Can Orbiting Bodies Slow Down Over Time?

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Discussion Overview

The discussion revolves around the dynamics of orbiting bodies in the solar system, specifically addressing whether their velocities can decrease over time and the implications of such changes. Participants explore various forces at play, the conservation of energy, and the potential for orbits to change due to external influences.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • Some participants question why the perpendicular velocity of planets does not seem to decrease, suggesting that various forces may affect their motion.
  • Others argue that planets can maintain their orbits indefinitely under ideal conditions, similar to an ideal pendulum, unless acted upon by significant external forces.
  • It is noted that gravitational interactions with other celestial bodies and forces like tidal effects could lead to energy loss, potentially affecting orbital stability over long timescales.
  • Some participants propose that friction from interstellar particles and many-body effects could eventually slow down orbits, leading to planets spiraling into the sun or colliding with each other.
  • There is a discussion about the conservation of energy, with some asserting that energy must be radiated away for orbits to slow down, while others mention that tidal forces and gravitational waves could contribute to energy loss.
  • Participants express uncertainty about the predictability of orbital changes and the long-term stability of planetary orbits, emphasizing that while energy is conserved, interactions with the environment could lead to eventual changes.

Areas of Agreement / Disagreement

Participants do not reach a consensus on whether orbiting bodies can slow down over time. Multiple competing views are presented regarding the effects of various forces and the implications for orbital stability.

Contextual Notes

Participants acknowledge limitations in their understanding of the many-body problem and the complexities involved in predicting orbital dynamics over extended periods.

micropulsar
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We see in our solar system the planets orbiting the sun, but why doesn't with all of the other forces in play the perpendicular velocity seemingly not decrease(or does it?). And if the perpendicular velocity of the planets slow down would that result in static planets not moving around the sun?
 
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Just like an ideal pendulum in a vacuum could go on forever, a planet orbiting can go on forever. A planet in our solar system will be constrained to orbiting the sun, just like a pendulum is constrained by the cable that it hangs from. A planet will speed up (slightly) as it heads toward a far away gravitational body, just like a pendulum will speed up as it heads toward the Earth. The planet will slow down (slightly) as it swings around the Sun and heads away from that gravitational body. Unlike a pendulum, the planets have enough velocity to continue all the way around the sun in an orbit without being slowed to a stop by a far off body. So a planet orbits instead of swinging back and forth like a pendulum. This can continue forever.
 
micropulsar said:
why doesn't with all of the other forces in play the perpendicular velocity seemingly not decrease(or does it?).

All the other forces are either affecting everything in the solar system just as much as they affecting the Earth (gravitational interactions with other stars, galaxies, etc), or don't affect the Earth the because their range is too small or the Earth is neutral (the other 3 forces of nature).
 
micropulsar said:
We see in our solar system the planets orbiting the sun, but why doesn't with all of the other forces in play the perpendicular velocity seemingly not decrease(or does it?).
The only way to decrease their total kinetic energy is through very small effects, like converting it into gravitational waves or EM-waves (heating though tidal forces).

micropulsar said:
And if the perpendicular velocity of the planets slow down would that result in static planets not moving around the sun?
Have you heard of gravity?
 
Last edited:
Well, I imagine given enough time the combination of friction from interstellar particles/gas and many-body effects, even without counting the possibility of some rogue body entering the system and altering its equilibrium, would slow down orbits and make the planets spiral down and fall into the sun or crash into each other. And by 'enough' I mean many times over the actual time the system will last before the Sun goes red giant and vaporises the Earth anyway.
 
micropulsar said:
We see in our solar system the planets orbiting the sun, but why doesn't with all of the other forces in play the perpendicular velocity seemingly not decrease(or does it?). And if the perpendicular velocity of the planets slow down would that result in static planets not moving around the sun?

What do you mean by pendicular velocity? If you mean the component of the velocity perpendicular to a line passing through the sun and the planet, it does change. If you're expecting the planets to slow down due to some effect, ask yourself why.
 
A force perpendicular to the direction of motion merely changes the direction, not the speed. Moreover, energy is conserved, so the only way for orbits to slow down is by radiating something, such as gravitational waves, which are really, really, really weak.
 
Khashishi said:
A force perpendicular to the direction of motion merely changes the direction, not the speed.

Right. But it's very rare that the force is perpendicular to the direction of motion.

Moreover, energy is conserved, so the only way for orbits to slow down is by radiating something, such as gravitational waves, which are really, really, really weak.

When an orbiting planet slows down it's kinetic energy decreases, but the potential energy of the planet-sun system increases. And vice-versa. It's happening in our solar system as we speak.
 
Gan_HOPE326 said:
Well, I imagine given enough time the combination of friction from interstellar particles/gas and many-body effects, even without counting the possibility of some rogue body entering the system and altering its equilibrium, would slow down orbits and make the planets spiral down and fall into the sun or crash into each other. And by 'enough' I mean many times over the actual time the system will last before the Sun goes red giant and vaporises the Earth anyway.

In general can we say that planets are in perpetual motion and as man made perpetual motion devices fail after some time of workout, the planets will also crash down after calculated time depending on all of the forces in action even if sun does not blast?
 
  • #10
electro-physics said:
In general can we say that planets are in perpetual motion and as man made perpetual motion devices fail after some time of workout, the planets will also crash down after calculated time depending on all of the forces in action even if sun does not blast?

In theory nothing prevents a conservative system to move perpetually as long as nothing extracts energy. In practice of course this is never perfectly true - planets exchange energy with the environment in small ways (including stuff like meteor impacts), so I suppose on the long, long, LONG run they will lose their orbits. Not a "calculated" time because there's nothing strictly predictable about it. Yes, the orbit's stability itself is somewhat of an approximation since the exact solution to the many-body problem isn't known, but that doesn't mean that the planets ought to crash - the energy is there and if nothing takes it away then the orbits' shapes might change but the total energy should be conserved, and therefore something would probably keep orbiting more or less forever.
 
  • #11
Gan_HOPE326 said:
Yes, the orbit's stability itself is somewhat of an approximation since the exact solution to the many-body problem isn't known, but that doesn't mean that the planets ought to crash - the energy is there and if nothing takes it away then the orbits' shapes might change but the total energy should be conserved, and therefore something would probably keep orbiting more or less forever.

There are tidal forces that generate a conversion of mechanical energy to thermal energy.
 
  • #12
Mister T said:
There are tidal forces that generate a conversion of mechanical energy to thermal energy.

Right, didn't think of that. So there's that too. Also orbiting bodies radiate gravitational waves I believe? So if we go from Newton to Einstein we have another source of energy loss which prevents orbits from being eternal.
 

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