Solar eclipse of October 27, 1780
Map
Type of eclipse
Nature	Total
Gamma	0.8083
Magnitude	1.0244
Maximum eclipse
Duration	120 s (2 min 0 s)
Coordinates	35°36′N 58°36′W / 35.6°N 58.6°W / 35.6; -58.6
Max. width of band	138 km (86 mi)
Times (UTC)
Greatest eclipse	17:18:27
References
Saros	120 (48 of 71)
Catalog # (SE5000)	8991

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.

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 blames Samuel Williams for miscalculating the path of totality.^[1]

Related eclipses

It is a part of solar Saros 120.

See also

• List of solar eclipses visible from the United Kingdom 1000–2090 AD

Notes

References

• NASA chart graphics
• Googlemap
• NASA Besselian elements
• Observations of a Solar Eclipse, October 27, 1780, Made at St. John's Island, by Mess'rs. Clarke and Wright, by Joseph Peters 1783 American Academy of Arts & Sciences.
• A Memoir, Containing Observations of a Solar Eclipse of October 27, 1780 by Joseph Willard, 1783
• Where Did the 1780 Eclipse Go? Rothschild, Robert F., Sky and Telescope, 63:558, 1982