Solar eclipse of November 2, 1910

Last updated
Solar eclipse of November 2, 1910
SE1910Nov02P.png
Map
Type of eclipse
NaturePartial
Gamma 1.0603
Magnitude 0.8515
Maximum eclipse
Coordinates 61°54′N155°06′W / 61.9°N 155.1°W / 61.9; -155.1
Times (UTC)
Greatest eclipse2:08:32
References
Saros 122 (52 of 70)
Catalog # (SE5000) 9305

A partial solar eclipse occurred at the Moon's descending node of orbit on Wednesday, November 2, 1910, [1] [2] with a magnitude of 0.8515. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

Contents

Eclipses in 1910

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 122

Inex

Triad

Solar eclipses of 1910–1913

This eclipse is a member of a semester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit. [3]

The partial solar eclipse on August 31, 1913 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 1910 to 1913
Ascending node Descending node
SarosMapGammaSarosMapGamma
117 May 9, 1910
SE1910May09T.png
Total		−0.9437122 November 2, 1910
SE1910Nov02P.png
Partial		1.0603
127 April 28, 1911
SE1911Apr28T.png
Total		−0.2294132 October 22, 1911
SE1911Oct22A.png
Annular		0.3224
137 April 17, 1912
SE1912Apr17H.png
Hybrid		0.528142 October 10, 1912
SE1912Oct10T.png
Total		−0.4149
147 April 6, 1913
SE1913Apr06P.png
Partial		1.3147152 September 30, 1913
SE1913Sep30P.png
Partial		−1.1005

Saros 122

This eclipse is a part of Saros series 122, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on April 17, 991 AD. It contains total eclipses from July 12, 1135 through August 3, 1171; hybrid eclipses on August 13, 1189 and August 25, 1207; and annular eclipses from September 4, 1225 through October 10, 1874. The series ends at member 70 as a partial eclipse on May 17, 2235. 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 totality was produced by member 9 at 1 minutes, 25 seconds on July 12, 1135, and the longest duration of annularity was produced by member 50 at 6 minutes, 28 seconds on October 10, 1874. All eclipses in this series occur at the Moon’s descending node of orbit. [4]

Series members 46–68 occur between 1801 and 2200:
464748
SE1802Aug28A.png
August 28, 1802		 SE1820Sep07A.gif
September 7, 1820		 SE1838Sep18A.gif
September 18, 1838
495051
SE1856Sep29A.gif
September 29, 1856		 SE1874Oct10An.gif
October 10, 1874		 SE1892Oct20P.gif
October 20, 1892
525354
SE1910Nov02P.png
November 2, 1910 		SE1928Nov12P.png
November 12, 1928 		SE1946Nov23P.png
November 23, 1946
555657
SE1964Dec04P.png
December 4, 1964 		SE1982Dec15P.png
December 15, 1982 		SE2000Dec25P.png
December 25, 2000
585960
SE2019Jan06P.png
January 6, 2019 		SE2037Jan16P.png
January 16, 2037 		SE2055Jan27P.png
January 27, 2055
616263
SE2073Feb07P.png
February 7, 2073 		SE2091Feb18P.png
February 18, 2091 		Saros122 63van70 SE2109Mar01P.jpg
March 1, 2109
646566
Saros122 64van70 SE2127Mar13P.jpg
March 13, 2127		 Saros122 65van70 SE2145Mar23P.jpg
March 23, 2145		 Saros122 66van70 SE2163Apr03P.jpg
April 3, 2163
6768
Saros122 67van70 SE2181Apr14P.jpg
April 14, 2181		 Saros122 68van70 SE2199Apr25P.jpg
April 25, 2199

