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Eccentricity of Elliptical Orbit is a measure of how stretched or elongated the orbit's shape is. It quantifies the deviation of the orbit from a perfect circle, where an eccentricity of 0 represents a circular orbit and values closer to 1 indicate more elongated elliptical orbits.
The calculator uses the formula:
Where:
Explanation: The formula calculates the eccentricity by dividing the distance between the two foci by twice the semi-major axis of the elliptical orbit.
Details: Calculating orbital eccentricity is crucial in astronomy and orbital mechanics for understanding the shape and characteristics of planetary orbits, satellite trajectories, and other celestial motions.
Tips: Enter the distance between two foci and the semi-major axis in meters. Both values must be positive numbers greater than zero for accurate calculation.
Q1: What does eccentricity value indicate?
A: Eccentricity values range from 0 to 1, where 0 indicates a perfect circle and values approaching 1 indicate highly elongated ellipses.
Q2: What are typical eccentricity values for planetary orbits?
A: Most planets in our solar system have low eccentricity values (close to 0), while comets and some asteroids have higher eccentricities.
Q3: Can eccentricity be greater than 1?
A: For elliptical orbits, eccentricity is always between 0 and 1. Values greater than 1 indicate hyperbolic orbits.
Q4: How does eccentricity affect orbital velocity?
A: Objects in elliptical orbits travel faster when closer to the focus (periapsis) and slower when farther away (apoapsis).
Q5: What's the relationship between eccentricity and orbital energy?
A: For a given semi-major axis, higher eccentricity means the orbit has the same total energy but different distribution between kinetic and potential energy throughout the orbit.