Orbits of objects of equal mass

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The discussion focuses on the types of stable orbits for sets of objects of equal mass, specifically addressing configurations of one, two, and three or more bodies. It establishes that with one object, the state is stationary, while two objects rotate around a common center at equal speeds. For three or more objects, the orbits become complex, but there are special cases, such as the Moon and Earth in relation to the Sun, that exhibit simpler orbital patterns. The conversation emphasizes the need for a generalization of these orbits and potential visualization methods.

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What basic types of stable orbits are there for sets of objects of equal mass?

For example,
with one object it would just be stationary,

with two objects they would rotate at equal speed around a common centre with a constant distance between them (and more complicated stable orbits where the distance oscillates).

What about with three objects and more?

I assume for each set there would be an orbit where each object moves around the common centre of gravity in some fashion, such that from the perspective of each object the movement of the other objects is the same. What other types of basic stable orbits are there?

What would be the best way to generalise all the types of orbits for each number of objects?

Is there a way to visualise these types of orbits?

If anyone can provide any other examples at all, or answer any of these questions, that would be great.
 
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Orbits of three or more bodies that attract each other via gravitational force may be very complicated.

There are some special cases for which three or more bodies can follows some simple orbits, like the motion of Moon and Earth in the reference frame of the Sun.

Perhaps here you can find some interesting reading on the topic:

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