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Solar eclipse of April 30, 1957

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Solar eclipse of April 30, 1957
Map
Type of eclipse
NatureAnnular
Gamma0.9992
Magnitude0.9799
Maximum eclipse
Duration-
Coordinates70°36′N 40°18′E / 70.6°N 40.3°E / 70.6; 40.3
Max. width of band- km
Times (UTC)
Greatest eclipse0:05:28
References
Saros118 (65 of 72)
Catalog # (SE5000)9414

An annular solar eclipse occurred at the Moon's descending node of orbit on Tuesday, April 30, 1957,[1] with a magnitude of 0.9799. 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 6.1 days after apogee (on April 23, 1957, at 22:20 UTC), the Moon's apparent diameter was smaller.[2]

It will be unusual in that while it is a total solar eclipse, it is not a central solar eclipse. A non-central eclipse is one where the center-line of totality does not intersect the surface of the Earth (when the gamma is between 0.9972 and 1.0260). Instead, the center line passes just above the Earth's surface. This rare type occurs when totality is only visible at sunset or sunrise in a polar region.

Annularity was visible from northern Soviet Union (today's Russia) and Bear Island, the southernmost island of Svalbard, Norway. A partial eclipse was visible for parts of East Asia, Northeast Asia, Alaska, Canada, and the Northwestern United States. This was the last of 57 umbral eclipses in Solar Saros 118.

Eclipse details

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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]

April 30, 1957 Solar Eclipse Times
Event Time (UTC)
First Penumbral External Contact 1957 April 29 at 21:50:57.6 UTC
First Umbral External Contact 1957 April 29 at 23:51:50.2 UTC
Ecliptic Conjunction 1957 April 29 at 23:54:18.0 UTC
Greatest Eclipse 1957 April 30 at 00:05:27.8 UTC
Last Umbral External Contact 1957 April 30 at 00:18:44.0 UTC
Equatorial Conjunction 1957 April 30 at 00:31:13.8 UTC
Last Penumbral External Contact 1957 April 30 at 02:19:40.2 UTC
April 30, 1957 Solar Eclipse Parameters
Parameter Value
Eclipse Magnitude 0.97988
Eclipse Obscuration -
Gamma 0.99918
Sun Right Ascension 02h27m57.4s
Sun Declination +14°37'21.8"
Sun Semi-Diameter 15'52.5"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 02h27m05.4s
Moon Declination +15°32'09.0"
Moon Semi-Diameter 15'22.0"
Moon Equatorial Horizontal Parallax 0°56'23.9"
ΔT 31.8 s

Eclipse season

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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 April–May 1957
April 30
Descending node (new moon)
May 13
Ascending node (full moon)
Annular solar eclipse
Solar Saros 118
Total lunar eclipse
Lunar Saros 130
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Eclipses in 1957

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Solar Saros 118

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Inex

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Triad

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Solar eclipses of 1957–1960

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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]

Solar eclipse series sets from 1957 to 1960
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
118 April 30, 1957

Annular (non-central)
0.9992 123 October 23, 1957

Total (non-central)
1.0022
128 April 19, 1958

Annular
0.275 133 October 12, 1958

Total
−0.2951
138 April 8, 1959

Annular
−0.4546 143 October 2, 1959

Total
0.4207
148 March 27, 1960

Partial
−1.1537 153 September 20, 1960

Partial
1.2057

Saros 118

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This eclipse is a part of Saros series 118, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on May 24, 803 AD. It contains total eclipses from August 19, 947 AD through October 25, 1650; hybrid eclipses on November 4, 1668 and November 15, 1686; and annular eclipses from November 27, 1704 through April 30, 1957. The series ends at member 72 as a partial eclipse on July 15, 2083. 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 34 at 6 minutes, 59 seconds on May 16, 1398, and the longest duration of annularity was produced by member 59 at 1 minutes, 58 seconds on February 23, 1849. All eclipses in this series occur at the Moon’s descending node of orbit.[5]

Metonic series

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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 descending node.

21 eclipse events between July 11, 1953 and July 11, 2029
July 10–11 April 29–30 February 15–16 December 4 September 21–23
116 118 120 122 124

July 11, 1953

April 30, 1957

February 15, 1961

December 4, 1964

September 22, 1968
126 128 130 132 134

July 10, 1972

April 29, 1976

February 16, 1980

December 4, 1983

September 23, 1987
136 138 140 142 144

July 11, 1991

April 29, 1995

February 16, 1999

December 4, 2002

September 22, 2006
146 148 150 152 154

July 11, 2010

April 29, 2014

February 15, 2018

December 4, 2021

September 21, 2025
156

July 11, 2029

Tritos series

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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 1837 and 2200

April 5, 1837
(Saros 107)

March 5, 1848
(Saros 108)

February 3, 1859
(Saros 109)

December 2, 1880
(Saros 111)

August 31, 1913
(Saros 114)

July 31, 1924
(Saros 115)

June 30, 1935
(Saros 116)

May 30, 1946
(Saros 117)

April 30, 1957
(Saros 118)

March 28, 1968
(Saros 119)

February 26, 1979
(Saros 120)

January 26, 1990
(Saros 121)

December 25, 2000
(Saros 122)

November 25, 2011
(Saros 123)

October 25, 2022
(Saros 124)

September 23, 2033
(Saros 125)

August 23, 2044
(Saros 126)

July 24, 2055
(Saros 127)

June 22, 2066
(Saros 128)

May 22, 2077
(Saros 129)

April 21, 2088
(Saros 130)

March 21, 2099
(Saros 131)

February 18, 2110
(Saros 132)

January 19, 2121
(Saros 133)

December 19, 2131
(Saros 134)

November 17, 2142
(Saros 135)

October 17, 2153
(Saros 136)

September 16, 2164
(Saros 137)

August 16, 2175
(Saros 138)

July 16, 2186
(Saros 139)

June 15, 2197
(Saros 140)

Inex series

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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

August 7, 1812
(Saros 113)

July 18, 1841
(Saros 114)

June 28, 1870
(Saros 115)

June 8, 1899
(Saros 116)

May 19, 1928
(Saros 117)

April 30, 1957
(Saros 118)

April 9, 1986
(Saros 119)

March 20, 2015
(Saros 120)

February 28, 2044
(Saros 121)

February 7, 2073
(Saros 122)

January 19, 2102
(Saros 123)

December 30, 2130
(Saros 124)

December 9, 2159
(Saros 125)

November 18, 2188
(Saros 126)

Notes

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  1. ^ "April 29–30, 1957 Annular Solar Eclipse". timeanddate. Retrieved 6 August 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 6 August 2024.
  3. ^ "Annular Solar Eclipse of 1957 Apr 30". EclipseWise.com. Retrieved 6 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 118". eclipse.gsfc.nasa.gov.

References

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