Three satellites orbit a planet of radius R, as shown in FIGURE EX13.24. Satellites S1 and S3 have mass m. Satellite S2 has mass 2m. Satellite S1 orbits in 250 minutes and the force on S1 is 10,000 N. What is the kinetic-energy ratio for K1 / K3 for S1 and S3?
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Satellite Motion: Speed & Period
Problem 42b
Textbook Question
Estimate the density of the Earth, given that a satellite near the surface orbits with a period of 85 min. Approximate the Earth as a uniform sphere.

1
Convert the orbital period of the satellite from minutes to seconds. Since 1 minute = 60 seconds, multiply 85 minutes by 60 to get the period in seconds.
Use Kepler's third law for circular orbits, which relates the orbital period \( T \) to the radius \( r \) of the orbit and the mass \( M \) of the Earth: \( T = 2\pi \sqrt{\frac{r^3}{GM}} \), where \( G \) is the gravitational constant. Rearrange this equation to solve for \( M \): \( M = \frac{4\pi^2r^3}{GT^2} \).
Assume the satellite is orbiting very close to the Earth's surface, so the orbital radius \( r \) is approximately equal to the Earth's radius. Use the known value of Earth's radius \( r \approx 6.371 \times 10^6 \ \text{m} \).
Once the mass \( M \) of the Earth is determined, calculate the density \( \rho \) of the Earth using the formula for the density of a sphere: \( \rho = \frac{M}{\frac{4}{3}\pi r^3} \). Substitute the values for \( M \) and \( r \) into this equation.
Simplify the expression to find the density of the Earth. Ensure all units are consistent (e.g., mass in kilograms, radius in meters) to obtain the density in \( \text{kg/m}^3 \).

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Key Concepts
Here are the essential concepts you must grasp in order to answer the question correctly.
Gravitational Force
The gravitational force is the attractive force between two masses, described by Newton's law of universal gravitation. It states that the force is proportional to the product of the masses and inversely proportional to the square of the distance between their centers. This force is crucial for understanding how satellites orbit the Earth, as it provides the necessary centripetal force to keep them in circular motion.
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Gravitational Forces in 2D
Orbital Period
The orbital period is the time it takes for an object to complete one full orbit around another object. For satellites, this period depends on the radius of the orbit and the mass of the central body, as described by Kepler's laws of planetary motion. In this case, the period of 85 minutes can be used to derive the gravitational parameters of the Earth, which are essential for estimating its density.
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Geosynchronous Orbits
Density
Density is defined as mass per unit volume and is a key property of materials. For Earth, density can be estimated by using the mass derived from gravitational calculations and the volume of the Earth, which can be approximated as a sphere. Understanding density is important in geophysics, as it provides insights into the composition and structure of the Earth.
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Intro to Density
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