How Can We Help?
You are here:
< Back

A total solar eclipse occurred on February 21, 1803. 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. The eclipse was visible in Pacific Ocean and Central America, while the totality was seen in Mexico.[1]

See also

References

  1. ^ "Solar eclipse of February 21, 1803". NASA. Retrieved June 15, 2012.

External links


Categories
Table of Contents