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Contents

   



(Top)
 


1 Observations  





2 Related eclipses  





3 See also  





4 Notes  





5 References  














Solar eclipse of October 27, 1780






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Solar eclipse of October 27, 1780

Map

Type of eclipse
NatureTotal
Gamma0.8083
Magnitude1.0244
Maximum eclipse
Duration120 s (2 min 0 s)
Coordinates35°36′N 58°36′W / 35.6°N 58.6°W / 35.6; -58.6
Max. width of band138 km (86 mi)
Times (UTC)
Greatest eclipse17:18:27
References
Saros120 (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[edit]

During the American Revolutionary War, the first American solar eclipse expedition was organized and sent out from Harvard CollegeinMassachusetts. 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[edit]

It is a part of solar Saros 120.

See also[edit]

Notes[edit]

References[edit]


Retrieved from "https://en.wikipedia.org/w/index.php?title=Solar_eclipse_of_October_27,_1780&oldid=1218843811"

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