Solar eclipse of September 7, 1858 explained

A total solar eclipse occurred on September 7, 1858. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly 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's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.It was visible across South America.

Observations


Emmanuel Liais from Brazil

Related eclipses

Saros series 142

References