Q.At what depth below the Earth's surface does the acceleration due to gravity reduce to exactly 50% of its value at the surface? Take R=6400 km.
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.
Set g(1−d/R)=0.5g and solve for d.
d=3200 km (exactly half the Earth's radius).
Requiring gd=0.5g in the exact depth formula gd=g(1−d/R),
g(1−Rd)=0.5g⟹1−Rd=0.5⟹Rd=0.5
So d=0.5R=0.5×6400 km=3200 km.
The acceleration due to gravity is exactly 50% of its surface value at a depth of 3200 km, i.e. exactly half the Earth's radius.
Set the depth formula equal to 0.5g, cancel g from both sides, and solve the resulting linear equation for d/R.
- Confusing this with the analogous altitude question (Example 3), which needs a different, squared formula and gives a different depth/height for the same 50% reduction.
- Forgetting to convert the ratio d/R=0.5 back into an actual distance using R=6400 km.
Showing the 12 most recent of 22 on this concept.
- CBSE 2026Set ANNUAL1 markQ.The value of an acceleration of a freely falling body is ______.
›Reveal solutionSolution
A freely falling body (falling under gravity alone, no air resistance) accelerates at the constant value g ≈ 9.8 m/s^2 downward.
Near the Earth's surface, every freely falling object experiences the same acceleration g, independent of its mass, given approximately by g = GM/R^2 where G is the universal gravitational constant, M is Earth's mass and R is Earth's radius. Its standard value is g ≈ 9.8 m/s^2 (often rounded to 9.81 m/s^2 or taken as 10 m/s^2 for quick calculations), always directed vertically downward.
✓Final answerg ≈ 9.8 m/s^2, directed vertically downward.
- CBSE 2026Set ANNUAL1 markMCQQ.Correct relation between g and density (ρ) of earth is:(a) g = (3/4)Rρ(b) g = (4/3)πRρ(c) g = (4/3)πGRρ(d) g = (3/4)πGRρ
›Reveal solutionSolution
g=GM/R2 combined with M=34πR3ρ (sphere of density ρ) gives g=34πGRρ.
The acceleration due to gravity at the Earth's surface is:
g=R2GM
Modeling the Earth as a uniform sphere of radius R and density ρ, its mass is:
M=ρ×Volume=ρ×34πR3
Substituting:
g=R2G×34πR3ρ=34πGRρ
✓Final answer(c) g=34πGRρ.
- CBSE 2026Set ANN1 markQ.At the centre of Earth, the value of g is ________ .
›Reveal solutionSolution
At the Earth's centre the acceleration due to gravity is zero, because no mass is enclosed below that point to produce a net gravitational pull.
Inside a uniform sphere, only the mass contained within the radius r at which the body sits contributes to the gravitational field (the outer shells exert no net force on a point inside them). The value of g at depth d below the surface is
g_d = g (1 - d/R),
where R is the Earth's radius. At the centre the depth d = R, so
g_centre = g (1 - R/R) = g x 0 = 0.
Physically, at the centre the mass is distributed symmetrically all around, and the pulls in all directions cancel, giving zero net gravity.
✓Final answerZero.
- CBSE 2025Set ANNUAL1 markMCQQ.Acceleration due to gravity for the earth is maximum at (A) equator (B) pole (C) centre (D) none of these
›Reveal solutionSolution
Acceleration due to gravity is maximum at the poles and minimum at the equator.
Two effects reduce g as one moves from the pole to the equator:
- Earth's shape: earth is an oblate spheroid, slightly flattened at the poles and bulging at the equator, so the equatorial radius is larger than the polar radius. Since g∝1/R2, a larger radius at the equator means smaller g.
- Earth's rotation: the effective gravity felt is reduced by the centrifugal effect of rotation, geff=g−ω2Rcos2λ, which is largest (most reduction) at the equator (λ=0) and zero at the poles (λ=90∘).
Both effects make g largest at the poles. (At the centre, g=0, since it lies inside the earth with equal pull from all sides.)
