Q.Choose the correct alternative:
Concept understanding — Variation Of Gravity
Variation of Gravity: Why Your Weight Changes Even When You Don't
Imagine you step on a weighing scale at sea level in Mumbai, then carry that same scale to the top of Mount Everest. The scale would show a smaller number — you'd weigh less. But you haven't lost any mass. What changed?
The force pulling you down — gravity — is not constant everywhere on Earth. It varies. That's what we mean by variation of gravity.
The Core Idea
Gravity is the force with which the Earth pulls objects toward its centre. The strength of this pull depends on two things: the mass of the Earth and your distance from its centre. Since the Earth is not a perfect sphere and it spins, that distance and the effective pull change from place to place.
The acceleration due to gravity, denoted by g, is approximately 9.8m/s2 at sea level. But that's an average. The actual value can be slightly higher or lower depending on where you are.
Why Does Gravity Vary? Three Main Reasons
1. Altitude (Height Above Sea Level)
This is the most intuitive one. As you go higher, you move farther from the Earth's centre. Gravity follows an inverse-square law: double the distance, and the force becomes one-fourth.
The formula for g at a height h above the Earth's surface (where R is Earth's radius, about 6400 km) is:
gh=(R+h)2GM
For small heights compared to R, we can approximate:
gh≈g(1−R2h)
This means for every kilometre you go up, g decreases by roughly 0.003m/s2. That's why at the top of a tall mountain, you weigh about 0.5% less than at sea level.
2. Depth (Going Underground)
What happens if you go down a mine or into the Earth's crust? Intuition might say gravity increases because you're closer to the centre. But the opposite happens.
Inside the Earth, the mass above you pulls upward, partially cancelling the pull from below. For a uniform Earth, only the mass inside the sphere of radius r (your distance from the centre) contributes to gravity at that point.
gd=r2GM′
Where M′ is the mass of the sphere of radius r. If Earth had uniform density ρ, then M′=34πr3ρ, giving:
gd=34πGρr
This means gravity decreases linearly as you go deeper. At the centre of the Earth, g=0 — you'd be weightless, pulled equally in all directions.
This linear decrease assumes uniform density. The real Earth has a dense iron core, so the actual variation is more complicated — gravity actually increases slightly as you go down through the crust before eventually decreasing.
3. Rotation of the Earth (Latitude Effect)
The Earth spins once every 24 hours. This rotation creates a centrifugal force that acts outward, away from the axis of rotation. This force effectively reduces the weight you feel.
The effect is strongest at the equator (where the rotational speed is highest, about 1670 km/h) and zero at the poles (where you're on the axis of rotation).
The effective g at latitude ϕ is:
geff=g−ω2Rcos2ϕ
Where ω is Earth's angular speed (7.3×10−5rad/s) and R is Earth's radius.
At the equator (ϕ=0∘), the reduction is about 0.034m/s2 — roughly 0.35% of g.
| Location | Approximate g (m/s²) | Why? |
|----------|------------------------|------|
| Equator (sea level) | 9.78 | Fastest rotation + bulging equator |
| 45° latitude | 9.81 | Intermediate |
| North Pole | 9.83 | No rotation effect + closer to centre |
4. Shape of the Earth (Oblateness)
The Earth is not a perfect sphere. Because of its rotation, it bulges at the equator and flattens at the poles. The equatorial radius is about 21 km larger than the polar radius.
This means:
- At the poles, you're closer to the Earth's centre → stronger gravity
- At the equator, you're farther from the centre → weaker gravity
This shape effect combines with the rotation effect to give the latitude variation shown in the table above.
The Complete Picture
Putting it all together, the variation of gravity with latitude ϕ and height h is given by:
g(ϕ,h)=g0(1−R2h)(1−g0ω2Rcos2ϕ)
Where g0≈9.806m/s2 is the standard value at 45° latitude at sea level.
The variation of gravity is small — typically less than 0.5% across the Earth's surface. But it matters for precise measurements, satellite orbits, and even for defining the kilogram (since a spring scale calibrated in Mumbai would read differently in London).
A Quick Summary
| Factor | Effect on g | Why |
|---|---|---|
| Going up (altitude) | Decreases | Farther from Earth's centre |
| Going down (depth) | Decreases (linearly for uniform Earth) | Less mass below you |
| Moving to equator | Decreases | Rotation + bulge |
| Moving to poles | Increases | No rotation + closer to centre |
The key takeaway: gravity is not a fixed number. It's a local property that depends on where you are on (or inside) the Earth. The 9.8m/s2 you memorise is just a convenient average — the real story is richer, and now you know why.
