The reference for a year is primarily defined by the Earth's orbit around the Sun, known as a solar year, which encompasses the complete cycle of seasons. A solar year lasts approximately 365.2425 days. In contrast, a sidereal year, which measures the time it takes for the Earth to complete one full orbit relative to distant stars, is about 365.256363 days, making it roughly 20 minutes longer than a solar year. This difference arises from the precession of the equinoxes, a gradual shift in the Earth's rotational axis that occurs over approximately 26,000 years. If the sidereal year were used as the standard, seasonal shifts would occur over time, which is why the solar year is the accepted measure. Other types of years include the anomalistic year, which tracks the time between perihelion passages, the eclipse year, marking the time between lunar node passages, and the tropical year, which is the average interval between vernal equinoxes.