Solar eclipse of June 8, 1956

Solar eclipse of June 8, 1956
Solar eclipse of June 8, 1956
	Map
Type of eclipse
Nature	Total
Gamma	−0.8934
Magnitude	1.0581
Maximum eclipse
Duration	285 s (4 min 45 s)
Coordinates	40°48′S140°42′W / 40.8°S 140.7°W
Max. width of band	429 km (267 mi)
Times (UTC)
Greatest eclipse	21:20:39
References
Saros	146 (24 of 76)
Catalog # (SE5000)	9412

Last updated January 23, 2025

A total solar eclipse occurred at the Moon's descending node of orbit between Friday, June 8 and Saturday, June 9, 1956,^[1] with a magnitude of 1.0581. 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. Occurring about 1.3 days before perigee (on June 10, 1956, at 4:10 UTC), the Moon's apparent diameter was larger.^[2]

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]

June 8, 1956 Solar Eclipse Times
Event	Time (UTC)
First Penumbral External Contact	1956 June 08 at 19:11:21.5 UTC
First Umbral External Contact	1956 June 08 at 20:31:34.6 UTC
First Central Line	1956 June 08 at 20:34:31.6 UTC
First Umbral Internal Contact	1956 June 08 at 20:37:38.2 UTC
Greatest Eclipse	1956 June 08 at 21:20:39.3 UTC
Greatest Duration	1956 June 08 at 21:20:59.3 UTC
Equatorial Conjunction	1956 June 08 at 21:21:17.5 UTC
Ecliptic Conjunction	1956 June 08 at 21:29:39.0 UTC
Last Umbral Internal Contact	1956 June 08 at 22:03:38.5 UTC
Last Central Line	1956 June 08 at 22:06:46.5 UTC
Last Umbral External Contact	1956 June 08 at 22:09:44.9 UTC
Last Penumbral External Contact	1956 June 08 at 23:29:54.1 UTC

June 8, 1956 Solar Eclipse Parameters
Parameter	Value
Eclipse Magnitude	1.05810
Eclipse Obscuration	1.11958
Gamma	−0.89341
Sun Right Ascension	05h07m54.5s
Sun Declination	+22°54'13.6"
Sun Semi-Diameter	15'45.2"
Sun Equatorial Horizontal Parallax	08.7"
Moon Right Ascension	05h07m52.9s
Moon Declination	+22°00'05.8"
Moon Semi-Diameter	16'32.9"
Moon Equatorial Horizontal Parallax	1°00'44.0"
ΔT	31.5 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 May–June 1956
May 24 Ascending node (full moon)	June 8 Descending node (new moon)

Partial lunar eclipse Lunar Saros 120	Total solar eclipse Solar Saros 146

Related eclipses

Eclipses in 1956

Solar eclipses of 1953–1956

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 February 14, 1953 and August 9, 1953 occur in the previous lunar year eclipse set.

Solar eclipse series sets from 1953 to 1956
Descending node			Ascending node
Saros	Map	Gamma	Saros	Map	Gamma
116	July 11, 1953 Partial	1.4388	121	January 5, 1954 Annular	−0.9296
126	June 30, 1954 Total	0.6135	131	December 25, 1954 Annular	−0.2576
136	June 20, 1955 Total	−0.1528	141	December 14, 1955 Annular	0.4266
146	June 8, 1956 Total	−0.8934	151	December 2, 1956 Partial	1.0923

Saros 146

This eclipse is a part of Saros series 146, repeating every 18 years, 11 days, and containing 76 events. The series started with a partial solar eclipse on September 19, 1541. It contains total eclipses from May 29, 1938 through October 7, 2154; hybrid eclipses from October 17, 2172 through November 20, 2226; and annular eclipses from November 30, 2244 through August 10, 2659. The series ends at member 76 as a partial eclipse on December 29, 2893. 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 26 at 5 minutes, 21 seconds on June 30, 1992, and the longest duration of annularity will be produced by member 63 at 3 minutes, 30 seconds on August 10, 2659. All eclipses in this series occur at the Moon’s descending node of orbit.^[5]

Series members 16–37 occur between 1801 and 2200:
16	17	18
March 13, 1812	March 24, 1830	April 3, 1848
19	20	21
April 15, 1866	April 25, 1884	May 7, 1902
22	23	24
May 18, 1920	May 29, 1938	June 8, 1956
25	26	27
June 20, 1974	June 30, 1992	July 11, 2010
28	29	30
July 22, 2028	August 2, 2046	August 12, 2064
31	32	33
August 24, 2082	September 4, 2100	September 15, 2118
34	35	36
September 26, 2136	October 7, 2154	October 17, 2172
37
October 29, 2190

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 descending node.

