• Source: Solar eclipse of March 31, 2090

A partial solar eclipse will occur at the Moon's descending node of orbit on Friday, March 31, 2090, with a magnitude of 0.7843. 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 partial solar eclipse will be visible for parts of Antarctica, southeastern Australia, and Oceania.




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 2090

=
A total lunar eclipse on March 15.
A partial solar eclipse on March 31.
A total lunar eclipse on September 8.
A total solar eclipse on September 23.




= Metonic

=
Preceded by: Solar eclipse of June 11, 2086
Followed by: Solar eclipse of January 16, 2094




= Tzolkinex

=
Preceded by: Solar eclipse of February 16, 2083
Followed by: Solar eclipse of May 11, 2097




= Half-Saros

=
Preceded by: Lunar eclipse of March 25, 2081
Followed by: Lunar eclipse of April 5, 2099




= Tritos

=
Preceded by: Solar eclipse of May 1, 2079
Followed by: Solar eclipse of February 28, 2101




= Solar Saros 150

=
Preceded by: Solar eclipse of March 19, 2072
Followed by: Solar eclipse of April 11, 2108




= Inex

=
Preceded by: Solar eclipse of April 20, 2061
Followed by: Solar eclipse of March 11, 2119




= Triad

=
Preceded by: Solar eclipse of May 31, 2003
Followed by: Solar eclipse of January 29, 2177




= Solar eclipses of 2087–2090

=
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 June 1, 2087 occurs in the previous lunar year eclipse set.




= Saros 150

=
This eclipse is a part of Saros series 150, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on August 24, 1729. It contains annular eclipses from April 22, 2126 through June 22, 2829. There are no hybrid or total eclipses in this set. The series ends at member 71 as a partial eclipse on September 29, 2991. 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 will be produced by member 45 at 9 minutes, 58 seconds on December 19, 2522. 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.




References






External links


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

Kata Kunci Pencarian:

• Daftar gerhana matahari pada abad ke-21
• Solar eclipse of March 31, 2090
• Solar eclipse of March 29, 2025
• List of solar eclipses in the 21st century
• Solar eclipse of May 31, 2003
• Solar eclipse of March 29, 2006
• Solar eclipse of April 8, 2024
• Solar eclipse of September 23, 2090
• Solar eclipse of March 31, 2071
• Solar eclipse of January 16, 2094
• List of solar eclipses visible from the British Isles