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originally posted by: ElectricUniverse
More, and more evidence keeps coming up pointing to the fact that there is at least one, or more planets, and planet 9 or X would be several times bigger than Earth (about 10 times) and possibly as large as Neptune or larger, up to 20 Earth masses and at a distance about 300 AU - 600 AU from our Sun.
originally posted by: ElectricUniverse
a reply to: NightSkyeB4Dawn
but in order for it to keep it's orbit out there, and in order for ETNOs to also keep their orbits all the way out there there has to be a brown dwarf in the outer reaches of the solar system. Otherwise planet 9 or X would have slingshotted away from the solar system as it encountered other stars or major planets from other solar systems throughout the millions of years of it's existence.
originally posted by: ElectricUniverse
a reply to: wildespace
No, you got it wrong. With a brown dwarf in the outer reaches of the solar system it would keep planet 9(X) and other planets out there in their orbits, just like the Sun is keeping the other 8 planets in an orbit around it. Without a failed star/brown dwarf out there even small astral rogues would have slingshotted planet 9 out of the solar system.
originally posted by: wildespace
With a brown dwarf in the outer reaches of the solar system it would keep planet 9(X) and other planets out there in their orbits, just like the Sun is keeping the other 8 planets in an orbit around it. Without a failed star/brown dwarf out there even small astral rogues would have slingshotted planet 9 out of the solar system.
originally posted by: ElectricUniverse
a reply to: MasterAtArms
Perhaps you haven't noticed that planet 9 has a highly elliptical orbit around our sun. You should refer to the diagram shown on the first page of this thread.
Here it is.
The aphelion of planet 9 is 1,200 AU and it has a perihelion of just 200 AU. So, If only the sun exists as the main point of gravity in our solar system, why does planet 9 have such an elliptical orbit?
It makes no sense. Only if another main point of gravity exists out there in the Oort cloud would planet 9 elliptical orbit make sense. If there was no companion star, or in this case a failed star then planet 9's orbit would have been circular.
Planet 9 has existed in our solar system for at least millions of years. It would be the only way all other ETNOs have a stable, but also highly elliptical orbit. Likewise, in order for planet 9 to have and keep such an elliptical orbit there has to be a failed star in our solar system. A brown or sub-brown dwarf.
The aphelion of planet 9 is 1,200 AU and it has a perihelion of just 200 AU. So, If only the sun exists as the main point of gravity in our solar system, why does planet 9 have such an elliptical orbit?
originally posted by: ElectricUniverse
a reply to: MasterAtArms
Perhaps you haven't noticed that planet 9 has a highly elliptical orbit around our sun. You should refer to the diagram shown on the first page of this thread.
Here it is.
The aphelion of planet 9 is 1,200 AU and it has a perihelion of just 200 AU. So, If only the sun exists as the main point of gravity in our solar system, why does planet 9 have such an elliptical orbit?
It makes no sense. Only if another main point of gravity exists out there in the Oort cloud would planet 9 elliptical orbit make sense. If there was no companion star, or in this case a failed star then planet 9's orbit would have been circular.
Planet 9 has existed in our solar system for at least millions of years. It would be the only way all other ETNOs have a stable, but also highly elliptical orbit. Likewise, in order for planet 9 to have and keep such an elliptical orbit there has to be a failed star in our solar system. A brown or sub-brown dwarf.
originally posted by: wildespace
I don't profess to know a lot about orbital mechanics, but even I see a lot of basic errors in your reasoning.
All planets in the Solars System have elliptical orbits, where the Sun is at one focus of the ellipse, and there's nothing at the other focus. As such, a body in an elliptical orbit doesn't need a second source of gravity for such an orbit.
Parabolic trajectory
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Under standard assumptions a body traveling along an escape orbit will coast along a parabolic trajectory to infinity, with velocity relative to the central body tending to zero, and therefore will never return. Parabolic trajectories are minimum-energy escape trajectories, separating positive-energy hyperbolic trajectories from negative-energy elliptic orbits.
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Hyperbolic trajectory
In astrodynamics or celestial mechanics, a hyperbolic trajectory is the trajectory of any object around a central body with more than enough speed to escape the central object's gravitational pull. The name derives from the fact that according to Newtonian theory such an orbit has the shape of a hyperbola. In more technical terms this can be expressed by the condition that the orbital eccentricity is greater than one.
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originally posted by: wildespace
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Highly elliptical orbits are quite normal in the Solar System, and, like Mogget mentioned, arise from interaction with Jupiter and perhaps some passing stars. They don't require a brown dwarf to always be there in the outer Solar System.
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A tiny tug over time
The two leading models for planetary formation both suggest that planets start out in nearly circular orbits, which corresponds to an eccentricity measurement of 0. Earth’s orbit is nearly circular at 0.02, which keeps the planet approximately the same distance from the Sun throughout the year.
An increased eccentricity means that the planet has a more elliptical, or stretched, orbit. Such planets may spend more time far from their stars, creating long, bitter winters. As they draw close to their stars, they could suffer scorching summers, particularly in the hemisphere pointed toward the star.
A planet could have a more eccentric orbit for a number of reasons. For example, collisions during the formation period could knock it out of its circular orbit.
Interactions with other planets could also change how they travel around their stars. Of the highly eccentric planets discovered, 78 percent of those with eccentricities greater than 0.5 have only one planet in the system, Hulsebus said. While the other planets could have been kicked out over the course of their evolution, Hulsebus and his team looked for a third option — the presence of a distant brown dwarf that could wreak havoc on the orbit of planets.
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