Disequilibrium of the solar system

In summary, the Sun's loss of mass affects the size of planetary orbits. The only way gravitational equilibrium can change is if the mass of the sun changes in a way that alters the center of gravity of the solar system. The analysis by Seligman is incorrect if the Sun's mass changes by a significant amount.
  • #1
petrushkagoogol
28
4
As the Sun's supply of hydrogen gradually gets exhausted gravity takes over and predominates over fusion energy. As this happens does the equilibrium of the solar system gets distorted, and if so is there a cut-off point for the same ? o0)
 
Astronomy news on Phys.org
  • #2
http://cseligman.com/text/stars/masslosseffects.htmDeriving the Effect of the Sun's Loss of Mass
With the above as background we are now ready to see how the loss of mass the Sun is bound to suffer when it gets very old affects the size of planetary orbits. In doing so we will assume that the orbits are sufficiently circular that we can use the simplifications applicable to that case, and that any friction due to gases lost by the Sun passing the various planetary orbits produces negligible effects on their motion. In that case, the only thing we need worry about is that as the Sun loses mass it exerts less gravitational force, and cannot hold the planets in the orbits that their current velocities require. As a result the planets would gradually move away from the Sun, attaining higher orbits and in the process, reducing their speeds to values which the Sun's reduced gravity could maintain in such orbits.
 
  • Like
Likes petrushkagoogol
  • #3
The only way gravitational equilibrium can change is if the mass of the sun changes in a way that alters the center of gravity of the solar system - i.e., ejecta. The sun is the only body in our solar system with enough mass to induce any such effect of any real significance. It appears safe to say this is unlikely to occur for at least a few billion years.
 
  • #4
And note that the linked analysis by Seligman is only correct in the limit of infinitesmal changes in the Sun's mass, which they fail to mention in their analysis. The analysis is incorrect if the Sun's mass changes by a significant amount, one cannot analyze that situation by saying that the planet then has the mechanical energy it had before, minus the change in potential energy, that's pretty much make believe physics. You can tell the analysis is wrong in general if you simply add a lot of mass instead of removing a little, and note the answer makes no sense. The correct way to do the analysis in general is to take their requirement that the potential energy must be -2 times the kinetic energy, which is correct, and couple it to the requirement of conservation of angular momentum of the Earth's orbit. Then you can include any mass change you like, the angular momentum is much harder to change than the mechanical energy of the Earth's orbit.
 

1. What causes disequilibrium in the solar system?

The main cause of disequilibrium in the solar system is the gravitational interactions between the planets, moons, and other celestial bodies. These interactions can cause slight changes in the orbits of these bodies, leading to a state of disequilibrium.

2. How does disequilibrium affect the solar system?

Disequilibrium can have a variety of effects on the solar system, including changes in the orbits of planets and moons, disruptions in the formation of new celestial bodies, and changes in the distribution of matter and energy throughout the system.

3. Is disequilibrium a normal occurrence in the solar system?

Yes, disequilibrium is a natural and ongoing process in the solar system. The gravitational forces between celestial bodies are constantly changing, leading to a state of disequilibrium that can last for thousands or even millions of years.

4. Can disequilibrium lead to major disruptions in the solar system?

While disequilibrium is a normal occurrence, it can sometimes lead to major disruptions in the solar system. For example, a large enough gravitational interaction between two planets could potentially alter their orbits or even cause a collision.

5. How do scientists study and measure disequilibrium in the solar system?

Scientists use a variety of techniques to study and measure disequilibrium in the solar system, including observations from telescopes and spacecraft, computer simulations, and mathematical models. They also study the geological and geological records of other planets and moons to better understand their past and present states of disequilibrium.

Similar threads

  • Astronomy and Astrophysics
Replies
10
Views
1K
  • Astronomy and Astrophysics
Replies
15
Views
1K
  • Astronomy and Astrophysics
Replies
1
Views
1K
Replies
15
Views
1K
Replies
18
Views
2K
Replies
11
Views
3K
  • Electrical Engineering
Replies
32
Views
2K
  • Astronomy and Astrophysics
Replies
6
Views
2K
  • Astronomy and Astrophysics
Replies
4
Views
2K
  • Astronomy and Astrophysics
4
Replies
109
Views
4K
Back
Top