How orbiting bodies arrange themselves in orbital resonance?

In summary, the conversation discusses the mechanics behind orbital resonances, particularly in regards to the Galilean moons of Jupiter. It is mentioned that these resonances can occur due to gravitational perturbations and have a self-correcting feature to maintain the correct speed and distance between orbiting bodies. The concept of clearing the neighborhood and the exchange of angular momentum is also brought up. It is noted that the understanding of complex resonances is still a challenge in the n-body problem, but resources such as the book "Solar System Dynamics" can provide more information on the topic.
  • #1
Neghentropia
18
0
Hi guys,
my first post here :)

lately I've been trying to understand how orbiting bodies (i.e. galileian moon of Jupiter) have arranged themselves in resonance

the 1:1 resonance is pretty straightforward to understand. but more complex relations like the one I cited above, how do they take place?



cheers
 
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  • #2
I would guess that they are either formed in such resonances, or are driven there by gravitational perturbations and once in the resonance they are stable.
 
  • #3
hi Drakkith, thanks for the reply

could you explain better how these gravitational perturbations take place?
I'm really curious to understand the mechanics behind the phenomenon
also, I'd like to introduce in the discussion the subject of clearing the neighbourhood which, as far as I understood, is strongly linked with resonance

in particulr, how does the gravitational field of a planet (Jupiter) both arranges in resonance its moons and clears, for example, the asteroids belt from layers upon layers os asteroids?
how does this duplex push-pull effect of gravity take place?
 
  • #4
I couldn't possible go into the details, as I don't know them, however I can say that certain orbits just happen to be stable orbits, resonances being some of them. Those bodies that aren't in stable orbits, well, don't stay in orbit! Resonances have a sort of self-correcting feature, where the orbiting bodies in resonance tug on each other in just the right ways to keep them at the right speed at the right distance. If one object starts to pull slightly ahead of the other, perhaps due to interactions with other objects, it's pulled back when they get close to each other, and vice-versa. There's no real "reason" behind this other than it's simply a result of gravity pulling on objects in certain ways.

That's about the best I could explain it. I'm sure I've butchered it enough for now, so I'll let someone else who's far more familiar with orbital mechanics take it from here.

See this article for more: http://en.wikipedia.org/wiki/Orbital_resonance
 
  • #5
mhh...

the picture is getting clearer.
and I mean that I'm given to understand the reason of complex resonances is not well understood (n-body problem)

on the other, I hand't considered that orbiting bodies can exchange angular momentum, which explain why a planet can eject an asteroid (or another planet...) from its orbit.
 
  • #6
I would advise getting a hold of Solar System Dynamics by Murray and Dermott since there's a lot on resonance and the disturbing function in the book. Since it focuses on the solar system, it covers Jupiters moons, Saturns rings, etc...
 
  • #7
thanks.
I'll give a look in the library. I may be luckyEdit: I am lucky! :)
I'll try to get hold of a copy tomorrow

cheers!
 

1. How do orbiting bodies arrange themselves in orbital resonance?

In orbital resonance, orbiting bodies arrange themselves in a specific pattern or ratio of orbits. This occurs when the orbital periods of two or more bodies are related by a simple mathematical ratio, such as 2:1 or 3:2. This means that for every two orbits of one body, the other body completes one orbit.

2. What factors influence orbital resonance?

The main factor that influences orbital resonance is the gravitational pull between the orbiting bodies. This pull causes a slight perturbation in the orbit of each body, which can lead to a resonance effect over time. Other factors that can influence orbital resonance include the shape and size of the orbiting bodies, as well as the presence of other nearby objects.

3. What are some examples of orbital resonance in our solar system?

One example of orbital resonance in our solar system is the relationship between Jupiter's moons Ganymede, Europa, and Io. They are in a 1:2:4 orbital resonance, meaning that for every orbit Ganymede completes, Europa completes two and Io completes four. Another example is the Pluto-Charon system, where Charon's orbital period is exactly half that of Pluto's.

4. Can orbital resonance have any negative effects?

Orbital resonance can have both positive and negative effects. In some cases, it can help stabilize the orbits of the bodies involved, preventing collisions and maintaining the overall structure of the system. However, it can also lead to instabilities and disruptions in the orbits, which can eventually result in collisions or ejections from the system.

5. How do scientists study orbital resonance?

Scientists study orbital resonance using a variety of methods, including mathematical modeling and computer simulations. They also observe the orbits of celestial bodies using telescopes and other instruments, and analyze data from spacecraft missions to gather more information about the dynamics of orbital resonance. Additionally, laboratory experiments and simulations can be used to mimic the conditions of orbital resonance and test different scenarios.

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