Solar eclipse of July 9, 1926

Last updated
Solar eclipse of July 9, 1926
SE1926Jul09A.png
Map
Type of eclipse
NatureAnnular
Gamma 0.0538
Magnitude 0.968
Maximum eclipse
Duration231 s (3 min 51 s)
Coordinates 25°36′N165°06′W / 25.6°N 165.1°W / 25.6; -165.1
Max. width of band115 km (71 mi)
Times (UTC)
Greatest eclipse23:06:02
References
Saros 135 (34 of 71)
Catalog # (SE5000) 9342

An annular solar eclipse occurred at the Moon's ascending node of orbit on Friday, July 9, 1926, with a magnitude of 0.968. 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. Annularity was visible from the islands of Pulo Anna and Merir in Japan's South Seas Mandate (now in Palau) and Wake Island on July 10 (Saturday), and Midway Atoll on July 9 (Friday).

Contents

Eclipses in 1926

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 135

Inex

Triad

Solar eclipses of 1924–1928

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. [1]

The partial solar eclipses on March 5, 1924 and August 30, 1924 occur in the previous lunar year eclipse set, and the solar eclipses on May 19, 1928 and November 12, 1928 occur in the next lunar year eclipse set.

Solar eclipse series sets from 1924 to 1928
Ascending node Descending node
SarosMapGammaSarosMapGamma
115 July 31, 1924
SE1924Jul31P.png
Partial
−1.4459120 January 24, 1925
SE1925Jan24T.png
Total
0.8661
125 July 20, 1925
SE1925Jul20A.png
Annular
−0.7193130
Solar eclipse of 1926-01-14, John A. Miller.jpg
Totality in Sumatra, Indonesia
January 14, 1926
SE1926Jan14T.png
Total
0.1973
135 July 9, 1926
SE1926Jul09A.png
Annular
0.0538140 January 3, 1927
SE1927Jan03A.png
Annular
−0.4956
145 June 29, 1927
SE1927Jun29T.png
Total
0.8163150 December 24, 1927
SE1927Dec24P.png
Partial
−1.2416
155 June 17, 1928
SE1928Jun17P.png
Partial
1.5107

Saros 135

This eclipse is a part of Saros series 135, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on July 5, 1331. It contains annular eclipses from October 21, 1511 through February 24, 2305; hybrid eclipses on March 8, 2323 and March 18, 2341; and total eclipses from March 29, 2359 through May 22, 2449. The series ends at member 71 as a partial eclipse on August 17, 2593. 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 16 at 10 minutes, 41 seconds on December 24, 1601, and the longest duration of totality will be produced by member 62 at 2 minutes, 27 seconds on May 12, 2431. All eclipses in this series occur at the Moon’s ascending node of orbit. [2]

Series members 28–49 occur between 1801 and 2200:
282930
SE1818May05A.png
May 5, 1818
SE1836May15A.png
May 15, 1836
SE1854May26A.png
May 26, 1854
313233
SE1872Jun06A.gif
June 6, 1872
SE1890Jun17A.png
June 17, 1890
SE1908Jun28A.png
June 28, 1908
343536
SE1926Jul09A.png
July 9, 1926
SE1944Jul20A.png
July 20, 1944
SE1962Jul31A.png
July 31, 1962
373839
SE1980Aug10A.png
August 10, 1980
SE1998Aug22A.png
August 22, 1998
SE2016Sep01A.png
September 1, 2016
404242
SE2034Sep12A.png
September 12, 2034
SE2052Sep22A.png
September 22, 2052
SE2070Oct04A.png
October 4, 2070
434445
SE2088Oct14A.png
October 14, 2088
SE2106Oct26A.png
October 26, 2106
SE2124Nov06A.png
November 6, 2124
464748
SE2142Nov17A.png
November 17, 2142
SE2160Nov27A.png
November 27, 2160
SE2178Dec09A.png
December 9, 2178
49
SE2196Dec19A.png
December 19, 2196

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 ascending node.

