Spacetime Curvature: Eliptical Orbital Paths & Keppler Laws

In summary, this demonstration shows that locally and for weak fields, space-time geometry just reproduces the same effect as Newton's force would have, resulting in an elliptical orbit. But globally, the orbit is not closed because of the additional effect of space curvature.
  • #1
Osvaldo
27
1
Though it is hard not to believe in the spacetime curvature that cause planets to follow curved path arround massive objects, I wander how come these paths are eliptical, the object change velocity when moving arround the massive object and what is more obeys the Keppler laws. If there is not such a gravitational force (as said byexperienced physics) which would really caused these conditions, how come these orbital movements do not belong to a central force? Can somebody give a clear explanation?
 
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  • #2
Kepler laws or eliptic orbit of planets is derivied from Newton's inverse square law of universal gravitation.
I understand this Newton's inverse square law of central force is a fairy good approximation of GR theory or curved spacetime around the Sun, a massive body.
 
  • #3
Osvaldo said:
I wander how come these paths are eliptical
They are actually not quite elliptical. GR explains both why they are almost elliptical and also correctly predicts how much they deviate from being completely elliptical.
 
  • #4
Osvaldo said:
Though it is hard not to believe in the spacetime curvature that cause planets to follow curved path arround massive objects, I wander how come these paths are eliptical, the object change velocity when moving arround the massive object and what is more obeys the Keppler laws. If there is not such a gravitational force (as said byexperienced physics) which would really caused these conditions, how come these orbital movements do not belong to a central force? Can somebody give a clear explanation?
Locally and for weak fields the space-time geometry just reproduces the same effect Newton's force would have, and would also result in an elliptical orbit:



But globally you get an additional effect from space curvature, so the orbit is not closed:
http://demoweb.physics.ucla.edu/content/10-curved-spacetime (Figure 2)
 
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Likes Dale
  • #5
A.T. said:
Locally and for weak fields the space-time geometry just reproduces the same effect Newton's force would have, and would also result in an elliptical orbit:



But globally you get an additional effect from space curvature, so the orbit is not closed:
http://demoweb.physics.ucla.edu/content/10-curved-spacetime (Figure 2)
 
  • #6
Wonderful demonstration. Never saw it like the one in the video. Thanks a lot
 

1. What is spacetime curvature?

Spacetime curvature is a concept in physics that describes the bending of space and time caused by the presence of massive objects. It is a fundamental aspect of Einstein's theory of general relativity and is essential for understanding the behavior of objects in the universe.

2. How does spacetime curvature affect orbital paths?

Spacetime curvature affects orbital paths by causing them to follow elliptical trajectories around massive objects. This is because the presence of a massive object, such as a planet or star, creates a curvature in spacetime that alters the straight path of an object and causes it to follow a curved path around the massive object.

3. What are elliptical orbital paths?

Elliptical orbital paths are curved paths that objects follow around a massive object, such as a planet or star. These paths are shaped like an ellipse, with the massive object located at one of the two foci of the ellipse. The eccentricity of the ellipse determines the shape of the orbit, with a higher eccentricity resulting in a more elongated orbit.

4. What are Kepler's laws of planetary motion?

Kepler's laws of planetary motion are three fundamental laws that describe the motion of objects in elliptical orbits around a central massive object. The first law, also known as the law of ellipses, states that all planets move in elliptical orbits with the sun at one of the foci. The second law, or the law of equal areas, states that a line connecting a planet to the sun will sweep out equal areas in equal amounts of time. The third law, or the law of harmonies, states that the square of a planet's orbital period is proportional to the cube of its average distance from the sun.

5. How do Kepler's laws relate to spacetime curvature?

Kepler's laws of planetary motion are a result of the effects of spacetime curvature on objects in elliptical orbits. The first law is a result of the curvature of spacetime caused by the massive object, while the second and third laws are consequences of the conservation of angular momentum and energy in a curved spacetime. Therefore, Kepler's laws provide a mathematical description of how spacetime curvature affects the motion of objects in elliptical orbits.

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