"Variation Of Gravity derivation" and "Variation Of Gravity numerical problems" are two of the most common searches tied to this topic, and Variation Of Gravity is a core, NCERT-aligned topic from the Gravitation portion of the Class 11 Physics curriculum, and it is tested regularly in CBSE board exams as well as in JEE Main and NEET. Pairing this explanation with NCERT Physics textbook practice and previous years' questions is the surest way to lock the concept in before an exam.
Concept: Variation of Gravity — acceleration due to gravity g changes with altitude, depth, and depends only on the attracting mass (Earth), not on the test mass.
(a) With increasing altitude, distance from Earth’s centre increases, so g decreases.
(b) With increasing depth, mass above the point no longer contributes; for uniform density, g∝ distance from centre, so g decreases.
(c) g=GM/R2 — independent of the mass of the body, but depends on Earth’s mass. So g is independent of mass of the body.
(d) The formula −GMm(1/r2−1/r1) uses the exact inverse‑square law, while mg(r2−r1) assumes constant g (valid only for small r2−r1). Hence the first is more accurate.
- decreases.
- decreases.
- mass of the body.
- more.
Gravity decreases with altitude and with depth, depends only on Earth's mass (not the body's mass), and the inverse‑square formula for potential energy is more accurate than the constant‑g approximation.
The core idea
The acceleration due to gravity g is not a universal constant — it changes as you move away from or into the Earth. The reason is simple: gravity depends on distance from the centre of mass, and on how much mass is “below” you. For a spherical Earth of uniform density, we can derive exact expressions for g at any point.
1. Effect of altitude (height above surface)
At the surface, g=R2GM where R is Earth’s radius and M its mass.
At a height h above the surface, distance from centre is r=R+h. The gravitational acceleration is:
gh=(R+h)2GM
Since the denominator is larger, gh<g. So gravity decreases with increasing altitude.
For h≪R, you can approximate: gh≈g(1−R2h). This is handy in multiple‑choice problems.
2. Effect of depth (inside the Earth)
Assume uniform density ρ. At a depth d below the surface, your distance from the centre is r=R−d. Only the mass inside the sphere of radius r pulls you inward — the outer shell contributes zero net force (shell theorem).
Mass inside radius r: Mr=ρ⋅34πr3=M⋅R3r3.
So the acceleration at depth d is:
gd=r2GMr=R3GM⋅r=g⋅Rr
Since r<R, we have gd<g. Gravity decreases linearly with depth, reaching zero at the centre.
A common mistake is to think gravity increases inside the Earth because you’re “closer to the centre”. But less mass is pulling you — and the net effect is a decrease.
3. Dependence on mass of the body
Newton’s law: F=r2GMm. The acceleration of a body of mass m is a=F/m=r2GM. The m cancels out. So g is independent of the mass of the body — it depends only on Earth’s mass and distance.
g=r2GM
This shows g depends on M (Earth’s mass) and r, not on the falling object’s mass.
4. Accuracy of potential energy formulas
The exact gravitational potential energy difference between two points at distances r1 and r2 from Earth’s centre is:
ΔU=−GMm(r21−r11)
The approximate formula mg(r2−r1) assumes g is constant — which is only true when r2−r1≪R. The exact formula works for any separation. So the inverse‑square formula is more accurate.
| Formula | When valid | Accuracy |
|---------|-----------|----------|
| −GMm(r21−r11) | Always (for a spherical Earth) | Exact |
| mg(r2−r1) | Only for small height changes | Approximate |
- decreases.
- decreases.
- mass of the body.
- more.
Step 1 (a, altitude): At height h, distance from Earth's centre is R+h, so gh=(R+h)2GM<R2GM=g — gravity decreases with altitude.
Step 2 (b, depth): By the shell theorem, only the mass inside radius r=R−d contributes; for uniform density that mass scales as r3, giving gd=g⋅Rr, which decreases linearly with depth (falling to zero at the centre).
Step 3 (c, mass dependence): From F=r2GMm=ma⇒a=r2GM, the body's own mass m cancels — g depends only on Earth's mass M and the distance r, never on the mass of the falling body.
Step 4 (d, PE formula accuracy): The exact potential-energy difference is ΔU=−GMm(r21−r11), valid for any separation. The approximation mg(r2−r1) assumes g stays constant, which only holds when r2−r1≪R — so the exact inverse-square formula is the more accurate one.
Showing the 12 most recent of 28 on this concept.
