Planetary Orbits in AU - Stability & Mass Limits

In summary, it is possible to have multiple planets orbiting within the habitable zone of a star, with orbital resonances stabilizing the system. This is demonstrated by the example of Venus, Earth, and Mars in our own solar system. However, it is important to consider factors such as atmospheric composition, magnetic fields, and water reserves when determining a planet's habitability. It is also necessary to consult peer-reviewed publications when making assertions about planetary systems.
  • #1
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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  • #2
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
 
  • #3
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.
 
  • #4
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
 
  • #5
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.
 
  • #6
but Venus is far from being habitable
and Mars isn't much better
 
  • #7
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.
 
  • #9
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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1. What is the significance of AU in planetary orbits?

AU stands for astronomical unit and is used as a unit of measurement to describe the distance between objects in space. It is defined as the average distance between the Earth and the Sun, which is about 149.6 million kilometers (93 million miles). This unit is commonly used in astronomy and is particularly useful in describing the distances between planets and their orbits.

2. How do planetary orbits remain stable?

Planetary orbits remain stable due to the gravitational force between the planet and the star it is orbiting. This force keeps the planet in a relatively stable orbit, and any slight deviations from this orbit can be corrected by the gravitational pull of the star. Additionally, the laws of motion and gravity, as described by Isaac Newton, help to maintain the stability of planetary orbits.

3. What factors affect the stability of planetary orbits?

The stability of planetary orbits can be affected by various factors, such as the mass and distance of the planet from its star, the presence of other nearby planets, and external forces like comets or asteroids. If the planet is too close to its star, it can be pulled in by the star's gravity, and if it is too far away, it may be ejected from its orbit.

4. Is there a limit to the mass of a planet that can have a stable orbit?

Yes, there is a limit to the mass of a planet that can have a stable orbit. This limit is known as the Roche limit and is determined by the balance between the planet's gravitational force and the tidal forces of its star. If the planet's mass exceeds the Roche limit, it may break apart or merge with its star.

5. How do scientists study the stability of planetary orbits?

Scientists use computer simulations and mathematical models to study the stability of planetary orbits. They also observe and analyze data from telescopes and spacecraft to gather information about the properties of planets and their orbits. Additionally, studies of exoplanets, which are planets outside of our solar system, provide valuable insights into the stability of planetary orbits and the factors that can affect them.

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