22 eclipse events between December 2, 1880 and July 9, 1964
December 2–3September 20–21July 9–10April 26–28February 13–14
111113115117119
SE1880Dec02P.gif
December 2, 1880
SE1888Jul09P.gif
July 9, 1888
SE1892Apr26T.gif
April 26, 1892
SE1896Feb13A.png
February 13, 1896
121123125127129
SE1899Dec03A.gif
December 3, 1899
SE1903Sep21T.png
September 21, 1903
SE1907Jul10A.png
July 10, 1907
SE1911Apr28T.png
April 28, 1911
SE1915Feb14A.png
February 14, 1915
131133135137139
SE1918Dec03A.png
December 3, 1918
SE1922Sep21T.png
September 21, 1922
SE1926Jul09A.png
July 9, 1926
SE1930Apr28H.png
April 28, 1930
SE1934Feb14T.png
February 14, 1934
141143145147149
SE1937Dec02A.png
December 2, 1937
SE1941Sep21T.png
September 21, 1941
SE1945Jul09T.png
July 9, 1945
SE1949Apr28P.png
April 28, 1949
SE1953Feb14P.png
February 14, 1953
151153155
SE1956Dec02P.png
December 2, 1956
SE1960Sep20P.png
September 20, 1960
SE1964Jul09P.png
July 9, 1964

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
SE1806Jun16T.png
June 16, 1806
(Saros 124)
SE1817May16A.gif
May 16, 1817
(Saros 125)
Saros126 37van72 SE1828Apr14H.jpg
April 14, 1828
(Saros 126)
SE1839Mar15T.gif
March 15, 1839
(Saros 127)
SE1850Feb12A.gif
February 12, 1850
(Saros 128)
SE1861Jan11A.gif
January 11, 1861
(Saros 129)
SE1871Dec12T.png
December 12, 1871
(Saros 130)
SE1882Nov10A.gif
November 10, 1882
(Saros 131)
SE1893Oct09A.gif
October 9, 1893
(Saros 132)
SE1904Sep09T.png
September 9, 1904
(Saros 133)
SE1915Aug10A.png
August 10, 1915
(Saros 134)
SE1926Jul09A.png
July 9, 1926
(Saros 135)
SE1937Jun08T.png
June 8, 1937
(Saros 136)
SE1948May09A.png
May 9, 1948
(Saros 137)
SE1959Apr08A.png
April 8, 1959
(Saros 138)
SE1970Mar07T.png
March 7, 1970
(Saros 139)
SE1981Feb04A.png
February 4, 1981
(Saros 140)
SE1992Jan04A.png
January 4, 1992
(Saros 141)
SE2002Dec04T.png
December 4, 2002
(Saros 142)
SE2013Nov03H.png
November 3, 2013
(Saros 143)
SE2024Oct02A.png
October 2, 2024
(Saros 144)
SE2035Sep02T.png
September 2, 2035
(Saros 145)
SE2046Aug02T.png
August 2, 2046
(Saros 146)
SE2057Jul01A.png
July 1, 2057
(Saros 147)
SE2068May31T.png
May 31, 2068
(Saros 148)
SE2079May01T.png
May 1, 2079
(Saros 149)
SE2090Mar31P.png
March 31, 2090
(Saros 150)
SE2101Feb28A.png
February 28, 2101
(Saros 151)
Saros152 18van70 SE2112Jan29T.jpg
January 29, 2112
(Saros 152)
Saros153 15van70 SE2122Dec28A.jpg
December 28, 2122
(Saros 153)
Saros154 13van71 SE2133Nov26A.jpg
November 26, 2133
(Saros 154)
Saros155 13van71 SE2144Oct26T.jpg
October 26, 2144
(Saros 155)
Saros156 09van69 SE2155Sep26A.jpg
September 26, 2155
(Saros 156)
SE2166Aug25A.png
August 25, 2166
(Saros 157)
Saros158 07van70 SE2177Jul25P.jpg
July 25, 2177
(Saros 158)
Saros159 04van70 SE2188Jun24P.jpg
June 24, 2188
(Saros 159)
Saros160 02van71 SE2199May24P.jpg
May 24, 2199
(Saros 160)

Inex series

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
SE1810Sep28A.gif
September 28, 1810
(Saros 131)
SE1839Sep07A.png
September 7, 1839
(Saros 132)
SE1868Aug18T.png
August 18, 1868
(Saros 133)
SE1897Jul29A.gif
July 29, 1897
(Saros 134)
SE1926Jul09A.png
July 9, 1926
(Saros 135)
SE1955Jun20T.png
June 20, 1955
(Saros 136)
SE1984May30A.png
May 30, 1984
(Saros 137)
SE2013May10A.png
May 10, 2013
(Saros 138)
SE2042Apr20T.png
April 20, 2042
(Saros 139)
SE2071Mar31A.png
March 31, 2071
(Saros 140)
SE2100Mar10A.png
March 10, 2100
(Saros 141)
SE2129Feb18T.png
February 18, 2129
(Saros 142)
SE2158Jan30A.png
January 30, 2158
(Saros 143)
SE2187Jan09A.png
January 9, 2187
(Saros 144)

Notes

  1. 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.
  2. "NASA - Catalog of Solar Eclipses of Saros 135". eclipse.gsfc.nasa.gov.

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References