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Solar eclipse of February 25, 1914

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Solar eclipse of February 25, 1914
Map
Type of eclipse
NatureAnnular
Gamma−0.9416
Magnitude0.9248
Maximum eclipse
Duration335 s (5 min 35 s)
Coordinates62°06′S 113°18′W / 62.1°S 113.3°W / -62.1; -113.3
Max. width of band839 km (521 mi)
Times (UTC)
Greatest eclipse0:13:01
References
Saros119 (60 of 71)
Catalog # (SE5000)9313

An annular solar eclipse occurred at the Moon's ascending node of orbit between Tuesday, February 24 and Wednesday, February 25, 1914,[1][2][3] with a magnitude of 0.9248. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 3.3 days before apogee (on February 28, 1914, at 9:10 UTC), the Moon's apparent diameter was smaller.[4]

It took place almost entirely over the Southern Ocean, near Antarctica;[2] at its widest, the shadow cast by the moon was 167 mi (269 km) wide.[2] As a result, it could be seen from small patches of land, most notably southern Patagonia and part of New Zealand.[2][3][5] Due to this limited visibility, the Star-Gazette of Elmira said that for readers in the United States it was "not particularly interesting from a popular perspective";[6] the Salina Daily Union in Salina, Kansas said that "you perhaps didn't notice it".[7] It was the first of four eclipses that occurred during the year 1914.[3][5] While its path passed over New Zealand, and some attempted to view it in Wellington, it was reported to not have been visible there due to cloud cover.[8][9]

Eclipse details

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Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.[10]

February 25, 1914 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 1914 February 24 at 21:45:44.8 UTC
First Umbral External Contact 1914 February 24 at 23:26:46.2 UTC
First Central Line 1914 February 24 at 23:34:33.5 UTC
First Umbral Internal Contact 1914 February 24 at 23:44:06.5 UTC
Equatorial Conjunction 1914 February 24 at 23:16:07.3 UTC
Ecliptic Conjunction 1914 February 25 at 00:02:02.3 UTC
Greatest Eclipse 1914 February 25 at 00:13:01.0 UTC
Greatest Duration 1914 February 25 at 00:13:07.8 UTC
Last Umbral Internal Contact 1914 February 25 at 00:42:30.0 UTC
Last Central Line 1914 February 25 at 00:52:04.0 UTC
Last Umbral External Contact 1914 February 25 at 00:59:52.3 UTC
Last Penumbral External Contact 1914 February 25 at 02:40:43.4 UTC
February 25, 1914 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 0.92478
Eclipse Obscuration 0.85522
Gamma −0.94158
Sun Right Ascension 22h29m29.1s
Sun Declination -09°28'36.0"
Sun Semi-Diameter 16'09.3"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 22h31m04.3s
Moon Declination -10°14'09.7"
Moon Semi-Diameter 14'52.3"
Moon Equatorial Horizontal Parallax 0°54'34.6"
ΔT 16.2 s

Eclipse season

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This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.

Eclipse season of February–March 1914
February 25
Ascending node (new moon)
March 12
Descending node (full moon)
Annular solar eclipse
Solar Saros 119
Partial lunar eclipse
Lunar Saros 131
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Eclipses in 1914

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Solar Saros 119

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Inex

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Triad

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Solar eclipses of 1913–1917

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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.[11]

The partial solar eclipses on April 6, 1913 and September 30, 1913 occur in the previous lunar year eclipse set, and the solar eclipses on December 24, 1916 (partial), June 19, 1917 (partial), and December 14, 1917 (annular) occur in the next lunar year eclipse set.

Solar eclipse series sets from 1913 to 1917
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
114 August 31, 1913

Partial
1.4512 119 February 25, 1914

Annular
−0.9416
124 August 21, 1914

Total
0.7655 129 February 14, 1915

Annular
−0.2024
134 August 10, 1915

Annular
0.0124 139
February 3, 1916

Total
0.4987
144 July 30, 1916

Annular
−0.7709 149 January 23, 1917

Partial
1.1508
154 July 19, 1917

Partial
−1.5101

Saros 119

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This eclipse is a part of Saros series 119, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on May 15, 850 AD. It contains total eclipses on August 9, 994 AD and August 20, 1012; a hybrid eclipse on August 31, 1030; and annular eclipses from September 10, 1048 through March 18, 1950. The series ends at member 71 as a partial eclipse on June 24, 2112. 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 10 at 32 seconds on August 20, 1012, and the longest duration of annularity was produced by member 44 at 7 minutes, 37 seconds on September 1, 1625. All eclipses in this series occur at the Moon’s ascending node of orbit.[12]

Metonic series

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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 ascending node.

