elipsical?
circular
The eccentricity of a planet's orbit describes how elliptical (or non-circular) the orbit is. It is a measure of how much the orbit deviates from a perfect circle. A value of 0 represents a perfect circle, while values closer to 1 indicate a more elongated orbit.
The circular path is known as an orbit.
No planet's orbit is perfectly circular. They are all elipses.
No, Neptune's orbit is actually more eccentric (less circular) than Earth's orbit. Neptune's orbit is more elongated, with a greater difference between its closest and farthest points from the Sun compared to Earth's orbit.
Venus has the almost circular orbit.
Most orbits are elliptical; all NATURAL orbits are. There are two foci, or focuses, to an ellipse. The distance between the foci determines how eccentric, or non-circular, they are. If the two foci are in the same place, then the ellipse becomes a circle. So a circular orbit would have only one focus.
circuitous path orbit
These terms represent two points in any non-circular satellite orbit around the earth.Perigee: The point in the orbit that is closest to the earth.Apogee: The point in the orbit that is farthest from the earth.
No planet has a perfectly circular orbit, though Venus has the least orbital eccentricity of any planet in our solar system.
An eliptical orbit. In theory a planet could also have a circular orbit, but no planet that we know of has a perfectly circular orbit, although some have a nearly circular orbit.
A circular orbit would have an eccentricity of 0, meaning the orbit is perfectly circular with no deviation. Eccentricity is a measure of how elongated an orbit is, ranging from 0 to 1, with 0 indicating a circle and 1 indicating a parabolic orbit.
The earths orbit around the sun is almost circular.
The velocity in a circular orbit changes all the time. The acceleration is towards the center.
circular
It is not in the plane of the ecliptic and is sometimes inside the orbit of Neptune
The circular orbit equation used to calculate the motion of objects in a circular path is called the centripetal force equation, which is F mv2/r.