Eccentricity is the measure of how much the conic section diverges into its circle form. One of the formulas for eccentricity is e=c/a this formula can be used to get the eccentricity of the ellipse.
Of the planets in our solar system, Venus has the smallest eccentricity.
The eccentricity of Psyche's orbit is 0.140
0.016710220 is the Earth's orbital eccentricity
The planet with the highest eccentricity (in other words the most stretched or elongated ellipse) in our solar system is Mercury, with an eccentricity of about 0.21. (Pluto's is higher but is no longer considered a true planet). By contrast, Venus is the most nearly a perfect circle with an eccentricity of about 0.007.
Earth's orbit around the sun is best represented by an ellipse with a very small eccentricity, which means it is almost a perfect circle. The eccentricity of Earth's orbit is about 0.0167, making it very close to a circular shape.
Mercury's orbit, like all planet's, is elliptical.The eccentricity of Mercury's orbit is 0.206
All natural orbits are ellipses. We can force an artificial satellite into a spherical orbit, but it won't STAY there without occasional adjustments. The "primary body" - in this case, the Sun - is at one of the two focuses (foci) of the orbit. If the focus is very close to the "center" of the ellipse, then the eccentricity of the orbit (how much it varies from a perfect circle) is close to zero.
More eccentric.
The elliptical orbit of Pluto has a semi-major axis of about 39,5 AU (astronomic units), the eccentricity is about 0,249.
The eccentricity of Earth's orbit around the Sun is approximately 0.0167. This value indicates how elliptical or circular the orbit is, with 0 being a perfect circle and 1 being a straight line. A lower eccentricity value like Earth's means the orbit is nearly circular.
The eccentricity of an object or orbit can be determined by calculating the ratio of the distance between the foci of the ellipse to the length of the major axis. This value ranges from 0 (perfect circle) to 1 (highly elongated ellipse).
The degree by which any ellipse departs from a circle is called its "eccentricity".
Planets don't have circular orbits; all orbits are ellipses. A circle has one center, but an ellipse has two focuses, or "foci". The further apart the foci, the greater the eccentricity, which is a measure of how far off circular the ellipse is. Venus has the lowest eccentricity, at 0.007. Neptune is next with an eccentricity of 0.011. (Earth's orbit has an eccentricity of 0.017.) So, Venus has the shortest focus-to-focus distance.
The actual shape of the earth's orbit around the sun is horrendously complicated. Partly because the earth does not orbit the sun and also because the orbit is influenced by the the gravitational attraction of the other planets. The earth does not orbit the sun: the centre of mass of the earth-sun system is at one of the foci of an ellipse whose eccentricity is 0.0167. The eccentricity varies from 0.0034 to 0.058.
Eccentricity is the measure of how much the conic section diverges into its circle form. One of the formulas for eccentricity is e=c/a this formula can be used to get the eccentricity of the ellipse.
An orbit can have an eccentricity greater than 1. It is the type of orbit that an object has when it comes in from outer space at high speed on a single encounter with the Sun before it disappears off into interstellar space again. This type of orbit is called a hyperbola, and it is the fourth type of conic section along with the circle, the ellipse and the parabola.