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Solar eclipse of October 27, 1780

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Nature
  
Total

Magnitude
  
1.0244

Max. width of band
  
138 km (86 mi)

Start date
  
October 27, 1780

Gamma
  
0.8083

Duration
  
120 sec (2 m 0 s)

Greatest eclipse
  
17:18:27

Solar eclipse of October 27, 1780

A total solar eclipse occurred on October 27, 1780. 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.

Contents

Observations

During the American Revolutionary War, the first American solar eclipse expedition was organized and sent out from Harvard College in Massachusetts. A special immunity agreement was negotiated with the British to allow the scientists to work unharmed. The Harvard expedition, after all their efforts, missed the eclipse because they chose a site outside the path of totality. Modern analysis of this embarrassing incident for embryonic American science blame Samuel Williams for miscalculating the path of totality.

It is a part of solar Saros 120.

References

Solar eclipse of October 27, 1780 Wikipedia


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