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Author: WikiMatrix

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English[en]
The equation of time, correctly based on the two major components of the Sun's irregularity of apparent motion, i.e. the effect of the obliquity of the ecliptic and the effect of the Earth's orbital eccentricity, was not generally adopted until after John Flamsteed's tables of 1672/3, published with the posthumous edition of the works of Jeremiah Horrocks.
Chinese[zh]
該均時差, 正常基於視運動的太陽不規則性的兩個主要組成部分,即黃赤交角與地球軌道偏心率之影響的效果,約翰·佛蘭斯蒂德的資料表直到1672/3之後,沒有被普遍採用,發表傑雷米亞·霍羅克斯之作品追授版。

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