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Solar eclipse of December 5, 2029

Solar eclipse of December 5, 2029
Map
Type of eclipse
NaturePartial
Gamma−1.0609
Magnitude0.8911
Maximum eclipse
Coordinates67°30′S 135°42′E / 67.5°S 135.7°E / -67.5; 135.7
Times (UTC)
Greatest eclipse15:03:58
References
Saros123 (54 of 70)
Catalog # (SE5000)9574

A partial solar eclipse will occur at the Moon's ascending node of orbit on Wednesday, December 5, 2029, with a magnitude of 0.8911. 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.

This will be the last of four partial solar eclipses in 2029, with the others occurring on January 14, 2029, June 12, 2029, and July 11, 2029.

It also follows a total lunar eclipse occurring on June 26, 2029 and precedes a total lunar eclipse occurring on and December 20, 2029.

Images


Animated path

Related eclipses

Eclipses in 2029

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 123

Inex

Triad

Solar eclipses of 2029–2032

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 eclipses on January 14, 2029 and July 11, 2029 occur on the previous lunar year eclipse set.

Solar eclipse series sets from 2029 to 2032
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
118 June 12, 2029

Partial
1.29431 123 December 5, 2029

Partial
-1.06090
128 June 1, 2030

Annular
0.56265 133 November 25, 2030

Total
-0.38669
138 May 21, 2031

Annular
-0.19699 143 November 14, 2031

Hybrid
0.30776
148 May 9, 2032

Annular
-0.93748 153 November 3, 2032

Partial
1.06431

Saros 123

It is a part of Saros cycle 123, repeating every 18 years, 11 days, containing 70 events. The series started with a partial solar eclipse on April 29, 1074. It contains annular eclipses from July 2, 1182 through April 19, 1651, hybrid eclipses from April 30, 1669 through May 22, 1705, and total eclipses from June 3, 1723 through October 23, 1957. The series ends at member 70 as a partial eclipse on May 31, 2318. The longest duration of totality was 3 minutes, 27 seconds on July 27, 1813.

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.

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.

External links

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