Solar eclipse of August 1, 1943

Last updated
Solar eclipse of August 1, 1943
SE1943Aug01A.png
Map
Type of eclipse
NatureAnnular
Gamma −0.8041
Magnitude 0.9409
Maximum eclipse
Duration419 s (6 min 59 s)
Coordinates 34°48′S108°36′E / 34.8°S 108.6°E / -34.8; 108.6
Max. width of band367 km (228 mi)
Times (UTC)
Greatest eclipse4:16:13
References
Saros 125 (50 of 73)
Catalog # (SE5000) 9383

An annular solar eclipse occurred at the Moon's ascending node of orbit on Sunday, August 1, 1943, [1] with a magnitude of 0.9409. 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 25 minutes before apogee (on August 1, 1943, at 4:40 UTC), the Moon's apparent diameter was near its minimum. [2] Apogee did occur as the eclipse was just before its greatest eclipse.

Contents

Annularity was visible in the southern Indian Ocean, with the only land being Île Amsterdam in French Madagascar (now belonging to French Southern and Antarctic Lands). A partial solar eclipse was visible from Australia, Indonesia, Malaysia, eastern Madagascar, Antarctica's Wilkes Land.

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]

August 1, 1943 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact1943 August 01 at 01:36:43.5 UTC
First Umbral External Contact1943 August 01 at 03:02:00.9 UTC
First Central Line1943 August 01 at 03:05:56.2 UTC
First Umbral Internal Contact1943 August 01 at 03:10:00.5 UTC
Ecliptic Conjunction1943 August 01 at 04:06:41.0 UTC
Greatest Duration1943 August 01 at 04:13:30.8 UTC
Greatest Eclipse1943 August 01 at 04:16:13.0 UTC
Equatorial Conjunction1943 August 01 at 04:31:47.4 UTC
Last Umbral Internal Contact1943 August 01 at 05:22:14.2 UTC
Last Central Line1943 August 01 at 05:26:18.8 UTC
Last Umbral External Contact1943 August 01 at 05:30:14.3 UTC
Last Penumbral External Contact1943 August 01 at 06:55:35.4 UTC
August 1, 1943 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.94090
Eclipse Obscuration0.88530
Gamma−0.80410
Sun Right Ascension08h41m53.3s
Sun Declination+18°15'27.8"
Sun Semi-Diameter15'45.5"
Sun Equatorial Horizontal Parallax08.7"
Moon Right Ascension08h41m24.1s
Moon Declination+17°32'46.0"
Moon Semi-Diameter14'41.9"
Moon Equatorial Horizontal Parallax0°53'56.6"
ΔT26.0 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 August 1943
August 1
Ascending node (new moon)
August 15
Descending node (full moon)
SE1943Aug01A.png Lunar eclipse chart close-1943Aug15.png
Annular solar eclipse
Solar Saros 125
Partial lunar eclipse
Lunar Saros 137

Eclipses in 1943

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 125

Inex

Triad

Solar eclipses of 1942–1946

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 16, 1942 and September 10, 1942 occur in the previous lunar year eclipse set, and the partial solar eclipses on May 30, 1946 and November 23, 1946 occur in the next lunar year eclipse set.

Solar eclipse series sets from 1942 to 1946
Ascending node Descending node
SarosMapGammaSarosMapGamma
115 August 12, 1942
SE1942Aug12P.png
Partial
−1.5244120 February 4, 1943
SE1943Feb04T.png
Total
0.8734
125 August 1, 1943
SE1943Aug01A.png
Annular
−0.8041130 January 25, 1944
SE1944Jan25T.png
Total
0.2025
135 July 20, 1944
SE1944Jul20A.png
Annular
−0.0314140 January 14, 1945
SE1945Jan14A.png
Annular
−0.4937
145 July 9, 1945
1945Jul09T.png
Total
0.7356150 January 3, 1946
SE1946Jan03P.png
Partial
−1.2392
155 June 29, 1946
SE1946Jun29P.png
Partial
1.4361

