“Kepler’s equation”的概念、定义、翻译、参考文献-科学参考

单词	Kepler’s equation
释义	Kepler’s equation Astronomy An equation that relates the eccentric anomaly of a body in an elliptical orbit to its mean anomaly. The equation is $E - e \sin E = M,$ where E is the eccentric anomaly, M the mean anomaly, and e the eccentricity of the orbit. It is important as one of the mathematical relations enabling the position of a planet about the Sun, or a satellite about its planet, to be calculated from the orbital elements for any time.
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