22 eclipse events between March 27, 1884 and August 20, 1971
March 27–29	January 14	November 1–2	August 20–21	June 8
108	110	112	114	116
March 27, 1884			August 20, 1895	June 8, 1899
118	120	122	124	126
March 29, 1903	January 14, 1907	November 2, 1910	August 21, 1914	June 8, 1918
128	130	132	134	136
March 28, 1922	January 14, 1926	November 1, 1929	August 21, 1933	June 8, 1937
138	140	142	144	146
March 27, 1941	January 14, 1945	November 1, 1948	August 20, 1952	June 8, 1956
148	150	152	154
March 27, 1960	January 14, 1964	November 2, 1967	August 20, 1971

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 2087
August 17, 1803 (Saros 132)	July 17, 1814 (Saros 133)	June 16, 1825 (Saros 134)	May 15, 1836 (Saros 135)	April 15, 1847 (Saros 136)
March 15, 1858 (Saros 137)	February 11, 1869 (Saros 138)	January 11, 1880 (Saros 139)	December 12, 1890 (Saros 140)	November 11, 1901 (Saros 141)
October 10, 1912 (Saros 142)	September 10, 1923 (Saros 143)	August 10, 1934 (Saros 144)	July 9, 1945 (Saros 145)	June 8, 1956 (Saros 146)
May 9, 1967 (Saros 147)	April 7, 1978 (Saros 148)	March 7, 1989 (Saros 149)	February 5, 2000 (Saros 150)	January 4, 2011 (Saros 151)
December 4, 2021 (Saros 152)	November 3, 2032 (Saros 153)	October 3, 2043 (Saros 154)	September 2, 2054 (Saros 155)	August 2, 2065 (Saros 156)
July 1, 2076 (Saros 157)	June 1, 2087 (Saros 158)

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
September 17, 1811 (Saros 141)	August 27, 1840 (Saros 142)	August 7, 1869 (Saros 143)
July 18, 1898 (Saros 144)	June 29, 1927 (Saros 145)	June 8, 1956 (Saros 146)
May 19, 1985 (Saros 147)	April 29, 2014 (Saros 148)	April 9, 2043 (Saros 149)
March 19, 2072 (Saros 150)	February 28, 2101 (Saros 151)	February 8, 2130 (Saros 152)
January 19, 2159 (Saros 153)	December 29, 2187 (Saros 154)

Notes

↑ "June 8, 1956 Total Solar Eclipse". timeanddate. Retrieved 6 August 2024.
↑ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 6 August 2024.
↑ "Total Solar Eclipse of 1956 Jun 08". EclipseWise.com. Retrieved 6 August 2024.
↑ 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.
↑ "NASA - Catalog of Solar Eclipses of Saros 146". eclipse.gsfc.nasa.gov.

Related Research Articles

A partial solar eclipse occurred at the Moon's descending node of orbit on Thursday, February 15, 2018, with a magnitude of 0.5991. 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.

<span class="mw-page-title-main">Solar eclipse of June 20, 1974</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit on Thursday, June 20, 1974, with a magnitude of 1.0592. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the view 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. Occurring about 1.4 days before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of March 28, 1968</span> 20th-century partial solar eclipse

A partial solar eclipse occurred at the Moon's ascending node of orbit between Thursday, March 28 and Friday, March 29, 1968, with a magnitude of 0.899. 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.

<span class="mw-page-title-main">Solar eclipse of May 9, 1967</span> 20th-century partial solar eclipse

A partial solar eclipse occurred at the Moon's ascending node of orbit on Tuesday, May 9, 1967, with a magnitude of 0.7201. 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.

