Why Do Orbits Take an Elliptical Shape?

In summary, the shape of orbits is elliptical because the solutions to the differential equations in the Newtonian two-body problem are in the form of conic sections, with ellipses being the only stable option. The perturbative effects of other bodies in the solar system also contribute to the approximately elliptical shape of orbits.
  • #1
koolraj
3
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why are the orbits elliptical in shape?i know that force equations give differential equations whose solutions imply that the orbits elliptical in shape.but what is the particular physical reason behind it?
 
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  • #2


You said it yourself: The solutions to the differential equations are ellipses. More precisely, the solutions to the Newtonian two-body problem are in the form of conic sections. Ellipses are one kind of conic section.

A better question: The solar system after all has more than two bodies in it, the whole solar system is orbiting the galaxy, and Newton's law of gravitation is only approximately correct. So why are orbits elliptical in shape?

The answer is that they aren't exactly elliptical in shape. They are instead approximately elliptical. The Sun is by far the dominant mass in the solar system. Planets perturb the orbits of each other from a purely elliptical shape. The primary effects are to slowly change the orientation and shape of the ellipse over time. General relativity similarly can be viewed, at least in our solar system, as a perturbative force. As far as the solar system orbiting the galaxy and the motion of the galaxy itself, those effects are so tiny as to be unmeasurable, at least as far as planetary orbits are concerned.
 
  • #3
koolraj said:
why are the orbits elliptical in shape?i know that force equations give differential equations whose solutions imply that the orbits elliptical in shape.but what is the particular physical reason behind it?

I think it's worth nothing that the solution to the differential equations yields a conic section. The only stable orbits are ellipses, which is why all the planets approximately have this form. Everything that had a parabolic of hyperbolic orbit has long since been ejected from the solar system, leaving us to observe only ellipses.
 

1. Why do planets orbit in an elliptical shape?

The shape of an orbit is determined by the balance between centripetal force and the gravitational force of the central body. In a perfect circular orbit, these two forces are equal. However, in an elliptical orbit, the gravitational force is stronger at certain points in the orbit, causing it to take on an elliptical shape.

2. How does the distance between a planet and its star affect the shape of its orbit?

The distance between a planet and its star plays a crucial role in determining the shape of its orbit. The closer a planet is to its star, the stronger the gravitational force, resulting in a more circular orbit. On the other hand, a planet that is farther away from its star will experience a weaker gravitational force, causing it to orbit in a more elongated, elliptical shape.

3. Can an orbit change from circular to elliptical or vice versa?

Yes, orbits can change from circular to elliptical or vice versa. This can happen due to various factors, such as the gravitational pull of other planets or stars, external forces like solar wind, or even collisions with other objects. These external influences can alter the balance between centripetal and gravitational forces, causing the orbit to change shape.

4. Are all orbits in the solar system elliptical?

No, not all orbits in the solar system are elliptical. While most planets and satellites have elliptical orbits, some have nearly circular orbits, such as Earth and Venus. Additionally, some small bodies, like comets, have highly elliptical orbits that can take them far away from the sun before returning on a long elliptical path.

5. How does the shape of an orbit affect the speed of a planet?

The shape of an orbit does not affect the speed of a planet directly. According to Kepler's laws of planetary motion, a planet's orbital speed is determined by its distance from the central body. However, in an elliptical orbit, the planet's speed will vary throughout its orbit. It will be moving faster when closer to the central body and slower when farther away, maintaining a constant average speed over time.

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