Solar eclipse of July 12, 2056

Last updated
Solar eclipse of July 12, 2056
SE2056Jul12A.png
Map
Type of eclipse
NatureAnnular
Gamma −0.0426
Magnitude 0.9878
Maximum eclipse
Duration86 s (1 min 26 s)
Coordinates 19°24′N123°42′W / 19.4°N 123.7°W / 19.4; -123.7
Max. width of band43 km (27 mi)
Times (UTC)
Greatest eclipse20:21:59
References
Saros 137 (38 of 70)
Catalog # (SE5000) 9633

An annular solar eclipse will occur on Wednesday, July 12, 2056. 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.

Contents

Solar eclipses 2054–2058

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]

Solar eclipse series sets from 2054 to 2058
Ascending node Descending node
SarosMapSarosMap
117 August 3, 2054
SE2054Aug03P.png
Partial
122 January 27, 2055
SE2055Jan27P.png
Partial
127 July 24, 2055
SE2055Jul24T.png
Total
132 January 16, 2056
SE2056Jan16A.png
Annular
137 July 12, 2056
SE2056Jul12A.png
Annular
142 January 5, 2057
SE2057Jan05T.png
Total
147 July 1, 2057
SE2057Jul01A.png
Annular
152 December 26, 2057
SE2057Dec26T.png
Total
157 June 21, 2058
SE2058Jun21P.png
Partial

Saros 137

It is a part of Saros cycle 137, repeating every 18 years, 11 days, containing 70 events. The series started with partial solar eclipse on May 25, 1389. It contains total eclipses from August 20, 1533 through December 6, 1695, first set of hybrid eclipses from December 17, 1713 through February 11, 1804, first set of annular eclipses from February 21, 1822 through March 25, 1876, second set of hybrid eclipses from April 6, 1894 through April 28, 1930, and second set of annular eclipses from May 9, 1948 through April 13, 2507. The series ends at member 70 as a partial eclipse on June 28, 2633. The longest duration of totality was 2 minutes, 55 seconds on September 10, 1569. Solar Saros 137 has 55 umbral eclipses from August 20, 1533 through April 13, 2507 (973.62 years). That's almost 1 millennium!

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.

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.

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References

  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.