Eccentricity is a measure of how much an orbit deviates from being circular, quantified by a value ranging from 0 (perfectly circular) to 1 (parabolic). It plays a significant role in understanding the long-term evolution of debris orbits and the dynamics that govern their paths through space. The shape of an orbit, as described by its eccentricity, can influence factors like orbital stability and interaction with gravitational fields, which are crucial when assessing debris behavior over time.
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