Solar eclipse of January 26, 2028

An annular solar eclipse will occur at the Moon's ascending node of orbit on Wednesday, January 26, 2028, with a magnitude of 0.9208. 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 2 days before apogee (on January 28, 2028, at 15:30 UTC), the Moon's apparent diameter will be smaller.

The path of annularity will pass through Ecuador, Peru, northern Brazil, and French Guiana. It will then travel across the Atlantic Ocean and end in southern Portugal (including the whole Madeira Islands), northern Morocco, and southern Spain. A partial eclipse will be visible over much of central and northern South America, Central America, the Caribbean, eastern North America and Western Europe, and West Africa.

Images

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.

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 2028

• A partial lunar eclipse on January 12.
• An annular solar eclipse on January 26.
• A partial lunar eclipse on July 6.
• A total solar eclipse on July 22.
• A total lunar eclipse on December 31.

Metonic

• Preceded by: Solar eclipse of April 8, 2024
• Followed by: Solar eclipse of November 14, 2031

Tzolkinex

• Preceded by: Solar eclipse of December 14, 2020
• Followed by: Solar eclipse of March 9, 2035

Half-Saros

• Preceded by: Lunar eclipse of January 21, 2019
• Followed by: Lunar eclipse of January 31, 2037

Tritos

• Preceded by: Solar eclipse of February 26, 2017
• Followed by: Solar eclipse of December 26, 2038

Solar Saros 141

• Preceded by: Solar eclipse of January 15, 2010
• Followed by: Solar eclipse of February 5, 2046

Inex

• Preceded by: Solar eclipse of February 16, 1999
• Followed by: Solar eclipse of January 5, 2057

Triad

• Preceded by: Solar eclipse of March 27, 1941
• Followed by: Solar eclipse of November 27, 2114

Solar eclipses of 2026–2029

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 June 12, 2029 and December 5, 2029 occur in the next lunar year eclipse set.

Saros 141

This eclipse is a part of Saros series 141, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on May 19, 1613. It contains annular eclipses from August 4, 1739 through October 14, 2640. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on June 13, 2857. 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 20 at 12 minutes, 9 seconds on December 14, 1955. 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.

External links

• Eclipse Predictions by Fred Espenak, NASA/GSFC