Solar eclipse of December 16, 2047

A partial solar eclipse will occur at the Moon's ascending node of orbit between Monday, December 16 and Tuesday, December 17, 2047, with a magnitude of 0.8816. 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.

This will be the last of four partial solar eclipses in 2047, with the others occurring on January 26, June 23, and July 22.

The partial solar eclipse will be visible for parts of Antarctica, southern Chile, and southern Argentina.

Images

Animated path

Eclipse timing

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 2047

• A total lunar eclipse on January 12.
• A partial solar eclipse on January 26.
• A partial solar eclipse on June 23.
• A total lunar eclipse on July 7.
• A partial solar eclipse on July 22.
• A partial solar eclipse on December 16.

Metonic

• Preceded by: Solar eclipse of February 28, 2044
• Followed by: Solar eclipse of October 4, 2051

Tzolkinex

• Preceded by: Solar eclipse of November 4, 2040
• Followed by: Solar eclipse of January 27, 2055

Half-Saros

• Preceded by: Lunar eclipse of December 11, 2038
• Followed by: Lunar eclipse of December 22, 2056

Tritos

• Preceded by: Solar eclipse of January 16, 2037
• Followed by: Solar eclipse of November 16, 2058

Solar Saros 123

• Preceded by: Solar eclipse of December 5, 2029
• Followed by: Solar eclipse of December 27, 2065

Inex

• Preceded by: Solar eclipse of January 6, 2019
• Followed by: Solar eclipse of November 26, 2076

Triad

• Preceded by: Solar eclipse of February 15, 1961
• Followed by: Solar eclipse of October 17, 2134

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 123

This eclipse is a part of Saros series 123, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on April 29, 1074. It contains annular eclipses from July 2, 1182 through April 19, 1651; hybrid eclipses from April 30, 1669 through May 22, 1705; and total eclipses from June 3, 1723 through October 23, 1957. The series ends at member 70 as a partial eclipse on May 31, 2318. 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 19 at 8 minutes, 7 seconds on November 9, 1398, and the longest duration of totality was produced by member 42 at 3 minutes, 27 seconds on July 27, 1813. 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.

The partial solar eclipses on March 27, 1884 (part of Saros 108) and December 24, 1916 (part of Saros 111) are also a part of this series but are not included in the table below.

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

External links

• Eclipse Predictions by Fred Espenak, NASA/GSFC