Why Earth's Orbit is Elliptical

In summary: An elliptical orbit is the default for planets because it is the simplest and most efficient way for them to orbit around a star. If Earth had a circular orbit, it would require perfect balance between all the different objects in the solar system and it would be moving too fast.
  • #1
rajatgl16
54
0
Why Earth's orbit is elliptical rather than being perfectly circular
 
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  • #2
It's very nearly circular - only 1.5% off

Being perfectly circular would require everythign to be absolutely perfectly balanced, the Earth to be a perfect sphere and no other planets, debris, moons, solar wind etc to disturb it.
 
  • #3
In terms of Energy, there is only a specific kinetic energy that a planet can have to be orbiting in a circle. This energy is based on the distance to the planet, and the masses of the planets. However, if Earth has more than this energy, it will orbit elliptically.

In simpler terms of speed, the Earth simply is going too fast to orbit in a circle. If you slowed down the Earth a bit it could be the right speed. If you increase the speed enough, the orbit will become hyperbolic and coincidentally the planet will leave the sun's orbit.

I'm not sure I'm being 100% clear so let me know if you have any questions
 
  • #4
dacruick said:
In terms of Energy, there is only a specific kinetic energy that a planet can have to be orbiting in a circle. This energy is based on the distance to the planet, and the masses of the planets. However, if Earth has more than this energy, it will orbit elliptically.

In simpler terms of speed, the Earth simply is going too fast to orbit in a circle. If you slowed down the Earth a bit it could be the right speed. If you increase the speed enough, the orbit will become hyperbolic and coincidentally the planet will leave the sun's orbit.

I'm not sure I'm being 100% clear so let me know if you have any questions

This is not quite right. The Earth's orbital speed changes over the course of its orbit; speeding up at perihelion and slowing down at aphelion. At perihelion is it moving too fast to maintain a circular orbit at that distance and at aphelion it is moving too slow. At a distance halfway between the two it is moving at just the right speed but in the wrong direction.

So what you need to do in order to circularize the Earth's orbit depends upon where it is in its orbit. You slow down at perihelion, speed up at aphelion and at its mean distance alter the direction of its path. Other points of the orbit would require a combination of change and speed and direction.
 
  • #5
Janus said:
This is not quite right. The Earth's orbital speed changes over the course of its orbit; speeding up at perihelion and slowing down at aphelion. At perihelion is it moving too fast to maintain a circular orbit at that distance and at aphelion it is moving too slow. At a distance halfway between the two it is moving at just the right speed but in the wrong direction.

So what you need to do in order to circularize the Earth's orbit depends upon where it is in its orbit. You slow down at perihelion, speed up at aphelion and at its mean distance alter the direction of its path. Other points of the orbit would require a combination of change and speed and direction.

Well of course, if you are in an elliptical orbit, your speed has to be inversely proportional to the distance from the sun. The easiest way to do this is in terms of energy though. Each orbit has an energy. The aphelion and perihelion will be the two extremes of the distribution of potential energy and kinetic energy.
 
  • #6
The shorter answer to the OP's question is that orbits are formed from a very, very wide array of proto-objects in terms of size, location and angular velocity. As they settle down into stable orbits (through collison, perturbation or ejection), their orbital momentum is averaged in the one remaining body.

In order for the remaining body's orbit to be circular, its final average velocity and its final average orbit would have to be perfectly balanced. It is simply highly improbable that so many events conspire to bring this about.

In general - all orbits are elliptical. This is default. They certainly start off this way in their infancy. A very few orbits have their parameters balanced (or have been subjected to forces that bring them into balance) so that their ellipticity is near zero.
 
  • #7
Is Earth's orbit exactly constant or it changes somewhat with time.
 
  • #8
dacruick said:
In terms of Energy, there is only a specific kinetic energy that a planet can have to be orbiting in a circle. This energy is based on the distance to the planet, and the masses of the planets. However, if Earth has more than this energy, it will orbit elliptically.
To overcome Janus' objections, this is better stated in terms of mechanical energy (kinetic plus potential). A planet's total mechanical energy must be exactly equal to some value that is a function of planet mass, solar mass, and radial distance from the Sun for the planet to be in a circular orbit. Any deviation from this precise value and the orbit will not be circular.


rajatgl16 said:
Is Earth's orbit exactly constant or it changes somewhat with time.
It changes over time. Describing an orbit in terms of an ellipse assumes the two body (two point mass) problem. The solar system comprises the Sun, eight planets, minor planets, and a slew of small miscellaneous objects. Jupiter and Venus, and to a much less extent all that other stuff, perturb the Earth's orbit.
 

1. Why is Earth's orbit elliptical?

Earth's orbit is elliptical because of the gravitational pull of the sun and other planets in our solar system. According to Kepler's laws of planetary motion, the shape of a planet's orbit depends on its distance from the sun and the strength of the sun's gravitational force.

2. How does the shape of Earth's orbit affect its seasons?

The shape of Earth's orbit does not significantly impact its seasons. The tilt of Earth's axis is the main factor that causes the change in seasons, as it determines the amount of sunlight each hemisphere receives throughout the year.

3. Can Earth's orbit become a perfect circle?

No, Earth's orbit will always be slightly elliptical due to the gravitational pull of other planets and objects in the solar system. However, the eccentricity (or ovalness) of Earth's orbit changes over time, ranging from 0.0 (perfect circle) to 0.07 (more elliptical).

4. Is Earth's elliptical orbit stable?

Yes, Earth's elliptical orbit is stable and has remained relatively consistent over thousands of years. The gravitational forces from the sun and other planets keep Earth's orbit in place, with only small variations over long periods of time.

5. How do scientists measure the eccentricity of Earth's orbit?

Scientists use mathematical calculations and observations of Earth's position in relation to the sun to determine the eccentricity of Earth's orbit. This can be done using Kepler's laws or by measuring the distance between Earth and the sun at different points in its orbit.

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