Stability of Counter-Planets: Examining the Possibility of Dual Planetary Orbits

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Discussion Overview

The discussion explores the theoretical possibility of two planets orbiting a star in a counter configuration, specifically addressing the stability of such an arrangement. Participants examine the implications of orbital physics and the concept of Lagrange points in relation to this scenario.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant questions the feasibility of two planets orbiting opposite each other, referencing the "Counter-Earth" theory and its implications for science fiction.
  • Another participant argues that the likelihood of such a configuration is extremely low, suggesting that differing distances from the star would lead to eventual collision.
  • A participant introduces the concept of metastability, comparing it to a pendulum and explaining that the discussed configuration is a metastable state that could easily be disrupted.
  • Further elaboration on Lagrange points indicates that the configuration in question (L3) is inherently unstable and would not persist under slight disturbances.
  • Some participants acknowledge the improbability of the initial configuration but suggest that in an infinite universe, such scenarios could be imagined, albeit with concerns about their long-term stability.
  • Clarifications are made regarding the stability of Lagrange points, emphasizing that collinear points are unstable regardless of mass ratios.

Areas of Agreement / Disagreement

Participants express differing views on the stability of the proposed planetary configuration, with some asserting that it is unlikely to be stable while others acknowledge the theoretical possibility but highlight significant challenges. No consensus is reached on the viability of the concept.

Contextual Notes

Participants note that the initial conditions required for such a configuration are astronomically improbable, and the discussion hinges on the definitions and assumptions surrounding stability and the nature of Lagrange points.

Nentuaby
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Is it possible to have two planets orbiting opposite each other across their star? Either with the two being of roughly equal mass, or with one giant planet and one terrestrial?

Everyone's heard of the old "Counter-Earth" theory, which of course is wrong, but I was wondering if given our current understanding of orbital physics it could have been right, or if the configuration just can't be stable. Could make a good element for some hard science fiction, but sadly my layman's knowledge isn't enough to know whether using it would end up with me dumped in the "Dan Brown pile." ;)
 
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It's so unlikely that it's ridiculous. Is it possible that 5 comets could collide into each other at once? Yes, it's possible.
The planets would likely differ in their distances from the star by some amount and would eventually collide.
Even how such exact positions could come to be by any natural formative process is beyond improbable.
 
The configuration is metastable. What that term means: Think of a pendulum, a long rod suspended from one end. The pendulum has one stable configuration and one metastable configuration. The stable configuration is with the pendulum oriented vertically and the suspension point at the top of the pendulum. The metastable configuration is with the pendulum oriented vertically and the suspension point at the bottom of the pendulum. If the pendulum is perfectly vertical it will stay in this metastable state. The slightest disturbance will make it tip. Another word for metastable is unstable.

There are two stable and three metastable states for a pair of objects orbiting a star. These configurations are called the Lagrange points. (Google that phrase.) The star and the two objects are collinear in the three metastable configurations. The configuration discussed in the original post is the L3 configuration. Suppose a counter Earth did somehow come into being. That configuration would not last very long. All it takes is the slightest of nudges to knock the Earth and counter Earth out of that configuration. The gravitational influence of a comet out beyond Pluto would suffice to provide the nudge.
 
D H said:
There are two stable and three metastable states for a pair of objects orbiting a star. These configurations are called the Lagrange points. (Google that phrase.) The star and the two objects are collinear in the three metastable configurations. The configuration discussed in the original post is the L3 configuration. Suppose a counter Earth did somehow come into being. That configuration would not last very long. All it takes is the slightest of nudges to knock the Earth and counter Earth out of that configuration. The gravitational influence of a comet out beyond Pluto would suffice to provide the nudge.

I do know the L points. As I understood it, the body in the Lagrangian orbit must be much smaller than the primary body for the system to be stable. You're saying, though, that L3 is not actually stable regardless of the ratio of masses?

And Helios, I'm aware the initial configuration is astronomically improbable. It is, however, an infinite universe. As a story element it was meant to be something of a wonder; I'm only really concerned with whether it can continue, or would fly apart inevitably.
 
Nentuaby said:
It is, however, an infinite universe.
Well, no it isn't, but your point is made.
 
Nentuaby said:
I do know the L points. As I understood it, the body in the Lagrangian orbit must be much smaller than the primary body for the system to be stable. You're saying, though, that L3 is not actually stable regardless of the ratio of masses?

The collinear Lagrange points are always unstable. Even the triangular Lagrange points are only stable if the mass of the third body is very small.
 
I see. I'll have to abandon that idea, then. Thanks for the help.
 

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