- TG EAPCET 2026Set eng-2026-05-09-AN1 markMCQQ.A solid sphere rolls down without slipping on an inclined plane of angle of inclination 30∘. If the angle of inclination of the plane is increased to 45∘, then the percentage increase in the acceleration of the sphere is nearly (A) 73.2 (B) 41.4 (C) 21.2 (D) 36.6
›Reveal solutionSolution
For a rolling rigid body, acceleration depends on sinθ and the moment of inertia factor. The percentage increase in acceleration when θ goes from 30∘ to 45∘ is about 41.4%, matching option (B).
The key idea is that for pure rolling down an incline, the acceleration is not simply gsinθ (as for sliding without friction) but is reduced by a factor that depends on the body's moment of inertia. For a solid sphere, that factor is 75. So the acceleration is a=75gsinθ. When θ changes, only sinθ changes — the 75 factor stays constant. The percentage increase in acceleration therefore equals the percentage increase in sinθ itself.
Let's work it through.
- Acceleration of a rolling sphere For a rigid body of mass m, radius R, and moment of inertia I=kmR2 (where k=52 for a solid sphere), the acceleration down an incline of angle θ under pure rolling is
a=1+kgsinθ
For a solid sphere, k=52, so 1+k=57, giving
a=7/5gsinθ=75gsinθ
- Acceleration at θ=30∘
a30=75gsin30∘=75g⋅21=145g
- Acceleration at θ=45∘
a45=75gsin45∘=75g⋅21=725g
- Percentage increase The percentage increase from a30 to a45 is
a30a45−a30×100%=145g725g−145g×100%
Cancel 75g from numerator and denominator (or simply cancel 5g everywhere):
=2121−21×100%=(22−1)×100%=(2−1)×100%
Since 2≈1.4142, we get
(1.4142−1)×100%=0.4142×100%=41.42%
TipNotice that the 75 factor cancels out completely. The percentage increase depends only on sinθ, not on the shape of the rolling body. So for any object rolling without slipping, the percentage increase in acceleration when θ goes from 30∘ to 45∘ is (2−1)×100%≈41.4%.
Watch outA common mistake is to use a=gsinθ (the sliding case) and get (sin45∘−sin30∘)/sin30∘=(2/2−1/2)/(1/2)=2−1≈0.414 — which accidentally gives the same number! But the reasoning is wrong because the actual acceleration is smaller. The percentage increase ratio is the same here only because the inertia factor cancels; don't assume this always works for other angle changes or other physical quantities.
✓Final answerThe percentage increase in acceleration is approximately 41.4%, which corresponds to option (B).
- TG EAPCET 2026Set eng-2026-05-09-FN1 markMCQQ.Consider the following statements: Statement-I: When two quantities are multiplied, the relative error in the result is the sum of the relative errors in the quantities Statement-II: When two quantities are divided, the relative error in the result is the difference of the relative errors in the quantities The correct answer among the following is (A) Both statements I and II are correct (B) Both statements I and II are not correct (C) Statement I is correct, but statement II is not correct (D) Statement I is not correct, but statement II is correct
›Reveal solutionSolution
The relative error in multiplication adds, but in division it also adds (not subtracts), so Statement I is correct and Statement II is false. The correct option is (C).
Concept & Intuition
When we measure quantities, each has an uncertainty (error). The relative error is the ratio of the absolute error to the measured value. For a product or quotient, we want to know how these uncertainties combine. The key rule: relative errors always add when quantities are multiplied or divided. Why? Because division is just multiplication by a reciprocal, and the relative error of a reciprocal is the same as the original relative error (since dividing 1 by a number flips the absolute error proportionally). So subtracting errors would be a mistake — it could even make the total error seem smaller, which is impossible.
Step-by-step reasoning
-
Define relative error
For a quantity x with measured value xˉ and absolute error Δx, the relative error is xˉΔx. This is a dimensionless fraction, often expressed as a percentage.
-
Multiplication case (Statement I)
Let z=x⋅y. The absolute error in z is approximately
Δz≈∣y∣Δx+∣x∣Δy
(from calculus: dz=ydx+xdy). Dividing by z=xy gives
zΔz≈xΔx+yΔy
So relative errors add. Statement I is correct.
- Division case (Statement II) Let z=yx. The absolute error is approximately
Δz≈y1Δx+y2xΔy
(from dz=ydx−y2xdy; the minus sign is irrelevant for error magnitude because errors add in quadrature or worst-case as absolute values). Dividing by z=x/y yields
zΔz≈xΔx+yΔy
The relative errors add, not subtract. Statement II says they subtract — that is false.
