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Solar eclipse of July 21, 1906
20th-century partial solar eclipse From Wikipedia, the free encyclopedia
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A partial solar eclipse occurred at the Moon's ascending node of orbit on Saturday, July 21, 1906,[1][2] with a magnitude of 0.3355. 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.
A partial eclipse was visible for parts of Argentina and Chile.
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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.[3]
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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. The first and last eclipse in this sequence is separated by one synodic month.
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Related eclipses
Eclipses in 1906
- A total lunar eclipse on February 9.
- A partial solar eclipse on February 23.
- A partial solar eclipse on July 21.
- A total lunar eclipse on August 4.
- A partial solar eclipse on August 20.
Metonic
- Followed by: Solar eclipse of May 9, 1910
Tzolkinex
- Preceded by: Solar eclipse of June 8, 1899
- Followed by: Solar eclipse of August 31, 1913
Half-Saros
- Preceded by: Lunar eclipse of July 14, 1897
- Followed by: Lunar eclipse of July 26, 1915
Tritos
- Preceded by: Solar eclipse of August 20, 1895
- Followed by: Solar eclipse of June 19, 1917
Solar Saros 115
- Preceded by: Solar eclipse of July 9, 1888
- Followed by: Solar eclipse of July 31, 1924
Inex
- Preceded by: Solar eclipse of August 9, 1877
- Followed by: Solar eclipse of June 30, 1935
Triad
- Preceded by: Solar eclipse of September 19, 1819
- Followed by: Solar eclipse of May 21, 1993
Solar eclipses of 1906–1909
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.[4]
The partial solar eclipses on February 23, 1906 and August 20, 1906 occur in the previous lunar year eclipse set.
Saros 115
This eclipse is a part of Saros series 115, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on June 21, 662 AD. It contains total eclipses from October 7, 842 AD through November 2, 1491; hybrid eclipses from November 12, 1509 through December 15, 1563; and annular eclipses from December 25, 1581 through May 27, 1816. The series ends at member 72 as a partial eclipse on August 12, 1942. 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 36 at 6 minutes, 24 seconds on July 5, 1293, and the longest duration of annularity was produced by member 65 at 1 minutes, 54 seconds on May 27, 1816. All eclipses in this series occur at the Moon’s ascending node of orbit.[5]
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.
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References
External links
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