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: \( h = \frac{R}{2}(\sqrt{5} - 1) \)
The portion of the line \( 4x + 5y = 20 \) in the first quadrant is trisected by the lines \( L_1 \) and \( L_2 \) passing through the origin. The tangent of an angle between the lines \( L_1 \) and \( L_2 \) is:
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