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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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.
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.
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.