Solar eclipse of June 8, 1956

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).

Solar eclipse of June 8, 1956
Map
Type of eclipse
NatureTotal
Gamma-0.8934
Magnitude1.0581
Maximum eclipse
Duration285 sec (4 m 45 s)
Coordinates40.8°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

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

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.

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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