Solar eclipse of April 11, 2051

A partial solar eclipse will occur at the Moon's descending node of orbit between Monday, April 10 and Tuesday, April 11, 2051, with a magnitude of 0.9849. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

The umbral shadow of the Moon will pass just above the North Pole. It will be the largest partial solar eclipse in 21st century.

The maximal phase of the partial eclipse (0.98) will be recorded in the Barents Sea. The partial solar eclipse will be visible for parts of Asia, Alaska, and western Canada.

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 2051

• A partial solar eclipse on April 11.
• A total lunar eclipse on April 26.
• A partial solar eclipse on October 4.
• A total lunar eclipse on October 19.

Metonic

• Preceded by: Solar eclipse of June 23, 2047
• Followed by: Solar eclipse of January 27, 2055

Tzolkinex

• Preceded by: Solar eclipse of February 28, 2044
• Followed by: Solar eclipse of May 22, 2058

Half-Saros

• Preceded by: Lunar eclipse of April 5, 2042
• Followed by: Lunar eclipse of April 15, 2060

Tritos

• Preceded by: Solar eclipse of May 11, 2040
• Followed by: Solar eclipse of March 11, 2062

Solar Saros 120

• Preceded by: Solar eclipse of March 30, 2033
• Followed by: Solar eclipse of April 21, 2069

Inex

• Preceded by: Solar eclipse of April 30, 2022
• Followed by: Solar eclipse of March 21, 2080

Triad

• Preceded by: Solar eclipse of June 10, 1964
• Followed by: Solar eclipse of February 9, 2138

Solar eclipses of 2051–2054

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 eclipse on August 3, 2054 occurs in the next lunar year eclipse set.

Saros 120

This eclipse is a part of Saros series 120, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on May 27, 933 AD. It contains annular eclipses from August 11, 1059 through April 26, 1492; hybrid eclipses from May 8, 1510 through June 8, 1564; and total eclipses from June 20, 1582 through March 30, 2033. The series ends at member 71 as a partial eclipse on July 7, 2195. 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 11 at 6 minutes, 24 seconds on September 11, 1113, and the longest duration of totality was produced by member 60 at 2 minutes, 50 seconds on March 9, 1997. 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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