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Topic: Motion of a satellite: orbital velocity, time period and energy· Gravitation

A satellite of mass m is orbiting the earth (of radius R) at a height h from its surface. The total energy of the satellite in terms of g_0, the value of acceleration due to gravity at the earth's surface, is

1. \(-\frac{mg_0R^2}{2(R+h)}\)

2. \(\frac{2mg_0R^2}{R+h}\)

3. \(-\frac{2mg_0R^2}{R+h}\)

4. \(\frac{mg_0R^2}{2(R+h)}\)

1 answer

Best answer

Answer: 1. \(-\frac{mg_0R^2}{2(R+h)}\)

For a satellite in orbit, total energy is half of its (negative) potential energy: \(E=-\dfrac{GMm}{2(R+h)}\).

Use \(g_0=\dfrac{GM}{R^2}\), so \(GM=g_0R^2\).

$$E=-\frac{mg_0R^2}{2(R+h)}$$

Option (1). Options (2) and (4) are positive, which is impossible for a bound orbit; option (3) is twice the correct magnitude.

Doubtly AI · 30 Oct 2026 AI-generated · not yet verified Report
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