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.
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: \( h = \frac{R}{2}(\sqrt{5} - 1) \)
A black body is at a temperature of 2880 K. The energy of radiation emitted by this body with wavelength between 499 nm and 500 nm is U1, between 999 nm and 1000 nm is U2 and between 1499 nm and 1500 nm is U3. The Wien's constant, b = 2.88×106 nm-K. Then,

What will be the equilibrium constant of the given reaction carried out in a \(5 \,L\) vessel and having equilibrium amounts of \(A_2\) and \(A\) as \(0.5\) mole and \(2 \times 10^{-6}\) mole respectively?
The reaction : \(A_2 \rightleftharpoons 2A\)
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 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
