• Source: Solar eclipse of November 25, 2030

A total solar eclipse will occur at the Moon's ascending node of orbit on Monday, November 25, 2030, with a magnitude of 1.0468. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 14 hours before perigee (on November 25, 2030, at 21:10 UTC), the Moon's apparent diameter will be larger.
Totality will be visible in Namibia, Botswana, South Africa, Lesotho, and Australia. A partial eclipse will be visible for much of Central and Southern Africa, Antarctica, Australia, and Indonesia.




Path


The path of totality will begin in the Atlantic Ocean. It will then pass through Namibia (serving the capital Windhoek), Botswana (serving Tsabong), and South Africa (serving Durban; also visible in parts of Lesotho). After that, it will pass through the Indian Ocean, where it will terminate in Australia (visiting the states of South Australia, New South Wales, and Queensland).




Images


Animated path




Details of totality in some places or cities






Eclipse details


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.




Eclipse season



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 2030

=
An annular solar eclipse on June 1.
A partial lunar eclipse on June 15.
A total solar eclipse on November 25.
A penumbral lunar eclipse on December 9.




= Metonic

=
Preceded by: Solar eclipse of February 6, 2027
Followed by: Solar eclipse of September 12, 2034




= Tzolkinex

=
Preceded by: Solar eclipse of October 14, 2023
Followed by: Solar eclipse of January 5, 2038




= Half-Saros

=
Preceded by: Lunar eclipse of November 19, 2021
Followed by: Lunar eclipse of November 30, 2039




= Tritos

=
Preceded by: Solar eclipse of December 26, 2019
Followed by: Solar eclipse of October 25, 2041




= Solar Saros 133

=
Preceded by: Solar eclipse of November 13, 2012
Followed by: Solar eclipse of December 5, 2048




= Inex

=
Preceded by: Solar eclipse of December 14, 2001
Followed by: Solar eclipse of November 5, 2059




= Triad

=
Preceded by: Solar eclipse of January 25, 1944
Followed by: Solar eclipse of September 26, 2117




= 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.
The partial solar eclipses on January 14, 2029 and July 11, 2029 occur in the previous lunar year eclipse set.




= Saros 133

=
This eclipse is a part of Saros series 133, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on July 13, 1219. It contains annular eclipses from November 20, 1435 through January 13, 1526; a hybrid eclipse on January 24, 1544; and total eclipses from February 3, 1562 through June 21, 2373. The series ends at member 72 as a partial eclipse on September 5, 2499. 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 annularity was produced by member 25 at 1 minutes, 14 seconds on November 30, 1453, and the longest duration of totality was produced by member 61 at 6 minutes, 50 seconds on August 7, 1850. 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.




References






External links


Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
Google interactive map
Besselian elements

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