Solar eclipse of August 20, 1906

Last updated
Solar eclipse of August 20, 1906
SE1906Aug20P.png
Map
Type of eclipse
NaturePartial
Gamma 1.3731
Magnitude 0.3147
Maximum eclipse
Coordinates 70°48′N66°24′W / 70.8°N 66.4°W / 70.8; -66.4
Times (UTC)
Greatest eclipse1:12:50
References
Saros 153 (3 of 70)
Catalog # (SE5000) 9295

A partial solar eclipse occurred at the Moon's ascending node of orbit on Monday, August 20, 1906, [1] [2] with a magnitude of 0.3147. 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. [3]

Contents

Eclipses in 1906

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 153

Inex

Triad

Solar eclipses of 1902–1906

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. [4]

The partial solar eclipses on May 7, 1902 and October 31, 1902 occur in the previous lunar year eclipse set, and the partial solar eclipse on July 21, 1906 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 1902 to 1906
Descending node Ascending node
SarosMapGammaSarosMapGamma
108 April 8, 1902
SE1902Apr08P.png
Partial
1.5024113October 1, 1902
118 March 29, 1903
SE1903Mar29A.png
Annular
0.8413123 September 21, 1903
SE1903Sep21T.png
Total
−0.8967
128 March 17, 1904
SE1904Mar17A.png
Annular
0.1299133 September 9, 1904
SE1904Sep09T.png
Total
−0.1625
138 March 6, 1905
SE1905Mar06A.png
Annular
−0.5768143
PSM V68 D565 Sun corona of August 30 1905 taken with 40 foot camera.png
August 30, 1905
SE1905Aug30T.png
Total
0.5708
148 February 23, 1906
SE1906Feb23P.png
Partial
−1.2479153 August 20, 1906
SE1906Aug20P.png
Partial
1.3731

Saros 153

This eclipse is a part of Saros series 153, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on July 28, 1870. It contains annular eclipses from December 17, 2104 through May 26, 2970. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on August 22, 3114. 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 will be produced by member 38 at 7 minutes, 1 seconds on September 5, 2537. All eclipses in this series occur at the Moon’s ascending node of orbit. [5]

Series members 1–19 occur between 1870 and 2200:
123
SE1870Jul28Pb.gif
July 28, 1870
SE1888Aug07P.gif
August 7, 1888
SE1906Aug20P.png
August 20, 1906
456
SE1924Aug30P.png
August 30, 1924
SE1942Sep10P.png
September 10, 1942
SE1960Sep20P.png
September 20, 1960
789
SE1978Oct02P.png
October 2, 1978
SE1996Oct12P.png
October 12, 1996
SE2014Oct23P.png
October 23, 2014
101112
SE2032Nov03P.png
November 3, 2032
SE2050Nov14P.png
November 14, 2050
SE2068Nov24P.png
November 24, 2068
131415
SE2086Dec06P.png
December 6, 2086
Saros153 14van70 SE2104Dec17A.jpg
December 17, 2104
Saros153 15van70 SE2122Dec28A.jpg
December 28, 2122
161718
Saros153 16van70 SE2141Jan08A.jpg
January 8, 2141
Saros153 17van70 SE2159Jan19A.jpg
January 19, 2159
Saros153 18van70 SE2177Jan29A.jpg
January 29, 2177
19
Saros153 19van70 SE2195Feb10A.jpg
February 10, 2195

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.

24 eclipse events between March 25, 1819 and August 20, 1906
March 25–26January 11–12October 30–31August 18–20June 6–7
107109111113115
SE1819Mar25P.gif
March 25, 1819
SE1823Jan12P.gif
January 12, 1823
SE1826Oct31P.gif
October 31, 1826
SE1830Aug18P.gif
August 18, 1830
SE1834Jun07P.gif
June 7, 1834
117119121123125
SE1838Mar25T.gif
March 25, 1838
SE1842Jan11A.gif
January 11, 1842
SE1845Oct30H.gif
October 30, 1845
SE1849Aug18T.gif
August 18, 1849
SE1853Jun06A.gif
June 6, 1853
127129131133135
SE1857Mar25T.gif
March 25, 1857
SE1861Jan11A.gif
January 11, 1861
SE1864Oct30A.gif
October 30, 1864
SE1868Aug18T.gif
August 18, 1868
SE1872Jun06A.gif
June 6, 1872
137139141143145
SE1876Mar25A.gif
March 25, 1876
SE1880Jan11T.gif
January 11, 1880
SE1883Oct30A.gif
October 30, 1883
SE1887Aug19T.png
August 19, 1887
SE1891Jun06A.gif
June 6, 1891
147149151153
SE1895Mar26P.gif
March 26, 1895
SE1899Jan11P.gif
January 11, 1899
SE1902Oct31P.png
October 31, 1902
SE1906Aug20P.png
August 20, 1906

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 1928
SE1808May25P.gif
May 25, 1808
(Saros 144)
SE1819Apr24P.gif
April 24, 1819
(Saros 145)
SE1830Mar24P.gif
March 24, 1830
(Saros 146)
SE1841Feb21P.gif
February 21, 1841
(Saros 147)
SE1852Jan21P.png
January 21, 1852
(Saros 148)
SE1862Dec21P.gif
December 21, 1862
(Saros 149)
SE1873Nov20P.png
November 20, 1873
(Saros 150)
SE1884Oct19P.gif
October 19, 1884
(Saros 151)
SE1895Sep18P.gif
September 18, 1895
(Saros 152)
SE1906Aug20P.png
August 20, 1906
(Saros 153)
SE1917Jul19P.png
July 19, 1917
(Saros 154)
SE1928Jun17P.png
June 17, 1928
(Saros 155)

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 1964
SE1819Oct19P.png
October 19, 1819
(Saros 150)
SE1848Sep27P.gif
September 27, 1848
(Saros 151)
SE1877Sep07P.gif
September 7, 1877
(Saros 152)
SE1906Aug20P.png
August 20, 1906
(Saros 153)
SE1935Jul30P.png
July 30, 1935
(Saros 154)
SE1964Jul09P.png
July 9, 1964
(Saros 155)

Notes

  1. "DIDN'T SEE ANY ECLIPSE OF THE SUN". The Eugene Guard. Eugene, Oregon. 1906-08-20. p. 1. Retrieved 2023-11-01 via Newspapers.com.
  2. "ECLIPSE DID NOT AFFECT THE RAYS OF OLD SOL IN OMAHA". Omaha World-Herald. Omaha, Nebraska. 1906-08-20. p. 3. Retrieved 2023-11-01 via Newspapers.com.
  3. "What Is a Solar Eclipse?". www.timeanddate.com. Retrieved 2020-04-24.
  4. 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.
  5. "NASA - Catalog of Solar Eclipses of Saros 153". eclipse.gsfc.nasa.gov.

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References