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A total solar eclipse occurs when the Moon passes directly between the Earth and the Sun, blocking the Sun's entire disk and casting a shadow on Earth. During a total solar eclipse, the sky darkens significantly, and the Sun's corona, the outer atmosphere, becomes visible. This phenomenon is considered one of the most spectacular celestial events.

Key features of a total solar eclipse include:

Totality: The moment when the Sun is completely covered by the Moon, and only the Sun's corona is visible. Totality is a brief period, usually lasting only a few minutes.

Partial Phases: Before and after totality, there are partial phases where the Moon covers a portion of the Sun. These phases can be observed without protective eyewear only during totality.

Path of Totality: The total solar eclipse is visible only along a narrow path on Earth's surface. People outside this path will witness a partial solar eclipse but not the complete blocking of the Sun.

Totality Viewing Safety: It is crucial to use proper eye protection, such as solar viewing glasses, during the partial phases. However, during totality, it is safe to view the eclipse with the naked eye.

Frequency: Total solar eclipses are relatively rare events and occur at specific locations on Earth about once every 18 months. However, the same location may experience a total solar eclipse only once every several decades.

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