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  1. The orbit of Venus is 224.7 Earth days (7.4 avg. Earth months [30.4 days]). The phases of Venus result from the planet's orbit around the Sun inside the Earth's orbit giving the telescopic observer a sequence of progressive lighting similar in appearance to the Moon's phases. It presents a full image when it is on the opposite side of the Sun.

  2. For one thing, your “day” would be 243 Earth days long – longer even than a Venus year (one trip around the Sun), which takes only 225 Earth days. For another, because of the planet's extremely slow rotation, sunrise to sunset would take 117 Earth days.

  3. Jan 22, 2023 · After eight years, it returns to the same place in our sky on about the same date. This is known as the eight-year cycle of Venus, and stems from the fact that 13 Venusian orbits (13 x 224.8 days ...

  4. Venus Phase Cycle, 1900-2050. Venus takes only 225 days to orbit the Sun. However, when she is viewed from Earth, her full synodic cycle (from inferior conjunction to inferior conjunction with the Sun) takes 584 days, or about 1.6 years. This is due to the interaction of Venus’s 225-day orbital period with the 365-day orbital period of the Earth.

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  5. Jun 18, 2014 · How long are years on other planets? A year is defined as the time it takes a planet to complete one revolution of the Sun, for Earth this is just over 365 days. This is also known as the orbital period. Unsurprisingly the the length of each planet’s year correlates with its distance from the Sun as seen in the graph above.

  6. So point toward a planet with one arm and toward the sun with the other arm — the angle between your arms is elongation. In the simple model of Copernicus — planets in circular orbits in the same plane — it allows a planet's position to be specified with a single coordinate. Click the button and then drag venus around noting the ...

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  8. Nov 21, 2016 · Starting at position 1, Venus is in superior conjunction with the Sun and has a phase of 100%. From Earth, the planet is very close to the Sun in the sky and is effectively not visible. As we move to position 2, Venus starts an eastern elongation and now appears in the evening sky – a 60mm telescope is sufficient to reveal that the planet has ...

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