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- The rotation period of an astronomical object is the time it takes to complete one revolution around its axis of rotation relative to the background stars12. It differs from the planet's solar day, which includes an extra fractional rotation needed to accommodate the portion of the planet's orbital period in one day1. A synodic day (or synodic rotation period or solar day) is the period for a celestial object to rotate once in relation to the star it is orbiting, and is the basis of solar time3.Learn more:✕This summary was generated using AI based on multiple online sources. To view the original source information, use the "Learn more" links.The rotation period o an astronomical object is the time that it taks tae complete ane revolution aroond its axis o rotation relative tae the backgrund starns. It differs frae the planet's solar day, whilk includes an extra fractional rotation needit tae accommodate the portion o the planet's orbital period in ane day.sco.wikipedia.org/wiki/Rotation_periodRotational period is the term describing the length of time necessary for a space object to make one complete rotation. This time varies from planet to planet, and on Earth it is 1 day.physics-network.org/what-is-the-period-of-a-rotation/A synodic day (or synodic rotation period or solar day) is the period for a celestial object to rotate once in relation to the star it is orbiting, and is the basis of solar time.en.wikipedia.org/wiki/Synodic_day
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