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 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
SE1801Sep08P.png
September 8, 1801
(Saros 112)
SE1812Aug07P.gif
August 7, 1812
(Saros 113)
SE1823Jul08P.gif
July 8, 1823
(Saros 114)
SE1834Jun07P.gif
June 7, 1834
(Saros 115)
SE1845May06An.gif
May 6, 1845
(Saros 116)
SE1856Apr05T.gif
April 5, 1856
(Saros 117)
SE1867Mar06A.gif
March 6, 1867
(Saros 118)
SE1878Feb02A.gif
February 2, 1878
(Saros 119)
SE1889Jan01T.png
January 1, 1889
(Saros 120)
SE1899Dec03A.png
December 3, 1899
(Saros 121)
SE1910Nov02P.png
November 2, 1910
(Saros 122)
SE1921Oct01T.png
October 1, 1921
(Saros 123)
SE1932Aug31T.png
August 31, 1932
(Saros 124)
SE1943Aug01A.png
August 1, 1943
(Saros 125)
SE1954Jun30T.png
June 30, 1954
(Saros 126)
SE1965May30T.png
May 30, 1965
(Saros 127)
SE1976Apr29A.png
April 29, 1976
(Saros 128)
SE1987Mar29H.png
March 29, 1987
(Saros 129)
SE1998Feb26T.png
February 26, 1998
(Saros 130)
SE2009Jan26A.png
January 26, 2009
(Saros 131)
SE2019Dec26A.png
December 26, 2019
(Saros 132)
SE2030Nov25T.png
November 25, 2030
(Saros 133)
SE2041Oct25A.png
October 25, 2041
(Saros 134)
SE2052Sep22A.png
September 22, 2052
(Saros 135)
SE2063Aug24T.png
August 24, 2063
(Saros 136)
SE2074Jul24A.png
July 24, 2074
(Saros 137)
SE2085Jun22A.png
June 22, 2085
(Saros 138)
SE2096May22T.png
May 22, 2096
(Saros 139)
SE2107Apr23A.png
April 23, 2107
(Saros 140)
SE2118Mar22A.png
March 22, 2118
(Saros 141)
SE2129Feb18T.png
February 18, 2129
(Saros 142)
SE2140Jan20A.png
January 20, 2140
(Saros 143)
SE2150Dec19A.png
December 19, 2150
(Saros 144)
SE2161Nov17T.png
November 17, 2161
(Saros 145)
SE2172Oct17H.png
October 17, 2172
(Saros 146)
Saros147 32van80 SE2183Sep16A.jpg
September 16, 2183
(Saros 147)
Saros148 31van75 SE2194Aug16T.jpg
August 16, 2194
(Saros 148)

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
SE1827Oct20H.gif
October 20, 1827
(Saros 121)
SE1856Sep29A.gif
September 29, 1856
(Saros 122)
SE1885Sep08T.png
September 8, 1885
(Saros 123)
SE1914Aug21T.png
August 21, 1914
(Saros 124)
SE1943Aug01A.png
August 1, 1943
(Saros 125)
SE1972Jul10T.png
July 10, 1972
(Saros 126)
SE2001Jun21T.png
June 21, 2001
(Saros 127)
SE2030Jun01A.png
June 1, 2030
(Saros 128)
SE2059May11T.png
May 11, 2059
(Saros 129)
SE2088Apr21T.png
April 21, 2088
(Saros 130)
SE2117Apr02A.png
April 2, 2117
(Saros 131)
SE2146Mar12A.png
March 12, 2146
(Saros 132)
SE2175Feb21T.png
February 21, 2175
(Saros 133)

Notes

  1. "August 1, 1943 Annular Solar Eclipse". timeanddate. Retrieved 4 August 2024.
  2. "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 4 August 2024.
  3. "Annular Solar Eclipse of 1943 Aug 01". EclipseWise.com. Retrieved 4 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