Planetary orbits -- Why do planets orbit at same “level”?

In summary, all of the planets in our solar system orbit the sun in a roughly similar orbital plane because this is the way the solar system formed from a collapsing cloud of material. The planets are also constrained to orbit in this plane unless they are perturbed significantly by planetary-sized objects.
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Josh0768
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TL;DR Summary
Why do planets orbit at same “level”?
Why is it that all of the planets in our solar system (to our knowledge) orbit the sun in such a way that they all go around the sun in roughly similar orbital planes? Why don’t we have planets with orbital planes at significantly different angles?
 
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Heritage of their origin from a rotating cloud of material in the form of a disk.
 
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As BillTre said, the solar system formed from a collapsing cloud of material that collapses into a disk. The center of this disk collapses further to become the Sun, and other areas collapse into proto-planetary bodies. By nature of their initial position as part of this disk, the resulting planets are constrained to closely orbit in a plane unless they are perturbed significantly by planetary-sized objects, which is extremely rare.
 
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Also Kozai resonance.
Bodies that orbit at large angle to other bodies are liable to large perturbations that change their orbits to something else.
There are such bodies, like comet Hale-Bopp. But those are long period comets, that rarely enter into inner solar system to get perturbed again. Periodic comets don´ t last on high inclination orbits, and neither would planets.
 
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Josh0768 said:
Summary:: Why do planets orbit at same “level”?

Why is it that all of the planets in our solar system (to our knowledge) orbit the sun in such a way that they all go around the sun in roughly similar orbital planes? Why don’t we have planets with orbital planes at significantly different angles?
Try this to start:



The flattening happened quite early in the solar system's development.
 
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Note that Kozai resonance only operates for large inclinations.
It does NOT operate for low inclination but retrograde objects. Which is why Halley comet is periodic - being at a low inclination orbit, it does not suffer from Kozai resonance. It is only comet sized, though - not a planet.
Of hot jupiters, a third (sic!) orbit retrograde to the rotation of star. How are the conditions about multiplanet systems? Has any multiplanet system yet been confirmed to contain planets orbiting in opposite directions? Solar System planets have been confirmed to orbit in the same direction, but any others?
 

1. How do planets stay in their orbits?

Planets stay in their orbits due to the balance between the gravitational pull of the sun and the planet's own inertia. The sun's gravity pulls the planet towards it, while the planet's inertia keeps it moving forward. This results in a circular or elliptical orbit around the sun.

2. Why do planets orbit in the same plane?

Planets orbit in the same plane because they were formed from a rotating disk of gas and dust around the young sun. This disk was already in a flat plane, and as the planets formed from it, they inherited this same orbital plane.

3. What determines the speed of a planet's orbit?

The speed of a planet's orbit is determined by its distance from the sun and its mass. The farther a planet is from the sun, the slower it will orbit. Similarly, a more massive planet will have a slower orbit compared to a less massive planet at the same distance from the sun.

4. Can a planet's orbit change over time?

Yes, a planet's orbit can change over time due to various factors such as gravitational interactions with other planets, asteroids, or comets. These interactions can cause a planet's orbit to become more elliptical or even change its orbital plane.

5. Do all planets orbit in the same direction?

No, not all planets orbit in the same direction. While most planets in our solar system orbit counterclockwise, Venus and Uranus have retrograde orbits, meaning they orbit in the opposite direction. This is believed to be due to past collisions or gravitational interactions with other objects in the solar system.

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