Question:

At what distance above and below the surface of the earth a body will have the same weight (take radius of earth as R)?

Updated On: Nov 3, 2025
  • \(\frac{R}{2}\)
  • \((\sqrt5-1)\frac{R}{2}\)
  • \((\sqrt3-1)\frac{R}{2}\)
  • \((\sqrt5-1)R\)
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The Correct Option is B

Approach Solution - 1

To determine the distance above and below the Earth's surface where a body has the same weight, we need to understand the concept of gravitational force variation above and below the Earth's surface.

The gravitational force experienced by a body at a distance \( x \) above or below the Earth's surface can be expressed using the formula for gravitational force: 

1. Above the Earth's surface:

The gravitational force at a height \( h \) above the Earth's surface:

\(F_{\text{above}} = \frac{GMm}{(R+h)^2}\)

2. Below the Earth's surface:

The gravitational force at a depth \( d \) below the Earth's surface:

\(F_{\text{below}} = \frac{GMm}{R^2} \cdot \left(1 - \frac{d}{R}\right)\)

We are given that these forces are equal, so:

\(\frac{GMm}{(R+h)^2} = \frac{GMm}{R^2} \cdot \left(1 - \frac{d}{R}\right)\)

By simplifying, we cancel out \(GMm\) from both sides and solve for \( h \) in terms of \( d \):

\(\frac{1}{(R+h)^2} = \frac{1}{R^2} \left(1 - \frac{d}{R}\right)\)

Simplifying further, we obtain:

\(R^2 = (R+h)^2 \left(1 - \frac{d}{R}\right)\)

Let \( d = h \) because they need to be symmetric for the weight to be the same. Hence the equation becomes:

\((R+h)^2 \left(1 - \frac{h}{R}\right) = R^2\)

Solving this quadratic equation for \( h \), we find:

\(h = (\sqrt5 - 1)\frac{R}{2}\)

This means that the body will have the same weight at a distance \( (\sqrt5 - 1)\frac{R}{2} \) both above and below the Earth's surface. Therefore, the correct answer is \((\sqrt5 - 1)\frac{R}{2}\).

This comprehensive solution confirms that the option \((\sqrt5 - 1)\frac{R}{2}\) is correct.

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Approach Solution -2

Step 1: Define Gravitational Acceleration Above and Below: - Above the earth’s surface at height h, gravitational acceleration gp is:

\( g_{p} = \frac{gR^2}{(R + h)^2} \)

- Below the earth’s surface at depth h, gravitational acceleration gq is:

\( g_{q} = g \left(1 - \frac{h}{R}\right) \)

Step 2: Set gp = gq:

\( \frac{gR^2}{(R + h)^2} = g \left(1 - \frac{h}{R}\right) \)

Step 3: Simplify the Equation:

\( \frac{1}{\left(1 + \frac{h}{R}\right)^2} = 1 - \frac{h}{R} \)

\( \left(1 - \frac{h}{R}\right) \left(1 + \frac{h}{R}\right) = 1 \)

Step 4: Let \( \frac{h}{R} = x \):

\( (1 - x)(1 + x) = 1 \)

\( 1 - x^2 = 1 \)

\( x = \frac{\sqrt{5} - 1}{2} \)

Step 5: Calculate h:

\( h = \frac{R}{2}(\sqrt{5} - 1) \)

So, the correct answer is: \( h = \frac{R}{2}(\sqrt{5} - 1) \)

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Concepts Used:

Distance and Displacement

Distance

Distance is the sum of the length of the path traveled by an object from one place to another. The path may or may not be directly from the initial point to the final point. It is a scalar quantity that only has a magnitude, and does not have any direction.

Speed = Distance / Time

Distance= Speed x Time

D = S x T

Displacement

Displacement is the length of the shortest path from the initial point to the final point. It is a vector quantity that has magnitude as well as direction.

Velocity= Displacement / Time Therefore, 

Displacement = Velocity x Time.

D = V x T

The Difference Between Distance and Displacement are: