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: Eccentricity is a fundamental parameter in orbital mechanics that helps determine the shape and characteristics of orbits, which is crucial for satellite deployment, astronomical observations, and space mission planning.
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: For elliptical orbits, eccentricity ranges from 0 (perfect circle) to values less than 1 (increasingly elongated ellipse).
Q2: How does eccentricity affect orbital characteristics?
A: Higher eccentricity means more elongated orbits with varying orbital speeds and greater distance variations between the orbiting body and the focus.
Q3: Can eccentricity be exactly 1 or greater than 1?
A: Eccentricity of 1 indicates a parabolic orbit, while values greater than 1 indicate hyperbolic orbits, both of which are open trajectories rather than closed elliptical orbits.
Q4: What are some real-world applications of eccentricity calculations?
A: Used in satellite orbit design, planetary motion studies, comet trajectory analysis, and spacecraft mission planning.
Q5: How accurate is this calculation method?
A: The formula provides exact mathematical results for ideal elliptical orbits based on the given parameters.