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Ch 13: Gravitation
Chapter 13, Problem 13

In its orbit each day, the International Space Station makes 15.65 revolutions around the earth. Assuming a circular orbit, how high is this satellite above the surface of the earth?

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1
Calculate the orbital period of the ISS by using the given number of revolutions per day. Since there are 24 hours in a day, divide 24 hours by the number of revolutions (15.65) to find the period of one revolution in hours.
Convert the orbital period from hours to seconds to use in further calculations. Multiply the period in hours by 3600 seconds/hour.
Use the formula for the orbital period of a satellite, T = 2\pi \sqrt{\frac{r^3}{GM}}, where T is the orbital period, r is the radius of the orbit, G is the gravitational constant (6.67430 \times 10^{-11} \, \text{m}^3 \, \text{kg}^{-1} \, \text{s}^{-2}), and M is the mass of the Earth (approximately 5.972 \times 10^{24} kg).
Rearrange the formula to solve for the radius of the orbit, r. The equation becomes r = \left(\frac{GMT^2}{4\pi^2}\right)^{1/3}.
Subtract the radius of the Earth (approximately 6,371 kilometers) from the calculated orbital radius to find the height of the ISS above the Earth's surface.

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Key Concepts

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

Circular Motion

Circular motion refers to the movement of an object along the circumference of a circle. In the context of satellites, this involves understanding how an object, like the International Space Station, travels in a circular path around the Earth due to gravitational forces. The speed and radius of this motion are crucial for determining the satellite's altitude.
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Gravitational Force

Gravitational force is the attractive force between two masses, such as the Earth and the International Space Station. This force is responsible for keeping the satellite in orbit. The strength of this force decreases with distance from the Earth's center, which is essential for calculating the height of the satellite above the Earth's surface.
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Orbital Mechanics

Orbital mechanics is the study of the motion of objects in space under the influence of gravitational forces. It involves principles such as Kepler's laws of planetary motion and the equations of motion for circular orbits. Understanding these principles allows us to calculate the altitude of satellites based on their orbital period and the mass of the Earth.
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Related Practice
Textbook Question
Find the magnitude and direction of the net gravitational force on mass A due to masses B and C in Fig. E13.6

. Each mass is 2.00 kg.

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Textbook Question
The point masses m and 2m lie along the x-axis, with m at the origin and 2m at x = L. A third point mass M is moved along the x-axis. (a) At what point is the net gravitational force on M due to the other two masses equal to zero?
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Textbook Question
Two satellites are in circular orbits around a planet that has radius 9.00 * 10^6 m. One satellite has mass 68.0 kg, orbital radius 7.00 * 10^7 m, and orbital speed 4800 m/s. The second satellite has mass 84.0 kg and orbital radius 3.00 * 10^7 m. What is the orbital speed of this second satellite?
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Textbook Question
On July 15, 2004, NASA launched the Aura spacecraft to study the earth's climate and atmosphere. This satellite was injected into an orbit 705 km above the earth's surface. Assume a circular orbit. (a) How many hours does it take this satellite to make one orbit?
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Textbook Question
For a satellite to be in a circular orbit 890 km above the surface of the earth, (a) what orbital speed must it be given?
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Textbook Question
Two uniform spheres, each of mass 0.260 kg, are fixed at points A and B (Fig. E13.5). Find the magnitude and direction of the initial acceleration of a uniform sphere with mass 0.010 kg if released from rest at point P and acted on only by forces of gravitational attraction of the spheres at A and B.
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