الگو:Total solar eclipse summary

از ویکی‌پدیا، دانشنامهٔ آزاد
پرش به: ناوبری، جستجو

A solar eclipse occurs when the ماه passes between Earth and the Sun, thereby totally or partially obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across the surface of the Earth, while a partial solar eclipse will be visible over a region thousands of kilometres wide.