Solar eclipse of November 25, 2049

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Solar eclipse of November 25, 2049
SE2049Nov25H.png
Map
Type of eclipse
Nature Hybrid
Gamma 0.2943
Magnitude 1.0057
Maximum eclipse
Duration 0m 38s
Coordinates 3.8S 95.2E
Max. width of band 21 km
Times (UTC)
Greatest eclipse 5:33:48
References
Saros 143 (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[edit]

SE2049Nov25H.gif
Animated path

Related eclipses[edit]

Solar eclipses 2047-2050[edit]

Each member 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.

Note: Partial lunar eclises on January 26, 2047 and July 22, 2047 occur on the previous lunar year eclipse set.

Solar eclipse series sets from 2047-2050
Ascending node   Descending node
118 June 23, 2047
SE2047Jun23P.png
Partial
123 December 16, 2047
SE2047Dec16P.png
Partial
128 June 11, 2048
SE2048Jun11A.png
Annular
133 December 5, 2048
SE2048Dec05T.png
Total
138 May 31, 2049
SE2049May31A.png
Annular
143 November 25, 2049
SE2049Nov25H.png
Hybrid
148 May 20, 2049
SE2050May20H.png
Hybrid
153 November 14, 2050
SE2050Nov14P.png
Partial

Saros 143[edit]

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.[1]

Series members 17-28 occur between 1901 and 2100:

17 18 19
SE1905Aug30T.png
August 30, 1905
SE1923Sep10T.png
September 10, 1923
SE1941Sep21T.png
September 21, 1941
20 21 22
SE1959Oct02T.png
October 2, 1959
SE1977Oct12T.png
October 12, 1977
SE1995Oct24T.png
October 24, 1995
23 24 25
SE2013Nov03H.png
November 3, 2013
SE2031Nov14H.png
November 14, 2031
SE2049Nov25H.png
November 25, 2049
26 27 28
SE2067Dec06H.png
December 6, 2067
SE2085Dec16A.png
December 16, 2085

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).

This series has 21 eclipse events, progressing from north to south 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
SE2000Jul01P.png
July 1, 2000
SE2004Apr19P.png
April 19, 2004
SE2008Feb07A.png
February 7, 2008
SE2011Nov25P.png
November 25, 2011
SE2015Sep13P.png
September 13, 2015
127 129 131 133 135
SE2019Jul02T.png
July 2, 2019
SE2023Apr20H.png
April 20, 2023
SE2027Feb06A.png
February 6, 2027
SE2030Nov25T.png
November 25, 2030
SE2034Sep12A.png
September 12, 2034
137 139 141 143 145
SE2038Jul02A.png
July 2, 2038
SE2042Apr20T.png
April 20, 2042
SE2046Feb05A.png
February 5, 2046
SE2049Nov25H.png
November 25, 2049
SE2053Sep12T.png
September 12, 2053
147 149 151 153 155
SE2057Jul01A.png
July 1, 2057
SE2061Apr20T.png
April 20, 2061
SE2065Feb05P.png
February 5, 2065
SE2068Nov24P.png
November 24, 2068
SE2072Sep12T.png
September 12, 2072
157
SE2076Jul01P.png
July 1, 2076

Notes[edit]

References[edit]