Formula Used:
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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.
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 the shape and characteristics of elliptical orbits in celestial mechanics and orbital dynamics.
Tips: Enter the distance between two foci and the semi-major axis in meters. Both values must be positive numbers greater than zero.
Q1: What is the range of possible values for eccentricity?
A: Eccentricity values range from 0 (perfect circle) to 1 (parabolic orbit).
Q2: How does eccentricity affect orbital characteristics?
A: Higher eccentricity means more elongated orbits with varying orbital speeds and distances from the central body.
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: What are some real-world applications of eccentricity calculation?
A: Used in astronomy, satellite orbit design, and space mission planning to determine orbital parameters.
Q5: How accurate is this calculation method?
A: The formula provides exact mathematical results for ideal elliptical orbits based on the input parameters.