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Solar eclipse of March 20, 2034
Total eclipse From Wikipedia, the free encyclopedia
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A total solar eclipse will occur at the Moon's descending node of orbit on Monday, March 20, 2034,[1] with a magnitude of 1.0458. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.3 days before perigee (on March 21, 2034, at 18:15 UTC), the Moon's apparent diameter will be larger.[2]
Totality will be visible from the extreme southern tip of Benin, Nigeria, northern Cameroon, Chad, Sudan, Egypt, Saudi Arabia, Kuwait, Iran, Afghanistan, Pakistan, northern India, and western China.[3] A partial eclipse will be visible for parts of eastern Brazil, Africa, Europe, the Middle East, Central Asia, and South Asia. Coincidentally, The eclipse passes through many Islamic countries around the date of Islamic New Year (estimated around March 20–21 according to local traditions, time zone and atmospheric conditions), and also passes through Iran only a few hours before the vernal equinox, marking the beginning of the Persian New Year. Since the Islamic lunar year is 11–12 days shorter than the solar year that the Iranian calendar observes, the Islamic New Year rotates through the seasons of the year, while the Persian one is on nearly fixed date on Gregorian calendar. It is an extremely rare case that the two new years meet.
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Eclipse timing
Places experiencing total eclipse
Places experiencing partial eclipse
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Eclipse details
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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.[4]
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.
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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 June 1, 2030
- Followed by: Solar eclipse of January 5, 2038
Tzolkinex
- Preceded by: Solar eclipse of February 6, 2027
- Followed by: Solar eclipse of April 30, 2041
Half-Saros
- Preceded by: Lunar eclipse of March 14, 2025
- Followed by: Lunar eclipse of March 25, 2043
Tritos
- Preceded by: Solar eclipse of April 20, 2023
- Followed by: Solar eclipse of February 16, 2045
Solar Saros 130
- Preceded by: Solar eclipse of March 9, 2016
- Followed by: Solar eclipse of March 30, 2052
Inex
- Preceded by: Solar eclipse of April 8, 2005
- Followed by: Solar eclipse of February 28, 2063
Triad
- Preceded by: Solar eclipse of May 20, 1947
- Followed by: Solar eclipse of January 19, 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.[5]
The partial solar eclipse on July 23, 2036 occurs in the next lunar year eclipse set.
Saros 130
This eclipse is a part of Saros series 130, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on August 20, 1096. It contains total eclipses from April 5, 1475 through July 18, 2232. There are no annular or hybrid eclipses in this set. The series ends at member 73 as a partial eclipse on October 25, 2394. 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 30 at 6 minutes, 41 seconds on July 11, 1619. All eclipses in this series occur at the Moon’s descending node of orbit.[6]
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.
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References
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