Definition of eccentric anomaly in English:

eccentric anomaly

noun

Astronomy

The actual anomaly of a planet in an elliptical orbit.
〔天文〕偏近点角。比较MEAN ANOMALY
Compare with mean anomaly
Example sentencesExamples
- We use Keplers eccentric anomaly in order to get explicit equations for the planetary orbits in a solar system.
- We need to convert this into the eccentric anomaly, and the formula is cos E = (e + cos n) / (1 + e cos n).
- The maximum difference in Eccentric Anomaly (in radians) will equal the eccentricity of the orbit.

Definition of eccentric anomaly in US English:

eccentric anomaly

noun

Astronomy

The actual anomaly of a planet in an elliptical orbit.
〔天文〕偏近点角。比较MEAN ANOMALY
Compare with mean anomaly
Example sentencesExamples
- We use Keplers eccentric anomaly in order to get explicit equations for the planetary orbits in a solar system.
- We need to convert this into the eccentric anomaly, and the formula is cos E = (e + cos n) / (1 + e cos n).
- The maximum difference in Eccentric Anomaly (in radians) will equal the eccentricity of the orbit.

单词	eccentric anomaly
释义	Definition of eccentric anomaly in English: eccentric anomaly noun Astronomy The actual anomaly of a planet in an elliptical orbit. 〔天文〕偏近点角。比较MEAN ANOMALY Compare with mean anomaly Example sentencesExamples We use Keplers eccentric anomaly in order to get explicit equations for the planetary orbits in a solar system. We need to convert this into the eccentric anomaly, and the formula is cos E = (e + cos n) / (1 + e cos n). The maximum difference in Eccentric Anomaly (in radians) will equal the eccentricity of the orbit. Definition of eccentric anomaly in US English: eccentric anomaly noun Astronomy The actual anomaly of a planet in an elliptical orbit. 〔天文〕偏近点角。比较MEAN ANOMALY Compare with mean anomaly Example sentencesExamples We use Keplers eccentric anomaly in order to get explicit equations for the planetary orbits in a solar system. We need to convert this into the eccentric anomaly, and the formula is cos E = (e + cos n) / (1 + e cos n). The maximum difference in Eccentric Anomaly (in radians) will equal the eccentricity of the orbit.
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