-
Common pitfall
Watch outStudents often think the minus sign in the derivative dz=ydx−y2xdy means errors subtract. But errors are magnitudes; we add absolute values (or squares) because uncertainties can’t cancel — they always increase total uncertainty.
-
Conclusion
Only Statement I is correct.
✓Final answerThe correct option is (C).
ANSWER: C
-
- TG EAPCET 2026Set eng-2026-05-10-AN1 markMCQQ.The intensive variables among thermodynamic state variables internal energy U, volume V, pressure P, absolute temperature T and total mass M are (A) M, V (B) U, M (C) U, V (D) P, T
›Reveal solutionSolution
Intensive variables are independent of system size; among U, V, P, T, M, only pressure P and temperature T are intensive, so the correct choice is (D).
Concept & Intuition
Thermodynamic variables come in two flavors: extensive (scale with the amount of substance) and intensive (independent of system size). If you double the system, extensive quantities double; intensive ones stay the same. Internal energy U, volume V, and total mass M all clearly double when you take two identical systems and combine them — they are extensive. Pressure P and temperature T, however, remain unchanged when you merge two systems at the same P and T — they are intensive. The question asks for the pair that are both intensive.
Step-by-step reasoning
-
Identify the nature of each variable
- Internal energy U: If you have two identical blocks of matter, each with energy U, the combined system has energy 2U. So U is extensive.
- Volume V: Similarly, volumes add: two blocks of volume V give total volume 2V. Extensive.
- Pressure P: If two identical gas samples at pressure P are combined (e.g., by removing a partition), the pressure remains P — it does not double. Intensive.
- Temperature T: Two bodies at the same temperature T in contact stay at T; temperature does not add. Intensive.
- Total mass M: Mass is additive: two blocks of mass M give 2M. Extensive.
-
Check the options
- (A) M, V: both extensive → not the answer.
- (B) U, M: both extensive → not the answer.
- (C) U, V: both extensive → not the answer.
- (D) P, T: both intensive → this is the correct pair.
-
Confirm with a classic test
Imagine dividing a system into two equal halves. Intensive variables (like P and T) have the same value in each half as in the whole. Extensive variables (like U, V, M) are halved. Only option (D) passes this test for both variables.
Watch outA common mistake is to think that “total mass” is intensive because it’s a property of the material. But “total” is the clue: it scales with system size. Specific properties (like density or specific heat) are intensive; total mass is not.
TipA quick mnemonic: Intensive = “inside” the system doesn’t change with size; extensive = “extends” with size. Pressure and temperature are the two most familiar intensive variables in thermodynamics.
✓Final answerThe correct option is (D).
ANSWER: D
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- TG EAPCET 2026Set eng-2026-05-11-AN1 markMCQQ.The fundamental force that operates among all the objects in the universe is (A) Electromagnetic force (B) Strong nuclear force (C) Weak nuclear force (D) Gravitational force
›Reveal solutionSolution
The question asks which fundamental force acts among all objects in the universe. The answer is gravitational force, because it is the only one that is universal (affects everything with mass/energy) and has infinite range.
The key concept here is universality — a force that operates on every object, everywhere. The four fundamental forces (electromagnetic, strong nuclear, weak nuclear, and gravitational) differ in their range and the types of particles they affect. Only one of them is truly universal.
- Electromagnetic force acts between charged particles. While it has infinite range, it does not affect neutral objects (like neutrons or neutral atoms). So it is not universal among all objects.
- Strong nuclear force holds atomic nuclei together. It only acts over extremely short distances (about the size of a nucleus) and only between quarks (protons and neutrons). It does not affect electrons or distant objects.
- Weak nuclear force is responsible for certain types of radioactive decay. It also has a very short range and only affects particles like quarks and leptons in specific interactions — not all objects.
- Gravitational force acts between any two objects that have mass or energy. Since all objects in the universe possess mass (or energy, via E=mc2), gravity affects everything. Its range is infinite, and it never switches off. This makes it the only force that operates among all objects.
Watch outA common mistake is to pick electromagnetic force because it seems "everywhere" in daily life. But remember: neutral objects (like a neutron star or a dark matter particle) feel no electromagnetic force, yet they still feel gravity.
TipGravity is the weakest force, but it dominates on cosmic scales precisely because it is universal and has no cancellation (positive and negative charges cancel electromagnetism, but mass only adds).
✓Final answerThe correct option is (D).
