Solar eclipse of January 1, 1889

A total solar eclipse occurred on January 1, 1889. 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. It was visible across western United States, and central Canada. Partiality was visible across the northern Pacific Ocean including Hawaii, and all of the United States.

Solar eclipse of January 1, 1889
Map
Type of eclipse
NatureTotal
Gamma0.8603
Magnitude1.0262
Maximum eclipse
Duration137 s (2 min 17 s)
Coordinates36°42′N 137°36′W / 36.7°N 137.6°W / 36.7; -137.6
Max. width of band175 km (109 mi)
Times (UTC)
Greatest eclipse21:16:50
References
Saros120 (54 of 71)
Catalog # (SE5000)9255

Observations and predictions

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Impact

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Wovoka the Paiute prophet received visions during the solar eclipse of January 1889. These visions were framework for the Pan-Indian religious movement known as the Ghost Dance.[1]

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Saros 120

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This eclipse is a part of Saros series 120, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on May 27, 933 AD. It contains annular eclipses from August 11, 1059 through April 26, 1492; hybrid eclipses from May 8, 1510 through June 8, 1564; and total eclipses from June 20, 1582 through March 30, 2033. The series ends at member 71 as a partial eclipse on July 7, 2195. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

The longest duration of annularity was produced by member 11 at 6 minutes, 24 seconds on September 11, 1113, and the longest duration of totality was produced by member 60 at 2 minutes, 50 seconds on March 9, 1997. All eclipses in this series occur at the Moon’s descending node of orbit.[2]

Series members 50–71 occur between 1801 and 2195:
50 51 52
 
November 19, 1816
 
November 30, 1834
 
December 11, 1852
53 54 55
 
December 22, 1870
 
January 1, 1889
 
January 14, 1907
56 57 58
 
January 24, 1925
 
February 4, 1943
 
February 15, 1961
59 60 61
 
February 26, 1979
 
March 9, 1997
 
March 20, 2015
62 63 64
 
March 30, 2033
 
April 11, 2051
 
April 21, 2069
65 66 67
 
May 2, 2087
 
May 14, 2105
 
May 25, 2123
68 69 70
 
June 4, 2141
 
June 16, 2159
 
June 26, 2177
71
 
July 7, 2195

References

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  1. ^ Andrew, Sherry. "Wovoka". apps.lib.umich.edu/. University of Michigan. Retrieved 6 May 2021.
  2. ^ "NASA - Catalog of Solar Eclipses of Saros 120". eclipse.gsfc.nasa.gov.

Further reading

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