Solar eclipse of November 19, 1816 explained

A total solar eclipse occurred on November 19, 1816. 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.

Observations

From Germany, this total eclipse could not be seen with clouded sky except by few observers at Pomerania only.[1]

Capel Lofft observed this eclipse from Ipswich.[2]

Related eclipses

It is a part of solar Saros 120.

Tritos series

References

Notes and References

  1. http://www.t1t-trebur.de/esop-2003/zaw1.htm ON THE ECLIPSES AND OCCULTATIONS SEEN IN GERMANY IN THE PAST
  2. The Monthly magazine. v.42 (1816). - Full View HathiTrust Digital Library HathiTrust Digital Library. Monthly Magazine and Critical Register of Books. 1796 . en. 2017-07-04. Blake . William .