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A planet's year consists of the time it takes it to orbit the Sun. The Earth takes 365 and a quarter days to do this. Every 4 years there is a leap year which catches us up on these fractional days.

The position of a planet in its orbit can be determined by comparing its relative position from Earth when the Earth is in the "same" location (same day of the year). The positions of Venus and Mercury, which are closer to the Sun than Earth, can be observed directly, or indirectly by their "phases." The observation of phases of outer planets is a much more complex process, but also illustrates comparative positions in their orbits.

The location of a planet can be determined with some precision should it experience occultation (blockage) by the Sun. This establishes it on the opposite side of the Sun from Earth.

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12y ago

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