The Geocentric Orbit of Venus

It is helpful to visually complete the movement of Venus over her synodic period (of 1.6 years) seen by an observer on the Earth.

figure 3.13 (left) of Sacred Goddess in Ancient Goddess Cultures
version 3 (c) 2024 Richard Heath

In the heliocentric world view all planets orbit the sun, yet we view them from the Earth and so, until the 16th century astronomy had a different world view where the planets either orbited the sun (in the inner solar system) which like the outer planets orbited the earth, this view called geocentric. The discovery of gravity confirmed the heliocentric view but the geocentric view is still that seen from the Earth.

The geocentric was then assumed to be wholly superseded, but there are many aspects of it that appear to have given our ancestors their various religious views and, I believe, the megalithic monuments express most clearly a form of astronomy based upon numbers rather than on laws, numbers embedded in the structure of Time seen from the Earth, and hence showing the geocentric view had more to it than the medieval view discarded by modern science.

Venus was once considered one part of the triple goddess and the picture above shows her complete circuit both in the heavens and in front of and behind the sun. The shape of this forms two horns, firstly in the West at evening after sunset. Then she rushes in front of the sun to reemerge in the East to form a symmetrical other horn after which she travels behind the sun to eventually re-emerge in the West in a circuit lasting 1.6 years of 365 days, more precisely in 583.92 days – her synodic period.

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