Solar eclipse of May 19, 1928

Last updated
Solar eclipse of May 19, 1928
SE1928May19T.png
Map
Type of eclipse
NatureTotal
Gamma 1.0048
Magnitude 1.014
Maximum eclipse
Duration-
Coordinates 63°18′S22°30′E / 63.3°S 22.5°E / -63.3; 22.5
Max. width of band- km
Times (UTC)
Greatest eclipse13:24:20
References
Saros 117 (64 of 71)
Catalog # (SE5000) 9347

A total solar eclipse occurred at the Moon's ascending node of orbit on Saturday, May 19, 1928, with a magnitude of 1.014. 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.

Contents

While it was a total solar eclipse, it was a non-central total eclipse.

This was the last of 56 umbral solar eclipses of Solar Saros 117. The 1st was in 936 AD and the 56th was in 1928. The total duration is 992 years.

Eclipses in 1928

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 117

Inex

Triad

Solar eclipses of 1928–1931

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 eclipse on June 17, 1928 occurs in the previous lunar year eclipse set, and the partial solar eclipse on September 12, 1931 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 1928 to 1931
Ascending node Descending node
SarosMapGammaSarosMapGamma
117 May 19, 1928
SE1928May19T.png
Total (non-central)
1.0048122 November 12, 1928
SE1928Nov12P.png
Partial
1.0861
127 May 9, 1929
SE1929May09T.png
Total
−0.2887132 November 1, 1929
SE1929Nov01A.png
Annular
0.3514
137 April 28, 1930
SE1930Apr28H.png
Hybrid
0.473142 October 21, 1930
SE1930Oct21T.png
Total
−0.3804
147 April 18, 1931
SE1931Apr18P.png
Partial
1.2643152 October 11, 1931
SE1931Oct11P.png
Partial
−1.0607

Saros 117

This eclipse is a part of Saros series 117, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on June 24, 792 AD. It contains annular eclipses from September 18, 936 AD through May 14, 1333; hybrid eclipses from May 25, 1351 through July 8, 1423; and total eclipses from July 18, 1441 through May 19, 1928. The series ends at member 71 as a partial eclipse on August 3, 2054. 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 9 minutes, 26 seconds on December 3, 1062, and the longest duration of totality was produced by member 62 at 4 minutes, 19 seconds on April 26, 1892. All eclipses in this series occur at the Moon’s ascending node of orbit. [2]

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 24, 1916 and July 31, 2000
December 24–25October 12July 31–August 1May 19–20March 7
111113115117119
SE1916Dec24P.png
December 24, 1916
SE1924Jul31P.png
July 31, 1924
SE1928May19T.png
May 19, 1928
SE1932Mar07A.png
March 7, 1932
121123125127129
SE1935Dec25A.png
December 25, 1935
SE1939Oct12T.png
October 12, 1939
SE1943Aug01A.png
August 1, 1943
SE1947May20T.png
May 20, 1947
SE1951Mar07A.png
March 7, 1951
131133135137139
SE1954Dec25A.png
December 25, 1954
SE1958Oct12T.png
October 12, 1958
SE1962Jul31A.png
July 31, 1962
SE1966May20A.png
May 20, 1966
SE1970Mar07T.png
March 7, 1970
141143145147149
SE1973Dec24A.png
December 24, 1973
SE1977Oct12T.png
October 12, 1977
SE1981Jul31T.png
July 31, 1981
SE1985May19P.png
May 19, 1985
SE1989Mar07P.png
March 7, 1989
151153155
SE1992Dec24P.png
December 24, 1992
SE1996Oct12P.png
October 12, 1996
SE2000Jul31P.png
July 31, 2000

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
SE1819Mar25P.gif
March 25, 1819
(Saros 107)
SE1830Feb23P.gif
February 23, 1830
(Saros 108)
SE1841Jan22P.gif
January 22, 1841
(Saros 109)
SE1862Nov21P.gif
November 21, 1862
(Saros 111)
SE1895Aug20P.gif
August 20, 1895
(Saros 114)
SE1906Jul21P.png
July 21, 1906
(Saros 115)
SE1917Jun19P.png
June 19, 1917
(Saros 116)
SE1928May19T.png
May 19, 1928
(Saros 117)
SE1939Apr19A.png
April 19, 1939
(Saros 118)
SE1950Mar18A.png
March 18, 1950
(Saros 119)
SE1961Feb15T.png
February 15, 1961
(Saros 120)
SE1972Jan16A.png
January 16, 1972
(Saros 121)
SE1982Dec15P.png
December 15, 1982
(Saros 122)
SE1993Nov13P.png
November 13, 1993
(Saros 123)
SE2004Oct14P.png
October 14, 2004
(Saros 124)
SE2015Sep13P.png
September 13, 2015
(Saros 125)
SE2026Aug12T.png
August 12, 2026
(Saros 126)
SE2037Jul13T.png
July 13, 2037
(Saros 127)
SE2048Jun11A.png
June 11, 2048
(Saros 128)
SE2059May11T.png
May 11, 2059
(Saros 129)
SE2070Apr11T.png
April 11, 2070
(Saros 130)
SE2081Mar10A.png
March 10, 2081
(Saros 131)
SE2092Feb07A.png
February 7, 2092
(Saros 132)
SE2103Jan08T.png
January 8, 2103
(Saros 133)
SE2113Dec08A.png
December 8, 2113
(Saros 134)
SE2124Nov06A.png
November 6, 2124
(Saros 135)
SE2135Oct07T.png
October 7, 2135
(Saros 136)
SE2146Sep06A.png
September 6, 2146
(Saros 137)
SE2157Aug05A.png
August 5, 2157
(Saros 138)
SE2168Jul05T.png
July 5, 2168
(Saros 139)
SE2179Jun05A.png
June 5, 2179
(Saros 140)
SE2190May04A.png
May 4, 2190
(Saros 141)

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
SE1812Aug07P.gif
August 7, 1812
(Saros 113)
SE1841Jul18P.gif
July 18, 1841
(Saros 114)
SE1870Jun28P.gif
June 28, 1870
(Saros 115)
SE1899Jun08P.gif
June 8, 1899
(Saros 116)
SE1928May19T.png
May 19, 1928
(Saros 117)
SE1957Apr30A.png
April 30, 1957
(Saros 118)
SE1986Apr09P.png
April 9, 1986
(Saros 119)
SE2015Mar20T.png
March 20, 2015
(Saros 120)
SE2044Feb28A.png
February 28, 2044
(Saros 121)
SE2073Feb07P.png
February 7, 2073
(Saros 122)
Saros123 58van70 SE2102Jan19P.jpg
January 19, 2102
(Saros 123)
Saros124 61van73 SE2130Dec30P.jpg
December 30, 2130
(Saros 124)
Saros125 62van73 SE2159Dec09P.jpg
December 9, 2159
(Saros 125)
Saros126 57van72 SE2188Nov18P.jpg
November 18, 2188
(Saros 126)

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 117". eclipse.gsfc.nasa.gov.

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References