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The 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, with values ranging from 0 (circular) to values approaching 1 (highly elliptical).
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 for understanding orbital mechanics, predicting satellite trajectories, and analyzing planetary motions in astronomy and aerospace engineering.
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 an eccentricity value of 0 mean?
A: An eccentricity value of 0 indicates a perfect circular orbit where both foci coincide at the center.
Q2: What is the maximum possible value for eccentricity?
A: For elliptical orbits, eccentricity values range from 0 to values approaching 1 (but never reaching 1, which would be a parabolic orbit).
Q3: How does eccentricity affect orbital period?
A: For a given semi-major axis, eccentricity does not affect the orbital period according to Kepler's third law.
Q4: Can eccentricity be negative?
A: No, eccentricity is always a non-negative value between 0 and 1 for elliptical orbits.
Q5: How is eccentricity related to orbital energy?
A: For a given semi-major axis, orbits with higher eccentricity have the same total energy but different distributions between kinetic and potential energy throughout the orbit.