Solar eclipse of July 20, 1925

Last updated
Solar eclipse of July 20, 1925
SE1925Jul20A.png
Map
Type of eclipse
NatureAnnular
Gamma −0.7193
Magnitude 0.9436
Maximum eclipse
Duration435 s (7 min 15 s)
Coordinates 25°18′S150°00′W / 25.3°S 150°W / -25.3; -150
Max. width of band300 km (190 mi)
Times (UTC)
Greatest eclipse21:48:42
References
Saros 125 (49 of 73)
Catalog # (SE5000) 9340

An annular solar eclipse occurred at the Moon's ascending node of orbit between Monday, July 20 and Tuesday, July 21, 1925, [1] with a magnitude of 0.9436. 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 8 hours after apogee (on July 20, 1925, at 13:30 UTC), the Moon's apparent diameter was smaller. [2]

Contents

Annularity was visible from northern part of Northland Region and the whole Kermadec Islands in New Zealand on July 21 (Tuesday), and Rapa Iti in French Polynesia on July 20 (Monday). A partial eclipse was visible for parts of Eastern Australia and Oceania.

Eclipse details

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. [3]

July 20, 1925 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact1925 July 20 at 19:03:41.7 UTC
First Umbral External Contact1925 July 20 at 20:23:08.9 UTC
First Central Line1925 July 20 at 20:26:27.5 UTC
First Umbral Internal Contact1925 July 20 at 20:29:50.5 UTC
Ecliptic Conjunction1925 July 20 at 21:40:09.2 UTC
Greatest Duration1925 July 20 at 21:46:03.5 UTC
Greatest Eclipse1925 July 20 at 21:48:41.6 UTC
Equatorial Conjunction1925 July 20 at 21:57:08.7 UTC
Last Umbral Internal Contact1925 July 20 at 23:07:26.9 UTC
Last Central Line1925 July 20 at 23:10:49.8 UTC
Last Umbral External Contact1925 July 20 at 23:14:08.3 UTC
Last Penumbral External Contact1925 July 21 at 00:33:37.3 UTC
July 20, 1925 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.94358
Eclipse Obscuration0.89035
Gamma−0.71927
Sun Right Ascension07h58m46.0s
Sun Declination+20°38'42.8"
Sun Semi-Diameter15'44.4"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension07h58m29.8s
Moon Declination+20°00'11.9"
Moon Semi-Diameter14'42.0"
Moon Equatorial Horizontal Parallax0°53'57.1"
ΔT23.7 s

Eclipse season

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 July–August 1925
July 20
Ascending node (new moon)
August 4
Descending node (full moon)
SE1925Jul20A.png Lunar eclipse chart close-1925Aug04.png
Annular solar eclipse
Solar Saros 125
Partial lunar eclipse
Lunar Saros 137

Eclipses in 1925

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 125

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. [4]

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 125

This eclipse is a part of Saros series 125, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on February 4, 1060. It contains total eclipses from June 13, 1276 through July 16, 1330; hybrid eclipses on July 26, 1348 and August 7, 1366; and annular eclipses from August 17, 1384 through August 22, 1979. The series ends at member 73 as a partial eclipse on April 9, 2358. 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 14 at 1 minutes, 11 seconds on June 25, 1294, and the longest duration of annularity was produced by member 48 at 7 minutes, 23 seconds on July 10, 1907. All eclipses in this series occur at the Moon’s ascending node of orbit. [5]

Series members 43–64 occur between 1801 and 2200:
434445
SE1817May16A.gif
May 16, 1817
SE1835May27A.gif
May 27, 1835
SE1853Jun06A.gif
June 6, 1853
464748
SE1871Jun18A.gif
June 18, 1871
SE1889Jun28A.png
June 28, 1889
SE1907Jul10A.png
July 10, 1907
495051
SE1925Jul20A.png
July 20, 1925
SE1943Aug01A.png
August 1, 1943
SE1961Aug11A.png
August 11, 1961
525354
SE1979Aug22A.png
August 22, 1979
SE1997Sep02P.png
September 2, 1997
SE2015Sep13P.png
September 13, 2015
555657
SE2033Sep23P.png
September 23, 2033
SE2051Oct04P.png
October 4, 2051
SE2069Oct15P.png
October 15, 2069
585960
SE2087Oct26P.png
October 26, 2087
Saros125 59van73 SE2105Nov06P.jpg
November 6, 2105
Saros125 60van73 SE2123Nov18P.jpg
November 18, 2123
616263
Saros125 61van73 SE2141Nov28P.jpg
November 28, 2141
Saros125 62van73 SE2159Dec09P.jpg
December 9, 2159
Saros125 63van73 SE2177Dec20P.jpg
December 20, 2177
64
Saros125 64van73 SE2195Dec31P.jpg
December 31, 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.