22 eclipse events between December 13, 1898 and July 20, 1982
December 13–14 October 1–2 July 20–21 May 9 February 24–25
111 113 115 117 119

December 13, 1898

July 21, 1906

May 9, 1910

February 25, 1914
121 123 125 127 129

December 14, 1917

October 1, 1921

July 20, 1925

May 9, 1929

February 24, 1933
131 133 135 137 139

December 13, 1936

October 1, 1940

July 20, 1944

May 9, 1948

February 25, 1952
141 143 145 147 149

December 14, 1955

October 2, 1959

July 20, 1963

May 9, 1967

February 25, 1971
151 153 155

December 13, 1974

October 2, 1978

July 20, 1982

Tritos series

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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

January 1, 1805
(Saros 109)

October 31, 1826
(Saros 111)

August 28, 1848
(Saros 113)

July 29, 1859
(Saros 114)

June 28, 1870
(Saros 115)

May 27, 1881
(Saros 116)

April 26, 1892
(Saros 117)

March 29, 1903
(Saros 118)

February 25, 1914
(Saros 119)

January 24, 1925
(Saros 120)

December 25, 1935
(Saros 121)

November 23, 1946
(Saros 122)

October 23, 1957
(Saros 123)

September 22, 1968
(Saros 124)

August 22, 1979
(Saros 125)

July 22, 1990
(Saros 126)

June 21, 2001
(Saros 127)

May 20, 2012
(Saros 128)

April 20, 2023
(Saros 129)

March 20, 2034
(Saros 130)

February 16, 2045
(Saros 131)

January 16, 2056
(Saros 132)

December 17, 2066
(Saros 133)

November 15, 2077
(Saros 134)

October 14, 2088
(Saros 135)

September 14, 2099
(Saros 136)

August 15, 2110
(Saros 137)

July 14, 2121
(Saros 138)

June 13, 2132
(Saros 139)

May 14, 2143
(Saros 140)

April 12, 2154
(Saros 141)

March 12, 2165
(Saros 142)

February 10, 2176
(Saros 143)

January 9, 2187
(Saros 144)

December 9, 2197
(Saros 145)

Inex series

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This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2200

April 26, 1827
(Saros 116)

April 5, 1856
(Saros 117)

March 16, 1885
(Saros 118)

February 25, 1914
(Saros 119)

February 4, 1943
(Saros 120)

January 16, 1972
(Saros 121)

December 25, 2000
(Saros 122)

December 5, 2029
(Saros 123)

November 16, 2058
(Saros 124)

October 26, 2087
(Saros 125)

October 6, 2116
(Saros 126)

September 16, 2145
(Saros 127)

August 27, 2174
(Saros 128)

References

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  1. ^ "February 24–25, 1914 Annular Solar Eclipse". timeanddate. Retrieved 31 July 2024.
  2. ^ a b c d "ECLIPSES OF 1914". The Washington Herald. Washington, District of Columbia. 1914-02-26. p. 4. Retrieved 2023-11-11 – via Newspapers.com.
  3. ^ a b c "AN ECLIPSE OF SUN TOMORROW". The Butte Daily Post. Butte, Montana. 1914-02-23. p. 12. Retrieved 2023-11-11 – via Newspapers.com.
  4. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 31 July 2024.
  5. ^ a b "Down in Patagonia and the Southeastern Coast of New Zealant Annular Eclipse of the Sun Is Visible". The Missoula Sentinel. Missoula, Montana. 1914-02-25. p. 6. Retrieved 2023-11-11 – via Newspapers.com.
  6. ^ "Moon Eclipses Sun Is Not Visible Here". Star-Gazette. Elmira, New York. 1914-02-23. p. 2. Retrieved 2023-11-11 – via Newspapers.com.
  7. ^ "ECLIPSE OF THE SUN". The Salina Daily Union. Salina, Kansas. 1914-02-25. p. 1. Retrieved 2023-11-11 – via Newspapers.com.
  8. ^ "ECLIPSE OF THE SUN". The Sydney Morning Herald. Sydney, New South Wales, New South Wales, Australia. 1914-02-26. p. 9. Retrieved 2023-11-11 – via Newspapers.com.
  9. ^ "Clouds obscure eclipse". The Daily Telegraph. Sydney, New South Wales, Australia. 1914-02-26. p. 9. Retrieved 2023-11-11 – via Newspapers.com.
  10. ^ "Annular Solar Eclipse of 1914 Feb 25". EclipseWise.com. Retrieved 31 July 2024.
  11. ^ 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.
  12. ^ "NASA - Catalog of Solar Eclipses of Saros 119". eclipse.gsfc.nasa.gov.