Planetary Orbits & Orbital Velocity

Click For Summary

Discussion Overview

The discussion revolves around the relationship between planetary orbits and orbital velocity, specifically why orbital velocity increases as planets get closer to the Sun. Participants explore concepts related to gravitational forces, centripetal acceleration, and the effects of planetary mass on orbital dynamics.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • One participant notes that while Jupiter is further from the Sun and has a slower orbital velocity, it experiences a stronger gravitational force due to its mass.
  • Another participant agrees and explains that Jupiter's greater mass requires a stronger centripetal force for its orbit, leading to a more complex interaction with the Sun.
  • There is a discussion about the concept of dividing out the mass of the planet when considering gravitational interactions, with some suggesting that the barycenter of the Jupiter-Sun system affects their motion.
  • A clarification is made that it is more accurate to say that the gravitational field is greater closer to the Sun, necessitating a higher velocity for planets to maintain their orbits.
  • A mathematical expression for orbital velocity is provided, emphasizing the relationship between gravitational acceleration and orbital radius.

Areas of Agreement / Disagreement

Participants generally agree on the principles of gravitational force and centripetal acceleration but express different nuances regarding the terminology and implications of these concepts. The discussion remains unresolved regarding the precise nature of the relationship between mass, gravitational pull, and orbital velocity.

Contextual Notes

Some assumptions about the negligible mass of planets compared to the Sun are mentioned, and the discussion does not resolve the complexities of gravitational interactions in multi-body systems.

Jimmy87
Messages
692
Reaction score
19
Hi pf, please could someone explain why the orbital velocity increases as you get closer to the sun. I treated the situation like circular motion and did a load of calculations. I calculated the orbital velocity of all 8 planets and then the force between each of the eight planets and the sun. I thought the force would drop off as you for further away which would explain the slower orbital velocity but that isn't the case. For instance, Jupiter is 5 times further away than Earth, has a much slower orbital velocity but has a stronger gravitational pull from the Sun.

The only thing I can think of is dividing out the mass of the planet. So although Jupiter has a greater gravitational force (despite orbiting slower) it is much more massive so will require a bigger force even to orbit at this slower speed. Or to put it another way if all 8 planets had the same mass as each other then the force would decrease for all planets with increasing distance. Is that right?
 
Astronomy news on Phys.org
Jimmy87 said:
The only thing I can think of is dividing out the mass of the planet. So although Jupiter has a greater gravitational force (despite orbiting slower) it is much more massive so will require a bigger force even to orbit at this slower speed. Or to put it another way if all 8 planets had the same mass as each other then the force would decrease for all planets with increasing distance. Is that right?

Yes, you have it basically right. Jupiter is more massive and so feels a stronger force between it and the Sun; however, because it is more massive, it requires a stronger centripetal force to give it the right centripetal acceleration for its orbit. You can "divide out" the mass of the Jupiter as long as you are not considering the reaction force on the Sun. The effect of Jupiter's large mass on the Sun means that both Jupiter and the Sun orbit the barycenter of the Jupiter-Sun system. The Barycenter is located within the Sun, but is not at the center of the Sun, so the Sun actually wobbles as Jupiter orbits around it.
 
Matterwave said:
Yes, you have it basically right. Jupiter is more massive and so feels a stronger force between it and the Sun; however, because it is more massive, it requires a stronger centripetal force to give it the right centripetal acceleration for its orbit. You can "divide out" the mass of the Jupiter as long as you are not considering the reaction force on the Sun. The effect of Jupiter's large mass on the Sun means that both Jupiter and the Sun orbit the barycenter of the Jupiter-Sun system. The Barycenter is located within the Sun, but is not at the center of the Sun, so the Sun actually wobbles as Jupiter orbits around it.

Thanks for the answer. So is it correct to still say that planets orbit faster closer to the Sun because the pull from the Sun is greater so they need to move quicker to remain in orbit.
 
Jimmy87 said:
Thanks for the answer. So is it correct to still say that planets orbit faster closer to the Sun because the pull from the Sun is greater so they need to move quicker to remain in orbit.

Not the "pull is greater", but the "gravitational field is greater" so they must have a higher velocity to remain in orbit.
 
  • Like
Likes   Reactions: Jimmy87
Treating all the planet masses as negligible (which they are compared to the sun), and dealing with gravitational accelerations only, you can simplify the velocity calculation of any orbiting planet to :
v = sqrt ( ( G * M ) / r )
Where :
G = 6.674 E-11 (a constant)
M = suns mass in kg
r = planet orbital radius in meters
 
  • Like
Likes   Reactions: Jimmy87

Similar threads

  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 84 ·
3
Replies
84
Views
7K
  • · Replies 11 ·
Replies
11
Views
2K
  • · Replies 58 ·
2
Replies
58
Views
6K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 9 ·
Replies
9
Views
3K
  • · Replies 2 ·
Replies
2
Views
3K
  • · Replies 27 ·
Replies
27
Views
4K
  • · Replies 86 ·
3
Replies
86
Views
9K
  • · Replies 7 ·
Replies
7
Views
2K