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Ch 13: Newton's Theory of Gravity
Chapter 13, Problem 13

A satellite in a circular orbit of radius r has period T. A satellite in a nearby orbit with radius r + Δr, where Δr≪r , has the very slightly different period T + ΔT. (a) Show that ΔT/T = (3/2) (Δr/r)

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Identify the relationship between the orbital period (T) and the radius (r) of the satellite's orbit. According to Kepler's third law, the square of the orbital period (T^2) is proportional to the cube of the orbit's radius (r^3), which can be expressed as T^2 \propto r^3.
Differentiate both sides of the equation T^2 \propto r^3 with respect to r to find the rate of change of T with respect to r. Use the chain rule for differentiation, which gives 2T \frac{dT}{dr} = 3r^2.
Rearrange the differentiated equation to solve for \frac{dT}{dr}, the rate of change of the period with respect to the radius. This gives \frac{dT}{dr} = \frac{3r^2}{2T}.
Express the small change in the period (ΔT) in terms of the small change in the radius (Δr) using the derivative: ΔT = \frac{dT}{dr} Δr. Substitute the expression for \frac{dT}{dr} from the previous step to get ΔT = \frac{3r^2}{2T} Δr.
Divide both sides of the equation ΔT = \frac{3r^2}{2T} Δr by T and simplify to find the fractional change in the period relative to the fractional change in the radius: \frac{ΔT}{T} = \frac{3}{2} \frac{Δr}{r}. This shows that the change in period relative to the period is 1.5 times the change in radius relative to the radius.

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Key Concepts

Here are the essential concepts you must grasp in order to answer the question correctly.

Kepler's Third Law

Kepler's Third Law states that the square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit. For circular orbits, this can be expressed as T² ∝ r³, which implies that as the radius increases, the period increases, but at a specific rate. This relationship is fundamental in understanding how changes in orbital radius affect the period of a satellite.
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Differential Calculus

Differential calculus is a branch of mathematics that deals with the rates at which quantities change. In this context, it helps us understand how a small change in radius (Δr) leads to a small change in period (ΔT). By applying the concept of derivatives, we can derive relationships between these small changes, which is essential for solving the problem presented.
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Circular Motion

Circular motion refers to the motion of an object traveling along a circular path. In the case of satellites, this involves understanding the forces acting on the satellite, such as gravitational force and centripetal force. The balance of these forces determines the satellite's speed and period, which are crucial for analyzing how changes in orbit affect the satellite's period.
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