- Source: Solar eclipse of September 12, 2034
An annular solar eclipse will occur at the Moon's ascending node of orbit on Tuesday, September 12, 2034, with a magnitude of 0.9736. 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 5.7 days before apogee (on September 18, 2034, at 8:05 UTC), the Moon's apparent diameter will be smaller.
The eclipse will commence over the southern Pacific Ocean and then enter South America. Countries under the path include northern Chile, southern Bolivia, northern Argentina, southern Paraguay, and southern Brazil. The eclipse will then enter the Atlantic Ocean, and terminate approximately 2,000 miles (3,200 km) southeast of South America. A partial eclipse will be visible for parts of Central America, the Caribbean, South America, and Antarctica.
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 2034
=A total solar eclipse on March 20.
A penumbral lunar eclipse on April 3.
An annular solar eclipse on September 12.
A partial lunar eclipse on September 28.
= Metonic
=Preceded by: Solar eclipse of November 25, 2030
Followed by: Solar eclipse of July 2, 2038
= Tzolkinex
=Preceded by: Solar eclipse of August 2, 2027
Followed by: Solar eclipse of October 25, 2041
= Half-Saros
=Preceded by: Lunar eclipse of September 7, 2025
Followed by: Lunar eclipse of September 19, 2043
= Tritos
=Preceded by: Solar eclipse of October 14, 2023
Followed by: Solar eclipse of August 12, 2045
= Solar Saros 135
=Preceded by: Solar eclipse of September 1, 2016
Followed by: Solar eclipse of September 22, 2052
= Inex
=Preceded by: Solar eclipse of October 3, 2005
Followed by: Solar eclipse of August 24, 2063
= Triad
=Preceded by: Solar eclipse of November 12, 1947
Followed by: Solar eclipse of July 14, 2121
= 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 135
=This eclipse is a part of Saros series 135, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on July 5, 1331. It contains annular eclipses from October 21, 1511 through February 24, 2305; hybrid eclipses on March 8, 2323 and March 18, 2341; and total eclipses from March 29, 2359 through May 22, 2449. The series ends at member 71 as a partial eclipse on August 17, 2593. 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 16 at 10 minutes, 41 seconds on December 24, 1601, and the longest duration of totality will be produced by member 62 at 2 minutes, 27 seconds on May 12, 2431. 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
NASA graphics
Kata Kunci Pencarian:
- Daftar gerhana matahari pada abad ke-21
- Solar eclipse of September 12, 2034
- Solar eclipse of August 12, 2045
- Solar eclipse of October 14, 2023
- September 2034 lunar eclipse
- September 2025 lunar eclipse
- Solar eclipse of September 1, 2016
- Solar eclipse of August 2, 2027
- Solar eclipse of August 12, 2026
- Solar eclipse of September 21, 2025
- Solar eclipse of March 29, 2025
