Solar eclipse of August 12, 2064

A total solar eclipse will occur at the Moon's descending node of orbit on Tuesday, August 12, 2064, with a magnitude of 1.0495. 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. This eclipse will pass through the Chilean cities of Valparaíso and the capital Santiago.

Solar eclipse of August 12, 2064
Map
Type of eclipse
NatureTotal
Gamma−0.4652
Magnitude1.0495
Maximum eclipse
Duration268 s (4 min 28 s)
Coordinates10°54′S 96°00′W / 10.9°S 96°W / -10.9; -96
Max. width of band184 km (114 mi)
Times (UTC)
Greatest eclipse17:46:06
References
Saros146 (30 of 76)
Catalog # (SE5000)9651

Eclipses in 2064

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 146

Inex

Triad

Solar eclipses of 2062–2065

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]

121March 11, 2062

Partial
126September 3, 2062

Partial
131February 28, 2063

Annular
136August 24, 2063

Total
141February 17, 2064

Annular
146August 12, 2064

Total
151February 5, 2065

Partial
156August 2, 2065

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.

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.

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.

21 eclipse events between June 1, 2011 and June 1, 2087
May 31 – June 1March 19–20January 5–6October 24–25August 12–13
118120122124126

June 1, 2011

March 20, 2015

January 6, 2019

October 25, 2022

August 12, 2026
128130132134136

June 1, 2030

March 20, 2034

January 5, 2038

October 25, 2041

August 12, 2045
138140142144146

May 31, 2049

March 20, 2053

January 5, 2057

October 24, 2060

August 12, 2064
148150152154156

May 31, 2068

March 19, 2072

January 6, 2076

October 24, 2079

August 13, 2083
158160162164166

June 1, 2087

October 24, 2098

Notes

References

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