A solar eclipse occurs when the moon passes between the sun and the Earth, and the moon fully or partially blocks the sun's light. This happens only during a new moon, when the three celestial bodies are aligned in a straight line. There are three main types of solar eclipses: total, partial, and annular.
In a total solar eclipse, the moon completely covers the sun, and the sun's outer atmosphere, called the corona, becomes visible. This type of eclipse is only visible from within the narrow path of totality, which is a small area on the Earth's surface.
In a partial solar eclipse, the moon partially covers the sun, creating a crescent shape. This type of eclipse is visible from a larger geographic area, as it occurs when the observer is within the penumbra, the outer part of the moon's shadow.
An annular solar eclipse occurs when the moon is too far from the Earth to completely cover the sun. As a result, a ring of the sun's surface is still visible around the moon. This type of eclipse is known as a "ring of fire" due to the appearance of the sun's outer edge surrounding the moon.
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