Is Velocity Consistent in Planetary Orbits?

In summary, the speed of different bodies in the same planetary orbit is not necessarily equal to each other. This is because the acceleration and force of gravity can vary depending on the mass and distance of the objects involved. Additionally, the orbit can change when the mass of an object changes due to the shifting of the barycenter, which affects the necessary velocity to maintain a circular path.
  • #1
AakashPandita
157
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Is the speed of different bodies in the same planetary orbit equal to each other?
I think it should be the same because the acceleration is always the same in such a case.

But it was not so when i compared the speed of moon per m/s with that of the international space station.
 
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  • #2
AakashPandita said:
Is the speed of different bodies in the same planetary orbit equal to each other?

yes

AakashPandita said:
But it was not so when i compared the speed of moon per m/s with that of the international space station.

not the same orbit
 
  • #3
The Moon is MUCH further away than the ISS. The ISS orbits between about 375 - 400 km from Earth's surface while the moon has an average orbital radius of about 384,000 km. So the Moon is about 1000 times further away than the ISS is.
 
  • #4
sorry..actually i intended to ask why the speed of the ISS as well as the moon is not the same...they are both accelerated and have the same "g".
 
  • #5
The accelerations are not the same. The force of gravity drops off as 1/r^2, and since the moon is about 60 times farther from the Earth's center than the ISS, its acceleration is about 1/3600 as large.
 
  • #6
AakashPandita said:
Is the speed of different bodies in the same planetary orbit equal to each other?
In general, NO.
I think it should be the same because the acceleration is always the same in such a case.
You are ignoring that the orbiting body also attracts the body that it is orbiting. That the Earth is many orders of magnitude more massive than even the biggest artificial satellite orbiting the Earth means that the acceleration of the Earth toward these artificial satellites will be negligible; two artificial satellites in the same orbit will have the same period. That the Moon is about 1/81 the mass of the Earth means that the acceleration of the Earth toward the Moon is not negligible.

Kepler's third law is only approximately correct. A better formula for the period at which two objects, one of mass M and the other of mass m, orbit one another is

[tex]P=2\pi\sqrt{\frac{a^3}{G(M+m)}}[/tex]
 
  • #7
D H said:
AakashPandita said:
Is the speed of different bodies in the same planetary orbit equal to each other?
In general, NO.

With different velocities it wouldn't be the same orbit.
 
  • #8
DrStupid said:
With different velocities it wouldn't be the same orbit.
Yes, it would. Consider the Moon. Suppose you magically replace the Moon with an object several orders of magnitude smaller in mass than the Moon but keep the position and velocity the same as the Moon's. This object will be in a different orbit. To get the same orbit as the Moon's current orbit you will have to change the velocity.

This is an important consideration in the formation of a planetary system from an accretion disk. Given a planetesimal in a circular orbit of radius a about a nascent star amidst some particles orbiting at the same distance, the planetesimal will be moving slightly faster than the individual particles. The planetesimal will have an orbital velocity of [itex]\sqrt{G(M+m)/a}[/itex] where M is the mass of the nascent star and m is the mass of the planetesimal; the orbital velocity small particles co-orbiting with the planetesimal will only be [itex]\sqrt{GM/a}[/itex]. The planetesimal will plow through and sweep up the surrounding particles. This can lead to the planetesimal migrating toward the star.
 
  • #9
Why would the orbit change when the mass of the object changes? Is it because of the objects reduced attraction of the Earth towards it?
 
  • #10
Drakkith said:
Why would the orbit change when the mass of the object changes? Is it because of the objects reduced attraction of the Earth towards it?

Because both the object and the Earth actually orbit their common barycenter.

As mass of the object increases, the barycenter moves closer to the object and away from the center of the Earth. The radius of its orbit around the barycenter decreases, while the distance between object and Earth remains the same.. Since the centripetal force needed to maintain a circular path is equal to

[tex]\frac{mv^2}{r}[/tex]

A decease in v is needed to maintain the same object-Earth distance.
 
  • #11
Ah ok, that makes sense Janus. Thanks.
 
  • #12
Janus said:
Because both the object and the Earth actually orbit their common barycenter.

As mass of the object increases, the barycenter moves closer to the object and away from the center of the Earth.
how?
wouldn't the distance from the barycenter remain the same when mass increases?
 
  • #13
D H said:
DrStupid said:
With different velocities it wouldn't be the same orbit.
Yes, it would.

Is the orbit really characterized by its shape of the only?
 
  • #14
AakashPandita said:
how?
wouldn't the distance from the barycenter remain the same when mass increases?

No, as the object would pull the Earth towards it more than it did before, hence the barycenter would move.
 
  • #15
:approve:
 

1. What is velocity in planetary orbits?

Velocity in planetary orbits is the speed at which a planet moves along its orbital path around the sun. It is measured in units of distance per time, such as kilometers per hour or miles per second.

2. How is velocity related to the size and shape of planetary orbits?

The velocity of a planet in its orbit is influenced by its distance from the sun (size of the orbit) and the shape of its orbit. Planets closer to the sun tend to have higher velocities, as they are affected by the sun's gravitational pull more strongly. The shape of the orbit can also affect the velocity, as planets in elliptical orbits have varying speeds as they move closer or further away from the sun.

3. How is velocity calculated in planetary orbits?

Velocity in planetary orbits can be calculated using the formula v = √(GM/r), where v is velocity, G is the gravitational constant, M is the mass of the sun, and r is the distance between the planet and the sun. This formula is derived from Newton's law of universal gravitation.

4. Can velocity change in planetary orbits?

Yes, the velocity of a planet in its orbit can change. This can happen due to the gravitational influence of other planets, as well as external forces such as comets or asteroids passing nearby. Additionally, changes in a planet's orbit, such as becoming more circular or elliptical, can also affect its velocity.

5. How does velocity affect the duration of a planetary orbit?

Velocity is directly related to the duration of a planetary orbit. The higher the velocity, the shorter the orbital period, or the time it takes for a planet to complete one full orbit around the sun. This is because a higher velocity means the planet is moving faster and covering more distance in a given amount of time.

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