Tritos series

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2200
SE1801Sep08P.png
September 8, 1801
(Saros 112)		 SE1812Aug07P.gif
August 7, 1812
(Saros 113)		 SE1823Jul08P.gif
July 8, 1823
(Saros 114)		 SE1834Jun07P.gif
June 7, 1834
(Saros 115)		 SE1845May06An.gif
May 6, 1845
(Saros 116)
SE1856Apr05T.gif
April 5, 1856
(Saros 117)		 SE1867Mar06A.gif
March 6, 1867
(Saros 118)		 SE1878Feb02A.gif
February 2, 1878
(Saros 119)		 SE1889Jan01T.png
January 1, 1889
(Saros 120)		 SE1899Dec03A.png
December 3, 1899
(Saros 121)
SE1910Nov02P.png
November 2, 1910
(Saros 122)		 SE1921Oct01T.png
October 1, 1921
(Saros 123)		 SE1932Aug31T.png
August 31, 1932
(Saros 124)		 SE1943Aug01A.png
August 1, 1943
(Saros 125)		 SE1954Jun30T.png
June 30, 1954
(Saros 126)
SE1965May30T.png
May 30, 1965
(Saros 127)		 SE1976Apr29A.png
April 29, 1976
(Saros 128)		 SE1987Mar29H.png
March 29, 1987
(Saros 129)		 SE1998Feb26T.png
February 26, 1998
(Saros 130)		 SE2009Jan26A.png
January 26, 2009
(Saros 131)
SE2019Dec26A.png
December 26, 2019
(Saros 132)		 SE2030Nov25T.png
November 25, 2030
(Saros 133)		 SE2041Oct25A.png
October 25, 2041
(Saros 134)		 SE2052Sep22A.png
September 22, 2052
(Saros 135)		 SE2063Aug24T.png
August 24, 2063
(Saros 136)
SE2074Jul24A.png
July 24, 2074
(Saros 137)		 SE2085Jun22A.png
June 22, 2085
(Saros 138)		 SE2096May22T.png
May 22, 2096
(Saros 139)		 SE2107Apr23A.png
April 23, 2107
(Saros 140)		 SE2118Mar22A.png
March 22, 2118
(Saros 141)
SE2129Feb18T.png
February 18, 2129
(Saros 142)		 SE2140Jan20A.png
January 20, 2140
(Saros 143)		 SE2150Dec19A.png
December 19, 2150
(Saros 144)		 SE2161Nov17T.png
November 17, 2161
(Saros 145)		 SE2172Oct17H.png
October 17, 2172
(Saros 146)
Saros147 32van80 SE2183Sep16A.jpg
September 16, 2183
(Saros 147)		 Saros148 31van75 SE2194Aug16T.jpg
August 16, 2194
(Saros 148)

Metonic series

The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's descending node.

22 eclipse events between March 27, 1884 and August 20, 1971
March 27–29January 14November 1–2August 20–21June 8
108110112114116
SE1884Mar27P.gif
March 27, 1884		 SE1895Aug20P.gif
August 20, 1895		 SE1899Jun08P.gif
June 8, 1899
118120122124126
SE1903Mar29A.png
March 29, 1903 		SE1907Jan14T.png
January 14, 1907 		SE1910Nov02P.png
November 2, 1910 		SE1914Aug21T.png
August 21, 1914 		SE1918Jun08T.png
June 8, 1918
128130132134136
SE1922Mar28A.png
March 28, 1922 		SE1926Jan14T.png
January 14, 1926 		SE1929Nov01A.png
November 1, 1929 		SE1933Aug21A.png
August 21, 1933 		SE1918Jun08T.png
June 8, 1937
138140142144146
SE1941Mar27A.png
March 27, 1941 		SE1945Jan14A.png
January 14, 1945 		SE1948Nov01T.png
November 1, 1948 		SE1952Aug20A.png
August 20, 1952 		SE1956Jun08T.png
June 8, 1956
148150152154
SE1960Mar27P.png
March 27, 1960 		SE1964Jan14P.png
January 14, 1964 		SE1967Nov02T.png
November 2, 1967 		SE1971Aug20P.png
August 20, 1971

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References

  1. ↑ "WHEN SUN OR MOON IS DIMMED". New-York Tribune. New York, New York. 1910-11-02. p. 6. Retrieved 2023-11-03– via Newspapers.com.
  2. ↑ "Evening Sky Map for November". Hartford Courant. Hartford, Connecticut. 1910-11-01. p. 15. Retrieved 2023-11-03– via Newspapers.com.
  3. ↑ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
  4. ↑ "NASA - Catalog of Solar Eclipses of Saros 122". eclipse.gsfc.nasa.gov.
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