Elliptical Orbits (Using Newton's Model)

In summary, it is theoretically possible for a planet to orbit the sun in a perfect circle if the initial conditions are just right. The elliptical orbits in the real world are not due to perturbations of the force law, but rather a matter of initial conditions. The precession of the perihelion of Mercury is not caused by the increased mass of the planet, but rather a deviation from an exact inverse square force law introduced by general relativity. The precession is explained by Newtonian mechanics, with only a small discrepancy that was later explained by GR. It is also influenced by the tidal forces of other planets. It is uncertain if a larger planet like Jupiter in the same orbit as Mercury would have a greater precession.
  • #1
stevmg
696
3
1) Is it theoretically possible in a universe of two planetary objects - a Sun in a fixed position and a planet of any other finite mass, for that planet to orbit the sun in a perfectly circular orbit (not an ellipse?)

2) Are the elliptical (or near elliptical) orbits that occur in the real world due to the perturbations of forces exerted on the planet which throw it "off" a perfect circle and once an imbalance is created the new balance is an ellipse?

3) Is the precession of the perihelion and aphelion of mercury about the Sun due to the increased mass of mercury (old term "relativistic mass") as it increases in velocity as it approaches its perihelion and thus forces the center of gravity or center of mass of the combined objects of the Sun and mercury to shift outward and thus force an almost imperceptible but present movement of the mercury-Sun dyad outward and thus the orbit to migrate?
 
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  • #2
stevmg said:
1) Is it theoretically possible in a universe of two planetary objects - a Sun in a fixed position and a planet of any other finite mass, for that planet to orbit the sun in a perfectly circular orbit (not an ellipse?)

Yes. If the initial conditions are just right, the orbit will be a perfect circle.

stevmg said:
2) Are the elliptical (or near elliptical) orbits that occur in the real world due to the perturbations of forces exerted on the planet which throw it "off" a perfect circle and once an imbalance is created the new balance is an ellipse?

No. It is not a matter of perturbations of the force law, it is a matter of initial conditions. Both circular and elliptical orbits are valid solutions of Newton's laws, it just depends on the position and velocity with which the planet starts - the initial conditions.

stevmg said:
3) Is the precession of the perihelion and aphelion of mercury about the Sun due to the increased mass of mercury (old term "relativistic mass") as it increases in velocity as it approaches its perihelion and thus forces the center of gravity or center of mass of the combined objects of the Sun and mercury to shift outward and thus force an almost imperceptible but present movement of the mercury-Sun dyad outward and thus the orbit to migrate?

No, I don't think this is the correct explanation for the precession of the perihelion. It has to do with a deviation form an exact inverse square force law which is introduced by general relativity. Even a test particle of vanishingly small mass will exhibit the precession.
 
  • #3
Originally Posted by stevmg
2) Are the elliptical (or near elliptical) orbits that occur in the real world due to the perturbations of forces exerted on the planet which throw it "off" a perfect circle and once an imbalance is created the new balance is an ellipse?

No. It is not a matter of perturbations of the force law, it is a matter of initial conditions. Both circular and elliptical orbits are valid solutions of Newton's laws, it just depends on the position and velocity with which the planet starts - the initial conditions.


I see and by mere real world probability it would be virtually impossible for the "perfect conditions" to exist at the initiation of a planetary orbit to send it into a perfect circle. We cannot even do that with the satellites we launch.

3) Is the precession of the perihelion and aphelion of mercury about the Sun due to the increased mass of mercury (old term "relativistic mass") as it increases in velocity as it approaches its perihelion and thus forces the center of gravity or center of mass of the combined objects of the Sun and Mercury to shift outward and thus force an almost imperceptible but present movement of the Mercury-Sun dyad outward and thus the orbit to migrate?

No, I don't think this is the correct explanation for the precession of the perihelion. It has to do with a deviation form an exact inverse square force law which is introduced by general relativity. Even a test particle of vanishingly small mass will exhibit the precession.


