Planetary Orbits & Orbital Velocity

In summary, the orbital velocity increases as you get closer to the sun because the gravitational field is greater, requiring a higher velocity to remain in orbit. This is due to the larger mass of the sun and the resulting stronger force between the sun and the planet. However, because the planet is also more massive, it requires a stronger centripetal force to maintain its orbit. If all planets had the same mass, the force would decrease with increasing distance from the sun. Additionally, the barycenter of the Jupiter-Sun system causes the sun to wobble as Jupiter orbits around it.
  • #1
Jimmy87
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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?
 
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  • #2
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.
 
  • #3
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.
 
  • #4
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.
 
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  • #5
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
 
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What is a planetary orbit?

A planetary orbit is the path an object takes around a star, planet, or other celestial body due to the force of gravity. In our solar system, the planets orbit around the sun.

What is orbital velocity?

Orbital velocity is the speed at which an object moves in its orbit around another object. It is determined by the mass of the two objects and the distance between them.

How is orbital velocity calculated?

The formula for calculating orbital velocity is V = √(GM/R), where V is the orbital velocity, G is the gravitational constant, M is the mass of the central object, and R is the radius of the orbit.

What factors affect orbital velocity?

The main factors that affect orbital velocity are the mass of the central object and the distance between the objects. The larger the mass of the central object, the faster the orbital velocity. The farther the distance between the objects, the slower the orbital velocity.

Why is orbital velocity important?

Orbital velocity is important because it determines the stability and shape of a planetary orbit. If the orbital velocity is too low, an object will crash into the central object. If it is too high, an object will escape the gravitational pull and fly off into space.

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