Why most of the planetary orbits are ellipitical?

In summary: Simplified, because it's all maths:In summary, the elliptical orbits of planets are the result of the combined gravitational forces of other planets and stars.
  • #1
hongkongrubbish
6
0
theoretically by GMm/r^2 = mv^2/r, planets in a particular distance to the star will move in the corresponding velocity in order to maintain a circular orbit...
either over speed they will pass by the star, or under speed they will be attracted towards the star in a spiral way

So why are there elliptical orbits?
 
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  • #2
Circular is just a perfect case of eliptical.
In natue there is no such thing as a circle it only exists in mathermatics. Measured in enough detail, all circles will be slightly eliptical to some degree.
Planetary orbits are almost circular, the Earth's is only about 4% eliptical.

It is due to the effects of all the other planets both now and when the orbits were first forming.
 
  • #3
hongkongrubbish said:
theoretically by GMm/r^2 = mv^2/r, planets in a particular distance to the star will move in the corresponding velocity in order to maintain a circular orbit...
either over speed they will pass by the star, or under speed they will be attracted towards the star in a spiral way

So why are there elliptical orbits?

If a planet in a circular orbit increases its speed, it begins to climb away from the star. As it does so, it loses kinetic energy to make up for the gravitational potential it gains, and loses speed. At some point, v becomes small enough that GMm/r^2 > mv^2/r, and the planet begins to fall back in towards the star gaining velocity again. It eventually gains enough speed that GMm/r^2 < m^2/r and it starts climbing back out again(this will happen at its orginal distance from the star) till it reaches the distance where it starting falling in, and repeats the cycle. IOW, it enters a elliptical orbit with its starting distance as the periapis. The only way it will leave the star is if its velocity increase to 141.4% of that needed to maintain the circular orbit at its given distance. This is known as the escape velocity.

If the planet loses speed, The reverse happens. It starts to fall in until it picks up enough speed to fling it back outward and when it reaches its orginal distance it starts to fall back in again. It enters an elliptical orbit with the original distance as the apoapis. It will not "spiral in". Only if it loses enough velocity such that the new periapis falls below the surface of the star will it hit the star. Using the Earth as an example, this would require the Earth to lose nearly all of its 30 km/sec orbital velocity.
 
  • #4
Not only does the Sun's gravity effect the trajectory of the planets, but the reverse is true as well. The Sun wobbles with the gravitational infuence of the planets. And as a result of this non-uniform rotation about a "central" solar-system gravitational axis, planetary motion about the Sun has been perturbed, thus an eliptical orbit. I believe the eliptical orbits follow the shift of the Sun's orbit like the tides on Earth follow the influence of Luna. Exagerated versions of this effect have led to the discovery of high mass planets circling other stars, because those stars act like binary systems in their degree of wobble and highly exagerated eliptical orbits (determined by shadow phase observations).
 
  • #5
Thank you all ! :)
So in conclusion the elliptical orbits are the results of combined gravitational forces from other planets and stars. Does it mean that the orbits are actually changing their shapes with time?
 
  • #6
For small enough values of 'change' yes. Although the inertia of a planet is pretty large so they tend to move pretty regularly.
Planets orbits are presumably stable over long periods ( we are still here !) but proving that is one of the famous (semi) unsolved problems in maths.
 
  • #7
Yes, Our star the Sun has a distinct vibration associated with the effects of planetary forces which has been measured.
 
  • #8
Some orbits can change their eccentricity dramatially over time but remain stable due to the Kozai mechanism, where inclination and eccentricity swap over for each other.
 
  • #9
There is a simple explanation. The sun is in motion. It is not static in the universe.
The Earth revolves around a moving object. Hence an elliptical orbit.
No Math required on this one.
 
  • #10
Visualedtech said:
There is a simple explanation. The sun is in motion. It is not static in the universe.
The Earth revolves around a moving object. Hence an elliptical orbit.
No Math required on this one.

Well... no. You're wrong on the explanation. It's all implicit in the mathematics of a radial force-law and comes out rather nicely. Geometry is involved in the shape of the possible orbits - circles, ellipses, parabolas and hyperbolas - which shows they're all related curves.

The motion of the Sun due to perturbations by the planets, other stars, even the Galaxy, makes the orbits wobble around else they'd always orbit in flat planes. Instead, over aeons, they fill - approximately - a volume which defines their possible range of variation.
 
  • #11
Just to clarify there - it doesn't matter if the sun is in motion or considered stationary. Either way, all orbits are elliptical (even if some of them are circular!).
 
  • #12
russ_watters said:
Just to clarify there - it doesn't matter if the sun is in motion or considered stationary. Either way, all orbits are elliptical (even if some of them are circular!).
It also doesn't matter whether - as mgb_phys keeps suggesting - there are or were other planets in the system. A single planet system will still be elliptical.
 
  • #13
To reiterate: orbits are always elliptical; the circle is just a special case of an ellipse. An orbit can only be circular if the planet starts off at the PERFECT speed. If that speed is precisely 30 km/s and the actual speed is 30.0000000001 km/s, the orbit's going to be slightly elliptical. The chances of finding a planet at the perfect speed is 0. Add in pertubations from other planets and eccentricity actually changes over time, though not drastically.
 
