• Source: Solar eclipse of March 9, 2035

An annular solar eclipse will occur at the Moon's descending node of orbit between Friday, March 9 and Saturday, March 10, 2035, with a magnitude of 0.9919. 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. The Moon's apparent diameter will be near the average diameter because it will occur 7.6 days after apogee (on March 2, 2035, at 9:30 UTC) and 5.1 days before perigee (on March 15, 2035, at 1:40 UTC).
Annularity will be visible for parts of New Zealand. A partial eclipse will be visible for parts of Australia, Oceania, Antarctica, and central Mexico.




Images


Animated path




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 2035

=
A penumbral lunar eclipse on February 22.
An annular solar eclipse on March 9.
A partial lunar eclipse on August 19.
A total solar eclipse on September 2.




= Metonic

=
Preceded by: Solar eclipse of May 21, 2031
Followed by: Solar eclipse of December 26, 2038




= Tzolkinex

=
Preceded by: Solar eclipse of January 26, 2028
Followed by: Solar eclipse of April 20, 2042




= Half-Saros

=
Preceded by: Lunar eclipse of March 3, 2026
Followed by: Lunar eclipse of March 13, 2044




= Tritos

=
Preceded by: Solar eclipse of April 8, 2024
Followed by: Solar eclipse of February 5, 2046




= Solar Saros 140

=
Preceded by: Solar eclipse of February 26, 2017
Followed by: Solar eclipse of March 20, 2053




= Inex

=
Preceded by: Solar eclipse of March 29, 2006
Followed by: Solar eclipse of February 17, 2064




= Triad

=
Preceded by: Solar eclipse of May 9, 1948
Followed by: Solar eclipse of January 8, 2122




= Solar eclipses of 2033–2036

=
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 July 23, 2036 occurs in the next lunar year eclipse set.




= Saros 140

=
This eclipse is a part of Saros series 140, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on April 16, 1512. It contains total eclipses from July 21, 1656 through November 9, 1836; hybrid eclipses from November 20, 1854 through December 23, 1908; and annular eclipses from January 3, 1927 through December 7, 2485. The series ends at member 71 as a partial eclipse on June 1, 2774. 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 totality was produced by member 11 at 4 minutes, 10 seconds on August 12, 1692, and the longest duration of annularity will be produced by member 53 at 7 minutes, 35 seconds on November 15, 2449. 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


NASA graphics

Kata Kunci Pencarian:

• Fred Espenak
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• Bulan
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• Solar eclipse of March 9, 2035
• Solar eclipse of March 29, 2006
• Solar eclipse of September 2, 2035
• Solar eclipse of April 8, 2024
• Solar eclipse of May 9, 1948
• Solar eclipse of March 9, 1997
• Solar eclipse of April 20, 2042
• Solar eclipse of August 23, 2044
• March 2026 lunar eclipse
• Solar eclipse of March 29, 2025