Solar eclipse of August 12, 2064

A total solar eclipse will occur on August 12, 2064, that occurs on the Pacific coast and in the southern cone, especially in the cities of Valparaíso and the capital Santiago. 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.

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

Related eclipses edit

Solar eclipses 2062–2065 edit

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]

121 March 11, 2062
 
Partial
126 September 3, 2062
 
Partial
131 February 28, 2063
 
Annular
136 August 24, 2063
 
Total
141 February 17, 2064
 
Annular
146 August 12, 2064
 
Total
151 February 5, 2065
 
Partial
156 August 2, 2065
 
Partial

Saros 146 edit

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 edit

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 edit

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 1 March 19–20 January 5–6 October 24–25 August 12–13
118 120 122 124 126
 
June 1, 2011
 
March 20, 2015
 
January 6, 2019
 
October 25, 2022
 
August 12, 2026
128 130 132 134 136
 
June 1, 2030
 
March 20, 2034
 
January 5, 2038
 
October 25, 2041
 
August 12, 2045
138 140 142 144 146
 
May 31, 2049
 
March 20, 2053
 
January 5, 2057
 
October 24, 2060
 
August 12, 2064
148 150 152 154 156
 
May 31, 2068
 
March 19, 2072
 
January 6, 2076
 
October 24, 2079
 
August 13, 2083
158 160 162 164 166
 
June 1, 2087
 
October 24, 2098

Notes edit

  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 edit