<span class="mw-page-title-main">Solar eclipse of November 4, 2040</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's descending node of orbit on Sunday, November 4, 2040, with a magnitude of 0.8074. 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.

<span class="mw-page-title-main">Solar eclipse of July 22, 2047</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's descending node of orbit between Monday, July 22 and Tuesday, July 23, 2047, with a magnitude of 0.3604. 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.

<span class="mw-page-title-main">Solar eclipse of January 16, 2075</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit on Wednesday, January 16, 2075, with a magnitude of 1.0311. 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. Occurring about 1.5 days after perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of May 22, 2058</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's ascending node of orbit on Wednesday, May 22, 2058, with a magnitude of 0.4141. 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.

<span class="mw-page-title-main">Solar eclipse of August 13, 2083</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's descending node of orbit on Friday, August 13, 2083, with a magnitude of 0.6146. 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.

<span class="mw-page-title-main">Solar eclipse of June 11, 2086</span> Total eclipse

A total solar eclipse will occur at the Moon's descending node of orbit on Tuesday, June 11, 2086, with a magnitude of 1.0174. 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. Occurring about 4.4 days after perigee, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of April 1, 2098</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's ascending node of orbit on Tuesday, April 1, 2098, with a magnitude of 0.7984. 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.

<span class="mw-page-title-main">Solar eclipse of October 26, 2087</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's ascending node of orbit on Sunday, October 26, 2087, with a magnitude of 0.4696. 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.

<span class="mw-page-title-main">Solar eclipse of March 31, 2090</span> Future partial solar eclipse

A partial solar eclipse will occur at the Moon's descending node of orbit on Friday, March 31, 2090, with a magnitude of 0.7843. 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.

<span class="mw-page-title-main">Solar eclipse of June 28, 1889</span> 19th-century annular solar eclipse

An annular solar eclipse occurred at the Moon's ascending node of orbit on Friday, June 28, 1889, with a magnitude of 0.9471. 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 1.1 days after apogee, the Moon's apparent diameter was smaller.

<span class="mw-page-title-main">Solar eclipse of May 30, 1946</span> 20th-century partial solar eclipse

A partial solar eclipse occurred at the Moon's ascending node of orbit on Thursday, May 30, 1946, with a magnitude of 0.8865. 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.

<span class="mw-page-title-main">Solar eclipse of January 3, 1946</span> 20th-century partial solar eclipse

A partial solar eclipse occurred at the Moon's descending node of orbit on Thursday, January 3, 1946, with a magnitude of 0.5529. 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.

<span class="mw-page-title-main">Solar eclipse of April 18, 1931</span> 20th-century partial solar eclipse

A partial solar eclipse occurred at the Moon's ascending node of orbit between Friday, April 17 and Saturday, April 18, 1931, with a magnitude of 0.5107. 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.

<span class="mw-page-title-main">Solar eclipse of May 29, 1938</span> Total eclipse

A total solar eclipse occurred at the Moon's descending node of orbit on Sunday, May 29, 1938, with a magnitude of 1.0552. 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. Occurring about 1.2 days before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of December 24, 1927</span> 20th-century partial solar eclipse

A partial solar eclipse occurred at the Moon's descending node of orbit on Saturday, December 24, 1927, with a magnitude of 0.549. 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.

<span class="mw-page-title-main">Solar eclipse of May 18, 1920</span> 20th-century partial solar eclipse

A partial solar eclipse occurred at the Moon's descending node of orbit on Tuesday, May 18, 1920, with a magnitude of 0.9734. 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.

References

Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
- Google interactive map
- Besselian elements

This page is based on this Wikipedia article
Text is available under the CC BY-SA 4.0 license; additional terms may apply.
Images, videos and audio are available under their respective licenses.

[1] "June 8, 1956 Total Solar Eclipse". timeanddate. Retrieved 6 August 2024.

[2] "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 6 August 2024.

[3] "Total Solar Eclipse of 1956 Jun 08". 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 146". eclipse.gsfc.nasa.gov.

[1]

[2]

[3]

[4]

[5]

Solar eclipse of June 8, 1956

Contents

Eclipse details

Eclipse season

Related eclipses

Eclipses in 1956

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 146

Inex

Triad