To find the height at which the weight of a body becomes \( \frac{1}{16} \)th of its weight on the Earth's surface, we need to utilize the concept of gravitational force.
The weight of a body at a distance \( r \) from the center of the Earth is given by:
W = \frac{GMm}{r^2}
where:
On the Earth's surface, the weight \( W_0 \) is:
W_0 = \frac{GMm}{R^2}
where \( R \) is the radius of the Earth.
Now, we want the weight to be \( \frac{1}{16} \) of \( W_0 \) at a height \( h \):
\frac{GMm}{(R + h)^2} = \frac{1}{16} \times \frac{GMm}{R^2}
Canceling out the common terms \( \frac{GMm}{R^2} \), we get:
\frac{1}{(1 + \frac{h}{R})^2} = \frac{1}{16}
This simplifies to:
(1 + \frac{h}{R})^2 = 16
Taking the square root on both sides:
1 + \frac{h}{R} = 4
Therefore,
\frac{h}{R} = 4 - 1 = 3
Hence, \( h = 3R \).
The correct answer is 3R.
The height from Earth's surface at which acceleration due to gravity becomes \(\frac{g}{4}\) is \(\_\_\)? (Where \(g\) is the acceleration due to gravity on the surface of the Earth and \(R\) is the radius of the Earth.)