Yes, I know that Einstein and Hilbert used what was later termed general relativity to explain the precession but I was trying to put it into a visual image that I could understand. That may not be possible. The interesting question about the "test particle of vanishingly small mass" might be: Is the precession as much as it would be as with a planet. If, say, Jupiter were the planet in in the "Mercury orbit" (so-to-speak), would the precession be greater than it is with Mercury?
 
  • #5
phyzguy said:
Yes, I know that Einstein and Hilbert used what was later termed general relativity to explain the precession but I was trying to put it into a visual image that I could understand. That may not be possible. The interesting question about the "test particle of vanishingly small mass" might be: Is the precession as much as it would be as with a planet. If, say, Jupiter were the planet in in the "Mercury orbit" (so-to-speak), would the precession be greater than it is with Mercury?

Anyone want to comment on this? Would a larger planet like Jupiter in the same "orbit" as Mercury have a greater precession of the perihelion-aphelion than Mercury does?

P.S.

How do you use "Multiquote?"
 
  • #6
stevmg said:
1) Is it theoretically possible in a universe of two planetary objects - a Sun in a fixed position and a planet of any other finite mass, for that planet to orbit the sun in a perfectly circular orbit (not an ellipse?)

2) Are the elliptical (or near elliptical) orbits that occur in the real world due to the perturbations of forces exerted on the planet which throw it "off" a perfect circle and once an imbalance is created the new balance is an ellipse?

It's theoretically possible to get a circular orbit if the two objects are perfectly spherical. That would be extremely unlikely, especially for rotating objects (the mass tends to shift towards the equator).

In other words, there's two reasons for no circular orbit. An incredibly low probability of initial conditions being correct is one good one. But even if the initial conditions were met, the orbital perturbations would make its "mean" orbit elliptical. (Perturbations also mean an elliptical orbit may appear "circular" for some given instant.)
 
  • #7
How about Jupiter instead of Mercury in Mercury's orbit. Wouild the precession go faster? After all, the shift of the center of gravity would be more than with mercury.
 

1. How does Newton's model explain elliptical orbits?

Newton's model of gravity states that all objects in the universe exert a force of attraction on each other. This force is directly proportional to the mass of the objects and inversely proportional to the square of the distance between them. In the case of an elliptical orbit, this force of attraction between the two objects (such as a planet and a star) causes the planet to continuously accelerate towards the star, resulting in a curved path known as an ellipse.

2. What are the key factors that affect the shape of an elliptical orbit?

The shape of an elliptical orbit is primarily influenced by two factors: the mass of the objects involved and the distance between them. The greater the mass of the objects, the stronger the force of attraction and the more elliptical the orbit will be. Similarly, the smaller the distance between the objects, the stronger the force of attraction and the more elliptical the orbit will be.

3. Can an object in an elliptical orbit ever escape the gravitational pull of the larger object?

No, an object in an elliptical orbit cannot escape the gravitational pull of the larger object. This is because the force of attraction between the objects is always present, causing the object to continuously accelerate towards the larger object. However, the shape and size of the elliptical orbit can change over time due to external influences such as the gravitational pull of other objects.

4. How does the eccentricity of an elliptical orbit affect its speed?

The eccentricity of an elliptical orbit, which measures how elongated the ellipse is, can affect the speed of the orbiting object. When the eccentricity is high, the orbiting object will experience a greater change in speed as it moves closer to and farther away from the larger object. This results in a faster speed at the perihelion (closest point) of the orbit and a slower speed at the aphelion (farthest point) of the orbit.

5. Can Newton's model accurately predict the path of all objects in the universe?

No, Newton's model of gravity has its limitations and cannot accurately predict the path of all objects in the universe. It assumes that objects are point masses and do not take into account the effects of relativity or other forces such as electromagnetism. For objects with extremely large masses or moving at high speeds, Einstein's theory of general relativity is a more accurate model for predicting their paths.

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