Worldwide, there are typically two to five solar eclipses each year. The last year with five solar eclipses was 1935, and the next year with five solar eclipses will be 2206. In comparison, lunar eclipses occur much less frequently. On average, there are two lunar eclipses per year, and sometimes none at all.
So, why do we perceive solar eclipses as being more rare, even though they occur so frequently each year? This is because solar eclipses occur when the shadow of the Moon falls on Earth, and the area where they can be observed is limited to the region where the Moon's shadow passes. This is especially true for annular and total solar eclipses, and even including the partial eclipse zone, the observable area on Earth is still relatively small. Therefore, for most people, the chance of witnessing a solar eclipse is not very high. On average, a specific location on Earth only gets to see a total or annular solar eclipse once every three to four hundred years. Although lunar eclipses occur less frequently, they can be observed anywhere on Earth where the Moon is visible. On Earth, the observable area of lunar eclipses is much larger, so the chance of seeing them is also higher.
Solar and lunar eclipses are natural phenomena that offer amazing spectacles to humanity. When we encounter such phenomena, we must seize the opportunity to observe them. Especially during a total solar eclipse, the uneven surface of the Moon blocks most of the sunlight while allowing some light to leak around the edges, creating spectacular phenomena like the "Baily's beads" and "diamond ring," which are truly breathtaking!