Instability of the Solar System

In summary: No, you would still get errors because GR is an approximation. If you tried to model the solar system using only GR, you would eventually run into problems because there are too many unknowns. Classical mechanics is an approximation to GR but it does a better job of capturing how the system behaves over a short period of time. Classical mechanics is more accurate over a short period of time than GR, but over a long period of time GR is more accurate.
  • #1
Silviu
624
11
Hello! I read in some books that the behavior of the Solar system can't be predicted indefinitely (up to several hundreds of million of years). Is this a numerical limitation, in trying to simulate it or is it some physics responsible for it? (I guess that this assumes that no other bodies interfere with the system, otherwise you would need to take into account the whole light cone for 100 million years and I think this is not doable with current technology) Thank you!
 
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  • #2
Simulations are often approximations to a real system and don't take into account every facet of the real system.

In the solar system case, over a long period of time you will need to factor in how one planet affects another and the then it becomes an n-body problem which is extremely impractical to impossible to model perfectly.

https://en.wikipedia.org/wiki/Stability_of_the_Solar_System

I've seen simulations of three body problem which easily become chaotic as they run. Error is introduced just from repeated summing which either adds energy to the system or takes it away. Often modelers try to use algorithms that while not perfect periodically add error and then remove it (error is manifest as energy in the run) so that over a long time the run is stable.



https://en.wikipedia.org/wiki/Three-body_problem

https://en.wikipedia.org/wiki/N-body_problem

https://en.wikipedia.org/wiki/N-body_simulation
 
  • #3
jedishrfu said:
Simulations are often approximations to a real system and don't take into account every facet of the real system.

In the solar system case, over a long period of time you will need to factor in how one planet affects another and the then it becomes an n-body problem which is extremely impractical to impossible to model perfectly.

https://en.wikipedia.org/wiki/Stability_of_the_Solar_System

I've seen simulations of three body problem which easily become chaotic as they run. Error is introduced just from repeated summing which either adds energy to the system or takes it away. Often modelers try to use algorithms that while not perfect periodically add error and then remove it (error is manifest as energy in the run) so that over a long time the run is stable.



https://en.wikipedia.org/wiki/Three-body_problem

https://en.wikipedia.org/wiki/N-body_problem

https://en.wikipedia.org/wiki/N-body_simulation

But in the end, this is a numerical problem. The Solar System motion is deterministic, it is just a limitation of our computers (like round-off errors), right?
 
  • #4
We don't know if the solar system is stable for the long term, only that it has been for some time and that it will be for some time. The solar system is not a stable system over the long run.

Chaotic systems can't be predicted because that computer has a finite precision in its numbers and no matter how many decimals we choose to save, its in these lost decimal values that chaos springs up. Saturn's moons have chaotic orbits and a couple of moons have a dance where they switch orbits as they cross.

Basically small changes in one state get magnified in future states until the simulation no longer matches reality. We say the system is non-linear.

https://en.wikipedia.org/wiki/Butterfly_effect
 
  • #5
jedishrfu said:
We don't know if the solar system is stable for the long term, only that it has been for some time and that it will be for some time.

Chaotic systems can't be predicted because that computer has a finite precision in its numbers no matter how many decimals we choose to save and its in these lost decimal values that chaos springs up. Saturn's moons have chaotic orbits and a couple of moons have a dance where they switch orbits as they cross.
But my question is, as classical mechanics is completely predictable, shouldn't the Solar System be, too? So if we now predict the orbits for the next 100 million years and create a computer that can have 10 times more accuracy, we can extend the prediction. So if we would have a computer with bigger and bigger accuracy, would we be able to predict the position of each planet indefinitely?
 
  • #6
You're missing the point. You can't just use orbital mechanics to model the system. There are so many other unknowns that over time get magnified and alter whatever simulation you make. From state to state these changes may be infinitesimally small but over time they magnify and cause the real system to deviate from the modeled approximation.
 
  • #7
jedishrfu said:
You're missing the point. You can't just use orbital mechanics to model the system. There are so many other unknowns that over time get magnified and alter whatever simulation you make. From state to state these changes may be infinitesimally small but over time they magnify and cause the real system to deviate from the modeled approximation.
I am not sure I understand. The only small effects I can think of, would be from GR (well of course there might be quantum fluctuations, but I assume they are insignificant for this purpose). So if you use GR instead of Newtonian Mechanics, shouldn't you get perfect results for a long period with a big enough computer accuracy?
 
  • #8
The sun radiates energy which pushes against the planets is not factored in. The sun is losing mass as it radiates energy. There are unpredictable solar storms which radiate even more energy. There's the loss of planetary rotational energy transferred to the moons... I'm sure there are other things some external influences... that I yet to hear about that would need to be considered.

https://en.wikipedia.org/wiki/Butterfly_effect
 
  • #9
How about the influences of each asteroid, or each object in the Kuiper Belt, each comet, radiation pressure, solar wind, geomagnetic storms? You can't say negligably small if you want millions of orbits.
 
  • #10
anorlunda said:
How about the influences of each asteroid, or each object in the Kuiper Belt, each comet, radiation pressure, solar wind, geomagnetic storms? You can't say negligably small if you want millions of orbits.
Ok, maybe I was not clear enough. My question is not if it is feasible to simulate all of these, but if the Solar System is intrinsically deterministic. Like quantum mechanics can't be simulated perfectly because it is not deterministic (by this I mean the measurement, not the evolution of the wave function). Is the solar system deterministic (I am not asking if it can be simulated on a computer now)?
 
  • #11
Silviu said:
Ok, maybe I was not clear enough. My question is not if it is feasible to simulate all of these, but if the Solar System is intrinsically deterministic. Like quantum mechanics can't be simulated perfectly because it is not deterministic (by this I mean the measurement, not the evolution of the wave function). Is the solar system deterministic (I am not asking if it can be simulated on a computer now)?

In that case, re-read #4. Also read about chaos theory on Wikipedia if you're not familiar with that.
 

What causes instability in the solar system?

The instability of the solar system can be caused by a variety of factors, including gravitational interactions between planets, the presence of large objects like comets or asteroids, and the influence of external forces such as passing stars or galaxies.

Can the instability of the solar system lead to major changes in our planetary orbits?

Yes, the instability of the solar system can potentially lead to major changes in the orbits of planets. For example, the gravitational pull of a large object passing by could alter the orbit of a planet, causing it to move closer or farther from the sun.

What would be the consequences of a major instability event in the solar system?

The consequences of a major instability event in the solar system could range from minor changes in planetary orbits to catastrophic collisions between planets or other celestial bodies. It could also potentially affect the habitability of planets and their ability to sustain life.

How do scientists study and monitor the stability of the solar system?

Scientists use a variety of methods to study and monitor the stability of the solar system, including computer simulations, astronomical observations, and mathematical models. They also analyze data from past events, such as asteroid impacts, to better understand the potential for instability in the future.

Is there a way to predict and prevent major instability events in the solar system?

While scientists can make predictions based on current data and models, it is difficult to predict and prevent major instability events in the solar system. However, ongoing research and monitoring can help us better understand the dynamics of the solar system and potentially develop strategies to mitigate the effects of instability.

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