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- Source: Solar eclipse of July 13, 2075
An annular solar eclipse will occur at the Moon's ascending node of orbit on Saturday, July 13, 2075, with a magnitude of 0.9467. 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 1.4 days after apogee (on July 11, 2075, at 20:20 UTC), the Moon's apparent diameter will be smaller.
The path of annularity will be visible from parts of eastern Spain, southern France, Monaco, Italy, San Marino, Austria, Slovenia, Croatia, northwestern Bosnia and Herzegovina, Hungary, Slovakia, southwestern Czech Republic, extreme northwestern Romania, southeastern Poland, Ukraine, Belarus, and Russia. A partial solar eclipse will also be visible for parts of Europe, North Africa, Greenland, northern Canada, Alaska, and Asia.
The annular eclipse will cross Europe and Russia. Eight European capitals will observe annual eclipse: Monaco, San Marino, Ljubljana, Zagreb, Vienna, Bratislava, Budapest and Moscow. For Moscow it will be the first central eclipse since 1887. Other European large cities (non-capitals), in which the annular eclipse will be seen include Barcelona, Marseille, Genoa, Graz, Kraków, Lviv, Nizhny Novgorod, Kirov.
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.
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 2075
=
A penumbral lunar eclipse on January 2.
A total solar eclipse on January 16.
A partial lunar eclipse on June 28.
An annular solar eclipse on July 13.
A partial lunar eclipse on December 22.
= Metonic
=
Preceded by: Solar eclipse of September 23, 2071
Followed by: Solar eclipse of May 1, 2079
= Tzolkinex
=
Preceded by: Solar eclipse of May 31, 2068
Followed by: Solar eclipse of August 24, 2082
= Half-Saros
=
Preceded by: Lunar eclipse of July 7, 2066
Followed by: Lunar eclipse of July 17, 2084
= Tritos
=
Preceded by: Solar eclipse of August 12, 2064
Followed by: Solar eclipse of June 11, 2086
= Solar Saros 147
=
Preceded by: Solar eclipse of July 1, 2057
Followed by: Solar eclipse of July 23, 2093
= Inex
=
Preceded by: Solar eclipse of August 2, 2046
Followed by: Solar eclipse of June 22, 2104
= Triad
=
Preceded by: Solar eclipse of September 11, 1988
Followed by: Solar eclipse of May 14, 2162
= Solar eclipses of 2073–2076
=
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 1, 2076 and November 26, 2076 occur in the next lunar year eclipse set.
= Saros 147
=
This eclipse is a part of Saros series 147, repeating every 18 years, 11 days, and containing 80 events. The series started with a partial solar eclipse on October 12, 1624. It contains annular eclipses from May 31, 2003 through July 31, 2706. There are no hybrid or total eclipses in this set. The series ends at member 80 as a partial eclipse on February 24, 3049. 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 38 at 9 minutes, 41 seconds on November 21, 2291. 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.
References
External links
Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
Google interactive map
Besselian elements
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