Planetary Orbits in AU - Stability & Mass Limits

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Discussion Overview

The discussion revolves around the stability of planetary orbits within a star system, specifically focusing on the potential for multiple planets to exist in the habitable zone between 0.7 AU and 1.5 AU. Participants explore the mass limits of these planets, comparing them to Mercury and Mars, and consider the gravitational interactions that may affect their orbits.

Discussion Character

  • Debate/contested
  • Exploratory
  • Technical explanation

Main Points Raised

  • Some participants propose that multiple planets could exist in the habitable zone, suggesting that orbital resonances might stabilize such a system.
  • Others argue that the gravitational interactions between two planets in the narrow habitable zone would likely lead to instability, making it improbable for them to coexist without destabilizing each other.
  • A participant points out that while Venus and Mars are within the habitable zone, they are not considered habitable due to atmospheric conditions and other factors.
  • Another participant provides online calculators to assess the stability of orbits, indicating that Earth destabilizes the region from 0.95 to 1.05 AU.
  • There is a request for peer-reviewed references to support claims about the possibility of multiple planets in the habitable zone, emphasizing the need for valid sources in the discussion.

Areas of Agreement / Disagreement

Participants express differing views on the feasibility of multiple planets existing in the habitable zone, with no consensus reached on the stability of such configurations. The discussion remains unresolved regarding the conditions under which multiple planets could coexist without destabilizing each other.

Contextual Notes

Limitations include assumptions about the gravitational interactions between planets and the specific conditions required for stability in the habitable zone. The discussion also depends on the definitions of habitability and the parameters used in the stability calculations.

QuantumPowered
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All of the planets should have individual orbits, and should be between the mass of Mercury and Mars. What can their orbits be in AU's? Is there a way to find out how close they can be without destabilizing each other? If we assume the star is about the same size as Sol.
 
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QuantumPowered said:
All of the planets should have individual orbits, and should be between the mass of Mercury and Mars. What can their orbits be in AU's? Is there a way to find out how close they can be without destabilizing each other? If we assume the star is about the same size as Sol.

have a look at our own solar system as an example. Considering that the habitable zone is relatively narrow, I would suggest that it's likely to be only one, with maybe the possibility of 2 planets sharing the same orbit but on opposite sides of the orbit ( and I'm not really sure that that scenario can exist ?)D
 
I think it is likely to be more than one, if we assume the habitable zone stretches from 0.7 AU to 1.5 AU.
 
QuantumPowered said:
I think it is likely to be more than one, if we assume the habitable zone stretches from 0.7 AU to 1.5 AU.

you miss the point

you wouldn't get 2 planets orbiting within that narrow zone and still have stable orbits
not going to happen, there would be too much gravitational interaction between the 2
 
No I'm not "missing the point", it is possible to get two or more planets in that zone. Venus orbits at 0.72 AU, Earth at 1.00 AU, and Mars at 1.52 AU. It should be possible to have multiple lower mass planets orbiting at similar distances from 0.7 AU to 1.5 AU, orbital resonances could stabilize such a system.
 
but Venus is far from being habitable
and Mars isn't much better
 
Mars is believed to have lost most of its atmosphere because of the lack of a magnetic field, and also asteroid impacts. With a thicker atmosphere and a magnetic field Mars would be habitable. The temperatures on Venus aren't caused by the closer distance to the sun, it is entirely related to the atmosphere, also the slow rotation leading to no magnetic field. A planet with a thinner atmosphere, magnetic field and a limited water reserve would be habitable at that distance.
 
Welcome to the PF.
QuantumPowered said:
No I'm not "missing the point", it is possible to get two or more planets in that zone.
Such an assertion requires a reference to a peer-reviewed publication about it. That's in the PF rules. Can you please provide such a link?

You started this thread with a question, which is fine. But turning around and making assertions requires valid references.
 
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