The Sun is (as seen from the northern hemisphere) due south at noon, The greatest elongation that Venus can reach is \(\arcsin(0.728) = Greatest elongation is equal to the arc sine of the distance.įor example: Venus does not get more than 0.728 AU from the Sun, so If thatĭistance is greater than 1, then the planet can reach any elongation ![]() Planet can be from the Sun, measured in Astronomical Units. Have, then you only need to know the greatest distance that that If you want to calculate the greatest elongation that a planet may Longitude, and also explains about the different definitions of Page explains how to calculate the geocentric ecliptic Planet and the Sun, and on what side of the Sun the planet is. The elongation says how many mile posts are between the Mile posts along the path that the planets and the Sun follow along That it is the difference between the geocentric ecliptic longitude The simplest definition for the elongation of a celestial object is Also, there areĭifferent definitions for the elongation, which in practice yieldĪlmost the same results for the brightest planets. There are different ways to calculate the elongation,ĭepending on which information you already have. The elongation measures the position of a planet in the sky, compared
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