Question about Orbits of Moon/Earth around Sun

  • Context: Undergrad 
  • Thread starter Thread starter Zarhult
  • Start date Start date
  • Tags Tags
    Orbits Sun
Click For Summary

Discussion Overview

The discussion centers on the mechanics of the Moon's orbit around the Earth while both bodies move in their orbit around the Sun. Participants explore the gravitational influences at play and the implications for orbital stability at various scales, including the solar system and the Milky Way galaxy.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • One participant questions how the Moon can maintain its orbit around the Earth while both are influenced by the Sun's gravity, noting that the net force on the Moon is not purely centripetal.
  • Another participant explains that the Moon's orbit is affected by both the Earth's and the Sun's gravitational forces, but these effects cancel out as the Moon and Earth orbit their barycenter.
  • It is suggested that during different parts of the Moon's orbit, it moves at varying speeds relative to its orbit around the Sun, but these variations balance out over time.
  • Discussion includes the idea that gravitational interactions among planets were significant in the early solar system, causing many objects to change orbits, which contributed to the formation of planets.
  • One participant notes that the Sun's orbit around the Milky Way is influenced by interactions with other stars, leading to a semi-random path rather than a simple circular orbit.

Areas of Agreement / Disagreement

Participants express differing views on the implications of gravitational forces on orbits, particularly regarding the stability of the Moon's orbit and the effects of other celestial bodies. The discussion remains unresolved with multiple competing perspectives on the nature of these gravitational interactions.

Contextual Notes

Participants acknowledge that the gravitational influences from other planets are relatively small and that the stability of orbits is a complex issue influenced by historical interactions in the solar system.

Zarhult
Messages
33
Reaction score
2
How, exactly, is the moon able to orbit the Earth while at the same time moving with Earth's orbit of the Sun? I understand that the Earth/Moon both have the same accelerations caused by the Sun's gravity, but accelerations are not additive - only forces. At any time, the moon will be pulled by both the Earth's gravitational force and the Sun's gravitational force, making the net force on the moon always slightly off from being purely a centripetal force around the Earth. Shouldn't this cause the moon to go off its orbit? This same thing can be applied at a larger scale - the moon goes around the Earth, which goes around the Sun, which goes around the center of the Milky Way. Why doesn't the net force, since there are more forces than only the Sun's pull, cause the planets and their moons to have their orbits messed up?
 
Astronomy news on Phys.org
Zarhult said:
At any time, the moon will be pulled by both the Earth's gravitational force and the Sun's gravitational force, making the net force on the moon always slightly off from being purely a centripetal force around the Earth. Shouldn't this cause the moon to go off its orbit?

It does. But as the Moon and the Earth circle around their barycenter, the effect ends up being canceled out. During half of its orbit around the Earth-Moon barycenter, the Moon is moving faster than necessary to stay in its orbit around the Sun. During the other half it is moving too slow. But like I said, the two cancel each other out.

Zarhult said:
This same thing can be applied at a larger scale - the moon goes around the Earth, which goes around the Sun, which goes around the center of the Milky Way. Why doesn't the net force, since there are more forces than only the Sun's pull, cause the planets and their moons to have their orbits messed up?

Well, in the case of the planets, the forces from other planets are too small to have a major effect on the Earth's orbit around the Sun. However, it's important to remember that all the planets are already in stable orbits. In the past, when the solar system was young and crowded with young proto-planets and other objects, gravitational interaction between these objects absolutely sent many of them out of their orbits and into new ones. That's the basic reason why planets can form in the first place. Gravitational interactions between many different objects gives them a chaotic orbit and many of them end up colliding with each other, building up larger and larger objects over time.

The Sun's path around the Milky Way is a bit different. You can't model the Milky Way as having a point-like source of gravity in the center like you can when modeling the solar system. Interactions with other stars gives the Sun a semi-random path around the galaxy. And by semi-random I mean that the general path of the Sun is around the center, but it dips above and below the plane, moves in and out a bit, and does other things as other stars pass nearby. Luckily the net effect tends to cancel out in the long run and we don't go flying off out of the plane of the galaxy or towards the center or something.
 
Drakkith said:
It does. But as the Moon and the Earth circle around their barycenter, the effect ends up being canceled out. During half of its orbit around the Earth-Moon barycenter, the Moon is moving faster than necessary to stay in its orbit around the Sun. During the other half it is moving too slow. But like I said, the two cancel each other out.
Well, in the case of the planets, the forces from other planets are too small to have a major effect on the Earth's orbit around the Sun. However, it's important to remember that all the planets are already in stable orbits. In the past, when the solar system was young and crowded with young proto-planets and other objects, gravitational interaction between these objects absolutely sent many of them out of their orbits and into new ones. That's the basic reason why planets can form in the first place. Gravitational interactions between many different objects gives them a chaotic orbit and many of them end up colliding with each other, building up larger and larger objects over time.

The Sun's path around the Milky Way is a bit different. You can't model the Milky Way as having a point-like source of gravity in the center like you can when modeling the solar system. Interactions with other stars gives the Sun a semi-random path around the galaxy. And by semi-random I mean that the general path of the Sun is around the center, but it dips above and below the plane, moves in and out a bit, and does other things as other stars pass nearby. Luckily the net effect tends to cancel out in the long run and we don't go flying off out of the plane of the galaxy or towards the center or something.
This helps, thanks!
 

Similar threads

  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 0 ·
Replies
0
Views
2K
  • · Replies 3 ·
Replies
3
Views
1K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 58 ·
2
Replies
58
Views
6K
  • · Replies 8 ·
Replies
8
Views
2K
  • · Replies 4 ·
Replies
4
Views
2K
Replies
17
Views
4K
  • · Replies 4 ·
Replies
4
Views
6K
  • · Replies 98 ·
4
Replies
98
Views
12K