The Same Plane: Orbits & Galaxies in Our Solar System

In summary, the reason why orbiting planets and galaxies tend to be in a 2D plane is still unknown. However, it is believed that the torques from nearby objects during their formation cause them to rotate faster and collapse into a disk shape due to conservation of angular momentum and loss of energy through radiative cooling.
  • #1
scott_alexsk
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Why is it that for the most part, all orbiting planets in our solar system orbit together on the same 2D plane. The same can be asked for the disk shape of all of the galaxies. (sp everywhere)
Thanks,
-scott
 
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  • #2
The short answer is that we don't know. The formation of disks on either galactic or planetary scales are extremely difficult to do because they require your simulation to have a huge dynamic range.

The long and crude answer is that the progenitors to these objects (molecular clouds and cosmological overdensities) can be given small torques by the tidal fields of other nearby objects. This causes the entire progenitor to rotate slowly in some arbitrary direction. Then, as it collapses gravitationally, angular momentum must be conserved and the cloud/overdensity begins to rotate more quickly. This rotation produces a strong asymmetry (along the axis of rotation) in the dynamical system. This system tends to conserve angular momentum about the rotation axis, but lose energy to radiative cooling. The net effect is contraction into a disk rotating roughly about the axis created by the original torque.
 

FAQ: The Same Plane: Orbits & Galaxies in Our Solar System

1. What is an orbit?

An orbit is the path that an object takes as it revolves around another object in space, such as a planet orbiting around a star.

2. How are orbits formed?

Orbits are formed due to the gravitational force between two objects. The larger object, such as a star, exerts a force on the smaller object, causing it to continuously move in a circular or elliptical path around the larger object.

3. What is the difference between a circular and elliptical orbit?

A circular orbit is a perfectly round path that an object takes around another object, while an elliptical orbit is a more elongated path with varying distances between the two objects. In our solar system, most planets have elliptical orbits around the sun.

4. How do galaxies form?

Galaxies are formed when large amounts of gas, dust, and stars are pulled together by gravity. The shape and size of a galaxy can vary depending on the amount of matter and the strength of the gravitational force.

5. Can orbits change over time?

Yes, orbits can change over time due to various factors such as the gravitational pull of other objects, collisions with other objects, or even the expansion of the universe. These changes can cause orbits to become more elliptical or even completely change direction.

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