Feynman's Lecture on Motion of Planets: Explained

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In summary: This relationship is important in understanding the motion of planets. In summary, Feynman explains that the change in velocity of a particle in an orbit is directly related to the velocity of the orbit and inversely related to the time it takes to go around the orbit. This is known as centripetal acceleration and is significant in understanding the motion of planets.
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WiFO215
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In Feynman's lecture on the motion of the planets [page 2] he says

Suppose we take a certain fractional part of an orbit, some fixed angle, a small angle and a particle has a certain velocity. And the change in velocity during an interval if time - a fixed time - which is the force, is evidently proportional to to the velocity of in the orbit times the time that it takes to go acoss this fraction of the orbit. I mean, divided by the time. So the velocity changes proportional to the velocity. And the time over which that change has taken place is proportional to the time it takes to go around the orbit. Therefore the centripetal acceleration, or change per second of velocit towards the center, is proportional to the velocity of the orbit divided by the time it takes to go around.


I don't understand. Can someone explain?
 
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Feynman is saying that the change in velocity (acceleration) of a particle in an orbit is proportional to the velocity of the particle and inversely proportional to the time it takes to go around the orbit. In other words, the centripetal acceleration (change in velocity per second towards the center of the orbit) is proportional to the velocity of the orbit divided by the time it takes to go around. This means that if the velocity increases, or the time decreases, the acceleration will increase.
 

Related to Feynman's Lecture on Motion of Planets: Explained

1. What is Feynman's Lecture on Motion of Planets?

Feynman's Lecture on Motion of Planets is a famous lecture given by physicist Richard Feynman in 1964. In this lecture, Feynman explains the principles of planetary motion and how they are derived from Newton's laws of motion and universal gravitation.

2. Why is Feynman's lecture on Motion of Planets important?

Feynman's lecture on Motion of Planets is important because it provides a clear and concise explanation of the complex principles behind planetary motion. It is also significant because it showcases Feynman's unique teaching style and his ability to make complicated concepts accessible to a wider audience.

3. What are some key takeaways from Feynman's Lecture on Motion of Planets?

Some key takeaways from Feynman's Lecture on Motion of Planets include the three laws of planetary motion proposed by Johannes Kepler, the concept of inertia and its role in planetary motion, and the importance of gravity in understanding the orbits of planets.

4. Is Feynman's Lecture on Motion of Planets still relevant today?

Yes, Feynman's Lecture on Motion of Planets is still relevant today as the principles of planetary motion and Newton's laws of motion are still widely used in modern physics and astronomy. The lecture also provides a foundation for understanding more complex concepts such as general relativity and the nature of black holes.

5. Can anyone understand Feynman's Lecture on Motion of Planets?

Yes, anyone with a basic understanding of physics and mathematics can understand Feynman's Lecture on Motion of Planets. Feynman's engaging teaching style and use of simple analogies make the lecture accessible to a wide range of audiences.

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