Q.A student measures the thickness of a human hair by looking at it through a microscope of magnification 100. He makes 20 observations and finds that the average width of the hair in the field of view of the microscope is 3.5 mm. What is the estimate on the thickness of hair?
🔒You're viewing a preview — the full solution, concept, methods & PYQ mapping are locked.
🔒 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 the microscope magnifies the true thickness by a factor of 100, so the measured average width must be divided by the magnification to recover the actual thickness.
Step 1: The average observed width in the magnified image is 3.5 mm.
Step 2: Magnification M=100 means the image is 100 times larger than the object. …
The problem is about measurement error estimation: the microscope magnifies the hair by 100×, so the actual thickness is the observed average divided by the magnification. The estimate is 3.5 mm/100=0.035 mm.
The key idea here is that the microscope magnifies the image — what the student sees in the field of view is 100 times larger than the real hair. So to get the actual thickness, you simply reverse the magnification: divide the measured average by 100.
This is not a statistics-heavy problem despite the 20 observations. The 20 readings help reduce random error in the observed width, but the conversion from observed to real is a straightforward scaling. The average observed width is already given as 3.5 mm, so the estimate of the true thickness is:
Actual thickness=MagnificationAverage observed width=1003.5 mm=0.035 mm
That’s the whole calculation. But let’s walk through it step by step to make the reasoning crystal clear.
-
Understand what magnification means.
A microscope with magnification 100 makes the object appear 100 times larger in the field of view. So if the real hair has thickness t, the image you see has thickness 100×t. The student measures this image thickness.
-
The student’s measurement is of the image, not the object.
He sees an average width of 3.5 mm in the microscope. That 3.5 mm is the size of the magnified hair. The real hair is 100 times smaller.
-
Reverse the magnification.
To find the real thickness t, divide the observed width by the magnification factor:
t=1003.5 mm=0.035 mm
- Why 20 observations matter (but don’t change the formula). …
Method: Direct Measurement with Magnification Correction
This is a single-measurement scaling problem — the microscope magnifies the actual thickness, so we simply divide the observed width by the magnification factor.
Steps
-
Identify the given data
- Magnification of microscope: M=100
- Average observed width in the field of view: Wobs=3.5 mm
- Number of observations: 20 (this tells us the average is reliable, but doesn't change the calculation)
-
Apply the magnification relation
- The microscope magnifies the actual thickness by a factor of 100.
- Therefore:
Actual thickness=MagnificationObserved width
- Calculate
t=1003.5 mm=0.035 mm
- Express in appropriate units
- 0.035 mm=3.5×10−2 mm …
Common Mistakes in Measurement Error Estimation (Microscope Magnification Problem)
This problem tests your understanding of magnification, significant figures, and error propagation — three concepts that frequently trip students up.
Mistake 1: Forgetting to Divide by Magnification
The error:
Students directly report 3.5 mm as the hair thickness, forgetting that the microscope magnifies the image by 100 times.
Why it’s wrong:
The measured 3.5 mm is the image size in the field of view. The actual hair thickness is:
Actual thickness=MagnificationImage size=1003.5 mm=0.035 mm
How to avoid:
Always ask: “Is this the real size or the magnified size?” Write the formula before plugging numbers:
Real size=MagnificationObserved size
Mistake 2: Ignoring Significant Figures / Precision
The error:
Reporting the answer as 0.035 mm without considering that the original measurement 3.5 mm has only 2 significant figures.
Why it’s wrong:
The division by 100 (an exact number) does not increase precision. The result should also have 2 significant figures:
0.035 mm(correctly written as 3.5×10−2 mm)
How to avoid:
- Count significant figures in the least precise measurement (here, 3.5 has 2 sig figs).
- The final answer must have the same number of sig figs.
- Use scientific notation to avoid ambiguity: 3.5×10−2 mm.
Mistake 3: Confusing Average Width with Error in Measurement
The error:
Students think “20 observations” implies they must calculate a standard deviation or error bar, and then report something like 0.035±0.001 mm.
Why it’s wrong:
The problem only gives the average width — no individual readings, no spread. Without the range or standard deviation, you cannot estimate random error. The question asks for the estimate of thickness, not an uncertainty interval.
How to avoid:
- Read carefully: “estimate” here means the best value (the mean after correction).
- Only compute error if the problem provides individual measurements or a stated uncertainty.
- If asked for “error estimation,” you need the spread — not just the number of observations.
Mistake 4: Misinterpreting “Magnification of 100”
The error:
Thinking magnification means the hair appears 100 times thinner (i.e., dividing the wrong way).
Why it’s wrong:
Magnification M=100 means the image is 100 times larger than the object. So:
Image size=M×Object size⇒Object size=MImage size
How to avoid:
- Remember: Magnification > 1 makes things look bigger. …
- 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: …
- 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. …
- 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. …
- AP EAPCET 2022Set ap-2022-07-11-FN1 markMCQQ.A concave lens of focal length 'f' produces an image x1 times the size of an object. The distance of the image from the lens is (A) x−1xf (B) xf (C) xx−1f (D) xx+1f
›Reveal solutionSolution
A concave (diverging) lens always forms a virtual, erect, diminished image. Combining the magnification relation m=v/u=1/x with the lens formula (using the sign convention where the concave lens's focal length is −f) gives the image distance ∣v∣=xx−1f.
Concept and Intuition
For any thin lens, magnification m=v/u and the lens formula is v1−u1=fsigned1. For a concave (diverging) lens of magnitude focal length f, the signed focal length is −f under the standard Cartesian sign convention.
Step-by-Step Solution
- From m=uv=x1, we get v=xu.
- Lens formula for a diverging lens (signed focal length =−f):
v1−u1=−f1
- Substitute v=u/x:
ux−u1=−f1⇒ux−1=−f1⇒u=−f(x−1)
- Then v=xu=x−f(x−1).
- The magnitude of the image distance from the lens is therefore ∣v∣=xx−1f. …
- AP EAPCET 2021Set eng-2021-08-24-AN1 markMCQQ.The focal length of a convex lens is 'f'. An object is placed at a distance 'x' from its first focal point. The ratio of the size of the real image to that of the object is ________ (A) x2f (B) fx2 (C) xf (D) fx
›Reveal solutionSolution
Newton's form of the lens formula measures object/image distances from the focal points rather than the lens centre; it gives magnification directly as f/x, avoiding the need for the usual u,v lens-formula algebra.
Concept and Intuition
The usual thin-lens formula v1−u1=f1 measures distances from the lens. Newton's alternative form measures the object's distance x from the FIRST focal point (beyond it, so the object is farther than f from the lens) and the image's distance x′ from the SECOND focal point. These satisfy the elegant relation xx′=f2, and the magnification works out to m=−f/x=−x′/f — a compact, symmetric result that is often faster than working with u and v directly.
Step-by-Step Solution
- Object distance from the lens is u=f+x (it sits a distance x beyond the first focal point). …
🎓Unlock everything free for 14 days
- ✓Full step-by-step solutions
- ✓Concept-first explanations
- ✓Methods, shortcuts & mistakes
- ✓PYQ mapping + timed mock tests
Full access for 14 days. No credit card required.