✓Final answer(B) pole.
- CBSE 2025Set ANNUAL1 markMCQQ.A body weighs 200 N on the surface of the earth. How much will it weigh half way down to the center of the earth?(a) 100 N(b) 50 N(c) 200 N(d) 400 N
›Reveal solutionSolution
Unlike the inverse-square fall-off above the surface, gravity inside a uniform earth decreases linearly with depth — so at half the radius, both g and the weight are exactly halved.
Assuming the earth is a uniform sphere of radius R, the acceleration due to gravity at depth d below the surface is:
gd=g(1−d/R)
'Half way down to the centre' means d=R/2:
gd=g(1−(R/2)/R)=g(1−1/2)=g/2
Weight at that depth:
Wd=mgd=m(g/2)=Wsurface/2=200/2=100 N
✓Final answerWeight halfway down to the centre =100 N — option (a).
- CBSE 2025Set sz1 markMCQQ.At what depth below the surface of earth the value of 'g' is same as that of height of 5 km? (A) 10 km (B) 7.5 km (C) 5 km (D) 2.5 km
›Reveal solutionSolution
Setting the depth expression equal to the height expression gives d = 2h = 10 km.
At height h above the surface: gh=g(1−R2h).
At depth d below the surface: gd=g(1−Rd).
For the two to be equal: 1−Rd=1−R2h⇒d=2h.
With h = 5 km, d=2×5=10 km.
✓Final answerThe correct option is (A) 10 km.
- CBSE 2024Set ANNUAL1 markMCQQ.If the earth starts rotating from east to west instead of west to east about its axis, then the value of g on equator (A) will increase (B) will decrease (C) will be same (D) will be zero
›Reveal solutionSolution
Reversing earth's spin direction doesn't change g at the equator, since the correction term depends on ω2.
At the equator, the effective (measured) value of gravity is reduced from the true gravitational value by the centrifugal effect of the earth's rotation: geq=gtrue−ω2R, where ω is the earth's angular speed and R its equatorial radius.
Reversing the direction of rotation (east-to-west instead of west-to-east) changes the sign of ω as a vector, but ω2 (which is what appears in the centrifugal term) stays exactly the same. So geq is unaffected.
✓Final answer(C) will be same.
- CBSE 2024Set ANNUAL1 markMCQQ.Where will it be profitable to purchase one kilogram of sugar?(a) At poles(b) At equator(c) At 45 degree latitude(d) At 40 degree latitude
›Reveal solutionSolution
Because g is minimum at the equator (due to Earth's bulge and rotation), buying sugar 'by weight' there gets you more actual mass for the same weight reading — so it is profitable to buy at the equator.
A spring balance measures WEIGHT (W = mg), not mass directly. Earth's value of g is slightly larger at the poles and slightly smaller at the equator (due to Earth's equatorial bulge and the effect of its rotation reducing effective gravity at the equator).
If you buy '1 kg' of sugar going by a spring-balance weight reading, you're really buying an amount whose weight (mg) matches a fixed reading. Since g is smaller at the equator, a LARGER mass m is needed to produce the same weight reading there compared to at the poles. So at the equator, a '1 kg-weight' worth of sugar actually corresponds to a slightly greater mass of sugar — making it more profitable to purchase there.
✓Final answer(b) At equator.
- CBSE 2024Set SET-AP55001 markMCQQ.At height h above the earth's surface, the value of g changes by the same amount as it does at depth x inside the earth (both x and h are much smaller than the earth's radius) when:(a) x = h(b) x = h/2(c) x = 2h(d) x = h^2
›Reveal solutionSolution
For small h, R: g at height h is g(1 − 2h/R); g at depth x is g(1 − x/R). Equating the fractional drops gives x = 2h.
At height h above Earth's surface (h << R):
g_h = g / (1 + h/R)^2 ≈ g(1 − 2h/R)
so the fractional decrease is Δg_h/g ≈ 2h/R.
