A solar eclipse occurs when the Sun, Moon, and Earth align in a straight line, with the Moon positioned between the Sun and Earth.
Frequency
Solar eclipses are relatively infrequent events, with an average of about two to five occurring worldwide each year.
Duration
The total phase of a solar eclipse, when the Sun is completely covered by the Moon, is relatively short, usually lasting only a few minutes at any given location.
Path of Totality
The path of totality is the narrow track on the Earth's surface where the total solar eclipse is visible. This path can vary with each eclipse.
Annular Solar Eclipse
An annular solar eclipse occurs when the Moon is too far from Earth to completely cover the Sun. This results in a ring-like appearance, and the outer edges of the Sun are still visible.