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Ch 15: Oscillations
Chapter 15, Problem 13

A rocket is launched straight up from the earth's surface at a speed of 15,000 m/s. What is its speed when it is very far away from the earth?

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Key Concepts

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

Kinetic Energy and Potential Energy

In the context of a rocket launch, kinetic energy (KE) is the energy of motion, while gravitational potential energy (PE) is the energy stored due to an object's position in a gravitational field. As the rocket ascends, its kinetic energy decreases while its potential energy increases until it reaches a point where gravitational influence is negligible.
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Conservation of Energy

The principle of conservation of energy states that the total energy in a closed system remains constant. For the rocket, the initial kinetic energy at launch will convert into gravitational potential energy as it rises, and when it is far from Earth, this energy will primarily be kinetic, allowing us to calculate its speed at that point.
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Escape Velocity

Escape velocity is the minimum speed needed for an object to break free from a celestial body's gravitational pull without further propulsion. For Earth, this speed is approximately 11,186 m/s. Since the rocket's launch speed of 15,000 m/s exceeds this threshold, it will continue to move away from Earth indefinitely, ultimately reaching a speed that can be calculated using energy conservation principles.
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Related Practice
Textbook Question
The Parker Solar Probe, launched in 2018, was the first spacecraft to explore the solar corona, the hot gases and flares that extend outward from the solar surface. The probe is in a highly elliptical orbit that, using the gravity of Venus, will be nudged ever closer to the sun until, in 2025, it reaches a closest approach of 6.9 million kilometers from the center of the sun. Its maximum speed as it whips through the corona will be 192 km/s. (b) The probe's highly elliptical orbit carries it out to a maximum distance of 160 Rₛ with a period of 88 days. What is its slowest speed, in km/s?
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Textbook Question
Nothing can escape the event horizon of a black hole, not even light. You can think of the event horizon as being the distance from a black hole at which the escape speed is the speed of light, 3.00 ✕ 10⁸ m/s, making all escape impossible. What is the radius of the event horizon for a black hole with a mass 5.0 times the mass of the sun? This distance is called the Schwarzschild radius.
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Textbook Question
What is the escape speed from Jupiter?
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Textbook Question
A space station orbits the sun at the same distance as the earth but on the opposite side of the sun. A small probe is fired away from the station. What minimum speed does the probe need to escape the solar system?
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Textbook Question
What is the total gravitational potential energy of the three masses in FIGURE P13.35?
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Textbook Question
September 2015 saw the historic discovery of gravitational waves, almost exactly 100 years after Einstein predicted their existence as a consequence of his theory of general relativity. Gravitational waves are a literal stretching and compressing of the fabric of space. Even the most sensitive instruments—capable of sensing that the path of a 4-km-long laser beam has lengthened by one-thousandth the diameter of a proton—can detect waves created by only the most extreme cosmic events. The first detection was due to the collision of two black holes more than 750 million light years from earth. Although a full description of gravitational waves requires knowledge of Einstein's general relativity, a surprising amount can be understood with the physics you've already learned. (d) Two black holes collide and merge when their Schwarzchild radii overlap; that is, they merge when their separation, which we've defined as 2r, equals 2RSch . Find an expression for ΔE=Ef−Ei , where Ei ≈ 0 because initially the black holes are far apart and Ef is their total energy at the instant they merge. This is the energy radiated away as gravitational waves. Your answer will be a fraction of Mc², and you probably recognize that this is related to Einstein's famous E=mc² . The quantity Mc² is the amount of energy that would be released if an entire star of mass M were suddenly converted entirely to energy.
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