Potential valleys in our solar system

In summary, a spherical potential has a peak and a valley before smoothing out around zero at large distances. One can have an unstable circular orbit at the position of the peak and a stable orbit at the position of the valley. However, the orbit with the spherical body only produces a single valley. This can be explained by the masses of the bigger planets changing the overall potential and inducing several potential wells.
  • #1
dianaj
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Hi all,

Our sun is approximately a spherical body and accordingly it has a spherical potential. I have just learned that this potential - accoring to general relativity - has a peak and a valley before smoothing out around zero at large distances. One can have an unstable circular orbit at the position of the peak and a stable orbit at the position of the valley. But what is more normal: one can have an elliptical orbit with a mean radius being that of the vally. This is the kind of orbits our planets move in. So far so good. But the model with the spherical body only produces a single valley while we clearly have several stable elliptical orbits in our solar system. How can this be? The only answer I can come up with is that the masses of the bigger planets change the overall potential and induce several potential wells. Is this correct?

/Diana
 
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  • #2
I assume you're talking about the effective potential as calculated from GR. In this case, elliptical orbits do not correspond to a minimum in potential, but rather the difference in two points around this minimum. (Which is why the radius of orbit is not constant: the turning points correspond to different radii)

Refer to this picture:
http://upload.wikimedia.org/wikipedia/commons/2/2c/EffektivesPotential.jpg

Note: This is actually a Newtonian potential, but for what you're considering it doesn't matter.

So, the circular orbit corresponds to the minimum in potential. Elliptical orbits correspond to drawing a line of constant E greater than that minimum, and then you get r+ and r- as the two turning points of the function it oscillates between. Clearly, for different values of energy you get different radii, and thus, our elliptical orbits.

Hope this clears it up at least a little.
 
  • #3
dianaj, Newtonian mechanics does a very good job of explaining the behavior of the solar system. Newtonian mechanics cannot fully explain the anomalistic recession of the planets. The error is greatest for Mercury, for which Newtonian mechanics misses the mark by all of 43 seconds of arc per century.

I think you might be talking about what is now called the "http://en.wikipedia.org/wiki/Interplanetary_Transport_Network" ". Read the link. If that hits the mark, you can google that phrase. You can also google the names Martin Lo, Jerrold E. Marsden, Wang Sang Koon, and Shane Ross, some of the key people behind this concept.
 
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Related to Potential valleys in our solar system

1. What are potential valleys in our solar system?

Potential valleys are low-lying regions on the surface of planets or moons in our solar system. They can be caused by a variety of factors such as impact craters, volcanic activity, or tectonic forces.

2. Where can potential valleys be found in our solar system?

Potential valleys can be found on many of the rocky planets and moons in our solar system, including Mars, Mercury, and the Moon. They can also be found on some of the icy moons of the outer planets, such as Europa and Enceladus.

3. How are potential valleys formed?

Potential valleys are formed through a combination of processes, such as impact events, volcanic activity, and erosion. For example, large impact craters can create deep valleys, while volcanic eruptions can create valleys and canyons through the flow of lava.

4. What is the significance of potential valleys in our solar system?

Potential valleys are important features in our solar system as they provide information about the geological history of a planet or moon. They can also reveal clues about past environmental conditions and potential sites for future exploration or even potential habitats for life.

5. How are potential valleys studied by scientists?

Scientists study potential valleys through a variety of methods, including remote sensing techniques such as satellite imagery and topographic mapping. They may also use rovers or landers to directly explore and collect data on potential valleys on the surface of other planets or moons.

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