What is an annular solar eclipse?
According to NASA, an annular solar eclipse occurs when the Moon is between the Sun and the Earth, but at its furthest point from our planet. Due to its greater distance, the Moon appears smaller and fails to completely block the view of the Sun. When the Moon is in front of the Sun, it appears as a dark disk on top of a larger bright disk, creating a ring-like appearance. around the Moon.
Difference between an annular solar eclipse and a total one
In a total solar eclipse, people who have the opportunity to witness it find themselves in the center of the Moon’s shadow when it reaches the Earth. At this time, the sky becomes dark, similar to twilight. If weather conditions permit, those in the path of the total solar eclipse will be able to observe the Sun’s corona, which constitutes its outer atmosphere. It is important to note that a total solar eclipse is the only type of solar eclipse that can be observed without the need to use special glasses.
How long does it last?
The duration of the eclipse will depend on your viewing location. The partial phases will last one to two hours both before and after totality. For most locations, totality will last between two and five minutes, but will be longer or shorter in some places.