ANSWER: D
- TG EAPCET 2026Set ap-2026-05-04-FN1 markMCQQ.Two blocks of masses 4.5kg and 5.5kg are connected to the two ends of a light inextensible string passing over a frictionless pulley fixed to a rigid support. At time t=0, the blocks are released from rest. The distance travelled by the larger block in a time t=4s is (Acceleration due to gravity =10ms−2) (A) 8 m (B) 4 m (C) 16 m (D) 32 m
›Reveal solutionSolution
The system is an Atwood machine with unequal masses; the net force gives a constant acceleration of 1m/s2, so in 4 seconds from rest the larger block travels 8m.
The problem is a classic Atwood machine: two masses connected by a light string over a frictionless pulley. The key insight is that the string is inextensible and the pulley is frictionless, so both blocks move with the same magnitude of acceleration — the heavier one goes down, the lighter one goes up. The net force driving the system is the difference in their weights, and the total mass being accelerated is the sum of the two masses.
Let’s work through it step by step.
- Identify the forces and the net driving force The heavier block (m2=5.5kg) wants to fall, the lighter block (m1=4.5kg) wants to rise. The weight of m2 is m2g downward, and the weight of m1 is m1g downward on its own side. But because they are connected, the net force that actually accelerates the whole system is the difference:
Fnet=m2g−m1g=(m2−m1)g
- Apply Newton’s second law to the whole system The total mass being accelerated is m1+m2. So:
(m1+m2)a=(m2−m1)g
Solve for acceleration a:
a=m1+m2(m2−m1)g
- Plug in the numbers m2=5.5kg, m1=4.5kg, g=10m/s2:
a=4.5+5.5(5.5−4.5)×10=101.0×10=1m/s2
So both blocks accelerate at 1m/s2 — the heavier one downward, the lighter one upward.
Watch outA common mistake is to think each block has its own independent acceleration. Because the string is inextensible, their accelerations are equal in magnitude. Also, do not forget to add the masses in the denominator — the net force accelerates the whole system, not just one block.
- Find the distance travelled by the larger block The larger block starts from rest (u=0) and moves with constant acceleration a=1m/s2 for t=4s. Using the kinematic equation:
s=ut+21at2
s=0+21×1×(4)2=21×16=8m
TipYou could also think of it as: in 4 seconds at 1m/s2, the average velocity is 2m/s (since vavg=20+4), giving s=2×4=8m. Same result, less algebra.
✓Final answerThe distance travelled by the larger block is 8m, which corresponds to option (A).
- TG EAPCET 2025Set eng-2025-05-02-AN1 markMCQQ.The ratio of times taken by a freely falling body to travel first 5m, second 5m, third 5m distances is (A) 1:2:3 (B) 1:2−1:3−2 (C) 1:3:5 (D) 1:2−1:3−2
›Reveal solutionSolution
For a freely falling body starting from rest, the times to cover successive equal distances are in the ratio 1:(2−1):(3−2). This follows from the relation s=21gt2 and subtracting cumulative times.
The key idea is that for uniform acceleration from rest, distance is proportional to the square of time. So the time to fall a total distance s is t∝s. To get the time for just the second 5 m segment, you subtract the time for the first 5 m from the time for the first 10 m. Similarly for the third segment.
Let’s work it through.
- Set up the relation For a body starting from rest under gravity (acceleration g), the distance fallen in time t is
s=21gt2⇒t=g2s.
So time is proportional to s.
- Time for the first 5 m Let t1 be the time to fall the first 5 m.
t1=g2×5=g10.
- Time for the first 10 m Let T2 be the time to fall the first 10 m (i.e., first two 5 m segments together).
T2=g2×10=g20.
Then the time for just the second 5 m segment, call it t2, is
t2=T2−t1=g20−g10=g10(2−1).
- Time for the first 15 m Let T3 be the time to fall the first 15 m.
T3=g2×15=g30.
Then the time for just the third 5 m segment, call it t3, is
t3=T3−T2=g30−g20=g10(3−2).
- Form the ratio The times t1:t2:t3 are
g10:g10(2−1):g10(3−2).
Cancelling the common factor 10/g, we get
1:(2−1):(3−2).
Watch outA common mistake is to think the times are in the ratio 1:2:3 because distances are in the ratio 1:2:3. But time is proportional to distance, not distance itself. Also, the times for successive equal segments are not the same as times for total distances.
TipThis ratio 1:(2−1):(3−2) is a classic result for any uniformly accelerated motion from rest. It’s worth remembering: the times for equal distances follow the pattern of differences of square roots.
✓Final answerThe correct option is (D).
