Solar eclipse of May 21, 2031

An annular solar eclipse will occur at the Moon's descending node of orbit on Wednesday, May 21, 2031, with a magnitude of 0.9589. 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 3.8 days before apogee (on May 25, 2031, at 3:10 UTC), the Moon's apparent diameter will be smaller.

Annularity will be visible from parts of Angola, Zambia, the southern Democratic Republic of the Congo, northern Malawi, Tanzania, southern India, northern Sri Lanka, the Andaman and Nicobar Islands, southern Thailand, Malaysia, and much of Indonesia. A partial eclipse will be visible for much of Africa, the Middle East, South Asia, Southeast Asia, and Australia.

Images

Animated path

Eclipse timing

Places experiencing annular eclipse

Places experiencing partial eclipse

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.

Stars and Planets during the Eclipse

Even those stars and planets bright enough to be visible during a total solar eclipse are in most cases not visible during an annular eclipse. The best candidate for naked-eye sighting is Venus, although it will be many degrees east of the Sun and therefore below the eastern horizon for morning observers in Africa. In southern India it will be well up in the east but at a lower altitude than the Sun. Venus will be best seen in those areas such as Malaysia and Indonesia where the eclipse peaks near sunset; it will be high in the west.

If any star is spotted during the eclipse it will be Sirius, which will be high in the east-southeast for observers in India and high in the west-southwest for observers in the East Indies.

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. The first and last eclipse in this sequence is separated by one synodic month.

Related eclipses

Eclipses in 2031

• A penumbral lunar eclipse on May 7.
• An annular solar eclipse on May 21.
• A penumbral lunar eclipse on June 5.
• A penumbral lunar eclipse on October 30.
• A hybrid solar eclipse on November 14.

Metonic

• Preceded by: Solar eclipse of August 2, 2027
• Followed by: Solar eclipse of March 9, 2035

Tzolkinex

• Preceded by: Solar eclipse of April 8, 2024
• Followed by: Solar eclipse of July 2, 2038

Half-Saros

• Preceded by: Lunar eclipse of May 16, 2022
• Followed by: Lunar eclipse of May 26, 2040

Tritos

• Preceded by: Solar eclipse of June 21, 2020
• Followed by: Solar eclipse of April 20, 2042

Solar Saros 138

• Preceded by: Solar eclipse of May 10, 2013
• Followed by: Solar eclipse of May 31, 2049

Inex

• Preceded by: Solar eclipse of June 10, 2002
• Followed by: Solar eclipse of April 30, 2060

Triad

• Preceded by: Solar eclipse of July 20, 1944
• Followed by: Solar eclipse of March 22, 2118

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 138

This eclipse is a part of Saros series 138, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on June 6, 1472. It contains annular eclipses from August 31, 1598 through February 18, 2482; a hybrid eclipse on March 1, 2500; and total eclipses from March 12, 2518 through April 3, 2554. The series ends at member 70 as a partial eclipse on July 11, 2716. 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 23 at 8 minutes, 2 seconds on February 11, 1869, and the longest duration of totality will be produced by member 61 at 56 seconds on April 3, 2554. All eclipses in this series occur at the Moon’s descending 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 descending 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.

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