The square of the rotation period of the planets around the sun is proportional to the cube of the semi-major axis of the ellipse. As a result, planets close to the star rotate faster.
This rule is automatically fixed in my main model.
At the same time as the core of the sun is formed, rings are created around it.
Each planet is in a ring. Naturally, the motion of the planets occurs only within the ring. Only when the planet or the sun is hit by an unwanted impact, it is possible for the planets and their components to penetrate into the other rings.
Result: When the mean orbit of the earth is at the beginning of its loop, it will have the highest speed in its orbit. When the mean orbit of the Earth is at the end of its loop, it will have the lowest speed in its orbit.
Every planet has to move in its layer for some reason. I explained all those situations in my discoveries.
Example: When a planet is forced to decrease its orbital speed for some reason, it is forced to increase its average distance from the Sun. As a result, its circuit is stretched and compressed. Like the planet Pluto.
And when the planet is forced to increase its orbital speed for some reason, it is forced to decrease its average distance from the Sun. As a result, its orbit becomes a circle. Like the planet Venus.
According to my findings: Pluto and Neptune are in the same circle.
A planet's orbital speed changes, depending on how far it is from the Sun. The closer a planet is to the Sun, the stronger the Sun's gravitational pull on it, and the faster the planet moves. The farther it is from the Sun, the weaker the Sun's gravitational pull, and the slower it moves in its orbit. The closer a planet is to the Sun, the stronger the Sun's gravitational pull on it, and the faster the planet moves. The farther it is from the Sun, the weaker the Sun's gravitational pull, and the slower it moves in its orbit. A planet does moves faster when it is closer to the sun in its orbit and vice versa because according to Kepler's Law, the line between the sun and the palnet sweeps equal areas in equal times. If a planet is close to the Sun, the distance it orbits around the Sun is fairly short. This distance is called an orbital path. The closer a planet travels to the Sun, the more the Sun's gravity can pull on the planet. The stronger the pull of the Sun's gravity, the faster the planet orbits. This actually varies slightly, since the Earth makes an elliptical orbit around the Sun: moving faster at perihelion (nearest the Sun) and slower at aphelion (farthest from the Sun).