Difference between revisions of "Solar declination"

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(Solar declination)
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Solar declination is the apparent angle of the [[sun]] north or south of the [[earth]]'s [[celestial equator]]. The earth's rotation on its axis causes a daily change in the declination.
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'''Solar declination''' is the apparent angle of the [[sun]] north or south of the [[earth]]'s [[celestial equator]]. The earth's rotation on its axis causes a daily change in the declination.
[[category:astronomy]]
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[[Category:Astronomy]]

Latest revision as of 19:28, July 13, 2016

Solar declination is the apparent angle of the sun north or south of the earth's celestial equator. The earth's rotation on its axis causes a daily change in the declination.