The height at which the weight of a body becomes one third of its weight on the surface of earth is (R is the radius of earth)
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Logic Tip: Do not use the approximation formula $g_h = g(1 - 2h/R)$ unless $h$ is specifically stated to be very small compared to $R$ (typically $< 5%$). Since the weight changes by a massive factor (1/3), the exact formula must be used.
Concept:
The acceleration due to gravity $g_h$ at a height $h$ above the Earth's surface is given by the exact formula:
$$g_h = \frac{g}{\left(1 + \frac{h}{R}\right)^2}$$
where $g$ is the acceleration at the surface and $R$ is the Earth's radius.
Since Weight $W = mg$, the weight scales identically to the local gravity.
Step 1: Set up the given condition.
We are given that the weight at height $h$ is one-third of the weight on the surface:
$$W_h = \frac{1}{3}W$$
$$m \cdot g_h = \frac{1}{3}m \cdot g$$
$$g_h = \frac{g}{3}$$
Step 2: Equate and solve for h/R.
Substitute $g_h$ into the gravity formula:
$$\frac{g}{3} = \frac{g}{\left(1 + \frac{h}{R}\right)^2}$$
Cancel $g$ from both sides and take the reciprocal:
$$3 = \left(1 + \frac{h}{R}\right)^2$$
Step 3: Solve the algebraic equation.
Take the square root of both sides:
$$\sqrt{3} = 1 + \frac{h}{R}$$
We know that $\sqrt{3} \approx 1.732$. Substitute this value:
$$1.732 = 1 + \frac{h}{R}$$
Subtract 1 from both sides:
$$\frac{h}{R} = 0.732$$
$$h = 0.732 R$$