Solar eclipse of June 8, 1956

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Solar eclipse of June 8, 1956
SE1956Jun08T.png
Map
Type of eclipse
NatureTotal
Gamma-0.8934
Magnitude1.0581
Maximum eclipse
Duration285 sec (4 m 45 s)
Coordinates40°48′S 140°42′W / 40.8°S 140.7°W / -40.8; -140.7
Max. width of band429 km (267 mi)
Times (UTC)
Greatest eclipse21:20:39
References
Saros146 (24 of 76)
Catalog # (SE5000)9412

A total solar eclipse occurred on June 8–9, 1956. 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. It began near sunrise over New Zealand on June 9th (Saturday), and ended west of South America on June 8th (Friday).

More details[]

Eclipse Magnitude: 1.05810

Eclipse Obscuration: 1.11958

Gamma: -0.89341

Saros Series: 146th (24 of 76)

Greatest Eclipse: 08 Jun 1956 21:20:07.7 UTC (21:20:39.3 TD)

Ecliptic Conjunction: 08 Jun 1956 21:29:07.4 UTC (21:29:39.0 TD)

Equatorial Conjunction: 08 Jun 1856 21:20:45.9 UTC (21:21:17.5 TD)

Sun right ascension: 5.13

Moon right ascension: 5.13

Earth's shadow right ascension: 17.13

Sun declination: 22.9

Moon declination: 22

Earth's shadow declination: -22.9

Sun diameter: 1890.4 arcseconds

Moon diameter: 1985.8 arcseconds

Path Width at Greatest Eclipse: 428.7 km (266.4 mi)

Path Width at Greatest Duration: 428.7 km (266.4 mi)

Central Duration at Greatest Eclipse: 4 minutes, 44.85 seconds

Central Duration at Greatest Duration: 4 minutes, 44.86 seconds

Related eclipses[]

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.[1]

Note: Partial solar eclipse of February 14, 1953 and August 9, 1953 belong to the last lunar year set.

Solar eclipse series sets from 1953–1956
Descending node   Ascending node
Saros Map Saros Map
116 SE1953Jul11P.png
1953 July 11
Partial
121 SE1954Jan05A.png
1954 January 5
Annular
126 SE1954Jun30T.png
1954 June 30
Total
131 SE1954Dec25A.png
1954 December 25
Annular
136 SE1955Jun20T.png
1955 June 20
Total
141 SE1955Dec14A.png
1955 December 14
Annular
146 SE1956Jun08T.png
1956 June 8
Total
151 SE1956Dec02P.png
1956 December 2
Partial

Saros 146[]

It is a part of Saros cycle 146, repeating every 18 years, 11 days, containing 76 events. The series started with 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 December 1, 2244 through August 10, 2659. The series ends at member 76 as a partial eclipse on December 29, 2893. The longest duration of totality was 5 minutes, 21 seconds on June 30, 1992.

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.

References[]

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