22 eclipse events between December 13, 1898 and July 20, 1982
December 13–14October 1–2July 20–21May 9February 24–25
111113115117119
SE1898Dec13P.gif
December 13, 1898
SE1906Jul21P.png
July 21, 1906
SE1910May09T.png
May 9, 1910
SE1914Feb25A.png
February 25, 1914
121123125127129
SE1917Dec14A.png
December 14, 1917
SE1921Oct01T.png
October 1, 1921
SE1925Jul20A.png
July 20, 1925
SE1929May09T.png
May 9, 1929
SE1933Feb24A.png
February 24, 1933
131133135137139
SE1936Dec13A.png
December 13, 1936
SE1940Oct01T.png
October 1, 1940
SE1944Jul20A.png
July 20, 1944
SE1948May09A.png
May 9, 1948
SE1952Feb25T.png
February 25, 1952
141143145147149
SE1955Dec14A.png
December 14, 1955
SE1959Oct02T.png
October 2, 1959
SE1963Jul20T.png
July 20, 1963
SE1967May09P.png
May 9, 1967
SE1971Feb25P.png
February 25, 1971
151153155
SE1974Dec13P.png
December 13, 1974
SE1978Oct02P.png
October 2, 1978
SE1982Jul20P.png
July 20, 1982

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
SE1805Jun26P.gif
June 26, 1805
(Saros 114)
SE1816May27A.gif
May 27, 1816
(Saros 115)
SE1827Apr26A.gif
April 26, 1827
(Saros 116)
SE1838Mar25T.gif
March 25, 1838
(Saros 117)
SE1849Feb23A.gif
February 23, 1849
(Saros 118)
SE1860Jan23A.png
January 23, 1860
(Saros 119)
SE1870Dec22T.png
December 22, 1870
(Saros 120)
SE1881Nov21A.gif
November 21, 1881
(Saros 121)
SE1892Oct20P.gif
October 20, 1892
(Saros 122)
SE1903Sep21T.png
September 21, 1903
(Saros 123)
SE1914Aug21T.png
August 21, 1914
(Saros 124)
SE1925Jul20A.png
July 20, 1925
(Saros 125)
SE1936Jun19T.png
June 19, 1936
(Saros 126)
SE1947May20T.png
May 20, 1947
(Saros 127)
SE1958Apr19A.png
April 19, 1958
(Saros 128)
SE1969Mar18A.png
March 18, 1969
(Saros 129)
SE1980Feb16T.png
February 16, 1980
(Saros 130)
SE1991Jan15A.png
January 15, 1991
(Saros 131)
SE2001Dec14A.png
December 14, 2001
(Saros 132)
SE2012Nov13T.png
November 13, 2012
(Saros 133)
SE2023Oct14A.png
October 14, 2023
(Saros 134)
SE2034Sep12A.png
September 12, 2034
(Saros 135)
SE2045Aug12T.png
August 12, 2045
(Saros 136)
SE2056Jul12A.png
July 12, 2056
(Saros 137)
SE2067Jun11A.png
June 11, 2067
(Saros 138)
SE2078May11T.png
May 11, 2078
(Saros 139)
SE2089Apr10A.png
April 10, 2089
(Saros 140)
SE2100Mar10A.png
March 10, 2100
(Saros 141)
SE2111Feb08T.png
February 8, 2111
(Saros 142)
SE2122Jan08A.png
January 8, 2122
(Saros 143)
SE2132Dec07A.png
December 7, 2132
(Saros 144)
SE2143Nov07T.png
November 7, 2143
(Saros 145)
SE2154Oct07T.png
October 7, 2154
(Saros 146)
Saros147 31van80 SE2165Sep05A.jpg
September 5, 2165
(Saros 147)
Saros148 30van75 SE2176Aug04T.jpg
August 4, 2176
(Saros 148)
Saros149 30van71 SE2187Jul06T.jpg
July 6, 2187
(Saros 149)
Saros150 27van71 SE2198Jun04A.jpg
June 4, 2198
(Saros 150)

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
SE1809Oct09T.gif
October 9, 1809
(Saros 121)
SE1838Sep18A.gif
September 18, 1838
(Saros 122)
SE1867Aug29T.gif
August 29, 1867
(Saros 123)
SE1896Aug09T.png
August 9, 1896
(Saros 124)
SE1925Jul20A.png
July 20, 1925
(Saros 125)
SE1954Jun30T.png
June 30, 1954
(Saros 126)
SE1983Jun11T.png
June 11, 1983
(Saros 127)
SE2012May20A.png
May 20, 2012
(Saros 128)
SE2041Apr30T.png
April 30, 2041
(Saros 129)
SE2070Apr11T.png
April 11, 2070
(Saros 130)
SE2099Mar21A.png
March 21, 2099
(Saros 131)
SE2128Mar01A.png
March 1, 2128
(Saros 132)
SE2157Feb09T.png
February 9, 2157
(Saros 133)
SE2186Jan20A.png
January 20, 2186
(Saros 134)

Notes

  1. "July 20–21, 1925 Annular Solar Eclipse". timeanddate. Retrieved 2 August 2024.
  2. "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 2 August 2024.
  3. "Annular Solar Eclipse of 1925 Jul 20". EclipseWise.com. Retrieved 2 August 2024.
  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 125". eclipse.gsfc.nasa.gov.

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References