At depth x below Earth's surface (x << R):
g_x = g(1 − x/R)
so the fractional decrease is Δg_x/g = x/R.
For the two changes to be equal:
2h/R = x/R
⟹ x = 2h
This is a standard result: going a certain height up decreases g about twice as fast (fractionally) as going the same distance down, so you need to go down twice as far to match the same drop.
✓Final answerThe correct option is (c) x = 2h.
- CBSE 2024Set SET-NDP60001 markMCQQ.The value of 'g' is maximum at:(a) At surface of earth(b) At height(c) At depth(d) At center
›Reveal solutionSolution
g is maximum at the earth's surface and decreases both with height above it and with depth below it.
Above the surface, at height h, gh=g(1−R2h) (for h≪R) — this is always less than the surface value g. Below the surface, at depth d, gd=g(1−Rd) — this too is always less than g, and g falls all the way to zero at the centre of the earth (d=R). So moving away from the surface in either direction (up or down) reduces g; the surface itself is where g takes its maximum value (for a uniform-density spherical earth, ignoring the small effect of the earth's rotation and non-uniform density in reality).
✓Final answerThe correct option is (a) At surface of earth.
- CBSE 2024Set ANNUAL1 markMCQQ.Value of acceleration due to gravity with increasing depth from earth surface :(a) increases(b) decreases(c) remains unaltered(d) None
›Reveal solutionSolution
Below the earth's surface, only the mass enclosed within radius (R−d) contributes to gravity, so g falls linearly with depth.
At depth d below the earth's surface, treating the earth as a uniform sphere of radius R and density ρ, only the mass of the sphere of radius (R − d) contributes to the gravitational field at that depth (the shell outside contributes zero net field). This gives:
gd=g(1−Rd)
As d increases from 0 (surface) toward R (centre), the factor (1−d/R) decreases from 1 toward 0. So g decreases with depth, becoming zero at the centre of the earth.
✓Final answerAcceleration due to gravity decreases with increasing depth below the earth's surface. Option (b) decreases.
- CBSE 2024Set ANNUAL1 markMCQQ.Match the values of Physical quantities given in Column I with the Numerical values given in Column II: Column-I (I) Acceleration due to gravity at the centre of earth (II) Escape speed of earth (III) Universal Gravitational constant (IV) Acceleration due to gravity Column-II (A) 9.8 ms^-2 (B) 6.67 x 10^-11 Nm^2 kg^-2 (C) 0 (D) 11.2 kms^-1(a) (I)-D (II)-A (III)-B (IV)-C(b) (I)-C (II)-A (III)-D (IV)-B(c) (I)-A (II)-B (III)-D (IV)-C(d) (I)-C (II)-D (III)-B (IV)-A
›Reveal solutionSolution
(I) g at earth's centre = 0 (C); (II) escape speed = 11.2 km/s (D); (III) G = 6.67x10^-11 N m^2 kg^-2 (B); (IV) g at surface = 9.8 m/s^2 (A). This is option (d).
Matching each physical quantity to its numerical value:
(I) Acceleration due to gravity at the centre of the earth: treating the earth as a uniform sphere, the gravitational field inside a uniform spherical shell is zero everywhere inside it (shell theorem), so at the very centre, contributions from all directions cancel and g = 0 -> matches (C).
(II) Escape speed of earth: v_e = sqrt(2GM/R) ~ 11.2 km/s, the minimum speed needed for an object to escape earth's gravitational field from the surface without further propulsion -> matches (D).
(III) Universal Gravitational constant G = 6.67 x 10^-11 N m^2 kg^-2, the constant of proportionality in Newton's law of gravitation F = G m1 m2/r^2 -> matches (B).
(IV) Acceleration due to gravity (at the earth's surface) ~ 9.8 m s^-2, the standard value used for g near the earth's surface -> matches (A).
So the correct matching is (I)-C, (II)-D, (III)-B, (IV)-A.
✓Final answerThe correct option is (d) (I)-C (II)-D (III)-B (IV)-A.
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