ANSWER: D
- TG EAPCET 2025Set ap-2025-04-29-AN1 markMCQQ.The fundamental force in nature which operates among heavier elementary particles only is (A) Strong nuclear force (B) Electromagnetic force (C) Gravitational force (D) Weak nuclear force
›Reveal solutionSolution
The strong nuclear force is the only fundamental force that acts exclusively on heavier elementary particles (hadrons like protons and neutrons), binding the atomic nucleus together.
The question asks which fundamental force operates only among heavier elementary particles. To answer, we need to recall the four fundamental forces of nature and their domains of action.
-
Gravitational force acts between all objects with mass or energy — it is universal, not restricted to heavier particles. It is the weakest force at the particle scale.
-
Electromagnetic force acts between all charged particles — electrons, protons, ions, etc. It is also universal for charged matter, not limited to heavier particles.
-
Weak nuclear force is responsible for certain types of radioactive decay (like beta decay). It acts on both quarks and leptons (including light particles like electrons and neutrinos), so it is not exclusive to heavier particles.
-
Strong nuclear force is the force that binds quarks together inside protons and neutrons, and holds the nucleus together. It acts only on particles called hadrons — which are the heavier elementary particles made of quarks (protons, neutrons, pions, etc.). It does not act on leptons (like electrons) or photons.
Watch outA common mistake is to think the weak nuclear force also acts only on heavy particles. But the weak force acts on all fermions, including light leptons like electrons and neutrinos — so it is not exclusive to heavier particles.
Thus, the strong nuclear force is the only fundamental force whose action is confined to heavier elementary particles (hadrons).
✓Final answerThe correct option is (A) Strong nuclear force.
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- TG EAPCET 2024Set ap-2024-05-08-FN1 markMCQQ.A body of mass 3kg is thrown vertically upward from the ground with a velocity of 10ms−1. If the maximum height reached by the body is 4.7m, then the loss of energy due to air resistance is (Acceleration due to gravity =10ms−2) (A) 9J (B) 18J (C) 30J (D) 47J
›Reveal solutionSolution
The problem asks us to find the energy lost due to air resistance when a body is thrown upwards. We calculate the initial kinetic energy and the potential energy gained at the maximum height. The difference between these two values represents the energy lost to air resistance, which is 9J.
When a body is thrown vertically upward, its initial kinetic energy is gradually converted into gravitational potential energy as it rises. In an ideal scenario, where there is no air resistance or any other non-conservative force, the total mechanical energy (kinetic + potential) of the body remains constant. This means that the initial kinetic energy would be entirely converted into potential energy at the maximum height.
However, in reality, forces like air resistance act against the motion. Air resistance is a non-conservative force, meaning it dissipates mechanical energy, usually converting it into heat and sound. Therefore, when air resistance is present, the final potential energy achieved at the maximum height will be less than the initial kinetic energy. The difference between the initial kinetic energy and the potential energy at the maximum height represents the energy lost due to the work done by air resistance.
We can express this using the work-energy theorem for non-conservative forces:
Initial Mechanical Energy + Work done by non-conservative forces = Final Mechanical Energy
KEi+PEi+Wnc=KEf+PEf
In this problem:
- The body starts from the ground, so initial potential energy PEi=0.
- At the maximum height, the body momentarily stops, so final kinetic energy KEf=0.
- The work done by non-conservative forces (Wnc) is negative, representing the energy lost due to air resistance. Let's call the magnitude of this loss Eloss. So, Wnc=−Eloss.
Substituting these into the equation:
KEi+0−Eloss=0+PEf
KEi−Eloss=PEf
Eloss=KEi−PEf
This equation tells us that the energy lost is simply the difference between the initial kinetic energy and the potential energy gained at the maximum height.
-
Calculate the initial kinetic energy of the body.
The body is thrown upward with an initial velocity. Its kinetic energy at the start is given by the formula KE=21mv2.
KE=21mv2
Given:
Mass m=3kg
Initial velocity u=10ms−1
Initial Kinetic Energy (KEi) =21×3kg×(10ms−1)2
KEi=21×3×100J
KEi=150J
-
Calculate the potential energy of the body at its maximum height.
As the body rises, its kinetic energy is converted into gravitational potential energy. The potential energy at a certain height is given by PE=mgh.
PE=mgh
Given:
Mass m=3kg
Acceleration due to gravity g=10ms−2
Maximum height reached h=4.7m
Potential Energy at maximum height (PEf) =3kg×10ms−2×4.7m
PEf=30×4.7J
PEf=141J
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Determine the loss of energy due to air resistance.
