Solar eclipse of September 23, 2033

A partial solar eclipse will occur at the Moon's ascending node of orbit on Friday, September 23, 2033, with a magnitude of 0.689. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

Solar eclipse of September 23, 2033
Map
Type of eclipse
NaturePartial
Gamma−1.1583
Magnitude0.689
Maximum eclipse
Coordinates72°12′S 121°12′W / 72.2°S 121.2°W / -72.2; -121.2
Times (UTC)
Greatest eclipse13:54:31
References
Saros125 (55 of 73)
Catalog # (SE5000)9582

Images

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Animated path

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Eclipses of 2033

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Solar Saros 125

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Inex

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Triad

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Solar eclipses of 2033–2036

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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 2033 to 2036
Descending node   Ascending node
120 March 30, 2033
 
Total
125 September 23, 2033
 
Partial
130 March 20, 2034
 
Total
135 September 12, 2034
 
Annular
140 March 9, 2035
 
Annular
145 September 2, 2035
 
Total
150 February 27, 2036
 
Partial
155 August 21, 2036
 
Partial
A partial solar eclipse on July 23, 2036 occurs in the next lunar year eclipse set.

Saros 125

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It is a part of Saros cycle 125, repeating every 18 years, 11 days, containing 73 events. The series started with a partial solar eclipse on February 4, 1060. It contains total eclipses from June 13, 1276 through July 16, 1330, hybrid eclipses on July 26, 1348 and August 7, 1366, and annular eclipses from August 17, 1384 through August 22, 1979. The series ends at member 73 as a partial eclipse on April 9, 2358. The longest duration of totality was 1 minutes, 11 seconds on June 25, 1294, and the longest duration of annularity was 7 minutes, 23 seconds on July 10, 1907.

Metonic series

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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.

References

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  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.
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