What are causing the Eccentricity of the planets?

In summary: This means that, over a long period of time, Mercury's eccentricity and inclination may vary strongly.In summary, the eccentricity of planets is caused by impacts and gravitational interactions with other objects in the solar system. While most planets have small eccentricities, exoplanets tend to have highly eccentric orbits. This challenges the standard model of planetary formation and highlights the chaotic nature of our solar system.
  • #1
Bjarne
344
0
What are causing the Eccentricity of the planets?
When reaching Neptune we have nearly a completely circular orbit.
Why ?
It seems not to be any logic in this !

Mercury 0,20563069
Venus 0,00677323
Earth 0,01670900
Mars 0,09340100
Jupiter 0,04849500
Saturn 0,05550900
Uranus 0,04629600
Neptun 0,00898800
 
Last edited:
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  • #2
Since the time the solar system was created, there have been lots of impacts onto planets caused by others objects either from outside of inside the system. The impacts are possible cause of the eccentricity.

There's hardly any rule about the list. Just may be it seems to me: the smaller the planet, the easier it can be hit out of its original (nearly) circular orbit (and the tilt as well).
Mercury, Pluto and Mars ...
 
  • #3
Why should they be perfectly circular? Each planet in the solar system is also experiencing small tugs from all the other planets so a perfectly circular orbit would not last long.
 
  • #4
Except for Mercury and Pluto, the planets in our solar system have very small eccentricities. Most exoplanets discovered to date have much highly eccentric orbits: circular (or nearly circular) orbits are not the norm. The standard models of planetary formation, which suggests nearly circular orbits will arise, need some tweaking.

Collisions are not needed to explain the eccentricities in our solar system. All that is needed is gravity. Suppose the planets all had perfectly circular orbits. Gravitational interactions among the planets would quickly result in non-circular orbits. Our solar system is not stable. It is chaotic. Jupiter, being by far the most massive, is the largest contributor to this chaotic behavior. Mercury's orbit, for example, has a strong secular resonance with Jupiter's orbit.
 

1. What is eccentricity in planetary motion?

Eccentricity is a measure of how elliptical the orbit of a planet is around its star. An eccentricity of 0 represents a perfectly circular orbit, while an eccentricity of 1 represents a highly elongated orbit.

2. What causes the eccentricity of planets?

There are a few factors that can contribute to the eccentricity of a planet's orbit. These include the gravitational pull of other planets and objects in the solar system, as well as the rotation and tilt of the planet itself.

3. How does eccentricity affect a planet's orbit?

The eccentricity of a planet's orbit affects its distance from its star and the speed at which it travels. A higher eccentricity means that the planet will have a more elongated orbit and will be farther from its star at certain points in its orbit.

4. Can the eccentricity of a planet change over time?

Yes, the eccentricity of a planet's orbit can change over time. This can be due to various factors, such as interactions with other planets or external forces acting on the planet.

5. How is the eccentricity of a planet measured?

The eccentricity of a planet's orbit is typically measured by observing its position in relation to its star over a period of time. By tracking the planet's motion, scientists can calculate its eccentricity using mathematical formulas.

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