The orbital eccentricity of an astronomical object is a parameter that determines the amount by which its orbit around another body deviates from a perfect circle. A value of 0 is a circular orbit, values between 0 and 1 form an elliptical orbit, and 1 is a parabolic escape orbit. The term derives its name from the parameters of conic sections, as every Kepler orbit is a conic section. It is normally used for the isolated two-body problem, but extensions exist for objects following a rosette orbit through the galaxy.
Read more about Orbital Eccentricity: Definition, Etymology, Calculation, Examples, Mean Eccentricity, Climatic Effect
Famous quotes containing the word eccentricity:
“Eccentricity has always abounded when and where strength of character has abounded; and the amount of eccentricity in a society has generally been proportional to the amount of genius, mental vigour, and moral courage which it contained.”
—John Stuart Mill (1806–1873)