The initial kinetic energy is the total energy supplied to the body at the start. If there were no losses, this entire energy would be converted into potential energy. However, since the actual potential energy gained is less than the initial kinetic energy, the difference must be the energy lost to air resistance.
Energy lost due to air resistance (Eloss) =KEi−PEf
Eloss=150J−141J
Eloss=9J
✓Final answerThe loss of energy due to air resistance is 9J.
- TG EAPCET 2024Set ap-2024-05-08-FN1 markMCQQ.In Geiger-Marsden experiment, if the initial speed of α particle is doubled, then the closest distance of approach of the α particle from the gold nucleus (Assume α particle is projected straight towards the gold nucleus) (A) becomes doubled (B) becomes quadrupled (C) becomes half (D) becomes one-fourth
›Reveal solutionSolution
The closest distance of approach is inversely proportional to the kinetic energy of the alpha particle. Doubling the speed quadruples the kinetic energy, so the distance becomes one-fourth. The correct option is (D).
The Geiger-Marsden experiment (Rutherford's gold foil experiment) is fundamentally about energy conservation. When an alpha particle is fired straight at a gold nucleus, it slows down as it approaches because of the strong electrostatic repulsion between the positively charged alpha particle and the positively charged gold nucleus. At the point of closest approach, the alpha particle momentarily comes to rest — all its initial kinetic energy has been converted into electrostatic potential energy.
This is a pure energy conversion problem. No forces other than the Coulomb repulsion do work, so mechanical energy is conserved. The key insight: the distance of closest approach r0 is found by equating the initial kinetic energy to the electrostatic potential energy at that distance.
Let's work through it step by step.
- Write the energy conservation equation. At the start, far from the nucleus, the alpha particle has kinetic energy K=21mv2 and negligible potential energy. At the closest distance r0, its speed is zero, so all energy is potential:
21mv2=4πϵ01r0(2e)(Ze)
Here 2e is the charge of the alpha particle, Ze is the charge of the gold nucleus (Z=79), and m is the mass of the alpha particle.
- Solve for r0. Rearranging gives:
r0=4πϵ0121mv22Ze2=4πϵ01mv24Ze2
The important thing is the dependence on speed: r0∝v21.
- Apply the change. If the initial speed is doubled, v→2v, then:
r0′∝(2v)21=4v21=41r0
The new distance is one-fourth of the original.
Watch outA common mistake is to think r0∝1/v because kinetic energy is 21mv2 and you might forget the square. Always write the full energy equation — the v2 in the denominator is unmistakable.
TipYou don't need the actual values of Z, e, or ϵ0 for this kind of reasoning. The proportionality r0∝1/v2 is all you need. This is a hallmark of many "distance of closest approach" problems in electrostatics.
✓Final answerThe closest distance of approach becomes one-fourth, so the correct option is (D).
- TG EAPCET 2024Set eng-2024-05-09-FN1 markMCQQ.A body is falling freely from the top of a tower of height 125 m. The distance covered by the body during the last second of its motion is x % of the height of the tower. Then x is (Acceleration due to gravity =10 ms−2) (A) 9 (B) 36 (C) 25 (D) 49
›Reveal solutionSolution
The key is to find the total time of fall using s=21gt2, then compute the distance in the last second as the difference between total distance and distance covered in (t−1) seconds, and finally express that as a percentage of the tower height. The result is x=36, so option (B).
We start with the concept: for a freely falling body starting from rest, the distance covered in any time interval is given by the equations of motion under constant acceleration. The "last second" distance is tricky because it depends on the total time of fall. Once we know that time, we can subtract the distance covered in all but the last second from the total height.
- Find the total time of fall. The tower height is h=125 m, g=10 m/s², initial velocity u=0. Using h=21gt2:
125=21⋅10⋅t2⇒125=5t2⇒t2=25⇒t=5 seconds.
- Distance covered in the first 4 seconds (i.e., all but the last second).
s4=21g(4)2=21⋅10⋅16=80 m.
- Distance covered in the last second (the 5th second). This is the total height minus the distance covered in the first 4 seconds:
last second distance=125−80=45 m.
- Express this as a percentage of the tower height.
x=12545×100=1254500=36.
TipA quick check: the distance covered in the nth second of free fall from rest is g(n−21). For n=5, that gives 10×4.5=45 m — same result, no subtraction needed.
Watch outA common mistake is to think the last second distance is simply 21g(1)2=5 m, but that would only be true if the body fell for exactly one second total. Always find the total time first.
✓Final answerThe correct option is (B).