  • #14
Parabolic and hyperbolic orbits aren't elliptical...

ideasrule said:
To reiterate: orbits are always elliptical; the circle is just a special case of an ellipse. An orbit can only be circular if the planet starts off at the PERFECT speed. If that speed is precisely 30 km/s and the actual speed is 30.0000000001 km/s, the orbit's going to be slightly elliptical. The chances of finding a planet at the perfect speed is 0. Add in pertubations from other planets and eccentricity actually changes over time, though not drastically.
 
  • #15
qraal said:
Parabolic and hyperbolic orbits aren't elliptical...
Parabolic and hyperbolic trajectories aren't orbits at all. So, yes, all orbits are elliptical.
 
  • #16
Mathematics describes the real world, it does not explain it. Math is a construct of the human mind. It helps us understand the real world.

Orbital calculations are based on assumptions. If we assume that the Sun is stationary, the calculations have to include formulas incorporating the non circular orbit observations.

We appear to live in a Spiral Galaxy. Observing such a spiral formation implies motion around a central point. If the Big Bang theory is valid, then all mass is in motion, by default. Once again, that is an assumption. Considering all the energy and forces in the universe, it is hard for me to conceive that anything could stand still.

So, assuming that the Sun has a direction and a velocity and assuming that a circular orbit would occur if the Sun was stationary, then, one should be able to calculate the velocity of the Sun. That could provide a PhD. thesis if you can stand the critizism and ridicule of your peers.

I am neither a scientist nor a mathematician, Just a little curious.
"We are here to question knowledge not to worship it".
I do not know who to attribute that quote to, but it has always been stuck in my head.

What do you think?
JJC
 
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  • #17
Visualedtech said:
Orbital calculations are based on assumptions. If we assume that the Sun is stationary, the calculations have to include formulas incorporating the non circular orbit observations.

...
So, assuming that the Sun has a direction and a velocity and assuming that a circular orbit would occur if the Sun was stationary, then, one should be able to calculate the velocity of the Sun. That could provide a PhD. thesis if you can stand the critizism and ridicule of your peers.


What do you think?
JJC

This is all factually incorrect.

Again, orbits are elliptical around stationary bodies just as they are elliptical around moving bodies. Period.

The elliptical path around a central body depends on exactly two things, no more, no less:
- the mass of the bodies
- the angular momentum of the orbiting body
 
  • #18
Visualedtech said:
If we assume that the Sun is stationary, the calculations have to include formulas incorporating the non circular orbit observations.
Only one formula is needed for this: Newton's law of gravitation. That orbits are conic sections (circles, ellipses, parabolae, or hyperbolae) falls right out. You seem to have the mistaken conception that orbits must be circular. That is not the case.
 
  • #19
Visualedtech said:
Mathematics describes the real world, it does not explain it. Math is a construct of the human mind. It helps us understand the real world.

Orbital calculations are based on assumptions. If we assume that the Sun is stationary, the calculations have to include formulas incorporating the non circular orbit observations.

We appear to live in a Spiral Galaxy. Observing such a spiral formation implies motion around a central point. If the Big Bang theory is valid, then all mass is in motion, by default. Once again, that is an assumption. Considering all the energy and forces in the universe, it is hard for me to conceive that anything could stand still.

So, assuming that the Sun has a direction and a velocity and assuming that a circular orbit would occur if the Sun was stationary, then, one should be able to calculate the velocity of the Sun. That could provide a PhD. thesis if you can stand the critizism and ridicule of your peers.

I am neither a scientist nor a mathematician, Just a little curious.
"We are here to question knowledge not to worship it".
I do not know who to attribute that quote to, but it has always been stuck in my head.

What do you think?
JJC

I think you have to reread this thread. It doesn't matter if the Sun is stationary or not; planetary orbits are NOT circular.
 

1. Why do most planetary orbits appear to be elliptical?

The shape of a planetary orbit is determined by the balance between the gravitational pull of the planet and the centrifugal force of its motion. If the gravitational pull is stronger, the orbit will be more circular. However, if the centrifugal force is stronger, the orbit will be more elliptical.

2. How do we know that planetary orbits are elliptical?

Through the use of telescopes and mathematical calculations, scientists have been able to observe and track the movements of planets in our solar system. This data has shown that the orbits of most planets are not perfectly circular, but instead have a slight elongation, indicating an elliptical shape.

3. Are all planetary orbits perfectly elliptical?

No, not all planetary orbits are perfectly elliptical. Factors such as gravitational pull from other nearby planets, collisions with other objects, and the shape and rotation of the planet itself can all cause slight variations in the shape of the orbit.

4. Is there a reason why planetary orbits tend to be elliptical?

The elliptical shape of planetary orbits is a result of the laws of gravity and motion, specifically Kepler's laws of planetary motion. These laws state that the shape of an orbit is determined by the balance between gravitational pull and centrifugal force, and that the speed of a planet in its orbit varies depending on its distance from the sun.

5. Do all planets in our solar system have elliptical orbits?

No, not all planets in our solar system have elliptical orbits. In fact, the eight planets in our solar system have a variety of orbit shapes, with some being more circular and others being more elliptical. The shape of a planet's orbit depends on its distance from the sun and its mass, among other factors.

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