distances swap: u2=v1, v2=u1, so m2=v2/u2=u1/v1=1/m1.
- Displacement between positions: d=u2−u1=v1−u1=u1(m1−1), giving u1=m1−1d. …
- MHT-CET 2024Set pcm-2024-05-02-M1 markMCQQ.A plane mirror produces a magnification of (A) −1 (B) zero (C) +1 (D) +2
›Reveal solutionSolution
+1.
A plane mirror forms an image of the same size, erect: m=+1. …
- MHT-CET 2024Set pcm-2024-05-03-E1 markMCQQ.A convex lens of focal length ' f ' produces a real image whose size is ' n ' times the size of an object. The distance of the object from the lens is (A) nfn+1 (B) f(1−n1) (C) n+1nf (D) f(1+n1)
›Reveal solutionSolution
Real image means ∣v∣=n∣u∣; substituting into the lens equation gives u=f(1+1/n).
Let object distance magnitude be u; for a real image of magnitude n times, image distance v=nu.
Lens formula (magnitudes, real object–real image): v1+u1=f1 …
- MHT-CET 2024Set pcm-2024-05-03-M1 markMCQQ.A convex lens of focal length ' f ' m forms a real, inverted image twice in size of the object. The object distance from the lens in metre is (A) 0.5 f (B) 0.66 f (C) f (D) 1.5 f
›Reveal solutionSolution
Magnification 2 with real image. …
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