ANSWER: B
- TG EAPCET 2024Set eng-2024-05-11-FN1 markMCQQ.A body of mass ‘m’ and radius ‘r’ rolling horizontally with a velocity ‘V’, rolls up an inclined plane to a vertical height gV2. The body is (A) a sphere (B) a circular disc (C) a circular ring (D) a solid cylinder
›Reveal solutionSolution
The key idea is that the maximum height reached by a rolling body depends on its moment of inertia via energy conservation. The given height gV2 corresponds to a body with k2/r2=1, which is a circular ring.
Concept and Intuition
When a body rolls without slipping, its total kinetic energy is the sum of translational kinetic energy 21mV2 and rotational kinetic energy 21Iω2, where ω=V/r for rolling. As it climbs the incline, this total kinetic energy converts entirely into gravitational potential energy mgh. The height h therefore depends on the moment of inertia I: a larger I means more rotational energy, so less height for the same initial speed. The problem gives a specific height; we can solve for the required I and match it to the shape.
Step-by-step solution
- Write the energy conservation equation Initial total kinetic energy = final gravitational potential energy at maximum height h:
21mV2+21Iω2=mgh.
For rolling without slipping, ω=V/r, so:
21mV2+21I(rV)2=mgh.
- Factor out 21mV2 Let I=mk2, where k is the radius of gyration. Then:
21mV2(1+r2k2)=mgh.
- Cancel m and solve for h
h=2gV2(1+r2k2).
- Plug in the given height The problem states h=gV2. Substitute:
gV2=2gV2(1+r2k2).
Cancel gV2 (nonzero):
1=21(1+r2k2).
- Solve for r2k2 Multiply both sides by 2:
2=1+r2k2⇒r2k2=1.
- Identify the body
The condition k2/r2=1 means the moment of inertia is I=mr2. This is exactly the moment of inertia of a circular ring (or thin hoop) about its central axis.
- Sphere: k2/r2=2/5
- Circular disc / solid cylinder: k2/r2=1/2
- Circular ring: k2/r2=1
TipA quick check: if the body were sliding (no rotation), h=V2/(2g). The given height is twice that, so the rotational energy equals the translational energy — that happens only when I=mr2, i.e., a ring.
Watch outA common mistake is to forget the rotational kinetic energy and assume h=V2/(2g), which would incorrectly suggest a sliding object. Always include rotation for a rolling body.
✓Final answerThe correct option is (C).
ANSWER: C
- TG EAPCET 2024Set eng-2024-05-11-FN1 markMCQQ.The maximum distance between the transmitting and receiving antennas is D. If the heights of both transmitting and receiving antennas are doubled, then the maximum distance between the two antennas is (A) 2D (B) D2 (C) 4D (D) 2D
›Reveal solutionSolution
The maximum line-of-sight distance between two antennas depends on the square root of the antenna heights. Doubling both heights multiplies the distance by 2, so the new distance is D2.
Concept & Intuition
This problem is about radio horizon — the maximum distance at which two antennas can have a direct line-of-sight, assuming the Earth is a smooth sphere. The key formula comes from geometry: the distance to the horizon from a height h (ignoring atmospheric refraction) is approximately 2Rh, where R is the Earth's radius. For two antennas at heights ht and hr, the total line-of-sight distance is the sum of their individual horizons:
D=2Rht+2Rhr
If both heights are doubled, each horizon distance increases by a factor of 2, so the total also scales by 2.
Step-by-step reasoning
- Recall the standard formula for maximum line-of-sight distance between two antennas of heights ht (transmitter) and hr (receiver) over a spherical Earth:
D=2Rht+2Rhr
where R is the Earth's radius. (This assumes standard atmospheric refraction is already accounted for in an effective Earth radius, but the scaling remains the same.)
-
Apply the given condition: both heights are doubled. So new heights are ht′=2ht and hr′=2hr.
-
Compute the new distance D′:
D′=2R(2ht)+2R(2hr)=2⋅2Rht+2⋅2Rhr
Factor out 2:
D′=2(2Rht+2Rhr)=2D
- Interpret the result: The new maximum distance is D multiplied by 2, not doubled or quadrupled. This makes physical sense — horizon distance grows slowly with height because of the square-root relationship.
Watch outA common mistake is to think doubling height doubles the distance (option A) or quadruples it (option C). But the square-root dependence means the effect is weaker: only a 2 factor.
TipIf both antennas were at the same height h, then D=22Rh. Doubling h gives D′=22R(2h)=222Rh=2⋅(22Rh)=2D. The same factor appears.
✓Final answerThe correct option is (B).
ANSWER: B
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