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- Source: Solar eclipse of November 25, 2049
A total solar eclipse will occur at the Moon's ascending node of orbit on Thursday, November 25, 2049, with a magnitude of 1.0057. 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. Occurring about 3.2 days before perigee (on November 28, 2049, at 11:05 UTC), the Moon's apparent diameter will be larger.
The path of the eclipse will be visible as an annular eclipse from parts of Saudi Arabia and Yemen before transitioning to a total eclipse. Totality will be visible from parts of Indonesia before the eclipse transforms back to an annular eclipse, then passing over Micronesia. A partial solar eclipse will also be visible for parts of East Africa, the Middle East, Central Asia, South Asia, Southeast Asia, and Australia.
Images
Animated path
Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.
This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.
Related eclipses
= Eclipses in 2049
=
A penumbral lunar eclipse on May 17.
An annular solar eclipse on May 31.
A penumbral lunar eclipse on June 15.
A penumbral lunar eclipse on November 9.
A hybrid solar eclipse on November 25.
= Metonic
=
Preceded by: Solar eclipse of February 5, 2046
Followed by: Solar eclipse of September 12, 2053
= Tzolkinex
=
Preceded by: Solar eclipse of October 14, 2042
Followed by: Solar eclipse of January 5, 2057
= Half-Saros
=
Preceded by: Lunar eclipse of November 18, 2040
Followed by: Lunar eclipse of November 30, 2058
= Tritos
=
Preceded by: Solar eclipse of December 26, 2038
Followed by: Solar eclipse of October 24, 2060
= Solar Saros 143
=
Preceded by: Solar eclipse of November 14, 2031
Followed by: Solar eclipse of December 6, 2067
= Inex
=
Preceded by: Solar eclipse of December 14, 2020
Followed by: Solar eclipse of November 4, 2078
= Triad
=
Preceded by: Solar eclipse of January 25, 1963
Followed by: Solar eclipse of September 26, 2136
= Solar eclipses of 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.
The partial solar eclipses on January 26, 2047 and July 22, 2047 occur in the previous lunar year eclipse set.
= Saros 143
=
This eclipse is a part of Saros series 143, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on March 7, 1617. It contains total eclipses from June 24, 1797 through October 24, 1995; 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, 2897. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
The longest duration of totality was produced by member 16 at 3 minutes, 50 seconds on August 19, 1887, and the longest duration of annularity will be produced by member 51 at 4 minutes, 54 seconds on September 6, 2518. All eclipses in this series occur at the Moon’s ascending node of orbit.
= 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.
= Tritos series
=
This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.
= Inex series
=
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.
Notes
References
Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
Google interactive map
Besselian elements
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