Solar eclipse of November 25, 2049
Map
Type of eclipse
NatureHybrid
Gamma0.2943
Magnitude1.0057
Maximum eclipse
Duration38 sec (0 m 38 s)
Coordinates3°48′S 95°12′E / 3.8°S 95.2°E / -3.8; 95.2
Max. width of band21 km (13 mi)
Times (UTC)
Greatest eclipse5:33:48
References
Saros143 (25 of 72)
Catalog # (SE5000)9618

A total solar eclipse will occur on November 25, 2049. It is a hybrid event, with only a fraction of its path as total, and longer sections at the start and end as an annular eclipse. 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.

Images


Animated path

Solar eclipses 2047–2050

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 lunar eclipses on January 26, 2047 and July 22, 2047 occur on the previous lunar year eclipse set.

Solar eclipse sets from 2047–2050
Descending node   Ascending node
118June 23, 2047

Partial
123December 16, 2047

Partial
128June 11, 2048

Annular
133December 5, 2048

Total
138May 31, 2049

Annular
143November 25, 2049

Hybrid
148May 20, 2050

Hybrid
153November 14, 2050

Partial

Saros 143

It is a part of Saros cycle 143, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on March 7, 1617 and total event from June 24, 1797 through October 24, 1995. It has hybrid eclipses from November 3, 2013 through December 6, 2067, and annular eclipses from December 16, 2085 through September 16, 2536. The series ends at member 72 as a partial eclipse on April 23, 2873. The longest duration of totality was 3 minutes, 50 seconds on August 19, 1887. All eclipses in this series occurs at the Moon’s ascending node.

Series members 17–28 occur between 1741 and 2100
8 9 10

May 23, 1743

June 3, 1761

June 14, 1779
11 12 13

June 24, 1797

July 6, 1815

July 17, 1833
14 15 16

July 28, 1851

August 7, 1869

August 19, 1887
17 18 19

August 30, 1905

September 10, 1923

September 21, 1941
20 21 22

October 2, 1959

October 12, 1977

October 24, 1995
23 24 25

November 3, 2013

November 14, 2031

November 25, 2049
26 27 28

December 6, 2067

December 16, 2085

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.

21 eclipse events, progressing from south to north between July 1, 2000 and July 1, 2076
July 1–2 April 19–20 February 5–7 November 24–25 September 12–13
117 119 121 123 125

July 1, 2000

April 19, 2004

February 7, 2008

November 25, 2011

September 13, 2015
127 129 131 133 135

July 2, 2019

April 20, 2023

February 6, 2027

November 25, 2030

September 12, 2034
137 139 141 143 145

July 2, 2038

April 20, 2042

February 5, 2046

November 25, 2049

September 12, 2053
147 149 151 153 155

July 1, 2057

April 20, 2061

February 5, 2065

November 24, 2068

September 12, 2072
157 159 161 163 165

July 1, 2076

Notes

  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

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